Planck 2015 results. XIII. Cosmological parameters

Abstract

We present results based on full-mission Planck observations of temperature and polarization anisotropies of the CMB. These data are consistent with the six-parameter inflationary LCDM cosmology. From the Planck temperature and lensing data, for this cosmology we find a Hubble constant, H0= (67.8 +/- 0.9) km/s/Mpc, a matter density parameter Omega_m = 0.308 +/- 0.012 and a scalar spectral index with n_s = 0.968 +/- 0.006. (We quote 68% errors on measured parameters and 95% limits on other parameters.) Combined with Planck temperature and lensing data, Planck LFI polarization measurements lead to a reionization optical depth of tau = 0.066 +/- 0.016. Combining Planck with other astrophysical data we find N_ eff = 3.15 +/- 0.23 for the effective number of relativistic degrees of freedom and the sum of neutrino masses is constrained to < 0.23 eV. Spatial curvature is found to be |Omega_K| < 0.005. For LCDM we find a limit on the tensor-to-scalar ratio of r <0.11 consistent with the B-mode constraints from an analysis of BICEP2, Keck Array, and Planck (BKP) data. Adding the BKP data leads to a tighter constraint of r < 0.09. We find no evidence for isocurvature perturbations or cosmic defects. The equation of state of dark energy is constrained to w = -1.006 +/- 0.045. Standard big bang nucleosynthesis predictions for the Planck LCDM cosmology are in excellent agreement with observations. We investigate annihilating dark matter and deviations from standard recombination, finding no evidence for new physics. The Planck results for base LCDM are in agreement with BAO data and with the JLA SNe sample. However the amplitude of the fluctuations is found to be higher than inferred from rich cluster counts and weak gravitational lensing. Apart from these tensions, the base LCDM cosmology provides an excellent description of the Planck CMB observations and many other astrophysical data sets.

Abstract severely abridged. Revised to match version accepted by Astronomy & Astrophysics. Many minor changes, but basic results remain unchanged

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• Fluctuating feedback-regulated escape fraction of ionizing radiation in low-mass, high-redshift galaxies
• Low-Mass Dark Matter Search with CDMSlite
• Tension and constraints on modified gravity parametrizations of $G_{\text{eff}}(z)$ from growth rate and Planck data
• Dark Matter, Millicharges, Axion and Scalar Particles, Gauge Bosons, and Other New Physics with LDMX
• Testing modified gravity at cosmological distances with LISA standard sirens
• Estimating the Contribution of Dynamical Ejecta in the Kilonova Associated with GW170817
• Prospects for resolving the Hubble constant tension with standard sirens
• Echo of interactions in the dark sector
• A Deep Chandra X-ray Study of Neutron Star Coalescence GW170817
• Probing the interaction between dark matter and dark energy in the presence of massive neutrinos
• The Local Group on FIRE: Dwarf galaxy populations across a suite of hydrodynamic simulations
• Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). V. Quasar Luminosity Function and Contribution to Cosmic Reionization at z = 6
• The Origin of r-Process Elements in the Milky Way
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: a tomographic measurement of cosmic structure growth and expansion rate based on optimal redshift weights
• Revisiting constraints on asteroid-mass primordial black holes as dark matter candidates
• Gravitational waves at interferometer scales and primordial black holes in axion inflation
• Systematic Identification of LAEs for Visible Exploration and Reionization Research Using Subaru HSC (SILVERRUSH). I. Program Strategy and Clustering Properties of ~2,000 Lya Emitters at z=6-7 over the 0.3-0.5 Gpc${}^2$ Survey Area
• Impact of ejecta morphology and composition on the electromagnetic signatures of neutron star mergers
• First evidence of running cosmic vacuum: challenging the concordance model
• Dark energy in Horndeski theories after GW170817: A review
• Cosmic phase transitions: their applications and experimental signatures
• The relationship between black hole mass and galaxy properties: Examining the black hole feedback model in IllustrisTNG
• The Atacama Cosmology Telescope: Two-Season ACTPol Spectra and Parameters
• Anatomy of the Inert Two Higgs Doublet Model in the light of the LHC and non-LHC Dark Matter Searches
• Voyager 1 $e^{\pm }$ Further Constrain Primordial Black Holes as Dark Matter
• Interacting scenarios with dynamical dark energy: observational constraints and alleviation of the $H_0$ tension
• GAMA/G10-COSMOS/3D-HST: The 0<z<5 cosmic star-formation history, stellar- and dust-mass densities
• Lensing is Low: Cosmology, Galaxy Formation, or New Physics?
• Neutrinoless double beta decay and neutrino mass
• Chemodynamical history of the Galactic Bulge
• H0LiCOW IV. Lens mass model of HE 0435-1223 and blind measurement of its time-delay distance for cosmology
• A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension
• Distance Priors from Planck Final Release
• RELICS: Reionization Lensing Cluster Survey
• Modeling the Radio Background from the First Black Holes at Cosmic Dawn: Implications for the 21 cm Absorption Amplitude
• On Effective Degrees of Freedom in the Early Universe
• The evidence for a spatially flat Universe
• Generalized framework for testing gravity with gravitational-wave propagation. I. Formulation
• The gravitational-wave luminosity distance in modified gravity theories
• Dark Quest. I. Fast and Accurate Emulation of Halo Clustering Statistics and Its Application to Galaxy Clustering
• Universal thermodynamic properties of the intracluster medium over two decades in radius in the X-COP sample
• Signatures of $f(Q)$-gravity in cosmology
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the configuration-space clustering wedges
• Two populations of LIGO-Virgo black holes
• Electroweak baryogenesis and gravitational waves from a real scalar singlet
• Pulsational pair-instability supernovae in very close binaries
• Planck 2018 results. XI. Polarized dust foregrounds
• Cosmological parameters derived from the final (PR4) Planck data release
• The implications of an extended dark energy cosmology with massive neutrinos for cosmological tensions
• A Future Percent-Level Measurement of the Hubble Expansion at Redshift 0.8 With Advanced LIGO
• Early-Universe Constraints on Dark Matter-Baryon Scattering and their Implications for a Global 21cm Signal
• Constraints on the Primordial Black Hole Abundance from the First Advanced LIGO Observation Run Using the Stochastic Gravitational-Wave Background
• Observation of Gravitational Waves from the Coalescence of a $2.5\text{-}4.5M_{\odot }$ Compact Object and a Neutron Star
• Baryons in the CosmicWeb of IllustrisTNG - I: Gas in Knots, Filaments, Sheets and Voids
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): The growth of structures at $0.5<z<1.2$ from redshift-space distortions in the clustering of the PDR-2 final sample
• KiDS-450: Testing extensions to the standard cosmological model
• KiDS-450: The tomographic weak lensing power spectrum and constraints on cosmological parameters
• Holographic dark energy through Tsallis entropy
• First Results from HERA Phase I: Upper Limits on the Epoch of Reionization 21 cm Power Spectrum
• Constraints on cosmic strings using data from the third Advanced LIGO-Virgo observing run
• Dark Sectors at the Fermilab SeaQuest Experiment
• 3-OGC: Catalog of gravitational waves from compact-binary mergers
• Primordial Black Holes from $\alpha$-attractors
• Testing sub-gravitational forces on atoms from a miniature, in-vacuum source mass
• Baryon Acoustic Oscillations and the Hubble Constant: Past, Present and Future
• Where are LIGO's Big Black Holes?
• A fast radio burst source at a complex magnetised site in a barred galaxy
• Standard Model-Axion-Seesaw-Higgs Portal Inflation. Five problems of particle physics and cosmology solved in one stroke
• GeV-Scale Thermal WIMPs: Not Even Slightly Dead
• Modified gravitational-wave propagation and standard sirens
• Effective Field Theory of Dark Energy: a Review
• Search for annihilating dark matter in the Sun with 3 years of IceCube data
• Measurements of the Temperature and E-Mode Polarization of the CMB from 500 Square Degrees of SPTpol Data
• Constraining Dark Energy Dynamics in Extended Parameter Space
• Axion Dark Matter Search around 6.7 $\mu$eV
• Non-thermal pressure support in X-COP galaxy clusters
• Charting the Parameter Space of the Global 21-cm Signal
• The dark-matter axion mass
• Interacting dark energy with time varying equation of state and the $H_0$ tension
• Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory
• Simulating galaxies in the reionization era with FIRE-2: galaxy scaling relations, stellar mass functions, and luminosity functions
• The Carnegie Supernova Project: Absolute Calibration and the Hubble Constant
• On the Progenitors of Type Ia Supernovae
• Cosmic Bell Test using Random Measurement Settings from High-Redshift Quasars
• The abundance, distribution, and physical nature of highly ionized oxygen OVI, OVII, and OVIII in IllustrisTNG
• Search for resonant and nonresonant new phenomena in high-mass dilepton final states at $\sqrt{s}=$ 13 TeV
• Parametric Resonance Production of Ultralight Vector Dark Matter
• Dark Matter Searches at Colliders
• Dark Energy Survey Year 1 Results: Measurement of the Baryon Acoustic Oscillation scale in the distribution of galaxies to redshift 1
• Dark, Cold, and Noisy: Constraining Secluded Hidden Sectors with Gravitational Waves
• Neutrino Mass Ordering from Oscillations and Beyond: 2018 Status and Future Prospects
• Search for gravitational lensing signatures in LIGO-Virgo binary black hole events
• Ejective and preventative: the IllustrisTNG black hole feedback and its effects on the thermodynamics of the gas within and around galaxies
• Quantifying baryon effects on the matter power spectrum and the weak lensing shear correlation
• Resolving small-scale cold circumgalactic gas in TNG50
• Euclid preparation: II. The EuclidEmulator -- A tool to compute the cosmology dependence of the nonlinear matter power spectrum
• A Multi-telescope Campaign on FRB 121102: Implications for the FRB Population
• Search for sub-solar mass ultracompact binaries in Advanced LIGO's second observing run
• Simulating cosmic ray physics on a moving mesh
• Large Population of ALMA Galaxies at z>6 with Very High [OIII]88um to [CII]158um Flux Ratios: Evidence of Extremely High Ionization Parameter or PDR Deficit?
• Reducing the $H_0$ and ${\sigma }_8$ tensions with Dark Matter-neutrino interactions
• Probing sub-GeV Dark Matter-Baryon Scattering with Cosmological Observables
• Cosmology with gamma-ray bursts: I. The Hubble diagram through the calibrated $E_{\mathrm{p},\mathrm{i}}$ - $E_{\mathrm{iso}}$ correlation
• The impact of clustering and angular resolution on far-infrared and millimeter continuum observations
• From Nuclei to the Cosmos: Tracing Heavy-Element Production with the Oldest Stars
• Improved Constraints on the 21 cm EoR Power Spectrum and the X-Ray Heating of the IGM with HERA Phase I Observations
• Estimating cosmological parameters by the simulated data of gravitational waves from the Einstein Telescope
• Planck 2015 results. XXI. The integrated Sachs-Wolfe effect
• Neutrino physics with the PTOLEMY project: active neutrino properties and the light sterile case
• Constraining the neutral fraction of hydrogen in the IGM at redshift 7.5
• The Present and Future Status of Heavy Neutral Leptons
• DeepSphere: Efficient spherical Convolutional Neural Network with HEALPix sampling for cosmological applications
• The Evolution of the IR Luminosity Function and Dust-obscured Star Formation in the Last 13 Billion Years
• A non-linear solution to the $S_8$ tension?
• Semi-analytic forecasts for JWST - I. UV luminosity functions at z = 4 - 10
• $H_0$ Tension, Phantom Dark Energy and Cosmological Parameter Degeneracies
• Constraints on neutrino masses from Lyman-alpha forest power spectrum with BOSS and XQ-100
• The Dust-to-Gas and Dust-to-Metals Ratio in Galaxies from z=0-6
• Planck intermediate results. LI. Features in the cosmic microwave background temperature power spectrum and shifts in cosmological parameters
• Galileon Gravity in Light of ISW, CMB, BAO and $H_0$ data
• On the improvement of cosmological neutrino mass bounds
• Multiband Gravitational-Wave Astronomy: Observing binary inspirals with a decihertz detector, B-DECIGO
• Vector dark matter production at the end of inflation
• Lack of clustering in low-redshift 21-cm intensity maps cross-correlated with 2dF galaxy densities
• Quantum diffusion during inflation and primordial black holes
• Unifying inflation with the axion, dark matter, baryogenesis and the seesaw mechanism
• From NANOGrav to LIGO with metastable cosmic strings
• The Local Nanohertz Gravitational-Wave Landscape From Supermassive Black Hole Binaries
• The cosmic merger rate density of compact objects: impact of star formation, metallicity, initial mass function and binary evolution
• The Distance to NGC 4993: The Host Galaxy of the Gravitational-wave Event GW170817
• New binary black hole mergers in the LIGO--Virgo O3a data
• The Sherwood simulation suite: overview and data comparisons with the Lyman-alpha forest at redshifts 2 < z < 5
• Predicting the LISA white dwarf binary population in the Milky Way with cosmological simulations
• The BAHAMAS project: the CMB--large-scale structure tension and the roles of massive neutrinos and galaxy formation
• What does the first highly-redshifted 21-cm detection tell us about early galaxies?
• Constraints on cosmic strings using data from the first Advanced LIGO observing run
• DarkSUSY 6 : An Advanced Tool to Compute Dark Matter Properties Numerically
• Graduated dark energy: Observational hints of a spontaneous sign switch in the cosmological constant
• Search for axion-like dark matter through nuclear spin precession in electric and magnetic fields
• The upper bound on the lowest mass halo
• hi_class: Horndeski in the Cosmic Linear Anisotropy Solving System
• The Atacama Cosmology Telescope: The Two-Season ACTPol Sunyaev-Zel'dovich Effect Selected Cluster Catalog
• Interacting Dark Sector and Precision Cosmology
• Blinded challenge for precision cosmology with large-scale structure: results from effective field theory for the redshift-space galaxy power spectrum
• The $H_0$ tension in light of vacuum dynamics in the Universe
• Effect of gravitational lensing on the distribution of gravitational waves from distant binary black hole mergers
• Building and testing models with extended Higgs sectors
• Measuring the Hubble constant with Type Ia supernovae as near-infrared standard candles
• Constraining Baryon--Dark Matter Scattering with the Cosmic Dawn 21-cm Signal
• General Cosmography Model with Spatial Curvature
• Accurate precision Cosmology with redshift unknown gravitational wave sources
• Exploring the effects of galaxy formation on matter clustering through a library of simulation power spectra
• The Observational Signatures of Supermassive Black Hole Seeds
• Early Structure Formation in $\Lambda$PBH Cosmologies
• The quenching and morphological evolution of central galaxies is facilitated by the feedback-driven expulsion of circumgalactic gas
• The ALMA Spectroscopic Survey in the HUDF: CO luminosity functions and the molecular gas content of galaxies through cosmic history
• Constraints on reionisation from the z=7.5 QSO ULASJ1342+0928
• No evidence for extensions to the standard cosmological model
• New Constraints on IGM Thermal Evolution from the Lyα Forest Power Spectrum
• Constraints on Dark Matter Microphysics from the Milky Way Satellite Population
• Digging deeper: Observing primordial gravitational waves below the binary black hole produced stochastic background
• Update on Coupled Dark Energy and the $H_0$ tension
• Can the $H_0$ tension be resolved in extensions to $\Lambda$CDM cosmology?
• Characterizing young protostellar disks with the CALYPSO IRAM-PdBI survey: large Class 0 disks are rare
• Using the Full Power of the Cosmic Microwave Background to Probe Axion Dark Matter
• KiDS-1000 catalogue: Redshift distributions and their calibration
• Euclid preparation: IX. EuclidEmulator2 -- Power spectrum emulation with massive neutrinos and self-consistent dark energy perturbations
• Tighter Limits on Dark Matter Explanations of the Anomalous EDGES 21cm Signal
• Generalized framework for testing gravity with gravitational-wave propagation. II. Constraints on Horndeski theory
• Grand Unified Neutrino Spectrum at Earth: Sources and Spectral Components
• Structure formation in $f(T)$ gravity and a solution for $H_0$ tension
• The formation and hierarchical assembly of globular cluster populations
• A Vacuum Phase Transition Solves $H_0$ Tension
• Strong gravitational lensing of explosive transients
• Model independent constraints on dark energy evolution from low-redshift observations
• Constraining Formation Models of Binary Black Holes with Gravitational-Wave Observations
• ProSpect: Generating Spectral Energy Distributions with Complex Star Formation and Metallicity Histories
• Galaxy Stellar Mass Functions from z~10 to z~6 using the Deepest Spitzer/IRAC Data: No Significant Evolution in the Stellar-to-Halo Mass Ratio of Galaxies in the First Gyr of Cosmic Time
• The QCD Axion Window and Low Scale Inflation
• A Unifying Theory of Dark Energy and Dark Matter: Negative Masses and Matter Creation within a Modified $\Lambda$CDM Framework
• Dark Matter Search in Nucleon, Pion, and Electron Channels from a Proton Beam Dump with MiniBooNE
• Detectability of compact binary merger macronovae
• Dark matter direct search sensitivity of the PandaX-4T experiment
• Short GRB 160821B: a reverse shock, a refreshed shock, and a well-sampled kilonova
• PBHs and secondary GWs from ultra slow roll and punctuated inflation
• SDSS-IV MaNGA: Stellar angular momentum of about 2300 galaxies: unveiling the bimodality of massive galaxy properties
• Gravitational probes of dark matter physics
• First star-forming structures in fuzzy cosmic filaments
• Search for pair and single production of vectorlike quarks in final states with at least one $Z$ boson decaying into a pair of electrons or muons in $pp$ collision data collected with the ATLAS detector at $\sqrt{s}=13$ TeV
• The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations at redshift of 0.72 with the DR14 Luminous Red Galaxy Sample
• Full-sky Gravitational Lensing Simulation for Large-area Galaxy Surveys and Cosmic Microwave Background Experiments
• A dark matter profile to model diverse feedback-induced core sizes of $\Lambda$CDM haloes
• Massive optimal data compression and density estimation for scalable, likelihood-free inference in cosmology
• The Foundation Supernova Survey: Motivation, Design, Implementation, and First Data Release
• Updated results on neutrino mass and mass hierarchy from cosmology with Planck 2018 likelihoods
• A New Target for Cosmic Axion Searches
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measurement of the growth rate of structure from the anisotropic correlation function between redshift 0.8 and 2.2
• FRB 121102 is coincident with a star forming region in its host galaxy
• Observational constraints on one-parameter dynamical dark-energy parametrizations and the $H_0$ tension
• Probing the missing baryons with the Sunyaev-Zel'dovich effect from filaments
• The MillenniumTNG Project: The hydrodynamical full physics simulation and a first look at its galaxy clusters
• Nonlocal gravity. Conceptual aspects and cosmological predictions
• Ultra-High-Energy Cosmic Rays
• Constraints from Ly-$\alpha$ forests on non-thermal dark matter including resonantly-produced sterile neutrinos
• The Cardassian expansion revisited: constraints from updated Hubble parameter measurements and Type Ia Supernovae data
• Testing $\Lambda$CDM at the lowest redshifts with SN Ia and galaxy velocities
• The status of varying constants: a review of the physics, searches and implications
• ALMA uncovers the [CII] emission and warm dust continuum in a z = 8.31 Lyman break galaxy
• First Results from the Lyman Alpha Galaxies in the Epoch of Reionization (LAGER) Survey: Cosmological Reionization at z ~ 7
• Strong Dependence of Type Ia Supernova Standardization on the Local Specific Star Formation Rate
• Clarifying the Hubble constant tension with a Bayesian hierarchical model of the local distance ladder
• Kiloparsec-scale gaseous clumps and star formation at $z=5-7$
• Constraints on scattering of keV--TeV dark matter with protons in the early Universe
• A precise extragalactic test of General Relativity
• Search for new physics in final states with an energetic jet or a hadronically decaying W or Z boson and transverse momentum imbalance at $\sqrt{s}=$ 13 TeV
• The impact of mass-transfer physics on the observable properties of field binary black hole populations
• Precision cosmology from future lensed gravitational wave and electromagnetic signals
• FRB Energetics and detectability from high redshifts
• First results from the NEWS-G direct dark matter search experiment at the LSM
• New synthesis models of consistent extragalactic background light over cosmic time
• Strong constraints on self-interacting dark matter with light mediators
• The ALMA Spectroscopic Survey Large Program: The Infrared Excess of z=1.5-10 UV-selected Galaxies and the Implied High-Redshift Star Formation History
• CPT-Symmetric Universe
• Phase transitions in the early universe
• Unifying Holographic Inflation with Holographic Dark Energy: a Covariant Approach
• Physical Bayesian modelling of the non-linear matter distribution: new insights into the Nearby Universe
• Cosmological model from the holographic equipartition law with a modified Rényi entropy
• Limits on the number of spacetime dimensions from GW170817
• Dynamical properties of z $\sim 4.5$ dusty star-forming galaxies and their connection with local early type galaxies
• High redshift JWST predictions from IllustrisTNG: Dust modelling and galaxy luminosity functions
• Results from the Super Cryogenic Dark Matter Search (SuperCDMS) experiment at Soudan
• Kiloparsec-scale ALMA Imaging of [CII] and Dust Continuum Emission of 27 Quasar Host Galaxies at z~6
• The Physics of Fast Radio Bursts
• Directly detecting sub-GeV dark matter with electrons from nuclear scattering
• ALMA reveals potential evidence for spiral arms, bars, and rings in high-redshift submillimeter galaxies
• A Critical Assessment of CMB Limits on Dark Matter-Baryon Scattering: New Treatment of the Relative Bulk Velocity
• Dark Energy Survey Year 1 Results: Galaxy clustering for combined probes
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: structure growth rate measurement from the anisotropic quasar power spectrum in the redshift range $0.8<z<2.2$
• A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations
• Neutrino Non-Standard Interactions: A Status Report
• The fraction of dark matter within galaxies from the IllustrisTNG simulations
• Precise LIGO Lensing Rate Predictions for Binary Black Holes
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Growth rate of structure measurement from anisotropic clustering analysis in configuration space between redshift 0.6 and 1.1 for the Emission Line Galaxy sample
• Extreme Value Statistics of the Halo and Stellar Mass Distributions at High Redshift: are JWST Results in Tension with ΛCDM?
• Rock 'n' Roll Solutions to the Hubble Tension
• Ultra-faint dwarfs in a Milky Way context: Introducing the Mint Condition DC Justice League Simulations
• Double inflation as a single origin of primordial black holes for all dark matter and LIGO observations
• The Opacity of the Intergalactic Medium Measured Along Quasar Sightlines at $z\sim 6$
• A Model for the Origin of Bursty Star Formation in Galaxies
• The electromagnetic counterparts of compact binary mergers
• Massive Warm/Hot Galaxy Coronae as Probed by UV/X-ray Oxygen Absorption and Emission: I - Basic Model
• New Physics in the Rayleigh-Jeans Tail of the CMB
• ISM properties of a Massive Dusty Star-Forming Galaxy discovered at z ~ 7
• Bayesian analysis of LIGO-Virgo mergers: Primordial vs. astrophysical black hole populations
• First Multimessenger Observations of a Neutron Star Merger
• Spin-2 Portal Dark Matter
• Possible signals of vacuum dynamics in the Universe
• On the radiation mechanism of repeating fast radio bursts
• Merging groups and clusters of galaxies from the SDSS data. The catalogue of groups and potentially merging systems
• A Proposal to Detect Dark Matter Using Axionic Topological Antiferromagnets
• The Herschel-ATLAS: a sample of 500μm-selected lensed galaxies over 600 square degrees
• Exploring Cosmic Origins with CORE: Inflation
• Dark Energy Survey Year 1 Results: Methods for Cluster Cosmology and Application to the SDSS
• Enhancement of Gravitational Waves Induced by Scalar Perturbations due to a Sudden Transition from an Early Matter Era to the Radiation Era
• PBH Dark Matter in Supergravity Inflation Models
• The Global 21-cm Signal in the Context of the High-z Galaxy Luminosity Function
• Probing Planckian corrections at the horizon scale with LISA binaries
• Modified cosmology through spacetime thermodynamics and Barrow horizon entropy
• 21cm Limits on Decaying Dark Matter and Primordial Black Holes
• Precision calculations of the cosmic shear power spectrum projection
• From galactic bars to the Hubble tension: weighing up the astrophysical evidence for Milgromian gravity
• The Ages of the Thin Disk, Thick Disk, and the Halo from Nearby White Dwarfs
• The FABLE simulations: A feedback model for galaxies, groups and clusters
• Cosmological Implications of Dark Matter Bound States
• The Evolution of the Baryons Associated with Galaxies Averaged over Cosmic Time and Space
• Determining the neutrino mass with Cyclotron Radiation Emission Spectroscopy - Project 8
• Toward (Finally!) Ruling Out Z and Higgs Mediated Dark Matter Models
• The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. VII. Properties of the Host Galaxy and Constraints on the Merger Timescale
• A cancellation mechanism for dark matter-nucleon interaction
• Texas Spectroscopic Search for Ly$\alpha$ Emission at the End of Reionization III. the Ly$\alpha$ Equivalent-width Distribution and Ionized Structures at $z>7$
• Black Hole Genesis of Dark Matter
• Lyman-$\alpha$ forest and non-linear structure characterization in Fuzzy Dark Matter cosmologies
• Testing gravity with cold atom interferometry: Results and prospects
• Large Fluctuations in the High-Redshift Metagalactic Ionizing Background
• Formation of ultra-diffuse galaxies in the field and in galaxy groups
• Binary black holes in young star clusters: the impact of metallicity
• Cosmic Archaeology with Gravitational Waves from Cosmic Strings
• A new approach to observational cosmology using the scattering transform
• Star cluster formation in cosmological simulations. I. Properties of young clusters
• Simulating the interstellar medium and stellar feedback on a moving mesh: Implementation and isolated galaxies
• Cosmographic analysis with Chebyshev polynomials
• No pulsed radio emission during a bursting phase of a Galactic magnetar
• KiDS-450: Cosmological Constraints from Weak Lensing Peak Statistics - II: Inference from Shear Peaks using N-body Simulations
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): Galaxy segregation inside filaments at $z\simeq 0.7$
• Planck 2015 results. XXIII. The thermal Sunyaev-Zeldovich effect--cosmic infrared background correlation
• Binary black holes in the pair-instability mass gap
• Exploring the Bayesian parameter estimation of binary black holes with LISA
• Non-circular motions and the diversity of dwarf galaxy rotation curves
• A Cold, Massive, Rotating Disk Galaxy 1.5 Billion Years after the Big Bang
• Brane-world extra dimensions in light of GW170817
• Cluster-galaxy weak lensing
• Dusty Starbursts Masquerading as Ultra-high Redshift Galaxies in JWST CEERS Observations
• Connecting the first galaxies with ultra faint dwarfs in the Local Group: chemical signatures of Population~III stars
• The primordial deuterium abundance of the most metal-poor damped Lyman-alpha system
• Inelastic Dark Matter at the LHC Lifetime Frontier: ATLAS, CMS, LHCb, CODEX-b, FASER, and MATHUSLA
• Dark energy, $\alpha$-attractors, and large-scale structure surveys
• On the FRB luminosity function -- II. Event rate density
• Violent Preheating in Inflation with Nonminimal Coupling
• SILVERRUSH. III. Deep Optical and Near-Infrared Spectroscopy for Lya and UV-Nebular Lines of Bright Lya Emitters at z=6-7
• The Planes of Satellite Galaxies Problem, Suggested Solutions, and Open Questions
• Exploring the Lower Mass Gap and Unequal Mass Regime in Compact Binary Evolution
• The zoo plot meets the swampland: mutual (in)consistency of single-field inflation, string conjectures, and cosmological data
• Search for high-mass resonances in dilepton final states in proton-proton collisions at $\sqrt{s}=$ 13 TeV
• Light Dark Matter Search with a High-Resolution Athermal Phonon Detector Operated Above Ground
• Relaxing cosmological tensions with a sign switching cosmological constant
• Constraining Primordial non-Gaussianity with Bispectrum and Power Spectum from Upcoming Optical and Radio Surveys
• The Atacama Cosmology Telescope: Two-Season ACTPol Lensing Power Spectrum
• Structure Formation and Microlensing with Axion Miniclusters
• The erratic dynamical life of black hole seeds in high-redshift galaxies
• No missing photons for reionization: moderate ionizing photon escape fractions from the FIRE-2 simulations
• Star formation histories of dwarf galaxies in the FIRE simulations: dependence on mass and Local Group environment
• Quintessential Inflation with $\alpha$-attractors
• Constraining $M_{\nu }$ with the Bispectrum I: Breaking Parameter Degeneracies
• Exploring Cosmic Origins with CORE: Cosmological Parameters
• An improved model-independent assessment of the late-time cosmic expansion
• XENON100 Dark Matter Results from a Combination of 477 Live Days
• KiDS-1000 Cosmology: constraints beyond flat $\Lambda$CDM
• Gravitational waves from gauge preheating
• From inflation to black hole mergers and back again: Gravitational-wave data-driven constraints on inflationary scenarios with a first-principle model of primordial black holes across the QCD epoch
• The Observational Future of Cosmological Scalar-Tensor Theories
• Redshift Evolution of the Black Hole Merger Rate from Globular Clusters
• The Brightest Galaxies in the Dark Ages: Galaxies' Dust Continuum Emission During the Reionization Era
• The Dawes Review 8: Measuring the Stellar Initial Mass Function
• The eROSITA Final Equatorial-Depth Survey (eFEDS): Catalog of galaxy clusters and groups
• A blinded determination of $H_0$ from low-redshift Type Ia supernovae, calibrated by Cepheid variables
• ALMA observations of atomic carbon in z~4 dusty star-forming galaxies
• A local resolution of the Hubble tension: The impact of screened fifth forces on the cosmic distance ladder
• Is the dark-matter halo spin a predictor of galaxy spin and size?
• First Cosmology Results Using Type Ia Supernovae From the Dark Energy Survey: Analysis, Systematic Uncertainties, and Validation
• The Formation of Ultra-Diffuse Galaxies in Clusters
• Discovery probability of next-generation neutrinoless double-$\beta$ decay experiments
• Primordial Black Hole Evaporation and Dark Matter Production: I. Solely Hawking radiation
• Limits on primordial black holes from $\mu$ distortions in cosmic microwave background
• Too Hot, Too Cold or Just Right? Implications of a 21-cm Signal for Dark Matter Annihilation and Decay
• $SU(5)$ Grand Unified Theory with $A_4$ Modular Symmetry
• Dust attenuation, dust emission, and dust temperature in galaxies at z>=5: a view from the FIRE-2 simulations
• The Palomar Transient Factory Core-Collapse Supernova Host-Galaxy Sample. I. Host-Galaxy Distribution Functions and Environment-Dependence of CCSNe
• Implications of Eccentric Observations on Binary Black Hole Formation Channels
• The Aemulus Project III: Emulation of the Galaxy Correlation Function
• Determining the Hubble constant from Hubble parameter measurements
• The origin of the diverse morphologies and kinematics of Milky Way-mass galaxies in the FIRE-2 simulations
• Lyman-$\alpha$ forest constraints on Primordial Black Holes as Dark Matter
• Intracluster light: a luminous tracer for dark matter in clusters of galaxies
• A magnetar-powered X-ray transient as the aftermath of a binary neutron-star merger
• A new measurement of the Hubble constant using Type Ia supernovae calibrated with surface brightness fluctuations
• Jeans Analysis for Dwarf Spheroidal Galaxies in Wave Dark Matter
• Speeding up the universe using dust with pressure
• The Science Case for LIGO-India
• Introducing RomulusC: A Cosmological Simulation of a Galaxy Cluster with Unprecedented Resolution
• Phat ELVIS: The inevitable effect of the Milky Way's disk on its dark matter subhaloes
• Eight new luminous z > 6 quasars selected via SED model fitting of VISTA, WISE and Dark Energy Survey Year 1 Observations
• Simulations of extragalactic magnetic fields and of their observables
• Galaxy Cold Gas Contents in Modern Cosmological Hydrodynamic Simulations
• Distance measures in gravitational-wave astrophysics and cosmology
• Cosmology in the dark: On the importance of source population models for gravitational-wave cosmology
• The Carnegie-Chicago Hubble Program. I. An Independent Approach to the Extragalactic Distance Scale Using only Population II Distance Indicators
• Non-Gaussian information from weak lensing data via deep learning
• Revisiting non-Gaussianity from non-attractor inflation models
• Measuring neutrino masses with large-scale structure: Euclid forecast with controlled theoretical error
• PArthENoPE reloaded
• A Search for Tensor, Vector, and Scalar Polarizations in the Stochastic Gravitational-Wave Background
• A low-mass dark matter search using ionization signals in XENON100
• The Koala: A Fast Blue Optical Transient with Luminous Radio Emission from a Starburst Dwarf Galaxy at $z=0.27$
• Model independent $H(z)$ reconstruction using the cosmic inverse distance ladder
• Search for Eccentric Binary Black Hole Mergers with Advanced LIGO and Advanced Virgo during their First and Second Observing Runs
• Dark Matter's secret liaisons: phenomenology of a dark U(1) sector with bound states
• A Triple Origin for the Heavy and Low-Spin Binary Black Holes Detected by LIGO/Virgo
• $f(Q,T)$ gravity models with observational constraints
• Make Dark Matter Charged Again
• Cosmological information in the redshift-space bispectrum
• Cluster Mass Calibration at High Redshift: HST Weak Lensing Analysis of 13 Distant Galaxy Clusters from the South Pole Telescope Sunyaev-Zel'dovich Survey
• The Complete Redshift Distribution of Dusty Star-forming Galaxies from the SPT-SZ Survey
• Beyond BAO: improving cosmological constraints from BOSS with measurement of the void-galaxy cross-correlation
• Finding the chiral gravitational wave background of an axion-SU(2) inflationary model using CMB observations and laser interferometers
• ALMA spectroscopic survey in the Hubble Ultra Deep Field: CO luminosity functions and the evolution of the cosmic density of molecular gas
• SILVERRUSH. V. Census of Lya, [OIII]5007, Ha, and [CII]158um Line Emission with ~1000 LAEs at z=4.9-7.0 Revealed with Subaru/HSC
• Time Inference with MUSE in Extragalactic Rings (TIMER): Properties of the Survey and High-Level Data Products
• Search for Low-Mass Dark Matter with CDMSlite Using a Profile Likelihood Fit
• Molecular gas in the Herschel-selected strongly lensed submillimeter galaxies at z~2-4 as probed by multi-J CO lines
• MassiveNuS: Cosmological Massive Neutrino Simulations
• Quenching star formation with quasar outflows launched by trapped IR radiation
• Reionization and galaxy inference from the high-redshift Lyα forest
• Converting non-relativistic dark matter to radiation
• Probing the Cosmological Principle in the counts of radio galaxies at different frequencies
• The THESAN project: properties of the intergalactic medium and its connection to Reionization-era galaxies
• Constraints on Binary Black Hole Populations from LIGO-Virgo Detections
• Constraints from thermal Sunyaev-Zeldovich cluster counts and power spectrum combined with CMB
• In the Wake of Dark Giants: New Signatures of Dark Matter Self Interactions in Equal Mass Mergers of Galaxy Clusters
• Accuracy of inference on the physics of binary evolution from gravitational-wave observations
• Evolution of dark energy reconstructed from the latest observations
• The High Latitude Spectroscopic Survey on the Nancy Grace Roman Space Telescope
• Modeling Biased Tracers at the Field Level
• Primordial Black Holes for the LIGO Events in the Axion-like Curvaton Model
• Thermal Friction as a Solution to the Hubble Tension
• Rethinking CMB foregrounds: systematic extension of foreground parameterizations
• Alleviating the $H_0$ and ${\sigma }_8$ anomalies with a decaying dark matter model
• Interacting neutrinos in cosmology: exact description and constraints
• Galaxy-galaxy lensing estimators and their covariance properties
• ELGAR -- a European Laboratory for Gravitation and Atom-interferometric Research
• ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Molecular gas reservoirs in high-redshift galaxies
• Probing Primordial Gravitational Waves: Ali CMB Polarization Telescope
• Baryon-induced dark matter cores in the EAGLE simulations
• Should Type Ia Supernova Distances be Corrected for their Local Environments?
• Exploring Cosmic Origins with CORE: Survey requirements and mission design
• Brans-Dicke gravity with a cosmological constant smoothes out $\Lambda$CDM tensions
• Theory and Phenomenology of Planckian Interacting Massive Particles as Dark Matter
• The Cosmic Evolution of Binary Black Holes in Young, Globular and Nuclear Star Clusters: Rates, Masses, Spins and Mixing Fractions
• Gravitational perturbations from oscillons and transients after inflation
• How to quench a galaxy
• On the normalised FRB luminosity function
• The Southern Stellar Stream Spectroscopic Survey ($S^5$): Overview, Target Selection, Data Reduction, Validation, and Early Science
• JWST UNCOVER: Extremely red and compact object at$z_{\mathrm{phot}}\simeq 7.6$ triply imaged by Abell 2744
• Cosmological window onto the string axiverse and the supersymmetry breaking scale
• Pushing back the limits: detailed properties of dwarf galaxies in a LCDM universe
• Dark Higgs Bosons at FASER
• Action Dynamics of the Local Supercluster
• Large-scale Stability and Astronomical Constraints for Coupled Dark-Energy Models
• Updated Bounds on Sum of Neutrino Masses in Various Cosmological Scenarios
• Constraining axion inflation with gravitational waves from preheating
• Joint constraints on thermal relic dark matter from strong gravitational lensing, the Lyman-$\alpha$ forest, and Milky Way satellites
• Parkes Pulsar Timing Array constraints on ultralight scalar-field dark matter
• SIMPs through the axion portal
• Descendants of the first stars: the distinct chemical signature of second generation stars
• Search for sub-solar mass ultracompact binaries in Advanced LIGO's first observing run
• Observational Constraints on Secret Neutrino Interactions from Big Bang Nucleosynthesis
• Constraints on a Bianchi type I spacetime extension of the standard $\Lambda$CDM model
• Clustering of quasars in SDSS-IV eBOSS : study of potential systematics and bias determination
• Distinguishing Primordial Black Holes from Astrophysical Black Holes by Einstein Telescope and Cosmic Explorer
• Productive Interactions: heavy particles and non-Gaussianity
• Standard Model Background of the Cosmological Collider
• Probing the scale of grand unification with gravitational waves
• The ALMA Spectroscopic Survey in the HUDF: CO Excitation and Atomic Carbon in Star-Forming Galaxies at $z=1-3$
• GW231123: a Binary Black Hole Merger with Total Mass 190-265 $M_{\odot }$
• Gravitational Waves from First-Order Phase Transitions: LIGO as a Window to Unexplored Seesaw Scales
• How blind are underground and surface detectors to strongly interacting Dark Matter?
• Joint constraints on the field-cluster mixing fraction, common envelope efficiency, and globular cluster radii from a population of binary hole mergers via deep learning
• Constraints on dark matter scenarios from measurements of the galaxy luminosity function at high redshifts
• Atomic and molecular gas in IllustrisTNG galaxies at low redshift
• On wormhole formation in $f(\text{R},\text{T})$ gravity: varying Chaplygin gas and barotropic fluid
• Constraints on the interacting vacuum -- geodesic CDM scenario
• Observational constraints on sign-changeable interaction models and alleviation of the $H_0$ tension
• Gravitational Waves and Intermediate-mass Black Hole Retention in Globular Clusters
• The 21 cm Power Spectrum from the Cosmic Dawn: First Results from the OVRO-LWA
• Using The Baryonic Tully-Fisher Relation to Measure $H_o$
• Cosmology and Accelerator Tests of Strongly Interacting Dark Matter
• A Fourth Exception in the Calculation of Relic Abundances
• Baryon Cycles in the Biggest Galaxies
• Reconciling the Diversity and Uniformity of Galactic Rotation Curves with Self-Interacting Dark Matter
• Low-mass halo perturbations in strong gravitational lenses at redshift z$\sim$0.5 are consistent with CDM
• Strongly lensed repeating Fast Radio Bursts as precision probes of the universe
• Are the ultra-high-redshift galaxies at z > 10 surprising in the context of standard galaxy formation models?
• Constraints on Sterile Neutrinos in the MeV to GeV Mass Range
• Modeling the atomic-to-molecular transition in cosmological simulations of galaxy formation
• Deep Extragalactic VIsible Legacy Survey (DEVILS): SED Fitting in the D10-COSMOS Field and the Evolution of the Stellar Mass Function and SFR-$M_{\star }$ relation
• Reionization with galaxies and active galactic nuclei
• Dynamics of test particles around a Bardeen black hole surrounded by perfect fluid dark matter
• Data-driven expectations for electromagnetic counterpart searches based on LIGO/Virgo public alerts
• Science with the TianQin observatory: Preliminary results on stellar-mass binary black holes
• Cosmology with the Wide-Field Infrared Survey Telescope -- Multi-Probe Strategies
• GW190521 may be an intermediate mass ratio inspiral
• The Milky Way's Disk of Classical Satellite Galaxies in Light of Gaia DR2
• Lyα emission line reconstruction for high-$z$ QSOs
• Scaling from gauge and scalar radiation in Abelian Higgs string networks
• Scalar-tensor theories of gravity, neutrino physics, and the $H_0$ tension
• Dielectric Haloscopes to Search for Axion Dark Matter: Theoretical Foundations
• Exploring the sensitivity of gravitational wave detectors to neutron star physics
• Mergers, Starbursts, and Quenching in the Simba Simulation
• H0LiCOW XII. Lens mass model of WFI2033-4723 and blind measurement of its time-delay distance and $H_0$
• Semi-analytic forecasts for JWST -- II. physical properties and scaling relations for galaxies at z = 4-10
• The Brightest $z\gtrsim 8$ Galaxies over the COSMOS UltraVISTA Field
• The Formation of Ultra-Diffuse Galaxies in the RomulusC Galaxy Cluster Simulation
• The SRG/eROSITA all-sky survey: Cosmology constraints from cluster abundances in the western Galactic hemisphere
• Too Big To Fail in Light of Gaia
• Modeling baryonic physics in future weak lensing surveys
• Ultra-compact structure in intermediate-luminosity radio quasars: building a sample of standard cosmological rulers and improving the dark energy constraints up to $z\sim 3$
• Setting the Stage for Cosmic Chronometers. I. Assessing the Impact of Young Stellar Populations on Hubble Parameter Measurements
• Formation of Intermediate-Mass Black Holes through Runaway Collisions in the First Star Clusters
• Search for anisotropic gravitational-wave backgrounds using data from Advanced LIGO and Advanced Virgo's first three observing runs
• Baryon acoustic oscillation, Hubble parameter, and angular size measurement constraints on the Hubble constant, dark energy dynamics, and spatial curvature
• The hierarchical assembly of galaxies and black holes in the first billion years: predictions for the era of gravitational wave astronomy
• An image of the dust sublimation region in the nucleus of NGC 1068
• Baryon Content in a Sample of 91 Galaxy Clusters Selected by the South Pole Telescope at 0.2 < z < 1.25
• The KBC void and Hubble tension contradict $\Lambda$CDM on a Gpc scale $-$ Milgromian dynamics as a possible solution
• Hydrogen-poor Superluminous Supernovae With Late-time H-alpha Emission: Three Events From the Intermediate Palomar Transient Factory
• Probing Fundamental Physics with Gravitational Waves: The Next Generation
• Gravitationally Lensed Quasars in Gaia: II. Discovery of 24 Lensed Quasars
• COSMOGRAIL XVI: Time delays for the quadruply imaged quasar DES J0408-5354 with high-cadence photometric monitoring
• Lensing substructure quantification in RXJ1131-1231: A 2 keV lower bound on dark matter thermal relic mass
• Testing Light Dark Matter Coannihilation With Fixed-Target Experiments
• Opening up the QCD axion window
• Properties of the extremely energetic GRB~221009A from Konus-WIND and SRG/ART-XC observations
• Emulating Simulations of Cosmic Dawn for 21cm Power Spectrum Constraints on Cosmology, Reionization, and X-ray Heating
• Quantifying tensions in cosmological parameters: Interpreting the DES evidence ratio
• An experiment to search for dark matter interactions using sodium iodide detectors
• Witnessing the Growth of the Nearest Galaxy Cluster: Thermodynamics of the Virgo Cluster Outskirts
• On the Level of Cluster Assembly Bias in SDSS
• Automatic physical inference with information maximising neural networks
• Bounds on Dark Matter annihilations from 21 cm data
• Improved constraints on H0 from a combined analysis of gravitational-wave and electromagnetic emission from GW170817
• The Global History of Reionisation
• Neutrino masses and their ordering: Global Data, Priors and Models
• KiDS-450: Cosmological Constraints from Weak Lensing Peak Statistics-I: Inference from Analytical Prediction of High Signal-to-Noise Ratio Convergence Peaks
• Stochastic gravitational-wave background from metastable cosmic strings
• The Black Hole Mass Function from Gravitational Wave Measurements
• FIREbox: Simulating galaxies at high dynamic range in a cosmological volume
• Formation pathway of Population III coalescing binary black holes through stable mass transfer
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions
• When the Universe Expands Too Fast: Relentless Dark Matter
• Measuring the Hubble constant with neutron star black hole mergers
• Gravitational Wave Signals of Electroweak Phase Transition Triggered by Dark Matter
• On the Progenitor of Binary Neutron Star Merger GW170817
• Giant radio galaxies in the LOFAR Two-metre Sky Survey-I
• Velocity-dependent Self-interacting Dark Matter from Groups and Clusters of Galaxies
• The cosmic merger rate density evolution of compact binaries formed in young star clusters and in isolated binaries
• On the Origin of GW190521-like events from repeated black hole mergers in star clusters
• The faint end of the Centaurus A satellite luminosity function
• Parameterized Post-Einsteinian Gravitational Waveforms in Various Modified Theories of Gravity
• A Testable Conspiracy: Simulating Baryonic Effects on Self-Interacting Dark Matter Halos
• Constraining Dark Matter -- Dark Radiation interactions with CMB, BAO, and Lyman-$\alpha$
• Scale-dependent galaxy bias, CMB lensing-galaxy cross-correlation, and neutrino masses
• Search for Dark Matter Effects on Gravitational Signals from Neutron Star Mergers
• FRII{\sl{CAT}}: A FIRST catalog of FR~II radio galaxies
• Revising natal kick prescriptions in population synthesis simulations
• Neutron stars: new constraints on asymmetric dark matter
• Constraining nonperturbative strong-field effects in scalar-tensor gravity by combining pulsar timing and laser-interferometer gravitational-wave detectors
• Baryogenesis and Dark Matter from $B$ Mesons
• An uncontaminated measurement of the escaping Lyman continuum at $z\sim 3$
• SILVERRUSH. VIII. Spectroscopic Identifications of Early Large Scale Structures with Protoclusters Over 200 Mpc at z~6-7: Strong Associations of Dusty Star-Forming Galaxies
• A Search for H-Dropout Lyman Break Galaxies at z~12-16
• GROWTH on S190814bv: Deep Synoptic Limits on the Optical/Near-Infrared Counterpart to a Neutron Star-Black Hole Merger
• Analyzing the Large-Scale Bulk Flow using CosmicFlows4: Increasing Tension with the Standard Cosmological Model
• First predictions of the angular power spectrum of the astrophysical gravitational wave background
• Directed searches for gravitational waves from ultralight bosons
• Constraining the intergalactic medium at $z\approx$ 9.1 using LOFAR Epoch of Reionization observations
• Tidal stripping as a possible origin of the ultra diffuse galaxy lacking dark matter
• Sample variance in the local measurements of the Hubble constant
• Stochastic Gravitational-Wave Background from Binary Black Holes and Binary Neutron Stars and Implications for LISA
• BBN for the LHC: constraints on lifetimes of the Higgs portal scalars
• Co-Decaying Dark Matter
• The ALMA Spectroscopic Survey in the HUDF: Multi-band constraints on line luminosity functions and the cosmic density of molecular gas
• Emergent scale symmetry: Connecting inflation and dark energy
• Limits on Pop III star formation with the most iron-poor stars
• Radiative cooling rates, ion fractions, molecule abundances and line emissivities including self-shielding and both local and metagalactic radiation fields
• Deep learning from 21-cm tomography of the Cosmic Dawn and Reionization
• Constraints on the curvature of the Universe and dynamical dark energy from the Full-shape and BAO data
• Future Cosmological Constraints from Fast Radio Bursts
• The X-SHOOTER/ALMA sample of Quasars in the Epoch of Reionization. I. NIR spectral modeling, iron enrichment and broad emission line properties
• Low Redshift Baryon Acoustic Oscillation Measurement from the Reconstructed 6-degree Field Galaxy Survey
• Constraining Non-Cold Dark Matter Models with the Global 21-cm Signal
• Coannihilation without chemical equilibrium
• Unveiling the Nature of Infrared Bright, Optically Dark Galaxies with Early JWST Data
• Cosmological dynamics of mimetic gravity
• A new interacting two fluid model and its consequences
• Supermassive Black Holes at High Redshift are Expected to be Obscured by their Massive Host Galaxies' Inter Stellar Medium
• Dark Energy from the Thermal Sunyaev Zeldovich Power Spectrum
• Ultra-slow-roll inflation with quantum diffusion
• Velocity correction for Hubble constant measurements from standard sirens
• Atomic hydrogen in IllustrisTNG galaxies: the impact of environment parallelled with local 21-cm surveys
• Self-Consistent Modeling of Reionization in Cosmological Hydrodynamical Simulations
• Large scale opacity fluctuations in the Lyman alpha forest: evidence for QSOs dominating the ionising UV background at z ~ 5.5-6 ?
• Analyzing the $H_0$ tension in $F(R)$ gravity models
• How the huge energy of quantum vacuum gravitates to drive the slow accelerating expansion of the Universe
• Using the tilted flat-$\Lambda$CDM and the untilted non-flat $\Lambda$CDM inflation models to measure cosmological parameters from a compilation of observational data
• Axion Gauge Field Inflation and Gravitational Leptogenesis: A Lower Bound on B Modes from the Matter-Antimatter Asymmetry of the Universe
• Cosmological Constraints from Multiple Probes in the Dark Energy Survey
• The Cosmic Ballet II: Spin alignment of galaxies and haloes with large-scale filaments in the EAGLE simulation
• Binary Black Hole Formation with Detailed Modeling: Stable Mass Transfer Leads to Lower Merger Rates
• Frame-dependence of higher-order inflationary observables in scalar-tensor theories
• HI constraints from the cross-correlation of eBOSS galaxies and Green Bank Telescope intensity maps
• Gravitational-wave detection rates for compact binaries formed in isolation: LIGO/Virgo O3 and beyond
• A new tension in the cosmological model from primordial deuterium?
• Constraints on dark energy dynamics and spatial curvature from Hubble parameter and baryon acoustic oscillation data
• The High-Energy Frontier of the Intensity Frontier: Closing the Dark Photon, Inelastic Dark Matter, and Muon g-2 Windows
• Gravitational waves and electroweak baryogenesis in a global study of the extended scalar singlet model
• Instant Preheating in Quintessential Inflation with $\alpha$-Attractors
• Predicting the binary black hole population of the Milky Way with cosmological simulations
• Anisotropic cosmological models in $f(R,T)$ gravity with variable deceleration parameter
• On the properties of the massive binary black hole merger GW170729
• Galaxy Formation with BECDM -- II. Cosmic Filaments and First Galaxies
• The uniformity and time-invariance of the intra-cluster metal distribution in galaxy clusters from the IllustrisTNG simulations
• On the Gas Content and Efficiency of AGN Feedback in Low-redshift Quasars
• FR0CAT: a FIRST catalog of FR0 radio galaxies
• The dependence of convective core overshooting on stellar mass: Additional binary systems and improved calibration
• The THESAN project: Lyman-alpha emission and transmission during the Epoch of Reionization
• Constraints on interacting dark energy models from Planck 2015 and redshift-space distortion data
• Cosmological simulation with dust formation and destruction
• Dark matter-neutrino interactions through the lens of their cosmological implications
• Barrow holographic dark energy with Hubble horizon as IR cutoff
• Multiband gravitational-wave event rates and stellar physics
• Bounce inflation in $f(T)$ Cosmology: A unified inflaton-quintessence field
• Cosmology with gamma-ray bursts: II Cosmography challenges and cosmological scenarios for the accelerated Universe
• The ISLAndS project II: The Lifetime Star Formation Histories of Six Andromeda dSphs
• Galaxy And Mass Assembly (GAMA): A forensic SED reconstruction of the cosmic star formation history and metallicity evolution by galaxy type
• Primordial Anisotropies in the Gravitational Wave Background from Cosmological Phase Transitions
• GRB 170817A as a jet counterpart to gravitational wave trigger GW 170817
• A census of cool core galaxy clusters in IllustrisTNG
• Charged Gravastars in Modified Gravity
• Preheating after Multifield Inflation with Nonminimal Couplings, I: Covariant Formalism and Attractor Behavior
• The VIMOS Ultra Deep Survey: Emerging from the Dark, a Massive Proto-Cluster at z~4.57
• Black Hole Mass Scaling Relations for Spiral Galaxies. I. $M_{\mathrm{BH}}$-$M_{\ast ,\mathrm{sph}}$
• The Viability of Phantom Dark Energy: A Brief Review
• Iterative initial condition reconstruction
• Formation and survival of Population III stellar systems
• Fingerprint of Low-Scale Leptogenesis in the Primordial Gravitational-Wave Spectrum
• Dust emission in an accretion-rate-limited sample of z>6 quasars
• Galaxy Evolution in the Radio Band: The Role of Starforming Galaxies and Active Galactic Nuclei
• The X-ray properties of $z>6$ quasars: no evident evolution of accretion physics in the first Gyr of the Universe
• A Local Universe Host for the Repeating Fast Radio Burst FRB 20181030A
• The Low Effective Spin of Binary Black Holes and Implications for Individual Gravitational-Wave Events
• SIGAME simulations of the [CII], [OI] and [OIII] line emission from star forming galaxies at z ~ 6
• Cooling flow solutions for the circumgalactic medium
• On the merger rate of primordial black holes: effects of nearest neighbours distribution and clustering
• Cosmological Constraints on Dark Matter Interactions with Ordinary Matter
• A Search for Extragalactic Fast Blue Optical Transients in ZTF and the Rate of AT2018cow-like Transients
• Field theoretic interpretations of interacting dark energy scenarios and recent observations
• First Cosmology Results using Type Ia Supernovae from the Dark Energy Survey: The Effect of Host Galaxy Properties on Supernova Luminosity
• First results from the DEAP-3600 dark matter search with argon at SNOLAB
• Primordial nucleosynthesis
• Weak lensing cosmology with convolutional neural networks on noisy data
• Density perturbations for running vacuum: a successful approach to structure formation and to the ${\sigma }_8$-tension
• Search for neutrinos from decaying dark matter with IceCube
• Analysis of Light Neutrino Exchange and Short-Range Mechanisms in $0\nu \beta \beta$ Decay
• Interacting radiation after Planck and its implications for the Hubble Tension
• Implications of a transition in the dark energy equation of state for the $H_0$ and ${\sigma }_8$ tensions
• The peculiar short-duration GRB 200826A and its supernova
• The PHLEK Survey: A New Determination of the Primordial Helium Abundance
• Dancing to ChaNGa: A Self-Consistent Prediction For Close SMBH Pair Formation Timescales Following Galaxy Mergers
• Search for dark matter at colliders
• A mass-dependent slope of the galaxy size-mass relation out to z~3: further evidence for a direct relation between median galaxy size and median halo mass
• Search for dark matter at $\sqrt{s}=13$ TeV in final states containing an energetic photon and large missing transverse momentum with the ATLAS detector
• Searching for Light Relics with Large-Scale Structure
• Novel approach towards the large-scale stable Interacting Dark-Energy models and their Astronomical Bounds
• Looking for the WIMP Next Door
• Neutrino Oscillations as a Probe of Light Scalar Dark Matter
• Astronomical bounds on a cosmological model allowing a general interaction in the dark sector
• A first search for a stochastic gravitational-wave background from ultralight bosons
• Naturalness, Vacuum Stability and Leptogenesis in the Minimal Seesaw Model
• Testing the low scale seesaw and leptogenesis
• RoboPol: Connection between optical polarization plane rotations and gamma-ray flares in blazars
• Revealing the galaxy-halo connection in IllustrisTNG
• Self-consistent proto-globular cluster formation in cosmological simulations of high-redshift galaxies
• Measurements of B-mode Polarization of the Cosmic Microwave Background from 500 Square Degrees of SPTpol Data
• Signs of eccentricity in two gravitational-wave signals may indicate a sub-population of dynamically assembled binary black holes
• FRICAT: A FIRST catalog of FRI radio galaxies
• Cosmological constraints from Planck galaxy clusters with CMB lensing mass bias calibration
• GW250114: testing Hawking's area law and the Kerr nature of black holes
• Mimicking dark matter and dark energy in a mimetic model compatible with GW170817
• Measuring the value of the Hubble constant "à la Refsdal"
• Dynamical dark energy after Planck CMB final release and $H_0$ tension
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Gravity test from the combination of redshift-space distortions and galaxy-galaxy lensing at $0.5<z<1.2$
• The Galactic Halo Contribution to the Dispersion Measure of Extragalactic Fast Radio Bursts
• Negative cosmological constant in the dark sector?
• A Measurement of the Cosmic Microwave Background Lensing Potential and Power Spectrum from 500 deg${}^2$ of SPTpol Temperature and Polarization Data
• Listening to the sound of dark sector interactions with gravitational wave standard sirens
• Lepton-Number-Charged Scalars and Neutrino Beamstrahlung
• The formation of direct collapse black holes under the influence of streaming velocities
• The S-PASS view of polarized Galactic Synchrotron at 2.3 GHz as a contaminant to CMB observations
• Planck 2015 results. IV. Low Frequency Instrument beams and window functions
• Weak-Lensing Mass Calibration of ACTPol Sunyaev-Zel'dovich Clusters with the Hyper Suprime-Cam Survey
• de Sitter Swampland, $H_0$ tension & observation
• Electroweak bubble wall expansion: gravitational waves and baryogenesis in Standard Model-like thermal plasma
• The Tip of the Red Giant Branch Distances to Type Ia Supernova Host Galaxies. IV. Color Dependence and Zero-Point Calibration
• Constraining the orbital eccentricity of inspiralling compact binary systems with Advanced LIGO
• 21-cm Fluctuations from Charged Dark Matter
• MUSE Analysis of Gas around Galaxies (MAGG) -- II: Metal-enriched halo gas around z~1 galaxies
• The dependence of convective core overshooting on stellar mass: semi-empirical determination using the diffusive approach with two different element mixtures
• Planck 2018 results. II. Low Frequency Instrument data processing
• Exotic energy injection with ExoCLASS: Application to the Higgs portal model and evaporating black holes
• Modelling the large scale structure of the Universe as a function of cosmology and baryonic physics
• Detection of the pairwise kinematic Sunyaev-Zel'dovich effect with BOSS DR11 and the Atacama Cosmology Telescope
• Self-Interacting Dark Matter Subhalos in the Milky Way's Tides
• Prethermalization Production of Dark Matter
• Low-Scale Leptogenesis in the Scotogenic Neutrino Mass Model
• When did Population III star formation end?
• Matter Bounce Scenario and the Dynamical aspects in f(Q,T) Gravity
• The X-shooter GRB afterglow legacy sample (XS-GRB)
• Planck 2015 results. III. LFI systematic uncertainties
• Search for dark matter annihilation signals in the H.E.S.S. Inner Galaxy Survey
• The Influence of Streaming Velocities on the Formation of the First Stars
• Turbulent Cold Flows Gave Birth to the First Quasars
• The imprint of neutrinos on clustering in redshift-space
• Density split statistics: joint model of counts and lensing in cells
• Improving Helium Abundance Determinations with Leo P as a Case Study
• Survey geometry and the internal consistency of recent cosmic shear measurements
• The KLEVER Survey: Spatially resolved metallicity maps and gradients in a sample of 1.2 < z < 2.5 lensed galaxies
• Dynamical system analysis for accelerating models in non-metricity $f(Q)$ gravity
• Perturbation, Non-Gaussianity and Reheating in a GB-$\alpha$-Attractor Model
• Constraints on the mass-richness relation from the abundance and weak lensing of SDSS clusters
• Insensitivity of The Distance Ladder Hubble Constant Determination to Cepheid Calibration Modeling Choices
• Combination of searches for invisible decays of the Higgs boson using 139 fb${}^{-1}$ of proton-proton collision data at $\sqrt{s}=13$ TeV collected with the ATLAS experiment
• Dark Energy Survey Year 1 Results: Curved-Sky Weak Lensing Mass Map
• On the observability of individual Population III stars and their stellar-mass black hole accretion disks through cluster caustic transits
• Parameter estimation with gravitational waves
• The Three Hundred Project: Backsplash galaxies in simulations of clusters
• BBN constraints on MeV-scale dark sectors. Part II. Electromagnetic decays
• Physical effects involved in the measurements of neutrino masses with future cosmological data
• The influence of streaming velocities and Lyman-Werner radiation on the formation of the first stars
• The Foundation Supernova Survey: Measuring Cosmological Parameters with Supernovae from a Single Telescope
• Rotation curves of high-resolution LSB and SPARC galaxies with fuzzy and multistate (ultra-light boson) scalar field dark matter
• Primordial Black Holes as Dark Matter: Converting Constraints from Monochromatic to Extended Mass Distributions
• Probing Cosmic Dawn with Emission Lines: Predicting Infrared and Nebular Line Emission for ALMA and JWST
• QCD Axion Dark Matter with a Small Decay Constant
• Planck 2015 results. V. LFI calibration
• Parameter estimation for binary black holes with networks of third generation gravitational-wave detectors
• Recovering a MOND-like acceleration law in mimetic gravity
• A Distant Fast Radio Burst Associated to its Host Galaxy with the Very Large Array
• Parameter estimation for heavy binary-black holes with networks of second-generation gravitational-wave detectors
• Direct Search for Dark Matter Axions Excluding ALP Cogenesis in the 63-67 micro-eV Range, with The ORGAN Experiment
• The M101 Satellite Luminosity Function and the Halo to Halo Scatter Among Local Volume Hosts
• The Palatini side of inflationary attractors
• 2MTF VI. Measuring the velocity power spectrum
• Cosmology and dark energy from joint gravitational wave-GRB observations
• Quasars That Have Transitioned from Radio-quiet to Radio-loud on Decadal Timescales Revealed by VLASS and FIRST
• 21CMMC with a 3D light-cone: the impact of the co-evolution approximation on the astrophysics of reionisation and cosmic dawn
• Quantifying the $S_8$ tension with the Redshift Space Distortion data set
• From the far-ultraviolet to the far-infrared -- galaxy emission at $0\le z\le 10$ in the Shark semi-analytic model
• Deflection angle of photon through dark matter by black holes and wormholes using the Gauss-Bonnet theorem
• New constraints on time-dependent variations of fundamental constants using Planck data
• Long-lived Heavy Neutrinos from Higgs Decays
• How to Quench a Dwarf Galaxy: The Impact of Inhomogeneous Reionization on Dwarf Galaxies and Cosmic Filaments
• Search for intermediate mass black hole binaries in the first observing run of Advanced LIGO
• Testing the general theory of relativity using gravitational wave propagation from dark standard sirens
• Cosmic reionization after Planck II: contribution from quasars
• Search for a narrow resonance lighter than 200 GeV decaying to a pair of muons in proton-proton collisions at $\sqrt{s}=$ 13 TeV
• In-vacuo-dispersion features for GRB neutrinos and photons
• An independent determination of the local Hubble constant
• Has JWST already falsified dark-matter-driven galaxy formation?
• How to constrain warm dark matter with the Lyman $\alpha$ forest
• Cosmic acceleration in dust only Universe via energy-momentum powered gravity
• The Most Massive Galaxies and Black Holes Allowed by $\Lambda$CDM
• Determining $H_0$ with Bayesian hyper-parameters
• Absolute HST Proper Motion (HSTPROMO) of Distant Milky Way Globular Clusters: Galactocentric Space Velocities and the Milky Way Mass
• First Cosmological Constraint on the Effective Theory of Dark Matter-Proton Interactions
• Reionization optical depth determination from Planck HFI data with ten percent accuracy
• The Galaxy Power Spectrum and Bispectrum in Redshift Space
• A light in the dark: searching for electromagnetic counterparts to black hole-black hole mergers in LIGO/Virgo O3 with the Zwicky Transient Facility
• First test of Verlinde's theory of Emergent Gravity using Weak Gravitational Lensing measurements
• Cosmological parameter constraints for Horndeski scalar-tensor gravity
• Dark calling Dark: Interaction in the dark sector in presence of neutrino properties after Planck CMB final release
• Primordial black holes dark matter from inflection point models of inflation and the effects of reheating
• Thermal Dark Matter Below an MeV
• Strong late-time circumstellar interaction in the peculiar supernova iPTF14hls
• Mining Gravitational-wave Catalogs To Understand Binary Stellar Evolution: A New Hierarchical Bayesian Framework
• Novel constraints on non-cold (non-thermal) Dark Matter from Lyman-$\alpha$ forest data
• From Planck data to Planck era: Observational tests of Holographic Cosmology
• The route to massive black hole formation via merger-driven direct collapse: a review
• Status of Dark Matter in the Universe
• COSMOS2020: The cosmic evolution of the stellar-to-halo mass relation for central and satellite galaxies up to z~5
• Precise Time Delays from Strongly Gravitationally Lensed Type Ia Supernovae with Chromatically Microlensed Images
• The Most Massive Binary Black Hole Detections and the Identification of Population Outliers
• Analysing the 21cm signal from the Epoch of Reionization with artificial neural networks
• AMICO galaxy clusters in KiDS-DR3: sample properties and selection function
• The origin of the mass discrepancy-acceleration relation in $\Lambda$CDM
• The Diversity of Kilonova Emission in Short Gamma-Ray Bursts
• Search for dark matter particle interactions with electron final states with DarkSide-50
• Search for sterile neutrinos in holographic dark energy cosmology: Reconciling Planck observation with the local measurement of the Hubble constant
• BBN constraints on the annihilation of MeV-scale dark matter
• Consistent lensing and clustering in a low-$S_8$ Universe with BOSS, DES Year 3, HSC Year 1 and KiDS-1000
• Quantifying scatter in galaxy formation at the lowest masses
• Substructure of fuzzy dark matter haloes
• Cover Your Basis: Comprehensive Data-Driven Characterization of the Binary Black Hole Population
• Hubble tension or a transition of the Cepheid SnIa calibrator parameters?
• The Emergence of Structure in the Binary Black Hole Mass Distribution
• Emulation of reionization simulations for Bayesian inference of astrophysics parameters using neural networks
• Search for intermediate mass black hole binaries in the third observing run of Advanced LIGO and Advanced Virgo
• Inflationary theory and pulsar timing investigations of primordial black holes and gravitational waves
• PBH dark matter from axion inflation
• Reconstructing Gravity on Cosmological Scales
• SDSS-IV MaNGA: stellar population gradients as a function of galaxy environment
• State-of-the-Art Calculation of the Decay Rate of Electroweak Vacuum in Standard Model
• Evidence for suppression of structure growth in the concordance cosmological model
• Impact of neutrino properties on the estimation of inflationary parameters from current and future observations
• The cosmic evolution of dust-corrected metallicity in the neutral gas
• 400 pc Imaging of a Massive Quasar Host Galaxy at a Redshift of 6.6
• AGN Feedback and Star Formation of Quasar Host Galaxies: Insights from the Molecular Gas
• Are stellar-mass black-hole binaries too quiet for LISA?
• The peculiar velocity field up to $z\sim 0.05$ by forward-modeling Cosmicflows-3 data
• Impacts of gravitational-wave standard siren observation of the Einstein Telescope on weighing neutrinos in cosmology
• New observational constraints on $f(T)$ gravity through gravitational-wave astronomy
• Constraints on Cosmological Parameters from the 500 deg${}^2$ SPTpol Lensing Power Spectrum
• A Deep Learning Approach to Galaxy Cluster X-ray Masses
• Fast galaxy bars continue to challenge standard cosmology
• Cosmology in the era of Euclid and the Square Kilometre Array
• Primordial black holes and associated gravitational waves in axion monodromy inflation
• A new measurement of the Hubble constant and matter content of the Universe using extragalactic background light $\gamma$-ray attenuation
• The Case for an EeV Gravitino
• Dark compact objects: an extensive overview
• New CMB constraints for Abelian Higgs cosmic strings
• Constraints on $\Lambda$CDM Extensions from the SPT-3G 2018 $EE$ and $TE$ Power Spectra
• Gravitational wave production from preheating: parameter dependence
• Wandering Supermassive Black Holes in Milky Way Mass Halos
• The synergy between CMB spectral distortions and anisotropies
• Massive donors in interacting binaries: effect of metallicity
• Loop corrections to dark matter direct detection in a pseudoscalar mediator dark matter model
• H${}_2$-based star formation laws in hierarchical models of galaxy formation
• Kinematics of Circumgalactic Gas: Feeding Galaxies and Feedback
• UNIT project: Universe $N$-body simulations for the Investigation of Theoretical models from galaxy surveys
• Bouncing cosmologies with dark matter and dark energy
• Cosmological viable models in $f(T,B)$ gravity as solutions to the $H_0$ tension
• Pseudoscalar Mediators: A WIMP model at the Neutrino Floor
• The SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: final Emission Line Galaxy Target Selection
• Dark matter self-interactions from a general spin-0 mediator
• Future CMB tests of dark matter: ultra-light axions and massive neutrinos
• Probing multiple populations of compact binaries with third-generation gravitational-wave detectors
• Non-Abelian Dark Forces and the Relic Densities of Dark Glueballs
• Baryon Asymmetry and Gravitational Waves from Pseudoscalar Inflation
• keV Sterile Neutrino Dark Matter from Singlet Scalar Decays: The Most General Case
• AX-GADGET: a new code for cosmological simulations of Fuzzy Dark Matter and Axion models
• Observational constraints on the tilted spatially-flat and the untilted nonflat $\varphi$CDM dynamical dark energy inflation models
• An Improved Method to Measure the Cosmic Curvature
• Legacy of star formation in the pre-reionization universe
• Astrophysics and cosmology with a decihertz gravitational-wave detector: TianGO
• Prospects for Measuring Cosmic Microwave Background Spectral Distortions in the Presence of Foregrounds
• Internal Robustness of Growth Rate data
• PSZ2LenS. Weak lensing analysis of the Planck clusters in the CFHTLenS and in the RCSLenS
• Emulation of baryonic effects on the matter power spectrum and constraints from galaxy cluster data
• IGM damping wing constraints on reionisation from covariance reconstruction of two $z\gtrsim 7$ QSOs
• Anomaly-Free Dark Matter Models are not so Simple
• Going, going, gone dark: Quantifying the scatter in the faintest dwarf galaxies
• Axion Quasiparticles for Axion Dark Matter Detection
• The dependence of cosmic ray driven galactic winds on halo mass
• Dark sectors with dynamical coupling
• Constraining heavy dark matter with cosmic-ray antiprotons
• Anisotropies in the astrophysical gravitational-wave background: Predictions for the detection of compact binaries by LIGO and Virgo
• Black Hole -- Galaxy Correlations in Simba
• Heating of Milky Way disc Stars by Dark Matter Fluctuations in Cold Dark Matter and Fuzzy Dark Matter Paradigms
• Where do the AMS-02 anti-helium events come from?
• The Kinematic Sunyaev-Zel'dovich Effect with Projected Fields II: prospects, challenges, and comparison with simulations
• Inflation and High-Scale Supersymmetry with an EeV Gravitino
• Angular Baryon Acoustic Oscillation measure at z=2.225 from the SDSS quasar survey
• Radiative Production of Non-thermal Dark Matter
• A High-Resolution View of Fast Radio Burst Host Environments
• The Birth Mass Function of Pop III Stars
• THESEUS: a key space mission concept for Multi-Messenger Astrophysics
• Inflation meets neutrinos
• Frequency-Dependent Responses in 3rd Generation Gravitational-Wave Detectors
• Planck 2015 results. XVIII. Background geometry & topology
• Dark Sirens to Resolve the Hubble-Lemaître Tension
• A designer approach to $f(Q)$ gravity and cosmological implications
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: theoretical systematics and Baryon Acoustic Oscillations in the galaxy correlation function
• Discovery of Magnetic Fields Along Stacked Cosmic Filaments as Revealed by Radio and X-Ray Emission
• Dynamical systems approach and generic properties of $f(T)$ cosmology
• Flavor effects in leptogenesis
• A tale of two sites -- I: Inferring the properties of minihalo-hosted galaxies from current observations
• The XMM Cluster Outskirts Project (X-COP): Thermodynamic properties of the Intracluster Medium out to $R_{200}$ in Abell 2319
• Effective Theory of WIMP Dark Matter supplemented by Simplified Models: Singlet-like Majorana fermion case
• Planck 2015 constraints on the non-flat $\Lambda$CDM inflation model
• Hints of a Local Matter Underdensity or Modified Gravity in the Low $z$ Pantheon data
• Observing intermediate-mass black holes and the upper--stellar-mass gap with LIGO and Virgo
• Mapping the kinetic Sunyaev-Zel'dovich effect toward MACS J0717.5+3745 with NIKA
• Reionization after JWST: a photon budget crisis?
• Invisible Neutrino Decay Resolves IceCube's Track and Cascade Tension
• Testing the binary hypothesis: pulsar timing constraints on supermassive black hole binary candidates
• Cosmology in cubic and $f(P)$ gravity
• The Horizon Run 5 Cosmological Hydrodynamic Simulation: Probing Galaxy Formation from Kilo- to Giga-parsec Scales
• Constraining the primordial black hole abundance with 21cm cosmology
• The impact of the cosmic variance on $H_0$ on cosmological analyses
• Non-minimal gravitational reheating during kination
• Unraveling the effective fluid approach for $f(R)$ models in the subhorizon approximation
• Baseline Metal Enrichment from Population III Star Formation in Cosmological Volume Simulations
• Cosmic particle colliders: simulations of self-interacting dark matter with anisotropic scattering
• General Physical Properties of CGRaBS Blazars
• Evidence for Emergent Dark Energy
• Gas and galaxies in filament between clusters of galaxies: The study of A399-A401
• Dynamics of black hole - neutron star binaries in young star clusters
• The Void Size Function in Dynamical Dark Energy Cosmologies
• Feedback reshapes the baryon distribution within haloes, in halo outskirts, and beyond: the closure radius from dwarfs to massive clusters
• Hyper Suprime-Cam Year 3 Results: Cosmology from Galaxy Clustering and Weak Lensing with HSC and SDSS using the Minimal Bias Model
• The angular momentum-mass relation: a fundamental law from dwarf irregulars to massive spirals
• Probabilistic Association of Transients to their Hosts (PATH)
• Massive Stellar Triples Leading to Sequential Binary Black-Hole Mergers in the Field
• Modeling evolution of dark matter substructure and annihilation boost
• Cosmological Constraints on Horndeski Gravity in Light of GW170817
• All-inclusive interacting dark sector cosmologies
• Linking galaxy structural properties and star formation activity to black hole activity with IllustrisTNG
• Let there be Light Dark Matter: The gauged $U(1{)}_{L_{\mu }-L_{\tau }}$ case
• A massive blow for $\Lambda$CDM $-$ the high redshift, mass, and collision velocity of the interacting galaxy cluster El Gordo contradicts concordance cosmology
• The impact of ultra-light axion self-interactions on the large scale structure of the Universe
• Primordial Black Hole Evaporation and Dark Matter Production: II. Interplay with the Freeze-In/Out Mechanism
• Subtracting compact binary foreground sources to reveal primordial gravitational-wave backgrounds
• Probing Dark Low-mass Halos and Primordial Black Holes with Frequency-dependent Gravitational Lensing Dispersions of Gravitational Waves
• Dark matter axion detection in the radio/mm-waveband
• The spatially resolved broad line region of IRAS 09149-6206
• Semi-analytic forecasts for JWST -- IV. Implications for cosmic reionization and LyC escape fraction
• Emerging spatial curvature can resolve the tension between high-redshift CMB and low-redshift distance ladder measurements of the Hubble constant
• A comparison between short GRB afterglows and AT2017gfo: shedding light on kilonovae properties
• Upper Bound of Neutrino Masses from Combined Cosmological Observations and Particle Physics Experiments
• A model with interaction of dark components and recent observational data
• Obstructions to Bell CMB Experiments
• Search and analysis of giant radio galaxies with associated nuclei (SAGAN) -- I : New sample and multi-wavelength studies
• Model-independent test of the FLRW metric, the flatness of the Universe, and non-local measurement of $H_0{r}_{\mathrm{d}}$
• Looking through the same lens: shear calibration for LSST, Euclid & WFIRST with stage 4 CMB lensing
• Probing Leptogenesis
• Probing cosmic anisotropy with gravitational waves as standard sirens
• A VLT/FORS2 view at $z\sim 6$: Lyman-$\alpha$ emitter fraction and galaxy physical properties at the edge of the epoch of cosmic reionization
• Assessing tension metrics with Dark Energy Survey and Planck data
• H-alpha emission in local galaxies: star formation, time variability and the diffuse ionized gas
• Current observations are insufficient to confidently associate the binary black hole merger GW190521 with AGN J124942.3+344929
• Quantum Field Theory of Interacting Dark Matter/Dark Energy: Dark Monodromies
• The Spectrum of the Universe
• A luminosity distribution for kilonovae based on short gamma-ray burst afterglows
• Heavy neutrino production via $Z^{\prime }$ at the lifetime frontier
• The WISSH quasars Project: II. Giant star nurseries in hyper-luminous quasars
• Forecasts for detecting the gravitational-wave memory effect with Advanced LIGO and Virgo
• Searching for dark matter - dark energy interactions: going beyond the conformal case
• Scalar Field Dark Matter: Helping or Hurting Small-Scale Problems in Cosmology?
