Planck 2013 results. XVI. Cosmological parameters

Abstract

We present the first results based on Planck measurements of the CMB temperature and lensing-potential power spectra. The Planck spectra at high multipoles are extremely well described by the standard spatially-flat six-parameter LCDM cosmology. In this model Planck data determine the cosmological parameters to high precision. We find a low value of the Hubble constant, H0=67.3+/-1.2 km/s/Mpc and a high value of the matter density parameter, Omega_m=0.315+/-0.017 (+/-1 sigma errors) in excellent agreement with constraints from baryon acoustic oscillation (BAO) surveys. Including curvature, we find that the Universe is consistent with spatial flatness to percent-level precision using Planck CMB data alone. We present results from an analysis of extensions to the standard cosmology, using astrophysical data sets in addition to Planck and high-resolution CMB data. None of these models are favoured significantly over standard LCDM. The deviation of the scalar spectral index from unity is insensitive to the addition of tensor modes and to changes in the matter content of the Universe. We find a 95% upper limit of r<0.11 on the tensor-to-scalar ratio. There is no evidence for additional neutrino-like relativistic particles. Using BAO and CMB data, we find N_eff=3.30+/-0.27 for the effective number of relativistic degrees of freedom, and an upper limit of 0.23 eV for the summed neutrino mass. Our results are in excellent agreement with big bang nucleosynthesis and the standard value of N_eff=3.046. We find no evidence for dynamical dark energy. Despite the success of the standard LCDM model, this cosmology does not provide a good fit to the CMB power spectrum at low multipoles, as noted previously by the WMAP team. While not of decisive significance, this is an anomaly in an otherwise self-consistent analysis of the Planck temperature data.

69 pages. Matches version to appear in Astronomy & Astrophysics

References in corpus (101)

• Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
• Planck 2013 results. XVI. Cosmological parameters
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• Cosmology and the Fate of Dilatation Symmetry
• Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples
• New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy
• Planck 2013 results. I. Overview of products and scientific results
• Improved Cosmological Constraints from New, Old and Combined Supernova Datasets
• Spectra and Light Curves of Six Type Ia Supernovae at 0.511 < z < 1.12 and the Union2 Compilation
• Planck 2013 results. XXII. Constraints on inflation
• Massive neutrinos and cosmology
• Supernova Constraints and Systematic Uncertainties from the First 3 Years of the Supernova Legacy Survey
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• CFHTLenS tomographic weak lensing cosmological parameter constraints: Mitigating the impact of intrinsic galaxy alignments
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• In response to the comments by Murphy et al. (arxiv:0708.3677)

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• Vertical disc heating in Milky Way-sized galaxies in a cosmological context
• The impact of galaxy formation on the total mass, mass profile and abundance of haloes
• 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
• Star formation relations and CO SLEDs across the J-ladder and redshift
• The Atacama Cosmology Telescope: CMB Polarization at $200<\ell <9000$
• On the Validity of the Effective Field Theory for Dark Matter Searches at the LHC, Part II: Complete Analysis for the s-channel
• Coaxing Cosmic 21cm Fluctuations from the Polarized Sky using m-mode Analysis
• Multi-field Conformal Cosmological Attractors
• Long troughs in the Lyman-$\alpha$ forest below redshift 6 due to islands of neutral hydrogen
• Cosmic evolution and metal aversion in super-luminous supernova host galaxies
• Flavour Covariant Transport Equations: an Application to Resonant Leptogenesis
• Far-infrared Fine-Structure Line Diagnostics of Ultraluminous Infrared Galaxies
• Thermal axion production
• The Sherwood simulation suite: overview and data comparisons with the Lyman-alpha forest at redshifts 2 < z < 5
• A Second Higgs Doublet in the Early Universe: Baryogenesis and Gravitational Waves
• The BAHAMAS project: the CMB--large-scale structure tension and the roles of massive neutrinos and galaxy formation
• Identification of the brightest Lyα emitters at z=6.6: implications for the evolution of the luminosity function in the re-ionisation era
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the correlation function of LOWZ and CMASS galaxies in Data Release 12
• Supermassive Black Holes with High Accretion Rates in Active Galactic Nuclei. V. A New Size-Luminosity Scaling Relation for the Broad-Line Region
• The upper bound on the lowest mass halo
• Counting voids to probe dark energy
• Constraining Baryon--Dark Matter Scattering with the Cosmic Dawn 21-cm Signal
• Coherent Propagation of PeV Neutrinos and the Dip in the Neutrino Spectrum at IceCube
• Planck intermediate results. XX. Comparison of polarized thermal emission from Galactic dust with simulations of MHD turbulence
• Angular momentum evolution of galaxies in EAGLE
• No evidence for extensions to the standard cosmological model
• Exploring the effects of galaxy formation on matter clustering through a library of simulation power spectra
• The quenching and morphological evolution of central galaxies is facilitated by the feedback-driven expulsion of circumgalactic gas
• GeV excess in the Milky Way: The Role of Diffuse Galactic gamma ray Emission template
• Accurate precision Cosmology with redshift unknown gravitational wave sources
• New Constraints on IGM Thermal Evolution from the Lyα Forest Power Spectrum
• Dynamical generation of the weak and Dark Matter scale
• The chosen few: the low mass halos that host faint galaxies
• Planck 2013 results. XVIII. Gravitational lensing-infrared background correlation
• Can the $H_0$ tension be resolved in extensions to $\Lambda$CDM cosmology?
• EDGE: the mass-metallicity relation as a critical test of galaxy formation physics
• Matter power spectrum and the challenge of percent accuracy
• Dark matter halo properties of GAMA galaxy groups from 100 square degrees of KiDS weak lensing data
• The Structure and Dynamical Evolution of the Stellar Disk of a Simulated Milky Way-Mass Galaxy
• Cosmology with Strong Lensing Systems
• Galaxy UV-luminosity function and reionization constraints on axion dark matter
• Clustering of intermediate redshift quasars using the final SDSS III-BOSS sample
• Subhalo abundance matching and assembly bias in the EAGLE simulation
• Feedback-regulated Super Massive Black Hole Seed Formation
• The LHC diphoton resonance and dark matter
• 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
• Limits on Neutrino-Neutrino Scattering in the Early Universe
• The one-dimensional power spectrum from the SDSS DR14 Ly$\alpha$ forests
• A Unifying Theory of Dark Energy and Dark Matter: Negative Masses and Matter Creation within a Modified $\Lambda$CDM Framework
• Physics at the e+ e- Linear Collider
• Diffuse Lyman-alpha Halos around Galaxies at z=2.2-6.6: Implications for Galaxy Formation and Cosmic Reionization
• The Foundation Supernova Survey: Motivation, Design, Implementation, and First Data Release
• Di-photon excess illuminates Dark Matter
• Limits on Dark Matter Annihilation Signals from the Fermi LAT 4-year Measurement of the Isotropic Gamma-Ray Background
• Equivalence of the Einstein and Jordan frames
• Planck 2013 results. XIX. The integrated Sachs-Wolfe effect
• CLASS: The Cosmology Large Angular Scale Surveyor
• Constraints from Ly-$\alpha$ forests on non-thermal dark matter including resonantly-produced sterile neutrinos
• Planck 2018 results. IX. Constraints on primordial non-Gaussianity
• Dust Formation in Milky Way-like Galaxies
• Standard big bang nucleosynthesis and primordial CNO Abundances after Planck
• The LOFAR window on star-forming galaxies and AGN - curved radio SEDs and IR-radio correlation at $0<z<2.5$
• The Cardassian expansion revisited: constraints from updated Hubble parameter measurements and Type Ia Supernovae data
• The Difficulty of Getting High Escape Fractions of Ionizing Photons from High-redshift Galaxies: a View from the FIRE Cosmological Simulations
• Chemodynamics of barred galaxies in cosmological simulations: On the Milky Way's quiescent merger history and in-situ bulge
• 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
• Search for narrow and broad dijet resonances in proton-proton collisions at $\sqrt{s}=$ 13 TeV and constraints on dark matter mediators and other new particles
• Piezoelectrically Tuned Multimode Cavity Search for Axion Dark Matter
• BBN And The CMB Constrain Neutrino Coupled Light WIMPs
• The Offset and Host Light Distributions of Long Gamma-Ray Bursts: A New View from HST Observations of Swift Bursts
• Quantifying the impact of mergers on the angular momentum of simulated galaxies
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS anisotropic galaxy clustering
• Effective Field Theory of Cosmological Perturbations
• Updated constraints on non-standard neutrino interactions from Planck
• Strong Lens Time Delay Challenge: II. Results of TDC1
• A joint analysis of Planck and BICEP2 B modes including dust polarization uncertainty
• A unified explanation for dark matter and electroweak baryogenesis with direct detection and gravitational wave signatures
• Eccentric Black Hole Gravitational-Wave Capture Sources in Galactic Nuclei: Distribution of Binary Parameters
• Fermion Portal Dark Matter
• Evidence for rapid disk formation and reprocessing in the X-ray bright tidal disruption event AT 2018fyk
• Characterizing mass, momentum, energy and metal outflow rates of multi-phase galactic winds in the FIRE-2 cosmological simulations