• The central parsec of NGC 3783: a rotating broad emission line region, asymmetric hot dust structure, and compact coronal line region
• Effects of neutrino mass hierarchies on dynamical dark energy models
• Multi-Messenger Time Delays from Lensed Gravitational Waves
• Quantum corrections to quartic inflation with a non-minimal coupling: metric vs. Palatini
• Escape of ionizing radiation from high redshift dwarf galaxies: role of AGN feedback
• Picky Partners: The Pairing of Component Masses in Binary Black Hole Mergers
• Star Cluster Formation in Cosmological Simulations. II. Effects of Star Formation Efficiency and Stellar Feedback
• The Three Hundred Project: Dynamical state of galaxy clusters and morphology from multi-wavelength synthetic maps
• The Massive and Distant Clusters of WISE Survey. I: Survey Overview and a Catalog of >2000 Galaxy Clusters at z~1
• A study of the sensitivity of shape measurements to the input parameters of weak lensing image simulations
• $H_0$ tension as a hint for a transition in gravitational theory
• Enrichment of the hot intracluster medium: observations
• Dispersion Measure Variation of Repeating Fast Radio Burst Sources
• Interpreting LOFAR 21-cm signal upper limits at z~9.1 in the context of high-z galaxy and reionisation observations
• A Minimalist Feedback-Regulated Model for Galaxy Formation During the Epoch of Reionization
• Observational constraints on generalized Proca theories
• Ultra-light axions and the $S_8$ tension: joint constraints from the cosmic microwave background and galaxy clustering
• Reconciling $H_0$ tension in a six parameter space?
• Resurrecting Quadratic Inflation with a non-minimal coupling to gravity
• Density profiles of ultracompact minihalos: Implications for constraining the primordial power spectrum
• The Aurora radiation-hydrodynamical simulations of reionization: calibration and first results
• Quantum-gravitational effects on gauge-invariant scalar and tensor perturbations during inflation: The slow-roll approximation
• And yet it flips: connecting galactic spin and the cosmic web
• Measurements of $H_0$ in modified gravity theories: The role of lensed quasars in the late-time Universe
• Properties of gas phases around cosmic filaments at z=0 in the Illustris-TNG simulation
• FAST-PT II: an algorithm to calculate convolution integrals of general tensor quantities in cosmological perturbation theory
• Heating of the intergalactic medium by the cosmic microwave background during cosmic dawn
• Evidence for Late-stage Eruptive Mass-loss in the Progenitor to SN2018gep, a Broad-lined Ic Supernova: Pre-explosion Emission and a Rapidly Rising Luminous Transient
• A frame independent classification of single field inflationary models
• The mass gap, the spin gap, and the origin of merging binary black holes
• Testing coupled dark energy models with their cosmological background evolution
• Is the expansion of the universe accelerating? All signs point to yes
• Galaxy Bispectrum from Massive Spinning Particles
• \textsc{The Three Hundred} project: The \textsc{Gizmo-Simba} run
• Dynamical dark energy: scalar fields and running vacuum
• Simply split SIMPs
• The impact of the observed baryon distribution in haloes on the total matter power spectrum
• Populations of filaments from the distribution of galaxies in numerical simulations
• Dark energy equation of state parameter and its variation at low redshifts
• A new diagnostic for the null test of dynamical dark energy in light of DESI 2024 and other BAO data
• Coleman-Weinberg linear inflation: metric vs. Palatini formulation
• Cosmological Analysis of Three-Dimensional BOSS Galaxy Clustering and Planck CMB Lensing Cross Correlations via Lagrangian Perturbation Theory
• Gaia17biu/SN 2017egm in NGC 3191: The closest hydrogen-poor superluminous supernova to date is in a "normal", massive, metal-rich spiral galaxy
• Primordial Black Hole Production in Inflationary Models of Supergravity with a Single Chiral Superfield
• Apparent cosmic acceleration from type Ia supernovae
• Effects of the surrounding primordial black holes on the merger rate of primordial black hole binaries
• Cosmological Constraints on Invisible Neutrino Decays Revisited
• When are LIGO/Virgo's Big Black-Hole Mergers?
• Constraint on energy-momentum squared gravity from neutron stars and its cosmological implications
• Status, Challenges and Directions in Indirect Dark Matter Searches
• Constraining the Inclination of Binary Mergers from Gravitational-wave Observations
• Search for strongly lensed counterpart images of binary black hole mergers in the first two LIGO observing runs
• Constraining Extended Scalar Sectors at the LHC and beyond
• New constraints on the magnetization of the cosmic web using LOFAR Faraday rotation observations
• Electroweak phase transition in the $\Sigma$SM - I: Dimensional reduction
• The mass-richness relation of optically-selected clusters from weak gravitational lensing and abundance with Subaru HSC first-year data
• A New Constraint on Reionization from Evolution of the Ly$\alpha$ Luminosity Function at $z\sim 6-7$ Probed by a Deep Census of $z=7.0$ Ly$\alpha$ Emitter Candidates to 0.3 $L^{\ast }$
• Accurate dust temperature determination in a $z=7.13$ galaxy
• The properties of He II 1640 emitters at z ~ 2.5-5 from the VANDELS survey
• The Evolution of the Lyman-Alpha Luminosity Function During Reionization
• Bounds on Dark Matter decay from 21 cm line
• Rates and Properties of Strongly Gravitationally Lensed Supernovae and their Host Galaxies in Time-Domain Imaging Surveys
• Formation of GW190521 via gas accretion onto Population III stellar black hole remnants born in high-redshift minihalos
• Oscillating Spin-2 Dark Matter
• Stochastic gravitational-wave background as a tool to investigate multi-channel astrophysical and primordial black-hole mergers
• Distorted Neutrino Oscillations From Ultralight Scalar Dark Matter
• Homeopathic Dark Matter, or how diluted heavy substances produce high energy cosmic rays
• The Impact of Scatter in the Galaxy UV Luminosity to Halo Mass Relation on Ly$\alpha$ Visibility During the Epoch of Reionization
• Cosmological constraints on neutrino self-interactions with a light mediator
• Search for dark matter produced in association with bottom or top quarks in $\sqrt{s}$ = 13 TeV pp collisions with the ATLAS detector
• Cosmological inference using only gravitational wave observations of binary neutron stars
• Indirect Detection of Neutrino Portal Dark Matter
• The XXL Survey XXV. Cosmological analysis of the C1 cluster number counts
• SILVERRUSH. VI. A simulation of Ly$\alpha$ emitters in the reionization epoch and a comparison with Subaru Hyper Suprime-Cam survey early data
• Higgsino Dark Matter or Not: Role of Disappearing Track Searches at the LHC and Future Colliders
• The Dramatic Size and Kinematic Evolution of Massive Early-Type Galaxies
• Simulating galaxies in the reionization era with FIRE-2: morphologies and sizes
• Are ultracompact minihalos really ultracompact?
• Inflation driven by Einstein-Gauss-Bonnet gravity
• $H_0$ Tension, Swampland Conjectures and the Epoch of Fading Dark Matter
• Measurement of the EBL spectral energy distribution using the VHE gamma-ray spectra of H.E.S.S. blazars
• The MillenniumTNG Project: High-precision predictions for matter clustering and halo statistics
• Experimental constraint on axion-like particle coupling over seven orders of magnitude in mass
• Phenomenology of Modified Gravity at Recombination
• Probing Primordial-Black-Hole Dark Matter with Gravitational Waves
• Effects of Anisotropic Stress in Interacting Dark Matter - Dark Energy Scenarios
• Cosmological discordances II: Hubble constant, Planck and large-scale-structure data sets
• Revisiting the Dark Photon Explanation of the Muon Anomalous Magnetic Moment
• The physics of gas phase metallicity gradients in galaxies
• MUSE Analysis of Gas around Galaxies (MAGG) -- III: The gas and galaxy environment of z = 3-4.5 quasars
• A detailed analysis of GW190521 with phenomenological waveform models
• Probing primordial features with future galaxy surveys
• The Irreducible Axion Background
• Searching for the QCD Axion with Gravitational Microlensing
• The effective field theory approach of teleparallel gravity, $f(T)$ gravity and beyond
• On the early-time excess emission in hydrogen-poor superluminous supernovae
• $Euclid$ preparation: XV. Forecasting cosmological constraints for the $Euclid$ and CMB joint analysis
• First Constraint on the Neutrino-Induced Phase Shift in the BAO Spectrum
• Mining for Dark Matter Substructure: Inferring subhalo population properties from strong lenses with machine learning
• The Effects of Environment on the Evolution of the Galaxy Stellar Mass Function
• Mitigating Internal Instrument Coupling II: A Method Demonstration with the Hydrogen Epoch of Reionization Array
• Early- and late-stage mergers among main sequence and starburst galaxies at 0.2<z<2
• ALMA [CI]${}^3{P}_1{-}^3{P}_0$ observations of NGC6240: a puzzling molecular outflow, and the role of outflows in the global ${\alpha }_{\mathrm{CO}}$ factor of (U)LIRGs
• HOLISMOKES -- II. Identifying galaxy-scale strong gravitational lenses in Pan-STARRS using convolutional neural networks
• Hunting Black Holes with Gaia
• Cosmological constraints on post-Newtonian parameters in effectively massless scalar-tensor theories of gravity
• Constraints on scalar-tensor theory of gravity by the recent observational results on gravitational waves
• The Evolution and Properties of Rotating Massive Star Populations
• Intergalactic medium dispersion measures of fast radio bursts estimated from IllustrisTNG simulation and their cosmological applications
• Implications from ASKAP Fast Radio Burst Statistics
• Is cosmic acceleration proven by local cosmological probes?
• Strong evidence for an accelerating universe
• How to Find Gravitationally Lensed Type Ia Supernovae
• On the impact of $f(Q)$ gravity on the Large Scale Structure
• IMAGINE: A comprehensive view of the interstellar medium, Galactic magnetic fields and cosmic rays
• A Detection of the Baryon Acoustic Oscillation Features in the SDSS BOSS DR12 Galaxy Bispectrum
• Coupled quintessence with a $\Lambda$CDM background: removing the ${\sigma }_8$ tension
• Dust scaling relations in a cosmological simulation
• PyUltraLight: A Pseudo-Spectral Solver for Ultralight Dark Matter Dynamics
• Improving time-delay cosmography with spatially resolved kinematics
• Primordial perturbations from inflation with a hyperbolic field-space
• The THESAN project: ionizing escape fractions of reionization-era galaxies
• Analysis of the Yukawa gravitational potential in $f(R)$ gravity I: semiclassical periastron advance
• Relieving the Tension between Weak Lensing and Cosmic Microwave Background with Interacting Dark Matter and Dark Energy Models
• Cosmological Constraints on Interacting Light Particles
• Spectral distortion constraints on photon injection from low-mass decaying particles
• Constraining the time evolution of dark energy, curvature and neutrino properties with cosmic chronometers
• Cosmological Simulations for Combined-Probe Analyses: Covariance and Neighbour-Exclusion Bias
• First detection of stacked X-ray emission from cosmic web filaments
• On the spatial distribution of neutral hydrogen in the Universe: bias and shot-noise of the HI Power Spectrum
• The ALMA Spectroscopic Survey in the HUDF: the molecular gas content of galaxies and tensions with IllustrisTNG and the Santa Cruz SAM
• A little FABLE: exploring AGN feedback in dwarf galaxies with cosmological simulations
• Lower Mass Bounds on FIMP Dark Matter Produced via Freeze-In
• H0 tension or T0 tension?
• The diverse dark matter density at sub-kiloparsec scales in Milky Way satellites:implications for the nature of dark matter
• Cosmic voids in modified gravity models with massive neutrinos
• Trinity I: Self-Consistently Modeling the Dark Matter Halo-Galaxy-Supermassive Black Hole Connection from $z=0-10$
• A Near-Infrared Period-Luminosity Relation for Miras in NGC 4258, an Anchor for a New Distance Ladder
• Bias due to neutrinos must not uncorrect'd go
• Search for intermediate mass black hole binaries in the first and second observing runs of the Advanced LIGO and Virgo network
• How baryons affect halos and large-scale structure: a unified picture from the Simba simulation
• Probing the Early Universe with Axion Physics and Gravitational Waves
• Long Lived Light Scalars as Probe of Low Scale Seesaw Models
• Tension of the $E_G$ statistic and RSD data with Planck/$\Lambda$CDM and implications for weakening gravity
• Updating the (Supermassive Black Hole Mass) - (Spiral Arm Pitch Angle) Relation: A Strong Correlation for Galaxies with Pseudobulges
• Linear spectropolarimetry of 35 Type Ia Supernovae with VLT/FORS: An analysis of the Si II line polarization
• Constraining a dark matter and dark energy interaction scenario with a dynamical equation of state
• GW$\times$LSS: Chasing the Progenitors of Merging Binary Black Holes
• Circumgalactic Mg II Emission from an Isotropic Starburst Galaxy Outflow Mapped by KCWI
• The next decade of black hole spectroscopy
• Spin evolution and feedback of supermassive black holes in cosmological simulations
• Constraining the UV emissivity of AGN throughout cosmic time via X-ray surveys
• High-redshift quasars and their host galaxies I: kinematical and dynamical properties and their tracers
• Relativistic N-body simulations with massive neutrinos
• Gravitational wave forest from string axiverse
• Exploring Cosmic Origins with CORE: B-mode Component Separation
• Cosmological constraints on parametrized interacting dark energy
• Reionization in Technicolor
• Bubble size statistics during reionization from 21-cm tomography
• A Low Lyman Continuum Escape Fraction of $<10\%$ for Extreme [OIII] Emitters in an Overdensity at z$\sim 3.5$
• CMB constraints on primordial black hole dark matter
• On the road to percent accuracy IV: ReACT -- computing the non-linear power spectrum beyond $\Lambda$CDM
• Combined analysis of Planck and SPTPol data favors the early dark energy models
• Axion Dark Matter Search around 4.55 $\mu$eV with Dine-Fischler-Srednicki-Zhitnitskii Sensitivity
• Constraint on the abundance of primordial black holes in dark matter from Planck data
• A tale of two populations: surviving and destroyed dwarf galaxies and the build up of the Milky Way's stellar halo
• CMB Delensing Beyond the B Modes
• Analysis of the Yukawa gravitational potential in $f(R)$ gravity II: relativistic periastron advance
• Early mass varying neutrino dark energy: Nugget formation and Hubble anomaly
• Dissecting the Local Environment of FRB 190608 in the Spiral Arm of its Host Galaxy
• Positivity in the sky
• Molecular Gas Contents and Scaling Relations for Massive Passive Galaxies at Intermediate Redshifts from the LEGA-C Survey
• The maximum accretion rate of hot gas in dark matter halos
• High-redshift post-reionization cosmology with 21cm intensity mapping
• The Berkeley sample of Type II supernovae: BVRI light curves and spectroscopy of 55 SNe II
• Sterile Neutrinos with Secret Interactions -- Cosmological Discord?
• Metal-poor star formation triggered by the feedback effects from Pop III stars
• The Dark Matter equation of state through cosmic history
• Impact of Resonance on Thermal Targets for Invisible Dark Photon Searches
• The dust-continuum size of TNG50 galaxies at $z=1-5$: a comparison with the distribution of stellar light, stars, dust and H${}_2$
• Gamma Ray Burst afterglow and prompt-afterglow relations: an overview
• New universal attractor in nonmininally coupled gravity: Linear inflation
• The Role of Galaxies and AGN in Reionising the IGM - I: Keck Spectroscopy of 5 < z < 7 Galaxies in the QSO Field J1148+5251
• The impact of stellar feedback on the density and velocity structure of the interstellar medium
• The Fast Radio Burst Luminosity Function and Death Line in the Low-Twist Magnetar Model
• Microlensing of Extremely Magnified Stars near Caustics of Galaxy Clusters
• Formation of the first stars and black holes
• Two can play at that game: constraining the role of supernova and AGN feedback in dwarf galaxies with cosmological zoom-in simulations
• The effect of Limber and flat-sky approximations on galaxy weak lensing
• The Globular Cluster - Dark Matter Halo Connection
• DeepCMB: Lensing Reconstruction of the Cosmic Microwave Background with Deep Neural Networks
• Outlook for detecting the gravitational wave displacement and spin memory effects with current and future gravitational wave detectors
• Quantum Gravity in the Sky: Interplay between fundamental theory and observations
• Tests and problems of the standard model in Cosmology
• The WISSH QSOs project IX. Cold gas content and environment of luminous QSOs at z~2.4-4.7
• RAVE J203843.2-002333: The first highly r-process-enhanced star identified in the RAVE survey
• Searches for dark photons at accelerators
• $A_4$ Flavour Model for Dirac Neutrinos: Type I and Inverse Seesaw
• Constraints on dark photons and axion-like particles from SuperCDMS Soudan
• Prospects for indirect dark matter searches with MeV photons
• Near-Infrared Spectroscopy of Galaxies During Reionization: Measuring CIII] in a Galaxy at $\mathbf{z}=7.5$
• Ages and masses of million Galactic disk main sequence turn-off and sub-giant stars from the LAMOST Galactic spectroscopic surveys
• Cosmological Forecasts for Combined and Next Generation Peculiar Velocity Surveys
• Exploring cosmic homogeneity with the BOSS DR12 galaxy sample
• An Updated Tomographic Analysis of the Integrated Sachs-Wolfe Effect and implications for Dark Energy
• The fate of disk galaxies in IllustrisTNG clusters
• Mini-quenching of $z=4-8$ galaxies by bursty star formation
• Tensor Non-Gaussianity from Axion-Gauge-Fields Dynamics : Parameter Search
• Cross-correlating Planck CMB lensing with SDSS: Lensing-lensing and galaxy-lensing cross-correlations
• Structure Formation and Exotic Compact Objects in a Dissipative Dark Sector
• The Lyman-$\alpha$ forest as a diagnostic of the nature of the dark matter
• X-ray Signatures of Black Hole Feedback: Hot Galactic Atmospheres in IllustrisTNG and X-ray Observations
• Reproducing sub-millimetre galaxy number counts with cosmological hydrodynamic simulations
• Looking at cosmic near-infrared background radiation anisotropies
• The Onset of Gravothermal Core Collapse in Velocity Dependent Self-Interacting Dark Matter Subhaloes
• Swampland Conjectures and Late-Time Cosmology
• Multipole analysis of redshift-space distortions around cosmic voids
• CLEAR I: Ages and Metallicities of Quiescent Galaxies at $1.0<\mathbf{z}<1.8$ Derived from Deep Hubble Space Telescope Grism Data
• Neutrinoless Double Beta Decay and the Baryon Asymmetry of the Universe
• Measuring the Hubble constant and spatial curvature from supernova apparent magnitude, baryon acoustic oscillation, and Hubble parameter data
• The Bright and the Slow -- GRBs 100724B \& 160509A with high-energy cutoffs at $\lesssim 100$MeV
• Improving fast generation of halo catalogs with higher-order Lagrangian perturbation theory
• The THESAN project: predictions for multi-tracer line intensity mapping in the epoch of reionization
• A Geometrical Upper Bound on the Inflaton Range
• Probing Light Dark Matter with a Hadrophilic Scalar Mediator
• Directional limits on persistent gravitational waves using data from Advanced LIGO's first two observing runs
• The ALMA Spectroscopic Survey in the HUDF: The Cosmic Dust and Gas Mass Densities in Galaxies up to $z\sim 3$
• Light-curve models of black hole - neutron star mergers: steps towards a multi-messenger parameter estimation
• Pulsar Timing Array Based Search for Supermassive Black Hole Binaries in the Square Kilometer Array Era
• Enabling Forbidden Dark Matter
• Exploring Features in the Binary Black Hole Population
• Neutrino oscillations: the rise of the PMNS paradigm
• The Need for Speed: Escape velocity and dynamical mass measurements of the Andromeda galaxy
• Catalogues of Active Galactic Nuclei From Gaia and unWISE Data
• Constraining cosmic curvature by using age of galaxies and gravitational lenses
• Minimal Gauged U(1)${}_{L_{\alpha }-L_{\beta }}$ Models Driven into a Corner
• Rational approximations of $f(R)$ cosmography through Padé polynomials
• Observational Constraints on New Exact Inflationary Scalar-field Solutions
• Multifractional theories: an unconventional review
• Observational constraints on interacting Tsallis holographic dark energy models
• Demonstration of Single Barium Ion Sensitivity for Neutrinoless Double Beta Decay using Single Molecule Fluorescence Imaging
• Erasing the Milky Way: new cleaning technique applied to GBT intensity mapping data
• Constraining the astrophysics and cosmology from 21cm tomography using deep learning with the SKA
• Stochastic Gravitational Wave Background from Global Cosmic Strings
• The Higgs Portal to Cosmology
• Running vacuum in the Universe: phenomenological status in light of the latest observations, and its impact on the ${\sigma }_8$ and $H_0$ tensions
• Strong FUV fields drive the [CII]/FIR deficit in z~3 dusty, star-forming galaxies
• Consistency of the growth rate in different environments with the 6dF Galaxy Survey: measurement of the void-galaxy and galaxy-galaxy correlation functions
• Full parameter scan of the Zee model: exploring Higgs lepton flavor violation
• Massive Warm/Hot Galaxy Coronae: II. Isentropic Model
• A Program for Multi-Messenger Standard Siren Cosmology in the Era of LIGO A+, Rubin Observatory, and Beyond
• Breaking degeneracies in modified gravity with higher (than 2nd) order weak-lensing statistics
• Does Matter Matter? Using the mass distribution to distinguish neutron stars and black holes
• MGCAMB with massive neutrinos and dynamical dark energy
• Properties of the stochastic astrophysical gravitational wave background: astrophysical sources dependencies
• 21cm foregrounds and polarization leakage: a user's guide on cleaning and mitigation strategies
• Uncertainties in WIMP Dark Matter Scattering Revisited
• The Future of Primordial Features with Large-Scale Structure Surveys
• First Sunyaev-Zel'dovich mapping with the NIKA2 camera: Implication of cluster substructures for the pressure profile and mass estimate
• Hubble Frontier Fields: systematic errors in strong lensing models of galaxy clusters - Implications for cosmography
• Towards a measurement of the spectral runnings
• Topology and Geometry of Gaussian random fields I: on Betti Numbers, Euler characteristic and Minkowski functionals
• Gravitational waves from Population III binary black holes formed by dynamical capture
• The Impact of Microlensing on the Standardisation of Strongly Lensed Type Ia Supernovae
• Suppressing structure formation at dwarf galaxy scales and below: late kinetic decoupling as a compelling alternative to warm dark matter
• The Persistence of Population III Star Formation
• The Effects of Population III X-ray and Radio Backgrounds on the Cosmological 21-cm Signal
• Asymmetric thermal-relic dark matter: Sommerfeld-enhanced freeze-out, annihilation signals and unitarity bounds
• CMB weak-lensing beyond the Born approximation: a numerical approach
• Gravitational wave cosmology with extreme mass-ratio inspirals
• Weak Lensing Light-Cones in Modified Gravity simulations with and without Massive Neutrinos
• The SDSS-DR12 large-scale cross-correlation of Damped Lyman Alpha Systems with the Lyman Alpha Forest
• Large-scale structure phenomenology of viable Horndeski theories
• Standardized long gamma-ray bursts as a cosmic distance indicator
• Observational evidence for a local underdensity in the Universe and its effect on the measurement of the Hubble Constant
• Cosmological Constraints on Decoupled Dark Photons and Dark Higgs
• Gravitational waves from the asymmetric-dark-matter generating phase transition
• Searching for Anisotropic Cosmic Birefringence with Polarization Data from SPTpol
• Phenomenology of fermion production during axion inflation
• A measurement of the Hubble constant from angular diameter distances to two gravitational lenses
• Dark Matter Production in an Early Matter Dominated Era
• Ricci-Gauss-Bonnet holographic dark energy
• Multi-messenger observations of binary neutron star mergers in the O4 run
• Hybrid loop quantum cosmology and predictions for the cosmic microwave background
• Search for subsolar-mass binaries in the first half of Advanced LIGO and Virgo's third observing run
• Three-Flavoured Non-Resonant Leptogenesis at Intermediate Scales
• Cosmological discordances: a new measure, marginalization effects, and application to geometry vs growth current data sets
• Think Global, Act Local: The Influence of Environment Age and Host Mass on Type Ia Supernova Light Curves
• Assessing the tension between a black hole dominated early universe and leptogenesis
• Ups and Downs in Dark Energy: phase transition in dark sector as a proposal to lessen cosmological tensions
• Freezing-in dark matter through a heavy invisible $Z^{\prime }$
• Impacts of dark energy on weighing neutrinos: mass hierarchies considered
• Velocity Dependence from Resonant Self-Interacting Dark Matter
• Detecting Dark Matter with Far-Forward Emulsion and Liquid Argon Detectors at the LHC
• Galaxy metallicities depend primarily on stellar mass and molecular gas mass
• Dynamical Dark Matter from Strongly-Coupled Dark Sectors
• Precision Scaling Relations for Disk Galaxies in the Local Universe
• Dawn of the dark: unified dark sectors and the EDGES Cosmic Dawn 21-cm signal
• Planck's dusty GEMS. VI. Multi-J CO excitation and interstellar medium conditions in dusty starburst galaxies at z=2-4
• A Comparison of Cosmological Parameters Determined from CMB Temperature Power Spectra from the South Pole Telescope and the Planck Satellite
• Probing dark matter annihilation in the Galaxy with antiprotons and gamma rays
• Reconciling mass-estimates of ultra-diffuse galaxies
• Inhomogeneous Cosmology with Numerical Relativity
• The PAU Survey: Early demonstration of photometric redshift performance in the COSMOS field
• Prospects for detecting gravitational waves at 5 Hz with ground-based detectors
• Modelling Kepler Red Giants in Eclipsing Binaries:Calibrating the Mixing Length Parameter with Asteroseismology
• Barrow agegraphic dark energy
• Constraining f(R) gravity in solar system, cosmology and binary pulsar systems
• Geometric Inflation
• Phenomenology of the generalized cubic covariant Galileon model and cosmological bounds
• Top-philic dark matter within and beyond the WIMP paradigm
• Late time transitions in the quintessence field and the $H_0$ tension
• Tagging a jet from a dark sector with Jet-substructures at colliders
• Simulation-Based Inference of Reionization Parameters From 3D Tomographic 21 cm Lightcone Images
• Cosmology from large scale galaxy clustering and galaxy-galaxy lensing with Dark Energy Survey Science Verification data
• Constant-Roll (Quasi-)Linear Inflation
• Deconstructing the neutrino mass constraint from galaxy redshift surveys
• Constraining the redshifted 21-cm signal with the unresolved soft X-ray background
• Five-percent measurements of the growth rate from simulation-based modelling of redshift-space clustering in BOSS LOWZ
• A Comprehensive Study of Ly$\alpha$ Emission in the High-redshift Galaxy Population
• The Three Hundred Project: correcting for the hydrostatic-equilibrium mass bias in X-ray and SZ surveys
• Multi-mode black hole spectroscopy
• Cosmological constraints on the neutrino mass including systematic uncertainties
• Higgs Portals for Thermal Dark Matter - EFT Perspectives and the NMSSM -
• Simulating the dynamics and non-thermal emission of relativistic magnetised jets I. Dynamics
• A Search for Neutron Star-Black Hole Binary Mergers in the Short Gamma-Ray Burst Population
• Reconstruction of the remote dipole and quadrupole fields from the kinetic Sunyaev Zel'dovich and polarized Sunyaev Zel'dovich effects
• Cosmology with the Large Synoptic Survey Telescope: an Overview
• LoTSS/HETDEX: Optical quasars I. Low-frequency radio properties of optically selected quasars
• The intergalactic magnetic field probed by a giant radio galaxy
• An FRB Sent Me a DM: Constraining the Electron Column of the Milky Way Halo with Fast Radio Burst Dispersion Measures from CHIME/FRB
• Reionization and Galaxy Formation in Warm Dark Matter Cosmologies
• Euclid: Forecasts from redshift-space distortions and the Alcock-Paczynski test with cosmic voids
• The inert doublet model in the light of Fermi-LAT gamma-ray data: a global fit analysis
• The X-ray emission of z>2.5 active galactic nuclei can be obscured by their host galaxies
• Remedy of some cosmological tensions via effective phantom-like behavior of interacting vacuum energy
• Falsifying $\Lambda$CDM: Model-independent tests of the concordance model with eBOSS DR14Q and Pantheon
• Exploring reionisation and high-z galaxy observables with recent multi-redshift MWA upper limits on the 21-cm signal
• Optimal identification of HII regions during reionization in 21-cm observations
• Singlet-Doublet Dark Matter Freeze-in: LHC displaced signatures versus cosmology
• Using SPTpol, Planck 2015, and non-CMB data to constrain tilted spatially-flat and untilted non-flat $\Lambda$CDM, XCDM, and $\varphi$CDM dark energy inflation cosmologies
• A comparative study of host galaxy properties between Fast Radio Bursts and stellar transients
• Energy functions of fast radio bursts derived from the first CHIME/FRB catalogue
• Predictions for deep galaxy surveys with JWST from $\Lambda$CDM
• The mean H$\alpha$ EW and Lyman-continuum photon production efficiency for faint $z\approx 4-5$ galaxies
• Closing in on Resonantly Produced Sterile Neutrino Dark Matter
• Statistics of Dark Matter Substructure: III. Halo-to-Halo Variance
• Evidence for galaxy assembly bias in BOSS CMASS redshift-space galaxy correlation function
• Test-particle dynamics in general spherically symmetric black hole spacetimes
• A predictive model of BEC dark matter halos with a solitonic core and an isothermal atmosphere
• The Importance of Quantum Pressure of Fuzzy Dark Matter on Lyman-Alpha Forest
• Extracting host galaxy dispersion measure and constraining cosmological parameters using fast radio burst data
• The Radial Acceleration Relation in CLASH Galaxy Clusters
• A LOFAR study of non-merging massive galaxy clusters
• Cosmological parameters, shear maps and power spectra from CFHTLenS using Bayesian hierarchical inference
• Einstein's Universe: Cosmological structure formation in numerical relativity
• The Implications of a Pre-reionization 21 cm Absorption Signal for Fuzzy Dark Matter
• Physical properties and evolution of (Sub-)millimeter selected galaxies in the galaxy formation simulation Shark
• $T_0$ censorship of early dark energy and AdS vacua
• After The Fall: The Dust and Gas in E+A Post-Starburst Galaxies
• CCCP and MENeaCS: (updated) weak-lensing masses for 100 galaxy clusters
• Bose-Einstein-condensed scalar field dark matter and the gravitational wave background from inflation: new cosmological constraints and its detectability by LIGO
• The FRB 20121102A November rain in 2018 observed with the Arecibo Telescope
• Validating estimates of the growth rate of structure with modified gravity simulations
• Full-Shape Galaxy Power Spectra and the Curvature Tension
• Galaxy formation with L-GALAXIES: Modelling the environmental dependency of galaxy evolution and comparing with observations
• Quasar outflows at $z\ge 6$: the impact on the host galaxies
• Multi-Component Dark Matter: the vector and fermion case
• The impact of the connectivity of the cosmic web on the physical properties of galaxies at its nodes
• Cosmology and the neutrino mass ordering
• A radiative seesaw model with three Higgs doublets in modular $A_4$ symmetry
• Cosmological constraints on alternative model to Chaplygin fluid revisited
• Morphologies of ~190,000 Galaxies at z=0-10 Revealed with HST Legacy Data. III. Continuum Profile and Size Evolution of Lya Emitters
• From actinides to zinc: Using the full abundance pattern of the brightest star in Reticulum II to distinguish between different r-process sites
• The 2014 TeV Gamma-ray Flare of Mrk 501 Seen with H.E.S.S.: Temporal and Spectral Constraints on Lorentz Invariance Violation
• Probing the Hot X-ray Corona around the Massive Spiral Galaxy, NGC 6753, Using Deep XMM-Newton observations
• Making a supermassive star by stellar bombardment
• Cosmological Forecast for non-Gaussian Statistics in large-scale weak Lensing Surveys
• HDUV: The Hubble Deep UV Legacy Survey
• Constraints on dark matter self-interaction from the internal density profiles of X-COP galaxy clusters
• The Swift/BAT AGN Spectroscopic Survey -- IX. The Clustering Environments of an Unbiased Sample of Local AGN
• HI and cosmological constraints from intensity mapping, optical, and CMB surveys
• The effect of the deforming dark matter haloes of the Milky Way and the Large Magellanic Cloud on the Orphan-Chenab stream
• Determination of the primordial helium abundance based on NGC 346 an HII region of the Small Magellanic Cloud
• Planck intermediate results. L. Evidence for spatial variation of the polarized thermal dust spectral energy distribution and implications for CMB $B$-mode analysis
• GA-NIFS: The core of an extremely massive proto-cluster at the Epoch of Reionization probed with JWST/NIRSpec
• Gamma-ray Emitting Narrow Line Seyfert 1 Galaxies in The Sloan Digital Sky Survey
• An inventory of galaxies in cosmic filaments feeding galaxy clusters: galaxy groups, backsplash galaxies, and pristine galaxies
• Robustness of baryon acoustic oscillation constraints for early-Universe modifications to $\Lambda$CDM
• Five new real-time detections of Fast Radio Bursts with UTMOST
• Ain't No Mountain High Enough: Semi-Parametric Modeling of LIGO-Virgos Binary Black Hole Mass Distribution
• Towards geometric inflation: the cubic case
• Cylindrical Systems in General Relativity
• Knocking on giants' doors: I. The evolution of the dust-to-stellar mass ratio in distant dusty galaxies
• Asymmetric dark matter: residual annihilations and self-interactions
• Axion Miniclusters in Modified Cosmological Histories
• Black Hole Mass Measurements of Radio Galaxies NGC 315 and NGC 4261 Using ALMA CO Observations
• The Infrared Emission and Opening Angle of the Torus in Quasars
• Universe's Worth of Electrons to Probe Long-Range Interactions of High-Energy Astrophysical Neutrinos
• Primordial Features from Linear to Nonlinear Scales
• Machine learning cosmological structure formation
• In search of the dark matter dark energy interaction: a kinematic approach
• Relaxing the ${\sigma }_8$-tension through running vacuum in the Universe
• Seeding the Second Star: enrichment from population III, dust evolution, and cloud collapse
• Linear Seesaw for Dirac Neutrinos with $A_4$ Flavour Symmetry
• Attractor Behaviour in Multifield Inflation
• Testing H0 in Acoustic Dark Energy Models with Planck and ACT Polarization
• Cosmological Measurements from Angular Power Spectra Analysis of BOSS DR12 Tomography
• GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run
• A flexible modelling of galaxy assembly bias
• Results from EDGES High-Band: III. New Constraints on Parameters of the Early Universe
• Constraining black hole mimickers with gravitational wave observations
• Model-independent reconstruction of $f(T)$ teleparallel cosmology
• The Megamaser Cosmology Project.IX. Black hole masses for three maser galaxies
• Primordial perturbations generated by Higgs field and $R^2$ operator
• Stellar binary black holes in the LISA band: a new class of standard sirens
• Advancing LHC Probes of Dark Matter from the Inert 2-Higgs Doublet Model with the Mono-jet Signal
• The mass-metallicity relations for gas and stars in star-forming galaxies: strong outflow vs variable IMF
• Strong Bayesian Evidence for the Normal Neutrino Hierarchy
• Constraining Warm Inflation with CMB data
• A Thermal Neutrino Portal to Sub-MeV Dark Matter
• Exploring cosmic origins with CORE: gravitational lensing of the CMB
• Scalar-field dark energy nonminimally and kinetically coupled to dark matter
• Radiative Neutrino Mass & Majorana Dark Matter within an Inert Higgs Doublet Model
• The atomic Hydrogen content of the post-reionization Universe
• Inferring the star formation histories of the most massive and passive early-type galaxies at z<0.3
• BBN constraints on MeV-scale dark sectors. Part I. Sterile decays
• Modeling $237$ Lyman-$\alpha$ spectra of the MUSE-Wide survey
• Conjoined constraints on modified gravity from the expansion history and cosmic growth
• String Theory and the Dark Glueball Problem
• Search for Boosted Dark Matter Interacting With Electrons in Super-Kamiokande
• A Search for Dark Matter Annihilation in Galaxy Groups
• Phase Portraits of general f(T) Cosmology
• The Circumgalactic Medium of Milky Way-like Galaxies in the TNG50 Simulation -- I: Halo Gas Properties and the Role of SMBH Feedback
• The rest-frame optical (900nm) galaxy luminosity function at z~4-7: abundance matching points to limited evolution in the Mstar/Mhalo ratio at z>4
• Do current cosmological observations rule out all Covariant Galileons?
• Independent Cosmological Constraints from high-z HII Galaxies
• Cosmological constraints from thermal Sunyaev Zeldovich power spectrum revisited
• The XMM Cluster Outskirts Project (X-COP): Physical conditions to the virial radius of Abell 2142
• KiDS+2dFLenS+GAMA: Testing the cosmological model with the $E_{\mathrm{G}}$ statistic
• CLUMPY v3: $\gamma$-ray and $\nu$ signals from dark matter at all scales
• Spatial fluctuations of the intergalactic temperature-density relation after hydrogen reionization
• SPIDERS: Selection of spectroscopic targets using AGN candidates detected in all-sky X-ray surveys
• Statistical properties of paired fixed fields
• Dark matter from gravitational particle production at reheating
• Unique Signatures of Population III Stars in the Global 21-cm Signal
• Critical Number of Fields in Stochastic Inflation
• Dark Neutrino interactions phase out the Hubble tension
• Non-Gaussian Enhancements of Galactic Halo Correlations in Quasi-Single Field Inflation
• Ruling out the light WIMP explanation of the galactic 511 keV line
• Neutrino masses and beyond-$\Lambda$CDM cosmology with LSST and future CMB experiments
• Quenching timescales of dwarf satellites around Milky Way-mass hosts
• Independent cosmological constraints from high-z HII galaxies: new results from VLT-KMOS data
• Search for CII Emission on Cosmological Scales at Redshift Z~2.6
• Modelling Void Abundance in Modified Gravity
• Statistical Inconsistencies in the KiDS-450 Dataset
• Light dark states with electromagnetic form factors
• Decay Rate of Electroweak Vacuum in the Standard Model and Beyond
• The coherent motion of Cen A dwarf satellite galaxies remains a challenge for $\Lambda$CDM cosmology
• Incompleteness Matters Not: Inference of $H_0$ from BBH-galaxy cross-correlations
• The Clustering of Galaxies in the Completed SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from DR12 galaxy clustering -- towards an accurate model
• Strong constraints from COSINE-100 on the DAMA dark matter results using the same sodium iodide target
• H0LiCOW II. Spectroscopic survey and galaxy-group identification of the strong gravitational lens system HE0435-1223
• The imprint of cosmic reionisation on the luminosity function of galaxies
• A comparison of Einstein-Boltzmann solvers for testing General Relativity
• Primordial backgrounds of relic gravitons
• CGM${}^2$ I: The Extent of the Circumgalactic Medium Traced by Neutral Hydrogen
• Semi-analytic forecasts for JWST -- VI. Simulated lightcones and galaxy clustering predictions
• Short-Range Neutrinoless Double Beta Decay Mechanisms
• Production of keV Sterile Neutrinos in Supernovae: New Constraints and Gamma Ray Observables
• The MUSE Ultra Deep Field (MUDF). II. Survey design and the gaseous properties of galaxy groups at 0.5 < z < 1.5
• Collapsed Dark Matter Structures
• The fundamental signature of star formation quenching from AGN feedback: A critical dependence of quiescence on supermassive black hole mass not accretion rate
• Concordance cosmology without dark energy
• The angular power spectrum of the diffuse gamma-ray emission as measured by the Fermi Large Area Telescope and constraints on its Dark Matter interpretation
• Systematic bias on parameterized tests of general relativity due to neglect of orbital eccentricity
• The impact of relativistic effects on cosmological parameter estimation
• Repeating and Non-repeating Fast Radio Bursts from Binary Neutron Star Mergers
• Properties of Dark Matter Halos as a Function of Local Environment Density
• MUSE Analysis of Gas around Galaxies (MAGG) -- I: Survey design and the environment of a near pristine gas cloud at z~3.5
• The contribution from stars stripped in binaries to cosmic reionization of hydrogen and helium
• Planck 2015 constraints on the non-flat $\varphi$CDM inflation model
• Joint gravitational wave -- gamma-ray burst detection rates in the aftermath of GW170817
• Characterising filaments in the SDSS volume from the galaxy distribution
• Testing extreme-axion wave dark matter using the BOSS Lyman-Alpha forest data
• Inflation in a scale invariant universe
• The Dark $L_{\mu }-L_{\tau }$ Rises via Kinetic Mixing
• Search for new particles decaying to a jet and an emerging jet
• Axion-Photon Conversion and Effects on 21cm Observation
• Public Release of A-SLOTH: Ancient Stars and Local Observables by Tracing Halos
• LISA parameter estimation and source localization with higher harmonics of the ringdown
• Model-independent Curvature Determination from Gravitational-Wave Standard Sirens and Cosmic Chronometers
• A large sample of shear selected clusters from the Hyper Suprime-Cam Subaru Strategic Program S16A wide field mass maps
• Crossing SNe Ia and BAO observational constraints with local ones in hybrid metric-Palatini gravity
• Gauss-Bonnet Chern-Simons gravitational wave leptogenesis
• HST/WFC3 grism observations of $z\sim 1$ clusters: The cluster vs. field stellar mass-size relation and evidence for size growth of quiescent galaxies from minor mergers
• Constraints on interacting dark energy models through cosmic chronometers and Gaussian process
• A Search for Fast Radio Bursts with the GBNCC Pulsar Survey
• Charged rotating black holes coupled with nonlinear electrodynamics Maxwell field in the mimetic gravity
• The Little Engines That Could? Globular Clusters Contribute Significantly to Reionization-era Star Formation
• Mapping the Real Space Distributions of Galaxies in SDSS DR7: II. Measuring the growth rate, clustering amplitude of matter and biases of galaxies at redshift $0.1$
• LATIS: The Ly$\alpha$ Tomography IMACS Survey
• Weighing neutrinos in the scenario of vacuum energy interacting with cold dark matter: application of the parameterized post-Friedmann approach
• Dark Energy Stars in Tolman-Kuchowicz spacetime in the context of Einstein Gravity
• Formation of primordial black holes in an axionlike curvaton model
• KiDS+GAMA: Constraints on Horndeski gravity from combined large-scale structure probes
• Dynamics of nonlinear interacting dark energy models
• DEMNUni: Massive neutrinos and the bispectrum of large scale structures
• Data-driven Reconstruction of the Late-time Cosmic Acceleration with f(T) Gravity
• Gravitino Decay in High Scale Supersymmetry with R-parity Violation
• Bayesian delensing of CMB temperature and polarization
• Explore Inert Dark Matter Blind Spots with Gravitational Wave Signatures
• Improved Constraints on Sterile Neutrinos in the MeV to GeV Mass Range
• Forming massive seed black holes in high-redshift quasar host progenitors
• Fundamental physics with the Hubble Frontier Fields: constraining Dark Matter models with the abundance of extremely faint and distant galaxies
• A New Precision Measurement of the Small-Scale Line-of-Sight Power Spectrum of the Ly$\alpha$ Forest
• Probing modified gravity theories and cosmology using gravitational-waves and associated electromagnetic counterparts
• Finding cosmic voids and filament loops using topological data analysis
• An Analysis of ALMA Deep Fields and the Perceived Dearth of High-z Galaxies
• The Price of Shifting the Hubble Constant
• An evaluation of cosmological models from expansion and growth of structure measurements
• The distribution and morphologies of Fornax Cluster dwarf galaxies suggest they lack dark matter
• EPOCHS IV: SED Modelling Assumptions and their impact on the Stellar Mass Function at 6.5 < z < 13.5 using PEARLS and public JWST observations
• A search for the host galaxy of FRB171020
• The galaxy-halo connection of emission-line galaxies in IllustrisTNG
• Light axion-like dark matter must be present during inflation
• Cosmological neutrino simulations at extreme scale
• CHORUS II. Subaru/HSC Determination of the Ly$\alpha$ Luminosity Function at $z=7.0$: Constraints on Cosmic Reionization Model Parameter
• Intergalactic Lyman continuum photon budget in the past 5 billion years
• Connecting early and late epochs by f(z)CDM cosmography
• Void Lensing as a Test of Gravity
• An extremely energetic supernova from a very massive star in a dense medium
• Modeling Fast Radio Burst Dispersion and Scattering Properties in the First CHIME/FRB Catalog
• Early Structure Formation Constraints on the Ultra-Light Axion in the Post-Inflation Scenario
• Improved constraints on lepton asymmetry from the cosmic microwave background
• Model independent inference of the expansion history and implications for the growth of structure
• Changing the prior: absolute neutrino mass constraints in nonlocal gravity
• Dark Matter Deficient Galaxies Produced Via High-velocity Galaxy Collisions In High-resolution Numerical Simulations
• Constraining the Hubble constant to a precision of about 1% using multi-band dark standard siren detections
• EMERGE: Empirical predictions of galaxy merger rates since $z\sim 6$
• Galaxy Clusters from the DESI Legacy Imaging Surveys. I. Cluster Detection
• Doubly-Charged Scalars in the Type-II Seesaw Mechanism: Fundamental Symmetry Tests and High-Energy Searches
• Obscure Higgs boson at Colliders
• Measuring the transverse baryonic acoustic scale from the SDSS DR11 galaxies
• Stellar Photometric Structures of the Host Galaxies of Nearby Type 1 Active Galactic Nuclei
• The impact of quenching on galaxy profiles in the Simba simulation
• First evidence of diffuse ultra-steep-spectrum radio emission surrounding the cool core of a cluster
• Chirp Mass and Spin of Binary Black Holes from First Star Remnants
• Black hole-neutron star mergers are unlikely multi-messenger sources
• The Herschel Bright Sources (HerBS): Sample definition and SCUBA-2 observations
• Constraining First Star Formation with 21cm-Cosmology
• Cosmological implications of scale-independent energy-momentum squared gravity: Pseudo nonminimal interactions in dark matter and relativistic relics
• Primordial Black Hole Formation During Slow Reheating After Inflation
• Cosmic viscosity as a remedy for tension between PLANCK and LSS data
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: constraining modified gravity
• First upper limits on the 21 cm signal power spectrum from cosmic dawn from one night of observations with NenuFAR
• An analytic implementation of the IR-resummation for the BAO peak
• Signatures of primordial black holes as seeds of supermassive black holes
• Line intensity mapping with [CII] and CO(1-0) as probes of primordial non-Gaussianity
• Constraints on a generalized deceleration parameter from cosmic chronometers
• Emulating galaxy clustering and galaxy-galaxy lensing into the deeply nonlinear regime: methodology, information, and forecasts
• Unifying leptogenesis, dark matter and high-energy neutrinos with right-handed neutrino mixing via Higgs portal
• The Aemulus Project V: Cosmological constraint from small-scale clustering of BOSS galaxies
• The Atacama Cosmology Telescope: Detection of the Pairwise Kinematic Sunyaev-Zel'dovich Effect with SDSS DR15 Galaxies
• Time-dependent behaviour of quasar proximity zones at $z\sim 6$
• The Three Hundred Project: The evolution of galaxy cluster density profiles
• Testing Modified Gravity with Wide Binaries in GAIA DR2
• AIC and BIC for cosmological interacting scenarios
• On the Gas Content, Star Formation Efficiency, and Environmental Quenching of Massive Galaxies in Proto-Clusters at z~2.0-2.5
• Precise measurements of inflationary features with 21 cm observations
• Beyond-mean-field approaches for nuclear neutrinoless double beta decay in the standard mechanism
• General Physical Properties of Gamma-ray Emitting Narrow-Line Seyfert 1 Galaxies
• Modeling the large-scale redshift-space 3-point correlation function of galaxies
• Classifying the Large Scale Structure of the Universe with Deep Neural Networks
• The Vev Flip-Flop: Dark Matter Decay between Weak Scale Phase Transitions
• HICOSMO - Cosmology with a complete sample of galaxy clusters: II. Cosmological results
• The history of star formation from the cosmic infrared background anisotropies
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: a tomographic analysis of structure growth and expansion rate from anisotropic galaxy clustering
• Efficient simulations of large scale structure in modified gravity cosmologies with comoving Lagrangian acceleration
• The cumulative star-formation histories of dwarf galaxies with TNG50. I: Environment-driven diversity and connection to quenching
• Mg II Absorption at 2<z<7 with Magellan/FIRE, III. Full Statistics of Absorption Towards 100 High-Redshift QSOs
• Hunting On- and Off-Axis for Light Dark Matter with DUNE-PRISM
• The baryon content of groups and clusters of galaxies in the FABLE simulations
• Dynamical evolution of cosmic supermassive binary black holes and their gravitational wave radiation
• How to assess the primordial origin of single gravitational-wave events with mass, spin, eccentricity, and deformability measurements
• Luminous Millimeter, Radio, and X-ray Emission from ZTF20acigmel (AT2020xnd)
• Connecting the X-ray properties of weak-line and typical quasars: testing for a geometrically thick accretion disk
• Systematic light curve modelling of TDEs: statistical differences between the spectroscopic classes
• Constraining Teleparallel Gravity through Gaussian Processes
• Resolving shocks and filaments in galaxy formation simulations: effects on gas properties and star formation in the circumgalactic medium
• Challenging bulk viscous unified scenarios with cosmological observations
• A Space-Based Observational Strategy for Characterizing the First Stars and Galaxies Using the Redshifted 21-cm Global Spectrum
• Gravitational-wave detection and parameter estimation for accreting black-hole binaries and their electromagnetic counterpart
• Spatially Resolved [CII] Emission in SPT0346-52: A Hyper-Starburst Galaxy Merger at z~5.7
• Self-interacting inelastic dark matter: A viable solution to the small scale structure problems
• A flexible subhalo abundance matching model for galaxy clustering in redshift space
• Dynamical analysis on $f(R,\mathcal{G})$ cosmology
• No strong dependence of Lyman continuum leakage on physical properties of star-forming galaxies at $3.1\lesssim \mathbf{z}\lesssim 3.5$
• Dark Matter Freeze-out During Matter Domination
• Supernova Host Galaxies in the Dark Energy Survey: I. Deep Coadds, Photometry, and Stellar Masses
• Gravitational Baryogenesis in Non-Minimal Coupled $f(R,T)$ Gravity
• Density and temperature of cosmic-web filaments on scales of tens of megaparsecs
• Neutrino propagation in the galactic dark matter halo
• The eROSITA Final Equatorial-Depth Survey (eFEDS): X-ray Properties and Scaling Relations of Galaxy Clusters and Groups
• Calibration of bias and scatter involved in cluster mass measurements using optical weak gravitational lensing
• Model-independent limits and constraints on extended theories of gravity from cosmic reconstruction techniques
• Scalar-torsion theories of gravity I: general formalism and conformal transformations
• Disentangling the Cosmic Web Towards FRB 190608
• 3D simulations with boosted primordial power spectra and ultracompact minihalos
• Tests of Gravitational-Wave Birefringence with the Open Gravitational-Wave Catalog
• The $H_0$ and ${\sigma }_8$ tensions and the scale invariant spectrum
• The merger and assembly histories of Milky Way- and M31-like galaxies with TNG50: disk survival through mergers
• CLEAR: Emission Line Ratios at Cosmic High Noon
• Cosmological Bounds on Non-Abelian Dark Forces
• On standardizing kilonovae and their use as standard candles to measure the Hubble constant
• SN2020bvc: a Broad-lined Type Ic Supernova with a Double-peaked Optical Light Curve and a Luminous X-ray and Radio Counterpart
• A precise deuterium abundance: Re-measurement of the z=3.572 absorption system towards the quasar PKS1937-101
• Mass and rate of hierarchical black hole mergers in young, globular and nuclear star clusters
• Bayesian statistical framework for identifying strongly lensed gravitational-wave signals
• An iterative reconstruction of cosmological initial density fields
• Exploring SMBH Assembly with Semi-analytic Modelling
• The Clustering of High-Redshift (2.9 $\le$ z $\le$ 5.1) Quasars in SDSS Stripe 82
• Expectations of the size evolution of massive galaxies at $3\le z\le 6$ from the TNG50 simulation: the CEERS/JWST view
• Lepton-Flavored Electroweak Baryogenesis
• Performance of the Quasar Spectral Templates for the Dark Energy Spectroscopic Instrument
• Partially Acoustic Dark Matter Cosmology and Cosmological Constraints
• Cosmological constraints on coupled dark energy
• Constraints on Spin-Dependent Dark Matter Scattering with Long-Lived Mediators from TeV Observations of the Sun with HAWC
• Constraints on the time variation of the gravitational constant using gravitational-wave observations of binary neutron stars
• Tracing Black Hole and Galaxy Co-evolution in the Romulus Simulations
• Euclid preparation: XIX. Impact of magnification on photometric galaxy clustering
• The Dark Side of the Littlest Seesaw: freeze-in, the two right-handed neutrino portal and leptogenesis-friendly fimpzillas
• Cosmic Microwave Background constraints for global strings and global monopoles
• The impact of EDGES 21-cm data on dark matter interactions
• Interpreting IceCube 6-year HESE data as an evidence for hundred TeV decaying Dark Matter
• A comparison of the R_h=ct and LCDM cosmologies using the Cosmic Distance Duality Relation
• Exploring neutrino mass and mass hierarchy in the scenario of vacuum energy interacting with cold dark matter
• Dark energy scenario consistent with GW170817 in theories beyond Horndeski gravity
• Variable Chaplygin gas cosmologies in f(R, T) gravity with particle creation
• Dark matter spike around Bumblebee black holes
• Constraining the Cosmology of the Phantom Brane using Distance Measures
• A Foreground Masking Strategy for [CII] Intensity Mapping Experiments Using Galaxies Selected by Stellar Mass and Redshift
• The Three Hundred Project: Ram pressure and gas content of haloes and subhaloes in the phase-space plane
• Cosmological data favor Galileon ghost condensate over $\Lambda$CDM
• R-parity as a residual gauge symmetry : probing a theory of cosmological dark matter
• A panchromatic spatially resolved analysis of nearby galaxies -- II. The main sequence - gas relation at sub-kpc scale in grand-design spirals
• Search for new physics in dijet angular distributions using proton-proton collisions at $\sqrt{s}=$ 13 TeV and constraints on dark matter and other models
• Observational constraints on Gauss-Bonnet cosmology
• Superluminous Supernovae in LSST: Rates, Detection Metrics, and Light Curve Modeling
• Model-independent estimations for the curvature from standard candles and clocks
• Witnessing galaxy assembly in an extended z~3 structure
• Can Non-standard Recombination Resolve the Hubble Tension?
• Ages and Masses of 0.64 million Red Giant Branch stars from the LAMOST Galactic Spectroscopic Survey
• Fitting the nonlinear matter bispectrum by the Halofit approach
• ALMA 200 pc imaging of a z~7 quasar reveals a compact, disk-like host galaxy
• The COS CGM Compendium. III: Metallicity and Physical Properties of the Cool Circumgalactic Medium at z<1
• Modeling dark matter subhalos in a constrained galaxy: Global mass and boosted annihilation profiles
• Scalar-torsion theories of gravity II: $L(T,X,Y,\varphi )$ theory
• Accurate emulator for the redshift-space power spectrum of dark matter halos and its application to galaxy power spectrum
• CONCERTO: High-fidelity simulation of millimeter line emissions of galaxies and [CII] intensity mapping
• Measuring the Innermost Stable Circular Orbits of Supermassive Black Holes
• Supermassive Black Holes in the Early Universe
• Predicting FIR lines from simulated galaxies
• Extensions to models of the galaxy-halo connection
• A cosmological open quantum system
• H0LiCOW VIII. A weak lensing measurement of the external convergence in the field of the lensed quasar HE0435$-$1223
• A robust estimate of the Milky Way mass from rotation curve data
• Searching for cosmological gravitational-wave backgrounds with third-generation detectors in the presence of an astrophysical foreground
• The Faraday Rotation Measure Grid of the LOFAR Two-metre Sky Survey: Data Release 2
• Cosmological beam dump: constraints on dark scalars mixed with the Higgs boson
• Fermionic WIMPs and Vacuum Stability in the Scotogenic Model
• Supervised deep learning in high energy phenomenology: a mini review
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• Signatures of Dark Radiation in Neutrino and Dark Matter Detectors
• Quantum Anomalies in String-Inspired Running Vacuum Universe: Inflation and Axion Dark Matter
• Dark Energy Survey Year 3 Results: Calibration of Lens Sample Redshift Distributions using Clustering Redshifts with BOSS/eBOSS
• Thermalization of large energy release in the early Universe
• A Deep View of a Fossil Relic in the Galactic Bulge: The Globular Cluster HP1
• HYREC-2: a highly accurate sub-millisecond recombination code
• Positivity Bounds on Dark Energy: When Matter Matters
• Updated observing scenarios and multi-messenger implications for the International Gravitational-wave Network's O4 and O5
• Bardeen black hole surrounded by perfect fluid dark matter
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• Cosmology with galaxy-galaxy lensing on non-perturbative scales: Emulation method and application to BOSS LOWZ
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• IllustrisTNG in the HSC-SSP: image data release and the major role of mini mergers as drivers of asymmetry and star formation
• Measuring the growth rate of structure with Type IA Supernovae from LSST
• Planck 2015 constraints on the non-flat XCDM inflation model
• Anisotropy of the Universe via the Pantheon supernovae sample revisited
• Gravitational wave signatures of dark matter cores in binary neutron star mergers by using numerical simulations
• Construction of explicit symplectic integrators in general relativity. III. Reissner-Nordstrom-(anti)-de Sitter black holes
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• A fresh look into the interacting dark matter scenario
• Inflation in a closed universe
• Detecting higher spin fields through statistical anisotropy in the CMB and galaxy power spectra
• SHARP - V. Modelling gravitationally-lensed radio arcs imaged with global VLBI observations
• Realistic simulations of galaxy formation in f(R) modified gravity
• Detection of the Missing Baryons toward the Sightline of H1821+643
• Cosmological bounds on dark matter-photon coupling
• The Carnegie-Chicago Hubble Program. III. The Distance to NGC 1365 via the Tip of the Red Giant Branch
• Gamma-ray Astrophysics in the MeV Range: the ASTROGAM Concept and Beyond
• Reducing Noise in Cosmological N-body Simulations with Neutrinos
• A Simple Testable Model of Baryon Number Violation: Baryogenesis, Dark Matter, Neutron-Antineutron Oscillation and Collider Signals
• From a Bounce to the Dark Energy Era with $F(R)$ Gravity
• Constraints on Scalar and Tensor spectra from $N_{eff}$
• Near-Quantum-Noise Axion Dark Matter Search at CAPP around 9.5 $\mu$eV
• Measuring the circum- and inter-galactic baryon contents with fast radio bursts
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• Targeted large mass ratio numerical relativity surrogate waveform model for GW190814
• Charting the Parameter Space of the 21-cm Power Spectrum
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• Bumpy Declining Light Curves Are Common in Hydrogen-poor Superluminous Supernovae
• Effective field description of the Anton-Schmidt cosmic fluid
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• Gaussian processes reconstruction of modified gravitational wave propagation
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• Parameters Estimation for the Cosmic Microwave Background with Bayesian Neural Networks
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• Kilonova Emission From Black Hole-Neutron Star Mergers. II. Luminosity Function and Implications for Target-of-opportunity Observations of Gravitational-wave Triggers and Blind Searches
• Forecasts on dark energy from the X-ray cluster survey with eROSITA: constraints from counts and clustering
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• Inflation from Nilpotent Kähler Corrections
• LSST Target-of-Opportunity Observations of Gravitational Wave Events: Essential and Efficient
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• Constraining the Baryon Abundance with the Kinematic Sunyaev-Zel'dovich Effect: Projected-Field Detection Using Planck, WMAP, and unWISE
• Imprints of the Early Universe on Axion Dark Matter Substructure
• MaNGA DynPop -- I. Quality-assessed stellar dynamical modelling from integral-field spectroscopy of 10K nearby galaxies: a catalogue of masses, mass-to-light ratios, density profiles and dark matter
• Large-scale (in-) stability Analysis of an Exactly Solved Coupled Dark-Energy Model
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• Deep Extragalactic VIsible Legacy Survey (DEVILS): Identification of AGN through SED Fitting and the Evolution of the Bolometric AGN Luminosity Function
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• The COSMOS-UltraVISTA stellar-to-halo mass relationship: new insights on galaxy formation efficiency out to $z\sim 5$
• Euclid: The importance of galaxy clustering and weak lensing cross-correlations within the photometric Euclid survey
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• Dissection of the collisional and collisionless mass components in a mini sample of CLASH and HFF massive galaxy clusters at $z\approx 0.4$
• Does circumgalactic OVI trace low-pressure gas beyond the accretion shock? Clues from HI and low-ion absorption, line kinematics, and dust extinction
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• Accelerated and decelerated expansion in a causal dissipative cosmology
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• Multi-wavelength view of the close-by GRB 190829A sheds light on gamma-ray burst physics
• An analysis of the $H_0$ tension problem in a universe with a viscous dark fluid
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• Lensing Reconstruction in Post-Born Cosmic Microwave Background Weak Lensing
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• Sizes of Lensed Lower-luminosity z=4-8 Galaxies from the Hubble Frontier Field Program
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• Galaxy spin as a formation probe: the stellar-to-halo specific angular momentum relation
• Discovery of three self-lensing binaries from Kepler
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• Leptogenesis from Low Energy $CP$ Violation
• Evidence for radial variations in the stellar mass-to-light ratio of massive galaxies from weak and strong lensing
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• Are Starburst Galaxies Proton Calorimeters?
• Following the Cosmic Evolution of Pristine Gas II: The search for Pop III-Bright Galaxies
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• On combining information from multiple gravitational wave sources
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• Ruling out 3 keV warm dark matter using 21 cm-EDGES data
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• High redshift JWST predictions from IllustrisTNG: II. Galaxy line and continuum spectral indices and dust attenuation curves
• Phenomenology of scotogenic scalar dark matter
• GUT Physics in the era of the LHC
• FRW Cosmology in $f(Q,T)$ Gravity
• The Relativistic Jet Dichotomy and the End of the Blazar Sequence
• A metal-poor damped Ly-alpha system at redshift 6.4
• A dense, solar metallicity ISM in the z=4.2 dusty star-forming galaxy SPT0418-47
• Characteristic Properties of Two Different Viscous Cosmology Models for the Future Universe
• Characterization of Two 2mm-detected Optically-Obscured Dusty Star-Forming Galaxies
• Prediction of the 21-cm signal from reionization: comparison between 3D and 1D radiative transfer schemes
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• Viable Twin Cosmology from Neutrino Mixing
• Dark Energy Survey Year 1 Results: tomographic cross-correlations between DES galaxies and CMB lensing from SPT+Planck
• White Paper and Roadmap for Quantum Gravity Phenomenology in the Multi-Messenger Era
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• Cosmological Constraint on ${\Omega }_m$ and ${\sigma }_8$ from Cluster Abundances using the $GalWCat19$ Optical-Spectroscopic SDSS Catalog
• The road ahead of Horndeski: cosmology of surviving scalar-tensor theories
• Breaching the limit: formation of GW190521-like and IMBH mergers in young massive clusters
• Mass and Age of Red Giant Branch Stars Observed with LAMOST and \emph{Kepler}
• GridSPT: Grid-based calculation for perturbation theory of large-scale structure
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• Afterglow constraints on the viewing angle of binary neutron star mergers and determination of the Hubble constant
• Filamentary structures as the origin of blazar jet radio variability
• Massive Black Holes from Dissipative Dark Matter
• Constraining dark matter properties with Cosmic Microwave Background observations
• Planck 2015 constraints on spatially-flat dynamical dark energy models
• Time-varying neutrino mass from a supercooled phase transition: current cosmological constraints and impact on the ${\Omega }_m$-${\sigma }_8$ plane
• Gravitational wave from dark sector with dark pion
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• Intermediate-Mass Black Hole Growth and Feedback in Dwarf Galaxies at High Redshifts
• Solar $\gamma$-rays as a Complementary Probe of Dark Matter
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• SILVERRUSH. II. First Catalogs and Properties of ~2,000 Lya Emitters and Blobs at z~6-7 Identified over the 14-21 deg2 Sky
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• No redshift evolution of non-repeating fast radio-burst rates
• The Hubble constant from SN Refsdal
• Sommerfeld-Enhanced $J$-Factors For Dwarf Spheroidal Galaxies
• Scalar-Fluid interacting dark energy: cosmological dynamics beyond the exponential potential
• Merging stellar and intermediate-mass black holes in dense clusters: implications for LIGO, LISA and the next generation of gravitational wave detectors
• Origin and evolution of ultra-diffuse galaxies in different environments
• Probing Baryogenesis through the Higgs Self-Coupling
• Affine Inflation
• The discreet charm of higgsino dark matter - a pocket review
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• Baryonic effects on the matter bispectrum
• (Non-)thermal production of WIMPs during kination
• Particle Dark Matter Constraints: the Effect of Galactic Uncertainties
• Improving Weak Lensing Mass Map Reconstructions using Gaussian and Sparsity Priors: Application to DES SV
• Position-dependent power spectra of the 21-cm signal from the epoch of reionization
• On structure formation from a small-scales-interacting dark sector
• Noether symmetries and stability of ideal gas solution in Galileon Cosmology
• Seismic measurement of the locations of the base of convection zone and helium ionization zone for stars in the {\it Kepler} seismic LEGACY sample
• Cosmological constraints of phantom dark energy models
• The molecular gas content in obscured AGN at z > 1
• Reconstructing teleparallel gravity with cosmic structure growth and expansion rate data
• CMB Lensing Beyond the Power Spectrum: Cosmological Constraints from the One-Point PDF and Peak Counts
• Probing pseudo-Goldstone dark matter at the LHC
• FOREVER22: galaxy formation in protocluster regions
• Probing sub-GeV mass SIMP dark matter with a low-threshold surface experiment
• MUFASA: The assembly of the red sequence
• An Asymmetric TBM Texture
• A novel approach to quantifying the sensitivity of current and future cosmological datasets to the neutrino mass ordering through Bayesian hierarchical modeling
• Shedding light on the small-scale crisis with CMB spectral distortions
• Gravitational clustering of cosmic relic neutrinos in the Milky Way
• A Systematic Study of the Stochastic Gravitational-Wave Background due to Stellar Core Collapse
• CoMaLit-V. Mass forecasting with proxies. Method and application to weak lensing calibrated samples
• Hints of Modified Gravity in Cosmos and in the Lab?
• Can Early Dark Energy Explain EDGES?
• Hidden Charged Dark Matter and Chiral Dark Radiation
• Phantom matter: a challenging solution to the cosmological tensions
• Exploring the squeezed three-point galaxy correlation function with generalized halo occupation distribution models
• Enhancing BOSS bispectrum cosmological constraints with maximal compression
• A direct calibration of the IRX-β relation in Lyman-break Galaxies at z=3-5
• Translation and Rotation Equivariant Normalizing Flow (TRENF) for Optimal Cosmological Analysis
• Dark Energy Survey Year 1 Results: Constraining Baryonic Physics in the Universe
• Recovering the HII region size statistics from 21-cm tomography
• How does the cosmic large-scale structure bias the Hubble diagram?
• Planck confronts large scale structure: methods to quantify discordance
• Testing Dark energy models in the light of ${\sigma }_8$ tension
• Dark matter constraints from dwarf galaxies: a data-driven analysis
• Like a spider in its web: a study of the Large Scale Structure around the Coma cluster
• Osaka Feedback Model: Isolated Disk Galaxy Simulations
• Automated galaxy-galaxy strong lens modelling: no lens left behind
• Calculation of the local density of relic neutrinos
• Ubiquitous Molecular Outflows in z > 4 Massive, Dusty Galaxies I. Sample Overview and Clumpy Structure in Molecular Outflows on 500pc Scales
• Signature of inflation in the stochastic gravitational wave background generated by cosmic string networks
• ETHOS -- an effective theory of structure formation: predictions for the high-redshift Universe -- abundance of galaxies and reionization
• Measuring the cosmic proper distance from fast radio bursts
• What can we learn from the stochastic gravitational wave background produced by oscillons?
• Phantom cosmological model with observational constraints in $f(Q)$ gravity
• Deformed black hole immersed in dark matter spike
• Semi-analytic forecasts for JWST -- III. Intrinsic production efficiency of Lyman-continuum radiation
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• Cosmological constraints and comparison of viable $f(R)$ models
• Minimal but non-minimal inflation and electroweak symmetry breaking
• Finding Horndeski theories with Einstein gravity limits
• LyaCoLoRe: Synthetic Datasets for Current and Future Lyman-$\alpha$ Forest BAO Surveys
• The Host Galaxy and Rapidly Evolving Broad-line Region in the Changing-look Active Galactic Nucleus 1ES 1927+654
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• The Low Redshift Circumgalactic Medium in Simba
• SDSS-IV eBOSS Spectroscopy of X-ray and WISE AGN in Stripe 82X: Overview of the Demographics of X-ray and Mid-Infrared Selected Active Galactic Nuclei
• Probing Cosmic Reionization and Molecular Gas Growth with TIME
• Features from the non-attractor beginning of inflation
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• A Measurement of CMB Cluster Lensing with SPT and DES Year 1 Data
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• A general theory of linear cosmological perturbations: stability conditions, the quasistatic limit and dynamics
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• Time Delay Lens Modelling Challenge
• Optimizing EDELWEISS detectors for low-mass WIMP searches
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• The impact of stellar and AGN feedback on halo-scale baryonic and dark matter accretion in the EAGLE simulations
• A Sterile Neutrino Origin for the Upward Directed Cosmic Ray Showers Detected by ANITA
• Novel color center platforms enabling fundamental scientific discovery
• Model-independent measurement of cosmic curvature with the latest $H(z)$ and SNe Ia data: A comprehensive investigation
• Cosmological constraints with self-interacting sterile neutrinos
• Reannihilation of self-interacting dark matter
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• CP Violation in the Lepton Sector and Implications for Leptogenesis
• Probing gravity with a joint analysis of galaxy and CMB lensing and SDSS spectroscopy
• Bayesian Evidence against Harrison-Zel'dovich spectrum in tension cosmology
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• Absorption Line Spectroscopy of Gravitationally-Lensed Galaxies: Further Constraints on the Escape Fraction of Ionizing Photons at High Redshift
• Rapid late-time X-ray brightening of the tidal disruption event OGLE16aaa
• Improving geometric and dynamical constraints on cosmology with intrinsic alignments of galaxies
• Modelling and testing the equation of state for (Early) dark energy
• Latest astronomical constraints on some nonlinear parametric dark energy models
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• A small-scale dynamo in feedback-dominated galaxies - III. Cosmological simulations
• Physical insights from the spectrum of the radio halo in MACS J0717.5+3745
• Galactic angular momentum in the IllustrisTNG simulation -- I. Connection to morphology, halo spin, and black hole mass
• Intimate Relationship Between Sterile Neutrino Dark Matter and $\Delta N_{\mathrm{eff}}$
• A New Viable Region of Inert Higgs Doublet Dark Matter Model with Scotogenic Extension
• Cosmological Parameters from pre-Planck CMB Measurements: a 2017 Update
• Precision cosmology with redshift-space bispectrum: a perturbation theory based model at one-loop order
• Observational constraints of a new unified dark fluid and the $H_0$ tension
• Large host-galaxy dispersion measure of fast radio bursts
• A preliminary forecast for cosmological parameter estimation with gravitational-wave standard sirens from TianQin
• Cosmological parameter forecasts for HI intensity mapping experiments using the angular power spectrum
• Dynamics of the cosmological relaxation after reheating
• Baryonic Imprints on DM Halos: Population Statistics from Dwarf Galaxies to Galaxy Clusters
• The manifestation of secondary halo bias on the galaxy population from IllustrisTNG300
• Correlating the anomalous results in $b\to s$ decays with inert Higgs doublet dark matter and muon $(g-2)$
• The XXL Survey: XVI. The clustering of X-ray selected galaxy clusters at z~0.3
• Semi-analytic forecasts for JWST -- V. AGN luminosity functions and helium reionization at z = 2-7
• Dark Matter and Neutrino Mass from the Smallest Non-Abelian Chiral Dark Sector
• Parsec-scale properties of the radio brightest jetted AGN at z > 6
• An ALMA CO(2-1) Survey of Nearby Palomar-Green Quasars
• Axion dark matter from Higgs inflation with an intermediate $H_{\ast }$
• Resurrection of large lepton number asymmetries from neutrino flavor oscillations
• Motivations for a Large Self-Interacting Dark Matter Cross Section from Milky Way Satellites
• Non-Gaussianity in inflationary scenarios for primordial black holes
• Ages of the Bulge globular clusters NGC 6522 and NGC 6626 (M28) from HST Proper-motion-cleaned Color-Magnitude Diagrams
• Large Magellanic Cloud Near-Infrared Synoptic Survey. V. Period-Luminosity Relations of Miras
• Constraining neutrino mass and extra relativistic degrees of freedom in dynamical dark energy models using Planck 2015 data in combination with low-redshift cosmological probes: basic extensions to $\Lambda$CDM cosmology
• A 3-D model of polarised dust emission in the Milky Way
• Exploring the Hyperchargeless Higgs Triplet Model up to the Planck Scale
• Cosmology with dropout selection: Straw-man surveys and CMB lensing
• Understanding the phenomenology of interacting dark energy scenarios and their theoretical bounds
• Displaced Photon Signal from a Light Scalar in Minimal Left-Right Symmetric Model
• The gravitational field of X-COP galaxy clusters
• A Deep CFHT Optical Search for a Counterpart to the Possible Neutron Star -- Black Hole Merger GW190814
• Optimising gravitational waves follow-up using galaxies stellar mass
• The web of the Giant: spectroscopic confirmation of a Large Scale Structure around the z=6.31 quasar SDSS J1030+0524
• Origin of the galaxy HI size-mass relation
• New Methods for Identifying Lyman Continuum Leakers and Reionization-Epoch Analogues
• Gauss-Bonnet term corrections in scalar field cosmology
• Dark matter in U(1) extensions of the MSSM with gauge kinetic mixing
• Multi-messenger Detection Rates and distributions of Binary Neutron Star Mergers and Their Cosmological Implications
• Relative distribution of dark matter, gas, and stars around cosmic filaments in the IllustrisTNG simulation
• Multimessenger Implications of AT2018cow: High-Energy Cosmic Ray and Neutrino Emissions from Magnetar-Powered Super-Luminous Transients
• Constraining the Kilonova Rate with Zwicky Transient Facility Searches Independent of Gravitational Wave and Short Gamma-ray Burst Triggers
• Accelerating Universe scenario in anisotropic $f\left(Q\right)$ cosmology
• Accurate fitting functions for peculiar velocity spectra in standard and massive-neutrino cosmologies
• Galaxy imaging surveys as spin-sensitive detector for cosmological colliders
• On the Stability of Infinite Derivative Abelian Higgs
• Elucidating Galaxy Assembly Bias in SDSS
• Roll of the Dice: A Stochastically Sampled IMF Alters the Stellar Content of Simulated Dwarf Galaxies
• Ubiquitous Molecular Outflows in z > 4 Massive, Dusty Galaxies II. Momentum-Driven Winds Powered by Star Formation in the Early Universe
• Updated constraints on decaying cold dark matter
• Search for sterile neutrinos in a universe of vacuum energy interacting with cold dark matter
• Minimal models for $g-2$ and dark matter confront asymptotic safety
• Gravitational Leptogenesis, Reheating, and Models of Neutrino Mass
• The skewed weak lensing likelihood: why biases arise, despite data and theory being sound
• Early Cosmological Period of QCD Confinement
• Toward an understanding of GRB prompt emission mechanism: II. Patterns of peak energy evolution and their connection to spectral lags
• Search for dark matter produced in association with a Higgs boson decaying to a pair of bottom quarks in proton-proton collisions at $\sqrt{s}=$ 13 TeV
• Current Constraints on Anisotropic and Isotropic Dark Energy Models
• Searching for Physics Beyond the Standard Model in an Off-Axis DUNE Near Detector
• Sustained super-Eddington accretion in high-redshift quasars
• Modified gravity for surveys
• The SAMI Galaxy Survey: stellar population and structural trends across the Fundamental Plane
• Constraints on quintessence scalar field models using cosmological observations
• On the influence of halo mass accretion history on galaxy properties and assembly bias
• First results from SMAUG: The need for preventative stellar feedback and improved baryon cycling in semi-analytic models of galaxy formation
• Exploring Early Dark Energy solution to the Hubble tension with Planck and SPTPol data
• Crossing phantom divide in $f(Q)$ gravity
• On the origin of the mass-metallicity gradient relation in the local Universe
• Lagrangian perturbation theory for modified gravity
• An empirical representation of a physical model for the ISM [CII], CO, and [CI] emission at redshift $1\le z\le 9$
• A Demonstration of Improved Constraints on Primordial Gravitational Waves with Delensing
• A measurement of the Hubble constant using galaxy redshift surveys
• Measuring the Hubble Constant with a sample of kilonovae
• Model-independent analysis of the DAMPE excess
• Constraining Reionization with the $z\sim 5-6$ Lyman-$\alpha$ Forest Power Spectrum: the Outlook after Planck
• Cosmological baryon transfer in the SIMBA simulations
• Absolute Calibration Strategies for the Hydrogen Epoch of Reionization Array and Their Impact on the 21 cm Power Spectrum
• Interstellar Medium and Star Formation of Starburst Galaxies on the Merger Sequence
• Accumulating errors in tests of general relativity with gravitational waves: overlapping signals and inaccurate waveforms
• Linking gas and galaxies at high redshift: MUSE surveys the environments of six damped Lyman alpha galaxies at z~3
• Hierarchical Inference of Binary Neutron Star Mass Distribution and Equation of State with Gravitational Waves
• Geodesics and the magnitude-redshift relation on cosmologically symmetric Finsler spacetimes
• Gravity in the infrared and effective nonlocal models
• Mapping Extragalactic Dark Matter Annihilation with Galaxy Surveys: A Systematic Study of Stacked Group Searches
• Constraining the era of helium reionization using fast radio bursts
• Origin of the Local Group satellite planes
• Efficient Computation of Galaxy Bias with Neutrinos and Other Relics
• The Search for Dark Matter
• Warm-hot Gas in X-ray Bright Galaxy Clusters and the H I-deficient Circumgalactic Medium in Dense Environments
• Dark matter as a Weyl geometric effect
• The Dispersion of Fast Radio Bursts from a Structured Intergalactic Medium at Redshifts z < 1.5
• Common Origin of Neutrino Mass and Dark Matter from Anomaly Cancellation Requirements of a $U(1{)}_{B-L}$ Model
• Dark Catalysis
• The formation of UCDs and massive GCs: Quasar-like objects for testing for a variable stellar initial mass function (IMF)
• Imprints of temperature fluctuations on the $z\sim 5$ Lyman-$\alpha$ forest: a view from radiation-hydrodynamic simulations of reionization
• Early-type galaxy density profiles from IllustrisTNG: I. Galaxy correlations and the impact of baryons
• Discovering gravitationally lensed gravitational waves: predicted rates, candidate selection, and localization with the Vera Rubin Observatory
• Power spectrum of halo intrinsic alignments in simulations
• Hybrid Loop Quantum Cosmology: An Overview
• Fitting rotation curve of galaxies by de Rham-Gabadadze-Tolley massive gravity
• Testing interacting dark matter and dark energy model with cosmological data
• Resolving the inner parsec of the blazar J1924-2914 with the Event Horizon Telescope
• Hidden sector explanation of $B$-decay and cosmic ray anomalies
• Implications of hydrodynamical simulations for the interpretation of direct dark matter searches
• Studying topological structure in the epoch of reionization with 3D-Minkowski functionals of 21cm line fluctuations
• Polarization of a stochastic gravitational wave background through diffusion by massive structures
• A first constraint on the average mass of ultra diffuse galaxies from weak gravitational lensing
• Quintessence Behaviour of an Anisotropic Bulk Viscous Cosmological Model in Modified $f(Q)$-Gravity
• ULYSSES: Universal LeptogeneSiS Equation Solver
• The matter power spectrum in redshift space using effective field theory
• Jellyfish galaxies with the IllustrisTNG simulations -- When, where, and for how long does ram pressure stripping of cold gas occur?
• A model explaining neutrino masses and the DAMPE cosmic ray electron excess
• Quantifying the evidence for the current speed-up of the Universe with low and intermediate-redshift data. A more model-independent approach
• A New Calibration of Star Formation Rate in Galaxies Based on Polycyclic Aromatic Hydrocarbon Emission
• Exploring the Properties of Choked Gamma-Ray Bursts with IceCube's High Energy Neutrinos
• Predicting the hypervelocity star population in Gaia
• Identifying WIMP dark matter from particle and astroparticle data
• Probing the imprints of generalized interacting dark energy on the growth of perturbations
• Inflation and Dark Matter in the Inert Doublet Model
• Constraining interacting dark energy with CMB and BAO future surveys
• The Apparent (Gravitational) Horizon in Cosmology
• Modified gravity realizations of quintom dark energy after DESI DR2
• Distinguishing between Neutrinos and time-varying Dark Energy through Cosmic Time
• Interplay of the LHC and non-LHC Dark Matter searches in the Effective Field Theory approach
• Cold light dark matter in extended seesaw models
• Probing Dark Matter Subhalos in Galaxy Clusters Using Highly Magnified Stars
• Black hole obscuration and duty cycles mediated by AGN feedback in high redshift galaxies
• Joint analysis of the thermal Sunyaev-Zeldovich effect and 2MASS galaxies: Probing gas physics in the local Universe and beyond
• Spectroscopically Confirmed Lyman-Alpha Emitters from Redshift 5 to 7 Behind Ten Galaxy Cluster Lenses
• Scaling solutions and weak gravity in dark energy with energy and momentum couplings
• Is well-tempered neutralino in MSSM still alive after 2016 LUX results?
• Boosted Self-interacting Dark Matter in a Multi-component Dark Matter Model
• Shapes and alignments of dark matter haloes and their brightest cluster galaxies in 39 strong lensing clusters
• Joint growth rate measurements from redshift-space distortions and peculiar velocities in the 6dF Galaxy Survey
• ${}^7$Li evolution in the thin and thick disks of the Milky Way
• Dark Matter properties through cosmic history
• The Abundance and Structure of Subhaloes near the Free Streaming Scale and Their Impact on Indirect Dark Matter Searches
• Clustering on very small scales from a large sample of confirmed quasar pairs: Does quasar clustering track from Mpc to kpc scales?
• The primordial deuterium abundance at z = 2.504 from a high signal-to-noise spectrum of Q1009+2956
• A limit on the warm dark matter particle mass from the redshifted 21 cm absorption line
• Black hole shadow to probe modified gravity
• Tensions between direct measurements of the lens power spectrum from Planck data
• The role of faint population III supernovae in forming CEMP stars in ultra-faint dwarf galaxies
• Exploring the epoch of hydrogen reionization using FRBs
• Cosmological simulations of dwarfs: the need for ISM physics beyond SN feedback alone
• Cosmology from non-minimal geometry-matter coupling
• What is parameterized $Om(z)$ diagnostics telling us in light of recent observations?
• Pathways for producing binary black holes with large misaligned spins in the isolated formation channel
• A tale of two sites -- II: Inferring the properties of minihalo-hosted galaxies with upcoming 21-cm interferometers
• A Minimum Dilution Scenario for Supernovae and Consequences for Extremely Metal-Poor Stars
• The Big Bang, CPT, and neutrino dark matter
• Prospects for Higgs physics at energies up to 100 TeV
• Asteroseismology of 36 Kepler subgiants -- II: Determining ages from detailed modelling
• Comprehensive Gas Characterization of a $z=2.5$ Protocluster: A Cluster Core Caught in the Beginning of Virialization?
• Exploring galaxies-gravitational waves cross-correlations as an astrophysical probe
• The Generation of Vorticity in Cosmological N-body Simulations
• Variable sound speed in interacting dark energy models
• Photometric properties of reionization-epoch galaxies in the Simba simulations
• Big bounce and closed universe from spin and torsion
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Angular clustering tomography and its cosmological implications
• Reconstruction of the Dark Energy equation of state from latest data: the impact of theoretical priors
• Weakening Gravity on Redshift-Survey Scales with Kinetic Matter Mixing
• The role of galaxies and AGN in reionizing the IGM - II: metal-tracing the faint sources of reionization at $5\lesssim z\lesssim 6$
• Testing one-loop galaxy bias: Power spectrum
• Statistical Analyses of Higgs- and Z-Portal Dark Matter Models
• The MUSE Hubble Ultra Deep Field Survey: XII. MgII emission and absorption in star-forming galaxies
• GenetIC -- a new initial conditions generator to support genetically modified zoom simulations
• A Revised SALT2 Surface for Fitting Type Ia Supernova Light Curves
• Galaxy And Mass Assembly (GAMA): The inferred mass--metallicity relation from z=0 to 3.5 via forensic SED fitting
• Evolutionary behaviour of cosmological parameters with dynamical system analysis in f (Q, T) gravity
• Dark Matter Sommerfeld-enhanced annihilation and Bound-state decay at finite temperature
• Systematic bias on the inspiral-merger-ringdown consistency test due to neglect of orbital eccentricity
• An imperfectly passive nature: Bright sub-millimeter emission from dust-obscured star formation in the z=3.717 "passive" system, ZF20115
• A lensed radio jet at milli-arcsecond resolution I: Bayesian comparison of parametric lens models
• Comparing galaxy formation in the L-GALAXIES semi-analytical model and the IllustrisTNG simulations
• Large-scale redshift space distortions in modified gravity theories
• Simulating the transport of relativistic electrons and magnetic fields injected by radio galaxies in the intracluster medium
• Priors on the effective Dark Energy equation of state in scalar-tensor theories
• ALMA hints at the presence of turbulent disk galaxies at z > 5
• Neutron star merger GW170817 strongly constrains doubly coupled bigravity
• AT 2019avd: A novel addition to the diverse population of nuclear transients
• Cosmological Simulation for Fuzzy Dark Matter Model
• Cosmological constraints from a joint analysis of cosmic growth and expansion
• Primordial Black-Hole Dark Matter via Warm Natural Inflation
• Early Cosmology Constrained
• MIGHTEE: Are giant radio galaxies more common than we thought?
• Filament profiles from WISExSCOS galaxies as probes of the impact of environmental effects
• Novel neutrino-floor and dark matter searches with deformed shell model calculations
• Binary black hole mergers from Population III stars: uncertainties from star formation and binary star properties
• A needle in a haystack? Catching Pop III stars in the Epoch of Reionization: I. Pop III star forming environments
• Resolving galaxy cluster gas properties at z~1 with XMM-Newton and Chandra
• Optimising growth of structure constraints on modified gravity
• Cosmology of Lorentz fiber-bundle induced scalar-tensor theories
• Evidence against a supervoid causing the CMB Cold Spot
• Prospects of detecting the nonlinear gravitational wave memory
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): An unbiased estimate of the growth rate of structure at $⟨\mathbf{z}⟩=0.85$ using the clustering of luminous blue galaxies
• Surprises from Complete Vector Portal Theories: New Insights into the Dark Sector and its Interplay with Higgs Physics
• Late time cosmology with LISA: probing the cosmic expansion with massive black hole binary mergers as standard sirens
• Swampland criteria for a dark-energy dominated universe, ensuing from Gaussian process and H(z) data analysis
• Primordial Black Hole Dark Matter and LIGO/Virgo Merger Rate from Inflation with Running Spectral Indices: Formation in the Matter- and/or Radiation-Dominated Universe
• Evaluating the QSO contribution to the 21-cm signal from the Cosmic Dawn
• Joint halo mass function for modified gravity and massive neutrinos I: simulations and cosmological forecasts
• Predicting the density profiles of the first halos
• Full of Orions: a 200-pc mapping of the interstellar medium in the redshift-3 lensed dusty star-forming galaxy SDP.81
• A comprehensive statistical study on gamma-ray bursts
• Model-independent constraints on cosmic curvature: implication from updated Hubble diagram of high-redshift standard candles
• Dark matter component decaying after recombination: Sensitivity to BAO and RSD probes
• Towards the routine use of subdominant harmonics in gravitational-wave inference: re-analysis of GW190412 with generation X waveform models
• Early growth of typical high redshift black holes seeded by direct collapse
• Multiple Ultralight Axionic Wave Dark Matter and Astronomical Structures
• Testing Gravity on Cosmic Scales: A Case Study of Jordan-Brans-Dicke Theory
• Falsifying cosmological models based on a non-linear electrodynamics
• Bayesian Evidences for Dark Energy models in light of current obsevational data
• Cosmological Structure Formation and Soliton Phase Transition in Fuzzy Dark Matter with Axion Self-Interactions
• From inflation to cosmological electroweak phase transition with a complex scalar singlet
• Implications of a positive cosmological constant for general relativity
• Bulk viscous embedded hybrid dark energy models
• Safely smoothing spacetime: backreaction in relativistic cosmological simulations
• Stellar streams as gravitational experiments I. The case of Sagittarius
• Updated observational constraints on quintessence dark energy models
• Darkness without dark matter and energy -- generalized unimodular gravity
• An Excess of Globular Clusters in UDGs Formed Through Tidal Heating
• Light inflaton completing Higgs inflation
• SIBELIUS-DARK: a galaxy catalogue of the Local Volume from a constrained realisation simulation
• Lossless, Scalable Implicit Likelihood Inference for Cosmological Fields
• Towards a model-independent reconstruction approach for late-time Hubble data
• The cold circumgalactic medium in emission: MgII halos in TNG50
• Radio spectral properties of star-forming galaxies in the MIGHTEE-COSMOS field and their impact on the far-infrared-radio correlation
• Rotation curves and scaling relations of extremely massive spiral galaxies
• ZTF20aajnksq (AT2020blt): A Fast Optical Transient at $z\approx 2.9$ With No Detected Gamma-Ray Burst Counterpart
• Probing secret interactions of eV-scale sterile neutrinos with the diffuse supernova neutrino background
• The Infrared Emission and Vigorous Star Formation of Low-redshift Quasars
• Barred galaxies in the Illustris-1 and TNG100 simulations
• A New Method to Measure Hubble Parameter $H(z)$ using Fast Radio Bursts
• Cosmic shear with small scales: DES-Y3, KiDS-1000 and HSC-DR1
• Phenomenology of Large Scale Structure in scalar-tensor theories: joint prior covariance of $w_{\text{DE}}$, $\Sigma$ and $\mu$ in Horndeski
• Cold dark matter plus not-so-clumpy dark relics
• A Hybrid Deep Learning Approach to Cosmological Constraints From Galaxy Redshift Surveys
• Evidences against cuspy dark matter halos in large galaxies
• Type Ia Supernovae are Excellent Standard Candles in the Near-Infrared
• Detailed investigation of the duration of inflation in loop quantum cosmology for a Bianchi-I universe with different inflaton potentials and initial conditions
• Leptonic and Hadronic Modeling of Fermi-LAT Hard Spectrum Quasars and Predictions for High-Energy Polarization
• How to relax the cosmological neutrino mass bound
• New constraints on the linear growth rate using cosmic voids in the SDSS DR12 datasets
• Reconstructing Horndeski theories from phenomenological modified gravity and dark energy models on cosmological scales
• Modelling and simulation of large-scale polarized dust emission over the southern Galactic cap using the GASS HI data
• Covariance of CMB anomalies
• $H_0$ tension and the String Swampland
• Resonance enhancement of dark matter interactions: the case for early kinetic decoupling and velocity dependent resonance width
• Time evolution of intrinsic alignments of galaxies
• Electroweak vacuum stability in presence of singlet scalar dark matter in TeV scale seesaw models
• The Stellar Mass, Star Formation Rate and Dark Matter Halo Properties of LAEs at $z\sim 2$
• Dark Sector Equilibration During Nucleosynthesis
• Unified Superfluid Dark Sector
• Model-independent Test of the Cosmic Distance Duality Relation
• Testing the isotropy of the Universe with type Ia supernovae in a model-independent way
• The highest-speed local dark matter particles come from the Large Magellanic Cloud
• Constraining the dark energy equation of state using Bayes theorem and the Kullback-Leibler divergence
• Multi-flavour SMBH seeding and evolution in cosmological environments
• Delayed triggering of radio Active Galactic Nuclei in gas-rich minor mergers in the local Universe
• Gravitational Leptogenesis in the Axion Inflation with an SU(2) gauge field
• On the dissection of degenerate cosmologies with machine learning
• Weak lensing constraints on splashback around massive clusters
• The need for accurate redshifts in supernova cosmology
• Absolute calibration of the polarisation angle for future CMB $B$-mode experiments from current and future measurements of the Crab nebula
• The effects of assembly bias on cosmological inference from galaxy-galaxy lensing and galaxy clusters
• Waveforms of compact binary inspiral gravitational radiation in screened modified gravity
• Dynamics of binary black holes in low-mass young star clusters
• Model-independent cosmological constraints from growth and expansion
• A high precision semi-analytic mass function
• Repeated Imaging of Massive Black Hole Binary Orbits with Millimeter Interferometry: measuring black hole masses and the Hubble constant
• High redshift JWST predictions from IllustrisTNG: III. Infrared luminosity functions, obscured star formation and dust temperature of high-redshift galaxies
• Indirect Signals from Solar Dark Matter Annihilation to Long-lived Right-handed Neutrinos
• A Catalog of 220 Offset and Dual AGNs: Increased AGN Activation in Major Mergers and Separations under 4 kpc
• Parameterized Post-Newtonian Cosmology
• Dark energy from $\alpha$-attractors: phenomenology and observational constraints
• The host galaxy of the short GRB111117A at $z=2.211$: impact on the short GRB redshift distribution and progenitor channels
• Exacerbating the cosmological constant problem with interacting dark energy
• Cosmic QCD Epoch at Nonvanishing Lepton Asymmetry
• Gauge-invariant quantum gravitational corrections to correlation functions
• Rip cosmological models in extended symmetric teleparallel gravity
• After The Fall: Resolving the Molecular Gas in Post-Starburst Galaxies
• Fast radio bursts to be detected with the Square Kilometre Array
• The growth of brightest cluster galaxies in the TNG300 simulation:dissecting the contributions from mergers and in situ star formation
• The AMIGA sample of isolated galaxies XIII. The HI content of an almost "nurture free" sample
• Calibration, event reconstruction, data analysis and limits calculation for the LUX dark matter experiment
• CLASH-VLT: a full dynamical reconstruction of the mass profile of Abell S1063 from 1 kpc out to the virial radius
• The Little Galaxies that Could (Reionize the Universe): Predicting Faint End Slopes & Escape Fractions at z > 4
• Accuracy of environmental tracers and consequence for determining the Type Ia Supernovae magnitude step
• Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations
• Cosmology in beyond-generalized Proca theories
• Cosmological Perturbations of Extreme Axion in the Radiation Era
• Cosmological applications of Myrzakulov gravity
• Unimodular $f(R,T)$ Gravity
• The Detection Rates of Merging Binary Black Holes Originating from Star Clusters and Their Mass Function
• Model independent constraints on transition redshift
• Black hole superradiance and polarization-dependent bending of light
• The nightmare scenario: measuring the stochastic gravitational-wave background from stalling massive black-hole binaries with pulsar-timing arrays
• On Inflationary Scale, Reheating Scale and Pre-BBN Cosmology with Scalar Fields
• On building a cluster watch-list for identifying strongly lensed supernovae, gravitational waves and kilonovae
• A UV Complete Framework of Freeze-in Massive Particle Dark Matter
• Equilibrium model prediction for the scatter in the star-forming main sequence
• A survey of the thermal and non-thermal properties of cosmic filaments
• Constraints on small-scale primordial power by annihilation signals from extragalactic dark matter minihalos
• Model-Independent Constraints on Lorentz Invariance Violation via the Cosmographic Approach
• Baryogenesis in Nonminimally Coupled $f(R)$ Theories
• Search for dark matter in association with an energetic photon in pp collisions at $\sqrt{s}$ = 13 TeV with the ATLAS detector
• Tree-Level Bispectrum in the Effective Field Theory of Large-Scale Structure extended to Massive Neutrinos
• Simple halo model formalism for the cosmic infrared background and its correlation with the thermal Sunyaev Zel'dovich effect
• Validation of EDGES Low-Band Antenna Beam Model
• Detection prospects for the Cosmic Neutrino Background using laser interferometers
• The AARTFAAC Cosmic Explorer: observations of the 21-cm power spectrum in the EDGES absorption trough
• Cosmological Bound from the Neutron Star Merger GW170817 in scalar-tensor and $F(R)$ gravity theories
• A Dark Matter Interpretation of the ANITA Anomalous Events
• Dark Energy Survey Year 1 Results: galaxy mock catalogues for BAO
• Constraining Cluster Virialization Mechanism and Cosmology using Thermal-SZ-selected clusters from Future CMB Surveys
• Protophobic Light Vector Boson as a Mediator to the Dark Sector
• Indirect dark matter searches in the dwarf satellite galaxy Ursa Major II with the MAGIC Telescopes
• The trouble with Hubble: Local versus global expansion rates in inhomogeneous cosmological simulations with numerical relativity
• Illustrating galaxy-halo connection in the DESI era with IllustrisTNG
• Characterizing hydrostatic mass bias with Mock-X
• Cosmological constraints from a joint analysis of cosmic microwave background and spectroscopic tracers of the large-scale structure
• Constraining the parameters of GW150914 & GW170104 with numerical relativity surrogates
• X-ray spectroscopic survey of highly-accreting AGN
• Data compression in cosmology: A compressed likelihood for Planck data
• Cosmology Inference from Biased Tracers using the EFT-based Likelihood
• WATCAT: a tale of wide-angle tailed radio galaxies
• Quintessential Affleck-Dine baryogenesis with non-minimal couplings
• The stellar population and initial mass function of NGC 1399 with MUSE
• Atomki anomaly and dark matter in a radiative seesaw model with gauged $B-L$ symmetry
• Magnetization of the intergalactic medium in the IllustrisTNG simulations: the importance of extended, outflow-driven bubbles
• Ultralight bosons for strong gravity applications from simple Standard Model extensions
• Modelling Galaxy Merger Timescales and Tidal Destruction
• Higgs Enhancement for the Dark Matter Relic Density
• X-ray Plateaus in Gamma-Ray Burst Afterglows and Their Application in Cosmology
• Late time acceleration due to generic modification of gravity and Hubble tension
• Scrutinizing Right-Handed Neutrino Portal Dark Matter With Yukawa Effect
• The one-loop matter bispectrum as a probe of gravity and dark energy
• Bimodal black-hole mass distribution and chirp masses of binary black-hole mergers
• Gravitational effects of condensed dark matter on strange stars
• Probing the MSSM explanation of the muon g-2 anomaly in dark matter experiments and at a 100 TeV $pp$ collider
• Massive neutrino self-interactions and inflation
• Impacts of gravitational-wave standard siren observations from Einstein Telescope and Cosmic Explorer on weighing neutrinos in interacting dark energy models
• Prospects of discovering sub-solar primordial black holes using the stochastic gravitational wave background from third-generation detectors
• Exploring the Thermal State of the Low-Density Intergalactic Medium at z=3 with an Ultra-High Signal-to-Noise QSO Spectrum
• Infrared emission of $z\sim 6$ galaxies: AGN imprints
• New Constraints on Dark Matter Production during Kination
• Relic density of Dark Matter in the Inert Doublet Model beyond Leading Order. I) The Heavy Mass Case
• Reconstruction of the neutrino mass as a function of redshift
• Constraints on QSO emissivity using H I and He II Lyman alpha forest
• Interacting galaxies in the IllustrisTNG simulations -- III: (the rarity of) quenching in post-merger galaxies
• Predictions for anisotropic X-ray signatures in the circumgalactic medium: imprints of supermassive black hole driven outflows
• Maps of the Southern Millimeter-wave Sky from Combined 2500 deg${}^2$ SPT-SZ and Planck Temperature Data
• Bardeen regular black hole as a quantum-corrected Schwarzschild black hole
• Constraining the volume density of Dusty Star-Forming Galaxies through the first 3mm Number Counts from ALMA
• Signatures of Ultralight Dark Matter in Neutrino Oscillation Experiments
• Axion Astrophysics
• Probing modified gravity theories with multiple measurements of high-redshift quasars
• New perspectives on the BOSS small-scale lensing discrepancy for the Planck $\Lambda$CDM Cosmology
• Color gradients and half-mass radii of galaxies out to $z=2$ in the CANDELS/3D-HST fields: further evidence for important differences in the evolution of mass-weighted and light-weighted sizes
• Generalized Uncertainty Principle and White Dwarfs Redux: How Cosmological Constant Protects Chandrasekhar Limit
• GAMA/H-ATLAS: The Local Dust Mass Function and Cosmic Density as a Function of Galaxy Type - A Benchmark for Models of Galaxy Evolution
• Milky Way Mass with K Giants and BHB Stars Using LAMOST, SDSS/SEGUE, and Gaia: 3D Spherical Jeans Equation and Tracer Mass Estimator
• Constraints on direction-dependent cosmic birefringence from Planck polarization data
• Warm FIRE: Simulating Galaxy Formation with Resonant Sterile Neutrino Dark Matter
• Model-independent cosmic acceleration and type Ia supernovae intrinsic luminosity redshift dependence
• The Redshift Evolution of Rest-UV Spectroscopic Properties to z~5
• Hunting the dark Higgs
• Model-independent analyses of non-Gaussianity in Planck CMB maps using Minkowski Functionals
• Cosmological perturbations in the Tsallis holographic dark energy scenarios
• X-ray Emission From Hot Gas in Galaxy Groups and Clusters in Simba
• Small-Field and Scale-Free: Inflation and Ekpyrosis at their Extremes
• Probing Decoupling in Dark Sectors with the Cosmic Microwave Background
• The Mass and Absorption Columns of Galactic Gaseous Halos
• Exploring the sky localization and early warning capabilities of third generation gravitational wave detectors in three-detector network configurations
• Asteroseismic constraints on the cosmic-time variation of the gravitational constant from an ancient main-sequence star
• Two-step strongly first-order electroweak phase transition modified FIMP dark matter, gravitational wave signals, and the neutrino mass
• The Extremely Luminous Quasar Survey in the Sloan Digital Sky Survey footprint. III. The South Galactic Cap Sample and the Quasar Luminosity Function at Cosmic Noon
• Imprints of Oscillatory Bispectra on Galaxy Clustering
• A deep X-ray view of the bare AGN Ark120. V. Spin determination from disc-Comptonisation efficiency method
• Internal delensing of Cosmic Microwave Background polarization B-modes with the POLARBEAR experiment
• Constraining the dark energy models with H(z) data: an approach independent of $H_0$
• The fate of the gaseous disks of galaxies that fall into clusters
• Realistic estimation for the detectability of dark matter sub-halos with Fermi-LAT
• Correlations between supermassive black holes and hot gas atmospheres in IllustrisTNG and X-ray observations
• Cosmological distance indicators
• The splashback radius of optically selected clusters with Subaru HSC Second Public Data Release
• Non-parametric deprojection of NIKA SZ observations: Pressure distribution in the Planck-discovered cluster PSZ1 G045.85+57.71
• The Extremely Luminous Quasar Survey (ELQS) in the SDSS footprint I.: Infrared Based Candidate Selection
• Dirichlet Process Gaussian-mixture model: An application to localizing coalescing binary neutron stars with gravitational-wave observations
• Measuring the delay time distribution of binary neutron stars. II. Using the redshift distribution from third-generation gravitational wave detectors network
• Measuring growth index in a universe with massive neutrinos: A revisit of the general relativity test with the latest observations
• POLOCALC: a Novel Method to Measure the Absolute Polarization Orientation of the Cosmic Microwave Background
• Detection of intercluster gas in superclusters using the thermal Sunyaev-Zel'dovich effect
• Natural Inflation After Planck 2018
• Bouncing and emergent cosmologies from ADM RG flows
• Type II Supernova Light Curves and Spectra From the CfA
• Angular power spectrum of galaxies in the 2MASS Redshift Survey
• KYDISC: Galaxy Morphology, Quenching, and Mergers in the Cluster Environment
• Neutrino Mass Priors for Cosmology from Random Matrices
• Search for dark matter produced in association with a Standard Model Higgs boson decaying into $b$-quarks using the full Run 2 dataset from the ATLAS detector
• On the Fast Radio Burst and Persistent Radio Source Populations
• Testing dark energy models with a new sample of strong-lensing systems
• Inflation in the closed FLRW model and the CMB
• A general relativistic signature in the galaxy bispectrum: the local effects of observing on the lightcone
• Baryogenesis from B Meson Oscillations
• Revisiting CMB constraints on Warm Inflation
• Exclusion of ALP Cogenesis Dark Matter in a Mass Window Above 100 $\mu$eV
• Asymmetric Dark Matter and the hadronic spectra of hidden QCD
• Naturalness and Dark Matter in the BLSSM
• Time-dependent mass of cosmological perturbations in the hybrid and dressed metric approaches to loop quantum cosmology
• Detection strategies for the first supernovae with JWST
• The HDUV Survey: Six Lyman Continuum Emitter Candidates at z~2 Revealed by HST UV Imaging
• Sloan Great Wall as a complex of superclusters with collapsing cores
• Measuring the 2D Baryon Acoustic Oscillation signal of galaxies in WiggleZ: Cosmological constraints
• A data-driven Reconstruction of Horndeski gravity via the Gaussian processes
• Cornering the Planck $A_{lens}$ tension with future CMB data
• Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA
• Implications of an Improved Neutron-Antineutron Oscillation Search for Baryogenesis: A Minimal Effective Theory Analysis
• The Bacco Simulation Project: Bacco Hybrid Lagrangian Bias Expansion Model in Redshift Space
• Power-law cosmology in Weyl-type $f(Q,T)$ gravity
• Forecasting the Interaction in Dark Matter-Dark Energy Models with Standard Sirens From the Einstein Telescope
• A Fast Radio Burst discovered in FAST drift scan survey
• The first Super Massive Black Holes: indications from models for future observations
• Cluster-void degeneracy breaking: Neutrino properties and dark energy
• de Sitter Cosmology on an expanding bubble
• Molecular gas and star formation in an absorption-selected galaxy: Hitting the bull's eye at z = 2.46
• On the faint-end of the galaxy luminosity function in the Epoch of Reionization: updated constraints from the HST Frontier Fields
• On the evolution of the entropy and pressure profiles in X-ray luminous galaxy clusters at z > 0.4
• An estimation of the Local growth rate from Cosmicflows-3 peculiar velocities
• The mass-metallicity relation at z~1-2 and its dependence on star formation rate
• Efficient cold outflows driven by cosmic rays in high redshift galaxies and their global effects on the IGM
• Signatures of metal-free star formation in Planck 2015 Polarization Data
• Warm dark matter and the ionization history of the Universe
• New binary black hole mergers in the LIGO-Virgo O3b data
• A Catalog of AGN Host Galaxies Observed with HST/ACS: Correlations between Star Formation and AGN Activity
• A persistent excess of galaxy-galaxy strong lensing observed in galaxy clusters
• The Three Hundred Project: quest of clusters of galaxies morphology and dynamical state through Zernike Polynomials
• Do joint CMB and HST data support a scale invariant spectrum?
• Constraints on the sum of neutrino masses using cosmological data including the latest extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample
• CO, H2O, H2O+ line and dust emission in a z = 3.63 strongly lensed starburst merger at sub-kiloparsec scales
• Post-collapse perturbation theory in 1D cosmology -- beyond shell-crossing
• Rare charm $\mathbf{c}\to \mathbf{u}\mathbf{\nu }\bar{\mathbf{\nu }}$ dineutrino null tests for ${\mathbf{e}}^{+}{\mathbf{e}}^{-}$-machines
• The Radio Galaxy Population in the SIMBA SImulations
• Fuzzy Dark Matter at Cosmic Dawn: New 21-cm Constraints
• The Neutrino Option
• Low redshift observational constraints on tachyon models of dark energy
• Minimal Seesaw extension for Neutrino Mass and Mixing, Leptogenesis and Dark Matter: FIMPzillas through the Right-Handed Neutrino Portal
• Probing the progenitors of spinning binary black-hole mergers with long gamma-ray bursts
• Impact of Relativistic Effects on the Primordial Non-Gaussianity Signature in the Large-Scale Clustering of Quasars
• Target Selection for the DESI Peculiar Velocity Survey
• Marked clustering statistics in $f(R)$ gravity cosmologies
• Black hole formation in a contracting universe
• New Exact Spherically Symmetric Solutions in $f(R,\varphi ,X)$ gravity by Noether's symmetry approach
• Finding the Missing Baryons with Fast Radio Bursts and Sunyaev-Zeldovich Maps
• Scalar dark matter, Type II Seesaw and the DAMPE cosmic ray $e^{+}+e^{-}$ excess
• Cosmological inference from standard sirens without redshift measurements
• Chasing Lyman alpha-emitting galaxies at z = 8.8
• Hiding neutrino mass in modified gravity cosmologies
• CMB anisotropy and BBN constraints on pre-recombination decay of dark matter to visible particles
• Direct Detection of Dark Matter Substructure in Strong Lens Images with Convolutional Neural Networks
• Emergence of the mass discrepancy-acceleration relation from dark matter-baryon interactions
• Bound-state dark matter and Dirac neutrino mass
• Transitioning Universe with hybrid scalar field in Bianchi I space-time
• The Relative Specific Type Ia Supernovae Rate From Three Years of ASAS-SN
• Is there enough star formation in simulated protoclusters?
• A feeble window on leptophilic dark matter
• Galaxy Cluster Mass Reconstruction Project: III. The impact of dynamical substructure on cluster mass estimates
• Searching for sterile neutrinos in dynamical dark energy cosmologies
• Painting halos from cosmic density fields of dark matter with physically motivated neural networks
• Reverberation Mapping Measurements of Black Hole Masses and Broad-Line Region Kinematics in Mrk 817 and NGC 7469
• Neutral island statistics during reionization from 21-cm tomography
• Analysis of apsidal motion in eclipsing binaries using TESS data II. A test of internal stellar structure}
• Constraining a general U(1)${}^{\prime }$ inverse seesaw model from vacuum stability, dark matter and collider
• A High Space Density of Luminous Lyman Alpha Emitters at z~6.5
• Eddington bias for cosmic neutrino sources
• CMB-lensing beyond the leading order: temperature and polarization anisotropies
• The inner dark matter distribution of the Cosmic Horseshoe (J1148+1930) with gravitational lensing and dynamics
• Constraints on cosmological viscosity and self interacting dark matter from gravitational wave observations
• Cosmic distance inference from purely geometric BAO methods: Linear Point standard ruler and Correlation Function Model Fitting
• Measurement of Hubble constant with stellar-mass binary black holes
• Cosmological Fast Optical Transients with the Zwicky Transient Facility: A Search for Dirty Fireballs
• Efficient exploration of cosmology dependence in the EFT of LSS
• Jet Feedback and the Photon Underproduction Crisis in Simba
• Implicit Likelihood Inference of Reionization Parameters from the 21 cm Power Spectrum
• Projected Cosmological Constraints from Strongly Lensed Supernovae with the Roman Space Telescope
• Stochastic Gravitational Waves from Inflaton Decays
• CMB distance priors revisited: effects of dark energy dynamics, spatial curvature, primordial power spectrum, and neutrino parameters
• Characterization of Population III Stars with Stellar Atmosphere and Evolutionary Modeling and Predictions of their Observability with the James Webb Space Telescope
• $\kappa$TNG: Effect of Baryonic Processes on Weak Lensing with IllustrisTNG Simulations
• The separate-universe approach and sudden transitions during inflation
• QCD Baryogenesis
• Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy
• Galaxy rotation curves in modified gravity models
• Biasing and the search for primordial non-Gaussianity beyond the local type
• Constraining the Asymptotically Safe Cosmology: cosmic acceleration without dark energy
• The Peculiar Transient AT2018cow: A Possible Origin of A Type Ibn/IIn Supernova
• A Consistent Theory of Decaying Dark Matter Connecting IceCube to the Sesame Street
• The Gravity Collective: A Search for the Electromagnetic Counterpart to the Neutron Star-Black Hole Merger GW190814
• Comprehensive asymmetric dark matter model
• Probing Dark Energy in The scope of Bianchi type I Spacetime
• Astronomical Distance Determination in the Space Age. Secondary distance indicators
• Cosmology with Gravitational Wave/Fast Radio Burst Associations
• $Z^{\prime }$ Mediated WIMPs: Dead, Dying, or Soon to be Detected?
• Luminosity-duration relations and luminosity functions of repeating and non-repeating fast radio bursts
• The Possibility of Modeling the Very High Energy Afterglow of GRB 221009A in a Wind Environment
• Searching for left sneutrino LSP at the LHC
• Blazars at the Cosmic Dawn
• Constraints on Dark Matter Annihilation/Decay from the Isotropic Gamma-Ray Background
• The rocky road to quiescence: compaction and quenching of quasar host galaxies at z~2
• Phase-Space Spectral Line De-confusion in Intensity Mapping
• Exploring the halo occupation of AGN using dark-matter cosmological simulations
• On the implementation of the spherical collapse model for dark energy models
• ERGO-ML I: Inferring the assembly histories of IllustrisTNG galaxies from integral observable properties via invertible neural networks
• Angular clustering properties of the DESI QSO target selection using DR9 Legacy Imaging Surveys
• On sub-GeV Dark Matter Production at Fixed-Target Experiments
• Constraints on Large-Scale Magnetic Fields in the Intergalactic Medium Using Cross-Correlation Methods
• Direct Probe of Dark Energy through Gravitational Lensing Effect
• Gravity in the Local Universe : density and velocity fields using CosmicFlows-4
• Holographic dark energy in Gauss-Bonnet gravity with Granda-Oliveros cut-off
• The Inhomogeneous Reionization Times of Present-day Galaxies
• Constraints on Minute-Scale Transient Astrophysical Neutrino Sources
• Anisotropic compact stars in the mimetic gravitational theory
• Radio wave scattering by circumgalactic cool gas clumps
• Power law cosmology model comparison with CMB scale information
• Revisiting CFHTLenS cosmic shear: Optimal E/B mode decomposition using COSEBIs and compressed COSEBIs
• Lithium pollution of a white dwarf records the accretion of an extrasolar planetesimal
• The Vacuum State of Primordial Fluctuations in Hybrid Loop Quantum Cosmology
• VLBI radio structure and radio brightening of the high-energy neutrino emitting blazar TXS 0506+056
• The galaxy-subhalo connection in low-redshift galaxy clusters from weak gravitational lensing
• The Fornax3D project: Assembly histories of lenticular galaxies from a combined dynamical and population orbital analysis
• Detection of anisotropic galaxy assembly bias in BOSS DR12
• The orbit of GW170817 was inclined by less than 28 degrees to the line of sight
• Resolving the hydrostatic mass profiles of galaxy clusters at z~1 with XMM-Newton and Chandra
• Minimum size of 21-cm simulations
• Viewing angle of binary neutron star mergers
• Cosmic variance of $z>7$ galaxies: Prediction from BlueTides
• Physical Correlations of the Scatter between Galaxy Mass, Stellar Content, and Halo Mass
• Impact of theoretical priors in cosmological analyses: the case of single field quintessence
• Star formation characteristics of CNN-identified post-mergers in the Ultraviolet Near Infrared Optical Northern Survey (UNIONS)
• The PAU Survey: Photometric redshifts using transfer learning from simulations
• Testing Super-Heavy Dark Matter from Primordial Black Holes with Gravitational Waves
• The BINGO telescope: a new instrument exploring the new 21-cm cosmology window
• Dynamical symmetries in Brans-Dicke cosmology
• Tidally induced warps of spiral galaxies in IllustrisTNG
• Sneutrino Tribrid Inflation, Metastable Cosmic Strings and Gravitational Waves
• Beyond dimensional analysis: Higgs and new Higgs inflations {\it do not} violate unitarity
• A new bright z=6.82 quasar discovered with VISTA: VHS J0411-0907
• Limit on the population of repeating fast radio bursts from the ASKAP/CRAFT lat50 survey
• The cosmological constant derived via galaxy groups and clusters
• Shadow cast by a rotating and nonlinear magnetic-charged black hole in perfect fluid dark matter
• Observational constraints on key-parameters of cosmic reionisation history
• The IRAM/GISMO two-millimeter survey in the COSMOS field
• Self-interacting dark matter without prejudice
• Running vacuum in QFT in FLRW spacetime: The dynamics of ${\rho }_{\mathrm{vac}}(H)$ from the quantized matter fields
• Stellar Winds and Coronae of Low-mass Pop. II/III Stars
• The phase-space structure of tidally stripped halos
• Noise reduction for weak lensing mass mapping: An application of generative adversarial networks to Subaru Hyper Suprime-Cam first-year data
• Improved post-Newtonian waveform model for inspiralling precessing-eccentric compact binaries
• Implications of right-handed neutrinos in $B-L$ extended standard model with scalar dark matter
• Self-interacting Spin-2 Dark Matter
• Constraints on warm dark matter from UV luminosity functions of high-z galaxies with Bayesian model comparison
• Discovery of a Possible Splashback Feature in the Intracluster Light of MACS J1149.5+2223
• Constraining the dark energy models using Baryon Acoustic Oscillations: An approach independent of $H_0\cdot r_d$
• Simulating and interpreting deep observations in the Hubble Ultra Deep Field with the JWST/NIRSpec low-resolution 'prism'
• Convergence properties of halo merger trees; halo and substructure merger rates across cosmic history
• Scalar assisted singlet doublet fermion dark matter model and electroweak vacuum stability
• Probing the sign-changeable interaction between dark energy and dark matter with current observations
• Searching for Decaying and Annihilating Dark Matter with Line Intensity Mapping
• COFFE: a code for the full-sky relativistic galaxy correlation function
• Evidence for a highly opaque large-scale galaxy void at the end of reionization
• The modified gravity lightcone simulation project I: Statistics of matter and halo distributions
• Gravitational wave signals and cosmological consequences of gravitational reheating
• The impact of inhomogeneous subgrid clumping on cosmic reionization
• Spin-dependent exotic interactions
• BAT AGN Spectroscopic Survey: XVI. General Physical Characteristics of BAT Blazars
• Morphological signatures of mergers in the TNG50 simulation and the Kilo-Degree Survey: the merger fraction from dwarfs to Milky Way-like galaxies
• Pre-processing, group accretion and the orbital trajectories of associated subhaloes
• Stability Analysis of Einstein Universe in $f(\mathcal{G},T)$ Gravity
• Growth of First Galaxies: Impacts of Star Formation and Stellar Feedback
• Limits on the cosmic neutrino background
• Serendipitous Discoveries of Kilonovae in the LSST Main Survey: Maximising Detections of Sub-Threshold Gravitational Wave Events
• Spin and Eccentricity Evolution in Triple Systems: from the Lidov-Kozai Interaction to the Final Merger of the Inner Binary
• Gravitino Problem in Minimal Supergravity Inflation
• Testing the distance duality relation using type Ia supernovae and ultracompact radio sources
• Gaussian Process Regression for foreground removal in HI intensity mapping experiments
• Cosmic homogeneity: a spectroscopic and model-independent measurement
• Revisiting Metastable Dark Energy and Tensions in the Estimation of Cosmological Parameters
• Disantangling the effects of Doppler velocity and primordial non-Gaussianity in galaxy power spectra
• Accidental Peccei-Quinn Symmetry from Discrete Flavour Symmetry and Pati-Salam
• Slowly rotating Bose Einstein Condensate galactic dark matter halos, and their rotation curves
• GA-NIFS: Early-stage feedback in a heavily obscured AGN at $z=4.76$
• The CGM${}^2$ Survey: Circumgalactic O VI from dwarf to massive star-forming galaxies
• The cosmological impact of future constraints on $H_0$ from gravitational-wave standard sirens
• High-resolution SMA imaging of bright submillimetre sources from the SCUBA-2 Cosmology Legacy Survey
• Testing Cosmic Distance-Duality Relation from Future Gravitational Wave Standard Sirens
• The HI content of dark matter halos at $z\approx 0$ from ALFALFA
• Strong orientation dependence of surface mass density profiles of dark haloes at large scales
• A Fully Self-Consistent Cosmological Simulation Pipeline for Interacting Dark Energy Models
• The Ages of Galactic Bulge Stars with Realistic Uncertainties
• Light Dark Matter from Leptogenesis
• The emergence of dark matter-deficient ultra-diffuse galaxies driven by scatter in the stellar mass-halo mass relation and feedback from globular clusters
• Probabilistic Mass Mapping with Neural Score Estimation
• Gravitational Collapse in General Relativity and in $R^2$-gravity: A Comparative Study
• Localization of binary mergers with gravitational-wave detectors of second and third generation
• Constraining the microlensing effect on time delays with new time-delay prediction model in $H_0$ measurements
• First Results on Dark Matter Substructure from Astrometric Weak Lensing
• Les Houches Lectures on Indirect Detection of Dark Matter
• Spitzer Planck Herschel Infrared Cluster (SPHerIC) survey: Candidate galaxy clusters at 1.3 < z < 3 selected by high star-formation rate
• A Critical Assessment of Solutions to the Galaxy Diversity Problem
• Measuring the scale of cosmic homogeneity with SDSS-IV DR14 quasars
• Inflection-point Higgs Inflation
• KiDS-Legacy calibration: unifying shear and redshift calibration with the SKiLLS multi-band image simulations
• Measuring gravity at cosmological scales
• Fermi GBM Observations of GRB 150101B: A Second Nearby Event with a Short Hard Spike and a Soft Tail
• Lyman-$\alpha$ forest constraints on interacting dark sectors
• Offset between X-ray and optical centers in clusters of galaxies: connecting eROSITA data and simulations
• Head-to-Toe Measurement of El Gordo: Improved Analysis of the Galaxy Cluster ACT-CL J0102-4915 with New Wide-field Hubble Space Telescope Imaging Data
• KiDS-450: Tomographic Cross-Correlation of Galaxy Shear with {\it Planck} Lensing
• Beyond $\Lambda$CDM constraints from the full shape clustering measurements from BOSS and eBOSS
• Molecular Line Observations in Two Dusty Star-Forming Galaxies at z = 6.9
• Testing logarithmic corrections on $R^2$-exponential gravity by observational data
• Fundamental differences in the radio properties of red and blue quasars: Insight from the LOFAR Two-metre Sky Survey (LoTSS)
• DES Y1 Results: Validating cosmological parameter estimation using simulated Dark Energy Surveys
• Forecasting Interacting Vacuum-Energy Models using Gravitational Waves
• The mass assembly of high-redshift black holes
• A New Light Higgs Boson and Short-Baseline Neutrino Anomalies
• Foreground Biases on Primordial Non-Gaussianity Measurements from the CMB Temperature Bispectrum: Implications for Planck and Beyond
• Quenching and morphological evolution due to circumgalactic gas expulsion in a simulated galaxy with a controlled assembly history
• A model of interacting dark fluids tested with supernovae and Baryon Acoustic Oscillations data
• The Atacama Cosmology Telescope DR6 and DESI: Structure formation over cosmic time with a measurement of the cross-correlation of CMB Lensing and Luminous Red Galaxies
• A new astrophysical solution to the Too Big To Fail problem - Insights from the MoRIA simulations
• Probing the small-scale structure in strongly lensed systems via transdimensional inference
• Relativistic numerical cosmology with Silent Universes
• Dark Matter Particle Explorer observations of high-energy cosmic ray electrons plus positrons and their physical implications
• Planck intermediate results. XL. The Sunyaev-Zeldovich signal from the Virgo cluster
• Exploring the GRB population: Robust afterglow modelling
• Strongly gravitational lensed SNe Ia as multi-messengers: Direct test of the Friedmann-Lema\^ıtre-Robertson-Walker metric
• Isotropy of low redshift type Ia Supernovae: A Bayesian analysis
• Testing Modified Gravity Theories via Wide Binaries and GAIA
• Statistical modelling of the cosmological dispersion measure
• Galaxy sizes and the galaxy-halo connection -- I: the remarkable tightness of the size distributions
• Dark energy with a gradient coupling to the dark matter fluid: cosmological dynamics and structure formation
• Cosmological Evolution and Exact Solutions in a Fourth-order Theory of Gravity
• Hydrostatic mass estimates of massive galaxy clusters: a study with varying hydrodynamics flavours and non-thermal pressure support
• Model-independent Constraints on Cosmic Curvature and Opacity
• Mass Calibration of Optically Selected DES clusters using a Measurement of CMB-Cluster Lensing with SPTpol Data
• Shocks in the Stacked Sunyaev-Zel'dovich Profiles of Clusters I: Analysis with the Three Hundred Simulations
• On Cepheid Distance Scale Bias due to Stellar Companions and Cluster Populations
• Milky Way Tomography with K and M Dwarf Stars: the Vertical Structure of the Galactic Disk
• Cosmic expansion parametrization: Implication for curvature and ${\text{H}}_0$ tension
• Common Origin of Dirac Neutrino Mass and Freeze-in Massive Particle Dark Matter
• Testing Bose-Einstein Condensate dark matter models with the SPARC galactic rotation curves data
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: Measuring the anisotropic Baryon Acoustic Oscillations with redshift weights
• The Pursuit of Dark Matter at Colliders - An Overview
• New method for initial density reconstruction
• Squeezed Bispectrum in the $\delta N$ Formalism: Local Observer Effect in Field Space
• Fast full N-body simulations of generic modified gravity: conformal coupling models
• SNIa-Cosmology Analysis Results from Simulated LSST Images: from Difference Imaging to Constraints on Dark Energy
• Null tests of the standard model using the linear model formalism
• A Statistical Semi-Empirical Model: Satellite galaxies in Groups and Clusters
• Minimal gauge inflation and the refined Swampland conjecture
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• Discovery of the first heavily obscured QSO candidate at $z>6$ in a close galaxy pair
• Stop Coannihilation in the CMSSM and SubGUT Models
• Dipolar modulation in the size of galaxies: The effect of Doppler magnification
• Nowhere to Hide: Radio-faint AGN in the GOODS-N field. I. Initial catalogue and radio properties
• Sensitivity of the Cherenkov Telescope Array to the detection of a dark matter signal in comparison to direct detection and collider experiments
• Discovery of a galaxy overdensity around a powerful, heavily obscured FRII radio galaxy at z=1.7: star formation promoted by large-scale AGN feedback?
• On the common nature of dark matter and dark energy: galaxy groups
• The origin of radio emission in broad absorption line quasars: Results from the LOFAR Two-metre Sky Survey
• Strong C IV emission from star-forming galaxies: a case for high Lyman continuum photon escape
• Probing the properties of relic neutrinos using the cosmic microwave background, the Hubble Space Telescope and galaxy clusters
• Spatial clustering and halo occupation distribution modeling of local AGN via cross-correlation measurements with 2MASS galaxies
• Hunting sub-GeV dark matter with NO$\nu$A near detector
• Electromagnetic Backgrounds and Potassium-42 Activity in the DEAP-3600 Dark Matter Detector
• Cosmic Magnetism in Centimeter and Meter Wavelength Radio Astronomy
• Chemical abundances and radial velocities in the extremely metal-poor galaxy DDO 68
• A highly predictive $A_4$ flavour 3-3-1 model with radiative inverse seesaw mechanism
• Varying fundamental constants principal component analysis: additional hints about the Hubble tension
• The Gaia DR2 halo white dwarf population: the luminosity function, mass distribution and its star formation history
• Integrated approach to cosmology: Combining CMB, large-scale structure and weak lensing
• Evidence for the existence of abundant intracluster light at z= 1.24
• Cosmic filaments in galaxy cluster outskirts: quantifying finding filaments in redshift space
• A measurement of the CMB E-mode angular power spectrum at subdegree scales from 670 square degrees of POLARBEAR data
• Probing the origin of extragalactic magnetic fields with Fast Radio Bursts
• A redshift-dependent IRX-$\beta$ dust attenuation relation for TNG50 galaxies
• Unveiling the hidden universe with JWST: The contribution of dust-obscured galaxies to the stellar mass function at $z\sim 3-8$
• Testing the Evolutionary Link between Type 1 and Type 2 Quasars with Measurements of the Interstellar Medium
• The MillenniumTNG Project: The impact of baryons and massive neutrinos on high-resolution weak gravitational lensing convergence maps
• Multi-Component Dark Matter in a Non-Abelian Dark Sector
• Statistical Test of Distance--Duality Relation with Type Ia Supernovae and Baryon Acoustic Oscillations
• Highly-ionized metals as probes of the circumburst gas in the natal regions of gamma-ray bursts
• Effects of baryons on weak lensing peak statistics
• A study of the hydrostatic mass bias dependence and evolution within The Three Hundred clusters
• Dynamic Localised Turbulent Diffusion and its Impact on the Galactic Ecosystem
• Cosmological parameter estimation via iterative emulation of likelihoods
• The POlarised GLEAM Survey (POGS) I: First Results from a Low-Frequency Radio Linear Polarisation Survey of the Southern Sky
• Galaxy Cluster Mass Reconstruction Project - IV. Understanding the effects of imperfect membership on cluster mass estimation
• Optimizing LIGO with LISA forewarnings to improve black-hole spectroscopy
• Dust continuum, CO, and [C I] 1-0 lines: self-consistent H2 mass estimates and the possibility of globally CO-dark galaxies at $z=0.35$
• Properties of the ionized CGM and IGM: a comparison of galaxy formation models via the Sunyaev-Zel'dovich effect
• CLUMP-3D. Three dimensional lensing and multi-probe analysis of MACS J1206.2-0847, a remarkably regular cluster
• Search for the birefringence of gravitational waves with the third observing run of Advanced LIGO-Virgo
• The Red Dead Redemption Survey of Circumgalactic Gas About Massive Galaxies. I. Mass and Metallicity of the Cool Phase
• Estimating the cosmological constant from shadows of Kerr--de Sitter black holes
• Extreme scenarios: the tightest possible constraints on the power spectrum due to primordial black holes
• Do Cosmic Rays Heat the Early Intergalactic Medium?
• COMAP Early Science: V. Constraints and Forecasts at $z\sim 3$
• Dark matter scattering cross section and dynamics in dark Yang-Mills theory
• Mapping the hot gas temperature in galaxy clusters using X-ray and Sunyaev-Zel'dovich imaging
• LIGO/Virgo black holes and dark matter: The effect of spatial clustering
• Testing Einstein's gravity and dark energy with growth of matter perturbations: Indications for new Physics?
• A novel way to determine the scale of inflation
• $H_0$ Tension and the Phantom Regime: A Case Study In Terms of an Infrared $f(T)$ Gravity
• Pseudo-Nambu-Goldstone dark matter and two-Higgs-doublet models
• Dark Matter interpretation of low energy IceCube MESE excess
• Atomic Interferometry Test of Dark Energy
• The Inflaton Portal to a Highly decoupled EeV Dark Matter Particle
• The redshift evolution of X-ray and Sunyaev-Zel'dovich scaling relations in the FABLE simulations
• Cosmological implications of Primordial Black Holes
• Deepest view of AGN X-ray variability with the 7 Ms Chandra Deep Field-South survey
• Gauged $U(1)$ Clockwork Theory
• Constraining the general reheating phase in the $\alpha$-attractor inflationary cosmology
• de Broglie-Proca and Bopp-Podolsky massive photon gases in cosmology
• Impact of Polarized Galactic Foreground Emission on CMB Lensing Reconstruction and Delensing of B-Modes
• Boosted Dark Matter and its implications for the features in IceCube HESE data
• Internal Delensing of Cosmic Microwave Background Acoustic Peaks
• A panchromatic spatially-resolved analysis of nearby galaxies -- I. Sub-kpc scale Main Sequence in grand-design spirals
• Cloud formation in the atomic and molecular phase: HI self absorption (HISA) towards a Giant Molecular Filament
• HI Asymmetries in LVHIS, VIVA and HALOGAS Galaxies
• Likelihood Analysis of the Minimal AMSB Model
• The MUSE Hubble Ultra Deep Field Survey. XV. The mean rest-UV spectra of Ly-alpha emitters at z>3
• Constraining FIMP from the structure formation of the Universe: analytic mapping from $m_{\mathrm{WDM}}$
• Connecting the structure of dark matter haloes to the primordial power spectrum
• A Supernova Candidate at z=0.092 in XMM-Newton Archival Data
• Isobaric Reconstruction of the Baryonic Acoustic Oscillation
• Galaxy formation in the brane world I: overview and first results
• Forecasting [C II] line-intensity mapping measurements between the end of reionization and the epoch of galaxy assembly
• Bayesian Analysis of Quasar Lightcurves with a Running Optimal Average: New Time Delay Measurements of COSMOGRAIL Gravitationally Lensed Quasars
• Gravitational wave observations, distance measurement uncertainties, and cosmology
• The Lick AGN Monitoring Project 2016: Dynamical Modeling of Velocity-Resolved H\b{eta} Lags in Luminous Seyfert Galaxies
• The High Fraction of Thin Disk Galaxies Continues to Challenge ΛCDM Cosmology
• Insight into primordial magnetic fields from 21-cm line observation with EDGES experiment
• Unification of Dark Matter - Dark Energy in Generalized Galileon Theories
• CosmicNet II: Emulating extended cosmologies with efficient and accurate neural networks
• Validating a minimal galaxy bias method for cosmological parameter inference using HSC-SDSS mock catalogs
• A comparative study of satellite galaxies in Milky Way-like galaxies from HSC, DECaLS and SDSS
• The Circumgalactic Medium of Milky Way-like Galaxies in the TNG50 Simulation -- II: Cold, Dense Gas Clouds and High-Velocity Cloud Analogs
• Abell 1201: Detection of an Ultramassive Black Hole in a Strong Gravitational Lens
• Gas contents of galaxy groups from thermal Sunyaev-Zel'dovich effects
• $R(K^{(\ast )})$ from dark matter exchange
• Revealing the Impact of Quasar Luminosity on Giant Ly$\alpha$ Nebulae
• Exposing Dark Sector with Future Z-Factories
• Dark Energy Survey Year 1 Results: Galaxy Sample for BAO Measurement
• SDSS J211852.96-073227.5: a new γ-ray flaring narrow-line Seyfert 1 galaxy
• Weak Lensing of Intensity Mapping: the Cosmic Infrared Background
• Stunted accretion growth of black holes by combined effect of the flow angular momentum and radiation feedback
• Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency
• Chandra Measurements of a Complete Sample of X-ray Luminous Galaxy Clusters: The Luminosity-Mass Relation
• Matter Lagrangian of particles and fluids
• Dark matter direct detection of a fermionic singlet at one loop
• Revolutionizing Our Understanding of AGN Feedback and its Importance to Galaxy Evolution in the Era of the Next Generation Very Large Array
• The boundary of cosmic filaments
• The heart of galaxy clusters: demographics and physical properties of cool-core and non-cool-core halos in the TNG-Cluster simulation
• Testing the Cosmic Shear Spatially-Flat Universe Approximation with Generalized Lensing and Shear Spectra
• Brane with variable tension as a possible solution to the problem of the late cosmic acceleration
• Machine Learning Applied to the Reionization History of the Universe in the 21 cm Signal
• Quenching and the UVJ diagram in the SIMBA cosmological simulation
• Testing the standard model of cosmology with the SKA: the cosmic radio dipole
• Unified Origin of Axion and Monopole Dark Matter, and Solution to the Domain-wall Problem
• Asymmetric Dark Matter Models in SO(10)
• Epoch of Reionisation 21cm Forecasting From MCMC-Constrained Semi-Numerical Models
• Big Bang Nucleosynthesis with an Inhomogeneous Primordial Magnetic Field Strength
• Consistent early and late time cosmology from the RG flow of gravity
• Constraining Neutrino Lifetimes and Magnetic Moments via Solar Neutrinos in the Large Xenon Detectors
• Beyond subhalos: Probing the collective effect of the Universe's small-scale structure with gravitational lensing
• Two dark matter candidates: the case of inert doublet and singlet scalars
• The MUSE Extremely Deep Field: Evidence for SFR-induced cores in dark-matter dominated galaxies at z=1
• Testing leptogenesis at the LHC and future muon colliders: a $Z^{\prime }$ scenario
• A Plane of High Velocity Galaxies Across the Local Group
• Astrophysical Distance Scale II. Application of the JAGB Method: A Nearby Galaxy Sample
• Isolated and dynamical black hole mergers with \texttt{B-POP}: the role of star formation and dynamics, star cluster evolution, natal kicks, mass and spins, and hierarchical mergers
• Discovery of a Supercluster in the eROSITA Final Equatorial Depth Survey: X-ray Properties, Radio Halo, and Double Relics
• Global Properties of M31's Stellar Halo from the SPLASH Survey: III. Measuring the Stellar Velocity Dispersion Profile
• The MillenniumTNG Project: Intrinsic alignments of galaxies and halos
• Constraining the primordial magnetic field with dwarf galaxy simulations
• Impact of young stellar components on quiescent galaxies: deconstructing cosmic chronometers
• Prospects for multi-messenger detection of binary neutron star mergers in the fourth LIGO-Virgo-KAGRA observing run
• The minimal type-I seesaw model with maximally-restricted texture zeros
• Constraints on $\gamma$-CDM interactions matching the Planck data precision
• The case for decaying spin-3/2 dark matter
• Gravitational-wave selection effects using neural-network classifiers
• A Deep Learning Approach to Infer Galaxy Cluster Masses from Planck Compton$-y$ parameter maps
• AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton
• The role of core-collapse physics in the observability of black-hole neutron-star mergers as multi-messenger sources
• SALT2 Versus SALT3: Updated Model Surfaces and Their Impacts on Type Ia Supernova Cosmology
• Cosmology with Stacked Cluster Weak Lensing and Cluster-Galaxy Cross-Correlations
• Transit cosmological models with observational constraints in f(Q, T) gravity
• The Arcminute Microkelvin Imager Catalogue of Gamma-ray Burst afterglows at 15.7 GHz
• The Evolving Effect Of Cosmic Web Environment On Galaxy Quenching
• The cosmic dust rate across the Universe
• On the decreasing fraction of Strong Ly$\alpha$ Emitters around $z$ $\sim$ $6$-$7$
• Effects of a neutrino-dark energy coupling on oscillations of high-energy neutrinos
• Deep and rapid observations of strong-lensing galaxy clusters within the sky localisation of GW170814
• Massive Star-Forming Galaxies Have Converted Most of Their Halo Gas into Stars
• Coupled quintessence and the impossibility of an interaction: a dynamical analysis study
• Cross-correlation of weak lensing and gamma rays: implications for the nature of dark matter
• Measuring the sound horizon and absolute magnitude of SNIa by maximizing the consistency between low-redshift data sets
• Reheating and Dark Radiation after Fibre Inflation
• Strongly Lensed Gravitational Waves and Electromagnetic Signals as Powerful Cosmic Rulers
• Surface effects on the red giant branch
• Multi-messenger constraints on Abelian-Higgs cosmic string networks
• Ringing of a black hole in a dark matter halo
• Blue Rest-Frame UV-Optical Colors in z~8 Galaxies from GREATS: Very Young Stellar Populations at ~650 Myr of Cosmic Time
• A search for low-energy neutrinos correlated with gravitational wave events GW150914, GW151226 and GW170104 with the Borexino detector
• A new direction for dark matter research: intermediate mass compact halo objects
• Impact of Ly$\alpha$ heating on the global 21-cm signal from the Cosmic Dawn
• Geometrical destabilization, premature end of inflation and Bayesian model selection
• Probing motion of fast radio burst sources by timing strongly lensed repeaters
• Particle motions and Gravitational Lensing in de Rham-Gabadadze-Tolley Massive Gravity Theory
• Leggett-Garg Inequalities for Squeezed States
• Constraining the spatial curvature with cosmic expansion history in a cosmological model with a non-standard sound horizon
• Speed from light: growth rate and bulk flow at z ~ 0.1 from improved SDSS DR13 photometry
• Following the Cosmic Evolution of Pristine Gas III: The Observational Consequences of the Unknown Properties of Population III Stars
• Formation channels of slowly rotating early-type galaxies
• Intensity mapping cross-correlations II: HI halo models including shot noise
• AGN Selection Methods Have Profound Impacts on the Distributions of Host Galaxy Properties
• Direct collapse to supermassive black hole seeds: the critical conditions for suppression of ${\mathrm{H}}_2$ cooling
• Graviton mass might reduce tension between early and late time cosmological data
• Using CMB spectral distortions to distinguish between dark matter solutions to the small-scale crisis
• Monte Carlo simulation of the SABRE PoP background
• Reconstructing the Inflationary Landscape with Cosmological Data
• Globular Clusters Formed within Dark Halos I: present-day abundance, distribution and kinematics
• The Contribution of In-situ and Ex-situ Star Formation in Early-Type Galaxies: MaNGA versus IllustrisTNG
• Search for dark matter produced in association with a Higgs boson decaying to $\gamma \gamma$ or ${\tau }^{+}{\tau }^{-}$ at $\sqrt{s}=$ 13 TeV
• Quark and Lepton Mixing Patterns from a Common Discrete Flavor Symmetry with Generalized CP
• A Search for Low-mass Dark Matter via Bremsstrahlung Radiation and the Migdal Effect in SuperCDMS
• The separate universe framework in group field theory condensate cosmology
• Bayesian Comparison of Interacting Scenarios
• Formation of Galactic Disks I: Why Did the Milky Way's Disk Form Unusually Early?
• Testing the anisotropy of cosmic acceleration from Pantheon supernovae sample
• Displaced vertex signature of type-I seesaw
• Hierarchical binary black hole mergers in globular clusters: mass function and evolution with redshift
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: Dynamical dark energy
• The Diverse Morphology, Stellar Population, and Black Hole Scaling Relations of the Host Galaxies of Nearby Quasars
• A study of stellar orbit fractions: simulated IllustrisTNG galaxies compared to CALIFA observations
• Conservative cosmology: combining data with allowance for unknown systematics
• No evidence for modifications of gravity from galaxy motions on cosmological scales
• Fuzzy Dark Matter as a Solution to Reconcile the Stellar Mass Density of High-z Massive Galaxies and Reionization History
• BAO from angular clustering: optimization and mitigation of theoretical systematics
• The Conditional Colour-Magnitude Distribution: I. A Comprehensive Model of the Colour-Magnitude-Halo Mass Distribution of Present-Day Galaxies
• The Shape and Size distribution of HII Regions near the percolation transition
• Radiation Hydrodynamical Simulations of the Birth of Intermediate-Mass Black Holes in the First Galaxies
• Cosmological model-independent test of $\Lambda$CDM with two-point diagnostic by the observational Hubble parameter data
• Exploring the astrophysics of dark atoms
• Jeans mass-radius relation of self-gravitating Bose-Einstein condensates and typical parameters of the dark matter particle
• Scalar dark matter interpretation of the DAMPE data with U(1) gauge interactions
• The impact of large-scale tides on cosmological distortions via redshift-space power spectrum
• Characterizing bias on large scale CMB $B$-modes after galactic foregrounds cleaning
• Future cosmic microwave background delensing with galaxy surveys
• Constraints on inflation with LSS surveys: features in the primordial power spectrum
• The Near and Mid-infrared photometric properties of known redshift $z\ge 5$ Quasars
• Testing Predictions of the Quantum Landscape Multiverse 2: The Exponential Inflationary Potential
• Constraining the kinetically dominated Universe
• Self-heating dark matter via semi-annihilation
• The foreground transfer function for HI intensity mapping signal reconstruction: MeerKLASS and precision cosmology applications
• Metal line emission from galaxy haloes at z~1
• Optimized Clustering Estimators for BAO Measurements Accounting for Significant Redshift Uncertainty
• Estimating QCD uncertainties in Monte Carlo event generators for gamma-ray dark matter searches
• The magnetic field structure in CTA 102 from high resolution mm-VLBI observations during the flaring state in 2016-2017
• Microphysics of Early Dark Energy
• MIGHTEE: Deep 1.4 GHz Source Counts and the Sky Temperature Contribution of Star Forming Galaxies and Active Galactic Nuclei
• Direct detection of the kinetic Sunyaev-Zel'dovich effect in galaxy clusters
• Dark Matter Halos in Interacting Dark Energy Models: Formation History, Density Profile, Spin and Shape
• Limits on statistical anisotropy from BOSS DR12 galaxies using bipolar spherical harmonics
• Dynamical analysis of cosmological models with non-Abelian gauge vector fields
• J-PLUS: Unveiling the brightest-end of the Lyα luminosity function at 2.0<z<3.3 over 1000 deg^2
• De Sitter Stability and Coarse Graining
• Euclid: Forecasts from the void-lensing cross-correlation
• ECoPANN: A Framework for Estimating Cosmological Parameters using Artificial Neural Networks
• Fractional Dark Matter decay: cosmological imprints and observational constraints
• Molecular hydrogen in IllustrisTNG galaxies: carefully comparing signatures of environment with local CO & SFR data
• Fitting string inflation to real cosmological data: the Fibre Inflation case
• Scale genesis and gravitational wave in a classically scale invariant extension of the standard model
• Studying high-z galaxies with [CII] intensity mapping
• Early-type galaxy density profiles from IllustrisTNG: II. Evolutionary trend of the total density profile
• Baryon acoustic oscillations signature in the three-point angular correlation function from the SDSS-DR12 quasar survey
• A Universe Without Dark Energy: Cosmic Acceleration from Dark Matter-Baryon Interactions
• Unexpected Topology of the Temperature Fluctuations in the Cosmic Microwave Background
• Fourier-series expansion of the dark-energy equation of state
• Geometrical compression: a new method to enhance the BOSS galaxy bispectrum monopole constraints
• Can a negative-mass cosmology explain dark matter and dark energy?
• A Synthetic Roman Space Telescope High-Latitude Imaging Survey: Simulation Suite and the Impact of Wavefront Errors on Weak Gravitational Lensing
• Unidentified Gamma-ray Sources as Targets for Indirect Dark Matter Detection with the Fermi-Large Area Telescope
• Phantom singularities and their quantum fate: general relativity and beyond
• The cross-correlation between 21cm intensity mapping maps and the Lyman-alpha forest in the post-reionization era
• Measurement of the Cold Dark Matter-Neutrino Dipole in the TianNu Simulation
• Is the dark matter particle its own antiparticle?
• On the statistics of proto-cluster candidates detected in the Planck all-sky survey
• Introduction to Big Bang Nucleosynthesis and Modern Cosmology
• Lepton-Jets and Low-Mass Sterile Neutrinos at Hadron Colliders
• Power-law solution for homogeneous and isotropic universe in $f(R,T)$ gravity
• Production and Backreaction of Fermions from Axion-$SU(2)$ Gauge Fields during Inflation
• Bayesian estimation of thermonuclear reaction rates for deuterium+deuterium reactions
• Viscous Dark Energy In Bianchi Type V Space-Time
• Probing Diffuse Gas with Fast Radio Bursts
• Secularly powered outflows from AGN: the dominance of non-merger driven supermassive black hole growth
• Tightening geometric and dynamical constraints on dark energy and gravity: galaxy clustering, intrinsic alignment and kinetic Sunyaev-Zel'dovich effect
• Generalized dark energy interactions with multiple fluids
• The Radiative Z2 Breaking Twin Higgs
• Bayesian Mass Estimates of the Milky Way: including measurement uncertainties with hierarchical Bayes
• An accurate perturbative approach to redshift space clustering of biased tracers in modified gravity
• Agegraphic dark energy: growth index and cosmological implications
• Evolution of CMB spectral distortion anisotropies and tests of primordial non-Gaussianity
• Massive and modified gravity as self-gravitating media
• Binary evolution, gravitational-wave mergers and explosive transients in multiple-populations gas-enriched globular-clusters
• Tsallis holographic dark energy in Fractal Universe
• A tale of dark matter capture, sub-dominant WIMPs, and neutrino observatories
• Multi-messenger-Athena Synergy White Paper
• Evidence for Inside-Out Galaxy Growth and Quenching of a z~2 Compact Galaxy from High-Resolution Molecular Gas Imaging
• Inferring high redshift large-scale structure dynamics from the Lyman-alpha forest
• Constraining An Exact Brans-Dicke gravity theory with Recent Observations
• Sensitivity of strong lensing observations to dark matter substructure: a case study with Euclid
• Vector Boson Scattering Processes: Status and Prospects
• Estimating Covariance Matrices for Two- and Three-Point Correlation Function Moments in Arbitrary Survey Geometries
• Does information entropy play a role in the expansion and acceleration of the Universe?
• High-resolution synthetic UV-submm images for simulated Milky Way-type galaxies from the Auriga project
• Can Cosmological Simulations Reproduce the Spectroscopically Confirmed Galaxies Seen at $z\ge 10$?
• No Evidence for Millimeter Continuum Source Overdensities in the Environments of $z\gtrsim 6$ Quasars
• Polypolar spherical harmonic decomposition of galaxy correlators in redshift space: Toward testing cosmic rotational symmetry
• Thermodynamic constraints on a varying cosmological-constant-like term from the holographic equipartition law with a power-law corrected entropy
• Exploring Cosmic Origins with CORE: Extragalactic sources in Cosmic Microwave Background maps
• Timing the Neutrino Signal of a Galactic Supernova
• Moving around the cosmological parameter space: a nonlinear power spectrum reconstruction based on high-resolution cosmic responses
• A ring accelerator? Unusual jet dynamics in the IceCube candidate PKS 1502+106
• An Accelerating Cosmological Model from a Parametrization of Hubble Parameter
• Jeans instability and turbulent gravitational collapse of Bose-Einstein Condensate dark matter halos
• Simulated forecasts for primordial B-mode searches in ground-based experiments
• Constraining self-interacting dark matter with scaling laws of observed halo surface densities
• Making the Universe at 20 MeV
• Self-consistent analysis of stellar clusters: An application to HST data of the halo globular cluster NGC 6752
• Group quenching and galactic conformity at low redshift
• Beyond delta: Tailoring marked statistics to reveal modified gravity
• Fundamental Plane of Black Hole Activity in Quiescent Regime
• Scale dependence of galaxy biasing investigated by weak gravitational lensing: An assessment using semi-analytic galaxies and simulated lensing data
• A New Signal Model for Axion Cavity Searches from N-Body Simulations
• A Projected Estimate of the Reionization Optical Depth Using the CLASS Experiment's Sample-Variance Limited E-Mode Measurement
• Precision CMB constraints on eV-scale bosons coupled to neutrinos
• Supersymmetry with Dark Matter is still natural
• The role of temperature dependent string-inspired CPT violating backgrounds in leptogenesis and the chiral magnetic effect
• Kantowski-Sachs Einstein-Aether Scalar Field Cosmological Models
• Dark Matter Halo Properties vs. Local Density and Cosmic Web Location
• Neutral versus ionized gas kinematics at z~2.6: The AGN-host starburst galaxy PKS 0529-549
• Neutrino Masses and Mass Hierarchy: Evidence for the Normal Hierarchy
• LHC Collider Phenomenology of Minimal Universal Extra Dimensions
• Discovery of the local counterpart of disc galaxies at z > 4: The oldest thin disc of the Milky Way using Gaia-RVS
• Probing extra dimension through gravitational wave observations of compact binaries and their electromagnetic counterparts
• Nonlocal gravity and gravitational-wave observations
• Observable gravitational waves in pre-big bang cosmology: an update
• Impact of Schumann resonances on the Einstein Telescope and projections for the magnetic coupling function
• Rapid bound-state formation of Dark Matter in the Early Universe
• Shortcomings of New Parametrizations of Inflation
• KiDS-i-800: Comparing weak gravitational lensing measurements in same-sky surveys
• Massive, Absorption-selected Galaxies at Intermediate Redshifts
• Mapping the Escape Fraction of Ionizing Photons Using Resolved Stars: A Much Higher Escape Fraction for NGC 4214
• Dark-ages Reionization and Galaxy Formation Simulation XX. The Ly$\alpha$ IGM transmission properties and environment of bright galaxies during the Epoch of Reionization
• Relieving tensions related to the lensing of CMB temperature power spectra
• Polarimetry at millimeter wavelengths with the NIKA camera: calibration and performance
• Dissecting the interstellar medium of a z=6.3 galaxy: X-shooter spectroscopy and HST imaging of the afterglow and environment of the Swift GRB 210905A
• Anisotropic stars made of exotic matter within the complexity factor formalism
• Constraints on $f(T)$ Cosmology with Pantheon+
• Studying the morphology of HI isodensity surfaces during reionization using Shapefinders and percolation analysis
• Tachyon Inflation in Teleparallel Gravity
• Primordial non-Gaussianities and zero bias tracers of the Large Scale Structure
• Enhancing AGN efficiency and cool-core formation with anisotropic thermal conduction
• Beyond the bulge-halo conspiracy? Density profiles of Early-type galaxies from extended-source strong lensing
• Reionisation in sterile neutrino cosmologies
• Wandering in the Lyman-alpha Forest: A Study of Dark Matter-Dark Radiation Interactions
• Effects of stellar-mass primordial black holes on first star formation
• Consistency of Modified Gravity with a decreasing $G_{\mathrm{eff}}(z)$ in a $\Lambda$CDM background
• The Effective Halo Model: Creating a Physical and Accurate Model of the Matter Power Spectrum and Cluster Counts
• Extracting cosmological information from the angular power spectrum of the 2MASS Photometric Redshift catalogue
• The WaZP galaxy cluster sample of the Dark Energy Survey Year 1
• Constraints on Cosmological Parameters from the Angular Power Spectrum of a Combined 2500 deg${}^2$ SPT-SZ and Planck Gravitational Lensing Map
• First axion dark matter search with toroidal geometry
• Quasar Sightline and Galaxy Evolution (QSAGE) Survey - I. The Galaxy Environment of OVI Absorbers up to z=1.4 around PKS 0232-04
• Weak lensing magnification in the Dark Energy Survey Science Verification Data
• Accelerated Bayesian inference using deep learning
• ALMA constraints on star-forming gas in a prototypical z=1.5 clumpy galaxy: the dearth of CO(5-4) emission from UV-bright clumps
• On the stability conditions for theories of modified gravity in presence of matter fields
• From large-scale environment to CGM angular momentum to star forming activities -- I: star-forming galaxies
• GAMBIT and its Application in the Search for Physics Beyond the Standard Model
• Testing Predictions of the Quantum Landscape Multiverse 1: The Starobinsky Inflationary Potential
• The formation of low surface brightness galaxies in the IllustrisTNG simulation
• A High-Resolution Investigation of the Multi-Phase ISM in a Galaxy during the First Two Billion Years
• Bayesian group finder based on marked point processes. Method and feasibility study using the 2MRS data set
• 2MTF - VII. 2MASS Tully-Fisher survey final data release: distances for 2,062 nearby spiral galaxies
• Impact of the reduced speed of light approximation on the post-overlap neutral hydrogen fraction in numerical simulations of the epoch of reionization
• Imprint of anisotropic primordial non-Gaussianity on halo intrinsic alignments in simulations
• Non-minimally coupled scalar field cosmology with torsion
• The Evolution of the Interstellar Medium in Post-Starburst Galaxies
• Constraining resonant dark matter with combined LHC electroweakino searches
• Gravitational waves $\times$ HI intensity mapping: cosmological and astrophysical applications
• Formation and Morphology of the First Galaxies in the Cosmic Morning
• Hubble Space Telescope Wide Field Camera 3 Observations of Escaping Lyman Continuum Radiation from Galaxies and Weak AGN at Redshifts $z$$\simeq$2.3-4.1
• Dark matter-baryon scaling relations from Einasto halo fits to SPARC galaxy rotation curves
• Bounds on Ultra-Light Hidden-Photon Dark Matter from 21cm at Cosmic Dawn
• The HI Velocity Function: a test of cosmology or baryon physics?