• Inflationary universe from perfect fluid and $F(R)$ gravity and its comparison with observational data
• Limits on sterile neutrino mixing using atmospheric neutrinos in Super-Kamiokande
• Measuring Dark Energy Properties with Photometrically Classified Pan-STARRS Supernovae. II. Cosmological Parameters
• Extended ionised and clumpy gas in a normal galaxy at z=7.1 revealed by ALMA
• Spreading out and staying sharp - Creating diverse rotation curves via baryonic and self-interaction effects
• The fraction of dark matter within galaxies from the IllustrisTNG simulations
• Blind foreground subtraction for intensity mapping experiments
• Binary Stars Can Provide the "Missing Photons" Needed for Reionization
• Simulating the dust content of galaxies: successes and failures
• Galaxy Strategy for LIGO-Virgo Gravitational Wave Counterpart Searches
• Editorial for the Special Issue 100 Years of Chronogeometrodynamics: The Status of the Einstein's Theory of Gravitation in Its Centennial Year
• Planck constraints on the tensor-to-scalar ratio
• Possible signals of vacuum dynamics in the Universe
• A Realistic Pattern of Lepton Mixing and Masses from S4 and CP
• Dynamical vacuum energy in the expanding Universe confronted with observations: a dedicated study
• ALFALFA Discovery of the Nearby Gas-Rich Dwarf Galaxy Leo~P. III. An Extremely Metal Deficient Galaxy
• Macro Dark Matter
• Exploring Cosmic Origins with CORE: Inflation
• Search for dijet resonances in proton-proton collisions at sqrt(s) = 13 TeV and constraints on dark matter and other models
• Light sterile neutrinos
• New Production Mechanism for keV Sterile Neutrino Dark Matter by Decays of Frozen-In Scalars
• Lyman continuum leakage from low-mass galaxies with Mstar < 1.E8 Msun
• A polynomial f(R) inflation model
• Indirect and direct search for dark matter
• Astrophysical limits on very light axion-like particles from Chandra grating spectroscopy of NGC 1275
• Revealing reionization with the thermal history of the intergalactic medium: new constraints from the Lyman-$\alpha$ flux power spectrum
• Deep into the structure of the first galaxies: SERRA views
• Supercal: Cross-Calibration of Multiple Photometric Systems to Improve Cosmological Measurements with Type Ia Supernovae
• Multiwavelength Study of Quiescent States of Mrk 421 with Unprecedented Hard X-Ray Coverage Provided by NuSTAR in 2013
• Planck Data Reconsidered
• The origin of scatter in the stellar mass - halo mass relation of central galaxies in the EAGLE simulation
• Black Hole Shadow of Sgr A${}^{\ast }$ in Dark Matter Halo
• WIMPs at the Galactic Center
• The Universe at z>10: Predictions for JWST from the UniverseMachine DR1
• Cosmology with massive neutrinos III: the halo mass function and an application to galaxy clusters
• The Aemulus Project I: Numerical Simulations for Precision Cosmology
• Constraints on the Coupling between Dark Energy and Dark Matter from CMB data
• A Measurement of the Cosmic Microwave Background Gravitational Lensing Potential from 100 Square Degrees of SPTpol Data
• NIHAO XV: The environmental impact of the host galaxy on galactic satellite and field dwarf galaxies
• From haloes to Galaxies - I. The dynamics of the gas regulator model and the implied cosmic sSFR history
• The Ep,i - Eiso correlation: type I gamma-ray bursts and the new classification method
• Origin of chemically distinct discs in the Auriga cosmological simulations
• Probing the scotogenic model with lepton flavor violating processes
• The alignment and shape of dark matter, stellar, and hot gas distributions in the EAGLE and cosmo-OWLS simulations
• The origin of galactic metal-rich stellar halo components with highly eccentric orbits
• Cosmological Constraints from the double source plane lens SDSSJ0946+1006
• The primordial deuterium abundance of the most metal-poor damped Lyman-alpha system
• Ultra large-scale cosmology in next-generation experiments with single tracers
• Two Field Matter Bounce Cosmology
• The Extended Distribution of Baryons Around Galaxies
• Asymptotic safety of quantum gravity beyond Ricci scalars
• On the Validity of the Effective Field Theory for Dark Matter Searches at the LHC Part III: Analysis for the $t$-channel
• The SCUBA-2 Cosmology Legacy Survey: Multi-wavelength Properties of ALMA-identified Submillimeter Galaxies in UKIDSS-UDS
• Updated fundamental constant constraints from Planck 2018 data and possible relations to the Hubble tension
• The distribution of atomic hydrogen in EAGLE galaxies: morphologies, profiles, and HI holes
• The Konus-Wind catalog of gamma-ray bursts with known redshifts. I. Bursts detected in the triggered mode
• Exploring Cosmic Origins with CORE: Cosmological Parameters
• Voids in massive neutrino cosmologies
• Zooming on the internal structure of $z\simeq 6$ galaxies
• Galactic outflow rates in the EAGLE simulations
• The Relationship between Galaxy and Dark Matter Halo Size from z~3 to the present
• Probing the innermost regions of AGN jets and their magnetic fields with RadioAstron. I. Imaging BL Lacertae at 21 microarcsecond resolution
• Resolving the ISM at the peak of cosmic star formation with ALMA - The distribution of CO and dust continuum in z~2.5 sub-millimetre galaxies
• Discovery of the broad-lined Type Ic SN 2013cq associated with the very energetic GRB 130427A
• New Light Species and the CMB
• The Observational Future of Cosmological Scalar-Tensor Theories
• A blinded determination of $H_0$ from low-redshift Type Ia supernovae, calibrated by Cepheid variables
• Super-Eddington growth of the first black holes
• The Scale of Dark QCD
• Planck 2013 results. XXVI. Background geometry and topology of the Universe
• The Mira-Titan Universe II: Matter Power Spectrum Emulation
• $\overline{D3}$ and dS
• The Mira-Titan Universe: Precision Predictions for Dark Energy Surveys
• The case for a cold dark matter cusp in Draco
• Probing Dark Energy with Atom Interferometry
• Constraining ultra large-scale cosmology with multiple tracers in optical and radio surveys
• Lattice QCD input for axion cosmology
• The nature of the Diffuse Gamma-Ray Background
• Semi-Analytic Galaxies - I. Synthesis of environmental and star-forming regulation mechanisms
• The Tiered Radio Extragalactic Continuum Simulation (T-RECS)
• Fast Radio Burst/Gamma-Ray Burst Cosmography
• Sgr A* and General Relativity
• Ultra-Light Dark Matter in Ultra-Faint Dwarf Galaxies
• Neutrino energy transport in weak decoupling and big bang nucleosynthesis
• Do the Most Massive Black Holes at $z=2$ Grow via Major Mergers?
• Planck Constraint on Relic Primordial Black Holes
• New test of the FLRW metric using the distance sum rule
• A Holographic Twin Higgs Model
• Cosmic Degeneracies I: Joint N-body Simulations of Modified Gravity and Massive Neutrinos
• Massive Neutrinos Leave Fingerprints on Cosmic Voids
• The impact of chemistry on the structure of high-z galaxies
• Supersonic Gas Streams Enhance the Formation of Massive Black Holes in the Early Universe
• The impact of stellar feedback on the structure, size and morphology of galaxies in Milky Way size dark matter haloes
• It's not easy being green: The evolution of galaxy colour in the EAGLE simulation
• CLASH-X: A Comparison of Lensing and X-ray Techniques for Measuring the Mass Profiles of Galaxy Clusters
• Beyond Assembly Bias: Exploring Secondary Halo Biases for Cluster-size Haloes
• The Effects of QCD Equation of State on the Relic Density of WIMP Dark Matter
• Galaxy Cold Gas Contents in Modern Cosmological Hydrodynamic Simulations
• Constraint on neutrino masses from SDSS-III/BOSS Ly$\alpha$ forest and other cosmological probes
• Sensitivity Projections for Dark Matter Searches with the Fermi Large Area Telescope
• A non Supersymmetric SO(10) Grand Unified Model for All the Physics below $M_{GUT}$
• The Aemulus Project II: Emulating the Halo Mass Function
• A modified naturalness principle and its experimental tests
• Redshift-Space Clustering of SDSS Galaxies --- Luminosity Dependence, Halo Occupation Distribution, and Velocity Bias
• The Carnegie-Chicago Hubble Program. I. An Independent Approach to the Extragalactic Distance Scale Using only Population II Distance Indicators
• Probing the thermal state of the intergalactic medium at $z>5$ with the transmission spikes in high-resolution Ly$\alpha$ forest spectra
• Null test of the cosmic curvature using $H(z)$ and supernovae data
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Signs of neutrino mass in current cosmological datasets
• The observational status of Galileon gravity after Planck
• Frontiers in Nuclear Astrophysics
• Nonlocal Models of Cosmic Acceleration
• Model independent $H(z)$ reconstruction using the cosmic inverse distance ladder
• The relation between gas density and velocity power spectra in galaxy clusters: high-resolution hydrodynamic simulations and the role of conduction
• MassiveNuS: Cosmological Massive Neutrino Simulations
• SDSS-IV MaNGA: Global stellar population and gradients for about 2000 early-type and spiral galaxies on the mass-size plane
• Sausage & Mash: The dual origin of the Galactic thick disc and halo from the gas-rich Gaia-Enceladus-Sausage merger
• The Hestia project: simulations of the Local Group
• [CII] emission in z ~ 6 strongly lensed, star-forming galaxies
• Observational Challenges for the Standard FLRW Model
• Probing cosmology and gravity with redshift-space distortions around voids
• Converting non-relativistic dark matter to radiation
• Constraints from thermal Sunyaev-Zeldovich cluster counts and power spectrum combined with CMB
• Effective Theories for Dark Matter Nucleon Scattering
• Gauged Supergravities
• New Observational $H(z)$ Data from Full-Spectrum Fitting of Cosmic Chronometers in the LEGA-C Survey
• Lyman-alpha emitters gone missing: evidence for late reionization?
• Teasing bits of information out of the CMB energy spectrum
• Measurements of Sub-degree B-mode Polarization in the Cosmic Microwave Background from 100 Square Degrees of SPTpol Data
• Detection of Thermal SZ -- CMB Lensing Cross-Correlation in Planck Nominal Mission Data
• Exploring Cosmic Origins with CORE: Survey requirements and mission design
• Shell model predictions for ${}^{124}$Sn double-beta decay
• 3D Cosmic Shear: Cosmology from CFHTLenS
• Cosmological window onto the string axiverse and the supersymmetry breaking scale
• Gamma-ray Burst Cosmology
• Deflection Angle and Shadow Behaviors of Quintessential Black Holes in arbitrary Dimensions
• Empirical Covariance Modeling for 21 cm Power Spectrum Estimation: A Method Demonstration and New Limits from Early Murchison Widefield Array 128-Tile Data
• AGNfitter: A Bayesian MCMC approach to fitting spectral energy distributions of AGN
• Constraining Velocity-dependent Self-Interacting Dark Matter with the Milky Way's dwarf spheroidal galaxies
• Joint constraints on thermal relic dark matter from strong gravitational lensing, the Lyman-$\alpha$ forest, and Milky Way satellites
• Descendants of the first stars: the distinct chemical signature of second generation stars
• Which spectral distortions does $\Lambda$CDM actually predict?
• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: 1000 multi-tracer mock catalogues with redshift evolution and systematics for galaxies and quasars of the final data release
• Clustering of quasars in SDSS-IV eBOSS : study of potential systematics and bias determination
• Planck Constraints on Holographic Dark Energy
• Constraints on a Bianchi type I spacetime extension of the standard $\Lambda$CDM model
• Velocity Bias from the Small Scale Clustering of SDSS-III BOSS Galaxies
• Aspects of asymptotic safety for quantum gravity
• A new life for sterile neutrinos: resolving inconsistencies using hot dark matter
• Dark Matter Constraints from a Joint Analysis of Dwarf Spheroidal Galaxy Observations with VERITAS
• Quantifying the non-Gaussianity in the EoR 21-cm signal through bispectrum
• Constraints on primordial non-Gaussianity from 800,000 photometric quasars
• A consistent measure of the merger histories of massive galaxies using close-pair statistics I: Major mergers at $z<3.5$
• Blue Tensor Spectrum from Particle Production during Inflation
• ALMA Long Baseline Observations of the Strongly Lensed Submillimeter Galaxy HATLAS J090311.6+003906 at z=3.042
• The Caterpillar Project: A Large Suite of Milky Way Sized Halos
• CMB lensing tomography with the DES Science Verification galaxies
• The Mass-Discrepancy Acceleration Relation: a Natural Outcome of Galaxy Formation in Cold Dark Matter halos
• Strongest model-independent bound on the lifetime of Dark Matter
• The Cosmic Ballet: spin and shape alignments of haloes in the cosmic web
• Reconciling the Diversity and Uniformity of Galactic Rotation Curves with Self-Interacting Dark Matter
• The impact of assembly bias on the halo occupation in hydrodynamical simulations
• Simulating nonlinear cosmological structure formation with massive neutrinos
• The Impact of Star Formation and Gamma-Ray Burst Rates at High Redshift on Cosmic Chemical Evolution and Reionization
• The splashback radius of halos from particle dynamics. II. Dependence on mass, accretion rate, redshift, and cosmology
• The local high velocity tail and the Galactic escape speed
• Search for gamma-ray emission from the Coma Cluster with six years of Fermi-LAT data
• Dark Energy at early times and ACT: a larger Hubble constant without late-time priors
• 21 cm signal from cosmic dawn: Imprints of spin temperature fluctuations and peculiar velocities
• Bouncing Cosmology made simple
• Observation of scaling in the dynamics of a strongly quenched quantum gas
• Standard Model with a Complex Scalar Singlet: Cosmological Implications and Theoretical Considerations
• The SINFONI Nearby Elliptical Lens Locator Survey: Discovery of two new low-redshift strong lenses and implications for the initial mass function in giant early-type galaxies
• The Parameterized Post-Friedmannian Framework for Interacting Dark Energy Theories
• Semi-analytic forecasts for JWST -- II. physical properties and scaling relations for galaxies at z = 4-10
• Modeling baryonic physics in future weak lensing surveys
• Dilepton constraints in the Inert Doublet Model from Run 1 of the LHC
• The Coevolution of Supermassive Black Holes and Massive Galaxies at High Redshift
• Ultra-compact structure in intermediate-luminosity radio quasars: building a sample of standard cosmological rulers and improving the dark energy constraints up to $z\sim 3$
• Simplified Models vs. Effective Field Theory Approaches in Dark Matter Searches
• A Note on Tsallis Holographic Dark Energy
• The Observational Status of Cosmic Inflation after Planck
• Anisotropic nature of space-time in $f(Q)$ gravity
• Baryons, Neutrinos, Feedback and Weak Gravitational Lensing
• The SDSS-IV extended Baryonic Oscillation Spectroscopic Survey: Luminous Red Galaxy Target Selection
• Reconciling Planck results with low redshift astronomical measurements
• Galaxy formation in the Planck Millennium: the atomic hydrogen content of dark matter halos
• The First Billion Years project: birthplaces of direct collapse black holes
• Enrichment of r-process elements in dwarf spheroidal galaxies in chemo-dynamical evolution model
• The hydrogen-poor superluminous supernova iPTF13ajg and its host galaxy in absorption and emission
• The diphoton signal of the light Higgs boson in Natural NMSSM
• Inspiraling Halo Accretion Mapped in Lyman-$\alpha$ Emission around a $z\sim 3$ Quasar
• Unbiased constraints on ultralight axion mass from dwarf spheroidal galaxies
• Baryonic clues to the puzzling diversity of dwarf galaxy rotation curves
• Constraining the primordial initial mass function with stellar archaeology
• Matter power spectrum: from Ly$\alpha$ forest to CMB scales
• Consensus report on 25 years of searches for damped Ly$\alpha$ galaxies in emission: Confirming their metallicity-luminosity relation at $z\gtrsim 2$
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions
• Impact of a complex singlet: From dark matter to baryogenesis
• Pseudoscalar - sterile neutrino interactions: reconciling the cosmos with neutrino oscillations
• Cosmology with self-interacting sterile neutrinos and dark matter - A pseudoscalar model
• Spiral-induced velocity and metallicity patterns in a cosmological zoom simulation of a Milky Way-sized galaxy
• The photoheating of the intergalactic medium in synthesis models of the UV background
• J0811+4730: the most metal-poor star-forming dwarf galaxy known
• Measuring Type Ia Supernova Populations of Stretch and Color and Predicting Distance Biases
• Sensitivity of Next-Generation Tritium Beta-Decay Experiments for keV-Scale Sterile Neutrinos
• Gas accretion and galactic fountain flows in the Auriga cosmological simulations: angular momentum and metal re-distribution
• Evidence for a Lower Value for $H_0$ from Cosmic Chronometers Data?
• Combining Experimental and Cosmological Constraints on Heavy Neutrinos
• Emulating the CFHTLenS Weak Lensing data: Cosmological Constraints from moments and Minkowski functionals
• Modelling galaxy clustering: halo occupation distribution versus subhalo matching
• Singlet Extensions of the Standard Model at LHC Run 2: Benchmarks and Comparison with the NMSSM
• Axion dark matter in the post-inflationary Peccei-Quinn symmetry breaking scenario
• The REQUIEM Survey I: A Search for Extended Ly-Alpha Nebular Emission Around 31 z>5.7 Quasars
• Contribution of stripped nuclear clusters to globular cluster and ultra-compact dwarf galaxy populations
• Stochastic star formation in early galaxies: JWST implications
• Short GRBs: opening angles, local neutron star merger rate and off-axis events for GRB/GW association
• The East Asian Observatory SCUBA--2 survey of the COSMOS field: unveiling 1147 bright sub-millimeter sources across 2.6 square degrees
• Sample variance in the local measurements of the Hubble constant
• Calibrating the cosmic distance scale ladder: the role of the sound horizon scale and the local expansion rate as distance anchors
• New reaction rates for improved primordial D/H calculation and the cosmic evolution of deuterium
• Distinguishing different scenarios of early energy release with spectral distortions of the cosmic microwave background
• Galaxy environment in the 3D-HST fields. Witnessing the onset of satellite quenching at z ~ 1-2
• Limits on Pop III star formation with the most iron-poor stars
• Radiative Feedback from high mass X-ray binaries on the formation of the first galaxies and early reionization
• Galaxy number counts to second order and their bispectrum
• A new interacting two fluid model and its consequences
• The $\bar{\Lambda }CDM$ cosmology: from inflation to dark energy through running $\Lambda$
• The effect of baryons on redshift space distortions and cosmic density and velocity fields in the EAGLE simulation
• Equilateral non-Gaussianity from heavy fields
• Pre-inflationary universe in loop quantum cosmology
• Pseudoscalar Portal Dark Matter
• Velocity correction for Hubble constant measurements from standard sirens
• Primordial black holes as biased tracers
• 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
• New Bounds for Axions and Axion-Like Particles with keV-GeV Masses
• Big Bang Synthesis of Nuclear Dark Matter
• Analyzing the $H_0$ tension in $F(R)$ gravity models
• The stellar-to-halo mass relation of GAMA galaxies from 100 square degrees of KiDS weak lensing data
• Dynamics of an Interacting Barrow Holographic Dark Energy Model and its Thermodynamic Implications
• Anisotropic cosmological models in $f(R,T)$ gravity with variable deceleration parameter
• keV Sterile Neutrino Dark Matter from Singlet Scalar Decays: Basic Concepts and Subtle Features
• Orbital decomposition of CALIFA spiral galaxies
• An effective field theory during inflation: reduced density matrix and its quantum master equation
• Decaying dark matter and the tension in ${\sigma }_8$
• The Abacus Cosmos: A Suite of Cosmological N-body Simulations
• The Copernicus Complexio: a high-resolution view of the small-scale Universe
• Hidden sector monopole, vector dark matter and dark radiation with Higgs portal
• Cosmological Constraints From Weak Lensing Peak Statistics With CFHT Stripe 82 Survey
• Weighing "El Gordo" with a Precision Scale: Hubble Space Telescope Weak-lensing Analysis of the Merging Galaxy Cluster ACT-CL J0102-4915 at z=0.87
• Is Main Sequence Galaxy Star Formation Controlled by Halo Mass Accretion?