• Probing dust-obscured star formation in the most massive Gamma-Ray Burst host galaxies
• Dark sector searches with the CMS experiment
• Measuring the reionization optical depth without large-scale CMB polarization
• The Not-So-Well Tempered Neutralino
• Measuring the Tidal Response of Structure Formation: Anisotropic Separate Universe Simulations using TreePM
• The imprint of $f(R)$ gravity on weak gravitational lensing II : Information content in cosmic shear statistics
• Structure formation in the Deser-Woodard nonlocal gravity model: a reappraisal
• Imprint of entanglement entropy in the power spectrum of inflationary fluctuations
• The Kinematics and Dark Matter Fractions of TNG50 Galaxies at z=2 from an Observational Perspective
• The degeneracy between primordial non-Gaussianity and foregrounds in 21cm intensity mapping experiments
• Systematic errors induced by the elliptical power-law model in galaxy-galaxy strong lens modeling
• Combining ILC and moment expansion techniques for extracting average-sky signals and CMB anisotropies
• Extensions to the halo occupation distribution model for more accurate clustering predictions
• Theoretical and observational constraints on regularized 4$D$ Einstein-Gauss-Bonnet gravity
• SDSS-IV MaNGA: drivers of stellar metallicity in nearby galaxies
• The New Numerical Galaxy Catalogue (ν^2 GC): Properties of Active Galactic Nuclei and Their Host Galaxies
• Properties of reionization-era galaxies from JWST luminosity functions and 21-cm interferometry
• Seeing-limited imaging sky surveys -- small vs. large telescopes
• Light Sterile Neutrino and Dark Matter in Left-Right Symmetric Models Without Higgs Bidoublet
• Estimating parameters of binary black holes from gravitational-wave observations of their inspiral, merger and ringdown
• Direction and redshift drifts for general observers and their applications in cosmology
• VVV CL001: Likely the Most Metal-Poor Surviving Globular Cluster in the Inner Galaxy
• Constraining spatial curvature with large-scale structure
• The velocity dispersion function of early-type galaxies and its redshift evolution: the newest results from lens redshift test
• Viscous dark matter and 21 cm cosmology
• Prediction of Supernova Rates in Known Galaxy-galaxy Strong-lens Systems
• Neutrinoless Double Beta Decay in Left-Right Symmetry with Universal Seesaw
• Local AGN Survey (LASr): I. Galaxy sample, infrared colour selection and predictions for AGN within 100 Mpc
• Generalized thermodynamic constraints on holographic-principle-based cosmological scenarios
• Semi-analytic forecasts for Roman -- the beginning of a new era of deep-wide galaxy surveys
• Search for supersymmetry with a compressed mass spectrum in events with a soft $\tau$ lepton, a highly energetic jet, and large missing transverse momentum in proton-proton collisions at $\sqrt{s}=$ 13 TeV
• Fuzzy Dark Matter from Infrared Confining Dynamics
• $R_{\mathrm{e}}$. I. Understanding galaxy sizes, associated luminosity densities, and the artificial division of the early-type galaxy population
• Cosmological consequences and statefinder diagnosis of a non-interacting generalized Chaplygin gas in $f(R,T)$ gravity
• Unequal-Time Correlators for Cosmology
• A new quadruple gravitational lens from the Hyper Suprime-Cam Survey: the puzzle of HSC~J115252+004733
• Analytical model for cluster radio relics
• Cosmological implications of an interacting model of dark matter \& dark energy
• On the Detection of Supermassive Primordial Stars
• The extended Baryon Oscillation Spectroscopic Survey: measuring the cross-correlation between the MgII flux transmission field and quasars and galaxies at $z=0.59$
• Impact of next-to-leading order contributions to CMB lensing
• Astrophysics & Cosmology from Line Intensity Mapping vs Galaxy Surveys
• Simulating the effect of photoheating feedback during reionization
• Intrinsic galaxy alignment from angular dependent primordial non-Gaussianity
• Small-scale galaxy clustering in the EAGLE simulation
• Testing strong lensing subhalo detection with a cosmological simulation
• Multipartite Dark Matter in $SU(2{)}_N$ extension of Standard Model and signatures at the LHC
• Testing scalar versus vector dark matter
• Starobinsky-Like Inflation and Neutrino Masses in a No-Scale SO(10) Model
• Theoretical systematics in testing the Cosmological Principle with the kinematic quasar dipole
• The Impact of Wrong Assumptions in BAO Reconstruction
• Probing bino-wino coannihilation dark matter under the neutrino floor at the LHC
• H$\alpha$ intensity map of the repeating fast radio burst FRB 121102 host galaxy from Subaru/Kyoto 3DII AO-assisted optical integral-field spectroscopy
• Tidal evolution of dark matter annihilation rates in subhalos
• Looking for the left sneutrino LSP with displaced-vertex searches
• Massive central galaxies of galaxy groups in the Romulus simulations: an overview of galaxy properties at z=0
• Dark Matter in Anomaly-Free Gauge Extensions
• Umbrella sampling: a powerful method to sample tails of distributions
• Forecasting Polarized Radio Sources for CMB observations
• ETHOS - an Effective Theory of Structure Formation: detecting dark matter interactions through the Lyman-$\alpha$ forest
• A natural $Z^{\prime }$-portal Majorana dark matter in alternative U(1) extended Standard Model
• Cosmological simulation in tides: power spectra and halo shape responses, and shape assembly bias
• Constraining the dark matter-vacuum energy interaction using the EDGES 21-cm absorption signal
• Non-Abelian $S$-term dark energy and inflation
• Global HI asymmetries in IllustrisTNG: a diversity of physical processes disturb the cold gas in galaxies
• Model independent bounds on Type Ia supernova absolute peak magnitude
• Intrinsic alignment statistics of density and velocity fields at large scales: Formulation, modeling, and baryon acoustic oscillation features
• Inflation Model Selection meets Dark Radiation
• Calculation of Momentum Distribution Function of a Non-thermal Fermionic Dark Matter
• Return of the X-rays: A New Hope for Fermionic Dark Matter at the keV Scale
• DES Y1 results: Splitting growth and geometry to test $\Lambda$CDM
• A multi-instrument non-parametric reconstruction of the electron pressure profile in the galaxy cluster CLJ1226.9+3332
• Neutrino mass and dark energy constraints from redshift-space distortions
• Measurement of the pairwise kinematic Sunyaev-Zeldovich effect with Planck and BOSS data
• Consistent Scalar and Tensor Perturbation Power Spectra in Single Fluid Matter Bounce with Dark Energy Era
• [CII] line intensity mapping the epoch of reionization with the Prime-Cam on FYST
• The First Quiescent Galaxies in TNG300
• Polarized Sunyaev Zel'dovich tomography
• Stability of the Einstein static universe in Eddington-inspired Born-Infeld theory
• Observational constraints on the physical nature of submillimetre source multiplicity: chance projections are common
• Models of vacuum energy interacting with cold dark matter: Constraints and comparison
• Mass profile decomposition of the Frontier Fields cluster MACS J0416-02403. Insights on the Dark-Matter inner profile
• Scalarons mimicking Dark Matter in the Hu-Sawicki model of f(R) gravity
• Cosmological searches for a non-cold dark matter component
• Observational Constraints on $f(T)$ Gravity from Model-Independent Data
• Photo-z outlier self-calibration in weak lensing surveys
• Random Potentials and Cosmological Attractors
• Learning to Concentrate: Multi-tracer Forecasts on Local Primordial Non-Gaussianity with Machine-Learned Bias
• Hamilton-Jacobi formalism for inflation with non-minimal derivative coupling
• Quenching Timescales in the IllustrisTNG Simulation
• Non-linear contributions to angular power spectra
• Beyond two-point statistics: using the minimum spanning tree as a tool for cosmology
• The critical geometry of a thermal big bang
• Analyzing the cosmic variance limit of remote dipole measurements of the cosmic microwave background using the large-scale kinetic Sunyaev Zel'dovich effect
• Forbidden Dark Matter at the Weak Scale via the Top Portal
• Relic Abundance in a Secluded Dark Matter Scenario with a Massive Mediator
• Impact of axisymmetric mass models for dwarf spheroidal galaxies on indirect dark matter searches
• Gamma Rays From Dark Matter Subhalos Revisited: Refining the Predictions and Constraints
• The Close AGN Reference Survey (CARS): Comparative analysis of the structural properties of star-forming and non-star-forming galaxy bars
• Nuclear kinematics in nearby AGN. I. An ALMA perspective on the Morphology and Kinematics of the molecular CO(2-1) emission
• Synthesizing the intrinsic FRB population using frbpoppy
• Non-Minimal Flavored ${\mathbf{S}}_3\otimes {\mathbf{Z}}_2$ Left-Right Symmetric Model
• A complete view of the outskirts of the Coma cluster
• Two is not always better than one: Single Top Quarks and Dark Matter
• Field redefinitions in theories beyond Einstein gravity using the language of differential forms
• Selection of massive evolved galaxies at $3\le z\le 4.5$ in the CANDELS fields
• Mass varying neutrinos, symmetry breaking, and cosmic acceleration
• The Three Hundred Project: the stellar and gas profiles
• Evolution of linear wave dark matter perturbations in the radiation-dominant era
• Barred spiral galaxies in modified gravity theories
• A paradigm of warm quintessential inflation and production of relic gravity waves
• A Survey of CH2DOH Towards Starless and Prestellar Cores in the Taurus Molecular Cloud
• High-redshift quasars at $z\ge 3$ -- I. Radio spectra
• Dynamics of relativistic radio jets in asymmetric environments
• Median statistics estimates of Hubble and Newton's Constant
• Inflection-point inflation in hyper-charge oriented U(1)${}_X$ model
• Non-parametric reconstruction of interaction in the cosmic dark sector
• The BPT Diagram in Cosmological Galaxy Formation Simulations: Understanding the Physics Driving Offsets at High-Redshift
• UV to submillimetre luminosity functions of TNG50 galaxies
• A Perturbative Approach to the Redshift Space Correlation Function: Beyond the Standard Model
• Collapse threshold for a cosmological Klein Gordon field
• Testing non-minimally coupled inflation with CMB data: a Bayesian analysis
• Evaporation of planetary atmospheres due to XUV illumination by quasars
• A First Look at Spatially Resolved Balmer Decrements at $1.0<z<2.4$ from JWST NIRISS Slitless Spectroscopy
• Constraining High-Energy Neutrino Emission from Supernovae with IceCube
• The Einstein dark energy model
• Spatially Homogeneous Einstein-Aether Cosmological Models: Scalar Fields with a Generalized Harmonic Potential
• Gravitational wave as probe of superfluid dark matter
• Systematics of Adiabatic Modes: Flat Universes
• Model-independent curvature determination with 21cm intensity mapping experiments
• Leptophilic dark matter in gauged $U(1{)}_{L_e-L_{\mu }}$ model in light of DAMPE cosmic ray $e^{+}+e^{-}$ excess
• Matter bispectrum beyond Horndeski
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measuring the evolution of the growth rate using redshift space distortions between redshift 0.8 and 2.2
• The Environments of the Most Energetic Gamma-Ray Bursts
• Weak Lensing Analysis of SPT selected Galaxy Clusters using Dark Energy Survey Science Verification Data
• Precision constraints on radiative neutrino decay with CMB spectral distortion
• A Parameter-Masked Mock Data Challenge for Beyond-Two-Point Galaxy Clustering Statistics
• Bayesian Redshift Classification of Emission-line Galaxies with Photometric Equivalent Widths
• The $H_0$ Tension in Non-flat QCDM Cosmology
• Texas Spectroscopic Search for Ly$\alpha$ Emission at the End of Reionization I. Constraining the Ly$\alpha$ Equivalent Width Distribution at 6.0 < $z$ < 7.0
• A new strong-lensing galaxy at z=0.066: Another elliptical galaxy with a lightweight IMF
• Observations in Quantum Cosmology
• Confronting fuzzy dark matter with the rotation curves of nearby dwarf irregular galaxies
• Ruling out Critical Higgs Inflation?
• Constraining the X-ray heating and reionization using 21-cm power spectra with Marginal Neural Ratio Estimation
• Dark Matter Interactions, Helium, and the CMB
• The fraction and kinematics of broad absorption line quasars across cosmic time
• Constraining the Expansion History and Early Dark Energy with Line Intensity Mapping
• The Pandora project. I: the impact of radiation and cosmic rays on baryonic and dark matter properties of dwarf galaxies
• Mock data study for next-generation ground-based detectors: The performance loss of matched filtering due to correlated confusion noise
• CODEX Weak Lensing: Concentration of Galaxy Clusters at z ~ 0.5
• Forward modeling of galaxy populations for cosmological redshift distribution inference
• Constraints on neutrino speed, weak equivalence principle violation, Lorentz invariance violation, and dual lensing from the first high-energy astrophysical neutrino source TXS 0506+056
• Probing the $z\gtrsim 6$ quasars in a universe with IllustrisTNG physics: Impact of gas-based black hole seeding models
• Investigation of dust attenuation and star formation activity in galaxies hosting GRBs
• Estimating the warm dark matter mass from strong lensing images with truncated marginal neural ratio estimation
• Beyond Starobinsky inflation
• Observational Constraints on Constant Roll Inflation
• The scatter in the galaxy-halo connection: a machine learning analysis
• On the Amplitude and Stokes Parameters of a Stochastic Gravitational-Wave Background
• Modeling Evolution of Galactic Bars at Cosmic Dawn
• Hadrophilic Dark Sectors at the Forward Physics Facility
• Fast Radio Burst Distributions Consistent with the First CHIME/FRB Catalog
• Fast full $N$-body simulations of generic modified gravity: derivative coupling models
• Investigating the relation between gravitational wave tests of general relativity
• On the relative effect of nodes and filaments of the cosmic web on the quenching of galaxies and the orientation of their spin
• Optimization of model independent gravitational wave search using machine learning
• Evidence for massive warm-hot circumgalactic medium around NGC 3221
• Dark Energy Survey Year 1 Results: Cross-correlation between DES Y1 galaxy weak lensing and SPT+Planck CMB weak lensing
• A fast semi-discrete optimal transport algorithm for a unique reconstruction of the early Universe
• Accurate tracer particles of baryon dynamics in the adaptive mesh refinement code Ramses
• Simulation-based inference of dynamical galaxy cluster masses with 3D convolutional neural networks
• Remarks on the weak cosmic censorship conjecture of RN-AdS black holes with cloud of strings and quintessence under the scalar field
• A joint ALMA-Bolocam-Planck SZ study of the pressure distribution in RX J1347.5-1145
• Testing the violation of the equivalence principle in the electromagnetic sector and its consequences in $f(T)$ gravity
• The baryonic Tully-Fisher relation in the Simba simulation
• Baryon acoustic oscillations reconstruction using convolutional neural networks
• Hamiltonian diagonalization in hybrid quantum cosmology
• Lightening Gravity-Mediated Dark Matter
• Linear Point and Sound Horizon as Purely Geometric standard rulers
• The dark matter component of the Gaia radially anisotropic substructure
• Cosmological Evidence Modelling: a new simulation-based approach to constrain cosmology on non-linear scales
• Probing the inert doublet model using jet substructure with a multivariate analysis
• Pre-inflation and Trans-Planckian Censorship
• WIMPflation
• Extracting the Subhalo Mass Function from Strong Lens Images with Image Segmentation
• Warm Dark Matter and Cosmic Reionization
• Constraints on Early Star Formation from the 21-cm Global Signal
• Minimal model for the fermion flavor structure, mass hierarchy, dark matter, leptogenesis, and the electron and muon anomalous magnetic moments
• AMICO galaxy clusters in KiDS-DR3: cosmological constraints from large-scale stacked weak lensing profiles
• NuSTAR perspective on high-redshift MeV blazars
• The Cosmic Ultraviolet Baryon Survey (CUBS) IV: The Complex Multiphase Circumgalactic Medium as Revealed by Partial Lyman Limit Systems
• Comparison between the Logotropic and $\Lambda$CDM models at the cosmological scale
• X-ray-inferred kinematics of the core ICM in Perseus-like clusters: Insights from the TNG-Cluster simulation
• Observational constraints on bimetric gravity
• Joint estimation of the Epoch of Reionization power spectrum and foregrounds
• Symmetry Breaking and Reheating after Inflation in No-Scale Flipped SU(5)
• Relaxion: A Landscape Without Anthropics
• Statistical Significance of spectral lag transition in GRB 160625B
• Implications of CHIME repeating fast radio bursts
• Late-time magnetogenesis driven by ALP dark matter and dark photon
• Stellar winds and metal enrichment from fast-rotating Population III stars
• Weak-lensing mass calibration of the Sunyaev-Zel'dovich effect using APEX-SZ galaxy clusters
• CMB internal delensing with general optimal estimator for higher-order correlations
• Numerical simulations of stochastic inflation using importance sampling
• Tensor Minkowski Functionals: first application to the CMB
• Origin of highly $r$-process-enhanced stars in a cosmological zoom-in simulation of a Milky Way-like galaxy
• Cosmology with the CMB temperature-polarization correlation
• Measuring the Small-Scale Matter Power Spectrum with High-Resolution CMB Lensing
• A Flexible Analytic Model of Cosmic Variance in the First Billion Years
• The Carnegie-Chicago Hubble Program. IV. The Distances to NGC 4424, NGC 4526, and NGC 4536 via the Tip of the Red Giant Branch
• Exploring dark matter, neutrino mass and $R_{K^{(\ast )},\varphi }$ anomalies in $L_{\mu }-L_{\tau }$ model
• Dynamics of the generalized unimodular gravity theory
• The Discovery of a Gravitationally Lensed Supernova Ia at Redshift 2.22
• DM halo morphological types of MW-like galaxies in the TNG50 simulation: Simple, Twisted, or Stretched
• Multi-band gravitational wave astronomy: science with joint space- and ground-based observations of black hole binaries
• Small-scale structure and the Lyman-$\alpha$ forest baryon acoustic oscillation feature
• Evolution of the Thermodynamic Properties of Clusters of Galaxies out to Redshift of 1.8
• The luminous host galaxy, faint supernova and rapid afterglow rebrightening of GRB 100418A
• The observed galaxy bispectrum from single-field inflation in the squeezed limit
• Converting entropy to curvature perturbations after a cosmic bounce
• Measurement of the Cosmic Microwave Background Polarization Lensing Power Spectrum from Two Years of POLARBEAR Data
• Induced Affine Inflation
• Mass Calibration of the CODEX Cluster Sample using SPIDERS Spectroscopy -- I. The Richness-Mass Relation
• The Collapse of Atomically-Cooled Primordial Haloes. I. High Lyman-Werner Backgrounds
• Test of the FLRW metric and curvature with strong lens time delays
• Initial condition for baryogenesis via neutrino oscillation
• Constraints on light dark matter particles using white dwarf stars
• How much metals did the first stars provide to the ultra-faint dwarfs?
• Searching for giga-Jansky fast radio bursts from the Milky Way with a global array of low-cost radio receivers
• Two-Loop $Z_4$ Dirac Neutrino Masses and Mixing, with Self-Interacting Dark Matter
• Observational constrained $F(R,\mathcal{G})$ gravity cosmological model and the dynamical system analysis
• Investigating Cluster Astrophysics and Cosmology with Cross-Correlation of the Thermal Sunyaev-Zel'dovich Effect and Weak Lensing
• Metal Mixing in Minihalos: The Descendants of Pair-Instability Supernovae
• Power Spectra Based Planck Constraints on Compensated Isocurvature, and Forecasts for LiteBIRD and CORE Space Missions
• Prediction of H$\alpha$ and [OIII] Emission Line Galaxy Number Counts for Future Galaxy Redshift Surveys
• Constraining the $\Lambda$CDM and Galileon models with recent cosmological data
• Radio signatures from encounters between Neutron Stars and QCD-Axion Minihalos around Primordial Black Holes
• The MillenniumTNG Project: Inferring cosmology from galaxy clustering with accelerated N-body scaling and subhalo abundance matching
• ProFuse: Physical Multi-Band Structural Decomposition of Galaxies and the Mass-Size-Age Plane
• Inflation in Loop Quantum Cosmology
• Narrowing down the possible explanations of cosmic acceleration with geometric probes
• Observability of intermittent radio sources in galaxy groups and clusters
• Constraining the dark-energy equation of state with cosmological data
• A search for prompt gamma-ray counterparts to fast radio bursts in the Insight-HXMT data
• Modelling of Lyman-alpha Emitting Galaxies and Ionized Bubbles at the Era of Reionization
• The physical drivers of the atomic hydrogen-halo mass relation
• CMB lensing power spectrum estimation without instrument noise bias
• Prospects for axion detection in natural SUSY with mixed axion-higgsino dark matter: back to invisible?
• Phase space of modified Gauss-Bonnet gravity
• The interstellar medium distribution, gas kinematics, and system dynamics of the far-infrared luminous quasar SDSS J2310+1855 at $z=6.0$
• Maximum Entropy Inferences on the Axion Mass in Models with Axion-Neutrino Interaction
• Implications from simulated strong gravitational lensing systems: constraining cosmological parameters using Gaussian Processes
• KODIAQ-Z: Metals and Baryons in the Cool Intergalactic and Circumgalactic Gas at 2.2<z<3.6
• What sparks the radio-loud phase of nearby quasars?
• Fermi-LAT kills dark matter interpretations of AMS-02 data. Or not?
• Magnetars in Ultra-Long Gamma-Ray Bursts
• A Broadband Spectro-polarimetric View of the NVSS Rotation Measure Catalogue I: Breaking the nπ-ambiguity
• Dark energy and Dark matter interaction in light of the second law of thermodynamics
• Flows around galaxies. I. The dependency of galaxy connectivity on cosmic environments and effects on the star-formation rate
• MaNGA DynPop -- III. Stellar dynamics versus stellar population relations in 6000 early-type and spiral galaxies: Fundamental Plane, mass-to-light ratios, total density slopes, and dark matter fractions
• Revising the Hubble constant, spatial curvature and dark energy dynamics with the latest observations of quasars
• Disentangling Dark Physics with Cosmic Microwave Background Experiments
• Do the observational data favor a local void?
• Kiloparsec-scale AGN Outflows and Feedback in Merger-Free Galaxies
• Parameter discordance in Planck CMB and low-redshift measurements: projection in the primordial power spectrum
• Modelling the Accelerating Universe with $f(Q)$ Gravity: Observational Consistency
• Detecting cosmological gravitational waves background after removal of compact binary coalescences in future gravitational wave detectors
• Thermal Instabilities and Shattering in the High-Redshift WHIM: Convergence Criteria and Implications for Low-Metallicity Strong HI Absorbers
• Multi-Frequency Observations of the Candidate Neutrino Emitting Blazar BZB J0955+3551
• Testing gravity with galaxy-galaxy lensing and redshift-space distortions using CFHT-Stripe 82, CFHTLenS and BOSS CMASS datasets
• Euclid preparation. XXXII. Evaluating the weak lensing cluster mass biases using the Three Hundred Project hydrodynamical simulations
• A comprehensive view of the interstellar medium in a quasar host galaxy at z~6.4
• Multiwavelength variability study and search for periodicity of PKS 1510-089
• On the consistency of $\Lambda$CDM with CMB measurements in light of the latest Planck, ACT, and SPT data
• Density modulated star formation efficiency: implications for the observed abundance of ultra-violet luminous galaxies at z>10
• WALLABY Pilot Survey: HI gas disc truncation and star formation of galaxies falling into the Hydra I cluster
• ODIN: Where Do Lyman-alpha Blobs Live? Contextualizing Blob Environments within the Large-Scale Structure
• The next non-Gaussianity frontier: what can a measurement with $\sigma (f_{\mathrm{NL}})\lesssim 1$ tell us about multifield inflation?
• Measuring galaxy cluster masses with CMB lensing using a Maximum Likelihood estimator: Statistical and systematic error budgets for future experiments
• X-ray properties of He II 1640 emitting galaxies in VANDELS
• Multicolor Optical Monitoring of the Blazar S5 0716+714 from 2017 to 2019
• Observational constraints on Starobinsky $f(R)$ cosmology from cosmic expansion and structure growth data
• Dark matter production via a non-minimal coupling to gravity
• Prospects for constraining interacting dark energy models from gravitational wave and gamma ray burst joint observation
• Constraints on the epoch of dark matter formation from Milky Way satellites
• Polarized accretion shocks from the cosmic web
• Physics with Reactor Neutrinos
• Curvature from strong gravitational lensing: a spatially closed Universe or systematics?
• Towards a census of high-redshift dusty galaxies with $Herschel$: A selection of "500 $\mu$m-risers"
• Cosmological inference from emulator based halo model I: Validation tests with HSC and SDSS mock catalogs
• A Census of the LyC Photons that Form the UV Background During Reionization
• Dynamical analysis of interacting dark energy model in the framework of particle creation mechanism
• Reheating predictions in Gravity Theories with Derivative Coupling
• SU(5)$\times$U(1)${}_X$ grand unification with minimal seesaw and $Z^{\prime }$-portal dark matter
• Primordial perturbations with pre-inflationary bounce
• The dispersion measure of Fast Radio Bursts host galaxies: estimation from cosmological simulations
• Probing features in inflaton potential and reionization history with future CMB space observations
• CMB constraints on $\beta$-exponential inflationary models
• Testing keV sterile neutrino dark matter in future direct detection experiments
• GA-NIFS: Multi-phase analysis of a star-forming galaxy at $z\sim 5.5$
• Singlet scalar Dark matter in $U(1{)}_{B-L}$ models without right-handed neutrinos
• Maximal extensions and singularities in inflationary spacetimes
• Can the GW190814 secondary component be a bosonic dark matter admixed compact star?
• Hidden strongly interacting massive particles
• Explaining the $W$ boson mass anomaly and dark matter with a $U(1)$ dark sector
• Revisiting the Hubble constant, spatial curvature and cosmography with time-delay and cosmic chronometer observations
• Evaluation of cosmological models in $f(R,T)$ gravity in different dark energy scenario
• Modifying PyUltraLight to model scalar dark matter with self-interactions
• Wide Binaries from GAIA EDR3: preference for GR over MOND ?
• Light gravitino dark matter: LHC searches and Hubble tension
• The importance of preventive feedback: inference from observations of the stellar masses and metallicities of Milky Way dwarf galaxies
• SPICE: the connection between cosmic reionisation and stellar feedback in the first galaxies
• Evolution of star formation rate-density relation over cosmic time in a simulated universe: the observed reversal reproduced
• Shattering of Cosmic Sheets due to Thermal Instabilities: a Formation Channel for Metal-Free Lyman Limit Systems
• Planck's dusty GEMS. V. Molecular wind and clump stability in a strongly lensed star-forming galaxy at z=2.2
• Exploring Fermionic Dark Matter via Higgs Boson Precision Measurements at the Circular Electron Positron Collider
• Electromagnetic cascade masquerade: a way to mimic $\gamma$--axion-like particle mixing effects in blazar spectra
• Evaluating Black Hole Detectability with LISA
• Conformal Realization of the Neutrino Option
• Testing the Distance-Duality Relation in the $R_h=ct$ Universe
• Challenging matter creation models in the phantom divide
• Scalar field dark matter in clusters of galaxies
• $f(Q)$-gravity and neutrino physics
• Foreground modelling via Gaussian process regression: an application to HERA data
• Analysing dissipative effects in the $\Lambda$CDM model
• Globular cluster numbers in dark matter haloes in a dual formation scenario: an empirical model within EMERGE
• Cosmographic analysis of a closed bouncing universe with the varying cosmological constant in $f(R,T)$ gravity
• From quantum gravity to gravitational waves through cosmic strings
• Understanding parameter differences between analyses employing nested data subsets
• Effect of CP violation in the singlet-doublet dark matter model
• Probing Cosmic Dawn: Modelling the Assembly History, SEDs, and Dust Content of Selected $z\sim 9$ Galaxies
• Probing Dark Matter with Disappearing Tracks at the LHC
• The Birth of Binary Direct-Collapse Black Holes
• The Physical Origin of Galactic Conformity: From Theory to Observation
• What is flat ΛCDM, and may we choose it?
• X-ray emission from the nuclear region of Arp 220
• Prospects of strongly lensed repeating fast radio bursts: complementary constraints on dark energy evolution
• Fast Weak Lensing Simulations with Halo Model
• Observing Cosmological Processes in Real Time with Repeating Fast Radio Bursts
• A VLA Study of High-redshift GRBs I - Multi-wavelength Observations and Modeling of GRB 140311A
• The Extremely Luminous Quasar Survey in the Pan-STARRS 1 Footprint (PS-ELQS)
• The First Direct Search for Inelastic Boosted Dark Matter with COSINE-100
• Characterising the intra-cluster light in The Three Hundred simulations
• Observability of Low-Luminosity AGN in the Early Universe with JWST
• Image segmentation for analyzing galaxy-galaxy strong lensing systems
• Energy Conditions in Higher Derivative $f(R,\square R,T)$ Gravity
• Strongly Coupled Quintessence
• The galaxy size - halo mass scaling relations and clustering properties of central and satellite galaxies
• Determining Cosmology for a Nonlocal Realization of MOND
• Supersymmetric Resonant Dark Matter: a Thermal Model for the AMS-02 Positron Excess
• Growth of matter perturbations in the extended viscous dark energy models
• Size distribution of galaxies in SDSS DR7: weak dependence on halo environment
• Revival of the Deser-Woodard nonlocal gravity model: Comparison of the original nonlocal form and a localized formulation
• Three observational differences for binary black holes detections with second and third generation gravitational-wave detectors
• Constraining Primordial Non-Gaussianity with Post-reconstructed Galaxy Bispectrum in Redshift Space
• Probing Cosmology with Dark Matter Halo Sparsity Using X-ray Cluster Mass Measurements
• How sound are our ultra-light axion approximations?
• X-ray emission from warm-hot intergalactic medium: the role of resonantly scattered cosmic X-ray background
• A Further Test of Lorentz Violation from the Rest-Frame Spectral Lags of Gamma-Ray Bursts
• SKYSURF: Constraints on Zodiacal Light and Extragalactic Background Light through Panchromatic HST All-Sky Surface-Brightness Measurements: I. Survey Overview and Methods
• On the direct detection of multi-component dark matter: implications of the relic abundance
• Forward Modeling of Double Neutron Stars: Insights from Highly-Offset Short Gamma-Ray Bursts
• On measuring the Galactic dark matter halo with hypervelocity stars
• Cosmological perturbation theory in Generalized Einstein-Aether models
• Axion-photon-dark photon oscillation and its implication for 21 cm observation
• Complementing the ground-based CMB Stage-4 experiment on large scales with the PIXIE satellite
• Cosmological solutions with gravitational particle production and non-zero curvature
• Quadratic estimator for CMB cross-correlation
• A magnified view of circumnuclear star formation and feedback around an AGN at z=2.6
• Flavor origin of dark matter and its relation with leptonic nonzero ${\theta }_{13}$ and Dirac CP phase $\delta$
• Neural Network Reconstruction of $H^{\prime }(z)$ and its application in Teleparallel Gravity
• Nuclear high-ionisation outflow in the Compton-thick AGN NGC6552 as seen by the JWST mid-infrared instrument
• Universality for quintessence
• New EoR Power Spectrum Limits From MWA Phase II Using the Delay Spectrum Method and Novel Systematic Rejection
• Non-minimal Derivative Coupling Scalar Field and Bulk Viscous Dark Energy
• Implications for primordial black holes from cosmological constraints on scalar-induced gravitational wave
• Non-parametric dark energy reconstruction using the tomographic Alcock-Paczynski test
• Cosmology-marginalized approaches in Bayesian model comparison: the neutrino mass as a case study
• The role of the tachyonic instability in Horndeski gravity
• VINTERGATAN-GM: The cosmological imprints of early mergers on Milky-Way-mass galaxies
• The Goldilocks problem of the quasar contribution to reionization
• Verlinde's emergent gravity versus MOND and the case of dwarf spheroidals
• The minimum and maximum gravitational-wave background from supermassive binary black holes
• Assessing Perturbativity and Vacuum Stability in High-Scale Leptogenesis
• Enhanced UV radiation and dense clumps in Mrk231's molecular outflow
• Extracting bias using the cross-bispectrum: An EoR and 21 cm-[CII]-[CII] case study
• How cosmological merger histories shape the diversity of stellar haloes
• NuSTAR Uncovers an Extremely Local Compton-thick AGN in NGC 4968
• A hint on the metal-free star formation rate density from 21cm-EDGES data
• Quasi-extremal primordial black holes are a viable dark matter candidate
• The impact of the Large Magellanic Cloud on dark matter direct detection signals
• The MaNGA FIREFLY Value-Added-Catalogue: resolved stellar populations of 10,010 nearby galaxies
• Constraints on anisotropic primordial non-Gaussianity from intrinsic alignments of SDSS-III BOSS galaxies
• Hot thermal universe endowed with massive dark vector fields and the Hubble tension
• Multi-wavelength properties of radio and machine-learning identified counterparts to submillimeter sources in S2COSMOS
• Dynamics of Chiral Cosmology
• Developing a unified pipeline for large-scale structure data analysis with angular power spectra -- I. The importance of redshift-space distortions for galaxy number counts
• Optical Observations Reveal Strong Evidence for High Energy Neutrino Progenitor
• Inferring the population properties of binary black holes from unresolved gravitational waves
• Including massive neutrinos in thermal Sunyaev Zeldovich power spectrum and cluster counts analyses
• General formulation of cosmological perturbations in scalar-tensor dark energy coupled to dark matter
• Investigating scalar-tensor-gravity with statistics of the cosmic large-scale structure
• Eccentricity-induced systematic error on parametrized tests of general relativity: Hierarchical Bayesian inference applied to a binary black hole population
• Optical and near-infrared observations of the SPT2349-56 proto-cluster core at z = 4.3
• Exploring the posterior surface of the large scale structure reconstruction
• $\alpha$ attractors in Quintessential Inflation motivated by Supergravity
• Lepton Portal Limit of Inert Higgs Doublet Dark Matter with Radiative Neutrino Mass
• The invisible decay of Higgs boson in the context of a thermal and non-thermal relic in MSSM
• Exploring Cosmic Origins with CORE: Cluster Science
• Large-Scale Velocity Dispersion and the Cosmic Web
• Analysis of accretion disk around a black hole in dRGT massive gravity
• Non-Abelian Vector Boson Dark Matter, its Unified Route and signatures at the LHC
• Reconstructing the Genealogy of LIGO-Virgo Black Holes
• Quantum Cosmology and the Evolution of Inflationary Spectra
• Joule-Thomson Expansion of RN-AdS Black Hole Immersed in Perfect Fluid Dark Matter
• Constraints on inflation revisited: An analysis including the latest local measurement of the Hubble constant
• Diagnostic of Horndeski Theories
• Increasing the Lensing Figure of Merit through Higher Order Convergence Moments
• Simulations of Galactic polarized synchrotron emission for Epoch of Reionization observations
• Inflationary predictions of double-well, Coleman-Weinberg, and hilltop potentials with non-minimal coupling
• Extracting foreground-obscured $\mu$-distortion anisotropies to constrain primordial non-Gaussianity
• Can Assembly Bias Explain the Lensing Amplitude of the BOSS CMASS Sample in a Planck Cosmology?
• A Model Connecting Galaxy Masses, Star Formation Rates, and Dust Temperatures Across Cosmic Time
• Do high-spin high-mass X-ray binaries contribute to the population of merging binary black holes?
• Electron Flavored Dark Matter
• Red quasars blow out molecular gas from galaxies during the peak of cosmic star formation
• Growth of stellar mass black holes in dense molecular clouds and GW190521
• Bright Extragalactic ALMA Redshift Survey (BEARS) III: Detailed study of emission lines from 71 Herschel targets
• Power Spectrum of Intrinsic Alignments of Galaxies in IllustrisTNG
• Dark matter assisted Dirac leptogenesis and neutrino mass
• VLA Legacy Survey of Molecular Gas in Massive Star-forming Galaxies at High Redshift
• The Event Horizon Telescope Image of the Quasar NRAO 530
• First study of reionization in the Planck 2015 normalized closed $\Lambda$CDM inflation model
• Combining the CLAUDS & HSC-SSP surveys: U+grizy(+YJHKs) photometry and photometric redshifts for 18M galaxies in the 20 deg2 of the HSC-SSP Deep and ultraDeep fields
• High Energy Neutrinos from Choked Gamma-Ray Bursts in AGN Accretion Disks
• Calibrating Cluster Number Counts with CMB lensing
• The Three Hundred Project: Substructure in hydrodynamical and dark matter simulations of galaxy groups around clusters
• Wavelet-Bayesian inference of cosmic strings embedded in the cosmic microwave background
• Deeper multi-redshift upper limits on the Epoch of Reionization 21-cm signal power spectrum from LOFAR between z=8.3 and z=10.1
• Heavy quark-philic scalar dark matter with a vector-like fermion portal
• Bounds on abundance of primordial black hole and dark matter from EDGES 21-cm signal
• Multipole expansion for HI intensity mapping experiments: simulations and modelling
• The Origin of the Dust Extinction Curve in Milky Way-like Galaxies
• A thermodynamics revision of Rastall gravity
• The Cosmic Baryon Partition between the IGM and CGM in the SIMBA Simulations
• Constraints on Supersymmetric Dark Matter for Heavy Scalar Superpartners
• CHEX-MATE: Constraining the origin of the scatter in galaxy cluster radial X-ray surface brightness profiles
• Towards a non-Gaussian model of redshift space distortions
• Towards an improved model of self-interacting dark matter haloes
• Massive quiescent galaxies at $z\sim 3$: a comparison of selection, stellar population and structural properties with simulation predictions
• Searching for gravitational wave bursts from cosmic string cusps with the Parkes Pulsar Timing Array
• Sensitivity of dark matter haloes to their accretion histories
• Deep optical observations contemporaneous with emission from the periodic FRB 180916.J0158+65
• MaNGIA: 10,000 mock galaxies for stellar population analysis
• SHAPing the Gas: Understanding Gas Shapes in Dark Matter Haloes with Interpretable Machine Learning
• Statistics of the fractional polarisation of compact radio sources in Planck maps
• Planck ISW-lensing likelihood and the CMB temperature
• ALMA observations of a metal-rich damped Lyα absorber at z = 2.5832: evidence for strong galactic winds in a galaxy group
• Isotropic vs. Anisotropic components of BAO data: a tool for model selection
• Detection of a high-redshift molecular outflow in a primeval hyperstarburst galaxy
• Detection of cross-correlation between gravitational lensing and gamma rays
• The formation of early-type galaxies through monolithic collapse of gas clouds in Milgromian gravity
• Potential Gravitational-wave and Gamma-ray Multi-messenger Candidate from Oct. 30, 2015
• Search for gamma-ray emission from super-luminous supernovae with the Fermi-LAT
• Analysis of a subsolar-mass compact binary candidate from the second observing run of Advanced LIGO
• Generalized covariant prescriptions for averaging cosmological observables
• MUSE Analysis of Gas around Galaxies (MAGG) -- V: Linking ionized gas traced by CIV and SiIV absorbers to Ly$\alpha$ emitting galaxies at $z\approx 3.0-4.5$
• A case for kinetically dominated initial conditions for inflation
• The MillenniumTNG Project: The large-scale clustering of galaxies
• Thermodynamically allowed phantom cosmology with viscous fluid
• Geometrical Destabilisation of Ultra-Light Axions in String Inflation
• Non-Gaussianity in the Weak Lensing Correlation Function Likelihood -- Implications for Cosmological Parameter Biases
• Core or cusps: The central dark matter profile of a redshift one strong lensing cluster with a bright central image
• Diffusion in unimodular gravity: Analytical solutions, late-time acceleration, and cosmological constraints
• Clustering with JWST: Constraining Galaxy Host Halo Masses, Satellite Quenching Efficiencies, and Merger Rates at z=4-10
• Spatially Resolved Water Emission from Gravitationally Lensed Dusty Star Forming Galaxies at z $\sim$ 3
• Isospin-violating dark matter in the light of recent data
• HST/WFC3 grism observations of $z\sim 1$ clusters: Evidence for rapid outside-in environmental quenching from spatially resolved H$\alpha$ maps
• Shock waves in the magnetized cosmic web: the role of obliquity and cosmic-ray acceleration
• Hillclimbing inflation
• The most luminous AGN do not produce the majority of the detected stellar-mass black hole binary mergers in the local Universe
• Large-scale clustering as a probe of the origin and the host environment of fast radio bursts
• Cosmological information content in redshift-space power spectrum of SDSS-like galaxies in the quasi-nonlinear regime up to $k=0.3h$Mpc${}^{-1}$
• SHARP -- VI. Evidence for CO (1-0) molecular gas extended on kpc-scales in AGN star forming galaxies at high redshift
• Extended Phase Space Analysis of Interacting Dark Energy Models in Loop Quantum Cosmology
• Charming Dark Matter
• Self-interacting dark matter with a stable vector mediator
• A multi-simulation study of relativistic SZ temperature scalings in galaxy clusters and groups
• Leptogenesis in fast expanding Universe
• Broad-lined type Ic supernova iPTF16asu: A challenge to all popular models
• The Linear Point: A cleaner cosmological standard ruler
• Late-time evolution of the Universe within a two-scalar-field cosmological model
• Estimating the Mass of the Local Group using Machine Learning Applied to Numerical Simulations
• Parameter Inference for Weak Lensing using Gaussian Processes and MOPED
• When is the growth index constant?
• Constraining the dark energy statefinder hierarchy in a kinematic approach
• A new measure of tension between experiments
• Substructure at High Speed II: The Local Escape Velocity and Milky Way Mass with Gaia DR2
• Lens modelling of the strongly lensed Type Ia supernova iPTF16geu
• How galaxies populate haloes in very low-density environments? An analysis of the Halo Occupation Distribution in cosmic voids
• From EMBER to FIRE: predicting high resolution baryon fields from dark matter simulations with Deep Learning
• Weak lensing peak statistics in the era of large scale cosmological surveys
• Propagators for gauge-invariant observables in cosmology
• A Mid-infrared Study of Superluminous Supernovae
• On the environmental influence of groups and clusters of galaxies beyond the virial radius: Galactic conformity at few Mpc scales
• Investigating the cause of the $\alpha$-$z$ relation
• VLA Radio Study of a Sample of Nearby X-ray and Optically Bright Early-Type Galaxies
• Modelling a bright z = 6 galaxy at the faint end of the AGN luminosity function
• Assessing the Importance of Noise from Thermal Sunyaev-Zel{'}dovich Signals for CMB Cluster Surveys and Cluster Cosmology
• Quantified diffuse light in compact groups of galaxies
• Characterization of binary black holes by heterogeneous gravitational-wave networks
• Scalar-tensor mixed polarization search of gravitational waves
• Survival of molecular gas in a stellar feedback-driven outflow witnessed with the MUSE TIMER project and ALMA
• Inflationary Features and Shifts in Cosmological Parameters from Planck 2015 Data
• Cosmology with the pairwise kinematic SZ effect: Calibration and validation using hydrodynamical simulations
• Theoretical predictions for dark matter detection in dwarf irregular galaxies with gamma rays
• Searching for Oscillations in the Primordial Power Spectrum with CMB and LSS Data
• QCD axion dark matter from long-lived domain walls during matter domination
• Anisotropic halo assembly bias and redshift-space distortions
• Revealing the cosmic reionisation history with fast radio bursts in the era of Square Kilometre Array
• A comment on power-law inflation with a dark radiation component
• Type Ia supernova Hubble diagram with near-infrared and optical observations
• Monte Carlo simulations of multiple populations in globular clusters: constraints on the cooling flow vs. accretion scenario using million bodies simulations
• Constraining power of cosmological observables: blind redshift spots and optimal ranges
• Probing features in the primordial perturbation spectrum with large-scale structure data
• The population of tidal disruption events discovered with eROSITA
• A model of spectral line broadening in signal forecasts for line-intensity mapping experiments
• Testing isotropy in the Universe using photometric and spectroscopic data from the SDSS
• Neural physical engines for inferring the halo mass distribution function
• Dynamics of warm power-law plateau inflation with a generalized inflaton decay rate: predicctions and constraints after Planck 2015
• Simulating galaxy formation in f(R) modified gravity: Matter, halo, and galaxy-statistics
• Dark Higgs Dark Matter
• WALLABY Pilot Survey: HI in the host galaxy of a Fast Radio Burst
• Exact solutions, finite time singularities and non-singular universe models from a variety of $\Lambda (t)$ cosmologies
• Constraining Dark Matter properties with the first generation of stars
• Baryon Number, Lepton Number, and Operator Dimension in the SMEFT with Flavor Symmetries
• High-resolution VLA Imaging of Obscured Quasars: Young Radio Jets Caught in a Dense ISM
• Exploring the origin of multiwavelength activities of high-redshift FSRQ PKS 1502+106 during 2014-2018
• Testing gravity theories using tensor perturbations
• Probing Feedback via IGM tomography and Ly$\alpha$ forest with Subaru PFS, TMT/ELT, and JWST
• The Escape Fraction of Ionizing Photons During the Epoch of Reionization: observability with the Square Kilometre Array
• On Minkowski Functionals of CMB polarization
• The first Hubble diagram and cosmological constraints using superluminous supernova
• Probing the thermal history during reionization using a semi-numerical photon-conserving code SCRIPT
• Can Conformal and Disformal Couplings Between Dark Sectors Explain the EDGES 21cm Anomaly?
• VLBA polarimetric monitoring of 3C 111
• Next generation design and prospects for CANNEX
• Constraining spontaneous black hole scalarization in scalar-tensor-Gauss-Bonnet theories with current gravitational-wave data
• Targeting Bright Metal-poor Stars in the Disk and Halo Systems of the Galaxy
• Detecting Cosmic Reionization using Bi-Spectrum Phase
• The Redshift Evolution of the Binary Black Hole Mass Distribution from Dense Star Clusters
• Understanding the relation between thermal Sunyaev-Zeldovich decrement and halo mass using the SIMBA and TNG simulations
• A Bayesian analysis of sneutrino DM in the NMSSM with Type-I seesaw mechanism
• On Neutron Star Mergers as the Source of r-process Enhanced Metal Poor Stars in the Milky Way
• The June 2016 Optical and Gamma-Ray Outburst and Optical Micro-Variability of the Blazar 3C454.3
• DEVILS: Cosmic evolution of SED-derived metallicities and their connection to star-formation histories
• Chandra and ALMA observations of the nuclear activity in two strongly lensed star forming galaxies
• A Hubble Space Telescope Imaging Survey of Low-Redshift Swift-BAT Active Galaxies
• Fast optimization algorithms and the cosmological constant
• Associating Host Galaxy Candidates to Massive Black Hole Binaries resolved by Pulsar Timing Arrays
• The dependence of intrinsic alignment of galaxies on wavelength using KiDS and GAMA
• Heavy right-handed neutrino dark matter in left-right models
• Acceleration and propagation of ultra high energy cosmic rays
• Compact Starburst Galaxies with Fast Outflows: Central Escape Velocities and Stellar Mass Surface Densities from Multi-band Hubble Space Telescope Imaging
• On dark matter - dark radiation interaction and cosmic reionization
• Decaying dark matter, the $H_0$ tension, and the lithium problem
• Type I Abelian Higgs strings: evolution and Cosmic Microwave Background constraints
• On the Detection of Supermassive Primordial Stars. II. Blue Supergiants
• Jet efficiencies and black hole spins in jetted quasars
• Future singularities if the universe underwent Starobinsky inflation in the past
• Identifying Universality in Warm Inflation
• HST followup observations of two bright z ~ 8 candidate galaxies from the BoRG pure-parallel survey
• HST/WFC3 grism observations of $z\sim 1$ clusters: evidence for evolution in the mass-size relation of quiescent galaxies from poststarburst galaxies
• Non-oscillating power spectra in Loop Quantum Cosmology
• The maximum luminosity of fast radio bursts
• Euclid: Modelling massive neutrinos in cosmology -- a code comparison
• Conformally Coupled Tachyonic Dark Energy
• On Approximation for Fractional Stochastic Partial Differential Equations on the Sphere
• The primordial magnetic field in our cosmic backyard
• Chaotic and Clumpy Galaxy Formation in an Extremely Massive Reionization-Era Halo
• Can the quantum vacuum fluctuations really solve the cosmological constant problem?
• Statistical and systematic uncertainties in extracting the source properties of neutron star - black hole binaries with gravitational waves
• Dark Matter in the Standard Model?
• Gravitational waves from Population III binary black holes are consistent with LIGO/Virgo O3a data for the chirp mass larger than $\sim 20M_{\odot }$
• Unveiling the spectrum of inspiralling binary black holes
• Simba: The average properties of the circumgalactic medium of $2\le z\le 3$ quasars are determined primarily by stellar feedback
• Tensor Minkowski Functionals for random fields on the sphere
• Persistent Radio Emission from Synchrotron Heating by a Repeating Fast Radio Burst Source in a Nebula
• Global view of neutrino interactions in cosmology: The freestreaming window as seen by Planck
• X-ray analysis of JWST's first galaxy cluster lens SMACS J0723.3-7327
• Mono-Higgs Signature in the Scotogenic Model with Majorana Dark Matter
• Accurate determination of halo velocity bias in simulations and its cosmological implications
• Tracing the Sources of Reionization in Cosmological Radiation Hydrodynamics Simulations
• Efficient Optimal Reconstruction of Linear Fields and Band-powers from Cosmological Data
• Breaking the Vainshtein screening in clusters of galaxies
• Gravitational Waves as a Probe of Globular Cluster Formation and Evolution
• Search for Sub-eV Sterile Neutrino at RENO
• Probing Cosmic Origins with CO and [CII] Emission Lines
• Searching for the possible signal of the photon-axionlike particle oscillation in the combined GeV and TeV spectra of supernova remnants
• The effect of tides on the Sculptor dwarf spheroidal galaxy
• Late-time quantum backreaction of a very light nonminimally coupled scalar
• Model Selection with Strong-lensing Systems
• Modeling holographic dark energy with particle and future horizons
• Constraining minimal Type-III Seesaw Model from naturalness, Lepton Flavor Violation and Electroweak Vacuum stability
• DustPedia - the relationships between stars, gas and dust for galaxies residing in different environments
• Cosmology and time dependent parameters induced by misaligned light scalar
• Statistical correlation between the distribution of Ly$\alpha$ emitters and IGM HI at $z\sim 2.2$ mapped by Subaru/Hyper Suprime-Cam
• H_0 tension: clue to common nature of dark sector?
• Implications of residual CP symmetry for leptogenesis in a model with two right-handed neutrinos
• Stringy Running Vacuum Model and current Tensions in Cosmology
• Dark Matter Search in Space: Combined Analysis of Cosmic Ray Antiproton-to-Proton Flux Ratio and Positron Flux Measured by AMS-02
• Constraints on Lorentz Invariance and CPT Violation using Optical Photometry and Polarimetry of Active Galaxies BL Lacertae and S5 B0716+714
• IRAM 30m-EMIR Redshift Search of z = 3-4 Lensed Dusty Starbursts selected from the HerBS sample
• Quintessential Cosmological Tensions
• Modeling HI at the field level
• Hierarchical Bayesian inference of photometric redshifts with stellar population synthesis models
• Reconstruction of interaction rate in Holographic dark energy model with Hubble horizon as the infrared cut-off
• Bayesian analysis of the break in DAMPE lepton spectra
• Angular Momentum of Early and Late Type Galaxies: Nature or Nurture?
• Investigating the accelerated expansion of the Universe through updated constraints on viable $f(R)$ models within the metric formalism
• Constraining the Cosmic Strings Gravitational Wave Spectra in No Scale Inflation with Viable Gravitino Dark matter and Non Thermal Leptogenesis
• Imaging Polarization of the Blue-Excess Hot Dust-Obscured Galaxy WISE J011601.41-050504.0
• Multiple measurements of quasars acting as standard probes: model independent calibration and exploring the Dark Energy Equation of States
• Forecast for weighing neutrinos in cosmology with SKA
• Probing cold gas in a massive, compact star-forming galaxy at z=6
• An improved model of redshift-space distortions around voids: application to quintessence dark energy
• Resolving 3D Disk Orientation using High-Resolution Images: New Constraints on Circumgalactic Gas Inflows
• Precision Gamma-Ray Constraints for Sub-GeV Dark Matter Models
• Measuring the viscosity of dark matter with strongly lensed gravitational waves
• A Leptonic ALP Portal to the Dark Sector
• Non-Gaussianity constraints from Planck spectral distortion cross-correlations
• Parametrising non-linear dark energy perturbations
• CLEAR: The Evolution of Spatially Resolved Star Formation in Galaxies between $0.5\lesssim z\lesssim 1.7$ using H$\alpha$ Emission Line Maps
• Prospects of type-II seesaw at future colliders in light of the DAMPE $e^{+}{e}^{-}$ excess
• Testing the warmness of dark matter
• Modeling the kinematics of globular cluster systems
• Physical constraints on interacting dark energy models
• From Blue Cloud to Red Sequence: Evidence of Morphological Transition Prior to Star Formation Quenching
• Imprints of local lightcone projection effects on the galaxy bispectrum. II
• Testing generalized logotropic models with cosmic growth
• Simulating cosmologies beyond $\Lambda$CDM with PINOCCHIO
• A novel probe of bubble size statistics and time scales of the epoch of reionization using the contour Minkowski Tensor
• Impact of natal kicks on merger rates and spin-orbit misalignments of black hole -- neutron star mergers
• Discovering Dark Matter at the LHC through Its Nuclear Scattering in Far-Forward Emulsion and Liquid Argon Detectors
• Unveiling the atomic hydrogen-halo mass relation via spectral stacking
• Tomographic imaging of the Fermi-LAT gamma-ray sky through cross-correlations: A wider and deeper look
• 125 GeV Higgs boson mass and muon g-2 in 5D MSSM
• Evolution of high-redshift quasar hosts and promotion of massive black hole seed formation
• Fundamental differences in the radio properties of red and blue quasars: kiloparsec-scale structures revealed by e-MERLIN
• Bayesian comparison of nonstandard cosmologies using type Ia supernovae and BAO data
• Measurement of a Cosmographic Distance Ratio with Galaxy and CMB Lensing
• New general parametrization of quintessence fields and its observational constraints
• A First Look at Spatially Resolved Star Formation at $4.8<z<6.5$ with JWST FRESCO NIRCam Slitless Spectroscopy
• On the influence of the environment on galactic chemical abundances
• A direct measure of free electron gas via the Kinematic Sunyaev-Zel'dovich effect in Fourier-space analysis
• Constraints on primordial lepton asymmetries with full neutrino transport
• Machine Learning methods to estimate observational properties of galaxy clusters in large volume cosmological N-body simulations
• Measuring the hydrostatic mass bias in galaxy clusters by combining Sunyaev-Zel'dovich and CMB lensing data
• Quintessential inflation and cosmological seesaw Mechanism: reheating and observational constraints
• What to expect from dynamical modelling of cluster haloes II. Investigating dynamical state indicators with Random Forest
• The ultra-diffuse dwarf galaxies NGC 1052-DF2 and 1052-DF4 are in conflict with standard cosmology
• Fluids, Superfluids and Supersolids: Dynamics and Cosmology of Self Gravitating Media
• New integrable models and analytical solutions in $f(R)$~cosmology with an ideal gas
• Multi-phase black-hole feedback and a bright [CII] halo in a Lo-BAL quasar at $z\sim 6.6$
• A novel search for gravitationally lensed radio sources in wide-field VLBI imaging from the mJIVE-20 survey
• Spatially Resolved Metal Loss from M31
• Black hole - neutron star mergers: The first mass gap and kilonovae
• Isolating the Lyman Alpha Forest BAO Anomaly
• Modelling redshift-space distortion in the post-reionization $\mathrm{HI}$ 21-cm power spectrum
• The Sphere of Influence of the Bright Central Galaxies in the Diffuse Light of SDSS Clusters
• Application of the TPB Wavelength Shifter to the DEAP-3600 Spherical Acrylic Vessel Inner Surface
• The impact of baryons on the sensitivity of dark energy measurements
• CosmoReionMC: A package for estimating cosmological and astrophysical parameters using CMB, Lyman-α absorption and global 21 cm data
• Holographic dark energy: constraints on the interaction from diverse observational data sets
• The impact of inhomogeneous subgrid clumping on cosmic reionization II: modelling stochasticity
• Using LISA-like Gravitational Wave Detectors to Search for Primordial Black Holes
• GOGREEN: a critical assessment of environmental trends in cosmological hydrodynamical simulations at z ~ 1
• The mean free path of hydrogen ionizing photons during the epoch of reionization
• A solar metallicity galaxy at $z>$ 7? Possible detection of the [N II] 122 $\mu$m and [O III] 52 $\mu$m lines
• Dark Matter Relics and the Expansion Rate in Scalar-Tensor Theories
• Prospects for indirect detection of frozen-in dark matter
• Phantom braneworld and the Hubble tension
• Galaxy Formation in the Santa Cruz semi-analytic model compared with IllustrisTNG -- I. Galaxy scaling relations, dispersions, and residuals at z=0
• COSMOS2020: Identification of High-z Protocluster Candidates in COSMOS
• Search for new physics in final states with a single photon and missing transverse momentum in proton-proton collisions at $\sqrt{s}=$ 13 TeV
• A first attempt to differentiate between modified gravity and modified inertia with galaxy rotation curves
• General relativistic 'screening' in cosmological simulations
• A multiband study and exploration of the radio wave - $\gamma$-ray connection in 3C 84
• Photometric Classification of 2315 Pan-STARRS1 Supernovae with Superphot
• The Dawn of Disk Formation in a Milky Way-sized Galaxy Halo: Thin Stellar Disks at $z>4$
• Precise weak lensing constraints from deep high-resolution $K_{\mathrm{s}}$ images: VLT/HAWK-I analysis of the super-massive galaxy cluster RCS2$J$232727.7$-$020437 at $z=0.70$
• Endothermic self-interacting dark matter in Milky Way-like dark matter haloes
• Constraining Cosmology with Big Data Statistics of Cosmological Graphs
• Gravitational lensing $H_0$ tension from ultralight axion galactic cores
• On the early evolution of Local Group dwarf galaxy types: star formation and supernova feedback
• Non-minimal quartic inflation in classically conformal U(1)${}_X$ extended Standard Model
• The warm-hot, extended, massive circumgalactic medium of NGC 3221: an XMM-Newton discovery
• Observing patchy reionization with future CMB polarization experiments
• The galaxy-halo size relation of low-mass galaxies in FIRE
• Measurement of $d{+}^7$Be cross sections for Big-Bang nucleosynthesis
• Cosmic convergence and shear with extended sources
• The Ionization and Destruction of Polycyclic Aromatic Hydrocarbons in Powerful Quasars
• Dust evolution with MUPPI in cosmological volumes
• On An Interacting New Holographic Dark Energy Model: observational constraints
• GRAPH mixing
• Buckyball-metal complexes as promising carriers of astronomical unidentified infrared emission bands
• On the Cosmic Web Elongation in Fuzzy Dark Matter Cosmologies: Effects on Density Profiles, Shapes and Alignments of Halos
• Evidence for a Massive Andromeda Galaxy Using Satellite Galaxy Proper Motions
• Mapping the Likelihood of GW190521 with Diverse Mass and Spin Priors
• Missing Giants: Predictions on Dust-Obscured Galaxy Stellar Mass Assembly Throughout Cosmic Time
• The CGM${}^2$ Survey: Quenching and the Transformation of the Circumgalactic Medium
• A constrained cosmological model in $f(R,L_m)$ gravity
• Demographics of Hierarchical Black Hole Mergers in Dense Star Clusters
• The Hubble constant tension with next-generation galaxy surveys
• Measuring galaxy cluster mass profiles into the low acceleration regime with galaxy kinematics
• Simulations of multi-field ultralight axion-like dark matter
• An extremely active repeating fast radio burst source in a likely non-magneto-ionic environment
• Detection of metallicity correlations in 100 nearby galaxies
• On the redshift evolution of the baryon and gas fraction in simulated groups and clusters of galaxies
• Dark energy in scalar-vector-tensor theories
• Constraints on long-lived, higher-spin particles from galaxy bispectrum
• Unraveling the early universe's equation of state and primordial black hole production with PTA, BBN, and CMB observations
• Fortifying gravitational-wave tests of general relativity against astrophysical assumptions
• Euclidean and Hamiltonian thermodynamics for regular black holes
• Linear bias and halo occupation distribution of emission line galaxies from Nancy Grace Roman Space Telescope
• Testing f(R) gravity with the simulated data of gravitational waves from the Einstein Telescope
• Dark photon dark matter from a rolling inflaton
• The hot circumgalactic media of massive cluster satellites in the TNG-Cluster simulation: existence and detectability
• Observable gravitational waves from tidal disruption events and their electromagnetic counterpart
• Supersymmetry at a 28 TeV hadron collider: HE-LHC
• Improving the absolute accuracy of the gravitational wave detectors by combining the photon pressure and gravity field calibrators
• ASASSN-15nx: A luminous Type II supernova with a "perfect" linear decline
• The 3D Lyman-$\alpha$ Forest Power Spectrum from eBOSS DR16
• Cluster counts: calibration issue or new physics?
• Reheating through the Higgs amplified by spinodal instabilities and gravitational creation of gravitons
• Constraints on general neutrino interactions with exotic fermion from neutrino-electron scattering experiments
• A Bayesian quantification of consistency in correlated datasets
• Exploring circular polarization in the CMB due to conventional sources of cosmic birefringence
• A revised lens time delay for JVAS B0218+357 from a reanalysis of VLA monitoring data
• Imprints of quasar duty cycle on the 21cm signal from the Epoch of Reionization
• SHAM through the lens of a hydrodynamical simulation
• New Gravitational Wave Discoveries Enabled by Machine Learning
• Velocity-dependent J-factors for annihilation radiation from cosmological simulations
• Are there really conformal frames? Uniqueness of affine inflation
• X-ray redshifts for obscured AGN: a case study in the J1030 deep field
• Inflation from High-Scale Supersymmetry Breaking
• Cosmic Reionization May Still Have Started Early and Ended Late: Confronting Early Onset with CMB Anisotropy and 21 cm Global Signals
• Gravitationally Bound Bose Condensates with Rotation
• Removing the giants and learning from the crowd: a new SZ power spectrum method and revised Compton $y$-map analysis
• First cosmological constraints combining Planck with the recent gravitational-wave standard siren measurement of the Hubble constant
• LoCuSS: The splashback radius of massive galaxy clusters and its dependence on cluster merger history
• Improved analysis of GW190412 with a precessing numerical relativity surrogate waveform model
• A Fundamental Test for Galaxy Formation Models: Matching the Lyman-$\alpha$ Absorption Profiles of Galactic Halos over Three Decades in Distance
• Growth of structure in interacting vacuum cosmologies
• Perturbations in a scalar field model with virtues of $\Lambda$CDM
• How to obtain a cosmological constant from small exotic R^4
• Stellar Mass Function of Active and Quiescent Galaxies via the Continuity Equation
• SDSS-IV MaNGA: Signatures of halo assembly in kinematically misaligned galaxies
• Thermodynamics and evaporation of perfect fluid dark matter black hole in phantom background
• On the impact of the structural surface effect on global stellar properties and asteroseismic analyses
• The atomic-to-molecular hydrogen transition in the TNG50 simulation: Using realistic UV fields to create spatially resolved HI maps
• Constraining Right Handed Gauge Boson Mass from Lepton Number Violating Meson Decays in a Low Scale Left Right Model
• An updated Type II supernova Hubble diagram
• Chandra reveals a luminous Compton-thick QSO powering a $Ly\alpha$ blob in a $z=4$ starbursting protocluster
• Stau Coannihilation, Compressed Spectrum and SUSY Discovery at the LHC
• Covariance of the matter power spectrum including the survey window function effect: N-body simulations vs. fifth-order perturbation theory on grid
• The Three Hundred project: galaxy cluster mergers and their impact on the stellar component of brightest cluster galaxies
• The LSST-DESC 3x2pt Tomography Optimization Challenge
• Easing cosmic tensions with an open and hotter universe
• Cosmic metal density evolution in neutral gas: insights from observations and cosmological simulations
• On the probability of the extremely lensed $z$=6.2 Earendel source being a Population~III star
• The Atacama Cosmology Telescope: Weighing distant clusters with the most ancient light
• Disformal Dark Matter
• H0LiCOW XI. A weak lensing measurement of the external convergence in the field of the lensed quasar B1608+656 using HST and Subaru deep imaging
• Real- and redshift-space halo clustering in $f(R)$ cosmologies
• Confirmed short periodic variability of subparsec supermassive binary black hole candidate Mrk 231
• Debiasing inference with approximate covariance matrices and other unidentified biases
• Constraints on nature of ultra light dark matter particles with 21cm forest
• Wave Dark Matter and Ultra Diffuse Galaxies
• Phenomenological Reconstruction of $f(T)$ Teleparallel Gravity
• Weak Lensing Analysis of CODEX Clusters using Dark Energy Camera Legacy Survey : Mass-Richness Relation
• Anisotropic separate universe simulations
• Model-independent Estimations for the Cosmic Curvature from the Latest Strong Gravitational Lensing Systems
• Tests of Neutrino and Dark Radiation Models from Galaxy and CMB surveys
• First detection of the 448 GHz ortho-H2O line at high redshift: probing the structure of a starburst nucleus at z = 3.63
• Extreme variability in an active galactic nucleus: Gaia16aax
• Convolution Lagrangian perturbation theory for biased tracers beyond general relativity
• Texas Spectroscopic Search for Ly$\alpha$ Emission at the End of Reionization II. The Deepest Near-Infrared Spectroscopic Observation at $z\gtrsim 7$
• Impact of inhomogeneous reionization on the Lyman-α forest
• HI 21cm mapping of the host galaxy of AT2018cow: a fast-evolving luminous transient within a ring of high column density gas
• Clustering and redshift-space distortions in modified gravity models with massive neutrinos
• Do halos that form early, have high concentration, are part of a pair, or contain a central galaxy potential host more pronounced planes of satellite galaxies?
• Neutron Star Structure in the Presence of Nonminimally Coupled Scalar Fields
• On Anomaly-Free Dark Matter Models
• The Thermal Proximity Effect: A New Probe of He II Reionization History and the Quasar Lifetime
• The hunt for sub-GeV dark matter at neutrino facilities: a survey of past and present experiments
• Classification of Kerr-de Sitter-like spacetimes with conformally flat Scri
• The String Soundscape at Gravitational Wave Detectors
• Constraints on Dark Matter-Baryon Scattering from the Temperature Evolution of the Intergalactic Medium
• Witnessing the reionization history using Cosmic Microwave Background observation from Planck
• Effects of electrically charged dark matter on cosmic microwave background anisotropies
• Inference from the small scales of cosmic shear with current and future Dark Energy Survey data
• SKA-Phase 1 sensitivity for synchrotron radio emission from multi-TeV Dark Matter candidates
• CMB and matter power spectra with non-linear dark-sector interactions
• Accurate initial conditions in mixed Dark Matter--Baryon simulations
• Covariance matrices for galaxy cluster weak lensing: from virial regime to uncorrelated large-scale structure
• Quantifying the Thermal Sunyaev-Zel'dovich Effect and Excess Millimeter Emission in Quasar Environments
• The impact of baryonic physics and massive neutrinos on weak lensing peak statistics
• A Detection of CMB-Cluster Lensing using Polarization Data from SPTpol
• New constraints on the mass bias of galaxy clusters from the power spectra of the thermal Sunyaev-Zeldovich effect and cosmic shear
• An alternative method to generate pre-initial conditions for cosmological $N$-body simulations
• Assessing Consistency Between WMAP 9-year and Planck 2015 Temperature Power Spectra
• A Comparison of Maps and Power Spectra Determined from South Pole Telescope and Planck Data
• The median density of the Universe
• High-redshift quasars and their host galaxies II: multiphase gas and stellar kinematics
• Globular Clusters in High-Redshift Dwarf Galaxies: A Case Study from the Local Group
• Small-scale structure from neutron dark decay
• Core mass -- halo mass relation of bosonic and fermionic dark matter halos harbouring a supermassive black hole
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. I. Construction and analysis of the mock data cubes
• Heavy stable charged tracks as signatures of non-thermal dark matter at the LHC : a study in some non-supersymmetric scenarios
• Limits on quantum gravity effects from Swift short gamma-ray bursts
• Lensing convergence in galaxy clustering in LambdaCDM and beyond
• Hybrid Higgs Inflation: The Use of Disformal Transformation
• The Mean Absorption Line Spectra of a Selection of Luminous z~6 Lyman Break Galaxies
• Chiral Dark Sector
• Features in the Spectrum of Cosmic-Ray Positrons from Pulsars
• Detecting the stochastic gravitational wave background with the TianQin detector
• Energy function, formation rate and low-metallicity environment of fast radio bursts
• Measuring the delay time distribution of binary neutron stars. I. Through Scaling Relations of the Host Galaxies of Gravitational Wave Events
• Evolution of Neutral Oxygen During the Epoch of Reionization and its Use in Estimating the Neutral Hydrogen Fraction
• Galaxy-galaxy weak gravitational lensing in $f(R)$ gravity
• Starburst and post-starburst high-redshift protogalaxies: The feedback impact of high energy cosmic rays
• The short gamma-ray burst population in a quasi-universal jet scenario
• Viewing angle constraints on S190425z and S190426c and the joint gravitational-wave/gamma-ray detection fractions for binary neutron star mergers
• Self-heating of Strongly Interacting Massive Particles
• CMB constraints on a physical model of reionization
• Isocurvature bounds on axion-like particle dark matter in the post-inflationary scenario
• Signature of Inverse Compton emission from blazars
• zBEAMS: A unified solution for supernova cosmology with redshift uncertainties
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• The phenomenology of beyond Horndeski gravity
• The triply-ionized carbon forest from eBOSS: cosmological correlations with quasars in SDSS-IV DR14
• The HI intensity mapping bispectrum including observational effects
• Constraints on cosmic curvature with lensing time delays and gravitational waves
• Icecube/DeepCore tests for novel explanations of the MiniBooNE anomaly
• Tidal effects of dark matter halo around a galactic black hole
• Comparison of cosmological simulations and deep submillimetre galaxy surveys
• Cosmological backreaction within the Szekeres model and emergence of spatial curvature
• Seeding the second star -- II. CEMP star formation enriched from faint supernovae
• Exploring the Milky Way Circumgalactic Medium in a Cosmological Context with a Semi-Analytic Model
• Gravitational waves and large field inflation
• Explaining the 3.5 keV X-ray Line in a $L_{\mu }-L_{\tau }$ Extension of the Inert Doublet Model
• The variance of the locally measured Hubble parameter explained with different estimators
• Rapid search for massive black hole binary coalescences using deep learning
• Projected constraints on the dispersion of gravitational waves using advanced ground- and space-based interferometers
• Electron-Positron Annihilation Freeze-Out in the Early Universe
• Gravitational leptogenesis in Natural Inflation
• Theoretical study of the direct $\alpha +d$ $\to$ ${}^6$Li + $\gamma$ astrophysical capture process in a three-body model II. Reaction rates and primordial abundance
• Predictions for the Abundance of High-redshift Galaxies in a Fuzzy Dark Matter Universe
• Detection of thermal Sunyaev-Zel'dovich Effect in the circumgalactic medium of low-mass galaxies -- a surprising pattern in self-similarity and baryon sufficiency
• Gravitational lensing by wave dark matter halos
• Power spectrum multipole expansion for HI intensity mapping experiments: unbiased parameter estimation
• Does the second law hold at cosmic scales?
• An Altarelli Cocktail for the MiniBooNE Anomaly?
• The Ubiquitous Imprint of Radiative Acceleration in the Mean Absorption Spectrum of Quasar Outflows
• On the capture rates of big bang neutrinos by nuclei within the Dirac and Majorana hypotheses
• Friedmann cosmology with decaying vacuum density in Brans-Dicke theory
• The first constraint from SDSS galaxy-galaxy weak lensing measurements on interacting dark energy models
• Life cycle of cosmic-ray electrons in the intracluster medium
• Scale-invariant inflation with one-loop quantum corrections
• Multi-resolution Bayesian CMB component separation through Wiener-filtering with a pseudo-inverse preconditioner
• Cold gas in the early Universe. Survey for neutral atomic-carbon in GRB host galaxies at 1 < z < 6 from optical afterglow spectroscopy
• Scrutinizing Various Phenomenological Interactions In The Context Of Holographic Ricci Dark Energy Models
• Projected sensitivity to sub-GeV dark matter of next-generation semiconductor detectors
• The interplay between feedback, accretion, transport and winds in setting gas-phase metal distribution in galaxies
• Molecular Chemistry for Dark Matter II: Recombination, Molecule Formation, and Halo Mass Function in Atomic Dark Matter
• Cosmological Tests of Everpresent $\Lambda$
• Galaxy Formation in Sterile Neutrino Dark Matter Models
• LIMFAST. II. Line Intensity Mapping as a Probe of High-Redshift Galaxy Formation
• Low-Scale D-term Inflation and the Relaxion
• Detection of Cosmic Structures using the Bispectrum Phase. II. First Results from Application to Cosmic Reionization Using the Hydrogen Epoch of Reionization Array
• Explicit Bayesian treatment of unknown foreground contaminations in galaxy surveys
• Cosmological dynamics of brane gravity: A global dynamical system perspective
• Impact of gas spin and Lyman-Werner flux on black hole seed formation in cosmological simulations: implications for direct collapse
• S2COSMOS: Evolution of Gas Mass with Redshift Using Dust Emission
• Double peaks of gravitational wave spectrum induced from inflection point inflation
• Studying the morphology of reionisation with the triangle correlation function of phases
• Predicting the Neutral Hydrogen Content of Galaxies From Optical Data Using Machine Learning
• Constraining interacting dark energy models with the halo concentration-mass relation
• Do cosmological data rule out $f(\mathcal{R})$ with $w\ne -1$?
• $\bar{T}$: A New Cosmological Parameter?
• Strong gravitational lensing in $f\left(\chi \right)={\chi }^{3/2}$ gravity
• Dynamical stability in models where dark matter and dark energy are non-minimally coupled to curvature
• Molecular gas in two companion cluster galaxies at z=1.2
• Quenching in Cosmic Sheets: Tracing the Impact of Large Scale Structure Collapse on the Evolution of Dwarf Galaxies
• Galaxy clusters and a possible variation of the fine structure constant
• Neutrino mass ordering and μ-τreflection symmetry breaking
• Constraints on the star formation histories of galaxies in the Local Cosmological Volume
• Measuring the duration of inflation with the curvaton
• An Atlas of Gas Motions in the TNG-Cluster Simulation: from Cluster Cores to the Outskirts
• Constraints on Cosmology and Baryonic Feedback with the Deep Lens Survey Using Galaxy-Galaxy and Galaxy-Mass Power Spectra
• Probing Cosmology and Cluster Astrophysics with Multi-Wavelength Surveys I. Correlation Statistics
• Implication of the Shape of the EDGES Signal for the 21 cm Power Spectrum
• Quantifying the Redshift Space Distortion of the Bispectrum II: Induced Non-Gaussianity at Second Order Perturbation
• Redshift evolution of the dark matter haloes shapes
• The HERA-19 Commissioning Array: Direction Dependent Effects
• New parametrization of the dark-energy equation of state with a single parameter
• The radio spectral turnover of radio-loud quasars at $z>5$
• New cosmological constraints with extended-Baryon Oscillation Spectroscopic Survey DR14 quasar sample
• Sub-structure and merger detection in resolved NIKA Sunyaev-Zel'dovich images of distant clusters
• A Model of Metastable EeV Dark Matter
• SCORCH. II. Radiation-Hydrodynamic simulations of reionization with varying radiation escape fractions
• Hot and counter-rotating star-forming disk galaxies in IllustrisTNG and their real-world counterparts
• Late-time cosmological evolution of a general class of f(R, T) gravity with minimal curvature-matter coupling
• Cosmological constrains on minimally and non-minimally coupled scalar field models
• The Effect of a Light Sterile Neutrino at NO$\nu$A and DUNE
• Running vacuum in Brans-Dicke theory: a possible cure for the ${\sigma }_8$ and $H_0$ tensions
• The bias of dark matter tracers: assessing the accuracy of mapping techniques
• Constraining the cross-section of dark matter with giant radial arcs in galaxy clusters
• Asteroseismic Inference of Subgiant Evolutionary Parameters with Deep Learning
• Constraints on neutrino mass in the scenario of vacuum energy interacting with cold dark matter after Planck 2018
• Binary black hole mergers from merged stars in the Galactic field
• Constraints on the dark photon from deep inelastic scattering
• In pursuit of giants: II. Evolution of dusty quiescent galaxies over the last six billion years from the hCOSMOS survey
• Detecting strongly lensed supernovae at z ~ 5-7 with LSST
• Cosmological Constraints from Galaxy Cluster Sparsity, Cluster Gas Mass Fraction and Baryon Acoustic Oscillations Data
• Constraining Sterile Neutrino Cosmology with Terrestrial Oscillation Experiments
• Chandra and Magellan/FIRE follow-up observations of PSO167-13: an X-ray weak QSO at $z=6.515$
• Probing the intergalactic turbulence with fast radio bursts
• Probing the innermost regions of AGN jets and their magnetic fields with RadioAstron. III. Blazar S5 0716+71 at microarcsecond resolution
• Green Peas in X-rays
• Anisotropic solid dark energy
• CMB constraints on dark matter phenomenology via reheating in minimal plateau inflation
• Cosmological lensing ratios with DES Y1, SPT and Planck
• Left-right model with TeV fermionic dark matter and unification
• The low-luminosity type II SN\,2016aqf: A well-monitored spectral evolution of the Ni/Fe abundance ratio
• Constraining holographic cosmology using Planck data
• Bounce and cyclic cosmology in weakly broken galileon theories
• Tsallis holographic model of dark energy: Cosmic behaviour, statefinder analysis and ${\omega }_D-{\omega }_D^{\prime }$ pair in the non-flat universe
• Forecasted constraints on modified gravity from Sunyaev Zel'dovich tomography
• Wiener filter reloaded: fast signal reconstruction without preconditioning
• Anisotropic Dark Matter Stars
• A hierarchical field-level inference approach to reconstruction from sparse Lyman-$\alpha$ forest data
• Properties of brightest group galaxies in cosmic web filaments
• Impact of cosmological and astrophysical constraints on dark matter simplified models
• Non-parametric reconstruction of dark energy and cosmic expansion from the Pantheon compilation of type Ia supernovae
• Fierz-Pauli theory reloaded: from a theory of a symmetric tensor field to linearized massive gravity
• New probe of gravity: strongly lensed gravitational wave multi-messenger approach
• Radio constraints on dark matter annihilation in Canes Venatici I with LOFAR
• Constraints on shear and rotation with massive galaxy clusters
• On the cosmology of scalar-tensor-vector gravity theory
• ALMA view of RX J1131-1231: Sub-kpc CO (2-1) mapping of a molecular disk in a lensed star-forming quasar host galaxy
• Reconstruction of interaction rate in Holographic dark energy
• Constraining f(R) Gravity with Planck Sunyaev-Zel'dovich Clusters
• A disturbing FABLE of mergers, feedback, turbulence, and mass biases in simulated galaxy clusters
• Cosmological constraints and phenomenology of a beyond-Horndeski model
• A non-parametric consistency test of the $\Lambda$CDM model with Planck CMB data
• The paradigm of warm quintessential inflation and spontaneous baryogenesis
• The Astrophysical Consequences of Intervening Galaxy Gas on Fast Radio Bursts
• Ergosphere, photon region structure, and the shadow of a rotating charged Weyl black hole
• Warm dark matter constraints from high-$z$ Direct Collapse Black Holes using the JWST
• The black hole and host galaxy growth in an isolated $z\sim 6$ QSO observed with ALMA
• Kinematic Constraints on Spatial Curvature from Supernovae Ia and Cosmic Chronometers
• Observational signatures of the parametric amplification of gravitational waves during reheating after inflation
• Identification of Basins of Attraction in the Local Universe
• Extended family of generalized Chaplygin gas models
• Dust in the first galaxies
• From $R^2$ Gravity to No-Scale Supergravity
• Cosmological forecasts for future galaxy surveys with the linear point standard ruler: Toward consistent BAO analyses far from a fiducial cosmology
• Constraints on MeV dark matter using neutrino detectors and their implication for the 21-cm results
• Neutron Star in Covariant $f(Q)$ gravity
• A dark matter model that reconciles tensions between the cosmic-ray $e^{\pm }$ excess and the gamma-ray and CMB constraints
• The Impact of Line Misidentification on Cosmological Constraints from Euclid and other Spectroscopic Galaxy Surveys
• keV Neutrino Dark Matter in a Fast Expanding Universe
• Complementarity for Dark Sector Bound States
• TARDIS Paper II: Synergistic Density Reconstruction from Lyman-alpha Forest and Spectroscopic Galaxy Surveys with Applications to Protoclusters and the Cosmic Web
• Does Planck 2015 polarization favor high redshift reionization?