• Quintessential inflation with canonical and noncanonical scalar fields and Planck 2015 results
• Indirect searches for sterile neutrinos at a high-luminosity Z-factory
• Thermal and non-thermal production of dark matter via Z'-portal(s)
• The Formation of Isolated Ultra-Diffuse Galaxies in Romulus25
• The detection rate of Inspiral and Quasi-normal modes of Pop III binary black holes which can confirm or refute the General Relativity in the strong gravity region
• Simulated Milky Way analogues: implications for dark matter direct searches
• Cosmology with gamma-ray bursts: II Cosmography challenges and cosmological scenarios for the accelerated Universe
• The Viability of Phantom Dark Energy: A Brief Review
• The environmental dependence of HI in galaxies in the EAGLE simulations
• Multipartite Interacting Scalar Dark Matter in the light of updated LUX data
• The fundamental plane of star formation in galaxies revealed by the EAGLE hydrodynamical simulations
• The physical properties of z>2 Lyman limit systems: new constraints for feedback and accretion models
• A consistent and robust measurement of the thermal state of the IGM at $2\le z\le 4$ from a large sample of Ly$\alpha$ forest spectra: Evidence for late and rapid HeII reionization
• Halo bias in mixed dark matter cosmologies
• Implications of a transition in the dark energy equation of state for the $H_0$ and ${\sigma }_8$ tensions
• Precision Epoch of Reionization studies with next-generation CMB experiments
• Primordial nucleosynthesis
• Partially Acoustic Dark Matter, Interacting Dark Radiation, and Large Scale Structure
• The effect of baryons on the inner density profiles of rich clusters
• ZOMG-I. How the cosmic web inhibits halo growth and generates assembly bias
• An uncertainty principle for star formation - II. A new method for characterising the cloud-scale physics of star formation and feedback across cosmic history
• The Missing Link: Bayesian Detection and Measurement of Intermediate-Mass Black-Hole Binaries
• Probing dark matter substructure in the gravitational lens HE0435-1223 with the WFC3 grism
• NIHAO IX: the role of gas inflows and outflows in driving the contraction and expansion of cold dark matter haloes
• On the jet properties of the gamma-ray loud active galactic nuclei
• A spatially resolved study of cold dust, molecular gas, HII regions, and stars in the $z=2.12$ submillimeter galaxy ALESS67.1
• Prospects for gravitational-wave detection and supermassive black hole astrophysics with pulsar timing arrays
• The gas fractions of dark matter haloes hosting simulated $\sim L^{\star }$ galaxies are governed by the feedback history of their black holes
• From Primordial Black Holes Abundance to Primordial Curvature Power Spectrum (and back)
• A search for pair production of new light bosons decaying into muons
• POLARBEAR Constraints on Cosmic Birefringence and Primordial Magnetic Fields
• Measurements of B-mode Polarization of the Cosmic Microwave Background from 500 Square Degrees of SPTpol Data
• Tidal debris morphology and the orbits of satellite galaxies
• Evidence for interacting dark energy from BOSS
• A consistent determination of the temperature of the intergalactic medium at redshift z=2.4
• Energy equipartition between stellar and dark matter particles in cosmological simulations results in spurious growth of galaxy sizes
• Robust collider limits on heavy-mediator Dark Matter
• Gaps in globular cluster streams: giant molecular clouds can cause them too
• Search for top-squark pair production in final states with one lepton, jets, and missing transverse momentum using 36 fb${}^{-1}$ of $\sqrt{s}=13$ TeV $pp$ collision data with the ATLAS detector
• The relation between galaxy morphology and colour in the EAGLE simulation
• The effect of magnetic fields on properties of the circumgalactic medium
• Modelling the large scale structure of the Universe as a function of cosmology and baryonic physics
• Green's function of the cosmological thermalization problem
• Galaxies in the EAGLE hydrodynamical simulation and in the Durham and Munich semi-analytical models
• Singlet-Catalyzed Electroweak Phase Transitions in the 100 TeV Frontier
• SIMPle Dark Matter: Self-Interactions and keV Lines
• Review of the theoretical and experimental status of dark matter identification with cosmic-ray antideuterons
• Cosmological Phase Transitions and their Properties in the NMSSM
• Probable or Improbable Universe? Correlating Electroweak Vacuum Instability with the Scale of Inflation
• Cosmological Simulations of Early Blackhole Formation: Halo Mergers, Tidal Disruption, and the Conditions for Direct Collapse
• Sunyaev-Zel'dovich Effect and X-ray Scaling Relations from Weak-Lensing Mass Calibration of 32 SPT Selected Galaxy Clusters
• Antideuteron Sensitivity for the GAPS Experiment
• Host galaxies of merging compact objects: mass, star formation rate, metallicity and colours
• Electroweak Baryogenesis driven by Extra Top Yukawa Couplings
• CMB spectral distortions from small-scale isocurvature fluctuations
• Dynamical analysis in scalar field cosmology
• A wide dispersion in star formation rate and dynamical mass of 10^8 solar mass black hole host galaxies at redshift 6
• The prevalence and influence of circumstellar material around hydrogen-rich supernova progenitors
• Feynman Diagrams for Stochastic Inflation and Quantum Field Theory in de Sitter Space
• The 6dF Galaxy Survey: Bulk Flows on $50-70h^{-1}$ Mpc scales
• A merger in the dusty, $z=7.5$ galaxy A1689-zD1?
• SIDM on FIRE: Hydrodynamical Self-Interacting Dark Matter simulations of low-mass dwarf galaxies
• An Alternative to Particle Dark Matter
• The connection between mass, environment and slow rotation in simulated galaxies
• The extended ROSAT-ESO Flux Limited X-ray Galaxy Cluster Survey (REFLEX II) IV. X-ray Luminosity Function and First Constraints on Cosmological Parameters
• Cutoff in the Lyman-$\alpha$ forest power spectrum: warm IGM or warm dark matter?
• Inflationary Magnetogenesis without the Strong Coupling Problem II: Constraints from CMB anisotropies and B-modes
• Cradles of the first stars: self-shielding, halo masses, and multiplicity
• Cosmic reionization after Planck II: contribution from quasars
• Measuring the speed of light with ultra-compact radio quasars
• IceCube events and decaying dark matter: hints and constraints
• Killing the cMSSM softly
• Combined Solar System and rotation curve constraints on MOND
• Effective WIMPs
• Evidence of Lensing of the Cosmic Microwave Background by Dark Matter Halos
• NLO+NLL Collider Bounds, Dirac Fermion and Scalar Dark Matter in the B-L Model
• The thermal Sunyaev Zel'dovich effect power spectrum in light of Planck
• An independent determination of the local Hubble constant
• Shell model studies of the ${}^{130}Te$ neutrinoless double-beta decay
• Timing the formation and assembly of early-type galaxies via spatially resolved stellar populations analysis
• Lack of large-angle TT correlations persists in WMAP and Planck
• Freeze-in through portals
• The diverse density profiles of galaxy clusters with self-interacting dark matter plus baryons
• Disformal couplings and the dark sector of the universe
• Cosmological consequences of an adiabatic matter creation process
• Asymptotics with a positive cosmological constant: II. Linear fields on de Sitter space-time
• Galaxy clustering, photometric redshifts and diagnosis of systematics in the DES Science Verification data
• No cores in dark matter-dominated dwarf galaxies with bursty star formation histories
• Minimal Left-Right Symmetric Dark Matter
• The SAMI Galaxy Survey: comparing 3D spectroscopic observations with galaxies from cosmological hydrodynamical simulations
• Are LGRBs biased tracers of star formation? Clues from the host galaxies of the $Swift$/BAT6 complete sample of bright LGRBs III: Stellar masses, star formation rates and metallicities at $z>1$
• Constraints on decaying dark matter from the extragalactic gamma-ray background
• Reionization optical depth determination from Planck HFI data with ten percent accuracy
• COSMOS2020: The cosmic evolution of the stellar-to-halo mass relation for central and satellite galaxies up to z~5
• Implication of the 750 GeV diphoton resonance on two-Higgs-doublet model and its extensions with Higgs field
• Large-scale alignments from WMAP and Planck
• Cosmological Information in the Intrinsic Alignments of Luminous Red Galaxies
• A dusty compact object bridging galaxies and quasars at cosmic dawn
• GUT-inspired SUSY and the muon g-2 anomaly: prospects for LHC 14 TeV
• Search for sterile neutrinos in holographic dark energy cosmology: Reconciling Planck observation with the local measurement of the Hubble constant
• Axion hot dark matter bounds after Planck
• A Path to the Direct Detection of sub-GeV Dark Matter Using Calorimetric Readout of a Superfluid ${}^4$He Target
• Measurement of Galaxy Clustering at z~7.2 and the Evolution of Galaxy Bias from 3.8<z<8 in the XDF, GOODS-S AND GOODS-N
• The origin of the mass discrepancy-acceleration relation in $\Lambda$CDM
• Eulerian BAO Reconstructions and N-Point Statistics
• SuperRAENN: A Semi-supervised Supernova Photometric Classification Pipeline Trained on Pan-STARRS1 Medium Deep Survey Supernovae
• Long Dark Gaps in the Ly$\beta$ Forest at $z<6$: Evidence of Ultra Late Reionization from XQR-30 Spectra
• The Nature of Massive Transition Galaxies in CANDELS, GAMA, and Cosmological Simulations
• Constraints on deviations from $\Lambda$CDM within Horndeski gravity
• Radio Galaxy populations and the multi-tracer technique: pushing the limits on primordial non-Gaussianity
• Hubble tension or a transition of the Cepheid SnIa calibrator parameters?