• LIMFAST. I. A Semi-Numerical Tool for Line Intensity Mapping
• The Dark Sequential Z' Portal: Collider and Direct Detection Experiments
• Probing large-scale magnetism with the Cosmic Microwave Background
• Unbiased Cosmological Parameter Estimation from Emission Line Surveys with Interlopers
• Emergent gravity in galaxies and in the Solar System
• GUT Models at Current and Future Hadron Colliders and Implications to Dark Matter Searches
• Cogenesis of LIGO Primordial Black Holes and Dark Matter
• Effects of Self-Calibration of Intrinsic Alignment on Cosmological Parameter Constraints from Future Cosmic Shear Surveys
• Fibre Inflation and Reheating
• Dark neutrino interactions make gravitational waves blue
• Can decaying particle explain cosmic infrared background excess?
• Primordial non-Gaussianity and non-Gaussian Covariance
• Search for binary black hole mergers in the third observing run of Advanced LIGO-Virgo using coherent WaveBurst enhanced with machine learning
• Inferring galaxy dark halo properties from visible matter with Machine Learning
• The effect of the environment-dependent stellar initial mass function on the photometric properties of star-forming galaxies
• Probing Modified Gravity with Integrated Sachs-Wolfe CMB and Galaxy Cross-correlations
• Lyα emitters in a cosmological volume I: the impact of radiative transfer
• Cosmological test on viscous bulk models using Hubble Parameter measurements and type Ia Supernovae data
• Asteroseismic modelling of the subgiant μ Herculis using SONG data: lifting the degeneracy between age and model input parameters
• K-mouflage Imprints on Cosmological Observables and Data Constraints
• SKA Science Data Challenge 2: analysis and results
• Investigating Dark Energy Equation of State With High Redshift Hubble Diagram
• The ILC as a natural SUSY discovery machine and precision microscope: from light higgsinos to tests of unification
• The Clustering of X-ray Luminous Quasars
• Dynamical systems analysis of phantom models
• WALLABY Early Science - I. The NGC 7162 Galaxy Group
• Dark-ages Reionization and Galaxy Formation Simulation -- XVII. Sizes, angular momenta and morphologies of high redshift galaxies
• A search for the afterglows, kilonovae, and host galaxies of two short GRBs: GRB 211106A and GRB 211227A
• The Assembly of Black Hole Mass and Luminosity Functions of High-redshift Quasars via Multiple Accretion Episodes
• The BINGO Project V: Further steps in Component Separation and Bispectrum Analysis
• Figuring Out Gas & Galaxies In Enzo (FOGGIE) V: The Virial Temperature Does Not Describe Gas in a Virialized Galaxy Halo
• Measuring the integrated Sachs-Wolfe effect from the low-density regions of the universe
• CLEAR: Boosted Ly$\alpha$ Transmission of the Intergalactic Medium in UV bright Galaxies
• Testing cosmic acceleration for $w(z)$ parameterizations using $f_{gas}$ measurements in galaxy clusters
• Doubly-charged Higgs Boson at Future Electron-Proton Collider
• Hořava-Lifshitz cosmology in light of new data
• Light neutrino masses from a non-Hermitian Yukawa theory
• Fermion Dark Matter with Scalar Triplet at Direct and Collider Searches
• Beyond Ultra-diffuse Galaxies. I. Mass--Size Outliers among the Satellites of Milky Way Analogs
• The case for a Casimir cosmology
• Into the Lyα jungle: exploring the circumgalactic medium of galaxies at z ~ 4-5 with MUSE
• A fast radio burst with a low dispersion measure
• The Peebles -- Vilenkin quintessential inflation model revisited
• On Model Selection in Cosmology
• Stability of the Closed Einstein Universe in Energy-Momentum Squared Gravity
• Observational Constraints in Nonlocal Gravity: the Deser-Woodard Case
• Cosmological Vlasov-Poisson Simulations of Structure Formation with Relic Neutrinos: Nonlinear Clustering and the Neutrino Mass
• Consistent and simultaneous modelling of galaxy clustering and galaxy-galaxy lensing with Subhalo Abundance Matching
• The OTELO survey. I. Description, data reduction, and multi-wavelength catalogue
• Characterizing the local gamma-ray Universe via angular cross-correlations
• One loop graviton corrections to dynamical photons in de Sitter
• From rest-frame luminosity functions to observer-frame colour distributions: tackling the next challenge in cosmological simulations
• RAiSE: simulation-based analytical model of AGN jets and lobes
• Testing Super-Eddington Accretion onto a Supermassive Black Hole: Reverberation Mapping of PG 1119+120
• A solution of the dark energy and its coincidence problem based on local antigravity sources without fine-tuning or new scales
• Constraining the intrinsic population of Long Gamma-Ray Bursts: implications for spectral correlations, cosmic evolution and their use as tracers of star formation
• Tidal disruption events can power the observed AGN in dwarf galaxies
• Impact of baryons in cosmic shear analyses with tomographic aperture mass statistics
• Optimal constraints on primordial gravitational waves from the lensed CMB
• Prior dependence of cosmological constraints on dark matter-radiation interactions
• The correlation between isotropic energy and duration of gamma-ray bursts
• Prospects for indirect MeV Dark Matter detection with Gamma Rays in light of Cosmic Microwave Background Constraints
• {\it Gauging} the cosmic acceleration with recent type Ia supernovae data sets
• Estimation of starting times of quasinormal modes in ringdown gravitational waves with the Hilbert-Huang transform
• Gravitino/Axino as Decaying Dark Matter and Cosmological Tensions
• Axion-like particle assisted strongly interacting massive particle
• Density spikes near black holes in self-interacting dark matter halos and indirect detection constraints
• The Three Hundred project: Galaxy groups do not survive cluster infall
• Holographic approach for dark energy - dark matter interaction in curved FLRW spacetime
• Anomalies in $B$ Decays and Muon $g-2$ from Dark Loops
• The chemical connection between damped Lyman-α systems and Local Group dwarf galaxies
• Clustering dark energy imprints on cosmological observables of the gravitational field
• Search for long-lived particles decaying into muon pairs in proton-proton collisions at $\sqrt{s}=$ 13 TeV collected with a dedicated high-rate data stream
• Probing dynamics of dark energy with latest observations
• Imprints of interacting dark energy on cosmological perturbations
• Quantum behavior of the "Little Sibling" of the Big Rip induced by a three-form field
• The density-bounded twilight of starbursts in the early Universe
• Energy-Momentum portal to dark matter and emergent gravity
• Multi-component Dark Matter in a Simplified E${}_6$SSM Model
• Hamiltonian Monte Carlo reconstruction from peculiar velocities
• Enhanced star formation in $z\sim 6$ quasar companions
• A Search for Optical Emission from Binary-Black-Hole Merger GW170814 with the Dark Energy Camera
• Parametrizing theories of gravity on large and small scales in cosmology
• Testing one-loop galaxy bias: cosmological constraints from the power spectrum
• Black hole formation in the context of dissipative dark matter
• Dark-photon searches via $ZH$ production at $e^{+}{e}^{-}$ colliders
• PNG-UNITsims: Halo clustering response to primordial non-Gaussianities as a function of mass
• Primordial features from ekpyrotic bounces
• SILVERRUSH. IX. Lya Intensity Mapping with Star-Forming Galaxies at z=5.7 and 6.6: A Possible Detection of Extended Lya Emission at $\gtrsim$100 comoving kpc around and beyond the Virial-Radius Scale of Galaxy Dark Matter Halos
• Fermion Proca Stars: Vector Dark Matter Admixed Neutron Stars
• An Optimal Estimator of Intrinsic Alignments for Star-forming Galaxies in IllustrisTNG Simulation
• An updated estimate of the cosmic radio background and implications for ultra-high-energy photon propagation
• Differences and similarities of stellar populations in LAEs and LBGs at $z\sim$ 3.4 - 6.8
• Dynamical instability of polytropic spheres in spacetimes with a cosmological constant
• Planck Satellite Constraints on Pseudo-Nambu--Goldstone Boson Quintessence
• Can intrinsic alignments of elongated low-mass galaxies be used to map the cosmic web at high redshift?
• Theoretical tidal evolution constants for stellar models from the pre-main sequence to the white dwarf stage Apsidal motion constants, moment of inertia, and gravitational potential energy
• General Modified Gravity With 21cm Intensity Mapping: Simulations and Forecast
• Impact of the 3D source geometry on time-delay measurements of lensed type-Ia Supernovae
• Multicomponent multiscatter capture of Dark Matter
• Constraints on Primordial non-Gaussianity from Future HI Intensity Mapping Experiments
• A black box for dark sector physics: Predicting dark matter annihilation feedback with conditional GANs
• Momentum distributions of cosmic relics: Improved analysis
• The Extremely Luminous Quasar Survey (ELQS) in the Sloan Digital Sky Survey footprint. II. The North Galactic Cap Sample
• Theoretical priors in scalar-tensor cosmologies: Thawing quintessence
• Spatial Curvature in $f(R)$ Gravity
• The interconnection between galaxy mergers, AGN activity and rapid quenching of star formation in simulated post-merger galaxies
• Axion Isocurvature Perturbations in Low-Scale Models of Hybrid Inflation
• Galaxy Evolution at High Redshift: Obscured Star Formation, GRB Rates, Cosmic Reionization, and Missing Satellites
• Are Faint Supernovae Responsible for Carbon-Enhanced Metal-Poor Stars?
• A spatially resolved analysis of star-formation burstiness by comparing UV and H$\alpha$ in galaxies at z$\sim$1 with UVCANDELS
• A blast from the infant Universe: the very high-z GRB 210905A
• A model-independent characterisation of strong gravitational lensing by observables
• Starobinsky Inflation: From Non-SUSY To SUGRA Realizations
• A unified framework for 21cm tomography sample generation and parameter inference with Progressively Growing GANs
• Detection of a gamma-ray flare from the high-redshift blazar DA 193
• Tensor perturbations during inflation in a spatially closed Universe
• Secondary neutrino and gamma-ray fluxes from SimProp and CRPropa
• Long gamma-ray burst rate at very high redshift
• The Impact of Beam Variations on Power Spectrum Estimation for 21-cm Cosmology I: Simulations of Foreground Contamination for HERA
• Extended $\Lambda$CDM model
• The scale of cosmic homogeneity as a standard ruler
• Simple single-field inflation models with arbitrarily small tensor/scalar ratio
• Big Bang Nucleosynthesis Constraint on Baryonic Isocurvature Perturbations
• Evidence for a Young Stellar Population in Nearby Type 1 Active Galaxies
• COWS: A filament finder for Hessian cosmic web identifiers
• Studying the Physical Properties of Tidal Features I. Extracting Morphological Substructure in CANDELS Observations and VELA Simulations
• The Formation History of Subhalos and the Evolution of Satellite Galaxies
• New Shapes of Primordial Non-Gaussianity from Quasi-Single Field Inflation with Multiple Isocurvatons
• Generalised model-independent characterisation of strong gravitational lenses VI: the origin of the formalism intrinsic degeneracies and their influence on $H_0$
• Gravitational wave fossils in nonlinear regime: halo tidal bias and intrinsic alignments from gravitational wave separate universe simulations
• Derivation of the physical parameters of the jet in S5 0836+710 from stability analysis
• A high baryon fraction in massive haloes at z~3
• Final results on neutrino oscillation parameters from the OPERA experiment in the CNGS beam
• Precision calculations of dark matter relic abundance
• Cosmic Near-infrared Background Tomography with SPHEREx Using Galaxy Cross-correlations
• An Improved Statistical Point-Source Foreground Model for the Epoch of Reionization
• Radio spectral index from NVSS and TGSS
• Jet kinematics in the transversely stratified jet of 3C 84 A two-decade overview
• Nuclear absorption and emission in the AGN merger NGC 6240: the hard X-ray view
• Non-Gaussianity of secondary anisotropies from ACTPol and Planck
• Improving Fisher matrix forecasts for galaxy surveys: window function, bin cross-correlation, and bin redshift uncertainty
• The $\alpha +d\to {}^6\mathrm{Li}+\gamma$ astrophysical $S$-factor and its implications for Big Bang Nucleosynthesis
• Probing Population III Initial Mass Functions with He II/H$\alpha$ Intensity Mapping
• Impact of LHC data on muon $g-2$ solutions in vector-like extension of the Constrained MSSM
• Gravitationally influenced particle creation models and late-time cosmic acceleration
• First Weak-lensing Results from "See Change": Quantifying Dark Matter in the Two Z>1.5 High-redshift Galaxy Clusters SPT-CL J2040-4451 and IDCS J1426+3508
• Vacuum dynamics in the Universe versus a rigid $\Lambda =$const
• Wormhole solutions with a complex ghost scalar field and their instability
• Modifications to Cosmological Power Spectra from Scalar-Tensor Entanglement and their Observational Consequences
• Testing the Cosmological Principle in the radio sky
• Indirect Detection of Composite (Asymmetric) Dark Matter
• On the degeneracy between baryon feedback and massive neutrinos as probed by matter clustering and weak lensing
• Optimal filtering for CMB lensing reconstruction
• Tau flavored dark matter and its impact on tau Yukawa coupling
• First Detection of Cosmic Microwave Background Lensing and Lyman-α Forest Bispectrum
• SUSY-QCD corrections for the direct detection of neutralino dark matter and correlations with the relic density
• Molecular Chemistry for Dark Matter III: DarkKROME
• Heavy Bino Dark Matter and Collider Signals in the MSSM with Vector-like 4th-Generation Particles
• Leptogenesis in the Neutrino Option
• Radio Spectra of Luminous, Heavily Obscured WISE-NVSS Selected Quasars
• Interactions between Ultra-High-Energy Particles and Protogalactic Environments
• Constraining the interaction between dark sectors with future HI intensity mapping observations
• Multi-Scale Pipeline for the Search of String-Induced CMB Anisotropies
• Spectroscopic confirmation and velocity dispersions for twenty Planck galaxy clusters at 0.16<z<0.78
• Common Origin of Non-zero ${\theta }_{13}$ and Baryon Asymmetry of the Universe in a TeV scale Seesaw Model with $A_4$ Flavour Symmetry
• Axion dark matter in a $3-3-1$ model
• Constraints on Patchy Reionization from Planck CMB Temperature Trispectrum
• Two Candidate High-Redshift X-ray Jets Without Coincident Radio Jets
• Isochrone fitting to the open cluster M67 in the era of Gaia and improved model physics
• A tomographic test of cosmological principle using the JLA compilation of type Ia supernovae
• Bounce Models within Teleparallel modified gravity
• Evidence for non-axisymmetry in M31 from wide-field kinematics of stars and gas
• New constraints on the 1.4 GHz source number counts and luminosity functions in the Lockman Hole field
• Hot Leptogenesis from Thermal Dark Matter
• The AGN contribution to the UV-FIR luminosities of interacting galaxies and its role in identifying the Main Sequence
• The effect of dark matter-dark radiation interactions on halo abundance -- a Press-Schechter approach
• Bianchi type-I Barrow holographic dark energy model in symmetric teleparallel gravity
• The Hunt for Red Quasars: Luminous Obscured Black Hole Growth Unveiled in the Stripe 82 X-ray Survey
• Source counts at 7.7 to 21 $\mu$m in CEERS field with James Webb Space Telescope
• PRUSSIC I - a JVLA survey of HCN/HCO+/HNC (1-0) emission in z$\sim$3 dusty galaxies: Low dense-gas fractions in high-redshift star-forming galaxies
• The redshift evolution of the baryonic Tully-Fisher relation in Simba
• $f(R)$ gravity modifications: from the action to the data
• Emergence of time
• Multiple Beads-on-a-string: Dark Matter-Deficient Galaxy Formation in a Mini-bullet Satellite-satellite Galaxy Collision
• The SRG/eROSITA All-Sky Survey: Constraints on AGN Feedback in Galaxy Groups
• Enhancing cosmic shear with the multi-scale lensing PDF
• The UV luminosity functions of Bright z>8 Galaxies: Determination from ~0.41 deg2 of HST Observations along ~sim 300 independent sightlines
• Expectation of primordial gravity waves generated during inflation
• Discriminating between Thermal and Nonthermal Cosmic Relic Neutrinos through Annual Modulation at PTOLEMY
• The de Broglie-Bohm Quantum Theory and its Application to Quantum Cosmology
• The Indirect Influence of Quasars on Reionization
• Big-bang nucleosynthesis and cosmic microwave background constraints on non-minimally coupled theories of gravity
• Singlino-dominated dark matter in $Z_3$-NMSSM
• Exploring Spin-3/2 Dark Matter with Effective Higgs Couplings
• Do we Come from a Quantum Anomaly?
• Constraining gravity at large scales with the 2MASS Photometric Redshift catalogue and Planck lensing
• An insight into the extragalactic transient and variable microJy radio sky across multiple decades
• Dark Matter, Muon Anomalous Magnetic Moment and the XENON1T Excess
• Integrated Sachs-Wolfe-galaxy cross-correlation bounds on the two branches of the minimal theory of massive gravity
• Developing a unified pipeline for large-scale structure data analysis with angular power spectra -- II. A case study for magnification bias and radio continuum surveys
• Exploring extensions to the standard cosmological model and the impact of baryons on small scales
• Cross-correlating 2D and 3D galaxy surveys
• The Variable Relativistic Outflow of IRAS 13224-3809
• The Frequency of Intrinsic X-ray Weakness Among Broad Absorption Line Quasars
• Hydrodynamical structure formation in Milgromian cosmology
• Feeding the spider with carbon -- [CII] emission from the circum galactic medium and active galactic nucleus
• Ultraviolet Signatures of the Multiphase Intracluster and Circumgalactic Media in the RomulusC Simulation
• Ordering the confusion: A study of the impact of lens models on gravitational-wave lensing detection capabilities
• The Three Hundred project: A Machine Learning method to infer clusters of galaxies mass radial profiles from mock Sunyaev-Zel'dovich maps
• Modelling Baryonic Effects on Galaxy Cluster Mass Profiles
• Modelling the solar twin 18 Sco
• Effect of Template Uncertainties on the WMAP and Planck Measures of the Optical Depth Due To Reionization
• Observation of Supersymmetry and its Spontaneous Breaking in a Trapped Ion Quantum Simulator
• Ultra-light axions and the kinetic Sunyaev-Zel'dovich Effect
• Hadronic Footprint of GeV-Mass Dark Matter
• Observing Merger Trees in a New Light
• Post-inflationary axion isocurvature perturbations facing CMB and large-scale structure
• Planck-PR4 anisotropy spectra show (better) consistency with General Relativity
• SN2017egm: A Helium-rich Superluminous Supernova with Multiple Bumps in the Light Curves
• Dust in galaxy clusters: Modeling at millimeter wavelengths and impact on Planck cluster cosmology
• An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies
• Bianchi type-I Dust Filled Accelerating Brans- Dicke Cosmology
• Primordial deuterium abundance at z=2.504 towards Q1009+2956
• Searching for Signatures of Dark matter-Dark Radiation Interaction in Observations of Large-scale Structure
• Cosmology with the sub-millimetre galaxies magnification bias: Tomographic Analysis
• The light curve and distance of Kepler supernova: news from four centuries ago
• Cosmological Studies from HSC-SSP Tomographic Weak Lensing Peak Abundances
• Determining Dark Matter properties with a XENONnT/LZ signal and LHC-Run3 mono-jet searches
• Kinetic inflation in deformed phase space Brans-Dicke cosmology
• Density reconstruction from biased tracers and its application to primordial non-Gaussianity
• Late decaying 2-component dark matter scenario as an explanation of the AMS-02 positron excess
• Constraining cosmology with the cosmic microwave and infrared backgrounds correlation
• $f(R)$ quantum cosmology: avoiding the Big Rip
• Evidence of a Flat Outer Rotation Curve in a Starbursting Disk Galaxy at $z=1.6$
• On inflation, cosmological constant, and SUSY breaking
• Cosmic ray $e^{+}{e}^{-}$ spectrum excess and peak feature observed by the DAMPE experiment from dark matter
• ROGER: Reconstructing Orbits of Galaxies in Extreme Regions using machine learning techniques
• Dielectric-Boosted Sensitivity to Cylindrical Azimuthally Varying Transverse-Magnetic Resonant Modes in an Axion Haloscope
• First detection of the [OI] 63-um emission from a redshift 6 dusty galaxy
• Constraints on the merging binary neutron star mass distribution and equation of state based on the incidence of jets in the population
• Obscured Star Formation in the Host Galaxies of Superluminous Supernovae
• Mass Estimation of Galaxy Clusters with Deep Learning II: CMB Cluster Lensing
• UV regulated star formation in high-redshift galaxies
• Signal Response Model in PandaX-4T
• SAGAN -- III: New insights into giant radio quasars
• Antimatter as Macroscopic Dark Matter
• Lepton portal dark matter at muon colliders: Total rates and generic features for phenomenologically viable scenarios
• Analysis of big bounce in Einstein--Cartan cosmology
• Multicomponent Dark Matter in Radiative Seesaw Models
• 21 cm Angular Power Spectrum from Minihalos as a Probe of Primordial Spectral Runnings
• A tale of seven narrow spikes and a long trough: constraining the timing of the percolation of HII bubbles at the tail-end of reionization with ULAS J1120+0641
• Constraining the reionization and thermal history of the Universe using a semi-numerical photon-conserving code SCRIPT
• Current status and future prospects of the singlet-doublet dark matter model with $CP$ violation
• The First Gamma-ray Emitting BL Lacertae Object at the Cosmic Dawn
• Cosmological acceleration
• The Three Hundred Project: The gas disruption of infalling objects in cluster environments
• The miniJPAS survey: AGN & host galaxy co-evolution of X-ray selected sources
• Evidence for Reduced Specific Star Formation Rates in the Centers of Massive Galaxies at z = 4
• The cosmological behaviour and the statefinder diagnosis for the New Tsallis agegraphic dark energy
• IDECAMB: an implementation of interacting dark energy cosmology in CAMB
• Universe opacity and Type Ia supernova dimming
• Scotogenic dark matter and single-zero textures of the neutrino mass matrix
• LEKID sensitivity for space applications between 80 and 600 GHz
• Exact and slow-roll solutions for exponential power-law inflation connected with f(R) gravity and observational constraints
• Strong lensing modeling in galaxy clusters as a promising method to test cosmography I. Parametric dark energy models
• The Bimodal Absorption System Imaging Campaign (BASIC) I. A Dual Population of Low-metallicity Absorbers at z $<1$
• A Southern sky search for repeating Fast Radio Bursts using the Australian SKA Pathfinder
• Bayesian correction of $H(z)$ data uncertainties
• Average fractional polarization of extragalactic sources at Planck frequencies
• Growth of Matter Perturbations in the Bi-Galileons Field Model
• C${}^3$-Cluster Clustering Cosmology II. First detection of the BAO peak in the three-point correlation function of galaxy clusters
• Revised bounds on local cosmic strings from NANOGrav observations
• Quadratic shape biases in three-dimensional halo intrinsic alignments
• Ultra-compact structure in radio quasars as a cosmological probe: a revised study of the interaction between cosmic dark sectors
• Multiwavelength cluster mass estimates and machine learning
• HOD-Dependent Systematics in Emission Line Galaxies for the DESI 2024 BAO analysis
• Hydrodynamic Shielding and the Survival of Cold Streams
• Probing spatial variation of the fine-structure constant using the CMB
• Light weakly interacting massive particles
• Unequal time correlators and the Zeldovich approximation
• Testing a quintessence model with Yukawa interaction from cosmological observations and N-body simulations
• Observational constraints on the generalized $\alpha$ attractor model
• Estimating the Milky Way's Mass via Hierarchical Bayes: A Blind Test on MUGS2 Simulated Galaxies
• Predictivity of Neutrino Mass Sum Rules
• Dynamical Dark Matter from Thermal Freeze-Out
• Multi-wavelength scaling relations in galaxy groups: a detailed comparison of GAMA and KiDS observations to BAHAMAS simulations
• Backreaction and FRW consistency conditions
• A multi-temperature universe can allow a sub-MeV dark photon dark matter
• Inflation as an amplifier: the case of Lorentz violation
• Nucleon - Light Dark Matter Annihilation through Baryon Number Violation
• Probing Intra-Halo Light with Galaxy Stacking in CIBER Images
• Perspectives of direct Detection of supersymmetric Dark Matter in the NMSSM
• An Improved Diffuse Foreground Subtraction by ILC method: CMB Map and Angular Power Spectrum using Planck and WMAP Observations
• Perturbation theory for the redshift-space matter power spectra after reconstruction
• Second-order Cosmological Perturbations Engendered by Point-like Masses
• The SAMI Galaxy Survey: Using Tidal Streams and Shells to Trace the Dynamical Evolution of Massive Galaxies
• Thermal Sunyaev-Zel'dovich effect in the intergalactic medium with primordial magnetic fields
• Mergers of supermassive and intermediate-mass black holes in galactic nuclei from disruptions of star clusters
• Testing parity-violating physics from cosmic rotation power reconstruction
• Account of the baryonic feedback effect in gamma-ray measurements of intergalactic magnetic fields
• Constraining Dark-Matter Ensembles with Supernova Data
• Radion induced inflation on non-flat brane and modulus stabilization
• Weak lensing distortions beyond shear
• Field Theories and Fluids for an Interacting Dark Sector
• Double charged heavy constituents of dark atoms and superheavy nuclear objects
• ETHOS - an effective theory of structure formation: formation of the first haloes and their stars
• MINOT: Modeling the intracluster medium (non-)thermal content and observable prediction tools
• Constraining dark matter annihilation with cosmic ray antiprotons using neural networks
• Joint Observations of Space-based Gravitational-wave Detectors: Source Localization and Implication for Parity-violating gravity
• Interacting Tsallis holographic dark energy: Cosmic behaviour, statefinder analysis and ${\omega }_D-{\omega }_D^{\prime }$ pair in the non-flat universe
• Multi-Dimensional Effective Field Theory Analysis for Direct Detection of Dark Matter
• Study of warm inflationary models and their parameter estimation from CMB
• Integrated Cosmological Probes: Extended Analysis
• Precise probing of the inert Higgs-doublet model at the LHC
• Matter Power Spectra in Viable $f(R)$ Gravity Models with Dynamical Background
• Mass Modeling of Frontier Fields Cluster MACS J1149.5+2223 Using Strong and Weak Lensing
• Geometric Baryogenesis from Shift Symmetry
• The dominant origin of diffuse Ly$\alpha$ halos around LAEs explored by SED fitting and clustering analysis
• TRINITY II: The Luminosity-dependent Bias of the Supermassive Black Hole Mass--Galaxy Mass Relation for Bright Quasars at $z=6$
• What to expect from dynamical modelling of cluster haloes I. The information content of different dynamical tracers
• Calibration of gamma-ray bursts luminosity correlations using gravitational waves as standard sirens
• Bayesian Model Selection with Future 21cm Observations of The Epoch of Reionisation
• Asymmetric Dark Matter and Baryogenesis from Pseudoscalar Inflation
• Cosmological constraints on the gas depletion factor in galaxy clusters
• Characterising Tidal Features Around Galaxies in Cosmological Simulations
• The simplest parametrization of equation of state parameter in the scalar field Universe
• How do Primordial Black Holes change the Halo Mass Function and Structure?
• UV completion of the Starobinsky model, tensor-to-scalar ratio, and constraints on non-locality
• Interference effects of two scalar boson propagators on the LHC search for the singlet fermion DM
• The Triangulum Extended (TREX) Survey: The Stellar Disk Dynamics of M33 as a Function of Stellar Age
• Toward a direct measurement of the cosmic acceleration: roadmap and forecast on FAST
• Tracing stars in Milky Way satellites with A-SLOTH
• The Alcock-Paczyński effect from Lyman-$\alpha$ forest correlations: Analysis validation with synthetic data
• Multi-Epoch Machine Learning 1: Unravelling Nature vs Nurture for Galaxy Formation
• Probing Majorana Neutrino Textures at DUNE
• Anisotropies of Cosmic Optical and Near-IR Background from China Space Station Telescope (CSST)
• Redshift space distortions of the {\rm HI} 21-cm intensity mapping signal due to the internal motions within galaxies
• Constraints on self-interacting Bose-Einstein condensate dark matter using large-scale observables
• Probing cosmology and gastrophysics with fast radio bursts: Cross-correlations of dark matter haloes and cosmic dispersion measures
• New scaling solutions in cubic Horndeski theories
• CP Symmetries as Guiding Posts: revamping tri-bi-maximal Mixing. Part II
• Connecting radio emission to AGN wind properties with Broad Absorption Line Quasars
• Redshift remapping and cosmic acceleration in dark-matter-dominated cosmological models
• The Massive and Distant Clusters of WISE Survey VII: The Environments and Properties of Radio Galaxies in Clusters at z~1
• Simulated metal and HI absorption lines at the conclusion of Reionization
• Reevaluation of the cosmic antideuteron flux from cosmic-ray interactions and from exotic sources
• Anapole dark matter annihilation into photons
• Dark matter halos in the multicomponent model. I. Substructure
• Inflation models in the light of self-interacting sterile neutrinos
• The Three Hundred project: connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
• Exact Inflation in Einstein-Gauss-Bonnet Gravity
• Modelling Non-Linear Effects of Dark Energy
• Accounting for object detection bias in weak gravitational lensing studies
• Foreground effect on the $J$-factor estimation of classical dwarf spheroidal galaxies
• Easily Interpretable Bulk Flows: Continuing Tension with the Standard Cosmological Model
• Beyond $\Lambda$CDM with HI intensity mapping: robustness of cosmological constraints in the presence of astrophysics
• Non-Universal Stellar Initial Mass Functions: Large Uncertainties in Star Formation Rates at $z\approx 2-4$ and Other Astrophysical Probes
• Primordial Black Holes from Affleck-Dine Mechanism
• Impact of magnetic fields on Population III star formation
• Unified Scenario for Composite Right-Handed Neutrinos and Dark Matter
• Late time sky as a probe of steps and oscillations in primordial Universe
• No evidence for dynamical dark energy in two models
• Gravitational waves from fermion production during axion inflation
• Probing dark matter signals in neutrino telescopes through angular power spectrum
• Wiener filtering and pure E/B decomposition of CMB maps with anisotropic correlated noise
• Dense-gas tracers and carbon isotopes in five 2.5<z<4 lensed dusty star forming galaxies from the SPT SMG sample
• Vector stability in quadratic metric-affine theories
• Spherical collapse model in agegraphic dark energy cosmologies
• Surveying the SO(10) Model Landscape: The Left-Right Symmetric Case
• Clustering Constraints on the Relative Sizes of Central and Satellite Galaxies
• Fast radio bursts and the stochastic lifetime of black holes in quantum gravity
• The KMOS Cluster Survey (KCS) III: fundamental plane of cluster galaxies at $z\simeq 1.80$ in JKCS 041
• Power spectra in warm G-inflation and its consistency: stochastic approach
• Probing GeV-scale MSSM neutralino dark matter in collider and direct detection experiments
• Studying the late evolution of a radio-loud AGN in a galaxy group with LOFAR
• Efficient adiabatic hydrodynamical simulations of the high-redshift intergalactic medium
• VLTI/GRAVITY Interferometric Measurements of Innermost Dust Structure Sizes around AGNs
• Modelling the post-reionization neutral hydrogen ($\mathrm{HI}$) 21-cm bispectrum
• The low redshift Lyman-$\alpha$ Forest as a constraint for models of AGN feedback
• LOFAR first look at the giant radio galaxy 3C 236
• Spectacular 240 kpc double-sided relativistic jets in a spiral-hosted narrow-line Seyfert 1 galaxy
• Sensitivity of primordial black hole abundance on the reheating phase
• Testing $f(R)$ Gravity With Scale Dependent Cosmic Void Velocity Profiles
• Testing the magnetar scenario for superluminous supernovae with circular polarimetry
• Structure and stability of high-redshift galaxies in cosmological simulations
• Does jackknife scale really matter for accurate large-scale structure covariances?
• LOFAR MSSS: Discovery of a 2.56 Mpc giant radio galaxy associated with a disturbed galaxy group
• What is the amplitude of the Gravitational Waves background expected in the Starobinsky model ?
• New Scalar Field Quartessence
• Lyman continuum leakage in faint star-forming galaxies at redshift z=3-3.5 probed by gamma-ray bursts
• East Asian VLBI Network Observations of Active Galactic Nuclei Jets: Imaging with KaVA+Tianma+Nanshan
• Constraints on axionic fuzzy dark matter from light bending and Shapiro time delay
• The Flavor of Cosmology
• Gravitationally induced matter creation in scalar-tensor $f(R,T_{\mu \nu }{T}^{\mu \nu })$ gravity
• Nowhere to Hide: Radio-faint AGN in the GOODS-N field. II. Multi-wavelength AGN selection techniques and host galaxy properties
• Resonant scattering of the OVII X-ray emission line in the circumgalactic medium of TNG50 galaxies
• Primordial power spectrum and cosmology from black-box galaxy surveys
• Variation of $\alpha$ from a Dark Matter Force
• Higher order statistics of shear field: a machine learning approach
• A Distance-Deviation Consistency and Model-Independent Method to Test the Cosmic Distance-Duality Relation
• Bayesian photometric redshifts of blended sources
• The distribution of dark matter and gas spanning six megaparsecs around the post-merger galaxy cluster MS0451-03
• Exploring triplet-quadruplet fermionic dark matter at the LHC and future colliders
• Revisiting the dynamics of interacting vector-like dark energy
• SN 2010kd: Photometric and Spectroscopic Analysis of a Slow-Decaying Superluminous Supernova
• Energy Scale of Lorentz Violation in Rainbow Gravity
• The stepping-stone sampling algorithm for calculating the evidence of gravitational wave models
• Extended $\Lambda$CDM model and viscous dark energy: A Bayesian analysis
• Merging Hierarchical Triple Black Hole Systems with Intermediate-mass Black Holes in Population III Star Clusters
• The EDGES signal: An imprint from the mirror world?
• Convolutional Neural Network-reconstructed velocity for kinetic SZ detection
• Robust model comparison tests of DAMA/LIBRA annual modulation
• Sweeping Horndeski Canvas: New Growth-Rate Parameterization for Modified-Gravity Theories
• A test for skewed distributions of dark matter and a possible detection in galaxy cluster Abell 3827
• Constraints on features in the inflationary potential from future Euclid data
• The CMB lensing bi-spectrum as a probe of modified gravity theories
• A detailed study of the bridge of excess X-ray emission between the galaxy clusters Abell 2029 and Abell 2033
• Dark-ages Reionization and Galaxy Formation Simulation -- XIX: Predictions of infrared excess and cosmic star formation rate density from UV observations
• $\mu$-Hybrid Inflation with Low Reheat Temperature and Observable Gravity Waves
• Lepton Flavor Violation Induced by Dark Matter
• General dynamical properties of cosmological models with nonminimal kinetic coupling
• Barrow Holographic Dark Energy Model with GO Cut-off -- An Alternative Perspective
• Astrophysical probes of inelastic dark matter with a light mediator
• A simulation-based inference pipeline for cosmic shear with the Kilo-Degree Survey
• Characterizing Astrophysical Binary Neutron Stars with Gravitational Waves
• Relaxion window
• Instrumental systematics biases in CMB lensing reconstruction: a simulation-based assessment
• Motion of massive particles around a charged Weyl black hole and the geodetic precession of orbiting gyroscopes
• Modified Dark Matter: Relating Dark Energy, Dark Matter and Baryonic Matter
• Effects of Completeness and Purity on Cluster Dark Energy Constraints
• Calculation of the critical overdensity in the spherical-collapse approximation
• Reconciling low multipole anomalies and reheating in single field inflationary models
• Bounds on Neutrino Mass in Viscous Cosmology
• Generalised model-independent characterisation of strong gravitational lenses V: reconstructing the lensing distance ratio by supernovae for a general Friedmann universe
• Extremely rapid x-ray flares of tev blazars in the rxte era
• Breaking cosmic degeneracies: Disentangling neutrinos and modified gravity with kinematic information
• A Hint of a Blue Axion Isocurvature Spectrum?
• Improving cosmological parameter estimation with the future 21 cm observation from SKA
• Simplified Smooth Hybrid Inflation in Supersymmetric SU(5)
• Most general cubic-order Horndeski Lagrangian allowing for scaling solutions and the application to dark energy
• A decades-long fast-rise-exponential-decay flare in low-luminosity AGN NGC 7213
• The SLUGGS Survey: The Inner Dark Matter Density Slope of the Massive Elliptical Galaxy NGC 1407
• Velocity dispersion and dynamical masses for 388 Galaxy Clusters and groups. Calibrating the $M_{\mathrm{SZ}}$--$M_{\mathrm{dyn}}$ scaling relation for the PSZ2 sample
• Reignited star formation in dwarf galaxies quenched during reionization
• Accurate Baryon Acoustic Oscillations reconstruction via semi-discrete optimal transport
• Repeated pattern of gamma-ray flares in the lightcurve of the blazar 3C 279
• Observable Predictions for Massive-Neutrino Cosmologies with Model-Independent Dark Energy
• A window for cosmic strings
• The Dark Side of Using Dark Sirens to Constrain the Hubble-Lemaître Constant
• Lagrangian theory for cosmic structure formation with vorticity: Newtonian and post-Friedmann approximations
• On using inspiralling supermassive binary black holes in the PTA frequency band as standard sirens to constrain dark energy
• Effects of galaxy environment on merger fraction
• Limiting Superluminal Neutrino Velocity and Lorentz Invariance Violation by Neutrino Emission from the Blazar TXS 0506+056
• Phenomenology of Quantum Reduced Loop Gravity in the isotropic cosmological sector
• Neutrino mass and asymmetric dark matter: study with inert Higgs doublet and high scale validity
• Roles of ${}^7$Be$(n,p{)}^7$Li resonances in big bang nucleosynthesis with time-dependent quark mass and Li reduction by a heavy quark mass
• The galaxy HI-(sub)halo connection and the HI spatial clustering of local galaxies
• Constraining the Epoch of Reionization With Highly Dispersed Fast Radio Bursts
• A tale of analogies: gravitomagnetic effects, rotating sources, observers and all that
• Structure and dynamics in low density regions: galaxy-galaxy correlations inside cosmic voids
• Quasars probing quasars X: The quasar pair spectral database
• The Cosmological Bias Factor of Damped Lyman Alpha systems: Dependence on Metal Line Strength
• Rapid pre-merger localization of binary neutron stars in third generation gravitational wave detectors
• Probing the Neutrino Mass Hierarchy beyond $\Lambda$CDM Model
• Constraints on the cosmological parameters with three-parameter correlation of Gamma-ray bursts
• Utilizing cosmic-ray positron and electron observations to probe the averaged properties of Milky Way pulsars
• Diagnosing Tsallis Holographic Dark Energy models with interactions
• Impact of QCD uncertainties on antiproton spectra from dark-matter annihilation
• Planck's Dusty GEMS. VIII. Dense-gas reservoirs in the most active dusty starbursts at z~3
• Testing gravity theories with cosmic microwave background in the degenerate higher-order scalar-tensor theory
• A novel CMB polarization likelihood package for large angular scales built from combined WMAP and Planck LFI legacy maps
• Renormalisation of linear halo bias in N-body simulations
• Inception of a first quasar at cosmic dawn
• Compact Molecular Gas Distribution in Quasar Host Galaxies
• SIMPler realisation of Scalar Dark Matter
• Astronomical Polarimetry with the RIT Polarization Imaging Camera
• Impact of dark matter models on the EoR 21-cm signal bispectrum
• Relic density of dark matter in the inert doublet model beyond leading order for the low mass region: 1. Renormalisation and constraints
• A persistent double nuclear structure in 3C 84
• Realistic synthetic integral field spectroscopy with RealSim-IFS
• Comparison of hydrostatic and dynamical masses of distant X-ray luminous galaxy clusters
• ALMA and MUSE observations reveal a quiescent multi-phase circumgalactic medium around the z~3.6 radio galaxy 4C 19.71
• Global radiation signature from early structure formation
• Interpretation of $f(\mathsf{R},\mathsf{T})$ gravity in terms of a conserved effective fluid
• BASS. XXXVI. Constraining the Local Supermassive Black Hole - Halo Connection with BASS DR2 AGN
• ELDAR, a new method to identify AGN in multi-filter surveys: the ALHAMBRA test-case
• Relic galaxy analogues in Illustris TNG50: the formation pathways of surviving red nuggets in a cosmological simulation
• Gravitational waves from mergers of Population III binary black holes: roles played by two evolution channels
• Spatial distribution of dark matter in and around galaxy clusters traced by galaxies, gas and intracluster stars in a simulated universe
• Dark energy versus modified gravity: Impacts on measuring neutrino mass
• Anisotropic cosmological models with two fluids
• Stellar angular momentum can be controlled from cosmological initial conditions
• Linking axionlike dark matter to neutrino masses
• Pure E and B polarization maps via Wiener filtering
• Configuration entropy of the Cosmic Web: Can voids mimic the dark energy?
• Insights into neutrino decoupling gleaned from considerations of the role of electron mass
• Consistency of the Planck CMB data and $\Lambda$CDM cosmology
• Characterization of the HAYSTAC axion dark matter search cavity using microwave measurement and simulation techniques
• Phantom energy dominated universe as a transient stage in $f(R)$ cosmology
• Globular Clusters and Streaming Velocities: Testing the new formation channel in high-resolution cosmological simulations
• Modeling globular clusters in the TNG50 simulation: predictions from dwarfs to giants
• SN 2016gsd: An unusually luminous and linear type II supernova with high velocities
• Galaxy source counts at 7.7 $\mu$m, 10 $\mu$m and 15 $\mu$m with the James Webb Space Telescope
• Improved model-independent constraints on the recombination era and development of a direct projection method
• Off-Diagonal Dark-Matter Phenomenology: Exploring Enhanced Complementarity Relations in Non-Minimal Dark Sectors
• Cosmological constraints with the sub-millimetre galaxies Magnification Bias after large scale bias corrections
• Extended Cosmology in Palatini f(R)-theories
• Probing the High-Redshift Universe with SPICA: Toward the Epoch of Reionization and Beyond
• Viscous universe with cosmological constant
• New observational limits on dark radiation in brane-world cosmology
• Extended X-ray emission in PKS 1718$-$649
• Fruitbat: A Python Package for Estimating Redshifts of Fast Radio Bursts
• On the impact of large angle CMB polarization data on cosmological parameters
• Light neutral CP-even Higgs boson within Next-to-Minimal Supersymmetric Standard model (NMSSM) at the Large Hadron electron Collider (LHeC)
• Constraints on spin-0 dark matter mediators and invisible Higgs decays using ATLAS 13 TeV $pp$ collision data with two top quarks and missing transverse momentum in the final state
• Evidence of a simple dark sector from XENON1T excess
• Several Problems in Particle Physics and Cosmology Solved in One SMASH
• On the dearth of ultra-faint extremely metal poor galaxies
• Multiband RadioAstron space VLBI imaging of the jet in quasar S5 0836+710
• Exploring the hot gaseous halo around an extremely massive and relativistic jet launching spiral galaxy with XMM-Newton
• Exploring CP-violation, via heavy neutrino oscillations, in rare B meson decays at Belle II
• WALLABY Pilot Survey: First Look at the Hydra I Cluster and Ram Pressure Stripping of ESO 501-G075
• Local Group star formation in warm and self-interacting dark matter cosmologies
• Scaling solutions in quintessential inflation
• Targeted search for the kinematic dipole of the gravitational-wave background
• Constraining the Mass of the Emerging Galaxy Cluster SpARCS1049+56 at z=1.71 with Infrared Weak Lensing
• Ionization degree and magnetic diffusivity in the primordial star-forming clouds
• SKYSURF: Constraints on Zodiacal Light and Extragalactic Background Light through Panchromatic HST All-Sky Surface-Brightness Measurements: II. First Limits on Diffuse Light at 1.25, 1.4, and 1.6 microns
• Group-scale intrinsic galaxy alignments in the Illustris-TNG and MassiveBlack-II simulations
• Radio spectral properties of star-forming galaxies between 150-5000MHz in the ELAIS-N1 field
• Strong lensing by fermionic dark matter in galaxies
• The lopsided distribution of satellites of isolated central galaxies
• Asymptotically Safe Non-Minimal Inflation
• The evolution of the low-density HI intergalactic medium from z=3.6 to 0: Data, transmitted flux and HI column density
• The Three Hundred Project: the evolution of physical baryon profiles
• Robust predictions for an oscillatory bispectrum in Planck 2015 data from transient reductions in the speed of sound of the inflaton
• The arbitrariness of potentials in interacting quintessence models
• Auto-identification of unphysical source reconstructions in strong gravitational lens modelling
• Constraining coupled quintessence with the 21cm signal
• Geometric Dark Matter
• Non-Gaussianity in multiple three-form field inflation
• Inflationary Dynamics and Particle Production in a Toroidal Bose-Einstein Condensate
• General quadrupolar statistical anisotropy: Planck limits
• Constraining the epoch of reionization from the observed properties of the high-z Universe
• Constraining quantum collapse inflationary models with CMB data
• The fate of bound systems through Sudden Future Singularities
• On the thermodynamic origin of the initial radiation energy density in warm inflation
• Gravitational Waves from Axion Monodromy
• Perspectives for tests of neutrino mass generation at the GeV scale: Experimental reach versus theoretical predictions
• No need for dark matter in galaxy clusters within Galileon theory
• Building the peanut: simulations and observations of peanut-shaped structures and ansae in face-on disk galaxies
• Weak lensing magnification of SpARCS galaxy clusters
• The relation between cosmological redshift and scale factor for photons
• Post-Newtonian parameters $\gamma$ and $\beta$ of scalar-tensor gravity for a homogeneous gravitating sphere
• Density perturbations in $f(R,\varphi )$-gravity with an application to the (varying power)-law model
• Mufasa:The strength and evolution of galaxy conformity in various tracers
• Measuring Polarized Emission in Clusters in the CMB S4 Era
• Dark matter spin determination with directional direct detection experiments
• Bayesian power-spectrum inference with foreground and target contamination treatment
• Stellar dynamics in the strong-lensing central galaxy of Abell 1201: A low stellar mass-to-light ratio, a large central compact mass, and a standard dark matter halo
• Observed galaxy power spectrum in cubic Galileon model
• Environmental Effect on the Interstellar Medium in Galaxies across the Cosmic Web at z=0.73
• First study of reionization in tilted flat and untilted non-flat dynamical dark energy inflation models
• Spotting hidden sectors with Higgs binoculars
• A new possibility for light-quark Dark Matter
• Predicting fully self-consistent satellite richness, galaxy growth and starformation rates from the STastical sEmi-Empirical modeL STEEL
• The Swampland Conjectures and Slow-Roll Thawing Quintessence
• Dwarfs in the Milky Way halo outer rim: first in-fall or backsplash satellites?
• Linking the small scale relativistic winds and the large scale molecular outflows in the z = 1.51 lensed quasar HS 0810+2554
• ALMA [CII] 158um imaging of an HI-Selected Major Merger at z~4
• The spin-temperature dependence of the 21cm -- LAE cross-correlation
• TXS 2116$-$077: A Gamma-ray Emitting Relativistic Jet Hosted in a Galaxy Merger
• A search for radio afterglows from gamma-ray bursts with the Australian Square Kilometre Array Pathfinder
• Evolution of subhalo orbits in a smoothly-growing host halo potential
• Out of sight, out of mind? The impact of correlated clustering in substructure lensing
• Modelling Population III stars for semi-numerical simulations
• Dynamical friction in Bose-Einstein condensed self-interacting dark matter at finite temperatures, and the Fornax dwarf spheroidal
• WALLABY pre-pilot survey: Two dark clouds in the vicinity of NGC 1395
• Comparing hypervelocity star populations from the Large Magellanic Cloud and the Milky Way
• Atacama Cosmology Telescope measurements of a large sample of candidates from the Massive and Distant Clusters of WISE Survey: Sunyaev-Zeldovich effect confirmation of MaDCoWS candidates using ACT
• Stochastic gravitational-wave background searches and constraints on neutron-star ellipticity
• New Insights into the Criteria of Fast Radio Burst in the Light of FRB 20121102A
• Principles of Gravitational-Wave Detection with Pulsar Timing Arrays
• Can accreting primordial black holes explain the excess radio background?
• Detecting Cosmic Strings with Lensed Fast Radio Bursts
• Multiband gravitational wave observations of stellar binary black holes at the low to middle and high frequencies
• Exploring the cosmic dawn and epoch of reionization with 21cm line
• eRASSt J074426.3+291606: prompt accretion disc formation in a 'faint and slow' tidal disruption event
• The cosmological star formation history from the Local Cosmological Volume of galaxies and constraints on the matter homogeneity
• A giant radio galaxy with three cycles of episodic jet activity from LoTSS DR2
• Fast SMBH growth in the SPT2349--56 protocluster at $z=4.3$
• Masquerading hybrid stars with dark matter
• The SRG/eROSITA All-Sky Survey : Constraints on the structure growth from cluster number counts
• McFacts III: Compact binary mergers from AGN disks over an entire synthetic universe
• Evidence for a toroidal magnetic field in the core of 3C 84
• Birth and Evolution of Fast Radio Bursts: Strong Population-Based Evidence for a Neutron-Star Origin
• Deflection of light by wormholes and its shadow due to dark matter within modified symmetric teleparallel gravity formalism
• Cosmological constraints from weak lensing scattering transform using HSC Y1 data
• Galaxy merger challenge: A comparison study between machine learning-based detection methods
• Correlated 0.01Hz-40Hz seismic and Newtonian noise and its impact on future gravitational-wave detectors
• Constraints on cosmic-ray boosted dark matter with realistic cross section
• Catalogue of model star clusters in the Milky Way and M31 galaxies
• The Dispersion Measure Contributions of the Cosmic Web
• The Obsidian model: Three regimes of black hole feedback
• A Model-independent Method to Determine $H_0$ Using Time-Delay Lensing, Quasars and Type Ia Supernovae
• LIGO-Virgo-KAGRA's Oldest Black Holes: Probing star formation at cosmic noon with GWTC-3
• A Mixture of LBG Overdensities in the Fields of Three $6<z<7$ Quasars: Implications for the Robustness of Photometric Selection
• Powerful Radio-Loud Quasars are Triggered by Galaxy Mergers in the Cosmic Bright Ages
• Dissect two-halo galactic conformity effect for central galaxies: The dependence of star formation activities on the large-scale environment
• Constraining ultralight dark matter using the Fermi-LAT pulsar timing array
• Exploring binary black hole mergers and host galaxies with Shark and COMPAS
• Insights into the reionization epoch from cosmic-noon-CIV emitters in the VANDELS survey
• Extending the Discovery Potential for Inelastic-Dipole Dark Matter with FASER
• Molecular Outflows in z > 6 QSO Hosts Driven by Star Formation
• DS+: a method for the identification of cluster substructures
• A General Bayesian Framework to Account for Foreground Map Errors in Global 21-cm Experiments
• The Rest-Frame Submillimeter Spectrum of High Redshift, Dusty, Star-Forming Galaxies from the SPT-SZ Survey
• Propagation of scalar and tensor gravitational waves in Horndeski theory
• Galactic rotation dynamics in a new $f(\mathcal{R})$ gravity model
• Electromagnetic Follow-up Observations of Binary Neutron Star Mergers with Early Warnings from Decihertz Gravitational-wave Observatories
• BeyondPlanck XII. Cosmological parameter constraints with end-to-end error propagation
• The Tianlai dish array low-z surveys forecasts
• There and back again: understanding the critical properties of backsplash galaxies
• Cosmological simulations of self-interacting Bose-Einstein condensate dark matter
• Integrated trispectrum detection from BOSS DR12 NGC CMASS
• Kilonova and Optical Afterglow from Binary Neutron Star Mergers. II. Optimal Search Strategy for Serendipitous Observations and Target-of-opportunity Observations of Gravitational-wave Triggers
• Reionization with Simba: How much does astrophysics matter in modeling cosmic reionization?
• Sizing from the Smallest Scales: The Mass of the Milky Way
• Brightest Cluster Galaxies Trace Weak Lensing Mass Bias and Halo Triaxiality in The Three Hundred Project
• Virial halo mass function in the $Planck$ cosmology
• Indirect dark-matter detection with MadDM v3.2 -- Lines and Loops
• Superclustering with the Atacama Cosmology Telescope and Dark Energy Survey: I. Evidence for thermal energy anisotropy using oriented stacking
• Search for High-Energy Neutrinos from Ultra-Luminous Infrared Galaxies with IceCube
• ALP-portal majorana dark matter
• Forensic reconstruction of galaxy colour evolution and population characterisation
• Lagrangian approach to super-sample effects on biased tracers at field level: galaxy density fields and intrinsic alignments
• Measuring the average molecular gas content of star-forming galaxies at $z=3-4$
• Modeling Redshift-Space Clustering with Abundance Matching
• Magnetar Models of Superluminous Supernovae from the Dark Energy Survey: Exploring Redshift Evolution
• Halo-model analysis of the clustering of photometric luminous red galaxies at $0.10\le z\le 1.05$ from the Subaru Hyper Suprime-Cam Survey
• The Impacts of Modeling Choices on the Inference of the Circumgalactic Medium Properties from Sunyaev-Zeldovich Observations
• The MUSE Hubble Ultra Deep Field Survey XVI. The angular momentum of low-mass star-forming galaxies. A cautionary tale and insights from TNG50
• Scope out multiband gravitational-wave observations of GW190521-like binary black holes with space gravitational wave antenna B-DECIGO
• Effect of axion-like particles on the spectrum of the extragalactic gamma-ray background
• Optimal computation of anisotropic galaxy three point correlation function multipoles using 2DFFTLOG formalism
• Biases and Cosmic Variance in Molecular Gas Abundance Measurements
• Radio Galaxy Zoo: New Giant Radio Galaxies in the RGZ DR1catalogue
• One-Two Quench: A Double Minor Merger Scenario
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• Covariance of the redshift-space matter power spectrum after reconstruction
• Supermassive black hole fueling in IllustrisTNG: Impact of environment
• Constraints on dark energy models from the Horndeski theory
• Clustering of Local Extrema in Planck CMB maps
• The Broad-lined Ic Supernova ZTF18aaqjovh (SN 2018bvw): An Optically-discovered Engine-driven Supernova Candidate with Luminous Radio Emission
• Quantifying EoR delay spectrum contamination from diffuse radio emission
• Luminosity-duration relation of fast radio bursts
• The ${}^6$Li/${}^7$Li isotopic ratio in the metal-poor binary CS22876--032
• Helium and Nitrogen Enrichment in Massive Main Sequence Stars: Mechanisms and Implications for the Origin of WNL Stars
• Time delay of timelike particles in gravitational lensing of Schwarzschild spacetime
• Deep-CEE I: Fishing for Galaxy Clusters with Deep Neural Nets
• Type I + II Seesaw in a Two Higgs Doublet Model
• An Inpainting Approach to Tackle the Kinematic and Thermal SZ Induced Biases in CMB-Cluster Lensing Estimators
• High-resolution spectroscopy of gaseous ${}^{83m}$Kr conversion electrons with the KATRIN experiment
• QSOs sigposting cluster size halos as gravitational lenses: halo mass, projected mass density profile and concentration at $z\sim 0.7$
• BE-HaPPY: Bias Emulator for Halo Power Spectrum including massive neutrinos
• Power spectrum of primordial perturbations for an emergent universe in quantum reduced loop gravity
• Ballistic Dark Matter oscillates above $\Lambda$CDM
• Median Statistics Analysis of Deuterium Abundance Measurements and Spatial Curvature Constraints
• Prospects of detecting dark matter through cosmic-ray antihelium with the antiproton constraints
• The Universe as an Oscillator
• Design and characterization of the Cosmology Large Angular Scale Surveyor (CLASS) 93 GHz focal plane
• Production Rate Measurement of Tritium and Other Cosmogenic Isotopes in Germanium with CDMSlite
• Limits on Interactions between Weakly Interacting Massive Particles and Nucleons Obtained with NaI(Tl) crystal Detectors
• When Freeze-out Precedes Freeze-in: Sub-TeV Fermion Triplet Dark Matter with Radiative Neutrino Mass
• Covariances for cosmic shear and galaxy-galaxy lensing in the response approach
• Impact of EDGES 21cm Global Signal on Primordial Power Spectrum
• Growth of perturbations in dark energy parametrization scenarios
• Reconstruction of primordial tensor power spectra from B-mode polarization of the cosmic microwave background
• Core formation from self-heating dark matter
• Multi-wavelength mock observations of the WHIM in a simulated galaxy cluster
• The frequency of very young galaxies in the local Universe: I. A test for galaxy formation and cosmological models
• The Cosmic Web Around The Brightest Galaxies During The Epoch Of Reionization
• A study on a minimally broken residual TBM-Klein symmetry with its implications on flavoured leptogenesis and ultra high energy neutrino flux ratios
• A new mechanism of sterile neutrino dark matter production
• Tight $H_0$ constraint from galaxy redshfit surveys: combining baryon acoustic osillation measurements and Alcock-Paczynski test
• Weak lensing probe of cubic Galileon model
• Dark Energy Constraints in light of Pantheon SNe Ia, BAO, Cosmic Chronometers and CMB Polarization and Lensing Data
• Phantom crossing dark energy in Horndeski's theory
• Confronting the DAMPE Excess with the Scotogenic Type-II Seesaw Model
• Tidal Stripping and Post-Merger Relaxation of Dark Matter Halos: Causes and Consequences of Mass Loss
• Majorana Dark Matter in a new B-L model
• Gravitational Waves, mu Term & Leptogenesis from B-L Higgs Inflation in Supergravity
• Solving the flatness problem with an anisotropic instanton in Hořava-Lifshitz gravity
• Large-scale structure in mimetic Horndeski gravity
• The dipole anisotropy of WISE x SuperCOSMOS number counts
• CP Violation at the Finite Temperature
• On general features of warm dark matter with reduced relativistic gas
• Investigating the Unification of LOFAR-detected powerful AGN in the Boötes Field
• Dark-ages Reionization and Galaxy Formation Simulation - XIII. AGN quenching of high-redshift star formation in ZF-COSMOS-20115
• Muon g-2 in an Alternative Quasi-Yukawa Unification with Low Fine-Tuned Inverse SeeSaw Mechanism
• Analytical expressions and numerical evaluation of the luminosity distance in a flat cosmology
• On nonlocally interacting metrics, and a simple proposal for cosmic acceleration
• General calculation of the cross section for dark matter annihilations into two photons
• Anisotropic inflation with a non-minimally coupled electromagnetic field to gravity
• Making maps of Cosmic Microwave Background polarization for B-mode studies: the POLARBEAR example
• Constraining cosmological ultra-large scale structure using numerical relativity
• Model-independent constraints on modified gravity from current data and from the Euclid and SKA future surveys
• The VVV survey: Long-period variable stars I. Photometric catalog of ten VVV/OGLE tiles
• On large lepton number asymmetries of the Universe
• Galaxy bias from galaxy-galaxy lensing in the DES Science Verification Data
• Classification and asymptotic structure of black holes in bimetric theory
• Probing Screening and the Graviton Mass with Gravitational Waves
• \bf $\delta M$ Formalism: A New Approach to Cosmological Perturbation Theory in Anisotropic Inflation
• Evolution of dark matter velocity dispersion
• The Inflaton Portal to Dark Matter
• Bulk viscous fluid in extended symmetric teleparallel gravity
• Parameter estimation with the current generation of phenomenological waveform models applied to the black hole mergers of GWTC-1
• Angular clustering and host halo properties of [OII] emitters at $z>1$ in the Subaru HSC survey
• Inferring the Morphology of Stellar Distribution in TNG50: Twisted and Twisted-Stretched shapes
• Analysis of the ${}^3\mathrm{He}(\alpha ,\gamma {)}^7\mathrm{Be}$ and ${}^3\mathrm{H}(\alpha ,\gamma {)}^7\mathrm{Li}$ astrophysical direct capture reactions in a modified potential-model approach
• Dark CP-violation through the $Z$-portal
• The miniJPAS survey: clusters and galaxy groups detection with AMICO
• Testing averaged cosmology with type Ia supernovae and BAO data
• The ultra-long GRB 220627A at z=3.08
• Gravitational waves and dark matter from classical scale invariance
• Observational constraints on interacting vacuum energy with linear interactions
• Robustness of the covariance matrix for galaxy clustering measurements
• Squark-pair annihilation into quarks at next-to-leading order
• Status of Flavour Maximal Non-minimal Universal Extra Dimension
• Exact non-linear equations for cosmological perturbations
• Structure formation in dark energy cosmologies described by PADE parameterization
• Correlation of normal neutrino mass ordering with upper octant of ${\theta }_{23}^{}$ and third quadrant of $\delta$ via RGE-induced $\mu$-$\tau$ symmetry breaking
• Impact of the small-scale structure on the Stochastic Background of Gravitational Waves from cosmic strings
• Modified Gauss-Bonnet Gravity with Radiating Fluids
• On the relative velocity distribution for general statistics and an application to big-bang nucleosynthesis under Tsallis statistics
• An ACA Survey of [CI] ${}^3{P}_1{-}^3{P}_0$, CO $J=4-3$, and Dust Continuum in Nearby U/LIRG
• The evolutionary pathways of disk galaxies with different sizes
• MUSE unravels the ionisation and origin of metal enriched absorbers in the gas halo of a z = 2.92 radio galaxy
• The THESAN project: Lyman-alpha emitter luminosity function calibration
• Signs of Higher Multipoles and Orbital Precession in GW151226
• Universality in generalized models of inflation
• Intensity mapping of the 21cm emission: lensing
• Signatures from a merging galaxy cluster and its AGN population: LOFAR observations of Abell 1682
• Radiative stability and observational constraints on dark energy and modified gravity
• Post-inflationary thermal histories and the refractive index of relic gravitons
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). The matter density and baryon fraction from the galaxy power spectrum at redshift $0.6<z<1.1$
• The variance of the CMB temperature gradient: a new signature of a multiply connected Universe
• Dynamical aspects for scalar fields coupled to cubic contractions of the Riemann tensor
• PopSED: Population-Level Inference for Galaxy Properties from Broadband Photometry with Neural Density Estimation
• Z-portal Continuum Dark Matter
• Light sterile neutrinos from a late phase transition
• Quantum Gravity, Time, Bounces and Matter
• Application of the iterative reconstruction to simulated galaxy fields
• Does black hole continuum spectrum signal f(R) gravity in higher dimensions?
• Mapping Lyman-alpha forest three-dimensional large scale structure in real and redshift space
• Impact of gas based seeding on supermassive black hole populations at $z\ge 7$
• Modeling Gamma-ray burst Afterglow observations with an Off-axis Jet emission
• Observational constraints of an anisotropic boost due to the projection effects using redMaPPer clusters
• The Search for Binary Supermassive Black Holes Amongst Quasars with Offset Broad Lines Using the Very Long Baseline Array
• Asteroseismology of KIC 7107778: a binary comprising almost identical subgiants
• CO Tully-Fisher Relation of Star-forming Galaxies at z=0.05-0.3
• WIMP and FIMP dark matter in the inert doublet plus singlet model
• $\Delta \left(27\right)$ flavor singlet-triplet Higgs model for fermion masses and mixings
• Impact of ringdown higher-order modes on black-hole mergers in dense environments: the scalar field case, detectability and parameter biases
• Gravitational lensing in LoTSS DR2 -- Extremely faint 144-MHz radio emission from two highly magnified quasars
• DAMPE excess from decaying right-handed neutrino dark matter
• Cosmology with the submillimetre galaxies magnification bias: Proof of concept
• J1615+5452: a remnant radio galaxy in the ELAIS-N1 field
• Lagrangian theory of structure formation in relativistic cosmology. IV. Lagrangian approach to gravitational waves
• Luminosity distribution of fast radio bursts from CHIME/FRB Catalog 1 by means of the updated Macquart relation
• Massive gravity and the suppression of anisotropies and gravitational waves in a matter-dominated contracting universe
• Scintillation can explain the spectral structure of the bright radio burst from SGR 1935+2154
• Gravitational Wave Opacity from Gauge Field Dark Energy
• Forecast constraints on Anisotropic Stress in Dark Energy using gravitational-waves
• ART${}^2$: A 3D Parallel Multi-wavelength Radiative Transfer Code for Continuum and Atomic and Molecular Lines
• Noether symmetry in a nonlocal f(T) Gravity
• Nebular Halpha emission in SN Ia 2016jae
• Alignment without Decoupling: the Portal to Light Dark Matter in the MSSM
• Strongly Interacting Neutrino Portal Dark Matter
• Constraining gravity with a new precision $E_G$ estimator using Planck + SDSS BOSS
• Cosmological Probes of Structure Growth and Tests of Gravity
• A Spectroscopic Survey of the Fields of 28 Strong Gravitational Lenses: Implications for $H_0$
• Determining $H_0$ with the latest HII galaxy measurements
• Explosive Axion Production from Saxion
• High-redshift Damped Ly-alpha Absorbing Galaxy Model Reproducing the N(HI)-Z Distribution
• On ${\mathbf{Q}}_6$ flavor symmetry and the breaking of $\mu \leftrightarrow \tau$ symmetry
• Exploring Non-Holomorphic Soft Terms in the Framework of Gauge Mediated Supersymmetry Breaking
• Dark Matter from a Vector Field in the Fundamental Representation of $SU(2{)}_L$
• Actual Physics behind Mono-X
• Lyman-$\alpha$ Polarization Intensity Mapping
• Effects of neutrino mass and asymmetry on cosmological structure formation
• Dark Matter Annihilation into Four-Body Final States and Implications for the AMS Antiproton Excess
• fkPT: Constraining scale-dependent modified gravity with the full-shape galaxy power spectrum
• Connecting Galactic Outflows and Star Formation: Inferences from H-alpha Maps and Absorption Line Spectroscopy at 1 < z < 1.5
• Internal dark matter structure of the most massive galaxy clusters
• Variability-selected low-luminosity active galactic nuclei candidates in the 7 Ms Chandra Deep Field-South
• A hyper luminous starburst at z=4.72 magnified by a lensing galaxy pair at z=1.48
• The Kinematic Sunyaev-Zel'dovich Effect with ACT, DES, and BOSS: a Novel Hybrid Estimator
• Impact of an eV-mass sterile neutrino on the neutrinoless double-beta decays: a Bayesian analysis
• Baryogenesis via Leptogenesis from Asymmetric Dark Matter and radiatively generated Neutrino mass
• High-resolution international LOFAR observations of 4C~43.15 -- Spectral ages and injection indices in a high-z radio galaxy
• European Spallation Source as a searching tool for an ultralight scalar field
• Constraining C iii] Emission in a Sample of Five Luminous z = 5.7 Galaxies
• A general study of decaying scalar dark matter: existing limits and projected radio signals at the SKA
• On new physics searches with multidimensional differential shapes
• Smoke on the water: CO and H2O in a circumnuclear disc around a quasar at redshift 2.64
• Probing higher-spin fields from inflation with higher-order statistics of the CMB
• Maximally Rotating Supermassive Stars at the Onset of Collapse: The Perturbative Effects of Gas Pressure, Magnetic Fields, Dark Matter and Dark Energy
• Explaining the statistical properties of Fast Radio Bursts with suppressed low-frequency emission
• New constraints on the physical conditions in H${}_2$-bearing GRB-host damped Lyman-$\alpha$ absorbers
• EDGES result versus CMB and low-redshift constraints on ionization histories
• Second-order cosmological perturbations. I. Produced by scalar-scalar coupling in synchronous gauge
• Cosmic acceleration and de Sitter expansion in hybrid mass varying neutrino model
• Ultra-high energy cosmic rays deflection by the Intergalactic Magnetic Field
• Quenching of Massive Disk Galaxies in the IllustrisTNG Simulation
• Cross-correlation between the 21-cm signal and [OIII] emitters during early cosmic reionization
• Model-independent and model-based local lensing properties of CL0024+1654 from multiply-imaged galaxies
• Generalized scalar-tensor theory of gravity reconstruction from physical potentials of a scalar field
• The BAHAMAS project: Effects of a running scalar spectral index on large-scale structure
• Analysing parameter space correlations of recent 13 TeV gluino and squark searches in the pMSSM
• Growth of perturbations in nonlocal gravity with non-$\Lambda$CDM background
• A hide-and-seek game: Looking for Population III stars during the Epoch of Reionization through the HeII$\lambda$1640 line
• A moment approach to compute quantum-gravity effects in the primordial universe
• Improved Galactic Foreground Removal for B-Modes Detection with Clustering Methods
• Constraints on $f(R)$ and nDGP Modified Gravity Model Parameters with Cluster Abundances and Galaxy Clustering
• Internal Calibration of the PandaX-II Detector with Radon Gaseous Sources
• Gaussian-process reconstructions and model building of quintom dark energy from latest cosmological observations
• Towards the first detection of strongly lensed HI emission
• Space-time second-quantization effects and the quantum origin of cosmological constant in covariant quantum gravity
• The metal-poor end of the Spite plateau. II. Detailed chemical investigation
• On the Impact of Neutron Star Binaries Natal-Kick Distribution on the Galactic r-process Enrichment
• AGN flares as counterparts to LIGO/Virgo mergers: No confident causal connection in spatial correlation analysis
• General Relativistic corrections in density-shear correlations
• Primordial magnetic fields during the cosmic dawn in light of EDGES 21-cm signal
• Narrow, Intrinsic CIV Absorption in Quasars as it Relates to Outflows, Orientation, and Radio Properties
• Fermions in Hybrid Loop Quantum Cosmology
• Gas clumping in the outskirts of the Virgo cluster
• Understanding the early stages of galaxy formation using very metal-poor stars from the Hamburg/ESO survey
• Constraint on the radius of five-dimensional dS spacetime with GW170817 and GRB 170817A
• Mean Energy Density of Photogenerated Magnetic Fields Throughout the Epoch of Reionization
• The Lyman-$\alpha$ power spectrum - CMB lensing convergence cross-correlation
• ALMA Observations of Molecular Absorption in the Gravitational Lens PMN 0134-0931
• Gauge invariant canonical cosmological perturbation theory with geometrical clocks in extended phase space - a review and applications
• The Impact of Realistic Foreground and Instrument Models on 21cm Epoch of Reionization Experiments
• Inflation, Swampland, and Landscape
• Multi-Phase ISM in the z = 5.7 Hyperluminous Starburst SPT0346-52
• Study of parameter degeneracy and hierarchy sensitivity of NO$\nu$A in presence of sterile neutrino
• One-off and Repeating Fast Radio Bursts: A Statistical Analysis
• On Bouncing and Nonsingular Solutions in Einstein-scalar-Gauss-Bonnet Cosmology
• Modelling high-resolution ALMA observations of strongly lensed dustystar forming galaxies detected by Herschel
• Cosmic Web Dissection in Fuzzy Dark Matter Cosmologies
• Planck Limits on Non-canonical Generalizations of Large-field Inflation Models
• Galaxy quenching timescales from a forensic reconstruction of their colour evolution
• Measuring the scale dependence of intrinsic alignments using multiple shear estimates
• Model Independent analysis of MeV scale dark matter: I. Cosmological constraints
• Second-order cosmological perturbations. II. Produced by scalar-tensor and tensor-tensor couplings
• Dynamical friction in self-interacting ultralight dark matter
• Using Artificial Neural Networks to Constrain the Halo Baryon Fraction during Reionization
• How feedback shapes galaxies: an analytic model
• Dynamical History Of The Local Group In $\Lambda$CDM $\mathrm{II}$ $-$ Including External Perturbers In 3D
• Unification of BL Lac objects, FR I and FR II(G) radio galaxies and Doppler factor Estimation for BL Lac Objects
• H.E.S.S. follow-up observations of Binary Black Hole Coalescence events during the second and third Gravitational Waves observing runs of Advanced LIGO and Advanced Virgo
• Probing the hot circumgalactic medium of external galaxies in X-ray absorption II: a luminous spiral galaxy at $z\approx 0.225$
• Numerical study of inflationary preheating with arbitrary power-law potential and a realization of curvaton mechanism
• Lonely Little Red Dots: Challenges to the AGN-nature of little red dots through their clustering and spectral energy distributions
• Xenon-1T excess as a possible signal of a sub-GeV hidden sector dark matter
• A new parametrization for dark energy density and future deceleration
• Wrong sign Yukawa coupling of the 2HDM plus a singlet scalar dark matter confronted with dark matter and Higgs data
• The zenithal 4-m International Liquid Mirror Telescope: a unique facility for supernova studies
• The Manhattan Suite: Accelerated galaxy evolution in the early Universe
• Imprints of non-standard Dark Energy and Dark Matter Models on the 21cm Intensity Map Power Spectrum
• Stellar-mass black-hole binaries in LISA: characteristics and complementarity with current-generation interferometers
• The tidal evolution of the Fornax dwarf spheroidal and its globular clusters
• Diagnosing the interstellar medium of galaxies with far-infrared emission lines I. The [C II] 158 microns line at z~0
• Geometry and growth contributions to cosmic shear observables
• The Origin of Stars in the Inner 500 Parsecs in TNG50 Galaxies
• Clumpy star formation and an obscured nuclear starburst in the luminous dusty z=4 galaxy GN20 seen by MIRI/JWST
• Dark matter production and reheating via direct inflaton couplings: collective effects
• Simplified galaxy formation with mesh-less hydrodynamics
• Cherenkov Telescope Array sensitivity to branon dark matter models
• Perspectives on constraining a cosmological constant-type parameter with pulsar timing in the Galactic Center
• Forecasting the Cross-Correlation of the CSST galaxy survey with the FAST HI Intensity Map
• Limits on Brane-World and Particle Dark Radiation from Big Bang Nucleosynthesis and the CMB
• On the effect of Lyman alpha trapping during the initial collapse of massive black hole seeds
• Unveiling the origins of galactic bars: insights from barred and unbarred galaxies
• Variations of cosmic large-scale structure covariance matrices across parameter space
• Agnostic Stacking of Intergalactic Doublet Absorption: Measuring the NeVIII Population
• One-loop quantum gravitational corrections to the scalar two-point function at fixed geodesic distance
• On the kinetic Sunyaev-Zel'dovich effect as an observational probe for halo spin bias
• Origins Space Telescope: predictions for far-IR spectroscopic surveys
• Effect of reheating on predictions following multiple-field inflation
• Distinguishing between $\Lambda$CDM and $f(R)$ gravity models using halo ellipticity correlations in simulations
• Leptogenesis and Dark Matter from Low Scale Seesaw
• Stellar cluster formation in a Milky Way-sized galaxy at z>4 -- I. The proto-globular cluster population and the imposter amongst us
• Radio Power from a Direct-Collapse Black Hole in CR7
• Optimizing simulation parameters for weak lensing analyses involving non-Gaussian observables
• Clustering of red-sequence galaxies in the fourth data release ofthe Kilo-Degree Survey
• Shadow of Schwarzschild Black Hole in the Cold Dark Matter Halo
• The Global 21 cm Absorption from Cosmic Dawn with Inhomogeneous Gas Distribution
• The radial dependence of dark matter distribution in M33
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: a tomographic measurement of structure growth and expansion rate from anisotropic galaxy clustering in Fourier space
• Massive graviton dark matter with environment dependent mass: A natural explanation of the dark matter-baryon ratio
• A general relativistic mass-to-distance ratio for a set of megamaser AGN black holes
• Is a top-heavy initial mass function needed to reproduce the submillimeter galaxy number counts?