• A Measurement of Gravitational Lensing of the Cosmic Microwave Background by Galaxy Clusters Using Data from the South Pole Telescope
• TeV Scale Left-Right Symmetry and Large Mixing Effects in Neutrinoless Double Beta Decay
• Black holes in vector-tensor theories
• On the use of semi-numerical simulations in predicting the 21-cm signal from the epoch of reionization
• Cosmological Applications of Pade Approximant
• Forecasts on the Dark Energy and Primordial Non-Gaussianity Observations with the Tianlai Cylinder Array
• Probing Baryogenesis with Displaced Vertices at the LHC
• Interacting quintessence from a variational approach Part II: derivative couplings
• Boosted Dark Matter in IceCube and at the Galactic Center
• Unification of inflation and dark energy {\it à la} quintessential inflation
• Thermal Dark Matter Through the Dirac Neutrino Portal
• Go with the Flow: Understanding Inflow Mechanisms in Galaxy Collisions
• ERQs are the BOSS of Quasar Samples: The Highest-Velocity [OIII] Quasar Outflows
• NIHAO XIV: Reproducing the observed diversity of dwarf galaxy rotation curve shapes in LCDM
• Strong phase transition, dark matter and vacuum stability from simple hidden sectors
• Constraints on $\Lambda$CDM Extensions from the SPT-3G 2018 $EE$ and $TE$ Power Spectra
• Ultra-High-Energy Cosmic Rays: The Intersection of the Cosmic and Energy Frontiers
• Dark compact objects: an extensive overview
• Gravitational Anomalies in the Solar System?
• Cross-correlation between the CMB lensing potential measured by Planck and high-z sub-mm galaxies detected by the Herschel-ATLAS survey
• Intra Cluster Light properties in the CLASH-VLT cluster MACS J1206.2-0847
• Constraints on Assembly Bias from Galaxy Clustering
• A 34.5 day quasi-periodic oscillation in gamma-ray emission from the blazar PKS 2247-131
• Fermionic dark matter with pseudo-scalar Yukawa interaction
• Spatial Clustering of Dark Matter Halos: Secondary Bias, Neighbor Bias, and the Influence of Massive Neighbors on Halo Properties
• Λ CDM is Consistent with SPARC Radial Acceleration Relation
• GHIGLS: HI mapping at intermediate Galactic latitude using the Green Bank Telescope
• Tight Constraints on the Excess Radio Background at $z=9.1$ from LOFAR
• Searching for Invisible Axion Dark Matter with an 18T Magnet Haloscope
• The Limits of Cosmic Shear
• Detection of isotropic cosmic birefringence and its implications for axion-like particles including dark energy
• $Om$ diagnostic applied to scalar field models and slowing down of cosmic acceleration
• How the Dark Energy Can Reconcile \textit{Planck} with Local Determination of the Hubble Constant
• Inflation meets neutrinos
• Unmasking the Masked Universe: the 2M++ catalogue through Bayesian eyes
• The supernova CSS121015:004244+132827: a clue for understanding super-luminous supernovae
• Diverse properties of Ly-alpha emission in low-redshift compact star-forming galaxies with extremely high [OIII]/[OII] ratios
• Combined analysis of effective Higgs portal dark matter models
• In-in and $\delta N$ calculations of the bispectrum from non-attractor single-field inflation
• Baryon Acoustic Oscillations from the SDSS DR10 galaxies angular correlation function
• The Imprint of Reionization on the Star Formation Histories of Dwarf Galaxies
• BICEP3: a 95 GHz refracting telescope for degree-scale CMB polarization
• Directional Dark Matter Detection Beyond the Neutrino Bound
• The Weak Lensing Signal and the Clustering of BOSS Galaxies I: Measurements
• The bright-end galaxy candidates at z ~ 9 from 79 independent HST fields
• An Extended Matter Bounce Scenario: current status and challenges
• Constraints on the identity of the dark matter from strong gravitational lenses
• Z-portal dark matter
• WIMP and SIMP Dark Matter from the Spontaneous Breaking of a Global Group
• Discovery Prospects for NMSSM Higgs Bosons at the High-Energy Large Hadron Collider
• Baryogenesis from Strong CP Violation and the QCD Axion
• Dark matter-radiation interactions: the impact on dark matter haloes
• Galaxy formation in the Planck cosmology - IV. Mass and environmental quenching, conformity and clustering
• Cosmological performance of SKA HI galaxy surveys
• Estimating the large-scale angular power spectrum in the presence of systematics: a case study of Sloan Digital Sky Survey quasars
• Modeling evolution of dark matter substructure and annihilation boost
• DAEdALUS and Dark Matter Detection
• Baryonic effects for weak lensing. Part I. Power spectrum and covariance matrix
• ALMA suggests outflows in z~5.5 galaxies
• Testing Sunyaev-Zel'dovich measurements of the hot gas content of dark matter haloes using synthetic skies
• Testing coupled dark energy with large scale structure observation
• Fourteen candidate RR Lyrae star streams in the inner Galaxy
• The Void Size Function in Dynamical Dark Energy Cosmologies
• Leptophilic Effective WIMPs
• Evaporating the Milky Way halo and its satellites with inelastic self-interacting dark matter
• Interacting quintessence from a variational approach Part I: algebraic couplings
• Gas and galaxies in filament between clusters of galaxies: The study of A399-A401
• Hiding in plain sight: An abundance of compact massive spheroids in the local Universe
• The Atacama Cosmology Telescope: Lensing of CMB Temperature and Polarization Derived from Cosmic Infrared Background Cross-Correlation
• New Scotogenic Model of Neutrino Mass with $U(1{)}_D$ Gauge Interaction
• Is there evidence for dark energy evolution?
• Integrable Scalar Cosmologies I. Foundations and links with String Theory
• The strongest bounds on active-sterile neutrino mixing after Planck data
• Intrinsic alignments of galaxies in the EAGLE and cosmo-OWLS simulations
• The Extent of the Stop Coannihilation Strip
• Precision cosmology with voids in the final BOSS data
• Axion Dark Matter eXperiment: Run 1B Analysis Details
• On Removing Interloper Contamination from Intensity Mapping Power Spectrum Measurements
• Semi-analytic forecasts for JWST -- IV. Implications for cosmic reionization and LyC escape fraction
• Can AGN feedback break the self-similarity of galaxies, groups, and clusters?
• Probing cosmic anisotropy with gravitational waves as standard sirens
• The Spitzer-HETDEX Exploratory Large-Area Survey
• Probing Leptogenesis
• Two-loop stability of a complex singlet extended Standard Model
• Obstructions to Bell CMB Experiments
• A model with interaction of dark components and recent observational data
• Introducing the FirstLight project: UV luminosity function and scaling relations of primeval galaxies
• Spatially unassociated galaxies contribute significantly to the blended submillimetre galaxy population: predictions for follow-up observations of ALMA sources
• An X-ray/SDSS sample (I): multi-phase outflow incidence and dependence on AGN luminosity
• Emerging spatial curvature can resolve the tension between high-redshift CMB and low-redshift distance ladder measurements of the Hubble constant
• A study of electroweak vacuum metastability with a singlet scalar dark matter
• High-redshift radio galaxies: a potential new source of 21-cm fluctuations
• What are $Om{h}^2(z_1,z_2)$ and $Om(z_1,z_2)$ diagnostics telling us in light of $H(z)$ data?