• Space-Time Quasicrystal Structures and Inflationary and Late Time Evolution Dynamics in Accelerating Cosmology
• Estimators of Bolometric Luminosity and Black Hole Mass with Mid-infrared Continuum Luminosities for Dust-obscured Quasars: Prevalence of Dust-obscured SDSS Quasars
• Aspects of Dark Matter Annihilation in Cosmology
• Consistency of Pantheon+ supernovae with a large-scale isotropic universe
• The Impact of Unresolved Turbulence on the Escape Fraction of Lyman Continuum Photons
• Not All Subhaloes Are Created Equal: Modelling the Diversity of Subhalo Density Profiles in TNG50
• Analysis of four-zero textures in $3+1$ framework
• Testing gravity with gravitational wave friction and gravitational slip
• A Test of MONDian Gravity in $\sim$300 pressure supported elliptical galaxies from the MaNGA survey
• Lopsided Galaxies in a cosmological context: a new galaxy-halo connection
• Measuring the delay time distribution of binary neutron stars. III. Using the individual star formation histories of gravitational wave event host galaxies in the local universe
• Testable predictions of outside-in age gradients in dwarf galaxies of all types
• A Global ILC Approach in Pixel Space over Large Angular Scales of the Sky using CMB Covariance Matrix
• Searching for a possible dipole anisotropy on acceleration scale with 147 rotationally supported galaxies
• A deep 1.4 GHz survey of the J1030 equatorial field: a new window on radio source populations across cosmic time
• Primordial magnetic fields: consistent initial conditions and impact on high-z structures
• A Grand-Unified Nelson-Barr Model
• Testing Texture Two Zero Neutrino Mass Matrices Under Current Experimental Scenario
• Detection of HI 21 cm emission from a strongly lensed galaxy at z~1.3
• Sine-Gordon solitonic scalar stars and black holes
• Anomalies in $b\to s$ transitions and dark matter
• The Integrated Bispectrum in Modified Gravity Theories
• Ultra high energy cosmic rays from non-relativistic quasar outflows
• Neutrinophilic Dark Matter in the epoch of IceCube and Fermi-LAT
• Constraining the cosmic merger history of intermediate-mass black holes with gravitational wave detectors
• Recovering a redshift-extended VSL signal from galaxy surveys
• Tracking Halo Orbits and Their Mass Evolution around Large-scale Filaments
• Peering beyond the horizon with standard sirens and redshift drift
• New parameterization for unified dark matter and dark energy
• Axially magnetized Dark Energy cosmological model
• Uniqueness of the Fock quantization of scalar fields in a Bianchi I cosmology with unitary dynamics
• Bounds on Higher Derivative $f(R,\square R,T)$ Models from Energy Conditions
• Recovering $\Lambda$CDM Model From a Cosmographic Study
• Chameleon Field Dynamics During Inflation
• The effects of the small-scale behaviour of dark matter power spectrum on CMB spectral distortion
• IceCube's astrophysical neutrino energy spectrum from CPT violation
• Cosmological aspects of a unified dark energy and dust dark matter model
• Extragalactic diffuse gamma-rays from dark matter annihilation: revised prediction and full modelling uncertainties
• Massive Galaxy Mergers Have Distinctive Global HI Profiles
• Euclid: A complete Einstein ring in NGC 6505
• Flaring radio lanterns along the ridge line: long-term oscillatory motion in the jet of S5 1803+784
• Probing Small Scale Primordial Power Spectrum with 21cm Line Global Signal
• Cosmological implications of Standard Model criticality and Higgs inflation
• Solving the conundrum of intervening strong MgII absorbers towards GRBs and quasars
• Star formation traced by optical and millimeter hydrogen recombination lines and free-free emissions in the dusty merging galaxy NGC 3256 -- MUSE/VLT and ALMA synergy
• ASASSN-15no: The Supernova that plays hide-and-seek
• Measuring our velocity from fluctuations in number counts
• Cluster counts III. $\Lambda$CDM extensions and the cluster tension
• The first GeV flare of the radio-loud narrow-line Seyfert 1 galaxy PKS 2004-447
• Detection of spatial clustering in the 1000 richest SDSS DR8 redMaPPer clusters with Nearest Neighbor distributions
• Quaternion algebra on 4D superfluid quantum space-time. Gravitomagnetism
• Primordial power spectrum features in phenomenological descriptions of inflation
• On the deuterium abundance and the importance of stellar mass loss in the interstellar and intergalactic medium
• On the tension between growth rate and CMB data
• Higgs and gauge boson phenomenology of the 3-3-1 model with CKS mechanism
• Asymmetric dark matter with a spontaneously broken $U(1{)}^{\prime }$: self-interaction and gravitational waves
• Linear and non-linear perturbations in dark energy models
• Cosmological evolution of viable models in the generalized scalar-tensor theory
• Reconsidering the dynamical states of galaxy clusters using PCA and UMAP
• Stability of a modified Jordan-Brans-Dicke theory in the dilatonic frame
• Quantifying Density-Ionization Correlations with the 21cm Power Spectrum
• Precise Clustering and Density Evolution of redMaPPer Galaxy Clusters versus MXXL Simulation
• Phenomenology of the Inert Doublet Model with a global U(1) symmetry
• Ram pressure stripping: An analytical approach
• The Escape Velocity Profile of the Milky Way from Gaia DR3
• Radial acceleration relation and dissipative dark matter
• On the nature of LOFAR RMs and new constraints on magnetic fields in cosmic filaments and on magnetogenesis scenarios
• Braids, 3-manifolds, elementary particles: number theory and symmetry in particle physics
• Supermassive Binary Black Hole Evolution can be traced by a small SKA Pulsar Timing Array
• Gravity lens critical test for gravity constants and dark sector
• X-ray morphology of cluster-mass haloes in self-interacting dark matter
• Leptonic scalar portal: Origin of muon $g-2$ anomaly and dark matter?
• Dark Matter search in dwarf irregular galaxies with the Fermi Large Area Telescope
• Quantifying the CMB Degeneracy Between the Matter Density and Hubble Constant in Current Experiments
• The dynamical structure of broken power-law and double power-law models for dark matter haloes
• Probing star formation in galaxies at $z\approx 1$ via a Giant Metrewave Radio Telescope stacking analysis
• Identification of the anomalous fast bulk events in a p-type point contact germanium detector
• Rapidly quenched galaxies in the Simba cosmological simulation and observations
• The OTELO survey as a morphological probe. Last ten Gyr of galaxy evolution. The mass--size relation up to z=2
• Constraining Density Fluctuations with Big Bang Nucleosynthesis in the Era of Precision Cosmology
• Probing Hot Gas Components of Circumgalactic Medium in Cosmological Simulations with the Thermal Sunyaev-Zel'dovich Effect
• An X-ray and SZ bright diffuse source toward M31: a Local Hot Bridge
• Backreaction from quantum fluxes at the Kerr inner horizon
• The impact and mitigation of broad absorption line quasars in Lyman$-\alpha$ forest correlations
• Bias of Damped Lyman-$\alpha$ systems from their cross-correlation with CMB lensing
• What if GW190425 did not produce a black hole promptly?
• Implications of the upper bound on $\mathbf{h}\to {\mathbf{\mu }}^{+}{\mathbf{\mu }}^{-}$ on the baryon asymmetry of the Universe
• Metallicity and Age of the Stellar Stream Around the Disk Galaxy NGC 5907
• Density Weighted Angular Redshift Fluctuations: a New Cosmological Observable
• A model independent parametrization of the late time cosmic acceleration: constraints on the parameters from recent observations
• Dark matter and observable Lepton Flavour Violation
• Vainshtein Screening in Bimetric Cosmology
• The magnetised and thermally unstable tails of jellyfish galaxies
• Post-inflationary Scalar Tensor Cosmology and Inflationary Parameters
• Current and future constraints on extended Bekenstein-type models for a varying fine-structure constant
• Enlightening the dark ages with dark matter
• Weak Lensing Study in VOICE Survey I: Shear Measurement
• Consistency of cosmic microwave background temperature measurements in three frequency bands in the 2500-square-degree SPT-SZ survey
• Dynamics of Polynomial Chaplygin Gas Warm Inflation
• The role of Dark Matter sub-halos in the non-thermal emission of galaxy clusters
• Quasi-isotropic cycles and non-singular bounces in a Mixmaster cosmology
• Inflation from higher dimensions
• SHARDS Frontier Fields: Physical properties of a low mass Lyman-alpha emitter at z=5.75
• Compatibility of a dark matter discovery at XENONnT/LZ with the WIMP thermal production mechanism
• On the general nature of 21cm-Lyman-$\alpha$ emitters cross-correlations during reionisation
• Dark-ages reionization and galaxy formation simulation -- XVIII. The high-redshift evolution of black holes and their host galaxies
• Current Status of Top-Specific Variant Axion Model
• Mutated hilltop inflation revisited
• Dark information of black hole radiation raised by dark energy
• Can AGN and galaxy clusters explain the surface brightness fluctuations of the cosmic X-ray background?
• An Empirical Study of Contamination in Deep, Rapid, and Wide-Field Optical Follow-Up of Gravitational Wave Events
• Kinetic Field Theory: Exact free evolution of Gaussian phase-space correlations
• Hubble multi-scalar inflation
• Fate of the true-vacuum bubbles
• Effect of lithium hydride on the cooling of primordial gas
• Running Vacuum Cosmological Models: Linear Scalar Perturbations
• Small field models with gravitational wave signature supported by CMB data
• Localization of binary neutron star mergers with a single Cosmic Explorer
• Dark sector unifications: dark matter-phantom energy, dark matter -- constant $w$ dark energy, dark matter-dark energy-dark matter
• A million-solar-mass object detected at cosmological distance using gravitational imaging
• Conversion of Gravitons into Dark Photons in Cosmological Dark Magnetic Fields
• Understanding the progenitor formation galaxies of merging binary black holes
• The impact of baryons on the internal structure of dark matter haloes from dwarf galaxies to superclusters in the redshift range 0<z<7
• D-brane Disformal Coupling and Thermal Dark Matter
• Scalar Field Theory Description of the Running Vacuum Model: the Vacuumon
• First search for invisible decays of ortho-positronium confined in a vacuum cavity
• Tomographic Constraints on Gravity from Angular Redshift Fluctuations in the Late Universe
• Hybrid modeling of redshift space distortions
• Quasinormal modes, Hawking radiation and absorption of the massless scalar field for Bardeen black hole surrounded by perfect fluid dark matter
• Afterglow light curves of the non-relativistic ejecta mass in a stratified circumstellar medium
• The contribution of globular clusters to cosmic reionization
• The Massive and Distant Clusters of WISE Survey V: Extended Radio Sources in Massive Galaxy Clusters at z~1
• Parameter constraints from weak lensing tomography of galaxy shapes and cosmic microwave background fluctuations
• Cosmic String Detection with Tree-Based Machine Learning
• Sensitivity of the Hydrogen Epoch of Reionization Array and its Build-out Stages to One-point Statistics from Redshifted 21 cm Observations
• The dispersion measure and rotation measure from fast radio burst host galaxies based on the IllustrisTNG50 simulation
• Constraining Scatter in the Stellar Mass--Halo Mass Relation for Haloes Less Massive than the Milky Way
• Brane inflation and the robustness of the Starobinsky inflationary model
• Cosmological constraints on sterile neutrino oscillations from Planck
• The observable $E_g$ statistics
• ASASSN-18am/SN 2018gk : An overluminous Type IIb supernova from a massive progenitor
• Monojet Searches for MSSM Simplified Models
• ERGO-ML: Comparing IllustrisTNG and HSC galaxy images via contrastive learning
• Photoevaporation of Minihalos during Cosmic Reionization: Primordial and Metal-Enriched Halos
• The Luminosity Functions and Redshift Evolution of Satellites of Low-Mass Galaxies in the COSMOS Survey
• Inflation in generalized unimodular gravity
• A multi-tracer empirically-driven approach to line-intensity mapping lightcones
• Dissipative dark matter halos: The steady state solution
• Stealth decaying spin-1 dark matter
• Rotation of the CMB polarisation by foreground lensing
• Cosmologically viable generalized Einstein-Aether theories
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs -- II. The catalogue
• Static-Fluid Black Holes
• CMB Lens Sample Covariance and Consistency Relations
• Evolutions and Calibrations of Long Gamma-Ray Bursts Luminosity Correlations Revisited
• Application of the third RIT binary black hole simulations catalog to parameter estimation of gravitational waves signals from the LIGO-Virgo O1/O2 observational runs
• Generalized Brans-Dicke theories in light of evolving dark energy
• Extracting high-order cosmological information in galaxy surveys with power spectra
• A partial inventory of observational anisotropies in single-dish line-intensity mapping
• Evaluating hydrodynamical simulations with green valley galaxies
• Investigating Clumpy Galaxies in the Sloan Digital Sky Survey Stripe 82 using the Galaxy Zoo
• Targeted modeling of GW150914's binary black hole source with dart_board
• Imprint of non-linear effects on HI intensity mapping on large scales
• Perfect fluids with $\omega =\mathrm{const}$ as sources of scalar cosmological perturbations
• The redshift dependence of Alcock-Paczynski effect: cosmological constraints from the current and next generation observations
• Intermittent fragmentation and statistical variations during gas collapse in magnetised atomic cooling haloes
• Uranium Abundances and Ages of $R$-process Enhanced Stars with Novel U II Lines
• Replacing dark energy by silent virialisation
• Dark matter and electroweak phase transition in the mixed scalar dark matter model
• Search for Semi-Annihilating Dark Matter with Fermi-LAT, H.E.S.S., Planck, and the Cherenkov Telescope Array
• Weak scale from Planck scale -- Mass Scale Generation in Classically Conformal Two Scalar System --
• Foreground effect on the $J$-factor estimation of ultra-faint dwarf spheroidal galaxies
• Astronomical random numbers for quantum foundations experiments
• Spatially resolved analysis of Superluminous Supernovae PTF~11hrq and PTF~12dam host galaxies
• A single parameterization for dark energy and modified gravity models
• Prospects of detecting soft X-ray emission from typical WHIM filaments around massive clusters and the Coma cluster soft excess
• Measuring the HI mass function below the detection threshold
• Lensing covariance on cut sky and SPT-Planck lensing tensions
• The interstellar medium of high-redshift galaxies: Gathering clues from C III] and [C II] lines
• Implications of the $z>5$ Lyman-$\alpha$ forest for the 21-cm power spectrum from the epoch of reionization
• The Integrated Sachs-Wolfe Effect in Interacting Dark Matter-Dark Energy Models
• Horizon thermodynamics in holographic cosmological models with a power-law term
• The satellite galaxy plane of NGC 4490 in light of ΛCDM - Sparsity of similarly extreme analogs and a possible role of satellite pairs
• Tidally induced velocity gradients in the Milky Way dwarf spheroidal satellites
• Braneworld inflation with effective α-attractor potential
• Downsizing of Star Formation Measured from the Clustered Infrared Background Correlated with Quasars
• Characterising the Structure of Halo Merger Trees Using a Single Parameter: The Tree Entropy
• Tentative Detection of the Circumgalactic Medium of the Isolated Low-Mass Dwarf Galaxy WLM
• Using galaxy pairs to investigate the three-point correlation function in the squeezed limit
• Particle decay in post inflationary cosmology
• Extragalactic Observatory Science with the ASTRI Mini-Array at the Observatorio del Teide
• Unveiling the warm dense ISM in $z>6$ quasar host galaxies via water vapor emission
• Precise Mass Determination of SPT-CL J2106-5844, the Most Massive Cluster at z>1
• Horndeski dark matter and beyond
• Estimates for the impact of Ultraviolet Background fluctuations on galaxy clustering measurements
• The outermost edges of the Milky Way halo from galaxy kinematics
• Observable Primordial Gravitational Waves from Non-minimally Coupled $R^2$ Palatini Modified Gravity
• AXES-SDSS: comparison of SDSS galaxy groups with all-sky X-ray extended sources
• Is the star formation rate in $z\sim 6$ quasars overestimated?
• Strong-lensing source reconstruction with variationally optimised Gaussian processes
• Loop induced type-II seesaw model and GeV dark matter with $U(1{)}_{B-L}$ gauge symmetry
• The Sejong Suite: Cosmological Hydrodynamical Simulations with Massive Neutrinos, Dark Radiation, and Warm Dark Matter
• Dwarf galaxies as a probe of a primordially magnetized Universe
• On the gravitational lensing interpretation of three gravitational wave detections in the mass gap by LIGO and Virgo
• Gravitational instability with a dark matter background: Exploring the different scenarios
• Tomography of flavoured leptogenesis with primordial blue gravitational waves
• A VLT/MUSE galaxy survey towards QSO Q1410: looking for a WHIM traced by BLAs in inter-cluster filaments
• Dark Matter Halo Sparsity of Modified Gravity Scenarios
• Cosmic Voids in Evolving Dark Sector Cosmologies: the Low Redshift Universe
• Cosmic strings and other topological defects in nonscaling regimes
• A search for gamma-ray prompt emission associated with the Lorimer Burst FRB010724
• Optical validation and characterization of \Planck\ PSZ2 sources at the Canary Islands observatories. I. First year of LP15 observations
• Imprint of thawing scalar fields on large scale galaxy overdensity
• Compact groups from semi-analytical models of galaxy formation -- III: purity and completeness of Hickson-like catalogues
• Mock HUBS observations of hot gas with IllustrisTNG
• Supergravity Models with 50-100 TeV Scalars, SUSY Discovery at the LHC and Gravitino Decay Constraints
• Panning for gold, but finding helium: discovery of the ultra-stripped supernova SN2019wxt from gravitational-wave follow-up observations
• The OTELO survey: Nature and mass-metallicity relation for H$\alpha$ emitters at $z\sim 0.4$
• Constraining CMB temperature evolution with Sunyaev-Zel'dovich galaxy clusters from the Atacama Cosmology Telescope
• RAiSE X: searching for radio galaxies in X-ray surveys
• Observational status of the Galileon model general solution from cosmological data and gravitational waves
• Perfectly parallel cosmological simulations using spatial comoving Lagrangian acceleration
• Cosmological constraints on the velocity-dependent baryon-dark matter coupling
• A multi-frequency study of sub-parsec jets with the Event Horizon Telescope
• Forecast and analysis of the cosmological redshift drift
• The impact of stellar bars on star-formation quenching: Insights from a spatially resolved analysis in the local Universe
• Ly$\alpha$ forest power spectrum as an emerging window into the epoch of reionization and cosmic dawn
• FIRST J153350.8+272729: the radio afterglow of a decades-old tidal disruption event
• Impact of dark matter spikes on the merger rates of Primordial Black Holes
• Calibrating gravitational-wave detectors with GW170817
• Hardness of ionizing radiation fields in MaNGA star-forming galaxies
• One-loop radiative seesaw dark matter and neutrinoless double beta decay with two zero flavor neutrino mass texture
• Local probes strongly favor $\Lambda$CDM against power-law and $R_h=ct$ universe
• Radio Power from Direct-Collapse Black Holes
• Evolution of central galaxy alignments in simulations
• Light or heavy supermassive black hole seeds: the role of internal rotation in the fate of supermassive stars
• Superconformal Subcritical Hybrid Inflation
• Enhanced neutrino emissivities in pseudoscalar-mediated Dark Matter annihilation in Neutron Stars
• Impact of generalized dissipative coefficient on warm inflationary dynamics in the light of latest Planck data
• Narrowing the window of inflationary magnetogenesis
• Cosmology and prospects for sub-MeV dark matter in electron recoil experiments
• Analysis method for 3D power spectrum of projected tensor field with fast estimator and window convolution modelling: an application to intrinsic alignments
• Screening corrections to Electron Capture Rates and resulting constraints on Primordial Magnetic Fields
• Phase transitions and entropy force of charged de Sitter black holes with cloud of string and quintessence
• The cosmic transparency measured with Type Ia supernovae: implications for intergalactic dust
• Scalar field dark matter in hybrid approach
• Forecasting cosmic acceleration measurements using the Lyman-$\alpha$ forest
• Search for high-energy neutrinos in coincidence with Fast Radio Bursts with the ANTARES neutrino telescope
• Down-the-barrel observations of a multiphase quasar outflow at high redshift: VLT/X-shooter spectroscopy of the proximate molecular absorber at z=2.631 towards SDSS J001514+184212
• The role of environment in galaxy evolution in the SERVS Survey I: density maps and cluster candidates
• Compact groups from semi-analytical models of galaxy formation -- I: a comparative study of frequency and nature
• Towards determining the neutrino mass hierarchy: weak lensing and galaxy clustering forecasts with baryons and intrinsic alignments
• HOLISMOKES -- XI. Evaluation of supervised neural networks for strong-lens searches in ground-based imaging surveys
• Deforming the Starobinsky model in ghost-free higher derivative supergravities
• Cosmic evolution of the H2 mass density and the epoch of molecular gas
• The VANDELS Survey: New constraints on the high-mass X-ray binary populations in normal star-forming galaxies at 3 < z < 5.5
• Measuring the Duration of Last Scattering
• The Hubble tension: Change in dark energy or a case for modified gravity?
• Inflation by spin and torsion in Poincare gauge theory of gravity
• The Two Body Problem in the Presence of Dark Energy and Modified Gravity: Application to the Local Group
• Leptophilic Composite Asymmetric Dark Matter and its Detection
• Can invisible objects be `seen' via forward proton detectors at the LHC?
• A joint 2- and 3-point clustering analysis of the VIPERS PDR2 catalogue at z~1: breaking the degeneracy of cosmological parameters
• The ISW effect and the lack of large-angle CMB temperature correlations
• On the cosmic distance duality relation and the strong gravitational lens power law density profile
• $\alpha$-attractor-type Double Inflation
• Was there an early reionization component in our universe?
• The Structural Evolution of Isolated Galaxies at Low Redshift in the IllustrisTNG Simulation
• Unveiling the main sequence of galaxies at $z\ge 5$ with the James Webb Space Telescope: predictions from simulations
• The environment of radio galaxies: A signature of AGN feedback at high redshifts
• Testing cosmic opacity with the combination of strongly lensed and unlensed supernova Ia
• Discovery of a [CI]-faint, CO-bright Galaxy: ALMA Observations of the Merging Galaxy NGC 6052
• CMB B-mode auto-bispectrum produced by primordial gravitational waves
• Detection of WHIM in the Planck data using Stack First approach
• A too-many dwarf satellite galaxies problem in the MATLAS low-to-moderate density fields
• Exploring compensated isocurvature perturbations with CMB spectral distortion anisotropies
• Triplet Leptogenesis, Type-II Seesaw Dominance, Intrinsic Dark Matter, Vacuum Stability and Proton Decay in Minimal SO(10) Breakings
• Impact of Massive Neutrinos and Dark Radiation on the High-redshift Cosmic Web. I. Lyman-Alpha Forest Observables
• New Physics Search at the CEPC: a General Perspective
• The classical and quantum fate of the Little Sibling of the Big Rip in $f(R)$ cosmology
• How much primordial tensor mode is allowed?
• Unveiling the largest structures in the nearby Universe: Discovery of the Quipu superstructure
• New non-singular cosmological solution of non-local gravity
• The Sommerfeld Enhancement in the Scotogenic Model with Large Electroweak Scalar Multiplets
• Detection of LIGO-Virgo binary black holes in the pair-instability mass gap
• Barbell-shaped giant radio galaxy with ~100 kpc kink in the jet
• A Multi-Wavelength Study of Multiple Spectral Component Jets in AGN: Testing the IC/CMB Model for the Large-Scale-Jet X-ray Emission
• Nonlinear spherical perturbations in Quintessence Models of Dark Energy
• Improved calculation of the gravitational wave spectrum from kinks on infinite cosmic strings
• Gravitational wave from warm inflation
• BAO Modulation as a Probe of Compensated Isocurvature Perturbations
• Na-based crystal scintillators for next-generation rare event searches
• The Northern Cross Fast Radio Burst project IV. Multi-wavelength study of the actively repeating FRB 20220912A
• Maximal CP Violation in Minimal Seesaw Model
• MIND THE GAP: Is The Too Big To Fail Problem Resolved?
• Testing General Relativity with the Doppler magnification effect
• The evolution of cosmic ray electrons in the cosmic web: seeding by AGN, star formation and shocks
• Marginalized Fisher Forecast for Horndeski Dark Energy Models
• Quasi Yukawa Unification and Fine-Tuning in U(1) Extended SSM
• Tachyon with an inverse power-law potential in a braneworld cosmology
• Stellar Feedback and the Energy Budget of Late-Type Galaxies: Missing Baryons and Core Creation
• Beyond optical depth: Future determination of ionization history from the CMB
• COSMOS-Web: The emergence of the Hubble Sequence
• $f(T)$ cosmology in the regime of quasar observations
• Cosmological histories in bimetric gravity: A graphical approach
• Exploring the CPT violation and birefringence of gravitational waves with ground- and space-based gravitational-wave interferometers
• Hybrid seesaw leptogenesis and TeV singlets
• Model-Independent Predictions for Smooth Cosmic Acceleration Scenarios
• Multi wavelength cross-correlation analysis of the simulated cosmic web
• Dynamical analysis in regularized $4D$ Einstein-Gauss-Bonnet gravity with non-minimal coupling
• Fuzzy Aquarius: evolution of a Milky-way like system in the Fuzzy Dark Matter scenario
• How the Galaxy-Halo Connection Depends on Large-Scale Environment
• No evidence for the evolution of mass density power-law index $\gamma$ from strong gravitational lensing observation
• Observing the dark sector
• Exploring vector-like supersymmetric extensions of the Standard Model with dark matter and colliders
• Cosmology with Galaxy Cluster Phase Spaces
• The ACCEL2 Project: Precision Measurements of EFT Parameters and BAO Peak Shifts for the Lyman-$\alpha$ Forest
• The cross-correlation of galaxies in absorption with the Lyman $\alpha$ forest
• Baryon asymmetry via leptogenesis in a neutrino mass model with complex scaling
• LoTSS/HETDEX: Disentangling star formation and AGN activity in gravitationally-lensed radio-quiet quasars
• Searching for gravitationally lensed gamma-ray bursts with their afterglows
• Using Gravitational Wave Parallax to Measure the Hubble Parameter with Pulsar Timing Arrays
• Probing Gravitational Lensing of the CMB with SDSS-IV Quasars
• ISiTGR: Testing deviations from GR at cosmological scales including dynamical dark energy, massive neutrinos, functional or binned parametrizations, and spatial curvature
• Coherent two-photon emission from hydrogen molecules excited by counter-propagating laser pulses
• Texture zeros of low-energy Majorana neutrino mass matrix in 3+1 scheme
• Giant Primeval Magnetic Dipoles
• Timescales for Hi consumption and SFR depletion of satellite galaxies in groups
• Role of magnetic fields in the formation of direct collapse black holes
• Baryonic Imprints on DM Halos: The concentration-mass relation in the CAMELS simulations
• Consistency relations in multi-field inflation
• Integrated cosmological probes: Concordance quantified
• The matter-ekpyrotic bounce scenario in Loop Quantum Cosmology
• Clustering in the Simulated H$\alpha$ Galaxy Redshift Survey from Nancy Grace Roman Space Telescope
• Measuring the Energy Scale of Inflation with Large Scale Structures
• Permanent Electric Dipole Moments of Single-, Two-, and Three-Nucleon Systems
• Scalar-tensor cosmologies without screening
• Detailed multi-wavelength modelling of the dark GRB 140713A and its host galaxy
• Evaluating the Merger Rate of Binary Black Holes from Direct Captures and Third-Body Soft Interactions Using the Milky Way Globular Clusters
• Void Galaxy Distribution: A Challenge for $\Lambda$CDM
• Gauging Fine-Tuning
• Ultra High Energy Cosmic Rays & Super-heavy Dark Matter
• Model-independent way to determine the Hubble constant and the curvature from phase shift of gravitational waves with DECIGO
• Effects of dark matter in star formation
• Excess of lensing amplitude in the Planck CMB power spectrum
• Finding structure in the dark: coupled dark energy, weak lensing, and the mildly nonlinear regime
• Constraining dynamical neutrino mass generation with cosmological data
• DE models with combined $H_0\cdot r_d$ from BAO and CMB dataset and friends
• Measurement of the small-scale 3D Lyman-$\alpha$ forest power spectrum
• Source structure and molecular gas properties from high-resolution CO imaging of SPT-selected dusty star-forming galaxies
• The ages of (the oldest) stars
• Hubble Constant from LSST Strong lens time delays with microlensing systematics
• The Stellar Mass Assembly of Low Redshift, Massive, Central Galaxies in SDSS and the TNG300 simulation
• Galaxy clustering from the bottom up: A Streaming Model emulator I
• Constraining power of open likelihoods, made prior-independent
• Extremely Massive Quasars are not Good Proxies for Dense Environments Compared to Massive Galaxies: Environments of Extremely Massive Quasars and Galaxies
• Sub-GeV Dark Matter Shining at Future MeV Gamma-Ray Telescopes
• Halo Scaling Relations and Hydrostatic Mass Bias in the Simba Simulation From Realistic Mock X-ray Catalogues
• Search and analysis of giant radio galaxies with associated nuclei (SAGAN) V. Study of giant double-double radio galaxies from LoTSS DR2
• Constraining the AGN formation channel for detected black hole binary mergers up to z=1.5 with the Quaia catalogue
• Efficient and accurate force replay in cosmological-baryonic simulations
• Uneven flows: On cosmic bulk flows, local observers, and gravity
• SHAMe-SF: Predicting the clustering of star-forming galaxies with an enhanced abundance matching model
• The SRG/eROSITA all-sky survey. X-ray emission from the warm-hot phase gas in long cosmic filaments
• Standardizing the Gamma-ray burst as a standard candle and applying to the cosmological probes: constraints on the two-component dark energy model
• Observational constrained Weyl type $f(Q,T)$ gravity cosmological model and the dynamical system analysis
• Constraining the history of reheating with the NANOGrav 15-year data
• Structure Formation in Various Dynamical Dark Energy Scenarios
• Anisotropic Massive Gauge-flation
• Constraining the emergent dark energy models with observational data at intermediate redshift
• Faint Dark Matter Annihilation Signals and the Milky Way's Supermassive Black Hole
• LHC Signatures of WIMP-triggered Baryogenesis
• Pseudo-Evolution of Galaxies in LCDM Cosmology
• Reexamination of the warm inflation curvature perturbations spectrum
• An Hamilton-Jacobi formulation of anisotropic inflation
• Baryogenesis From Flavon Decays
• Robustness of the pairwise kinematic Sunyaev-Zeldovich power spectrum shape as a cosmological gravity probe
• Excited cosmic strings with superconducting currents
• Three Dusty Star Forming Galaxies at $z\sim 1.5$: Mergers and Disks on the Main Sequence
• QCD axions and axionlike particles in a two-inflation scenario
• Non-sphericity of ultralight axion dark matter haloes in the Galactic dwarf spheroidal galaxies
• Constraining the delay time distribution of compact binary objects from the stochastic gravitational wave background searches
• Forecasts of cosmological constraints from HI intensity mapping with FAST, BINGO & SKA-I
• Cosmological Constraints on Scalar Field Dark Matter
• Observing Correlations Between Dark Matter Accretion and Galaxy Growth: I. Recent Star Formation Activity in Isolated Milky Way-Mass Galaxies
• Leptogenesis due to oscillating Higgs field
• The eccentricity enhancement effect of intermediate-mass-ratio-inspirals: dark matter and black hole mass
• Cosmic backreaction and Gauss's law
• Ionized Gas Kinematics around an Ultra-luminous X-ray Source in NGC 5252 : Additional Evidence for an Off-nuclear AGN
• Constraints on interacting dynamical dark energy and a new test for $\Lambda$CDM
• Low-$\ell$ power suppression in punctuated inflation
• Spin characterisation of systematics in CMB surveys -- a comprehensive formalism
• Coherence and mixedness of neutrino oscillations in a magnetic field
• Neutrino masses and lepton mixing from $A_5\times \mathrm{CP}$
• The Shape of Bouncing Universes
• Voids and Superstructures: correlations and induced large-scale velocity flows
• The radial acceleration relation and dark baryons in MOND
• On the dust properties of high redshift molecular clouds and the connection to the 2175 Å extinction bump
• Search for dark matter in events with a leptoquark and missing transverse momentum in proton-proton collisions at 13 TeV
• Kinetic Inductance Detectors and readout electronics for the OLIMPO experiment
• Clustering of CODEX clusters
• Nonlocal Entanglement and Directional Correlations of Primordial Perturbations on the Inflationary Horizon
• Qualitative description of the universe in the interacting fluids scheme
• Triggering the formation of direct collapse black holes by their congeners
• How Decoherence Affects the Probability of Slow-Roll Eternal Inflation
• Dynamical Screening Effects on Big Bang Nucleosynthesis
• The OTELO survey. III. Demography, morphology, IR luminosity and environment of AGN hosts
• Primordial gravitational wave phenomenology with polarized Sunyaev Zel'dovich tomography
• 3C 17: The BCG of a galaxy cluster at z=0.22
• Projected distances to host galaxy reduce SNIa dispersion
• Instability of Higgs Vacuum via String Cloud
• Parsec-scale properties of the peculiar gigahertz-peaked spectrum quasar 0858-279
• Empirical inference on the Majorana mass of the ordinary neutrinos
• A tale of two tails: insights from simulations into the formation of the peculiar dwarf galaxy NGC 1427A
• Quenching, Mergers and Age Profiles for z=2 Galaxies in IllustrisTNG
• Constraining density and metallicity of the Milky Way's hot gas halo from O VII spectra and ram-pressure stripping
• Assessment of the Systematic Uncertainties in the Cosmological Analysis of the SDSS Supernovae Photometric Sample
• Post-Newtonian parameter $\gamma$ and the deflection of light in ghost-free massive bimetric gravity
• Over-density of SMGs in fields containing z~0.3 galaxies: magnification bias and the implications for studies of galaxy evolution
• On the absence of backsplash analogues to NGC 3109 in the $\Lambda$CDM framework
• A high coverage view of the thermodynamics and metal abundance in the outskirts of the nearby galaxy cluster Abell 2199
• An Orientation Bias in Observations of Submillimetre Galaxies
• Towards Searching for Entangled Photons in the CMB Sky
• Multileptonic signals of co-annihilating left-right supersymmetric dark matter
• Impact of the latest measurement of Hubble constant on constraining inflation models
• Geodesic Congruences and a Collapsing Stellar Distribution in f (T ) Theories
• Assessing non-linear models for galaxy clustering II: model validation and forecasts for Stage IV surveys
• A Monte Carlo approach to magnetar-powered transients: II. Broad-lined type Ic supernovae not associated with GRBs
• Filament Hunting: Integrated HI 21cm Emission From Filaments Inferred by Galaxy Surveys
• Imprint of a Steep Equation of State in the growth of structure
• Compact groups from semi-analytical models of galaxy formation -- II: Different assembly channels
• Detection of an ionized gas outflow in the extreme UV-luminous star-forming galaxy BOSS-EUVLG1 at z=2.47
• Optimally Mapping Large-Scale Structures with Luminous Sources
• Galaxy And Mass Assembly: Group and field galaxy morphologies in the star-formation rate - stellar mass plane
• Black hole mass and spin estimates of the most distant quasars
• An Optical Observational Cluster Mass Function at $z\sim 1$ with the ORELSE Survey
• Common Origin of Non-zero ${\theta }_{13}$ and Dark Matter in an $S_4$ Flavour Symmetric Model with Inverse Seesaw
• Search for gamma-ray emission from the 12 nearby dwarf spheroidal galaxies with 12 years of Fermi-LAT data
• The definition of mass in asymptotically de Sitter space-times
• PS J1721+8842: A gravitationally lensed dual AGN system at redshift 2.37 with two radio components
• Technically natural Higgs boson from Planck scale
• Properties of globular clusters formed in dark matter mini-halos
• Predictions for the sky-averaged depth of the 21cm absorption signal at high redshift in cosmologies with and without non-baryonic cold dark matter
• Testing isotropy in the Two Micron All-Sky redshift survey with information entropy
• The minimum magnetic field of millisecond pulsars calculated according to accretion: application to the X-ray neutron star SAX J1808.4-3658 in a low-mass X-ray binary
• Inducing Gravity From Connections and Scalar Fields
• Limits on Dark Matter annihilation cross sections to gamma-ray lines with subhalo distribution in N-body simulation and Fermi LAT data
• Some Recent Results on Ricci-Based Gravity Theories
• Milli-charged fermion vacuum polarization in cosmic magnetic fields and generation of CMB elliptic polarization
• The Column Densities of Molecular Gas across Cosmic Time: Bridging Observations and Simulations
• Constraining low redshift [CII] Emission by Cross-Correlating FIRAS and BOSS Data
• Reionization in the dark and the light from Cosmic Microwave Background
• Joint constraints on reionization: a framework for combining the global 21cm signal and the kinetic Sunyaev-Zel'dovich effect
• Observational constraints on the fractal cosmology
• Optimal cosmic microwave background map-making in the presence of cross-correlated noise
• Cosmic Voids in Evolving Dark Sector Cosmologies: the High Redshift Universe
• The Supersymmetric R-Parity Violating Dine-Fischler-Srednicki-Zhitnitsky Axion Model
• ALMACAL VIII: A pilot survey for untargeted extragalactic CO emission lines in deep ALMA calibration data
• Dark matter cores in massive high-$z$ galaxies formed by baryonic clumps
• The local dark sector. Probing gravitation's low-acceleration frontier and dark matter in the Solar System neighborhood
• Reionization time of the Local Group and Local-Group-like halo pairs
• Eternal inflation and the quantum birth of cosmic structure
• X-ray spectral variations of synchrotron peak in BL Lacs
• The Long and the Short of It: The Benefits and Leverage of Ultraviolet-Radio Galaxy Fitting
• The Physical Nature of Circumgalactic Medium Absorbers in Simba
• Impact of radio sources and cosmic infrared background on thermal Sunyaev-Zel'dovich - gravitational lensing cross correlation
• Throwing away antimatter via neutrino oscillations during the reheating era
• Detection of a Super-Virial Hot Component in the Milky Way Circumgalactic Medium Along Multiple Sight-Lines by Using the Stacking Technique
• Disk flaring with TNG50: diversity across Milky Way and M31 analogs
• The Unusual Milky Way-Local Sheet System: Implications for Spin Strength and Alignment
• Testing the growth rate in homogeneous and inhomogeneous interacting vacuum models
• Matching the mass function of Milky Way satellites in competing dark matter models
• A Search for Neutrino Point-Source Populations in 7 Years of IceCube Data with Neutrino-count Statistics
• Minimal model dependent constraints on cosmological nuisance parameters and cosmic curvature from combinations of cosmological data
• Searches for New Particles Including Dark Matter with Atomic, Molecular and Optical Systems
• Lyman-alpha Emitters in Ionized Bubbles: Constraining the Environment and Ionized Fraction
• Recoiling Supermassive Black Hole Escape Velocities from Dark Matter Halos
• The RATAN-600 multi-frequency catalogue of blazars -- BLcat
• MeerKAT follow-up of enigmatic GLEAM 4-Jy (G4Jy) sources
• How accurately can we measure the baryon acoustic oscillation feature?
• Calibrating Long Period Variables as Standard Candles with Machine Learning
• Deep Synoptic Array Science: Implications of Faraday Rotation Measures of Localized Fast Radio Bursts
• Exploring the Cosmological Model in $f(R,T^{\varphi })$ Gravity with Observational Constraints
• Effect of a High-Precision Semi-Analytical Mass Function on the Merger Rate of Primordial Black Holes in Dark Matter Halos
• Decaying axinolike dark matter: Discriminative solution to small-scale issues
• MeV to multi-TeV thermal WIMPs: most conservative limits
• Observational implications of cosmologically coupled black holes
• Cosmology with the Square Kilometre Array by SKA-Japan
• Axion dark matter and the Lattice
• Constraining Chameleon screening using galaxy cluster dynamics
• Shining Light on the Mass Scale and Nature of Neutrinos with $e\gamma \to e\nu \overline{\nu }$
• Radio Emission from the First Quasars at $z\sim$ 6-15
• A catalogue of faint local radio AGN and the properties of their host galaxies
• Structure Formation in Nonlocal MOND
• Stellar mass dependence of the 21-cm signal around the first star and its impact on the global signal
• Quantifying the abundance of faint, low-redshift satellite galaxies in the COSMOS survey
• Non-Gaussianities in a two-field generalization of Natural Inflation
• Testing the nature of Dark Energy with Precision Cosmological constraints
• A radiative seesaw model with higher order terms under an alternative $U(1{)}_{B-L}$
• Testing the dark matter subhalo hypothesis of the gamma-ray source 3FGL J2212.5+0703
• An Analytic Formulation of 21-cm Signal from Early Phase of Epoch of Reionization
• FORECAST: a flexible software to forward model cosmological hydrodynamical simulations mimicking real observations
• Constraining the reionization history with CMB and spectroscopic observations
• Non-minimal coupling influence on the deviation from de Sitter cosmological expansion
• Forecasting the power of Higher Order Weak Lensing Statistics with automatically differentiable simulations
• Dark matter halos in the multicomponent model. II. Density profiles of galactic halos
• Redshift-space distortions from vector perturbations
• Low-Scale Seesaw and the CP Violation in Neutrino Oscillations
• Gravitational waves from strong first order phase transitions
• Fuzzy Dark Matter in Relativistic Stars
• Toward a Physical Understanding of Galaxy-Halo Alignment
• Shaping the Milky Way: The interplay of mergers and cosmic filaments
• Recent progress in simulating galaxy formation from the largest to the smallest scales
• HI within and around observed and simulated galaxy discs -- Comparing MeerKAT observations with mock data from TNG50 and FIRE-2
• Probing the Supersymmetry-Mass Scale With F-term Hybrid Inflation
• Massive black hole formation in Population III star clusters
• Discovery of large-scale diffuse radio emission in low-mass galaxy cluster Abell 1931
• Simplified dark matter models with loop effects in direct detection and the constraints from indirect detection and collider search
• First constraints on non-minimally coupled Natural and Coleman-Weinberg inflation and massive neutrino self-interactions with Planck+BICEP/Keck
• Constraints on brane inflation after Planck 2015: Impacts of the latest local measurement of the Hubble constant
• Galaxy formation physics behind bar formation: A view from cosmological hydrodynamical simulations
• Direct Detection of Ultralight Dark Matter via Astronomical Ephemeris
• Dynamic analysis of noncanonical warm inflation
• The Impact of Primordial Magnetic Fields on Future CMB Bounds on Inflationary Gravitational Waves
• `Upper-Limit Lensing': Constraining galaxy stellar masses with singly-imaged background sources
• Imitating intrinsic alignments: A bias to the CMB lensing-galaxy shape cross-correlation power spectrum induced by the large-scale structure bispectrum
• Mathematical Underpinnings of the Multi-Wavelength Structure of the TRGB
• Local fragmentation of thin disks in Eddington-inspired gravity
• What's in a binary black hole's mass parameter?
• The impact of theoretical assumptions in the determination of the neutrino effective number from future CMB measurements
• Validating the methodology for constraining the linear growth rate from clustering anisotropies
• Sunyaev-Zel'dovich Signal from Quasar Hosts: Implications for Detection of Quasar Feedback
• Spacetime Deformation Effect on the Early Universe and the PTOLEMY Experiment
• A catalog of optical to X-ray spectral energy distributions of z~2 quasars observed with Swift. I: First results
• Weak gravity on a $\Lambda$CDM background
• Energy stored on a cosmological horizon and its thermodynamic fluctuations in holographic equipartition law
• Surface Tension of Cosmic Voids as a Possible Source for Dark Energy
• The high-redshift Universe with Spitzer
• Dark-ages reionization and galaxy formation simulation XI: Clustering and halo masses of high redshift galaxies
• High-fidelity reproduction of central galaxy joint distributions with Neural Networks
• Search for lensing signatures in the gravitational-wave observations from the first half of LIGO-Virgo's third observing run
• Flux-density measurements of the high-redshift blazar PSO J047.4478+27.2992 at 4.7 and 8.2 GHz with RATAN-600
• Size and Spectroscopic Evolution of HectoMAP Quiescent Galaxies
• Fisher matrix for multiple tracers: model independent constraints on the redshift distortion parameter
• MAHGIC: A Model Adapter for the Halo-Galaxy Inter-Connection
• HI Deficiencies and Asymmetries in HIPASS Galaxies
• Two-component millicharged dark matter and the EDGES 21cm signal
• Study on the magnetic field strength of NGC 300 ULX1
• Constraining Cosmological Parameters using the Cluster Mass-Richness Relation
• Optical follow-up study of 32 high-redshift galaxy cluster candidates from Planck with the William Herschel Telescope
• A Novel CMB Component Separation Method: Hierarchical Generalized Morphological Component Analysis
• Dissipative Unified Dark Fluid Model
• The Uchuu-GLAM BOSS and eBOSS LRG lightcones: Exploring clustering and covariance errors
• $\mathcal{O}(10)M_{\odot }$ primordial black holes and string axion dark matter
• Search for gamma-ray emission from the nearby dwarf spheroidal galaxies with 9 years of Fermi-LAT data
• Developing a unified pipeline for large-scale structure data analysis with angular power spectra -- III. Implementing the multi-tracer technique to constrain neutrino masses
• An Effective Field Theory Analysis of the First LUX Dark Matter Search
• Theoretical study of an LAE-CIV absorption pair at z = 5.7
• Baryogenesis through Asymmetric Hawking Radiation from Primordial Black Holes as Dark Matter
• de Sitter Harmonies: Cosmological Spacetimes as Resonances
• Decoding Long-duration Gravitational Waves from Binary Neutron Stars with Machine Learning: Parameter Estimation and Equations of State
• Constraining the impact of standard model phase transitions on primordial black holes
• Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR
• Hubble-rate-dependent Dark Energy in Brans-Dicke Cosmology
• Circular polarization of cosmic photons due to their interactions with Sterile neutrino dark matter
• Cosmological N-body simulations with generic hot dark matter
• The Fermi-LAT view of the changing-look blazar OQ 334
• The effect of inhomogeneities on dark energy constraints
• Numerical simulations of dark matter haloes produce polytropic central cores when reaching thermodynamic equilibrium
• One-loop quantum gravitational backreaction on the local Hubble rate
• JWST/NIRSpec and MIRI observations of an expanding, jet-driven bubble of warm H${}_2$ in the radio galaxy 3C 326 N
• Constraining the star formation rate with the extragalactic background light
• $f(\bar{R},L(X))$-gravity in the context of dark energy with power law expansion and energy conditions
• Conformal gravity: light deflection revisited and the galactic rotation curve failure
• Mock Observations: Formation and Evolution of diffuse light in Galaxy Groups and Clusters in the IllustrisTNG Simulations
• Effect of observational holes in fractal analysis of galaxy survey masks
• Implications of GWTC-3 on primordial black holes from vacuum bubbles
• The background Friedmannian Hubble constant in relativistic inhomogeneous cosmology and the age of the Universe
• Light vector dark matter with scalar mediator and muon g-2 anomaly
• Painting baryons onto N-body simulations of galaxy clusters with image-to-image deep learning
• The 1/c expansion of nonminimally coupled curvature-matter gravity model and constraints from planetary precession
• A modified Friedmann equation for a system with varying gravitational mass
• Simulations for 21 cm radiation lensing at EoR redshifts
• Revision of Faraday rotation measure constraints on the primordial magnetic field using the IllustrisTNG simulation
• Still alive and kicking: A significant outburst in changing-look AGN Mrk 1018
• The kinematic Sunyaev-Zel'dovich effect of the large-scale structure (II): the effect of modified gravity
• High scale boundary conditions with an additional complex singlet
• Viscous Cosmologies
• Deformation of Axion Potentials: Implications for Spontaneous Baryogenesis, Dark Matter, and Isocurvature Perturbations
• The environmental monitoring system at the COSINE-100 experiment
• Not Hydro: Using Neural Networks to estimate galaxy properties on a Dark-Matter-Only simulation
• Joint cosmology and mass calibration from tSZ cluster counts and cosmic shear
• Supermassive black hole seeds from sub-keV dark matter
• Linear Density Perturbations in Multifield Coupled Quintessence
• Neutrino phenomenology in the flavored NMSSM without domain wall problems
• Testing the paradigm: First spectroscopic evidence of a quasar-galaxy Mpc-scale association at cosmic dawn
• Exploring the thermal energy contents of the intergalactic medium with the Sunyaev-Zel'dovich effect
• The Massive and Distant Clusters of WISE Survey IX: High Radio Activity in a Merging Cluster
• Asymmetric dark matter with a possible Bose-Einstein condensate
• Alternative $[SU(3){]}^4$ Model of Leptonic Color and Dark Matter
• A new probe of magnetic fields in the pre-reionization epoch: II. Detectability
• $f(T,B)$ gravity in a Friedmann-Lema\^ıtre-Robertson-Walker universe with nonzero spatial curvature
• Parametrized tests of general relativity using eccentric compact binaries
• The anisotropy of the power spectrum in periodic cosmological simulations
• Galaxy Clustering in the Mira-Titan Universe I: Emulators for the redshift space galaxy correlation function and galaxy-galaxy lensing
• On the Prospects for Detecting a Net Photon Circular Polarization Produced by Decaying Dark Matter
• Quantum computational complexity, Einstein's equations and accelerated expansion of the Universe
• Constraints on ${\tau }_{\mathrm{NL}}$ from Planck temperature and polarization
• Testing the $R_{\mathrm{h}}=ct$ Universe Jointly with the Redshift-dependent Expansion rate and Angular-diameter and Luminosity Distances
• Precise predictions for Dirac neutrino mixing
• Signatures of Massive Black Hole Merger Host Galaxies from Cosmological Simulations I: Unique Galaxy Morphologies in Imaging
• Detection of Einstein Telescope gravitational wave signals from binary black holes using deep learning
• Asteroseismic Study of Subgiants and Giants of the Open Cluster M67 using Kepler/K2: Expanded Sample and Precise Masses
• Rhapsody-C simulations -- Anisotropic thermal conduction, black hole physics, and the robustness of massive galaxy cluster scaling relations
• Constraining Holographic Dark Energy and Analyzing Cosmological Tensions
• Weak Lensing Skew-Spectrum
• Living with Neighbors. III. The Origin of the Spin$-$Orbit Alignment of Galaxy Pairs: A Neighbor versus the Large-scale Structure
• Search for Light Dark Matter with NEWS-G at the Laboratoire Souterrain de Modane Using a Methane Target
• Exploring collider aspects of a neutrinophilic Higgs doublet model in multilepton channels
• Fast Sampling from Wiener Posteriors for Image Data with Dataflow Engines
• Three-point intrinsic alignments of dark matter halos in the IllustrisTNG simulation
• Detection of Cosmic Structures using the Bispectrum Phase. I. Mathematical Foundations
• Chandra follow up of the Hectospec Cluster Survey: Comparison of Caustic and Hydrostatic Masses and Constraints on the Hydrostatic Bias
• Production of gravitational waves during preheating in the Starobinsky inflationary model
• Emulating Sunyaev-Zeldovich Images of Galaxy Clusters using Auto-Encoders
• Qualitative classification of extraterrestrial civilizations
• Warm Higgs G-inflation: predictions and constraints from Planck 2015 likelihood
• Interferometric HI intensity mapping: perturbation theory predictions and foreground removal effects
• Neural network time-series classifiers for gravitational-wave searches in single-detector periods
• Study of QCD generalized ghost dark energy in FRW universe
• The Integrated Sachs-Wolfe Effect in the Bulk Viscous Dark Energy Model
• Cosmological constraints on $\gamma$-gravity models
• Current bounds on baryogenesis from complex Yukawa couplings of light fermions
• Redshift space distortions in the presence of non-minimally coupled dark matter
• Constraints on dark matter self-interaction from galactic core size
• Observationally constrained accelerating cosmological model with higher power of non-metricity and squared trace
• Quasar -- CIV forest cross-correlation with SDSS DR12
• Stochastic Metric Space and Quantum Mechanics
• Explaining low l anomalies in the CMB power spectrum with resonant superstring excitations during inflation
• Direct couplings of mimetic dark matter and their cosmological effects
• Testing MOG theory in the Milky Way
• Generalized $\alpha$-attractor models from elementary hyperbolic surfaces
• A matched-filter approach to radio variability and transients: searching for orphan afterglows in the VAST Pilot Survey
• Characterising abundance-age relations of GALAH stars using oxygen-enhanced stellar models
• Inhomogeneous Initial Data and Small-Field Inflation
• Gravity waves in parity-violating Copernican Universes
• The Beyond-Halo Mass Effects of the Cosmic Web Environment on Galaxies
• Late-formed halos prefer to host quiescent central galaxies. I. Observational results
• Soft X-ray emission from warm gas in IllustrisTNG circum-cluster environments
• Bottom-quark Forward-Backward Asymmetry, Dark Matter and the LHC
• Non-minimally coupled quintessence DE model with a cubic galileon term --A Dynamical System Analysis
• The little rip in classical and quantum $f(R)$ cosmology
• CONCERTO: Extracting the power spectrum of the [C II ] emission line
• Modeling iterative reconstruction and displacement field in the large scale structure
• $\mu -\tau$ Reflection Symmetry and Its Explicit Breaking for Leptogenesis in a Minimal Seesaw Model
• SU(2)${}_{\mathrm{CMB}}$ and the cosmological model: angular power spectra
• The cooler past of the intracluster medium in TNG-Cluster
• Precision cosmology with baryons: non-radiative hydrodynamics of galaxy groups
• Anisotropic Satellite Galaxy Quenching: A Unique Signature of Energetic Feedback by Supermassive Black Holes?
• Indirect effects of dark matter
• CLEAR: Spatially Resolved Emission Lines and Active Galactic Nuclei at $0.6<z<1.3$
• LMC-driven anisotropic boosts in stream--subhalo interactions
• Lepton Number Violation, Lepton Flavour Violation and Baryogenesis in Left-Right Symmetric Model
• Search for Light Dark Matter with 259-day data in PandaX-4T
• Tracking the orbit of unresolved subhalos for semi-analytic models
• Weak Lensing Measurement of Filamentary Structure with the SDSS BOSS and Subaru Hyper Suprime-Cam Data
• The Impact of Cosmic Variance on Inferences of Global Neutral Fraction Derived from Ly$\alpha$ Luminosity Functions During Reionization
• Gravitational baryogenesis without CPT violation
• Intrinsic Entropy Perturbations from the Dark Sector
• Renyi Holographic Dark Energy models in Teleparallel gravity
• Detection of ${}^7$Be II in the Small Magellanic Cloud
• Star-formation rates of two GRB host galaxies at z~2 and a [CII] deficit observed with ALMA
• The Early Light Curve of a Type Ia Supernova 2021hpr in NGC 3147: Progenitor Constraints with the Companion Interaction Model
• Probing flavored regimes of leptogenesis with gravitational waves from cosmic strings
• Coupled quintessence with a generalized interaction term
• Early Science with the Large Millimeter Telescope: a 1.1 mm AzTEC Survey of Red-$Herschel$ dusty star-forming galaxies
• Reconstructing Orbits of Galaxies in Extreme Regions (ROGER) II: reliability of projected phase-space in our understanding of galaxy populations
• Impact of Galaxy Mergers on Stellar Population Profiles of Early-type Galaxies
• Concordance between observations and simulations in the evolution of the mass relation between supermassive black holes and their host galaxies
• Development of dark disk model of positron anomaly origin
• Spin portal to dark matter
• Analysis of the subsolar-mass black hole candidate SSM200308 from the second part of the third observing run of Advanced LIGO-Virgo
• The hot gas mass fraction in halos. From Milky Way-like groups to massive clusters
• The Highest-Energy Cosmic Rays Cannot be Dominantly Protons from Steady Sources
• The extent of intergalactic metal enrichment from galactic winds during the Cosmic Dawn
• The study of Kantowski-Sachs perfect fluid cosmological model in modified gravity
• Hickson-like compact groups inhabiting different environments
• Reionization effect enhancement due to primordial black holes
• asevolution: a relativistic N-body implementation of the (a)symmetron
• Search for $B$ Mesogenesis at BABAR
• Investigating the effect of cosmic opacity on standard candles
• Revisiting the Cosmological Constant Problem within Quantum Cosmology
• The cosmic microwave background Cold Spot anomaly: the impact of sky masking and the expected contribution from the Integrated Sachs-Wolfe effect
• Searching for dark matter annihilation from individual halos: uncertainties, scatter and signal-to-noise ratios
• Systematic effects induced by Half Wave Plate precession into Cosmic Microwave Background polarization measurements
• No evidence for EDE from Planck data in extended scenarios
• Ghost free boson-fermion co-existence system
• Dark Matter in B-L Supersymmetric Standard Model with Inverse Seesaw
• Cosmological Constraints on Unstable Particles: Numerical Bounds and Analytic Approximations
• Gamma-ray-emitting narrow-line Seyfert 1 galaxies: the Swift view
• Shape and Spin of Minihaloes. II: The Effect of Streaming Velocities
• A Simple Model of Dark Matter and CP Violation
• The SCUBA-2 Web Survey: I. Observations of CO(3-2) in hyper-luminous QSO fields
• Coupled dark energy model inspired from general conformal transformation
• Calibrating magnification bias for the $E_G$ statistic to test general relativity
• Constraints on kinematic parameters at $z\ne 0$
• Directional dark matter detection sensitivity of a two-phase liquid argon detector
• Testing the galaxy collision induced formation scenario for the trail of dark matter deficient galaxies with the susceptibility of globular clusters to the tidal force
• Revisiting dark energy models using differential ages of galaxies
• Dark-siren Cosmology with Decihertz Gravitational-wave Detectors
• Serendipitous discovery of a strong-lensed galaxy in integral field spectroscopy from MUSE
• Inflation with explicit parametric connection between General Relativity and Scalar-Tensor gravity
• Constraints on Dark Matter-Photon Coupling in the Presence of Time-Varying Dark Energy
• Bayesian inference of stellar parameters based on 1D stellar models coupled with 3D envelopes
• A method for reconstructing the Galactic magnetic field using dispersion of fast radio bursts and Faraday rotation of radio galaxies
• Gauge-Invariant Tensor Perturbations Induced from Baryon-CDM Relative Velocity and the B-mode Polarization of the CMB
• Extended FLRW Models: dynamical cancellation of cosmological anisotropies
• Faint $\gamma$-ray sources at low-redshift: the radio galaxy IC 1531
• A thermodynamic point of view on dark energy models
• Quantum Cosmology and the Inflationary Spectra from a Non-Minimally Coupled Inflaton
• Exact Geodesic Distances in FLRW Spacetimes
• Cosmological Boundary Flux Parameter
• Milky Way-like galaxies: stellar population properties of dynamically defined disks, bulges and stellar halos
• Impact of SZ cluster residuals in CMB maps and CMB-LSS cross-correlations
• Resonant Electric Probe to Axionic Dark Matter
• On the primordial origin of the smoothing excess in the $Planck$ temperature power spectrum in light of LSS data
• Probing cosmic anisotropy with GW/FRB as upgraded standard sirens
• Shear and vorticity in the spherical collapse of dark matter haloes
• The Statistical Similarity of Repeating and Non-Repeating Fast Radio Bursts
• Searching for heavy neutrino in terms of tau lepton at future hadron collider
• Decaying fermionic warm dark matter and XENON1T electronic recoil excess
• Halo Counts-in-cells for Cosmological Models with Different Dark Energy
• Angular distribution of cosmological parameters as a probe of inhomogeneities: a kinematic parametrisation
• Theoretical implications of the galactic radial acceleration relation of McGaugh, Lelli, and Schombert
• Dark energy reconstruction analysis with artificial neural networks: Application on simulated Supernova Ia data from Rubin Observatory
• Probing modified gravity in cosmic filaments
• Distant foreground and the Planck-derived Hubble constant
• Hamilton-Jacobi approach for quasi-exponential inflation: predictions and constraints after Planck 2015 results
• Baryogenesis from spontaneous CP violation in the early Universe
• Non-parametric Reconstruction of Photon Escape Fraction from Reionization
• An old stellar population or diffuse nebular continuum emission discovered in green pea galaxies
• Self-interacting neutrinos, the Hubble parameter tension, and the Cosmic Microwave Background
• Constraining the physics of star formation from CIB-cosmic shear cross-correlations
• Quantifying the redshift space distortion of the bispectrum III : Detection prospects of the multipole moments
• Diffuse neutrino supernova background as a cosmological test
• Revisit of constraints on dark energy with Hubble parameter measurements including future redshift drift observations
• Cosmology with extragalactic proper motions: harmonic formalism, estimators, and forecasts
• Dynamical signature of a stellar bulge in a quasar host galaxy at $z\simeq 6$
• A semi-analytical perspective on massive galaxies at $z\sim 0.55$
• Kinetic theory and classical limit for real scalar quantum field in curved space-time
• Thermal and Reionisation History within a Large-Volume Semi-Analytic Galaxy Formation Simulation
• The Photon Spectrum of Asymmetric Dark Stars
• The role of $T_0$ in CMB anisotropy measurements
• Roles of sterile neutrinos in particle physics and cosmology
• Unravelling the Origin of the Counter-Rotating Core in IC 1459 with KMOS and MUSE
• Average X-ray properties of galaxy groups. From Milky Way-like halos to massive clusters
• Detecting primordial gravitational waves with circular polarization of the redshifted 21 cm line: II. Forecasts
• Weak field and slow motion limits in energy-momentum powered gravity
• Morphology of Weak Lensing Convergence Maps
• Secretly Asymmetric Dark Matter
• Dynamical friction in the primordial neutrino sea
• Observational constraints in Delta Gravity: CMB and supernovas
• Relating galaxies across different redshift to study galaxy evolution
• Efficient exploration of reionization parameters for the upcoming 21 cm observations using a photon conserving semi-numerical model SCRIPT
• Implications on the cosmic coincidence by a dynamical extrinsic curvature
• Higgs-like particle decays into $\gamma Z$ and $\gamma \gamma$ : Fingerprints of some non-supersymmetric models
• Extended anisotropic models in noncompact Kaluza-Klein theory
• Investigating the galaxy-halo connection of DESI Emission-Line Galaxies with SHAMe-SF
• A Standard Siren Cosmological Measurement from the Potential GW190521 Electromagnetic Counterpart ZTF19abanrhr
• Cosmological tests of gravity with latest observations
• How to empirically model star formation in dark matter halos: I. Inferences about central galaxies from numerical simulations
• Can Tonne-Scale Direct Detection Experiments Discover Nuclear Dark Matter?
• Electroweak phase transition confronted with dark matter detection constraints
• The Effective Fluid approach for Modified Gravity and its applications
• Where are the extremely metal-poor stars in the Milky Way and Andromeda? Expectations from TNG50
• Quadratic energy-momentum squared gravity: constraints from big bang nucleosynthesis
• Matter Parity Violating Dark Matter Decay in Minimal SO(10), Unification, Vacuum Stability and Verifiable Proton Decay
• Alignment in the orientation of LOFAR radio sources
• Observational Constraints on Varying Alpha in $\Lambda (\alpha )$CDM Cosmology
• Star Formation and Chemical Enrichment in Protoclusters
• Large scalar multiplet dark matter in the high-mass region
• Dark Matter Annihilation in the Circumgalactic Medium at High Redshifts
• Testing statistical Isotropy in Cosmic Microwave Background Polarization maps
• Probing nonstandard neutrino cosmology with terrestrial neutrino experiments
• Galactic black hole immersed in a dark halo with its surrounding thin accretion disk
• CMB spectral distortions in generic two-field models
• Revealing the non-adiabatic nature of dark energy perturbations from galaxy clustering data
• Lyth Bound, eternal inflation and future cosmological missions
• Wasserstein distance as a new tool for discriminating cosmologies through the topology of large scale structure
• The alignment of galaxies at the Baryon Acoustic Oscillation scale
• Covariant Canonical Gauge Gravitation and Cosmology
• MusE GAs FLOw and Wind (MEGAFLOW) XII. Rationale and design of a MgII survey of the cool circum-galactic medium with MUSE and UVES: The MEGAFLOW Survey
• On the Stability of Einstein Universe in f(R,T,R_{μν}T^{μν}) Gravity
• Stellar Neutrino Emission Across The Mass-Metallicity Plane
• Probing the connection between IceCube neutrinos and MOJAVE AGN
• Causality Aspects of Modified Kerr-Newman spacetimes
• Explanation of the 511 keV line: Cascade annihilating dark matter with the ${}^8$Be anomaly
• Universes without the Weak Force: Astrophysical Processes with Stable Neutrons
• Cost of inferred nuclear parameters towards the f-mode dynamical tide in binary neutron stars
• Constraining VLBI-optical offsets in high redshift galaxies using strong gravitational lensing
• Resolution Convergence in Cosmological Hydrodynamical Simulations Using Adaptive Mesh Refinement
• Final Thoughts on the Power Spectra of Scalar Potential Models
• Tensor Perturbations in Anisotropically Curved Cosmologies
• Observational constraints on warm quasi-exponential inflation
• The Logotropic Dark Fluid: Observational and Thermodynamic Constraints
• MaNGA DynPop -- IV. Stacked total density profile of galaxy groups and clusters from combining dynamical models of integral-field stellar kinematics and galaxy-galaxy lensing
• Noether symmetry approach in the cosmological alpha-attractors
• Sensitivity of Proposed Search for Axion-induced Magnetic Field using Optically Pumped Magnetometers
• Lack of Correlations between Cold Molecular Gas and AGN Properties in Type 1 AGNs at $z\lesssim 0.5$
• Gravitino Problem in Inflation Driven by Inflaton-Polonyi Kähler Coupling
• Late-time acceleration by a residual cosmological constant from sequestering vacuum energy in ultimate collapsed structures
• Euclid preparation: XLVIII. The pre-launch Science Ground Segment simulation framework
• A fast method of reionization parameter space exploration using GPR trained SCRIPT
• The Alcock Paczynski test with Baryon Acoustic Oscillations: systematic effects for future surveys
• Zoom-in cosmological hydrodynamical simulation of a star-forming barred, spiral galaxy at redshift z=2
• New approach to neutrino masses and leptogenesis with Occam's razor
• Fate of global symmetries in the Universe: QCD axion, quintessential axion and trans-Planckian inflaton decay-constant
• Scalar Quintuplet Minimal Dark Matter with Yukawa Interactions: Perturbative up to the Planck Scale
• Multistate scalar field dark matter and its correlation with galactic properties
• Estimation of HII Bubble Size Distribution from 21cm Power Spectrum with Artificial Neural Networks
• Carbon envelopes around merging galaxies at z ~ 4.5
• Scalar Bispectrum Beyond Slow-Roll in the Unified EFT of Inflation
• An Enhanced Massive Black Hole Occupation Fraction Predicted in Cluster Dwarf Galaxies
• Radiation-pressure Waves and Multiphase Quasar Outflows
• The DESI One-Percent Survey: Modelling the clustering and halo occupation of all four DESI tracers with Uchuu
• Cosmology with powerful radio-loud AGNs
• Kinematic analysis of $\mathbf{z}=4.3$ galaxies in the SPT2349$-$56 protocluster core
• Investigating the evolution of the dual AGN system ESO~509-IG066
• Connecting the Cosmic Star Formation Rate with the Local Star Formation
• The probability of identifying the cosmic web environment of galaxies around clusters motivated by the Weave Wide Field Cluster Survey
• Self-consistent redshift estimation using correlation functions without a spectroscopic reference sample
• The luminous, massive and solar metallicity galaxy hosting the Swift gamma-ray burst, GRB 160804A at z = 0.737
• Reconciling Mass Functions with the Star-Forming Main Sequence Via Mergers
• Host galaxy identification for binary black hole mergers with long baseline gravitational wave detectors
• Increased Prevalence of Bent Lobes for Double-Lobed Radio Galaxies in Dense Environments
• Mitigating the impact of fiber assignment on clustering measurements from deep galaxy redshift surveys
• Quantum quenches during inflation
• Measuring the BAO peak position with different galaxy selections
• Maximum amplitude of the high-redshift 21-cm absorption feature
• Near- and sub-solar-mass naked singularities and black holes from transmutation of white dwarfs
• Reference level of the vacuum energy density of the Universe and astrophysical data
• Testing the scale-dependent hemispherical asymmetry with the 21-cm power spectrum from the epoch of reionization
• Modeling the Statistics of the Cold Neutral Medium in Absorption-selected High-redshift Galaxies
• Model Independent analysis of MeV scale dark matter: II. Implications from $e^{-}{e}^{+}$ colliders and Direct Detection
• $SO(10)\to SU(5)\times U(1{)}_{\chi }$ as the Origin of Dark Matter
• Evolution of the grain size distribution in Milky Way-like galaxies in post-processed IllustrisTNG simulations
• Interpretation of the gamma-ray excess and AMS-02 antiprotons: Velocity dependent dark matter annihilations
• A machine learning approach to infer the accreted stellar mass fractions of central galaxies in the TNG100 simulation
• Complete classification of Friedmann-Lemaître-Robertson-Walker solutions with linear equation of state: parallelly propagated curvature singularities for general geodesics
• Lensing Effects in Retarded Gravity
• MILCANN : A neural network assessed tSZ map for galaxy cluster detection
• Rapid-response radio observations of short GRB 181123B with the Australia Telescope Compact Array
• A novel approach to investigate chemical inhomogeneities in GRB host galaxies: The $Z_{\mathrm{abs}}-Z_{\mathrm{emiss}}$ relation
• A comparison of the R_h=ct and LCDM cosmologies based on the observed halo mass function
• Angular correlations of causally-coherent primordial quantum perturbations
• Primordial anisotropies from cosmic strings during inflation
• Classical and quantum $f(R)$ cosmology: The big rip, the little rip and the little sibling of the big rip
• Vector perturbations in bouncing cosmology
• Simultaneous Dependence of Matter Clustering on Scale and Environment
• Constraints on the production of primordial magnetic seeds in pre-big bang cosmology
• Matter-antimatter asymmetry induced by non-linear electrodynamics
• Impact of baryonic feedback on HSC Y1 weak lensing non-Gaussian statistics
• Astrophysical information from the Rayleigh-Jeans Tail of the CMB
• Towards an accurate model of small-scale redshift-space distortions in modified gravity
• Bulk viscosity, interaction and the viability of phantom solutions
• Sub-MeV Self Interacting Dark Matter
• Expectations for Inflationary Observables: Simple or Natural?
• Cross Correlation of the Extragalactic Gamma-ray Background with Thermal Sunyaev-Zel'dovich Effect in the Cosmic Microwave Background
• Scalar-tensor black holes in an expanding universe
• Gas and Star Formation from HD and Dust Emission in a Strongly Lensed Galaxy
• The PICASSO map-making code: application to a simulation of the QUIJOTE northern sky survey
• New Interpretations of the Cosmological Preference for a Negative Neutrino Mass
• $J$-factor estimation of Draco, Sculptor and Ursa Minor dwarf spheroidal galaxies with the member/foreground mixture model
• Prospects of Indirect Searches for Dark Matter at INO
• Distinguish the $f(T)$ model from $\Lambda$CDM model with Gravitational Wave observations
• Perturbations in Tachyon Dark Energy and their Effect on Matter Clustering
• Exploring evidence of interaction between dark energy and dark matter
• 21 cm power spectrum in interacting cubic Galileon model
• The Radial Acceleration Relation and a Magnetostatic Analogy in Quasilinear MOND
• Giant low-surface-brightness dwarf galaxy as a test bench for MOdified Gravity
• Probing the Early History of Cosmic Reionization by Future Cosmic Microwave Background Experiments
• The galaxy bias at second order in general relativity with Non-Gaussian initial conditions
• PTF11rka: an interacting supernova at the crossroads of stripped-envelope and H-poor super-luminous stellar core collapses
• NICER, NuSTAR, and Swift follow-up observations of the $\gamma$-ray flaring blazar BL Lacertae in 2020 August-October
• Anisotopic inflation with a non-abelian gauge field in Gauss-Bonnet gravity
• The CMB neutrino mass / vacuum energy degeneracy: a simple derivation of the degeneracy slopes
• Galaxy-galaxy lensing data: $f(T)$ gravity challenges General Relativity
• Accretion of Self-interacting Scalar Field Dark Matter Onto a Reissner-Nordström Black Hole
• Forecast for growth-rate measurement using peculiar velocities from LSST supernovae
• Perturbation level interacting dark energy model and its consequence on late-time cosmological parameters
• Over-massive Central Black Holes in the Cosmological Simulations ASTRID and Illustris TNG50
• Dark Energy and Modified Scale Covariant Theory of Gravitation
• Light Higgsinos, Heavy Gluino and $b-\tau$ Quasi-Yukawa Unification: Will the LHC find the Gluino?
• Multi-spectral Sirens: Gravitational-wave Cosmology with (Multi-) Sub-populations of Binary Black Holes
• Tunable Rectangular Resonant Cavities for Axion Haloscopes
• Variants of Kinetically Modified Non-Minimal Higgs Inflation in Supergravity
• Simulations of Gravitational Heating Due to Early Matter Domination
• Constraints on the dark sector from electroweak precision observables
• Non-parametric modeling of the cosmological data, base on the ${\chi }^2$ distribution
• Power spectrum in the presence of large-scale overdensity and tidal fields: breaking azimuthal symmetry
• HOLISMOKES XIII: Strong-lens candidates at all mass scales and their environments from the Hyper-Suprime Cam and deep learning
• Smoothing expansion rate data to reconstruct cosmological matter perturbations
• A Gaia DR2 search for dwarf galaxies towards Fermi-LAT sources: implications for annihilating dark matter
• Testing the ABS method with the simulated Planck temperature maps
• The gas and stellar mass of low-redshift damped Lyman-$\alpha$ absorbers
• Formation and fate of low metallicity stars in IllustrisTNG50
• An X-ray fading, UV brightening QSO at $z\approx 6$
• First and second order cosmological perturbations in light mass Galileon models
• Aether-quasi-dilaton massive gravity
• The gravitational and lensing-ISW bispectrum of 21cm radiation
• A coherent view of Li depletion and angular momentum transport to explain the Li plateau -- from Population II to Population I stars
• Multimessenger TeV Dark Matter: a mini review
• Can HI 21 cm line trace the Missing Baryons in the Filamentary Structures?
• Probing bursty star formation by cross-correlating extragalactic background light and galaxy surveys
• The Environments of Fast Radio Bursts Viewed Using Adaptive Optics
• Ultra faint dwarf galaxies: an arena for testing dark matter versus modified gravity
• Fast generation of mock galaxy catalogues with COLA
• Dark matter kinetic decoupling with a light particle
• On the influence of environment on star forming galaxies
• Pairwise kSZ signal extraction efficacy and optical depth estimation
• Constraining neutrino mass and dark energy with peculiar velocities and lensing dispersions of Type Ia supernovae
• Two-photon atomic level widths at finite temperatures
• Modified Equations of State for Dark Energy and Observational Limitations
• Pendulum Leptogenesis
• The dispersion measure and scattering of Fast Radio Bursts: contributions from multi-components, and clues for the intrinsic properties
• Probing dark gauge boson with observations from neutron stars
• Cosmological effects on $f(\bar{R},\bar{T})$ gravity through a non-standard theory
• LRS Bianchi I model with constant deceleration parameter
• Right sneutrino with $\Delta L=2$ masses as non-thermal dark matter
• The Number of Possible CETIs within Our Galaxy and the Communication Probability among These CETIs
• Modifying dark matter indirect detection signals by thermal effects at freeze-out
• Quantifying Observational Projection Effects with a Simulation-based hot CGM model
• Collapsing scenarios of K-essence generalized Vaidya spacetime under $f(\bar{R},\bar{T})$ gravity
• Balancing Anisotropic Curvature with Gauge Fields in a Class of Shear-Free Cosmological Models
• A new logotropic model based on a complex scalar field with a logarithmic potential
• Maximal X-ray feedback in the pre-reionization universe
• Fast numerical method to generate halo catalogs in modified gravity (part I): second-order Lagrangian Perturbation Theory
• Initial Energy of a Spatially Flat Universe -- a Hint of its Possible Origin
• Probing galaxy evolution from $z=0$ to $z\simeq 10$ through galaxy scaling relations in three L-Galaxies flavours
• Indirect Searches of the Degenerate MSSM
• Massive Fermi Gas in the Expanding Universe
• Premerger localization of intermediate mass binary black holes with LISA and prospects of joint observations with Athena and LSST
• The dust effects on galaxy scaling relations
• Type II Seesaw with scalar dark matter in light of AMS-02, DAMPE and Fermi-LAT
• Is it Mixed dark matter or neutrino masses?
• ASymba: HI global profile asymmetries in the Simba simulation
• Dynamical stability of an interacting quintessence with varying-mass dark matter particles in Lyra manifold
• Black Holes merging with Low Mass Gap Objects inside Globular Clusters
• Constraints on ultracompact minihalos from the extragalactic gamma-ray background observation
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. -- III. Stellar metallicity drivers in MaNGA and TNG50
• Constraining primordial and gravitational mode coupling with the position-dependent bispectrum of the large-scale structure
• Cosmology with moving bimetric fluids
• Testing emergent gravity with mass densities of galaxy clusters
• Mixed WIMP-axion dark matter
• Effects of a local physics change on the SH0ES determination of $H_0$
• Predictions for LISA and PTA based on SHARK galaxy simulations
• The influence of Hickson-like compact group environment on galaxy luminosities
• Probing stochastic inter-galactic magnetic fields using blazar-induced gamma ray halo morphology
• Muon g-2 and rare top decays in up-type specific variant axion models
• Velocity-dependent annihilation radiation from dark matter subhalos in cosmological simulations
• On the Origin of Gamma-ray Flares from Bright Fermi Blazars
• A Minimal Model for Massive Neutrinos in Newtonian N-body Simulations
• SDSS-IV MaNGA: When is morphology imprinted on galaxies?
• The search for Light Dark Matter with NEWS-G
• Statistical measurements of dispersion measure fluctuations of FRBs
• Is there another coincidence problem at the reionization epoch?
• Cosmic Degeneracies III: N-body Simulations of Interacting Dark Energy with Non-Gaussian Initial Conditions
• Imprints of decaying dark matter on cosmic voids
• Lagrangian formulation for an extended cosmological equation-of-state
• Blueberry galaxies up to 200 Mpc and their optical and infrared properties
• Exponentially growing bubbles around early super massive black holes
• Cosmic shear calibration with forward modeling
• Optical Photometric Indicators of Galaxy Cluster Relaxation
• Bound Dark Energy: towards understanding the nature of the Dark Energy
• Effects of dust sources on dust attenuation properties in IllustrisTNG galaxies at $z\sim 7$
• Astroinformatics based search for globular clusters in the Fornax Deep Survey
• Cosmological constraints from the redshift dependence of the volume effect using the galaxy 2-point correlation function across the line-of-sight
• Cosmology and CPT violating neutrinos
• Does space-time torsion determine the minimum mass of gravitating particles?