• Merger-Induced Metallicity Dilution in Cosmological Galaxy Formation Simulations
• NuSTAR unveils a Compton-thick Type 2 quasar in Mrk 34
• Ultra-diffuse galaxies in the Auriga simulations
• Neutron star mergers and rare core-collapse supernovae as sources of r-process enrichment in simulated galaxies
• On Longevity of I-ball/Oscillon
• A General Analysis of Direct Dark Matter Detection: From Microphysics to Observational Signatures
• Searching for Oscillations in the Primordial Power Spectrum: Constraints from Planck (Paper II)
• Hubble Frontier Fields: The Geometry and Dynamics of the Massive Galaxy Cluster Merger MACSJ0416.1-2403
• Asymptotics with a positive cosmological constant: III. The quadrupole formula
• What next for the CMSSM and the NUHM: Improved prospects for superpartner and dark matter detection
• Dark matter and collider signatures of the MSSM
• Testing models of vacuum energy interacting with cold dark matter
• Detection of eccentric supermassive black hole binaries with pulsar timing arrays: Signal-to-noise ratio calculations
• Cosmological Hints of Modified Gravity ?
• Implications of Improved Higgs Mass Calculations for Supersymmetric Models
• Simulated Milky Way analogues: implications for dark matter indirect searches
• Homogeneity and isotropy in the 2MASS Photometric Redshift catalogue
• Vacuum models with a linear and a quadratic term in H: structure formation and number counts analysis
• Fingerprints of Galactic Loop I on the Cosmic Microwave Background
• Determining the full satellite population of a Milky Way-mass halo in a highly resolved cosmological hydrodynamic simulation
• Where are the Low-Mass Population III Stars ?
• Hot gas around SN 1998bw: Inferring the progenitor from its environment
• $\nu \Lambda$MDM: A Model for Sterile Neutrino and Dark Matter Reconciles Cosmological and Neutrino Oscillation Data after BICEP2
• Felix: A Topology based Framework for Visual Exploration of Cosmic Filaments
• The slight spin of the old stellar halo
• Primordial power spectrum from Planck
• Dark energy equation of state parameter and its variation at low redshifts
• MUSE searches for galaxies near very metal-poor gas clouds at z~3: new constraints for cold accretion models
• Binned Hubble parameter measurements and the cosmological deceleration-acceleration transition
• Radiative Linear Seesaw model, Dark Matter and $U(1{)}_{B-L}$
• The Metagalactic Ionizing Background: A Crisis in UV Photon Production or Incorrect Galaxy Escape Fractions?
• A Machine Learning Approach for Dynamical Mass Measurements of Galaxy Clusters
• First Measurement of the Cross-Correlation of CMB Lensing and Galaxy Lensing
• NIHAO project II: Halo shape, phase-space density and velocity distribution of dark matter in galaxy formation simulations
• Einstein's legacy in galaxy surveys
• Simulations of ultra-high Energy Cosmic Rays in the local Universe and the origin of Cosmic Magnetic Fields
• Exploring collider signatures of the inert Higgs doublet model
• Non-local gravity and comparison with observational datasets
• A new diagnostic for the null test of dynamical dark energy in light of DESI 2024 and other BAO data
• Planck 2013 results. XXXI. Consistency of the Planck data
• Deep HeII and CIV Spectroscopy of a Giant Lyman alpha Nebula: Dense Compact Gas Clumps in the Circumgalactic Medium of a z~2 Quasar
• Models of the Primordial Standard Clock
• Ultrafaint Dwarf Galaxies - the lowest mass relics from before reionization
• Cosmological Models and Gamma-Ray Bursts Calibrated by Using Pade Method
• The subtlety of Ly-a photons: changing the expected range of the 21-cm signal
• Flaring from the supermassive black hole in Mrk 335 studied with Swift and NuSTAR
• Bayesian model selection without evidences: application to the dark energy equation-of-state
• Cosmological perturbation theory in 1+1 dimensions
• Resonant Di-Higgs Production in the $b\bar{b}WW$ Channel: Probing the Electroweak Phase Transition at the LHC
• Clustering and Halo Abundances in Early Dark Energy Cosmological Models
• Inspecting the supernova gamma-ray burst connection with high-energy neutrinos
• 750 GeV Resonance in the Dark Left-Right Model
• High-Redshift Star Formation in a Time-Dependent Lyman-Werner Background
• Dark Matter Fraction in Lens Galaxies: New Estimates from Microlensing
• CosmoBolognaLib: C++ libraries for cosmological calculations
• Low-mass right-handed sneutrino dark matter: SuperCDMS and LUX constraints and the Galactic Centre gamma-ray excess
• Minimal semi-annihilating ${\mathbb{Z}}_N$ scalar dark matter
• Majorana Dark Matter with a Coloured Mediator: Collider vs Direct and Indirect Searches
• MeV scale leptonic force for cosmic neutrino spectrum and muon anomalous magnetic moment
• SILVERRUSH. VI. A simulation of Ly$\alpha$ emitters in the reionization epoch and a comparison with Subaru Hyper Suprime-Cam survey early data
• End of inflation, oscillons and matter-antimatter asymmetry
• Anatomy of Coannihilation with a Scalar Top Partner
• Direct Detection Signatures of Self-Interacting Dark Matter with a Light Mediator
• Search for Dark Matter Annihilation in the Galactic Center with IceCube-79
• Massive black hole evolution models confronting the n-Hz amplitude of the stochastic gravitational wave background
• The Tully-Fisher and mass-size relations from halo abundance matching
• The Lyman-alpha signature of the first galaxies
• The rich complexity of 21-cm fluctuations produced by the first stars
• A New Measurement of the Temperature Density Relation of the IGM From Voigt Profile Fitting
• Probing the scotogenic FIMP at the LHC
• Cosmological constraints on post-Newtonian parameters in effectively massless scalar-tensor theories of gravity
• A $\Lambda$CDM bounce scenario
• Generalised CP and $\Delta (6n^2)$ Family Symmetry in Semi-Direct Models of Leptons
• The impact of baryonic discs on the shapes and profiles of self-interacting dark matter halos
• Two-Step Electroweak Baryogenesis
• NIHAO X: Reconciling the local galaxy velocity function with Cold Dark Matter via mock HI observations
• Structure formation with massive neutrinos: going beyond linear theory
• Prospects for dark matter searches in the pMSSM
• Global fits of the dark matter-nucleon effective interactions
• Revisiting the tension between fast bars and the $\Lambda$CDM paradigm
• General Analytic Solutions of Scalar Field Cosmology with Arbitrary Potential
• Gaussian Process Estimation of Transition Redshift
• Constraining the time evolution of dark energy, curvature and neutrino properties with cosmic chronometers
• Stability of the flat FLRW metric in $f(T)$ gravity
• Testing the electroweak phase transition and electroweak baryogenesis at the LHC and a circular electron-positron collider
• Standard Clock in Primordial Density Perturbations and Cosmic Microwave Background
• unWISE tomography of Planck CMB lensing
• An accurate bound on tensor-to-scalar ratio and the scale of inflation
• The power spectrum and bispectrum of SDSS DR11 BOSS galaxies II: cosmological interpretation
• Constraints on low-mass WIMPs from the EDELWEISS-III dark matter search
• Relieving the Tension between Weak Lensing and Cosmic Microwave Background with Interacting Dark Matter and Dark Energy Models
• Search for extended gamma-ray emission from the Virgo galaxy cluster with Fermi-LAT
• Constraining cosmic deceleration-acceleration transition with type Ia supernova, BAO/CMB and H(z) data
• The critical dark matter halo mass for Population III star formation: dependence on Lyman-Werner radiation, baryon-dark matter streaming velocity, and redshift
• An effective field theory during inflation II: stochastic dynamics and power spectrum suppression
• Lepton Mixing Predictions including Majorana Phases from $\Delta (6n^2)$ Flavour Symmetry and Generalised CP
• Inflationary tensor fossils in large-scale structure
• DEMNUni: ISW, Rees-Sciama, and weak-lensing in the presence of massive neutrinos
• Constraining Gravity at the Largest Scales through CMB Lensing and Galaxy Velocities
• Primordial 4He abundance: a determination based on the largest sample of HII regions with a methodology tested on model HII regions
• de Sitter Vacua in Type IIB String Theory: Classical Solutions and Quantum Corrections
• A Comparative Analysis of the Supernova Legacy Survey Sample with ΛCDM and the $R_{\mathrm{h}}=ct$ Universe
• Constraining a dark matter and dark energy interaction scenario with a dynamical equation of state
• Properties of HI discs in the Auriga cosmological simulations
• The Local Hole revealed by galaxy counts and redshifts
• Modeling the neutral hydrogen distribution in the post-reionization Universe: intensity mapping
• A comparison of observed and simulated absorption from HI, CIV, and SiIV around $z\approx 2$ star-forming galaxies suggests redshift-space distortions are due to inflows
• The Peccei-Quinn Symmetry from a Gauged Discrete R Symmetry
• Constraining the UV emissivity of AGN throughout cosmic time via X-ray surveys
• Comparison of dark energy models after Planck 2015
• Unveiling the nature of dark matter with high redshift 21 cm line experiments
• LBT observations of compact star-forming galaxies with extremely high [OIII]/[OII] flux ratios: HeI emission-line ratios as diagnostics of Lyman continuum leakage
• A model for core formation in dark matter haloes and ultra diffuse galaxies by outflow episodes
• Disruption of satellite galaxies in simulated groups and clusters: the roles of accretion time, baryons, and pre-processing
• Lepton Mixing Parameters from $\Delta (48)$ Family Symmetry and Generalised CP
• Strongly anomalous non-thermal fixed point in a quenched two-dimensional Bose gas
• Constraints on inert dark matter from metastability of the electroweak vacuum
• Cosmological constraints from baryon acoustic oscillations and clustering of large-scale structure
• The bias of cosmic voids in the presence of massive neutrinos
• Fast simulations for intensity mapping experiments
• Probing the galaxy-halo connection in UltraVISTA to $z\sim 2$
• MOA-II Galactic Microlensing Constraints: The Inner Milky Way has a Low Dark Matter Fraction and a Near Maximal Disk
• Constraints on particle dark matter from cosmic-ray antiprotons
• Phantom behavior via cosmological creation of particles
• Breaking of the equivalence principle in the electromagnetic sector and its cosmological signatures
• The evolution of the star formation rate function in the EAGLE simulations: A comparison with UV, IR and H$\alpha$ observations from z ~ 8 to z ~ 0
• Quenching timescales of galaxies in the EAGLE simulations
• CMB Delensing Beyond the B Modes
• Probing kinematics and fate of the Universe with linearly time-varying deceleration parameter
• First search for a dark matter annual modulation signal with NaI(Tl) in the Southern Hemisphere by DM-Ice17
• Cosmic variance of the local Hubble flow in large-scale cosmological simulations
• The SCUBA-2 Cosmology Legacy Survey: Multi-wavelengths counterparts to 10${}^3$ submillimeter galaxies in the UKIDSS-UDS field
• Milky Way mass constraints from the Galactic satellite gap
• Cosmology From CMB Lensing and Delensed EE Power Spectra Using 2019-2020 SPT-3G Polarization Data
• Rest-frame Optical Spectra and Black Hole Masses of 3<z<6 Quasars
• Cosmological evolution of a complex scalar field with repulsive or attractive self-interaction
• Theory for Baryon Number and Dark Matter at the LHC
• The quenching of galaxies, bulges, and disks since cosmic noon: A machine learning approach for identifying causality in astronomical data
• DHOST Bounce
• White Dwarfs constrain Dark Forces
• The Carnegie-Chicago Hubble Program. II. The Distance to IC 1613: The Tip of the Red Giant Branch and RR Lyrae Period-Luminosity Relations
• Dynamics of interacting quintessence
• The effect of Limber and flat-sky approximations on galaxy weak lensing
• Cosmic slowing down of acceleration for several dark energy parametrizations
• Double Beta Decay, Lepton Flavour Violation and Collider Signatures of Left-Right Symmetric Models with Spontaneous D Parity Breaking
• Cosmological perturbations in mimetic matter model
• Neutrinoless Double Beta Decay and the Baryon Asymmetry of the Universe
• Predicting the locations of possible long-lived low-mass first stars: Importance of satellite dwarf galaxies
• Direct detection of fermion dark matter in the radiative seesaw model
• Improving fast generation of halo catalogs with higher-order Lagrangian perturbation theory
• Just enough inflation: power spectrum modifications at large scales
• Cosmic expansion histories in massive bigravity with symmetric matter coupling
• Simulations for single-dish intensity mapping experiments
• Sterile neutrinos help reconcile the observational results of primordial gravitational waves from Planck and BICEP2
• Non-perturbative approach for curvature perturbations in stochastic-$\delta N$ formalism
• A multi-wavelength polarimetric study of the blazar CTA 102 during a Gamma-ray flare in 2012
• Looking at cosmic near-infrared background radiation anisotropies
• Nonlinear structure formation in Nonlocal Gravity
• Evolution of cosmological perturbations and the production of non-Gaussianities through a nonsingular bounce: Indications for a no-go theorem in single field matter bounce cosmologies
• Axions: Bose Einstein Condensate or Classical Field?
• A Minimal Model of Gravitino Dark Matter
• Measuring the Hubble constant and spatial curvature from supernova apparent magnitude, baryon acoustic oscillation, and Hubble parameter data
• The Grism Lens-Amplified Survey from Space (GLASS). II. Gas-phase metallicity and radial gradients in an interacting system at z~2
• Matter Power Spectrum in Hidden Neutrino Interacting Dark Matter Models: A Closer Look at the Collision Term
• SIMP model at NNLO in chiral perturbation theory
• Dark Matter Axion Search Using a Josephson Traveling Wave Parametric Amplifier
• Cosmological Parameter Estimation with Large Scale Structure Observations
• Teleparallel quintessence with a nonminimal coupling to a boundary term
• Testing the dark matter scenario in the inert doublet model by future precision measurements of the Higgs boson couplings
• Spatially adaptive radiation-hydrodynamical simulations of galaxy formation during cosmological reionization
• First CO(17-16) emission line detected in a z > 6 quasar
• P- and T-Violating Lagrangians in Chiral Effective Field Theory and Nuclear Electric Dipole Moments
• Radiative Neutrino Mass with Scotogenic Scalar Triplet
• Holographic dark energy from minimal supergravity
• GASP XXI. Star formation rates in the tails of galaxies undergoing ram-pressure stripping
• A Possible Explanation of Low Energy $\gamma$-ray Excess from Galactic Centre and Fermi Bubble by a Dark Matter Model with Two Real Scalars
• Measuring the speed of cosmological gravitational waves
• Acceleration of Universe by Nonlinear Electromagnetic Fields
• NIHAO XIII: Clumpy discs or clumpy light in high redshift galaxies?
• Revisiting cosmological bounds on sterile neutrinos
• Probing the baryogenesis and dark matter relaxed in phase transition by gravitational waves and colliders
• Halo model and halo properties in Galileon gravity cosmologies
• Constraints on cosmological parameters in power-law cosmology
• Coleman-Weinberg Inflation in light of Planck
• High-energy gamma-ray and neutrino backgrounds from clusters of galaxies and radio constraints
• The intra-cluster light as a tracer of the total matter density distribution: a view from simulations
• New approach for precise computation of Lyman-alpha forest power spectrum with hydrodynamical simulations
• Concentrations of Dark Haloes Emerge from Their Merger Histories
• A 14 $h^{-3}$ Gpc${}^3$ study of cosmic homogeneity using BOSS DR12 quasar sample
• The surprising accuracy of isothermal Jeans modelling of self-interacting dark matter density profiles
• Chemical evolution library for galaxy formation simulation
• Search for 100 MeV to 10 GeV gamma-ray lines in the Fermi-LAT data and implications for gravitino dark matter in the $\mu \nu$SSM
• Conformal Frame Dependence of Inflation
• The multiplicity and anisotropy of galactic satellite accretion
• From galactic nuclei to the halo outskirts: tracing supermassive black holes across cosmic history and environments
• CMB and BAO constraints for an induced gravity dark energy model with a quartic potential
• CO-dark molecular gas at high redshift: very large H${}_2$ content and high pressure in a low metallicity damped Lyman-alpha system
• RAiSE III: 3C radio AGN energetics and composition
• Baryonic acoustic oscillations from 21cm intensity mapping: the Square Kilometre Array case
• Evolution and Dynamics of a Matter creation model
• Dark matter and Higgs bosons in the MSSM
• Variations of the initial mass function in semi-analytical models: implications for the mass assembly and the chemical enrichment of galaxies in the GAEA model
• Biases in parameter estimation from overlapping gravitational-wave signals in the third generation detector era
• Higher order statistics of curvature perturbations in IFF model and its Planck constraints
• The Second Love Number of Dark Compact Planets and Neutron Stars with Dark Matter
• CMB weak-lensing beyond the Born approximation: a numerical approach
• Where the world stands still: turnaround as a strong test of ΛCDM cosmology
• NIHAO XX: The impact of the star formation threshold on the cusp-core transformation of cold dark matter haloes
• First observation of the thermal Sunyaev-Zel'dovich effect with kinetic inductance detectors
• Collisional production of sterile neutrinos via secret interactions and cosmological implications
• NIHAO VIII: Circum-galactic medium and outflows - The puzzles of HI and OVI gas distributions
• Multi-momentum and multi-flavour active-sterile neutrino oscillations in the early universe: role of neutrino asymmetries and effects on nucleosynthesis
• NIHAO VI. The hidden discs of simulated galaxies
• Cosmological Perturbations in Unimodular Gravity
• Probing the anisotropic expansion from supernovae and GRBs in a model-independent way
• Measurement Accuracy of Inspiraling Eccentric Neutron Star and Black Hole Binaries Using Gravitational Waves
• Dark Matter in the minimal Inverse Seesaw mechanism
• A robust deuterium abundance; Re-measurement of the z=3.256 absorption system towards the quasar PKS1937-1009
• Baryonic Dark Matter
• Dark Stars: A Review
• A Robust and Efficient Deep Learning Method for Dynamical Mass Measurements of Galaxy Clusters
• Combined search for neutrinos from dark matter self-annihilation in the Galactic Centre with ANTARES and IceCube
• A New Test of Lorentz Invariance Violation: the Spectral Lag Transition of GRB 160625B
• Inflation after False Vacuum Decay: Observational Prospects after Planck
• Leptogenesis via Axion Oscillations after Inflation
• Massive neutrinos and cosmic composition
• HALOGEN: A tool for fast generation of mock halo catalogues
• Probing the Majorana neutrinos and their CP violation in decays of charged scalar mesons $\pi ,K,D,D_s,B,B_c$
• The Impact of the Fiducial Cosmology Assumption on BAO Cosmological Parameter Inference
• A 331 WIMPy Dark Radiation Model
• Results from the Wilkinson Microwave Anisotropy Probe
• Dark matter monopoles, vectors and photons