• Neutrino Masses, Scale-Dependent Growth, and Redshift-Space Distortions
• Challenges in Constraining Gravity with Cosmic Voids
• A semi-analytic model of pairwise velocity distribution between dark matter halos
• Natural Alignment of Quark Flavors and Radiatively Induced Quark Mixings
• Beyond Ultra-diffuse Galaxies. II. Environmental Quenching of Mass-Size Outliers among the Satellites of Milky Way Analogs
• Wheeler's It from Bit Proposal in Loop Quantum Gravity
• Constraining the Milky Way Mass with Its Hot Gaseous Halo
• Lagrangian theory of structure formation in relativistic cosmology. V. Irrotational fluids
• Backsplash galaxies and their impact on galaxy evolution: a three-stage, four-type perspective
• Thermodynamic Constraints on the Dark Sector
• Gravitational waves, CMB polarization, and the Hubble tension
• Angular power spectra of anisotropic stochastic gravitational wave background: developing statistical methods and analyzing data from ground-based detectors
• Determining the systemic redshift of Lyman-alpha emitters with neural networks and improving the measured large-scale clustering
• Characterizing the Conditional Galaxy Property Distribution using Gaussian Mixture Models
• Dark against luminous matter around isolated central galaxies: a comparative study between modern surveys and Illustris-TNG
• Optimal and fast E/B separation with a dual messenger field
• The extended Baryon Oscillation Spectroscopic Survey (eBOSS): testing a new approach to measure the evolution of the structure growth
• Reentrant pion superfluidity and cosmic trajectories within PNJL model
• Are redshift-space distortions actually a probe of growth of structure?
• Nonthermal Pressure in the Outskirts of Abell 2142
• Constraining quenching timescales in galaxy clusters by forward-modelling stellar ages and quiescent fractions in projected phase space
• Antisymmetric Cross-correlation between H I and CO Line Intensity Maps as a New Probe of Cosmic Reionization
• Testing theories of Gravity and Supergravity with inflation and observations of the cosmic microwave background
• Gemini Multi-Object Spectrograph Integral Field Unit Spectroscopy of the Double-peaked Broad Emission Line of a Red Active Galactic Nucleus
• High-energy Neutrino Productions from AGN Disk Transients Impacted by Circum-disk Medium
• Measuring the local Dark Matter density in the laboratory
• Isotropic non-Gaussian $g_{\mathrm{NL}}$-like toy models that reproduce the cosmic microwave background anomalies
• Emergence of space and expansion of universe
• Electron-positron pair plasma in TXS 0506+056 and the "neutrino flare" in 2014-2015
• A Framework for Simultaneously Measuring Field Densities and the High-z Luminosity Function
• Large-Distance Lens Uncertainties and Time-Delay Measurements of $H_0$
• Cosmic evolution of the incidence of Active Galactic Nuclei in massive clusters: Simulations versus observations
• An exploration of the properties of cluster profiles for the thermal and kinetic Sunyaev-Zel'dovich effects
• Holographic cosmology and tachyon inflation
• The origin of correlations between mass, metallicity and morphology in galaxies from the EAGLE simulation
• Square-Root parametrization of dark energy in $f(Q)$ cosmology
• A first-order approach to conformal gravity
• The Scale of Homogeneity in the $R_h=ct$ Universe
• Formation of metal-free binaries: Impact of H${}_2$ line cooling and CIE cooling
• Relic Density of Asymmetric Dark Matter in Modified Cosmological Scenarios
• Computational Techniques for Parameter Estimation of Gravitational Wave Signals
• ALMA resolves the molecular gas in a young low-metallicity starburst galaxy at z=1.7
• Testing Lorentz invariance of dark matter with satellite galaxies
• Probing dark-matter effects with gravitational waves using the parameterized post-Einsteinian framework
• The XXL Survey XXXII. Spatial clustering of the XXL-S AGN
• Probing Velocity Dependent Self-Interacting Dark Matter with Neutrino Telescopes
• Towards understanding thermal history of the Universe through direct and indirect detection of dark matter
• Accretion onto supermassive and intermediate mass black holes in cosmological simulations
• Charged Higgs in MSSM and Beyond
• Iterative map-making with two-level preconditioning for polarized Cosmic Microwave Background data sets
• Cosmology from multimeasure multifield model
• Cosmic transparency and acceleration
• Measuring the baryonic Tully-Fisher relation below the detection threshold
• Structure Formation with Two Periods of Inflation: Beyond PLaIn $\Lambda$CDM
• Dissipative dark matter halos: The steady state solution II
• Multipole vectors of completely random microwave skies for $l\le 50$
• Understanding the Impact of Semi-numeric Reionization Models when using CNNs
• Very-High-Energy Gamma-Ray Afterglows of GRB 201015A and GRB 201216C
• Parametrizing growth in dark energy and modified gravity models
• Least Fine-Tuned U(1) Extended SSM
• Detecting Baryon Acoustic Oscillations with third generation gravitational wave observatories
• Dark energy with the help of interacting dark sectors
• Cosmology of Dirac-Born-Infeld dRGT massive gravity
• Pattern of perturbations from a coherent quantum inflationary horizon
• A Study of NaI(Tl) crystal Encapsulation using Organic scintillators for the Dark Matter Search
• eROSITA Detection Rates for Tidal Disruptions of White Dwarfs by Intermediate Mass Black Holes
• Fermion Mass and Mixing in a Low-Scale Seesaw Model based on the S4 Flavor Symmetry
• Forecasting Super-Sample Covariance in Future Weak Lensing Surveys with SuperSCRAM
• Modified initial power spectrum and too big to fail problem
• Observable spectral and angular distributions of $\gamma$-rays from extragalactic ultrahigh energy cosmic ray accelerators: the case of extreme TeV blazars
• Consequences of $\mu$-$\tau$ reflection symmetry for $3+1$ neutrino mixing
• The viable f(G) gravity models via reconstruction from the observations
• The Alcock Paczynski test with 21cm intensity field
• Global alignments of parsec-scale AGN radio jets and their polarization planes
• Gravitational wave background from kink-kink collisions on infinite cosmic strings
• Interpretation of the cosmic ray positron and electron excesses with an annihilating-decaying dark matter scenario
• Analysis of the spatially-resolved $V$-3.6$\mu$m colors and dust extinction in 257 nearby NGC and IC galaxies
• Constraints on circum-galactic media from Sunyaev-Zel'dovich effects and X-ray data
• Characterizing galaxy clusters by their gravitational potential: systematics of cluster potential reconstruction
• Flavon Magneto-Baryogenesis
• Dying of the Light: An X-ray Fading Cold Quasar at z ~ 0.405
• AGILE, Fermi, Swift, and GASP-WEBT multi-wavelength observations of the high-redshift blazar 4C $+$71.07 in outburst
• Reconstruction of $\alpha$-attractor supergravity models of inflation
• Specific Effect of Peculiar Velocities on Dark-Energy Constraints from Type Ia Supernovae
• On Dark Matter Explanations of the Gamma-Ray Excesses from the Galactic Center and M31
• Non minimally coupled condensate cosmologies: matching observational data with phase space
• A search for X-ray absorbed sources in the 3XMM catalogue, using photometric redshifts and Bayesian spectral fits
• Non-comoving baryons and cold dark matter in cosmic voids
• Trading kinetic energy: How late kinetic decoupling of dark matter changes $N_{\text{eff}}$
• CP-violating inflation and its cosmological imprints
• Metastable Conformal Dark Matter
• Solving the Cosmological Entropy Issue with a Higgs Dilaton
• Resolving Complex Inner X-ray Structure of the Gravitationaly Lensed AGN MGB2016+112
• Mitigating baryonic effects with a theoretical error covariance
• Mapping the Universe in HD
• High Scale Boundary Conditions in Models with Two Higgs Doublets
• Search for AGN counterparts of unidentified Fermi-LAT sources with optical polarimetry: Demonstration of the technique
• Gaussianization of peculiar velocities and bulk flow measurement
• Galaxy populations in haloes in high-density environments
• Shape and Spin of Minihaloes: From Large Scales to the Centres
• The Dark Matter Halos of HI Selected Galaxies
• The four cosmic tidal web elements from the $\beta$-skeleton
• Non-adiabatic evolution of dark sector in the presence of $U(1{)}_{L_{\mu }-L_{\tau }}$ gauge symmetry
• Relic neutrinos: Antineutrinos of Primordial Nucleosynthesis
• The Effect of Microlensing On the Observed X-ray Energy Spectra of Gravitationally Lensed Quasars
• The geometrical meaning of statistical isotropy of smooth random fields in two dimensions
• Scotogenesis in Hybrid Textures of Neutrino Mass Matrix and Neutrinoless Double Beta Decay
• Close, bright and boxy: the superluminous SN 2018hti
• High Scale Type-II Seesaw, Dominant Double Beta Decay within Cosmological Bound and Verifiable LFV Decays in SU(5)
• Whac-a-constraint with anomaly-free dark matter models
• The shape distribution of superclusters in SDSS DR 12
• Testing generalized scalar-tensor theories of gravity with clusters of galaxies
• Estimation of spectrum and parameters of relic gravitational waves using space-borne interferometers
• On the asymptotic behaviour of cosmic density-fluctuation power spectra of cold dark matter
• Constraints on galaxy formation from the cosmic-far-infrared-background\,$-$\,optical-imaging cross-correlation using \textit{Herschel} and UNIONS
• Astrophysical Source Classification and Distance Estimation for PyCBC Live
• Photometrically-Classified Superluminous Supernovae from the Pan-STARRS1 Medium Deep Survey: A Case Study for Science with Machine Learning-Based Classification
• Evolution of density and velocity profiles of dark matter and dark energy in spherical voids
• The spatial distribution of satellites in galaxy clusters
• Cosmological Constraints on the Global Star Formation Law of Galaxies: Insights From Baryon Acoustic Oscillation Intensity Mapping
• Deep VLBI Observations Challenge Previous Evidence of a Binary Supermassive Black Hole Residing in the Seyfert Galaxy NGC 7674
• Study on the mapping of halo clustering from real space to redshift space
• The quasi-adiabatic relaxation of haloes in the IllustrisTNG and EAGLE cosmological simulations
• Gravitational Fluctuations as an Alternative to Inflation
• A search for dark matter among Fermi-LAT unidentified sources with systematic features in Machine Learning
• Joint HST, VLT/MUSE and XMM-Newton observations to constrain the mass distribution of the two strong lensing galaxy clusters: MACS J0242.5-2132 & MACS J0949.8+1708
• Coupled scalar field cosmology with effects of curvature
• Studying the Warm Hot Intergalactic Medium in emission: a reprise
• Cosmological Constraints from Fourier Phase Statistics
• Baryonic Effects on Lagrangian Clustering and Angular Momentum Reconstruction
• Radiative Symmetry breaking, Cosmic Strings and Observable Gravity Waves in $U(1{)}_R$ symmetric $SU(5)\times U(1{)}_{\chi }$
• Probing Ensemble Properties of Vortex-avalanche Pulsar Glitches with a Stochastic Gravitational-Wave Background Search
• Constraining Temporal Oscillations of Cosmological Parameters Using Type Ia Supernovae
• Scalar Dark Matter, GUT baryogenesis and Radiative neutrino mass
• Photometric and Spectroscopic Observations of GRB 210104A: Bright Reverse shock Emission and Dense Circumburst Environment
• Measuring inflaton couplings via dark radiation as $\Delta N_{\mathrm{eff}}$ in CMB
• Resonant probing spin-0 and spin-2 dark matter mediators with fixed target experiments
• Noncommutative Universe and Chameleon Field Dynamics
• Revisiting Friedmann-like cosmology with torsion: newest constraints from high-redshift observations
• Probing redshift-space distortions with phase correlations
• A Unified $p_{\mathrm{astro}}$ for Gravitational Waves: Consistently Combining Information from Multiple Search Pipelines
• HSC-CLAUDS survey: The star formation rate functions since z ~ 2 and comparison with hydrodynamical simulations
• The MUSE-Faint survey. III. Constraining scalar field dark matter with Antlia B
• Dynamical systems analysis of an interacting scalar field model in an anisotropic universe
• Analysis of Fermi-LAT data from Tucana-II: Possible constraints on the Dark Matter models with an intriguing hint of a signal
• Nonlinear redshift space distortion in halo ellipticity correlations: Analytical model and N-body simulations
• How do baryonic effects on the cosmic matter distribution vary with scale and local density environment?
• PAC.V. The Roles of Mass and Environment in the Quenching of Galaxies
• What drives the corpulence of galaxies? I. The formation of central compact dwarf galaxies in TNG50
• Spherical collapse and cluster number counts in dark energy models disformally coupled to dark matter
• A power spectrum approach to the search for Axion-like Particles from resolved galaxy clusters using CMB as a backlight
• Accurate Measurement of the Lensing Magnification by BOSS CMASS Galaxies and Its Implications for Cosmology and Dark Matter
• Non-thermal WIMP baryogenesis
• The Three Hundred project: Estimating the dependence of gas filaments on the mass of galaxy clusters
• Cosmological solutions in spatially curved universes with adiabatic particle production
• Revisiting the energy distribution and formation rate of CHIME fast radio bursts
• Reconstruction of the two-dimensional gravitational potential of galaxy clusters from X-ray and Sunyaev-Zel'dovich measurements
• Cosmological bounds on neutrino statistics
• Optical photometry and spectroscopy of the low-luminosity, broad-lined Ic supernova iPTF15dld
• The effect of quantum decoherence on inflationary gravitational waves
• Challenges in Cosmology from the Big Bang to Dark Energy, Dark Matter and Galaxy Formation
• Cold Dark Matter Based on an Analogy with Superconductivity
• Eddington Ratios of Dust-obscured Quasars at $z\lesssim 1$: Evidence Supporting Dust-obscured Quasars as Young Quasars
• Early formation of supermassive black holes from the collapse of strongly self-interacting dark matter
• NGDEEP: The Star Formation and Ionization Properties of Galaxies at $1.7<z<3.4$
• Impact of dark boson mediated feeble interaction between dark matter and hadronic matter on $f$-mode oscillation of neutron stars
• A topological approach to Neutrino masses by using exotic smoothness
• How bad could it be? Modelling the 3D complexity of the polarised dust signal using moment expansion
• Emergent Dark Energy from Dark Matter
• Unveiling a 36 Billion Solar Mass Black Hole at the Centre of the Cosmic Horseshoe Gravitational Lens
• Fundamental Physics and Cosmology with TianQin
• The mass-dependent UVJ diagram at cosmic noon: A challenge for galaxy evolution models and dust radiative transfer
• Molecules in the early Universe
• Cosmic filament spin -- II: filament spin and its impact on galaxy spin-filament alignment in a cosmological simulation
• SMBH Seeds: Model Discrimination with High Energy Emission Based on Scaling Relation Evolution
• The THESAN-ZOOM project: Star-formation efficiencies in high-redshift galaxies
• CMB Spectral $\mu$-Distortion of Multiple Inflation Scenario
• Observational Constraint on Spherical Inhomogeneity with CMB and Local Hubble Parameter
• Evidence of a fraction of LIGO/Virgo/KAGRA events coming from active galactic nuclei
• Dark energy, scalar singlet dark matter and the Higgs portal
• Observational Status of Tachyon Natural Inflation and Reheating
• Mass-morphology relation of TNG50 galaxies
• J1342+0928 Supports the Timeline in the R_h=ct Cosmology
• A Hyperactive FRB Pinpointed in an SMC-Like Satellite Host Galaxy
• Results from the Pan-STARRS Search for Kilonovae: Contamination by Massive Stellar Outbursts
• No-scale SUGRA Inflation and Type-I seesaw
• Probing departures from $\Lambda$CDM by late-time datasets
• A counter-image to the gravitational arc in Abell 1201: Evidence for IMF variations, or a $10^{10}$M${}_{\odot }$ black hole?
• Cosmological singlet diagnostics of neutrinophilic dark matter
• Cosmological implications of different baryon acoustic oscillation data
• Conformally Coupled General Relativity
• Observable tensor-to-scalar ratio and secondary gravitational wave background
• Unseen Progenitors of Luminous High-z Quasars in the R_h=ct Universe
• Determining Cosmological-model-independent $H_0$ with Gravitationally Lensed Supernova Refsdal
• The Origin of Massive Compact Galaxies: Lessons from IllustrisTNG
• Resolved star formation in TNG100 central and satellite galaxies
• Distinguishing AGN Feedback Models with the Thermal Sunyaev-Zel'dovich Effect
• Predictions on the stellar-to-halo mass relation in the dwarf regime using the empirical model for galaxy formation EMERGE
• Neutrinoless double beta decay in minimal left-right symmetric model with universal seesaw
• Another X-ray UFO without a momentum-boosted molecular outflow. ALMA CO(1-0) observations of the galaxy pair IRAS 05054+1718
• A variable active galactic nucleus at $z=2.06$ triply-imaged by the galaxy cluster MACS J0035.4-2015
• GalRotpy: an educational tool to understand and parametrize the rotation curve and gravitational potential of disk-like galaxies
• Eliminating the Hubble Tension in the Presence of the Interconnection between Dark Energy and Matter in the Modern Universe
• Dark matter repulsion could thwart direct detection
• Near-infrared Extragalactic Background Light Fluctuations on Nonlinear Scales
• A Survey of Deuterated Ammonia in the Cepheus Star-Forming Region L1251
• Probing dark energy using convergence power spectrum and bi-spectrum
• Dark Sector first results at Belle II
• Spatially resolved gas and stellar kinematics in compact starburst galaxies
• Testing for relics of past strong buckling events in edge-on galaxies: Simulation predictions and data from S${}^4$G
• Probing dark gauge boson via Einstein-Cartan portal
• Emergence of Galactic Morphologies at Cosmic Dawn: Input from Numerical Modeling
• High Energy Gamma Rays from Nebulae Associated with Extragalactic Microquasars and Ultra-Luminous X-ray Sources
• Scalar warm inflation in holographic cosmology
• Features in single field slow-roll inflation
• Cosmological Constraints using the newest VLT-KMOS HII Galaxies and the full Planck CMB spectrum
• Searching for the shadows of giants II: the effect of local ionisation on the Lyman-$\alpha$ absorption signatures of protoclusters at redshift $z\sim 2.4$
• [NII] fine-structure emission at 122 and 205um in a galaxy at z=2.6: a globally dense star-forming interstellar medium
• RAiSERed: radio continuum redshifts for lobed AGNs
• Size, shade or shape? The contribution of galaxies of different types to the star-formation history of the Universe from SDSS-IV MaNGA
• ΛCDM suitably embedded in f(R) with a non-minimal coupling to matter
• On the alignment of haloes, filaments and magnetic fields in the simulated cosmic web
• Contribution of Galactic free-free emission to the foreground for EoR signal in SKA experiments
• Spatially Resolved Molecular Gas Properties of Host Galaxy of Type I Superluminous Supernova SN 2017egm
• Model independent measurement of the growth rate from the consistency relations of the LSS
• Dark Matter Candidates in a Visible Heavy QCD Axion Model
• Local properties of the large-scale peaks of the CMB temperature
• The impact of signal-to-noise, redshift, and angular range on the bias of weak lensing 2-point functions
• Observations of [OI]63micron line emission in main-sequence galaxies at z~1.5
• Growth of massive black holes at high-z via accretion predominantly driven by magnetic outflows
• Multiple Components in the Broadband $\gamma$-ray Emission of the Short GRB 160709A
• Observation and Confirmation of Nine Strong Lensing Systems in Dark Energy Survey Year 1 Data
• Absolute calibration of the polarisation angle for future CMB B-mode experiments from current and future measurements of the Crab nebula
• Constraining the non-gravitational scattering of baryons and dark matter with early cosmic structure formation
• New mixing schemes for (3+1) neutrinos
• A sensitive search for unknown spectral emission lines in the diffuse X-ray background with XMM-Newton
• Non-Gaussianity from Entanglement During Inflation
• Induced Gravity and Quantum Cosmology
• Axion and Neutrino physics in a $U(1)$-enhanced supersymmetric model
• SU(2)$_{\tiny\mbox{CMB}}$ at high redshifts and the value of $H_0$
• Dependence of accessible dark matter annihilation cross-sections on the density profiles of dwarf spheroidal galaxies with the Cherenkov Telescope Array
• Non-Gaussianity in two-field inflation beyond the slow-roll approximation
• On wormholes with long throats and the stability problem
• Light sterile neutrinos, dark matter, and new resonances in a $U(1)$ extension of the MSSM
• Revised Uncertainties in Big Bang Nucleosynthesis
• An i2HDM Strongly Coupled to a non-Abelian Vector Resonance
• Simulations of imaging extended sources using the GMRT and the U-GMRT: Implications to observing strategies
• Galactic wind X-ray heating of the intergalactic medium during the Epoch of Reionization
• Lens covariance effects on likelihood analyses of CMB power spectra
• Universal subhalo accretion in cold and warm dark matter cosmologies
• How to confirm the existence of population III stars by observations of gravitational waves
• Limits on Entanglement Effects in the String Landscape from Planck and BICEP/Keck Data
• Study of WIMP annihilations into a pair of on-shell scalar mediators
• Spontaneous Baryogenesis without Baryon Isocurvature
• The Velocity Distribution Function of Galaxy Clusters as a Cosmological Probe
• High-redshift test of gravity using enhanced growth of small structures probed by the neutral hydrogen distribution
• Forays into the dark side of the swamp
• Circularly Polarized Gamma Rays in Effective Dark Matter Theory
• Pati-Salam unification with a spontaneous CP violation
• Gravitational production of superheavy baryonic and dark matter in quintessential inflation: nonconformally coupled case
• Perturbation Theory Remixed: Improved Nonlinearity Modeling beyond Standard Perturbation Theory
• Finsler space-time can explain both parity asymmetry and power deficit seen in CMB temperature anisotropies
• Isolating the linear signal when making redshift space distortion measurements
• AGN feedback in an infant galaxy cluster: the LOFAR-Chandra view of the giant FRII radio galaxy J103025+052430 at z=1.7
• VERITAS and Fermi-LAT constraints on the Gamma-ray Emission from Superluminous Supernovae SN2015bn and SN2017egm
• Dynamics of Molecular Gas in the Central Region of the Quasar IZwicky1
• Spin speed correlations and the evolution of galaxy-halo systems
• X-ray surface brightness observations of galaxy clusters, cosmic opacity and the limits on the matter density parameter
• Andromeda XXV -- a dwarf galaxy with a low central dark matter density
• The triple-peaked afterglow of GRB 210731A from X-ray to radio frequencies
• The Effects of Dark Matter Annihilation on Cosmic Reionization
• Galaxy populations in protoclusters at cosmic noon
• Self-calibrating optical galaxy cluster selection bias using cluster, galaxy, and shear cross-correlations
• Quantum Entanglement in Multi-field Inflation
• The Quest for the Inflationary Spectral Runnings in the Presence of Systematic Errors
• X-ray Absorption Lines in the Warm-Hot Intergalactic Medium: Probing Chandra observations with the CAMEL simulations
• Inference of the optical depth to reionization $\tau$ from $\text{Planck}$ CMB maps with convolutional neural networks
• eRO-ExTra: eROSITA extragalactic non-AGN X-ray transients and variables in eRASS1 and eRASS2
• A possible role for the merger of clusters/voids in the cosmological expansion
• CHEX-MATE: A non-parametric deep learning technique to deproject and deconvolve galaxy cluster X-ray temperature profiles
• Scalar Dark Energy Models and Scalar-Tensor Gravity: Theoretical Explanations for the Accelerated Expansion of Present Universe
• Growth and Geometry Split in Light of the DES-Y3 Survey
• Anisotropic correlation functions as tracers of central galaxy alignments in simulations
• Asymmetric Drift of Andromeda Analogs in the IllustrisTNG Simulation
• Testing the anisotropy of the Universe with the distance duality relation
• Discrimination of anisotropy in dark matter velocity distribution with directional detectors
• Supergravity Model of Inflation and Explaining IceCube HESE Data via PeV Dark Matter Decay
• What if the universe expands linearly? A local general relativity to solve the "zero active mass" problem
• BAO Extractor: bias and redshift space effects
• Light polarization oscillations induced by photon-photon scattering
• Circumgalactic Environments around Distant Quasars 3C 9 and 4C 05.84
• Probing Inhomogeneity in the Helium Ionizing UV Background
• The effect of AGN feedback on the X-ray morphologies of clusters -- simulations vs. observations
• CHEX-MATE: the intracluster medium entropy distribution in the gravity-dominated regime
• Improving Constraints on Fundamental Physics Parameters with the Clustering of Sunyaev-Zeldovich Selected Galaxy Clusters
• The left-right supersymmetric option at a high-energy upgrade of the LHC
• Effects of tidal gravitational fields in clustering dark energy models
• Likelihood analysis of small field polynomial models of inflation yielding a high Tensor-to-Scalar ratio
• Emergent gravity fails to explain color-dependent galaxy-galaxy lensing signals from SDSS Dr7
• Does spatial flatness forbid the turnaround epoch of collapsing structures?
• Resolution of the small scale structure issues with dissipative dark matter from multiple Standard Model sectors
• Sterile Neutrinos and B-L Symmetry
• Probing the nature of Dark Matter through the metal enrichment of the intergalactic medium
• Black Hole Mass Function of Coalescing Neutron Star-Black Hole Binary Systems: The Prospect of Reconstruction with the Gravitational Wave Observations
• The perils of stacking optically selected groups in eROSITA data. The Magneticum perspective
• Simulated [CII] in high-z galaxies
• MaNGA DynPop -- VI. Matter density slopes from dynamical models of 6000 galaxies versus cosmological simulations: the interplay between baryonic and dark matter
• Euclid preparation. LXVIII. Extracting physical parameters from galaxies with machine learning
• Hubble flow variations as a test for inhomogeneous cosmology
• Measurement of directional range components of nuclear recoil tracks in a fiducialised dark matter detector
• The reheating era leptogenesis in models with seesaw mechanism
• Sharp spectral features from light dark matter decay via gravity portals
• Cosmological perturbations in the $\Lambda$CDM-like limit of a polytropic dark matter model
• Dark Matter Annihilation Feedback in cosmological simulations I: Code convergence and idealised halos
• Studying galaxy cluster morphological metrics with Mock-X
• An efficient hybrid method to produce high resolution large volume dark matter simulations for semi-analytic models of reionisation
• An efficient and robust method to estimate halo concentration
• General bounds in Hybrid Natural Inflation
• Modeling Post-Reionization HI Distributions in Fuzzy Dark Matter Cosmologies Using Conditional Normalizing Flows
• A forecast for the detection of the power asymmetry from galaxy surveys
• The Atacama Cosmology Telescope: Delensed Power Spectra and Parameters
• On the initial regime of pre-big bang cosmology
• Proca-stinated Cosmology I: A N-body code for the vector Galileon
• The Fisher gAlaxy suRvey cOde ($\text{FARO}$)
• Dark matter from CP symmetry of order 4: evolution in the asymmetric regime
• Neutrino mass generation and leptogenesis via pseudo-Nambu-Goldstone Higgs portal
• Testing the phenomenological interacting dark energy model with gamma-ray bursts and Pantheon+ type Ia supernovae
• A model-independent constraint on the Hubble constant with gravitational waves from the Einstein Telescope
• Lux ex tenebris: The imprint of annihilating dark matter on the intergalactic medium during Cosmic Dawn
• Neutrino Mass, Dark Matter and Baryon Asymmetry without Lepton Number Violation
• Towards understanding the Planck thermal dust models
• From Non-trivial Geometries to Power Spectra and Vice Versa
• Light sterile neutrinos and their implications on currently running long-baseline and neutrinoless double beta decay experiments
• Curvaton as dark matter with secondary inflation
• A Novel Estimator for the Equation of State of the IGM by Ly$\alpha$ Forest Tomography
• Measuring the mass and concentration of dark matter halos from the velocity dispersion profile of their stars
• Linear cosmological perturbations in Scalar-tensor-vector gravity
• Probing gaseous halos of galaxies with radio jets
• Reheating constraints on modified quadratic chaotic inflation
• Seesaw Scale and CP Phases in a Minimal Model of Leptogenesis
• Scalar and Fermion field interactions with a gravitational wave
• Lense-Thirring precession and gravito-gyromagnetic ratio
• From "universal" profiles to "universal" scaling laws in X-ray galaxy clusters
• Can the periodic spectral modulations of the 236 SETI candidate Sloan Survey stars be due to Dark Matter effects?
• Warm Modified Chaplygin Gas Shaft Inflation
• Dark Matter candidates in a Type-II radiative neutrino mass model
• A new method to test the cosmic distance duality relation using the strongly lensed gravitational waves
• Spectroscopic AGN survey at $z$ $\sim$ 2 with NTT/SOFI for GRAVITY+ observations
• Constraints on dimension-seven operators with a derivative in effective field theory for Dirac dark matter
• EMERGE: Constraining merging probabilities and timescales of close galaxy pairs
• Cosmological decay of Higgs-like scalars into a fermion channel
• Extreme [OIII] Emitters at z $\sim$ 0.5
• Intra-Cluster Light as a Dynamical Clock for Galaxy Clusters: Insights from the MAGNETICUM, IllustrisTNG, Hydrangea and Horizon-AGN Simulations
• Quantification of the multi-streaming effect in Redshift Space Distortion
• A back-linked Fabry-Perot interferometer for space-borne gravitational wave observations
• Simulation of neutron background for a dark matter search experiment at JUSL
• Testing general relativity via direct measurement of black hole kicks
• Impact of photometric redshifts on the galaxy power spectrum and BAO scale in the LSST survey
• Stable contraction in Brans-Dicke cosmology
• Correlations between mass, stellar kinematics and gas metallicity in EAGLE galaxies
• Probing Large-scale UV Background Inhomogeneity Associated with Quasars using Metal Absorption
• First upper limits on the 21-cm signal power spectrum of neutral hydrogen at $z=9.16$ from the LOFAR 3C196 field
• Statistical anisotropies in temperature and polarization fluctuations from a scale-dependent trispectrum
• Mechanism for dark matter depopulation
• Minimal and non-minimal Universal Extra Dimension models in the light of LHC data at 13 TeV
• Constraining the X-ray AGN halo occupation distribution: implications for eROSITA
• Flatness without CMB - the Entanglement of Spatial Curvature and Dark Energy Equation of State
• Hubble drift in Palatini $f(\mathcal{R})$-theories
• DEMNUni: cross-correlating the nonlinear ISWRS effect with CMB-lensing and galaxies in the presence of massive neutrinos
• Bright Type IIP Supernovae in Low-Metallicity Galaxies
• The Einstein-Boltzmann equations revisited
• Search for the optical counterpart of the GW170814 gravitationalwave event with the VLT Survey Telescope
• The THESAN-ZOOM project: Star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts
• Toward a more stringent test of gravity with redshift space power spectrum: simultaneous probe of growth and amplitude of large-scale structure
• Investigating the Dark Matter Halo of NGC 5128 using a Discrete Dynamical Model
• Cosmological Model Independent Time Delay Method
• Primordial perturbations in a rainbow universe with running Newton constant
• Hilltop inflation and generation of helical magnetic field
• Tachyonic vs Quintessence dark energy: linear perturbations and CMB data
• Modified Kerr black holes surrounded by dark matter spike
• Structure formation in clustering DBI dark energy model with constant sound speed
• Cosmological production of black holes: a way to constrain alternative theories of gravity
• Gauge field and brane-localized kinetic terms on the chiral square
• General Perfect Fluid Perturbations of Homogeneous and Orthogonal Locally Rotationally Symmetric Class II Cosmologies
• Electric dipole moments and dark matter in a CP violating MSSM
• Turbulence-induced deviation between baryonic field and dark matter field in the spatial distribution of the Universe
• Lense-Thirring precession and modified gravity constraints
• Lyman Alpha Emitters and the 21cm Power Spectrum as Probes of Density-Ionization Correlation in the Epoch of Reionization
• Does the structure of Pop III supernova ejecta affect the elemental abundance of extremely metal-poor stars?
• Who Ordered That? Unequal-Mass Binary Black Hole Mergers Have Larger Effective Spins
• Clifford algebra Cl(0,6) approach to beyond the standard model and naturalness problems
• Scale-invariant dynamics in the Solar System
• Evidence for a Dusty Dark Dwarf Galaxy in the Quadruple Lens MG0414+0534
• On tachyonic stability priors for dark energy
• On improving analytical models of cosmic reionization for matching numerical simulation
• A new nonlinear instability for scalar fields
• Probing Ultra-light Axion Dark Matter from 21cm Tomography using Convolutional Neural Networks
• Gamma-ray signals from multicomponent scalar dark matter decays
• Purely Triplet Seesaw and Leptogenesis within Cosmological Bound, Dark Matter and Vacuum Stability
• Multiwavelength analysis of low surface brightness galaxies to study possible dark matter signature
• The Ages of M31 Star Clusters: Spectral Energy Distribution Versus Color-Magnitude Diagram
• Electroweak Phase Transition in an Inert Complex Triplet Model
• Sterile neutrino dark matter from right-handed neutrino oscillations
• Compactified Cosmological Simulations of the Infinite Universe
• Space-based optical lattice clocks as gravitational wave detectors in search for new physics
• Bubble Trouble: a Review on Electroweak Baryogenesis
• Symmetry breaking, and the effect of matter density on neutrino oscillation
• Reconstruction of a direction-dependent primordial power spectrum from Planck CMB data
• Multi-wavelength consensus of large-scale linear bias
• A Diffused Background from Axion-like Particles in the Microwave Sky
• Universal Seesaw and $0\nu \beta \beta$ in new 3331 left-right symmetric model
• Lepto-philic 2-HDM + singlet scalar portal induced fermionic dark matter
• Tests of Acoustic Scale Shifts in Halo-based Mock Galaxy Catalogues
• Untargeted Bayesian search of anisotropic gravitational-wave backgrounds through the analytical marginalization of the posterior
• Early-type galaxy density profiles from IllustrisTNG: III. Effects on outer kinematic structure
• Surface Tension: Accelerated Expansion, Coincidence Problem & Hubble Tension
• Strong Dark Matter Self-Interaction from a Stable Scalar Mediator
• Stability and pulsation of the first dark stars
• Analysis cosmological tachyon and fermion model and observation data constraints
• Virial clouds explaining the observed rotational asymmetry in the galactic halos
• Could the 21-cm absorption be explained by the dark matter suggested by ${}^8$Be transitions?
• Is the Big Rip unreachable?
• Hunting for Statistical Anisotropy in Tensor Modes with B-mode Observations
• Beyond $\Lambda$CDM: Exploring a Dynamical Cosmological Constant Framework Consistent with Late-Time Observations
• Constraining the 21cm brightness temperature of the IGM at $z$=6.6 around LAEs with the Murchison Widefield Array
• A new test of gravity -- I: Introduction to the method
• Secluded and Putative Flipped Dark Matter and Stueckelberg Extensions of the Standard Model
• Halos in Dark Ages: formation and chemistry
• Optical galaxy cluster mock catalogs with realistic projection effects: Validations with the SDSS clusters
• Unveiling the Universe with Emerging Cosmological Probes
• Cosmological Dynamics of D-BIonic and DBI Scalar Field and Coincidence Problem of Dark Energy
• Universal dark halo scaling relation for the dwarf spheroidal satellites
• Models for Self-resonant Dark Matter
• Impact of cosmic rays on the global 21-cm signal during cosmic dawn
• Magnification bias in the shear-ratio test: a viable mitigation strategy
• A WHIM origin for the soft excess emission in the Coma cluster
• CTA Sensitivity on TeV scale Dark Matter Models with Complementary Limits from Direct Detection
• Bounds on the Polymer Scale from Gamma Ray Bursts
• Correlation between centre offsets and gas velocity dispersion of galaxy clusters in cosmological simulations
• The contribution of magnetized galactic outflows to extragalactic Faraday rotation
• Scatter in the satellite galaxy SHMR: fitting functions, scaling relations & physical processes from the IllustrisTNG simulation
• VLA Snapshot Continuum Survey of FRI Quasar Candidates Selected from the LOFAR Two-Metre Sky Survey (LoTSS)
• On the lepton CP violation in a $\nu$2HDM with flavor
• Testing Higgs boson scenarios in the phenomenological NMSSM
• The survival of stellar discs in Fornax-like environments, from TNG50 to real galaxies
• Deviations from Tribimaximal and Golden Ratio mixings under radiative corrections of neutrino masses and mixings
• A stochastic model to reproduce the star-formation history of individual galaxies in hydrodynamic simulations
• Fingerprints of modified gravity on galaxies in voids
• Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
• Cosmological Solutions to the Lithium Problem
• IllustrisTNG Snapshots for 10 Gyr of Dynamical Evolution of Brightest Cluster Galaxies and Their Host Clusters
• The rotational kinetic Sunyaev-Zeldovich contribution to the temperature asymmetry toward the M31 halo
• Constraints on dark matter models from the observation of Triangulum-II with the Fermi Large Area Telescope
• Precise peculiar velocities from gravitational waves accompanied by electromagnetic signals and cosmological applications
• A Unified Universe
• The extended Planetary Nebula Spectrograph (ePN.S) early-type galaxy survey: The specific angular momentum of ETGs
• Covariant evolution of perturbations during reheating in two-field inflation
• Effects of dark boson mediated feeble interaction between dark matter (DM) and quark matter on $f$-mode oscillation of DM admixed quark stars
• Anticipating the XRISM search for the decay of resonantly produced sterile neutrino dark matter
• Exploring the distance-redshift relation with gravitational wave standard sirens and tomographic weak lensing
• Non-linear Structure Formation for Dark Energy Models with a Steep Equation of State
• Novel standard candle: Collapsing axion stars
• Quasi-Stellar Objects acting as potential Strong Gravitational Lenses in the SDSS-III BOSS survey
• Nonlinear structure formation in Bound Dark Energy
• Some Phenomenologies of a Simple Scotogenic Inverse Seesaw Model
• Cosmological parameters from Planck data in SU(2)${}_{\mathrm{CMB}}$, their local $\Lambda$CDM values, and the modified photon Boltzmann equation
• Elucidating Dark Energy with Future 21 cm Observations at the Epoch of Reionization
• Mass Modeling and Kinematics of Galaxy Clusters in Modified Gravity
• Cosmological Simulation of Galaxy Groups and Clusters-II: Studying Different Modes of Feedback through X-ray Observations
• Cluster Cosmology with the Velocity Distribution Function of the HeCS-SZ Sample
• Determining the time before or after a galaxy merger event
• Empirical Dust Attenuation Model Leads to More Realistic UVJ Diagram for TNG100 Galaxies
• Comparison of Burst Properties between FRB 20190520B and FRB 20121102A
• Gravitational production of dark matter in the Peebles-Vilenkin model
• Direct Parameter Inference from Global EoR Signal with Bayesian Statistics
• Combining cosmic shear data with correlated photo-$z$ uncertainties: constraints from DESY1 and HSC-DR1
• Major Mergers Mean Major Offset: Drivers of Intrinsic Scatter in The $M_{GCS}-M_h$ Scaling Relation for Massive Elliptical Galaxies
• Gravitational waves from binary black holes as probes of the structure formation history
• Revealing new high redshift quasar populations through Gaussian mixture model selection
• Confining Burst Energy Function and Spectral Fringe Pattern of FRB 20121102A with Multifrequency Observations
• Kinematics and dynamics of the luminous infrared galaxy pair NGC 5257/58 (Arp 240)
• Axion production from primordial magnetic fields
• Multi-Component Decomposition of Cosmic Infrared Background Fluctuations
• Optimization of Coulomb Energies in Gigantic Configurational Spaces of Multi-Element Ionic Crystals
• Observing with NIKA2Pol from the IRAM 30m telescope. Early results on the commissioning phase
• VLT-MUSE spectroscopy of AGNs misclassified by BPT diagnostic or with weak emission lines
• Interpretations of galactic center gamma-ray excess confronting the PandaX-II constraints on dark matter-neutron spin-dependent scatterings in the NMSSM
• A study of holographic dark energy models using configuration entropy
• Nuclear Processes in Other Universes: Varying the Strength of the Weak Force
• PRUSSIC II -- ALMA imaging of dense-gas tracers in SDP.81: Evidence for low mechanical heating and a sub-solar metallicity in a z=3.04 dusty galaxy
• On the Cooling Flow Problem in the Gaseous Halo of the Milky Way
• Potential Impact of the Sagittarius Dwarf Galaxy on the Formation of Young O-rich Stars
• Are there more galaxies than we see around high-$z$ quasars?
• Graviton-photon oscillation in alternative theories of gravity
• Fast DAQ system with image rejection for axion dark matter searches
• Population Synthesis of Black Hole Binaries with Compact Star Companions
• An Alternate Left-Right Symmetric Model with Dirac Neutrinos
• On the Effects of Local Environment on Active Galactic Nucleus (AGN) in the Horizon Run 5 Simulation
• Cosmic recombination history in light of EDGES measurements of the cosmic dawn 21-cm signal
• The Viability of Phantom Dark Energy as a Quantum Field in 1st-Order FLRW Space
• The Chandra Deep Field South as a test case for Global Multi Conjugate Adaptive Optics
• Search for decaying heavy dark matter in an effective interaction framework: a comparison of $\gamma$-ray and radio observations
• How complex is the cosmic web?
• Parameter inference for coalescing massive black hole binaries using deep learning
• Fisher forecast for the BAO measurements from the CSST spectroscopic and photometric galaxy clustering
• Galaxy pairs in The Three Hundred simulations: a study on the performance of observational pair-finding techniques
• Calibrating excursion set reionization models to approximately conserve ionizing photons
• The time delay of JVAS B1030+074 from VLA polarization monitoring
• Dynamics of two-scalar-field cosmological models beyond the exponential potential
• The Shape of FIREbox Galaxies and a Potential Tension with Low-mass Disks
• Coordinated X-ray and UV absorption within the accretion disk wind of the active galactic nucleus PG 1126-041
• KISS: a spectrometric imager for millimetre cosmology
• Phantom Dirac-Born-Infeld Dark Energy
• Testing Horndeski gravity as dark matter with $\texttt{hi_class}$
• Measuring the reionization 21 cm fluctuations using clustering wedges
• Evidence for evolving dark energy from DESI DR2 BAO and Pantheon${}^{+}$, DES-Dovekie, and Union3
• Present and Future constraints on Secluded Dark Matter in the Galactic Halo with TeV Gamma-ray Observatories
• Weak-lensing tunnel voids in simulated light cones: A new pipeline to investigate modified gravity and massive neutrinos signatures
• Foreground and sensitivity analysis for broad band (2D) 21cm--Ly-alpha and 21cm--H-alpha correlation experiments probing the Epoch of Reionization
• Charged dilatonic black holes in dilaton-massive gravity
• Non-Gaussian Effects of the Saha's Ionization in the Early Universe
• A serendipitous discovery of HI-rich galaxy groups with MeerKAT
• Reionization in the Light of Dark Stars
• Measuring galaxy-galaxy-galaxy-lensing with higher precision and accuracy
• Generalized Interacting Dark Energy Model and Loop Quantum Cosmology
• Non-linear logarithmic interactions and a varying polytropic gas
• Anamorphic Quasiperiodic Universes in Modified and Einstein Gravity with Loop Quantum Gravity Corrections
• Electroweak Corrections to Dark Matter Direct Detection in the Dark Singlet Phase of the N2HDM
• Constraining cosmological parameters using void statistics from the SDSS survey
• The Three Hundred Project: Mapping The Matter Distribution in Galaxy Clusters Via Deep Learning from Multiview Simulated Observations
• Matter power spectrum induced by primordial magnetic fields: from the linear to the non-linear regime
• Application of the FRADO model of BLR formation to the Seyfert galaxy NGC 5548 and the first step toward determining the Hubble constant
• Constraints on Lorentz invariance violation from the extraordinary Mrk 421 flare of 2014 using a novel analysis method
• One Extension to Explain Them All, One Scale-Invariant Spectrum to Test Them All, and in One Model Bind Them
• Minimal asymptotically safe dark matter
• A two-phase model of galaxy formation: III. The formation of globular clusters
• Power spectrum response of large-scale structure in 1D and in 3D: tests of prescriptions for post-collapse dynamics
• New exact and analytic solutions in Weyl Integrable cosmology from Noether symmetry analysis
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• Gravitational wave spectrum from kinks on infinite cosmic superstrings with Y-junctions
• Early Growth of Structure in Warm Wave Dark Matter
• A Machine Learning Approach to Correct for Mass Resolution Effects in Simulated Halo Clustering Statistics
• A New Probe of the High-z BAO scale: BAO tomography With CMB $\times$ LIM-Nulling Convergence
• Exploring the physical origins of halo assembly bias from early times
• Growth of Linear Perturbations in a Universe with Superfluid Dark Matter
• Stochastic inflation and non-perturbative power spectrum beyond slow roll
• Dynamical analysis of a first order theory of bulk viscosity
• Effects of Redshift Uncertainty on Cross-Correlations of CMB Lensing and Galaxy Surveys
• The SABRE South Technical Design Report Executive Summary
• A note on non singular Einstein-Aether cosmologies
• Analytic Formulation of 21 cm Signal from Cosmic Dawn: Ly$\alpha$ Fluctuations
• Scalar-tensor extension of the $\Lambda$CDM model
• Optimal strategy for polarization modulation in the LSPE-SWIPE experiment
• Interacting Chaplygin gas revisited
• Large-Scale Structure Topology in Non-Standard Cosmologies: Impact of Dark Sector Physics
• Condition for dust evacuation from the first galaxies
• Dissociation of dark matter and gas in cosmic large-scale structure
• Stellar Populations in a semi-analytic model I: bulges of Milky Way-like galaxies
• On the contributions of extragalactic CO emission lines to ground-based CMB observations
• Ionization from Cosmic Strings at Cosmic Dawn
• Reviewing the prospect of fermion triplets as dark matter and source of baryon asymmetry in non-standard cosmology
• Entanglement Entropy and Decoupling in the Universe
• Are Lyα emitters segregated in protoclusters regions?
• Ricci-cubic holographic dark energy
• G-Warm inflation: Intermediate model
• Slowly rotating Bose-Einstein Condensate confronted with the rotation curves of 12 dwarf galaxies
• Constant-roll, cosmic acceleration, and massive neutrinos
• Prospects for probing small-scale dark matter models with pulsars around Sagittarius A*
• Cosmological Simulations of Stellar Halos with Gaia Sausage-Enceladus Analogues: Two Sausages, One Bun?
• Access via laboratory experiments to the level mixing effect induced by blackbody radiation and its influence on the cosmological hydrogen recombination problem
• High-redshift quasar selection from the CFHQSIR survey
• Cosmological constant constraints from observation-derived energy condition bounds and their application to bimetric massive gravity
• Gamma-ray line constraints on Coy Dark Matter
• Full-Sky Lensing Reconstruction of 21 cm Intensity Maps
• A $K_s$-band selected catalogue of objects in the ALHAMBRA survey
• A pilot study on canonical gravity with mass dimension one fermions
• Design, operation and performance of the PAON4 prototype transit interferometer
• Are early-type galaxies quenched by present-day environment? A study of dwarfs in the Fornax Cluster
• Solving particle-antiparticle and cosmological constant problems
• Collective behavior of light in vacuum
• Magnetic braking during direct collapse black hole formation
• Probing spatial orientability of Friedmann--Robertson--Walker spatially flat spacetime
• Traversable wormholes in bi-metric gravity
• Dark charge versus electric charge
• Interplay between the muon $g-2$ anomaly and the PTA nHZ gravitational waves from domain walls in next-to minimal supersymmetric standard model
• Low-mass neutralino dark matter in supergravity scenarios: phenomenology and naturalness
• Two Channels of Metal-Rich Compact Stellar System Formation: Starbursts under High Ram Pressure versus Tidal Stripping
• The Smallest Scale of Hierarchy Survey (SSH) III. Dwarf-dwarf satellite merging phenomena in the low-mass regime
• Instabilities Appearing in Cosmological Effective Field theories: When and How?
• The Galaxy Halo Connection in Modified Gravity Cosmologies: Environment Dependence of Galaxy Luminosity function
• A MARVEL-ous study of how well galaxy shapes reflect Dark Matter halo shapes in Cold Dark Matter Simulations
• Parity in Planck full-mission CMB temperature maps
• Large-scale inhomogeneity of dark energy produced in the ancestor vacuum
• What if gravity becomes really repulsive in the future?
• Investigating magnetically-induced distortions of neutron stars through gamma-ray burst X-ray plateaus
• Semi-analytical frameworks for subhalos from the smallest to the largest scale
• Suppressing the thermal SZ-induced variance in CMB-cluster lensing estimators
• Can EDGES observation favour any dark matter model?
• Forecasting cosmological parameter constraints using multiple sparsity measurements as tracers of the mass profiles of dark matter haloes
• Hemispherical Variance Anomaly and Reionization Optical Depth
• Bayesian Search of Massive Scalar Fields from LIGO-Virgo-KAGRA Binaries
• Measuring cosmic filament spin with the kinetic Sunyaev-Zel'dovich effect
• Endowing $\mathbf{\Lambda }$ with a dynamic nature: constraints in a spatially curved Universe
• Refined Study of Isocurvature Fluctuations in the Curvaton Scenario
• A Novel Scheme for Dark Matter Annihilation Feedback in Cosmological Simulations
• Measurements of one-point statistics in 21 cm intensity maps via foreground avoidance strategy
• Predictions for Detecting a Turndown in the Baryonic Tully Fisher Relation
• All-sky angular power spectra from cleaned WISE$\times$SuperCOSMOS galaxy number counts
• Galaxy clusters as intrinsic alignment tracers: present and future
• New insight into the variability of the Be star $\pi$ Aquarii: Determination of stellar and disk parameters
• Enabling discovery of gravitationally lensed explosive transients: a new method to build an all-sky watch-list of groups and clusters of galaxies
• Probing Large Scale Ionizing Background Fluctuation with Lyman $\alpha$ Forest and Galaxy Cross-correlation at z=2.4
• Modified dispersion relations, inflation and scale invariance
• Statistical sensitivity on right-handed currents in presence of eV scale sterile neutrinos with KATRIN
• Improved Lemaitre-Tolman model and the mass and turn-around radius in group of galaxies II: the role of dark energy
• Visualizing Invisible Dark Matter Annihilation with the CMB and Matter Power Spectrum
• Model Selection based on the Angular-Diameter Distance to the Compact Structure in Radio Quasars
• Studying neutral hydrogen structures during the epoch of reionization using fractal dimensions
• Using $\gamma$-ray observations of dwarf spheroidal galaxies to test the possible common origin of the W-boson mass anomaly and the GeV $\gamma$-ray/antiproton excesses
• Vacuum fluctuations in an ancestor vacuum: A possible dark energy candidate
• Einstein gravity with torsion induced by the scalar field
• Galaxy Zoo JWST: Up to 75% of discs are featureless at $3<z<7$
• Lepton mass and mixing in a simple extension of the Standard Model based on T7 flavor symmetry
• Testing $\Lambda$CDM With Dwarf Galaxy Morphology
• The environment-dependence of the growth of the most massive objects in the Universe
• Baryon acoustic oscillations from HI intensity mapping: the importance of cross-correlations in the monopole and quadrupole
• On the variation in stellar $\alpha$-enhancements of star-forming galaxies in the EAGLE simulation
• The interstellar medium in Andromeda's dwarf spheroidal galaxies: II. Multi-phase gas content and ISM conditions
• Photometric IGM Tomography: Efficiently Mapping Quasar Light Echoes with Deep Narrow Band Imaging
• Revisiting kink-like parametrization and constraints using OHD/Pantheon+/BAO samples
• Estimating Hubble Constant with Gravitational Observations: A Concise Review
• Deconfinement Transition Effects on Cosmological Parameters and Primordial Gravitational Wave Spectrum
• Dark matter in Inert Doublet Model with one scalar singlet and $U(1{)}_X$ gauge symmetry
• Constraining Cosmology With the CMB $\times$ LIM-Nulling Convergence
• Infrared (in)sensitivity of relativistic effects in cosmological observable statistics
• Black holes and wormholes in $f(R)$ gravity with a kinetic curvature scalar
• Brane inflation driven by an arctan potential: CMB constraints and Reheating
• More about a successful vector-tensor theory of gravitation
• Broken $S_{3\mathrm{L}}^{}\times S_{3\mathrm{R}}^{}$ Flavor Symmetry and Leptonic CP Violation
• Small-scale Effects of Thermal Inflation on Halo Abundance at High-$z$, Galaxy Substructure Abundance and 21-cm Power Spectrum
• The effect of hydrodynamical simulation inspired dark matter velocity profile on directional detection of dark matter
• Spatial variation of fundamental constants: testing models with thermonuclear supernovae
• Energy injection in pre-recombination era and EDGES detection
• Cosmic curvature on large-scale structures with homogeneous dark energy
• Insights from leptohadronic modelling of the brightest blazar flare
• Study of entropy production due to electroweak phase transition in $Z_2$ symmetric extension of the Standard Model
• Comparison of results on $N_{\mathrm{eff}}$ from various Planck likelihoods
• Super-Eddington accreting massive black holes explore high-$z$ cosmology: Monte-Carlo simulations
• 2D BAO vs 3D BAO: Hints for new physics?
• Positronium Decays with Dark $Z$ and Fermionic Dark Matter
• Ray-tracing log-normal simulation for weak gravitational lensing: application to the cross-correlation with galaxies
• A new method to probe the mass density and the cosmological constant using configuration entropy
• Constraining cosmology with the velocity function of low-mass galaxies
• Gamma-Ray Burst detection prospects for next generation ground-based VHE facilities
• XXL-HSC: Host properties of X-ray detected AGNs in XXL clusters
• Quintessential Inflation for Exponential Type Potentials: Scaling and Tracker Behavior
• Observational consequences of an interacting multiverse
• Vector Self-Interacting Dark Matter
• Observational constraints on tachyonic chameleon dark energy model
• Pushing the boundaries of asteroseismic individual frequency modelling: unveiling two evolved very-low metallicity red giants
• Covariance matrices for variance-suppressed simulations
• Scalar Triplet Leptogenesis with a CP violating phase
• Central galaxy alignments. Dependence on the mass and the large-scale environment
• Semi-dark Higgs decays: sweeping the Higgs neutrino floor
• Accelerating behavior from dynamical system analysis parameters
• Black holes inside cosmic voids
• Late-times asymptotic equation of state for a class of nonlocal theories of gravity
• The End of Galaxy Surveys
• Non-canonical Conformal Attractors for Single Field Inflation
• Assessing coincident neutrino detections using population models
• What Drives Cluster Cool-Core Transformations? A Population Level Analysis of TNG-Cluster
• Physical cool-core condensation radius in massive galaxy clusters
• Forecasts for Warm Dark Matter from Photometric Galaxy Surveys
• Backreaction of axion coherent oscillations
• Beyond GWTC-3: Analysing and verifying new gravitational-wave events from community catalogues
• Quantum vacuum energy in General Relativity
• Fully Constrained Majorana Neutrino Mass Matrices Using $\Sigma (72\times 3)$
• The beaming effect for Fermi-LAT-detected FR-I radio galaxies
• The effective field theory of dark energy diagnostic of linear Horndeski theories after GW170817 and GRB170817A
• Deviations to Tri-Bi-Maximal mixing in the limit of $\mu -\tau$ symmetry
• Star formation across cosmic time
• Premature supermassive black hole mergers in cosmological simulations of structure formation
• The powerful lens galaxy cluster PLCK G287.0+32.9 (${\theta }_E\sim 43^{\prime \prime }$)
• Moduli Backreaction on Inflationary Attractors
• Reheating constraints to modulus mass for single field inflationary models
• Impact of the primordial fluctuation power spectrum on the reionization history
• A measurement of cluster masses using Planck and SPT-SZ CMB lensing
• Probing $z\gtrsim 6$ massive black holes with gravitational waves
• The KSVZ Axion Model with Quasi-Degenerate Minima: A Unified Model for Dark Matter and Dark Energy
• Pseudo-Periodic Natural Higgs Inflation
• Milliarcsecond X-ray astrometry to resolve inner regions of AGN at $z>1$ using gravitational lensing
• The formation and disruption of globular cluster populations in simulations of present-day $L^{\ast }$ galaxies with controlled assembly histories
• Does radiative feedback make faint z>6 galaxies look small?
• Towards a sound massive cosmology
• The galaxy bias profile of cosmic voids
• Cosmic reflections I: the structural diversity of simulated and observed low-mass galaxy analogues
• Intertwined Formation of ${\mathrm{H}}_2$, Dust, and Stars in Cosmological Simulations
• Background information: a study on the sensitivity of astrophysical gravitational-wave background searches
• Probing Self-Interacting Dark Matter via Gravitational-Wave Background from Eccentric Supermassive Black Hole Mergers
• Scale invariance of the primordial tensor power spectrum
• Dynamics of cosmological perturbations in modified Brans-Dicke cosmology with matter-scalar field interaction
• The role of Dark Matter annihilation in the radio emission of the galaxy cluster A520
• Cosmic scenarios in $f(R)$ gravity: a complete evolution
• Probability Densities of the effective neutrino masses $m_{\beta }$ and $m_{\beta \beta }$
• The Schr$\ddot{o}$dinger-Poisson equations as the large-N limit of the Newtonian N-body system: applications to the large scale dark matter dynamics
• Measuring the velocity field from type Ia supernovae in an LSST-like sky survey
• The Three Hundred Project: Modeling Baryon and Hot-Gas Fraction Evolution in Simulated Clusters
• Signatures of Massive Black Hole Merger Host Galaxies from Cosmological Simulations II: Unique Stellar Kinematics in Integral Field Unit Spectroscopy
• Multi-Epoch Machine Learning 2: Identifying physical drivers of galaxy properties in simulations
• Waging a Campaign: Results from an Injection-Recovery Study involving 35 numerical Relativity Simulations and three Waveform Models
• Global fits of scalar singlet dark matter with GAMBIT
• Dark matter as the source of neutrino mass: theory overview and experimental prospects
• A young galaxy cluster in the old Universe
• Impact of our local environment on cosmological statistics
• Cosmology with Recombination Spectrum
• The relation between optical and $\gamma$-ray emission in BL Lac sources
• Symmetron with a non-minimal kinetic term
• HD 42659: The only known roAp star in a spectroscopic binary observed with B photometry, TESS and SALT
• Anisotropic effective redshift and evolving clustering amplitude
• On the $2^{\text{nd}}$ feature of the matter two-point function
• Constraining the quintessential $\alpha$-attractor inflation through dynamical horizon exit method
• Search for Ultra-High Energy WIMPs by detecting neutrino signatures from the earth core
• Axion-like particle inflation and dark matter
• Galaxy pairs in The Three Hundred simulations II: studying bound ones and identifying them via machine learning
• Radio-Optical Galaxy Shape and Shear Correlations in the COSMOS Field using 3 GHz VLA Observations
• Radio continuum properties of OH megamaser galaxies
• Hawaii Two-0: High-redshift galaxy clustering and bias
• Growth problems of stellar black holes in early galaxies
• Dilaton Field Released under Collision of Dilatonic Black Holes with Gauss-Bonnet Term
• The environments of the radio galaxy population in SIMBA
• Conditions for the Absence of Infrared Sensitivity in Cosmological Probes in Any Gravity Theories
• VLT/MUSE and ATCA observations of the host galaxy of the short GRB 080905A at z=0.122
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: Possibility of estimateing the non-linear systematics using fast simulations
• Cosmic acceleration in screening hybrid quintessence model
• Probing WIMPs in space-based gravitational wave experiments
• Spacetime geometry fluctuations and geodesic deviation
• Growth of cosmic perturbations in the modified $f(R,T)$ gravity
• Dark-Ages Reionisation & Galaxy Formation Simulation XVI: The Thermal Memory of Reionisation
• Voids in the Cosmic Web as a probe of dark energy
• Contributions from primordial non-Gaussianity and General Relativity to the galaxy power spectrum
• A search for cosmological anisotropy using the Lyman alpha forest from SDSS quasar spectra
• Fast multiscale galaxy cluster detection with weak lensing: towards a mass-selected sample
• A comparison of the excess mass around CFHTLenS galaxy-pairs to predictions from a semi-analytic model using galaxy-galaxy-galaxy lensing
• Cosmological Lithium Problems
• Zooming in on eV-MeV Scale Sterile Neutrinos in light of Neutrinoless Double Beta Decay
• Gravitational Wave From Axion-like Particle Inflation
• Scalar triplet leptogenesis in the presence of right-handed neutrinos with S3 symmetry
• Emergent universe revisited through the CSL theory
• Polarized gamma rays from dark matter annihilations
• Multiscale analysis of the CMB temperature derivatives
• A Very Heavy Sneutrino as Viable Thermal Dark Matter Candidate in $U(1{)}^{\prime }$ Extensions of the MSSM
• Non-local cosmological models
• Intrinsic mass-richness relation of clusters from THE THREE HUNDRED hydrodynamic simulations
• Gravitational Lensing of the Cosmic Neutrino Background
• Is a pole type singularity an alternative to inflation?
• Constraining the optical depth of galaxies and velocity bias with cross-correlation between kinetic Sunyaev-Zeldovich effect and peculiar velocity field
• Testing the Reliability of Fast Methods for Weak Lensing Simulations: WL-MOKA on PINOCCHIO
• Dark energy effects on realistic neutron stars
• Search for the Sagittarius Tidal Stream of Axion Dark Matter around 4.55 $\mu$eV
• Effect of turbulent reacceleration on electrons produced by dark matter annihilation in the Coma cluster
• First-order QCD transition in a primordial magnetic field
• Dark matter vorticity and velocity dispersion from truncated Dyson$\unicode{x2013}$Schwinger equations
• Testing the coincidence problem with strong gravitational lens, Type Ia supernovae and Hubble parameter observational data
• Is the local Hubble flow consistent with concordance cosmology?
• Constraining late-time transitions in the dark energy equation of state
• The Complex X-ray Obscuration Environment in the Radio Loud Type 2 Quasar 3C 223
• Vacuum thin shells in Einstein-Gauss-Bonnet brane-world cosmology
• BRS structure of Simple Model of Cosmological Constant and Cosmology
• Ammonia in the interstellar medium of a starbursting disc at z=2.6
• Reconstruction of the scalar field potential in nonmetricity gravity through Gaussian processes
• Unravelling the orbits of cluster galaxy populations according to their dominant gas ionization source
• SN 2016iyc: A Type IIb supernova arising from a low-mass progenitor
• Unraveling emission line galaxy conformity at z~1 with DESI early data
• Shapes and features of the primordial bispectrum
• \bf $\delta M$ Formalism and Anisotropic Chaotic Inflation Power Spectrum
• Photometric IGM tomography with Subaru/HSC: the large-scale structure of Ly$\alpha$ emitters and IGM transmission in the COSMOS field at $z\sim 5$
• Hints of a universal width-energy relation for classified fast radio bursts
• Tilted non-spatially-flat inflation
• A Sub-solar Fe/O, logT~7.5 Gas Component Permeating the Milky Way's CGM
• Survival of black holes through a cosmological bounce
• Prospects of FRBs and Large Scale 21 cm Power Spectra in Constraining the Epoch of Reionization
• Evolution of Dark Energy Perturbations for Slotheon Field and Power Spectrum
• Metal line emission around z<1 galaxies
• Texture Zero Neutrino Models and Their Connection with Resonant Leptogenesis
• Identifying Galaxy Cluster Mergers with Deep Neural Networks using Idealized Compton-y and X-ray maps
• Structure and large scale environment of galaxy pairs in the S-PLUS DR4
• A post-merger enhancement only in star-forming Type 2 Seyfert galaxies: the deep learning view
• The bi-modal ${}^7$Li distribution of the Milky Way's thin-disk dwarf stars: The role of Galactic-scale events and stellar evolution
• Neutrino masses and mixing from milli-charged dark matter
• Gravity and Nonlinear Symmetry Realisation
• Combined dark matter search towards dwarf spheroidal galaxies with Fermi-LAT, HAWC, H.E.S.S., MAGIC, and VERITAS
• The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
• On a quadratic equation of state and a universe mildly bouncing above the Planck temperature
• Gaussian Processes, Median Statistics, Milky Way Rotation Curves
• The matter fluctuation amplitude inferred from the weak lensing power spectrum and correlation function in CFHTLenS data
• Escape, bound and capture geodesics in local static coordinates in Schwarzschild spacetime
• Gravitation as a source of decoherence
• Total and dark mass from observations of galaxy centers with Machine Learning
• Constraints on the very high energy gamma-ray emission from short GRBs with HAWC
• Relaxing Constraints on Dark Matter Annihilation Near the Supermassive Black Hole in M87
• CO(1--0) imaging reveals 10-kiloparsec molecular gas reservoirs around star-forming galaxies at high redshift
• Cosmological Parameter Estimation with a Joint-Likelihood Analysis of the Cosmic Microwave Background and Big Bang Nucleosynthesis
• Transient dark energy, cosmological constant boundary crossing and dark energy $w(z)$ data fits
• A domain wall description of brane inflation and observational aspects
• Can an Anti-de Sitter Vacuum in the Dark Energy Sector Explain JWST High-Redshift Galaxy and Reionization Observations?
• Neutrino mass matrices with three or four vanishing cofactors and non diagonal charged lepton sector
• Universality of the halo mass function in screened gravity theories
• Fitting functions on the cheap: the relative nonlinear matter power spectrum
• Noether Symmetry Approach in Eddington-inspired Born-Infeld gravity
• Lensing Bias to CMB Polarization Measurements of Compensated Isocurvature Perturbations
• Investigating cosmic strings using large-volume hydrodynamical simulations in the context of JWST's massive UV-bright galaxies
• Impact of lensing magnification on the analysis of galaxy clustering in redshift space
• Entropy methods for CMB analysis of anisotropy and non-Gaussianity
• Effects of Dark Energy anisotropic stress on the matter power spectrum
• Environmental effects on halo abundance and weak lensing peak statistics toward large underdense regions
• Upper Limits on the Mass of Cool Gas in the Circumgalactic Medium of Dwarf Galaxies
• CFHTLenS: Galaxy bias as function of scale, stellar mass, and colour. Conflicts with predictions by semi-analytic models
• Loop corrections to primordial non-Gaussianity
• Novel vacuum conditions in inflationary collapse models
• What if? - Exploring the Multiverse through Euclidean wormholes
• Varying constants driven baryogenesis
• Kinetic Field Theory applied to Vector-Tensor Gravity
• GW230814: investigation of a loud gravitational-wave signal observed with a single detector
• The XXL Survey LI. Pressure profile and $Y_{\mathrm{SZ}}$-$M$ scaling relation in three low-mass galaxy clusters at $z\sim 1$ observed with NIKA2
• A large thermal energy reservoir in the nascent intracluster medium at a redshift of 4.3
• Asteroseismology of the young open cluster NGC 2516 II. Constraining cluster age using gravity-mode pulsators
• Milky Way-Like Gas Excitation in an Ultrabright Submillimeter Galaxy at $z=1.6$
• Neutrino assisted GUT baryogenesis - revisited
• Big Bang nucleosynthesis in a weakly non-ideal plasma
• H$\alpha$-based Star Formation Rates in and around z $\sim$ 0.5 EDisCS clusters
• Wavefunction for the Universe Circa the Beginning with Dynamically Determined Unique Initial Conditions
• Collisionless shocks in self-interacting dark matter
• Reconstructing the early-universe expansion and thermal history
• Impacts of pre-initial conditions on anisotropic separate universe simulations: a boosted tidal response in the epoch of reionization
• Gamma-ray lines may reveal the CP nature of the dark matter particle
• Euclid preparation. Exploring the properties of proto-clusters in the Simulated Euclid Wide Survey
• Mock Observations: Three Different Types of Galaxy Alignment in TNG100 Simulations
• Impact of primordial black holes on the formation of the first stars and galaxies
• Reconstructing patchy helium reionization using the cosmic microwave background and large-scale structure
• Reconstructing the Long-wavelength Matter Density Fluctuation Modes from the Scalar-Type Clustering Fossils
• Improved Halo Model Calibrations for Mixed Dark Matter Models of Ultralight Axions
• Physical Processes Behind the Co-Evolution of Halos, Galaxies and Supermassive Black Holes in the IllustrisTNG Simulation
• Detection significance of Baryon Acoustic Oscillations peaks in galaxy and quasar clustering
• The assembly of the most rotationally supported disc galaxies in the TNG100 simulations
• Core prominence as a signature of restarted jet activity in the LOFAR radio-galaxy population
• Spectral features of non-equilibrium antineutrinos of primordial nucleosynthesis
• Asymmetric dark matter, baryon asymmetry and lepton number violation
• Magnetic contributions in Bekenstein type models
• Modified $f(R,T)$ theory in light of gravitational wave standard sirens
• Realization of Sneutrino Self-interacting Dark Matter in the Focus Point Supersymmetry
• Local Limit of Nonlocal Gravity: Cosmological Perturbations
• Generative modelling for mass-mapping with fast uncertainty quantification
• Cosmology with voids from the Nancy Grace Roman Space Telescope
• A statistical study of lopsided galaxies using random forest
• Upper Limit on Star Formation and Metal Enrichment in Minihalos
• Collapse of spherical overdensities in superfluid models of dark matter
• Buchdahl bound, photon ring, ISCO and radial acceleration in Einstein-æther theory
• Comparison of Bayesian inference methods using the Loreli II database of hydro-radiative simulations of the 21-cm signal
• Quasi-steady emission from repeating fast radio bursts can be explained by magnetar wind nebulae
• Quantum Gravitational Hair in Gravastars and Observational Tests
• The Three Hundred Project hydrodynamical simulations: Hydrodynamical weak-lensing cluster mass biases and richnesses using different hydro models
• Looking To The Horizon: Probing Evolution in the Black Hole Spectrum With Gravitational Wave Catalogs
• Characterising galaxy clusters' completeness function in Planck with hydrodynamical simulations
• The Three Hundred: $M_{sub}-V_{circ}$ relation
• The multi-wavelength Tully-Fisher relation in the TNG50 cosmological simulation
• Identifying intermediate mass binary black hole mergers in AGN disks using LISA
• One spectrum to rule them all?
• X-Ray Spectral Variability of Thirteen TeV High Energy Peaked Blazars with XMM-Newton
• Inferring astrophysics and cosmology with individual compact binary coalescences and their gravitational-wave stochastic background
• Non-Parametric Analysis for the Dark Matter Density Evolution
• Reconstructing the epoch of reionisation with Planck PR4
• Pixel-level modelling of group-scale strong lens CASSOWARY 19
• Retrieving the hot circumgalactic medium physics from the X-ray radial profile from eROSITA with an IlustrisTNG-based forward model
• On the unique evolutionary mechanisms of massive quiescent galaxies in the epoch of reionisation
• Quantifying the Impact of Incompleteness on Identifying and Interpreting Galaxy Protocluster Populations with the TNG-Cluster Simulation
• A radio-frequency WIMP search with the MeerKAT Galaxy Cluster Legacy Survey
• Constraints on Generalized Gravity-Thermodynamic Cosmology from DESI DR2
• Self-Similarities and Power-laws in the Time-resolved Spectra of GRB 190114C, GRB 130427A, GRB 160509A, and GRB 160625B
• Survivors and Zombies: The Quenching and Disruption of Satellites around Milky Way Analogs
• The long-lasting effect of X-ray preheating in the post-reionization intergalactic medium
• Primordial black holes and magnetic fields in conformal neutrino mass models
• On the Formation of GW190521-like Binary Black Hole Merger Systems
• Cosmology with Independently Varying Neutrino Temperature and Number
• Tiny galaxies and dark substructures: exploring the "dark" subhaloes in TNG50
• Uncertainty in the visibility mask of a survey and its effects on the clustering of biased tracers
• XENON1T Takes a Razor to a Dark $E_6$-Inspired Model
• Modeling HF-QPOs in Microquasars and AGNs: Charged Particles around Black Holes with CDM Halos
• Kinematics of Circumgalactic O VI Gas and Disk Rotation of $z\approx 0.2$ Star-forming Galaxies
• UNIONS Optical Identifications for VLASS Radio Sources in the Euclid Sky (UNVEIL) I. A Catalog of ~146,000 Radio Galaxies up to z~5
• On the Metallicities and Kinematics of the Circumgalactic Media of Damped Ly$\alpha$ Systems at $z\sim 2.5$
• Effect of Massive Neutrinos on the Position of Cold Dark Matter Halo: Revealed via Delaunay Triangulation Void
• Dark matter as an effect of the quantum vacuum
• LATIS: A Sample of IGM-selected Protoclusters and Protogroups at $z\sim 2.5$
• Dwarf-Dwarf interactions and their influence on star formation : Insights from post-merger galaxies
• Constraints on the varying electron mass and early dark energy in light of ACT DR6 and DESI DR2 and the implications for inflation
• Machine Learning and Structure Formation in Modified Gravity
• PRUSSIC III -- ALMA and NOEMA survey of dense gas in high-redshift star-forming galaxies
• Simulating Cosmological Evolution by Quantum Quench of an Atomic BEC
• Detectability of Gravitational-Wave Memory with LISA: A Bayesian Approach
• Effect of Dark Energy Perturbation on Cosmic Voids Formation
• Impact of a primordial magnetic field on cosmic microwave background $B$ modes with weak lensing
• Holographic connection of f(G) gravity through Barrow and a generalized version of holographic dark fluid
• Impact of cosmic web on the properties of galaxies in IllustrisTNG simulations
• Reoriented Memory of Galaxy Spins for the Early Universe
• Andromeda's asymmetric satellite system as a challenge to cold dark matter cosmology
• The impact of ram pressure on cluster galaxies, insights from GAEA and TNG
• Direct signals from electroweak singlets through the Higgs portal
• Explaining Dark Matter and Neutrino Mass in the light of TYPE-II Seesaw Model
• Gravitational radiation in Infinite Derivative Gravity and connections to Effective Quantum Gravity
• Chern-Simons Gravity in Four Dimensions
• Modelling of long gamma-ray burst host galaxies at cosmic noon from damped Lyman-α absorption statistics
• The robustness of inferred envelope and core rotation rates of red-giant stars from asteroseismology
• Universal multi-stream radial structures of cold dark matter halos
• Assessing the dark matter content of two quasar host galaxies at z~6 through gas kinematics
• LHC Run-3, $b-\tau$ Yukawa Unification and Dark Matter Implications in SUSY 4-2-2 model
• Investigating higgsino dark matter in the semi-constrained NMSSM
• Large-scale geometry and topology of gas fields: Effects of AGN and stellar feedback
• Redshifts of candidate host galaxies of four fast X-ray transients using VLT/MUSE
• Can Hubble tension be eased by invoking a finite range for gravity?
• The hot gas distribution, X-ray luminosity and baryon budget in the L-Galaxies semi-analytic model of galaxy formation
• QueryCheetah: Fast Automated Discovery of Attribute Inference Attacks Against Query-Based Systems
• Pixel space convolution for cosmic microwave background experiments
• Axionic extension of the Proca action
• Local burst model of CMB temperature fluctuations: luminescence in lines of primary para- and orthohelium
• Positive curvature and scalar field tunneling in the landscape
• Cluster analysis of the Roma-BZCAT blazars
• Enhanced cosmic-ray antihelium production from dark matter annihilation through light mediators
• Asteroseismology: Looking for axions in the red supergiant star Alpha Ori
• Oscillating cosmic evolution and constraints on big bang nucleosynthesis in the extended Starobinsky model
• Probing General Relativity in galactic scales at z $\sim 0.3$
• Oscillating solutions of the matter density contrast in Horndeski's theory
• Vacuum energy, the Casimir effect, and Newton's non-constant
• Cosmological Solutions of Chameleon Scalar Field Model
• Modeling Strong Lenses from Wide-Field Ground-Based Observations in KiDS and GAMA
• Hybrid seesaw neutrino model in SUSY $SU(5)\times {\mathbb{A}}_4$
• Dark Matter, Neutrino mass, Cutoff for Cosmic-Ray Neutrino, and Higgs Boson Invisible Decay from a Neutrino Portal Interaction
• Resolution of cosmological singularity in Hořava-Lifshitz cosmology
• Leveraging cross-correlations and linear covariance-based filtering for line-intensity map reconstructions at linear scales
• Simulating the collapse of rotating primordial gas clouds to study the survival possibility of Pop III protostars
• Testing atomic collision theory with the two-photon continuum of astrophysical nebulae
• Conditional Colour-Magnitude Distribution of Central Galaxies in Galaxy Formation Models
• Neutral outflows in high-z QSOs
• Entropy Production in the Inflationary Epoch Using the Gouy-Stodola Theorem
• A note on the initial conditions within the effective field theory approach of cosmic acceleration
• Energy Conditions in Extended $f(R,G,T)$ Gravity
• Testing the weak equivalence principle with the binary neutron star merger GW170817: the gravitational contribution of the host galaxy
• Cross-correlating Planck with VST ATLAS LRGs: a new test for the ISW effect in the Southern Hemisphere
• Probing the No-Scale $\mathcal{F}$-$SU(5)$ One-Parameter Model via Gluino Searches at the LHC2
• HI 21-cm absorption in radio-loud AGN with double-peaked [OIII] emission
• GRB Afterglow of the Sub-relativistic Materials with Energy Injection
• Cosmology in the dark: How compact binaries formation impact the gravitational-waves cosmological measurements
• Can anisotropy in the galaxy distribution tell the bias?
• High Energy Physics and Cosmology at the Unification Frontier: Opportunities and Challenges in the coming years
• Renormalization-Group Running Induced Cosmic Inflation
• New method of exponential potentials reconstruction based on given scale factor in phantonical two-field models
• Fermionic Dark Matter in a simple $t$-channel model
• A scale at 10 MeV, gravitational topological vacuum, and large extra dimensions
• A new instability in clustering dark energy?
• General Perturbations of Homogeneous and Orthogonal Locally Rotationally Symmetric Class II Cosmologies with Applications to Dissipative Fluids
• A quintessence dynamical dark energy model from ratio gravity
• Classifying galaxies according to their HI content
• Inverse seesaw mechanism with compact supersymmetry: enhanced naturalness and light super-partners
• X-Ray Redshifts of Obscured Chandra Source Catalog AGN
• Dust SEDs in Milky Way-like galaxies in the IllustrisTNG simulations based on the evolution of grain size distribution
• Quark deconfinement in compact stars through sexaquark condensation
• Spin alignment around TNG300-1 voids
• The Einstein ring GAL-CLUS-022058s: a Lensed Ultrabright Submillimeter Galaxy at z=1.4796
• Trace Anomaly, Perelman's Functionals and the Cosmological Constant
• Degeneracy in the spectrum and bispectrum among featured inflaton potentials
• Making use of sub-resolution halos in N-body simulations
• Fingerprint matching of beyond-WIMP dark matter: neural network approach
• On the Dynamical Instability of Monatomic Fluid Spheres in (N+1)-Dimensional Spacetime
• On the dark radiation problem in the axiverse
• Revealing mass-degenerate states in Higgs boson signals
• Galaxy rotation curve from classical Cepheids
• Data Analysis and Phenomenological Cosmology
• Natural inflation with natural number of e-foldings
• Higher-Order Spectra of Weak Lensing Convergence Maps in Parameterized Theories of Modified Gravity
• Searching for obscured AGN in z $\sim$ 2 submillimetre galaxies
• Dynamic Zoom Simulations: a fast, adaptive algorithm for simulating lightcones
• Lessons on early structure formation from a mature galaxy cluster observed at cosmic noon
• A simple supergravity model of inflation constrained with Planck 2018 data
• An Optimized Ly$\alpha$ Forest Inversion Tool Based on a Quantitative Comparison of Existing Reconstruction Methods
• The $\Lambda$ to zero limit of spacetimes and its physical interpretation
• New measures to test modified gravity cosmologies
• Cosmological boost factor for dark matter annihilation at redshifts of $z=10$-$100$ using the power spectrum approach
• Optimistic estimation on probing primordial gravitational waves with CMB B-mode polarization
• The XFaster Power Spectrum and Likelihood Estimator for the Analysis of Cosmic Microwave Background Maps
• Primordial black holes in a dimensionally oxidizing Universe
• The Three Hundred Project: The stellar angular momentum evolution of cluster galaxies
• Harvesting quantum coherence from axion dark matter
• On the regularity of the covariance matrix of a discretized scalar field on the sphere
• Fourier imaging of non-linear structure formation
• LRS Bianchi I model with perfect fluid equation of state
• Evolution of dwarf galaxy observable parameters
• Stacked phase-space density of galaxies around massive clusters: Comparison of dynamical and lensing masses
• Triaxiality in galaxy clusters: Mass versus Potential reconstructions
• The bias from hydrodynamic simulations: mapping baryon physics onto dark matter fields
• Dark Matter Annihilation Feedback in Cosmological Simulations II: The Influence on Gas and Halo Structure
• Proca-stinated Cosmology II: Matter, Halo, and Lensing Statistics in the vector Galileon
• Flavor structure, Higgs boson mass and dark matter in supersymmetric model with vector-like generations
• Superclusters from velocity divergence fields
• Tantalizing New Physics from the Cosmic Purview
• Pseudo Newtonian Potential For a Rotating Kerr Black Hole Embedded in Quintessence
• IllustrisTNG and S2COSMOS: possible conflicts in the evolution of neutral gas and dust
• Calculable Cosmological CP Violation and Resonant Leptogenesis
• Proposal for a degree of scientificity in cosmology
• Cosmological Unification, Dark Energy and the Origin of Neutrino Mass
• Dark matter model favoured by reionization data: 7 keV sterile neutrino vs cold dark matter
• Restricting Majorana phases in the Tri-Bi-Maximal limit
• Effect of the Early Reionization on the Cosmic Microwave Background and Cosmological Parameter Estimates
• Establishing the origin of CMB B-mode polarization
• A class of regular bouncing cosmologies
• CTA in the Context of Searches for Particle Dark Matter - a glimpse
• Warm and Cold Dark Matter in Bouncing Universe
• Characterisation of Dark Matter in Direct Detection Experiments: Singlino Versus Higgsino
• Big Bang Nucleosynthesis with Stable ${}^8$Be and the Primordial Lithium Problem
• Identifying the nature of dark matter at $e^{-}{e}^{+}$ Colliders
• A viable D-term hybrid inflation
• The cosmological constant of emergent spacetime in the Newtonian approximation
• Constraining the ionized gas evolution with CMB-spectroscopic survey cross-correlation
• Supersymmetric Clockwork Axion Model and Axino Dark Matter
• Measuring neutrino mass imprinted on the anisotropic galaxy clustering
• Transient weak gravity in scalar-tensor theories
• The reconstruction of dark energy with Ridge Regression Approach
• One-loop Type II Seesaw Neutrino Model with Stable Dark Matter Candidates
• An analytical approach to the CMB anisotropies in a Spatially Closed background
• Unification Predictions With or Without Supersymmetry
• The variance of dispersion measure of high-redshift transient objects as a probe of ionized bubble size during reionization
• Rapidly accreting black hole of the Lyα-luminous quasar PSO J006.1240+39.2219
• Towards a new proposal for the time delay in gravitational lensing
• The Atacama Cosmology Telescope: SZ-based masses and dust emission from IR-selected cluster candidates in the SHELA survey
• MSSM without a free parameter
• Dark Energy and Inflation from Gravitational Waves
• Revealing the Warm and Hot Halo Baryons via Thomson Scattering of Quasar Light
• Constraint on magnetized galactic outflows from LOFAR rotation measure data
• Shapes of dark matter haloes with discrete globular cluster dynamics: The example of NGC 5128 (Centaurus A)
• The impact of AGN X-ray selection on the AGN halo occupation distribution
• Dynamical systems analysis of a cosmological model with interacting Umami Chaplygin fluid in adiabatic particle creation mechanism: Some bouncing features
• Improving SDSS cosmological constraints through $\beta$-skeleton weighted correlation functions
• Thermodynamics of charged black holes in Maxwell-dilaton-massive gravity
• The host galaxy of low-luminosity compact sources
• The COS-Holes Survey: Connecting Galaxy Black Hole Mass with the State of the CGM
• Constraining the average magnetic field in galaxy clusters with current and upcoming CMB surveys
• Neutrino phenomenology and keV dark matter in 2HDM with $A_4$ symmetry
• The evolution of low-mass central galaxies in the vicinity of massive structures and its impact on the two-halo conformity
• Implications of ${\delta }_l^{CP}\sim 270^{\circ }$ and ${\theta }_{23}\gtrsim 45^{\circ }$ for texture specific lepton mass matrices and $0\nu \beta \beta$ decay
• IllustrisTNG in the HSC-SSP: No Shortage of Thin Disk Galaxies in TNG50
• Conversations in the dark: cross-correlating birefringence and LSS to constrain axions
• Big-bang nucleosynthesis and Leptogenesis in CMSSM
• Potential impact of noise correlation in next-generation gravitational wave detectors
• Phenomenological power spectrum models for H$\alpha$ emission line galaxies from the Nancy Grace Roman Space Telescope
• Constraints on fast radio burst emission in the aftermath of gamma-ray bursts
• Axion, mu Term, and Supersymmetric Hybrid Inflation
• Exploring Faraday rotation signatures and population bounds for primordial magnetic black holes
• Broadband Dark Matter Axion Detection using a Cylindrical Capacitor
• Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
• Hermeian haloes: extreme objects with two interactions in the past
• Effect of lensing magnification on type Ia supernova cosmology
• Predicting the Non-Thermal Pressure in Galaxy Clusters
• Simulating the epoch of Helium Reionization in photon-conserving semi-numerical code SCRIPT
• Thermodynamics of scalar field models with kinetic corrections
• Evaluating a Sigmoid Dark Energy Model to Explain the Hubble Tension
• Observational constraints on cosmological parameters in the Bianchi type III Universe with f(R,T) gravity theory
• Constraining the swiss-cheese IR-fixed point cosmology with cosmic expansion
• Redshift and stellar mass dependence of intrinsic shapes of disc-dominated galaxies from COSMOS observations below $z=1.0$
• Inflationary Solution of Hamilton Jacobi Equations during Weak Dissipative Regime
• Detecting 21 cm EoR Signal using Drift Scans: Correlation of Time-ordered Visibilities
• Some Implications of the Leptonic Annihilation of Dark Matter: Possible Galactic Radio Emission Signatures and the Excess Radio Flux of Extragalactic Origin
• SpectrAx: Spectral Search of Axion-Like Particles Using Multi-Band Observations of Galaxy Clusters from SKA, SO, CMB-S4 and eROSITA
• On the scaling relations of bulges and early-type galaxies
• Constraining galaxy properties with complete samples of lenses
• Bright siren without electromagnetic counterpart by LISA-Taiji-TianQin network
• Cluster density slopes from Dark Matter-Baryons Energy Transfer
• Parsec-scale evolution of the gigahertz-peaked spectrum quasar PKS 0858-279
• Dynamical Symmetry Breaking and Negative Cosmological Constant
• Anthropic Selection of Physical Constants, Quantum Entanglement, and the Multiverse Falsifiability
• The impact of halo concentration on the Sunyaev Zel'dovich effect signal from massive galaxy clusters
• Considering light-matter interactions in the Friedmann equations
• Dark matter constraints and the neutralino sector of the scNMSSM
• Constraints on the Helium Abundance from Fast Radio Bursts
• Gravitational wave backgrounds from coalescing black hole binaries at cosmic dawn: an upper bound
• Tracking Pre-inflation Era from density perturbation spectra
• Results from the SuperModel Analysis of the X-COP Galaxy Clusters Sample
• A high-resolution view of the source-plane magnification near cluster caustics in wave dark matter models
• The "Little Dark Dot": Evidence for Self-interacting Dark Matter in the Strong Lens SDSS J0946+1006?
• Relativistic and non-Gaussianity contributions to the one-loop power spectrum
• An Introduction to the Planck Mission
• AGN -- host galaxy photometric decomposition using a fast, accurate and precise deep learning approach
• The origin of the galaxy size-stellar metallicity relation: A semi-analytical perspective
• $\Delta N_{\text{eff}}$ and entropy production from early-decaying gravitinos
• Magnetogenesis From Baryon Asymmetry During an Early Matter Dominated Era
• Lethal radiation from nearby supernovae helps to explain the small cosmological constant
• ACACIA: a new method to produce on-the-fly merger trees in the RAMSES code
• Fisher matrix forecasts on the astrophysics of galaxies during the epoch of reionisation from the 21-cm power spectra
• An Exploration of Heterogeneity in Supernova Type Ia Samples
• Gamma rays from Dark Matter Annihilation in Three-loop Radiative Neutrino Mass Generation Models
• The Correlation Function and Detection of Baryon Acoustic Oscillation Peak from the Spectroscopic SDSS GalWCat Galaxy Cluster Catalogue
• Newly born extragalactic millisecond pulsars as efficient emitters of PeV neutrinos
• Hidden sector behind the CKM matrix
• Six Higgs Doublets Model for Dark Matter
• Constraining violations of the Weak Equivalence Principle Using CHIME FRBs
• Turnaround density evolution encodes cosmology in simulations
• HI in and behind the Hubble Frontier Field Clusters: A Deep MeerKAT Pilot Search out to $z\sim 0.5$
• Intrinsic and Environmental Effects on the Distribution of Star Formation in TNG100 Galaxies
• Black holes in massive Einstein-dilaton gravity
• Densified pupil spectrograph as high-precision radial velocimetry: From direct measurement of the Universe's expansion history to characterization of nearby habitable planet candidates
• Top-Hat Spherical Collapse with Clustering Dark Energy. I. Radius Evolution and Critical Contrast Density
• From particles to orbits: precise dark matter density profiles using dynamical information
• Counts-in-Cells of subhaloes in the IllustrisTNG simulations: the role of baryonic physics
• Far-infrared - radio correlation and magnetic field strength in star-forming early-type galaxies
• Exploring the possible evolution of the mass density power-law index of strong gravitational lenses with a model-independent method
• Cosmoparticle physics of dark matter
• The spatially-resolved effect of mergers on the stellar mass assembly of MaNGA galaxies
• Non-linear coupling in the dark sector as a running vacuum model
• Axion and FIMP Dark Matter in a $U(1)$ extension of the Standard Model
• Environmental history of filament galaxies: stellar mass assembly and star-formation of filament galaxies
• DarkFlux: A new tool to analyze indirect-detection spectra of next-generation dark matter models
• Direct Collapse Accretion Disks Within Dark Matter Halos: Saturation of the Magnetorotational Instability and the Field Expulsion
• Inferring Galactic Parameters from Chemical Abundances: A Multi-Star Approach
• Long Journey toward the Detection of Gravitational Waves and New Era of Gravitational Wave Astrophysics
• Neutrino emission from FRB-emitting magnetars
• Deviation to the Tri-Bi-Maximal flavor pattern and equivalent classes
• Detection of a radio-filled X-ray cavity within the interstellar medium of NGC 5141
• Limits on Polarized Dust Spectral Index Variations for CMB Foreground Analysis
• Dark Energy from pNGB Mediated Dirac Neutrino Condensate
• Dynamics and chaos in the unified scalar field cosmology II. System in a finite box
• Dissecting Cosmological Filaments at High Redshifts: Emergence of Spaghetti-type Flow Inside DM Haloes
• Astrophysical systematics in Kinematic Lensing: quantifying an Intrinsic Alignment analog
• Joint inference on the redshift distribution of fast radio burst and on the intergalactic baryon content
• Lyman-$\alpha$ Emitting Galaxies (LAEs) at Cosmic Dawn: Implications and Predictions
• Post-processing of galaxies due to major cluster mergers I. hints from galaxy colours and morphologies
• Effects of calibration uncertainties on the detection and parameter estimation of isotropic gravitational-wave backgrounds
• An optimal envelope ejection efficiency for merging neutron stars
• The evolution of the barred galaxy population in the TNG50 simulation
• Mean Occupation Function of High Redshift Quasars from the Planck Cluster Catalog
• Revisiting the Dragonfly Galaxy I. High-resolution ALMA and VLA Observations of the Radio Hotspots in a Hyper-luminous Infrared Galaxy at $z=1.92$
• Growth and Feedback from the First Black Holes
• Feedback from intermediate mass black holes on dwarf galaxy morphology at z=2
• Searching for low-mass dark matter via Migdal effect in COSINE-100
• Mass in cosmological perspective
• MaNGA DynPop. VII. A Unified Bulge-Disk-Halo Model for Explaining Diversity in Circular Velocity Curves of 6000 Spiral and Early-Type Galaxies
• A Stronger Case for Superunification Post Higgs Boson Discovery
• Is there a need for dark matter in galaxies?
• Updated neutrino mass constraints from galaxy clustering and CMB lensing-galaxy cross-correlation measurements
• Hubble Tension and Dark Energy in Teleparallel Gauss-Bonnet Gravity: New Constraints from DESI BAO, Pantheon${}^{+}$ and Hubble Data
• Pulse Shape Discrimination of low-energy nuclear and electron recoils for improved particle identification in NaI:Tl
• Parameter Estimation for Scarce Stellar Populations
• Reconstructing the Cosmic Expansion History with a Monotonicity Prior
• Does Quantum Cosmology Predict the Age of the Universe?
• Tomographic Alcock-Paczynski Method with Redshift Errors
• Cosmological implications of the Gaia Milky Way declining rotation curve
• Testing the variation of the fine structure constant with strongly lensed gravitational waves
• A cosmological distance measure using radio-loud quasars
• Accelerating linear system solvers for time domain component separation of cosmic microwave background data
• Feebly-interacting dark matter
• Cosmology from a running vacuum model driven by a scalar field
• A comparison of cosmological models with high-redshift quasars
• The Three Hundred Project: deducing the stellar splashback structure of galaxy clusters from their orbiting profiles
• Characterising the z $\sim$ 7.66 Type-II AGN candidate SMACS S06355 using BEAGLE-AGN and JWST NIRSpec/NIRCam
• On the occurrence of gauge-dependent secularities in nonlinear gravitational waves
• Elucidating the z-dependence of the MOND acceleration (a_0) within the Scale Invariant Vacuum (SIV) paradigm
• Fabrication of antenna-coupled KID array for Cosmic Microwave Background detection
• A full reconstruction of two galaxy clusters intra-cluster medium with strong gravitational lensing
• Globular cluster orbital decay in dwarf galaxies with MOND and CDM: Impact of supernova feedback
• Perturbative treatment of the luminosity distance
• Detectability of dark matter density distribution via gravitational waves from binary black holes in the Galactic center
• Extreme AGN feedback in the fossil galaxy group SDSSTG 4436
• Gas excitation in galaxies and active galactic nuclei with He IIλ4686 and X-ray emission
• Understanding Stellar Mass-Metallicity and Size Relations in Simulated Ultra-Faint Dwarf Galaxies
• Cosmological nanolensing by dense gas clouds
• de Sitter spacetime with a Becchi-Rouet-Stora quartet
• Intermediate Mass Ratio Inspirals in Milky Way Galaxies
• Bayesian inference methodology for Primordial Power Spectrum reconstructions from Large Scale Structure
• Constraint on Matter Power Spectrum on $10^6-10^9{M}_{\odot }$ Scales from ${\tau }_e$
• Influence of the correlation prior on reconstruction of the dark energy equation of state
• SAGAN-VI: When Jets Meet Filaments -- Environmental Imprints on the Growth of Giant Radio Galaxies
• Constraining the Secluded and Catalyzed Annihilation Dark Matter with Fermi-LAT and Planck Data
• Reionization relics in the cross-correlation between the Ly$\alpha$ forest and 21 cm intensity mapping in the post-reionization era
• LATIS: Comparing Galaxy and IGM Tomography Maps as Tracers of Large-scale Structure and Protoclusters at $z\sim 2.5$
• Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
• Stochastic Order Redshift Technique (SORT): a simple, efficient and robust method to improve cosmological redshift measurements
• Towards discovery of gravitationally lensed explosive transients: the brightest galaxies in massive galaxy clusters from Planck-SZ2
• Constraining the parameter space of branon dark matter using white dwarf stars
• The Higgs properties in the MSSM after the LHC Run-2
• Stellar halos tracing the assembly of ultra-faint dwarf galaxies
• CMB Polarization by the Asymmetric Template of Scalar Perturbations
• Caustic and hydrostatic mass bias: Implications for modified gravity
• Galaxy cluster mass bias from projected mass maps: The Three Hundred-NIKA2 LPSZ twin samples
• An optically-dark merging system at z~6 detected by JWST
• The Three Hundred: Gas Properties Outside of Galaxy Cluster with the WHIM Contribution and Detection
• Astrophysical and relativistic modeling of the recoiling black-hole candidate in quasar 3C 186
• Non-linear Phenomenology of Disformally Coupled Quintessence
• Exploring effects of IMF sampling and SN feedback injection on star formation and metallicity in ultra-faint dwarf galaxies
• Thermal Inflation with a Thermal Waterfall Scalar Field Coupled to a Light Spectator Scalar Field
• kSZ Pairwise Velocity Reconstruction with Machine Learning
• A new Bowen Fluorescence Flare and Extreme Coronal Line Emitter discovered by SRG/eROSITA
• Improving the Determination of Supernova Cosmological Redshifts by Using Galaxy Groups
• Probing the shape and internal structure of dark matter halos with the halo-shear-shear three-point correlation function
• Improved SED-Fitting Assumptions Result in Inside-Out Quenching at $z\sim 0.5$ and Quenching at All Radii Simultaneously at $z\sim 1$
• Triggered Population III star formation: the effect of H${}_2$ self-shielding
• K-mouflage at high $k$: extending the reach of $\text{Hi-COLA}$
• Neutrino and Collider Implications of a Left-Right Extended Zee Model
• Decorrelating the errors of the galaxy correlation function with compact transformation matrices
• Diversity of the Lyman continuum escape fractions of high-$z$ galaxies and its origins
• Scalar spectral index in the presence of Primordial Black Holes
• Deciphering Baryonic Feedback from ACT tSZ Galaxy Clusters
• Vacuum Energy and Renormalization of the Field-Independent Term
• Tracing the cosmological origin of gas that fuels in situ star formation in TNG50 galaxies
• Reconstructing HI power spectrum with minimal parameters using the dark matter distribution beyond halos
• GrAviPaSt's Lens to the Past: Unveiling the Evolution of Filamentary Structures
• Detecting Baryon Acoustic Oscillations in Dark Matter from Kinematic Weak Lensing Surveys
• Quantum dual-path interferometry scheme for axion dark matter searches
• Inflation of the Universe by the Non-minimal $Y(R)F^2$ Models
• Rigorous derivation of dark energy and inflation as geometry effects in Covariant Canonical Gauge Gravity
• The $\nu$THDM with the Inverse Seesaw Mechanisms
• Lagrangian displacement field estimators in cosmology
• The prospects of gravitational waves on constraining the anisotropy of the Universe
• Scalar field unification of interacting viscous dark fluid from a geometrical scalar-tensor theory of gravity
• Impact of Population III stars on the astrophysical gravitational-wave background
• Reionization Parameter Inference from 3D Minkowski Functionals of the 21 cm Signals
• Constraining cosmic polarization rotation and implications for primordial B-modes
• IllustrisTNG + Cosmic Rays with a Simple Transport Model: From Dwarfs to L${}^{\star }$ Galaxies
• Dark matter and low scale leptogenesis in a flavor symmetric neutrino two Higgs doublet model($\nu$2HDM)
• Detection for Intermediate-mass Binary Black Holes in Population III Star Clusters with TianQin
• Analysis of the Intrinsic Mid-Infrared L-band to Visible--Near-Infrared Flux Ratios in Spectral Synthesis Models of Composite Stellar Populations
• Observations and Simulations of Radio Emission and Magnetic Fields in Minkowski's Object
• Assess the neutrino mass with micro and macro calorimeter approach
• Higgsino Dark Matter in an economical Scherk-Schwarz setup
• The NIKA polarimeter on science targets. Crab nebula observations at 150 GHz and dual-band polarization images of Orion Molecular Cloud OMC-1
• The Large Number Limit of Multifield Inflation
• High-redshift AGN population in radiation-hydrodynamics simulations
• Physical conditions in high$-$z optically thin C III absorbers: Origin of cloud sizes and associated correlations
• The Use of Binary Black Holes Merging in AGN Disks for Hubble Constant Measurements
• Characterising EP241107a: Multiwavelength Observations of an Einstein Probe-detected Fast X-ray Transient
• A dense dark matter core of the subhalo in the strong lensing system JVAS B1938+666
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• Thermodynamic Prescription of Cosmological Constant in Randall Sundrum-II Brane
• Cosmological Zero Modes
• A convolutional-neural-network estimator of CMB constraints on dark matter energy injection
• Calibrating the effective magnitudes of type Ia supernovae with a model-independent method
• Investigation of the Radial Profile of Galactic Magnetic Fields using Rotation Measure of Background Quasars
• Can the Near-Horizon Black Hole Memory be detected through Binary Inspirals?
• Phase space analysis of a FRW cosmology in the Maxwell$-$Cattaneo approach
• Model independent calibration for sound horizon combining observations of supernovae and transversal BAO measurements
• The double-soft limit in cosmological correlation functions and graviton exchange effects
• A Simple No-Scale Model of Modulus Fixing and Inflation
• Big Bang Nucleosynthesis, the CMB, and the Origin of Matter and Space-Time
• Calibration requirement for Epoch of Reionization 21-cm signal observation -- III. Bias and variance in uGMRT ELAIS-N1 field power spectrum
• The Cosmic Causal Mass
• Rapid Hierarchical Inference of Neutron Star Equation of State from multiple Gravitational Wave Observations of Binary Neutron Star Coalescences
• Electroweak Dark Matter
• Probing stellar-mass primordial black holes with type Ia supernova microlensing
• An LBT view of the co-rotating group of galaxies around NGC 2750: Deep imaging and new satellite candidates
• Scalar and tensor perturbation in vacuum inflation
• Improving the Accuracy of Halo Mass Based Statistics For Fast Approximate N-body Simulations
• Constraining Axially Symmetric Bianchi Type I Model with Self-Consistent Recombination History and Observables
• Black hole solutions in Cotton gravity coupled to nonlinear electrodynamics
• Impact of redshift distribution uncertainties on Lyman-break galaxy cosmological parameter inference
• Charged Higgs bosons in the NMSSM under current LHC constraints
• Galaxy cluster count cosmology with simulation-based inference
• Probing gravity with the DES-CMASS sample and BOSS spectroscopy
• Multi-wavelength follow-up of FRB 180309
• The Atacama Cosmology Telescope: A Test of the Gravitational Force Law on Cosmological Scales Using the Kinematic Sunyaev-Zeldovich Effect
• Constraining the halo-ISM connection through multi-transition carbon monoxide line-intensity mapping
• Neutrinos propagating in curved spacetimes
• The Trans-Planckian Censorship Conjecture in different frameworks of viable inflation
• Absorption of Photons from Distant Gamma-Ray Sources
• HARMONI view of the host galaxies of active galactic nuclei around cosmic noon: Resolved stellar morpho-kinematics and the M${}_{BH}$-${\sigma }_{\star }$ relation
• Pseudo scalar dark matter in a generic U$(1{)}_X$ model
• UNITSIM-Galaxies: data release and clustering of emission-line galaxies
• A Geometric Probe of Cosmology: I. Gravitational Lensing Time Delays and Quasar Reverberation Mapping
• Tests of general relativity at the fourth post-Newtonian order
• Cosmological Constraints on Chiral Tensor Particles
• Identifying Halos in Cosmological Simulations with Continuous Wavelet Analysis: The 2D Case
• Magnetogenesis from Sawtooth Coupling: Gravitational Wave Probe of Reheating
• A Homogeneous and Isotropic Universe in Lorentz Gauge Theory of Gravity
• Curvaton: Perturbations and reheating
• Direct Collapse to Precursors of Supermassive Black Hole Seeds:Radiation-feedback-generated Outflows
• Energy conditions and constraints on the generalized non-local gravity model
• The evolution of the halo occupation distribution in cosmic voids
• Kilonova rates from spherical and axisymmetrical models
• Revisiting Ryskin's Model of Cosmic Acceleration
• Study on the magnetic field of the ultraluminous X-ray pulsar RX J0209.6-7427
• Efficient Modelling of Lyman-α opacity fluctuations during late reionization epoch
• SIGAME v3: Gas Fragmentation in Post-processing of Cosmological Simulations for More Accurate Infrared Line Emission Modeling
• Super-Eddington accretion in high-redshift quasar hosts: Black-hole driven outflows, galaxy quenching, and the nature of little red dots
• SU(5) unification of two triplet seesaw and leptogenesis with dark matter and vacuum stability
• Stirring the cosmic pot: how black hole feedback shapes the matter power spectrum in the Fable simulations
• Euclid Quick Data Release (Q1): The evolution of the passive-density and morphology-density relations between $z=0.25$ and $z=1$
• The Sterile-Active Neutrino Flavor Model: the Imprint of Dark Matter on the Electron Neutrino Spectra
• Reexamine the dark matter scenario accounting for the positron excess in a new cosmic ray propagation model
• Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities
• Emergent Universe as an interaction in the dark sector
• Dirac stars with wormhole topology
• The presence of a Phantom field in a Randall-Sundrum scenario
• Kinetically Modified Non-Minimal Inflation With Exponential Frame Function
• Hypergeometric viable models in $f(R)$ gravity
• Spectral Energy Distribution of the First Galaxies: Contribution from Pre-Main-Sequence Stars
• Homology reveals significant anisotropy in the cosmic microwave background
• A comparison of shrinkage estimators of the cosmological precision matrix
• Describing the Nonuniversal Galaxy Merger Timescales in IllustrisTNG: Effects of Host Halo Mass, Baryons, and Sample Selection
• The Cosmic Evolution of CIV Absorbers at $1.4<z<4.5$: Insights from $100,000$ Systems in DESI Quasars
• Hybrid inflation and gravitational waves from accidentally light scalars
• Effective field theory analysis of composite higgsino-like and wino-like thermal relic dark matter
• High Performance Computing for gravitational lens modeling: single vs double precision on GPUs and CPUs
• LHC Dark Matter Signals from Vector Resonances and Top Partners
• Constraints from the Giant Arc in Abell 370. A New Framework for Understanding Systematic Errors in Cluster Lens Modeling. IV. Constraints from the Giant Arc in Abell 370
• The intervelocity of galaxy pairs in $\Lambda$CDM -- The observed velocity peak at ~130 km/s is not unique to MOND
• Relic Density of Asymmetric Dark Matter with Sommerfeld enhancement
• The role of gas stripping in the quenching of satellite galaxies using SHARK v2.0
• Exploiting the high-resolution NIKA2 data to study the intracluster medium and dynamical state of ACT-CL J0240.0+0116
• PEARLS: Discovery of Point-Source Features Within Galaxies in the North Ecliptic Pole Time Domain Field
• Cosmological Evolution of Semilocal String Networks
• Interacting Dark Energy and Its Implications for Unified Dark Sector
• Exploring the halo-galaxy connection with probabilistic approaches
• On the Impact of Random Residual Calibration Error on the Gibbs ILC Estimates over Large Angular Scales
• GRB 180728A and SN 2018fip: the nearest high-energy cosmological gamma-ray burst with an associated supernova
• Neutrino Interactions with perturbed Rastall Gravity: A Novel Approach to Reducing the Hubble Tension
• Unique fermionic vacuum in de Sitter spacetime from hybrid quantum cosmology
• Coordinate independent approach to the calculation of the effects of local structure on the luminosity distance
• Six Maxims of Statistical Acumen for Astronomical Data Analysis
• Impact of filaments on galaxy cluster properties in The Three Hundred simulation
• Confirmation of the detection of B-modes in the Planck polarization maps
• FAST drift scan survey for HI intensity mapping: simulation on hunting HI filament with pairwise stacking
• A new pressure-parametric cosmological model
• ${}^3\mathrm{He}(\alpha ,\gamma {)}^7\mathrm{Be}$ and ${}^3\mathrm{H}(\alpha ,\gamma {)}^7\mathrm{Li}$ reaction rates and the implication for Big Bang nucleosynthesis in the potential model
• Optimization of the half wave plate configuration for the LSPE-SWIPE experiment
• Constructing an entangled state in Heisenberg picture for inflationary cosmology
• Higgs domain walls in the thermal background
• FLRW spaces as submanifolds of ${\mathbb{R}}^6$: restriction to the Klein-Gordon operator
• A Proposal for Constraining Initial Vacuum by CMB
• Hyperbolic space in the Newtonian limit: the cosmological constant
• How bright was the Big Bang?
• Copositive criteria for a two-component dark matter model
• CMB delensing with deep learning
• Neutrino phenomenology of a high scale supersymmetry model
• Differences in baryonic and dark matter scaling relations of galaxy clusters: A comparison between IllustrisTNG simulations and observations
• Dynamical disequilibrium in dwarf galaxies: rethinking gas dynamics, rotation curves, and dark matter inference
• Inelastic Dark Matter at the Fermilab Short Baseline Neutrino Program
• Consistency Relation and Non-Gaussianity in a Galileon Inflation
• The need for a nonlocal expansion in general relativity
• The Type Ia Supernova 2021hem: A 2003fg-like Event in an Apparently Hostless Environment
• Cosmological Dark Matter in a Conformal Model
• SuperCLASS -- II: Photometric Redshifts and Characteristics of Spatially-Resolved $\mu$Jy Radio Sources
• A Joint Analysis of Strong Lensing and Type Ia Supernovae to Determine the Hubble Constant
• New analysis of SNeIa Pantheon Catalog: Variable speed of light as an alternative to dark energy
• Phenomenological modification of horizon temperature
• Search for Solar Boosted Dark Matter Particles at the PandaX-4T Experiment
• The Boosted Potential
• Lensing anomalies from the epoch of reionisation
• Quantum fluctuations of the compact phase space cosmology
• On the use of galaxy catalogs in gravitational-wave parameter estimation
• HI asymmetries in spatially resolved SIMBA galaxies
• Galaxies and Cluster of Galaxies as Peak Patches of the Density Field
• Evolution of Cluster Alignments as Evidence of Large-scale Structure Formation in the Universe
• Atomic Hydrogen Shows its True Colours: Correlations between HI and Galaxy Colour in Simulations
• From Halos to Galaxies. X: Decoding Galaxy SEDs with Physical Priors and Accurate Star Formation History Reconstruction
• Connecting low-energy CP violation, resonant leptogenesis and neutrinoless double beta decay in a radiative seesaw model
• Intergalactic-Absorption Confounding Circumgalactic Observations
• The mass ratios parametrization
• An analytical joint prior for effective spins for inference on the spin distribution of binary black holes
• Toward a Measurement of the Transverse Peculiar Velocity of Galaxy Pairs
• Accreted stars and stellar haloes of simulated galaxies in TNG50
• Spatially Resolved [O III] Emission Line Kinematics of Reverberation-Mapped AGNs with the Keck Cosmic Web Imager
• Anomalous EDGES 21-cm Signal and Moduli Dominated Era
• Extracting 21cm signal by frequency and angular filtering
• Inflation and Leptogenesis in a $U(1)$-enhanced supersymmetric model
• Detectability of Population III stellar remnants as X-ray binaries from tidal captures in the local Universe
• Kilogauss magnetic field and jet dynamics in the quasar NRAO 530
• Direct detection of Ultra-High Energy WIMPs with a satellite detector like JEM-EUSO
• Constraints on Multicomponent Dark Energy from Cosmological Observations
• VEGA: Voids idEntification using Genetic Algorithm
• Analytic expressions for the background evolution of massive neutrinos and dark matter particles
• The Pseudo Evolution of Galaxy-Cluster Masses and Its Connection to Mass Density Profile
• What determines the maximum stellar surface density of galaxies?
• Dark matter candidate induced by Horndeski theory: dark matter halo and cosmological evolution
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• Detectability of Massive Boson Stars using Gravitational Waves from Fundamental Oscillations
• The SRG/eROSITA all-sky survey: Constraints on Ultra-light Axion Dark Matter through Galaxy Cluster Number Counts
• The Complexity and Information Content of Simulated Universes
• Cosmology of the non-local Proca theory
• Relativistic mean-field corrections for interactions of dark matter particles with nucleons
• Detecting Fluorescent Dark Matter with X-ray lasers
• Bright [CII]158$\mu$m Streamers as a Beacon for Giant Galaxy Formation in SPT2349$-$56 at $z=4.3$
• Noether symmetry approach in non-minimal derivative coupling gravity
• LOFAR Deep Fields: Probing the sub-mJy regime of polarized extragalactic sources in ELAIS-N1. II. Analysis
• Too small to succeed: the difficulty of sustaining star formation in low-mass haloes
• Data-driven Cosmology from Three-dimensional Light Cones
• Mass function of stellar black holes as revealed by the LIGO-Virgo-KAGRA observations
• Studying baryon acoustic oscillations using photometric redshifts from the DESI Legacy Imaging survey DR9
• Dark Matter and Electroweak Baryogenesis with Spontaneous $CP$ Violation in the Early Universe
• Observational scalings testing modified gravity
• Numerical effects on the stripping of dark matter and stars in IllustrisTNG galaxy groups and clusters
• A Comparative Test of the LCDM and R_h=ct Cosmologies Based on Upcoming Redshift Drift Measurements
• Star-forming galaxies in the cosmic web in the last 11 Gyr
• A mock redshift catalogue of the dusty star-forming galaxy population with intrinsic clustering and lensing for deep millimetre surveys
• Dark matter, extra-terrestrial gamma-rays and the MSSM: a viability study
• The Impact of $\text{CLEAN}$ing on Strong Gravitational Lens Modelling
• Phantom Domain Walls
• Fast map-based simulations of systematics in CMB surveys including effects of the scanning strategy
• On the evolution of Betti curves in the Cosmic web
• Role of Spatial Curvature in a Dark Energy Interacting Model
• The Hidden Role of Anisotropies in Shaping Structure Formation in Cosmological N-Body Simulations
• Z-Sequence: Photometric redshift predictions for galaxy clusters with sequential random k-nearest neighbours
• An alternative attractor in gauged NJL inflation
• Classifying merger stages with adaptive deep learning and cosmological hydrodynamical simulations
• A MeerKAT study of a neutral hydrogen rich grouping of galaxies with megaparsec-scale filamentary-like structure
• Cosmic no-hair theorems for viscous contracting Universes
• Axi-Higgs portal Dark Matter via Wess-Zumino mechanism
• Chameleon Gravity as an Alternative to Dark Matter
• Estimating the contribution of foreground halos to the FRB 180924 dispersion measure
• The signature of galaxy formation models in the power spectrum of the hydrogen 21cm line during reionization
• Probing pre-inflationary anisotropy with directional variations in the gravitational wave background
• The impact of baryons on the sparsity of simulated galaxy clusters from The Three Hundred Project
• Limits on the existence of totally reflective exotic compact objects with current and future gravitational-wave detectors
• Spatial correlations of extended cosmological structures
• Perturbation theory challenge for cosmological parameters estimation II.: Matter power spectrum in redshift space
• Magnetic fields in the intracluster medium with TNG-Cluster: properties, morphology, and tangential anisotropy
• Observational biases on rotation curves from IFU data at cosmic noon
• A Redshift Survey of the Coma Cluster (A1656): Understanding the Nature of Subhalos in the Weak-lensing Map
• Fixing cosmological constant on the event horizon
• Reconstruction of real-space linear matter power spectrum from multipoles of BOSS DR12 results
• Quantum interference among heavy NMSSM Higgs bosons
• The Three Hundred Project: dissecting the fundamental plane of galaxy clusters up to $z=1$
• Comparative testing of dark matter models with 15 HSB and 15 LSB galaxies
• Neutrino mass and the Higgs portal dark matter in the ESSFSM
• Effect of the Cosmological Constant on Halo Size
• Note on Thermalization of Non-resonantly Produced Sterile Neutrinos
• An overview of DarkBit, the GAMBIT dark matter module
• Model-independent constraints on clustering and growth of cosmic structures from BOSS DR12 galaxies in harmonic space
• The cusp properties of High Harmonic Loops
• Breaking degeneracies with the Sunyaev-Zeldovich full bispectrum
• Approximate Likelihood Approaches for Detecting the Influence of Primordial Gravitational Waves in Cosmic Microwave Background Polarization
• CMB anisotropies at all orders: the non-linear Sachs-Wolfe formula
• Mapping the cosmic expansion history from LIGO-Virgo-KAGRA in synergy with DESI and SPHEREx
• Accounting for Correlations When Fitting Extra Cosmological Parameters
• VST ATLAS Galaxy Cluster Catalogue I: cluster detection and mass calibration
• Diverse Rotation Curves of Galaxies in a Simulated Universe: the Observed Dependence on Stellar Mass and Morphology Reproduced
• Collins in Wonderland
• The running of featureful primordial power spectra
• A stellar dynamical mass measurement of an inactive black hole at redshift 2
• Search for Slow Bars in Two Barred Galaxies with Nuclear Structures: NGC 6951 and NGC 7716
• Minicharged Particle Sensitivity of the MAPP Outrigger Detector
• Some perspective of thermodynamical and optical properties of black holes in Maxwell-dilaton-dRGT-like massive gravity
• LATIS Data Release: $\sim 4200$ Spectra of $z\sim 2-3$ Galaxies, Redshifts, and Intergalactic Medium Tomography Maps
• Interacting tachyon with varying mass dark matter
• Ads spacetime in Lorentz covariant gauges
• Linear growth of structure in massive gravity
• Tracing black hole and galaxy growth across environments since cosmic noon
• Unifying turnaround-bounce cosmology in a cyclic universe considering a running vacuum model
• Testing for directionality in the Planck polarization and lensing data
• Dynamical analysis of Brans-Dicke Universe with inverse power-law effective potential
• Perturbation Theory Remixed II: Improved Modeling of Nonlinear Bispectrum
• Gravitational Waves with Dark Energy
• Detecting and analysing the topology of the cosmic web with spatial clustering algorithms I: Methods
• X-Ray Spectral Variability of the TeV HBL Blazar PG 1553+113 with XMM-Newton
• Can luminous Lyman alpha emitters at $z$ $\simeq$ 5.7 and $z$ $\simeq$ 6.6 suppress star formation?
• Eternally oscillating zero energy Universe
• Cosmological Dynamics of Exponential Quintessence Constrained by BAO, Cosmic Chronometers, and DES-SN5YR/Pantheon+ Data
• The CMB angular power spectrum via component separation: a study on Planck data
• Detecting PAHs in high-z galaxies in proxy: Modelling physical conditions in an extremely strong damped Lyman-alpha absorber towards QSO SDSS J1143+1420 at z=2.323
• Singularities and Conjugate Points in FLRW Spacetimes
• The Role of Mass and Environment on Satellite distributions around Milky Way analogs in the Romulus25 simulation
• Galaxy And Mass Assembly (GAMA): The Dependence of Star Formation on Surface Brightness in Low Redshift Galaxies
• Probing stops in the coannihilation region at the HL-LHC: a comparative study of different processes
• Diffuse flux of PeV neutrinos from centrifugally accelerated protons in active galactic nuclei
• Measurement of the Hubble constant using the Dark Energy Survey Year 6 Gold galaxy catalogue and the fourth Gravitational-Wave Transient Catalogue
• Measurement prospects for the pair-instability mass cutoff with gravitational waves
• Growing in number, passive in nature: tracing the evolution of the most massive quiescent galaxies since z ~ 0.8 with BOSS and DESI
• Free-floating molecular clumps and gas mixing: hydrodynamic aftermaths of the intracluster$-$interstellar medium interaction
• Disc instability and bar formation: view from the IllustrisTNG simulations
• The assembly history of NGC 1365 through chemical archaeology
• Estimating Cluster Masses from SDSS Multi-band Images with Transfer Learning
• The Forward Physics Facility at the High-Luminosity LHC
• The impact of lunar topography on the 21-cm power spectrum for grid-based arrays : Insights for the Dark-ages EXplorer (DEX)
• A Hamiltonian, post-Born, three-dimensional, on-the-fly ray tracing algorithm for gravitational lensing
• Implications of Mixed Axion-Neutralino Dark Matter
• Holographic Ricci DE as running vacuum with nonlinear interactions
• On Nash theory of gravity with matter contents
• Multiphase Powerful Outflows Detected in High-z Quasars
• A first look at a complete view of spatially resolved star formation at 1<z<1.8 with JWST NGDEEP+FRESCO slitless spectroscopy
• Revealing the formation histories of the first stars with the cosmic near-infrared background
• ODIN: Using multiplicity of Lyman-Alpha Emitters to assess star formation activity in dark matter halos
• Implementing spectra response function approaches for fast calculation of power spectra and bispectra
• Measuring the baryon fraction in cluster of galaxies with Kinematic Sunyaev Zeldovich and a Standard Candle
• The impact of precession and higher-order multipoles for gravitational wave cosmological inference
• Galaxy assembly bias in cosmological hydrodynamical simulations: a comparison between SIMBA and IllustrisTNG
• Naturalness in Soft Leptogenesis and Gravitino Mass Bound due to Primordial Black Holes
• X-ray analysis of the Planck-detected triplet-cluster system PLCK G334.8-38
• High-energy Neutrinos from Stellar Explosions in Active Galactic Nuclei Accretion Disks
• Lensing by primordial black holes: constraints from gravitational wave observations
• Combined lensed estimator to probe the post reionization H I power spectrum
• Galaxy-halo internal alignments across cosmic time
• Observing the influence of growing black holes on the pre-reionization IGM
• Using Strong Lensing to Detect Subhalos with Steep Inner Density Profiles
• Symmetry restoration due to preheating and lepton number asymmetry
• Neural Post-Einsteinian Test of General Relativity with the Third Gravitational-Wave Transient Catalog
• Precision Cosmology in Modified and Extended Theories of Gravity: an insightful test
• The Hosts of X-ray Absorption Lines Toward AGNs
• SKYSURF-11: A New Zodiacal Light Model Optimized for Optical Wavelengths
• Archival Inference for Eccentric Stellar-Mass Binary Black Holes in Space-Based Gravitational Wave Observations
• Deriving accurate galaxy cluster masses using X-ray thermodynamic profiles and graph neural networks
• The SRG/eROSITA All-Sky Survey. Detection of shock-heated gas beyond the halo boundary into the accretion region
• Probing Systematic Bias in Low-Redshift Type Ia Supernova Measurements by Cross Analyzing Surface Brightness and Hubble Residuals
• Galaxy-galaxy strong lens perturbations: line-of-sight haloes versus lens subhaloes
• The impact of cosmic filaments on the abundance of satellite galaxies
• Observing Double White Dwarfs with the Lunar GW Antenna
• Black-hole mass estimation through accretion disk spectral fitting for high-redshift blazars
• Detecting the hidden population of low-mass haloes in strong lenses
• Mitigating the impact of fiber assignment on the measurement of galaxy-lensing cross correlation
• Galaxy Velocity Bias in Cosmological Simulations: Towards Percent-level Calibration
• Interplanetary Dust as a Foreground for the LiteBIRD CMB Satellite Mission
• Modified Cosmology or Modified Galaxy Astrophysics is Driving the z>6 JWST Results? CMB Experiments can discover the Origin in the Near Future
• Investigating the residuals in the $M_{\bullet }-M_{\ast }$ relation using the SIMBA cosmological simulation
• Acceleration of cosmic expansion through huge cosmological constant progressively reduced by submicroscopic information transfer
• GRB160203A: an exploration of lumpy space
• Effect of high harmonic loops on gravitational wave bounds from cosmic strings
• Vacuum arbitrariness and the Hubble tension
• Quarks to Cosmos: Particles and Plasma in Cosmological evolution
• Systematics in ETG Mass Profile Modelling: Strong Lensing & Stellar Dynamics
• Constraining Merging Galaxy Clusters with X-ray and Lensing Simulations and Observations: The case of Abell 2146
• The Brown Dwarf Kinematics Project (BDKP). V. Radial and Rotational Velocities of T Dwarfs from Keck/NIRSPEC High-Resolution Spectroscopy
• Predicting the resolved CO emission of $z=1-3$ star-forming galaxies
• Exploiting Non-linear Scales in Galaxy-Galaxy Lensing and Galaxy Clustering: A Forecast for the Dark Energy Survey
• Search for light dark matter with NEWS-G
• Performance of the First 150 mm Diameter Cryogenic Silicon Ionization Detectors with Contact-Free Electrodes
• Leptonic Dark Matter with Scalar Dilepton Mediator
• Delensing CMB B-modes using galaxy surveys: the effect of galaxy bias and matter clustering non-linearities
• Inflation Story: slow-roll and beyond
• The PARADIGM project II: The lifetimes and quenching of satellites in Milky Way-mass haloes
• Local dark energy in the Sculptor Filament of galaxies
• Radiative transfer of 21-cm line through ionised cavities in an expanding universe
• Low-luminosity galaxies in the early universe have observed sizes similar to star cluster complexes
• "Observations" of simulated dwarf galaxies: Star-formation histories from color-magnitude diagrams
• Does the Reionization Model Influence the Constraints on Dark Matter Decay or Annihilation?
• Using strong gravitational lensing to probe the post reionization \HI power spectrum
• Towards an Observational Detection of Halo Spin Bias using Spin-Orbit Coherence
• AGN with massive black holes have closer galactic neighbors: k-Nearest-Neighbor statistics of an unbiased sample of AGN at z~0.03
• Impact of the large-scale cosmic web on the X-ray emitting circumgalactic medium
• Extreme Digitisation For Ground-Based Cosmic Microwave Background Experiments
• First joint absorption and T${}_e$-based metallicity measured in a GRB host galaxy at $z=4.28$ using JWST/NIRSpec
• Predicting the SUSY breaking scale in SUGRA models with degenerate vacua
• Observational constraints on the free parameters of an interacting Bose-Einstein gas as a dark-energy model
• Resolved Neutral Outflow from a Lensed Dusty Star Forming Galaxy at z=2.09
• Black hole ringdown spectroscopy of curvature-coupled scalar and pseudoscalar fields
• Signatures of Hierarchical Mergers in Black Hole Spin and Mass distribution
• Soft X-ray line emission from hot gas in intervening galaxy halos and diffuse gas in the cosmic web
• Forecasts on Interacting Dark Energy from 21-cm Angular Power Spectrum with BINGO and SKA observations
• Fast Luminous Blue Transients in the Reionization Era and Beyond
• Listening Across the Cosmic Time: Standard Sirens from Ground- and Space-Based Missions in the Next Decade
• A group finder algorithm optimised for the study of local galaxy environment
• Quantization ambiguities and the robustness of effective descriptions of primordial perturbations in hybrid Loop Quantum Cosmology
• Flat Space, Dark Energy, and the Cosmic Microwave Background
• First Light And Reionization Epoch Simulations (FLARES) -- XIX: Supermassive black hole mergers in the early Universe and their environmental dependence
• Insights into the dependence of galaxy properties on the environment with explainable machine learning models
• SNITCH: Seeking a simple, informative star formation history inference tool
• Triplet scalar flavored leptogenesis with spontaneous CP violation
• On the dependence of galaxy assembly bias on the selection criteria, number density, and redshift of galaxy samples
• Search for the Optical Counterpart of Einstein Probe Discovered Fast X-ray Transients from Lulin Observatory
• Matter-antimatter asymmetry in generalized coupling theories
• An Interpretation of the Cosmic Ray $e^{+}+e^{-}$ Spectrum from 10 GeV to 3 TeV Measured by CALET on the ISS
• Compact groups from semi-analytical models of galaxy formation -- VI: Evolution of the two first-ranked galaxies
• JWST Spectroscopic View of a Rapidly Growing Dust-obscured Quasar at $z\sim 4$: Effect of Dust Extinction Correction on Black Hole Mass and Eddington Ratio Estimation
• Emulating the Non-Linear Matter Power-Spectrum in Mixed Axion Dark Matter Models
• The abundance and origin of cool gas in galaxy clusters in the TNG-Cluster simulation
• Thermodynamics of sign-switching dark energy models
• Prospects for constraining quasar ages with fiber spectrographs: quasar-induced Ly$\alpha$ emission from the intergalactic medium
• Dissecting the Thermal SZ Power Spectrum by Halo Mass and Redshift in SPT-SZ Data and Simulations
• A Hierarchical Shock Model of Ultra-High-Energy Cosmic Rays
• Searching for continuous gravitational waves from highly deformed compact objects with DECIGO
• The Effects of Spatial Curvature on Cosmic Evolution
• One Galaxy Sample to Rule Them All: Halo Occupation Distribution Modeling of DES Year 3 Source Galaxies
• ComPACT: ACT+Planck galaxy cluster catalogue
• Sommerfeld Enhancements for Asymmetric Dark Matter
• Galaxy clustering in modified gravity from full-physics simulations. I: two-point correlation functions
• Cosmology with 21cm intensity mapping
• Remarks on cosmological gravitational waves
• Galactic sparsity and $\Lambda$-gravity
• A Search for Low-frequency Radio Pulses from Long Gamma-ray Bursts with the Murchison Widefield Array
• Thorne-Żytkow objects with mirror neutron star cores?
• Cosmic Microwave Background as a thermal gas of SU(2) photons: Implications for the high-z cosmological model and the value of $H_0$
• Standard candles and sirens rescue $H_0$
• Cosmic Microwave Background Science at Commercial Airline Altitudes
• Analysis of the angular dependence of time delay in gravitational lensing
• Big-Bang Nucleosynthesis on a bubble universe nucleated in Kerr-AdS${}_5$ Black Hole
• Using two point correlation functions to understand the assembly histories of Milky Way-like galaxies
• 21-cm power spectrum and ionization bias as a probe of long-mode modulated non Gaussian sky
• Measuring the Stellar-to-Halo Mass Relation at $\sim 10^{10}$ Solar masses, using forthcoming space-based imaging of galaxy-galaxy strong lenses
• Constraining the scalar singlet and inert dark matter models using neutron stars
• Gravitational baryogenesis of cosmological constant dominated universe
• Primordial Black Holes Formed during Magneto-Hydrodynamic Turbulence in The Early Universe as Dominant Part of Dark Matter
• Probing Time-Dependent Dark Energy with the Flux Power Spectrum of the Lyman $\alpha$ Forest
• Astrophysical and Cosmological Relevance of the High-Frequency Features in the Stochastic Gravitational-Wave Background
• Cosmology with Type II Supernovae
• Statistical biases in parametrized searches for gravitational-wave polarizations
• The catalogue of virtual early-type galaxies from IllustrisTNG: validation and real observation consistency
• Optical Follow-up of Planck Cluster Candidates with Small Instruments
• Detection of Unresolved Strongly Lensed Supernovae with 7-Dimensional Telescope
• CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform
• Through a Mini Halo, Darkly
• Constraining primordial black hole abundance with Insight-HXMT
• Phenomenological Analysis of an ${\mathrm{E}}_6$-inspired Seesaw Model
• On the role of dust in the microwave emission of galactic halos
• Getting the Most Neutrinos out of IsoDAR
• State of practice: evaluating GPU performance of state vector and tensor network methods
• A novel mechanism for the distance-redshift relation
• Does History Repeat Itself? Periodic Time Cosmology
• Searching for MeV-mass neutrinophilic Dark Matter with Large Scale Dark Matter Detectors
• On the invalidity of "negative mass" description of the dark sector
• Black Holes and Non-perturbative Gravitational Waves in $f(R)$ Gravity
• The mass and redshift dependence of halo star clustering
• Interpreting deviations between AR-VTG and GR
• Gamma-ray bursts at extremely small fluence
• Star-formation Properties of z ~ 1 Galaxy Clusters and Groups from Horizon Run 5
• Toward accurate measurement of property-dependent galaxy clustering: II. Tests of the smoothed density-corrected $V_{\max }$ method
• Exploring the evolution of red and blue galaxies in different cosmic web environments using IllustrisTNG simulation
• Double power series method for approximating cosmological perturbations
• Largest scales from the largest galaxy surveys: the pseudo Karhunen-Loève method
• The holographic principle comes from finiteness of the universe's geometry
• The multi-component fitting to the star formation histories in the TNG simulation
• Intervening nuclear obscuration changing the X-ray look of the $z\approx 6$ QSO CFHQS J164121+375520
• Constraining cosmology with N-body simulations for future spectroscopic galaxy surveys at $2\le z\le 3$
• Nonperturbative collapse models for collisionless self-gravitating flows
• Probing time orientability of spacetime
• Radio Galaxies in SIMBA: A MIGHTEE Comparison
• The cosmological nature of the dark Universe
• Cosmological implications of electromagnetically interacting dark matter: milli-charged particles and atoms with singly and doubly charged dark matter
• The Baryonic Mass Estimates of the Milky Way Halo in the form of High Velocity Clouds
• A study on late time UV-emission in core collapse supernovae and the implications for the peculiar transient AT2018cow
• Gas thermodynamics meets galaxy kinematics: Joint mass measurements for eROSITA galaxy clusters
• Emergence of the Galaxy Morphology-Star Formation Activity-Clustercentric Radius Relations in Galaxy Clusters
• Inference of morphology and dynamical state of nearby $Planck$-SZ galaxy clusters with Zernike polynomials
• First IFU observations of two GRB host galaxies at cosmic noon with JWST/NIRSpec
• A new mechanism for generating particle number asymmetry through interactions
• On observational signatures of multi-fractional theory
• Finite geometry and black hole stability: Embedding discrete space into classical manifolds
• A positive correlation between broad HI Ly$\alpha$ absorptions and local overdensities of galaxies
• Simulating gravitational motion, gas dynamics, and structure in the cosmos
• Recent star formation in 0.5<z<1.5 quiescent galaxies
• The Three Hundred Project: A fast semi-analytic model emulator of hydrodynamical galaxy cluster simulations
• Correlation of structure growth index with current cosmic acceleration: constraints on dark energy models
• Higgs information in Split-SUSY at the LHC
• Cosmology of Quasi-Dilaton Massive Gravity with Non-minimal Kinetic Coupling
• Constraints on the Epoch of Reionization with Roman Space Telescope and the Void Probability Function of Lyman-Alpha Emitters
• Multi-wavelength properties of $z\gtrsim 6$ LISA detectable events
• Early galaxy evolution: The complex interstellar medium distribution of the z~7 galaxy A1689-zD1
• Revisiting Galaxy Cluster Scaling Relations through Dark Matter-Gas Coherence: Scatter Dependence on Dynamical State
• Spatial Dependence of the Growth Factor in Scalar-Tensor Cosmology
• The Spitzer Extragalactic Representative Volume Survey and DeepDrill extension: clustering of near-infrared galaxies
• An Interpretable AI Framework to Disentangle Self-Interacting and Cold Dark Matter in Galaxy Clusters: The CKAN Approach
• The Filament Rift: $\Lambda$CDM's Structural Challenge Against Observation
• The impact of radial migration on disk galaxy star formation histories: II. Role of bar strength, disk thickness, and merger history
• Deep Learning generated observations of galaxy clusters from dark-matter-only simulations
• The Thermodynamic and Kinematic Evolution of Circumgalactic Gas around $z=1$ in the IllustrisTNG model
• The effects of self-interacting dark matter on the stripping of galaxies that fall into clusters
• Tracing correlations between galaxy properties across the Cosmic Web: An IllustrisTNG-based study
• A Radio Continuum Study of NGC 2082
• Capability for detection of GW190521-like binary black holes with TianQin
• Direct Measurement of Upward-going Ultrahigh Energy Dark Matter at the Pierre Auger Observatory
• Exploring the Voids: Luminosity Functions and Magnetic Field
• The Bias to Cosmic Microwave Background Lensing Reconstruction from the Kinematic Sunyaev-Zel'dovich Effect at Reionization
• Particle-antiparticle oscillation modes crossing horizon: baryogenesis and dark-matter waves
• Cosmological implications of the full shape of anisotropic clustering measurements in BOSS and eBOSS
• The origin of the intra-cluster light in The Three Hundred simulations
• Modeling supernova feedback in galaxy formation simulations with energy-conserving momentum injection
• Inflationary epoch in the presence of holographic dark energy
• $keV$ sterile neutrino as dark matter in doublet left-right symmetric model with $A_4$ modular symmetry
• Ultra-fast model emulation with PRISM; analyzing the Meraxes galaxy formation model
• A test of MOND and Emergent Gravity with SMACS J0723.3-7327 using eROSITA observations
• Testing a New Star Formation History Model from Principal Component Analysis to Facilitate Spectral Synthesis Modeling
• A bubble size distribution model for the Epoch of Reionization
• Constraints on dark matter annihilation and turbulent reacceleration set by high-frequency observations of the radio halo in the Coma cluster
• Inflation in a scalar-vector gravity theory
• The evolution of extragalactic peaked-spectrum sources down to 54 megahertz
• How Dark is Dark Energy? A Lightcones Comparison Approach
• Galaxy rotation curves in the light of the Spinor Theory of Gravity
• R-Symmetric NMSSM
• Bispectrum of induced gravitational waves in the poltergeist mechanism
• Phase space analysis of Bianchi III Universe with $f(R,T)$ gravity theory
• A 400 Trillion-Grid Vlasov Simulation on Fugaku Supercomputer: Large-Scale Distribution of Cosmic Relic Neutrinos in a Six-dimensional Phase Space
• Galaxy Proximate Damped Lyman-Alpha Systems and HI Reionization Topology in TECHNICOLOR DAWN
• Can accelerated expansion of the universe be due to spacetime vorticity?
• Implications of baryon-dark matter interaction on IGM temperature and tSZ effect with magnetic field
• Impact of particle production during inflation on the CMB detection
• Halo spin and orientation in Interacting Dark Matter Dark Energy Cosmology
• A probabilistic deep learning model to distinguish cusps and cores in dwarf galaxies
• Black Hole Zeroth Law in Horndeski Gravity
• How to Build an Empirical Speed Distribution for Dark Matter in the Solar Neighborhood
• Dark Matter profiles of "in silico" galaxies: deep learning inference
• Upper limits on Einstein's weak equivalence principle placed by uncertainties of dispersion measures of fast radio bursts
• Cross-tests of CMB features in the primordial spectra
• Exploring the Viability of $f(Q,T)$ Gravity: Constraining Parameters with Cosmological Observations
• A joint measurement of galaxy luminosity functions and large-scale field densities during the Epoch of Reionization
• Using strong lensing to understand the microJy radio emission in two radio quiet quasars at redshift 1.7
• Gravitational background from dynamical binaries and detectability with 2G detectors
• Testing the key role of the stellar mass-halo mass relation in galaxy merger rates and morphologies via DECODE, a novel Discrete statistical sEmi-empiriCal mODEl
• Primordial Perturbations Including Second-Order Derivatives of the Inflationary Potential
• Unveiling the evolution of the CO excitation ladder through cross-correlation of CONCERTO-like experiments and galaxy redshift surveys
• No Stream Left Unscathed: The imprint of a host galaxy
• Mesoscopic Energy Ranking Constraints in the IllustrisTNG Simulations
• Can we remove the systematic error due to isotropic inhomogeneities?
• Constraints on energy scales from dark matter decay in a gauged $B-L$ model
• HI Observations of Baryon-Dominated Dwarf Galaxy Candidates
• A New Gamma-ray Emitting Population of FR0 Radio Galaxies
• Merger fraction in galaxy groups and clusters at z < 0.2: A non-parametric morphological study with Subaru Hyper Suprime-Cam
• Particle Cosmology
• Beyond single tracers: CNN-based inference of galaxy mass profiles from combined gas and stellar kinematics
• A Gravitational Wave Background from Primordial Black Hole Lattices in Matter Dominated Era
• Viscous Dark Energy Accretion Activities : Sonic Speed, Angular Momentum and Mach Number Studies
• OO Dra: an Algol-type binary formed through an extremely helium-poor mass accretion revealed by asteroseismology
• Constraints on the dark energy dipole from large-scale structures
• Enhancing Cosmological Constraints by Two-dimensional $\beta$-cosmic-web Weighted Angular Correlation Functions
• Kalb-Ramond field induced cosmological bounce in generalized teleparallel gravity
• Accelerating reionization constraints: An ANN-emulator framework for the SCRIPT Semi-numerical Model
• Exploring the constraints on cosmological models with CosmoEJS
• Quasar clustering at redshift 6
• Estimating the triaxiality of massive clusters from 2D observables in MillenniumTNG with machine learning
• Characterizing Binary Black Hole Subpopulations in GWTC-4 with Binned Gaussian Processes: On the Origins of the $35M_{\odot }$ Peak
• Mimicking the halo-galaxy connection using machine learning
• Ranking Theoretical Supernovae Explosion Models from Observations of the Intracluster Gas
• Energy and waiting time distributions of FRB 121102 observed by FAST
• Search for the production of dark fermion candidates in association with heavy neutral gauge boson decaying to dimuon in proton-proton collisions at $\sqrt{s}=8$ TeV using the CMS open data
• Cosmological aspects of cubic Galileon massive gravity
• SuperModel Predictions in the Outskirts of the Galaxy Cluster Zwicky 3146
• Forbidden Channels and SIMP Dark Matter
• The origin of ionized gas in retired galaxies: dynamical clues
• Probing beyond-Horndeski gravity on ultra-large scales
• The most distant optically polarised GRB afterglow: GRB 240419A at z = 5.178
• Galaxy cluster temperature maps from joint X-ray and SZ maps with The Three Hundred hydrodynamical simulations
• Effect of dark matter halos on the orbital and escape dynamics of barred galaxies
• Exploring the CMB Power Suppression in Canonical Inflation Models
• Evolution of matter perturbations in the context of cosmic slowing down
• The frame-dragging vector potential on galaxy scales from Dark-Matter-only Newtonian $N$-body simulations
• Cosmic magnification in beyond-Horndeski gravity
• Axion-like Particle Search with a Light-Shining-Through-Walls Setup at a $\gamma$-$\gamma$ Collider
• Alignment of the central galaxies with the environment
• CWTHF: Subhalo Identification with Continuous Wavelet Transform
• The Glow of Axion Quark Nugget Dark Matter: (IV) CMB Spectral and Anisotropy Signatures
• A Mass Dependent Density Profile from Dwarfs to Clusters
• Mirror magnetic field and its impact on dark matter distribution in galaxies
• Spatially non-parametric recovery of intrinsic kinematic maps in pre- to post-merger galaxies
• Galaxy mergers can initiate quenching by unlocking an AGN-driven transformation of the baryon cycle
• On gravitational preheating
• Can Eccentric Binary Black Hole Signals Mimic Gravitational-Wave Microlensing?
• Cross-correlations between mm-wave line-intensity mapping and weak lensing surveys: preliminary consideration of long-term prospects
• Prospects for distinguishing dynamical tides in inspiralling binary neutron stars with third generation gravitational-wave detectors
• Galaxy clustering in the VVV Near-IR Galaxy Catalogue
• Implications of the cosmological 21-cm absorption profile for high-redshift star formation and deep JWST surveys
• Neutrino Condensate Dark Energy from TeV Scale Extra Dimensions
• Searching Far and Long I: Pilot ALMA 2mm Follow-up of Bright Dusty Galaxies as a Redshift Filter
• Galaxy And Mass Assembly (GAMA): Deconstructing the galaxy stellar mass function by star formation and environment
• Dark photon searches via Higgs boson production at the LHC and beyond
• Evaluating quenching in cosmological simulations of galaxy formation with spectral covariance in the optical window
• Merger rates of intermediate-mass black hole binaries in nuclear star clusters
• Impact of correlated seismic and correlated Newtonian noise on the Einstein Telescope
• Observed cosmic evolution of galaxy dust properties with metallicity and tensions with models
• Unravelling the role of merger histories in the population of In situ stars: linking IllustrisTNG cosmological simulation to H3 survey
• A Study of Systematics on the Cosmological Inference of the Hubble Constant from Gravitational Wave Standard Sirens
• Phase space analysis and cosmography of a two-fluid cosmological model
• Newcomers and suburbanites can drive the evolution of the size-stellar mass relation of early type galaxies in galaxy clusters
• Enhancing online estimation of CBC parameters with the low-latency MBTA analysis
• The 21-cm signal from the Cosmic Dawn: metallicity dependence of high mass X-ray binaries
• Modeling Cosmological Evolution of Jetted Seyfert Galaxies for z<10
• Marked statistics across the cosmic web: Environmental dependent clustering in modified gravity simulations
• Constraints on the velocity dispersion of Dark Matter from Cosmology and new bounds on scattering from the Cosmic Dawn
• Testing subhalo abundance matching with galaxy kinematics
• A Population Study for Searching Supermassive Binary Black Holes in Active Galactic Nuclei: Continuum Spectral Features and Periodic Variabilities
• NeutralUniverseMachine: Predictions of HI gas in Different Theoretical Models
• Simulating Jellyfish Galaxies: A Case Study for a Gas-Rich Dwarf Galaxy
• RXTE Observation of the Non-thermal Emission from the Early Stage Merger in Abell 1750
• The role of gas fragmentation during the formation of supermassive black holes
• The interplay between AGN feedback and precipitation of the intracluster medium in simulations of galaxy groups and clusters
• The BINGO project X. Cosmological parameter constraints from HI Intensity Mapping lognormal simulations
• Hubble Expansion Signature on Simulated Halo Density Profiles: A Path to Observing the Turnaround Radius
• The detectability of bars at high redshift: a case study using Euclid-like mock observations of TNG50 simulated galaxies
• Accidental deep field bias in CMB T and SNe $z$ correlation
• Interacting dark matter and q-deformed dark energy non-minimally coupled to gravity
• Training Custom Light Curve Models of SN Ia Sub-Populations Selected According to Host Galaxy Properties
• Inflationary study of non-Gaussianity using two-dimensional geometrical measures of CMB temperature maps
• Extended Haloscope Search and Exclusion of a Candidate Signal near 1.036 GHz
• Co-evolution of the Brightest Cluster Galaxies and their Host Clusters in IllustrisTNG
• Unclustered tracers remain unclustered: the lack of primordial non-Gaussianity response of bias-zero tracers
• Dwarf Galaxy Number Counts within 25 Mpc: Predictions from Local Group Analogues in TNG50
• Morphologies for DECaLS Galaxies through a combination of non-parametric indices and machine learning methods: A comprehensive catalog using the Galaxy Morphology Extractor (galmex) code
• New leaves of the tree: percolation analysis for cosmic web with discrete points
• Forged by Feedback: Stellar Properties of Brightest Group Galaxies in Cosmological Simulations
• Cosmological simulations predict that AGN preferentially live in gas-rich, star-forming galaxies despite effective feedback
• Generating Galaxy Clusters Mass Density Maps from Mock Multiview Images via Deep Learning
• Asymmetric Dark Matter Abundance Including Non-thermal production
• The life and times of dark matter haloes: what will I be when I grow up?
• The stability analysis of the extended singlet scalar model with two high scale minima
• 3D scaling laws and projection effects in The300-NIKA2 Sunyaev-Zeldovich Large Program Twin Samples
• UltraDark.jl: A Julia package for simulation of cosmological scalar fields
• Tidal disruption of solitons in self-interacting ultralight axion dark matter
• Deciphering the ultra-steep spectrum diffuse radio sources discovered in the cool-core cluster Abell~980
• Mitigating Cosmic Microwave Background Shadow Degradation of Tensor-to-scalar Ratio Measurements through Map-based Studies
• The Distribution of Satellite Galaxies in the TNG100 Simulation
• The impact of black hole feedback on the UV luminosity and stellar mass assembly of high-redshift galaxies
• Constraining Quintessence Models with ISW-tSZ Cross-Correlations: A Comparative Analysis of Thawing, Tracker, and Scaling-Freezing Dynamics
• Uncovering the absorbed atomic Universe with the [OI]63um line
• On the Tidal Formation of Dark Matter Deficient Galaxies
• A Non-parametric Method for the Inference of Halo Occupation Distributions
• Do photons travel faster than gravitons?
• Quantifying the Poor Purity and Completeness of Morphological Samples Selected by Galaxy Colour
• The nonlinear equation of correlation function of galaxies in the expanding universe and the solution in linear approximation
• Exploratory scenarios for the differential nuclear and tidal evolution of TZ Fornacis
• SF-R You Sure? The Conflicting Role of Star Formation Rates in Constraining the Evolution of Milky Way Analogues in Cosmological Simulations
• Radio Galaxy Zoo: Giant Radio Galaxy Classification using Multi-Domain Deep Learning
• Inferring the mass of the circumgalactic medium using X-ray resonant scattering
• Implications of correlations and fluctuations in small systems
• Cosmological constraints on the decay of heavy relics into neutrinos
• The galaxy starburst/main-sequence bimodality over five decades in stellar mass at z ~ 3-6.5
• Where within the 3C 84 jet are $\gamma$-rays produced?
• Timing the last major merger of galaxy clusters with large halo sparsity
• $TeV$-Scale Resonant Leptogenesis with New Scaling Ansatz on Neutrino Dirac Mass Matrix from $A_4$ Flavor Symmetry
• Searches for Compact Binary Coalescence Events Using Neural Networks in LIGO/Virgo Third Observation Period
• Optimizing Foreground Modelling for Global 21cm Cosmology with GPU-Accelerated Nested Sampling
• Probing the low-energy spectrum of non-thermal electrons in galaxy clusters with soft gamma ray observations
• SDSS-IV MaNGA: A Catalogue of Spectroscopically Detected Strong Galaxy-Galaxy Lens Candidates
• DeepVoid: A Deep Learning Void Detector
• Probing gravity with non-linear clustering in redshift space
• Fast Baryonic Field Painting for Sunyaev-Zel'dovich Analyses: Transfer Function vs. Hybrid Effective Field Theory
• Forecasting Galaxy Cluster HI Mass Recovery with CHIME at Redshifts z = 1 and 2 via the IllustrisTNG Simulations
• Predicting Halo Formation Time Using Machine Learning
• Modelling the host galaxies of binary compact object mergers with observational scaling relations
• Universality of the halo mass function in modified gravity cosmologies
• Comparison of simulations and semi-analytical model for WDM subhalo mass functions
• Super Interacting Dark Sector: An Improvement on Self-Interacting Dark Matter via Scaling Relations of Galaxy Clusters
• Clustering properties of TGSS radio sources
• On Weak Lensing Response Functions
• Diffusion of Cosmic Antiprotons Generated throughout the Dark Matter Halo -- A Semi-Analytical Solution for a Linear Galactic Wind Model
• Multi-frequency study of large size radio galaxies 3C 35 and 3C 284
• NaI(Tl) crystal scintillator encapsulated in two organic-scintillator layers with pulse shape data analysis
• GalSBI-SPS: a stellar population synthesis-based galaxy population model for cosmology and galaxy evolution applications
• A preliminary study about gravitational wave radiation and cosmic heat death
• AliCPT Sensitivity to Cosmic Reheating
• Redshift-space distortion from dynamical dark energy with time-dependent Lagrangian perturbation theory
• Primordial ${}^4\text{He}$ constraints on inelastic macro dark matter revisited
• Intermediate-mass black holes and contribution to extragalactic background light from Population III stars in Milky Way-like galaxies
• The Effect of a positive cosmological constant on the bounce of Loop Quantum Cosmology
• On the capability of high redshift kSZ measurement with galaxy surveys
• Assessment of normalizing flows for parameter estimation on time-frequency representations of gravitational-wave data
• Stealing galaxies from galaxy clusters
• Observing GW190521-like binary black holes and their environment with LISA
• Search for dark matter production in association with the Z${}^{\prime }$ boson at the LHC in pp collisions at $\sqrt{s}$ = 8 TeV using Monte Carlo simulations
• Impact of Sommerfeld enhancement on helium reionization via WIMP dark matter
• Constraining D-foam via the 21-cm Line
• Gravitational Lensing By a Massive Object in a Dark Matter Halo. I. Critical Curves and Caustics
• The DORCHA suite: nature, nurture, and the phase space distribution of the Milky Way's high redshift progenitors today
• A revisited Correction to the Halo Mass Function for local-type Primordial non-Gaussianity
• The BAO scale -- how standard is the standard ruler?
• The dynamical lineage of ultra-diffuse galaxies from TNG50-1
• The two-component virial theorem and the acceleration-discrepancy relation
• Structure Formation under Inelastic Two-Component Dark Matter: Halo Statistics and Matter Power Spectra in the High-$z$ Universe
• Deep ATCA and VLA radio observations of short-GRB host galaxies. Constraints on star-formation rates, afterglow flux, and kilonova radio flares
• Tracing cosmic voids with fast simulations
• Searching for Dark Photons with Existing Haloscope Data
• Axion dark matter with not quite black hole domination
• Forgotten treasures in the HST/FOC UV imaging polarimetric archives of active galactic nuclei. IV. 5 Orphaned AGNs
• Condensate decay in a radiation dominated cosmology
• The impact of the locally measured Hubble parameter on the mass of Sterile neutrino
• Non-Hermitian Gravitational Wave Scattering
• Probing possible effects of circumgalactic media on the metal content of galaxies through the mass-metallicity relationship
• Non-Gaussianity in D3-brane inflation
• B-mode polarization forecasts for GreenPol
• From simulations to observations. Methodology and data release of mock TNG50 galaxies at 0.3 < z < 0.7 for WEAVE-StePS
• An empirical nonlinear power spectrum overdensity-response
• Mass transport in galaxy discs limits black hole growth to sub-Eddington rates
• Gravitational-wave astronomy requires population-informed parameter estimation
• Measurement of anisotropy of dark matter velocity distribution using directional detection
• Finite inflation in curved space
• Blowing Star Formation Away in AGN Hosts (BAH) -- III. Serendipitous discovery of a $z\sim 2.9$ star-forming galaxy lensed by the galactic bulge of CGCG 012-070 using JWST NIRSpec
• Measuring Scaling Relationships: Fitting Technique Matters
• The LHC upper bounds for $pp\to \text{diboson}$, $t\bar{t}$ cross section on fermionic dark matter
• Sample Variance for Supernovae Distance Measurements and the Hubble tension
• Light exotic Higgs bosons at the LHC
• On the role of $\Lambda$ on accretion disks
• Gamma rays as leptonic portals to energetic neutrinos: a new Monte Carlo approach
• Iterative reconstruction excursions for Baryon Acoustic Oscillations and beyond
• Chasing Gamma-Ray Signals from Binary Neutron Star Coalescences with the Cherenkov Telescope Array: Prospects and Observing Strategies
• Mapping the emission and spectral properties of the FRI radio galaxy 3C 449 with LOFAR and the VLA
• Primordial black holes and uncertainties in the choice of the window function
• A comprehensive study of $\delta$ Scuti-type pulsators in eclipsing binaries: oscillating eclipsing Algols
• A Monte Carlo Implementation of Galactic Free-Free Emission for the EoR Foreground Models
• A semi-analytical perspective on massive red galaxies: I. Assembly history, environment & redshift evolution
• Is the acceleration scale of the radial acceleration relation tracking the cosmic expansion rate?
• Examining the Gap in the Chirp Mass Distribution of Binary Black Holes
• Scaling Relations in the Phase-Space Structure of Dark Matter Haloes
• Streaming Velocity Effects on the Post-reionization 21 cm Baryon Acoustic Oscillation Signal
• From the Densest Clusters to the Emptiest Voids: No Evidence For Environmental Effects on the Galaxy Size-Mass Relation at Low Redshift
• The Evolution of the SFR-M_* relation at 0.1<z<4: Environmental and Morphological Dependencies
• Hybrid Inflation in Quasi-minimal Supergravity with Monotonic Inflationary Potentia
• Superhorizon isocurvature fluctuations relax tensions
• Nonlinear matter terms in general scalar-tensor braneworld cosmology
• Leptogenesis in exponential $f(R)$ gravity model
• Intergalactic Medium Tomography with the Sunburst Arc
• A group of merging galaxies falling onto Abell 2142
• Neutrino phenomenology from leptogenesis
• Mass functions from the excursion set model
• Direct Collapse Pre-supermassive Black Hole Objects as Ly$\alpha$ Emitters
• Primordial gravitational waves spectrum in the interacting Bose-Einstein gas model
• Probing small-scale baryon and dark matter isocurvature perturbations with cosmic microwave background anisotropies
• The Radio and Microwave Sky as Seen by Juno on its Mission to Jupiter
• Inferring binary black holes stellar progenitors with gravitational wave sources
• An anti-correlation between barycentre offsets and velocity dispersion for highest overdensity subhalos in cosmological simulations
• The stellar population of a $z\sim 3.25$ Ly$\alpha$ emitting group associated with a damped Ly$\alpha$ absorber