• Baryon Content of Massive Galaxy Clusters (0.57 < z < 1.33)
• Reionization and Galaxy Formation in Warm Dark Matter Cosmologies
• Cross-correlation of Planck CMB Lensing and CFHTLenS Galaxy Weak Lensing Maps
• Active Galactic Nuclei and their Large-scale Structure: an eROSITA mock catalogue
• Global analysis of the pMSSM in light of the Fermi GeV excess: prospects for the LHC Run-II and astroparticle experiments
• Light, medium-weight or heavy? The nature of the first supermassive black hole seeds
• Extracting HI cosmological signal with Generalized Needlet Internal Linear Combination
• Music from the heavens - Gravitational waves from supermassive black hole mergers in the EAGLE simulations
• Constraining the redshifted 21-cm signal with the unresolved soft X-ray background
• Test of the cosmic evolution using Gaussian processes
• CMB Polarization B-mode Delensing with SPTpol and Herschel
• Deconstructing the neutrino mass constraint from galaxy redshift surveys
• Flavor-specific Interaction Favors Strong Neutrino Self-coupling in the Early Universe
• CνB absorption line in the neutrino spectrum at IceCube
• iPTF14yb: The First Discovery of a GRB Afterglow Independent of a High-Energy Trigger
• Parity-violating and anisotropic correlations in pseudoscalar inflation
• Tests of redshift-space distortions models in configuration space for the analysis of the BOSS final data release
• Multicomponent Dark Matter from Gauge Symmetry
• On the effect of the ionising background on the Lyα forest autocorrelation function
• Probing leptogenesis with GeV-scale sterile neutrinos at LHCb and BELLE II
• Fast and accurate CMB computations in non-flat FLRW universes
• Model-independent constraints on the cosmological anisotropic stress
• Clustering properties of $g$-selected galaxies at $z\sim 0.8$
• BAO+BBN revisited -- Growing the Hubble tension with a 0.7km/s/Mpc constraint
• A physical model for the evolving UV luminosity function of high redshift galaxies and their contribution to the cosmic reionization
• The Weak Lensing Radial Acceleration Relation: Constraining Modified Gravity and Cold Dark Matter theories with KiDS-1000
• Cosmological constraints on late-universe decaying dark matter as a solution to the $H_0$ tension
• Closing in on Resonantly Produced Sterile Neutrino Dark Matter
• A bias to CMB lensing measurements from the bispectrum of large-scale structure
• Relativistic stars in vector-tensor theories
• Cross-Correlation of Cosmic Shear and Extragalactic Gamma-ray Background: Constraints on the Dark Matter Annihilation Cross-Section
• Two-zero Majorana textures in the light of the Planck results
• Impacts of dark energy on weighing neutrinos after Planck 2015
• Present-day mass-metallicity relation for galaxies using a new electron-temperature method
• Constrained Local UniversE Simulations: A Local Group Factory
• Bright [CII] 158$\mu$m emission in a quasar host galaxy at $z=6.54$
• The formation of hot gaseous haloes around galaxies
• CMB and reheating constraints to α-attractor inflationary models
• Accuracy of Estimating Highly Eccentric Binary Black Hole Parameters with Gravitational-Wave Detections
• KiDS-1000: cosmic shear with enhanced redshift calibration
• Aurigaia: mock Gaia DR2 stellar catalogues from the Auriga cosmological simulations
• Bose-Einstein-condensed scalar field dark matter and the gravitational wave background from inflation: new cosmological constraints and its detectability by LIGO
• Geodesic Motion in Schwarzschild Spacetime Surrounded by Quintessence
• HST Emission Line Galaxies at z ~ 2: Comparing Physical Properties of Lyman Alpha and Optical Emission Line Selected Galaxies
• The SCUBA-2 Cosmology Legacy Survey: The EGS deep field I - Deep number counts and the redshift distribution of the recovered Cosmic Infrared Background at 450 and 850 um
• Combining power spectrum and bispectrum measurements to detect oscillatory features
• Reconstruction of the primordial power spectrum of curvature perturbations using multiple data sets
• Wormholes minimally violating the null energy condition
• Cross-correlating Planck tSZ with RCSLenS weak lensing: Implications for cosmology and AGN feedback
• Cosmological constraints from the CFHTLenS shear measurements using a new, accurate and flexible way of predicting nonlinear mass clustering
• Abundances of lithium, oxygen, and sodium in the turn-off stars of Galactic globular cluster 47 Tuc
• Probing Cosmological Isotropy With Type IA Supernovae
• Warm Dark Matter Constraints Using Milky-Way Satellite Observations and Subhalo Evolution Modeling
• Antimatter and antistars in the universe and in the Galaxy
• Constraints on massive neutrinos from the pairwise kinematic Sunyaev-Zel'dovich effect
• Generalized second law of thermodynamics in f(R,T) theory of gravity
• $N_{\mathrm{eff}}$ in low-scale seesaw models versus the lightest neutrino mass
• Testing loop quantum cosmology
• 3FGL Demographics Outside the Galactic Plane using Supervised Machine Learning: Pulsar and Dark Matter Subhalo Interpretations
• Can a supervoid explain the Cold Spot?
• Statistics of the epoch of reionization (EoR) 21-cm signal -- II. The evolution of the power spectrum error-covariance
• Results from EDGES High-Band: III. New Constraints on Parameters of the Early Universe
• BICEP2 III: Instrumental Systematics
• Scalar dark matter in the B-L model
• Large-scale clustering of Lyman-alpha emission intensity from SDSS/BOSS
• Effective Fluid Description of the Dark Universe
• Disformal Gravity Theories: A Jordan Frame Analysis
• Gravity and Scalar Fields
• Nonlinear Electromagnetic Fields As a Source of Universe Acceleration
• An Antenna for Directional Detection of WISPy Dark Matter
• From Resonant to Broadband Searches for WISPy Cold Dark Matter
• LHC Phenomenology of Type II Seesaw: Nondegenerate Case
• Imaging the redshifted 21-cm pattern around the first sources during the cosmic dawn using the SKA
• In search of the dark matter dark energy interaction: a kinematic approach
• Impact of Semi-annihilation of Z3 Symmetric Dark Matter with Radiative Neutrino Masses
• Detecting Relic Gravitational Waves by Pulsar Timing Arrays: Effects of Cosmic Phase Transitions and Relativistic Free-Streaming Gases
• Spherical collapse in $\nu \Lambda CDM$
• Cosmological constraints from galaxy-lensing cross correlations using BOSS galaxies with SDSS and CMB lensing
• Degree-Scale CMB Polarization Measurements from Three Years of BICEP1 Data
• Exploring cosmic origins with CORE: gravitational lensing of the CMB
• New Insights of Electroweak Phase Transition in NMSSM
• The halo model in a massive neutrino cosmology
• Advancing LHC Probes of Dark Matter from the Inert 2-Higgs Doublet Model with the Mono-jet Signal
• A spinning supermassive black hole binary model consistent with VLBI observations of the S5 1928+738 jet
• How to Reconcile the Observed Velocity Function of Galaxies with Theory
• The matter distribution in the local Universe as derived from galaxy groups in SDSS DR12 and 2MRS
• Anisotropic dark energy model with a hybrid scale factor
• Universal at last? The splashback mass function of dark matter halos
• Dissecting the high-z interstellar medium through intensity mapping cross-correlations
• Search for CII Emission on Cosmological Scales at Redshift Z~2.6
• NMSSM with a singlino LSP: possible challenges for searches for supersymmetry at the LHC
• Independent Cosmological Constraints from high-z HII Galaxies
• Prospects for Delensing the Cosmic Microwave Background for Studying Inflation
• Independent cosmological constraints from high-z HII galaxies: new results from VLT-KMOS data
• The scatter and evolution of the global hot gas properties of simulated galaxy cluster populations
• Models of dark matter halos based on statistical mechanics: I. The classical King model
• Gravitational waves: Classification, Methods of detection, Sensitivities, and Sources
• Primordial backgrounds of relic gravitons
• Cosmology in bimetric theory with an effective composite coupling to matter
• Distinguishing a Kerr-like black hole and a naked singularity in perfect fluid dark matter via precession frequencies
• H0LiCOW II. Spectroscopic survey and galaxy-group identification of the strong gravitational lens system HE0435-1223
• Statistical Inconsistencies in the KiDS-450 Dataset
• Tidal dwarf galaxies in cosmological simulations
• The impact of relativistic effects on cosmological parameter estimation
• Light curves and spectra from off-axis gamma-ray bursts
• The Clustering of Galaxies in the Completed SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from DR12 galaxy clustering -- towards an accurate model
• The Edge of the Galaxy
• Assessing Astrophysical Uncertainties in Direct Detection with Galaxy Simulations
• Light Dark Matter, Naturalness, and the Radiative Origin of the Electroweak Scale
• The Clustering of Galaxies in the SDSS-III DR10 Baryon Oscillation Spectroscopic Survey: No Detectable Colour Dependence of Distance Scale or Growth Rate Measurements
• Exploring the origin of low-metallicity stars in Milky Way-like galaxies with the NIHAO-UHD simulations
• Improving cosmological parameter estimation with the future gravitational-wave standard siren observation from the Einstein Telescope
• Limits on Population III star formation in minihaloes implied by Planck
• Light sterile neutrinos after BICEP-2
• Unifying inflation and dark matter with the Peccei-Quinn field: observable axions and observable tensors
• Properties of Dark Matter Halos as a Function of Local Environment Density
• The imprint of cosmic reionisation on the luminosity function of galaxies
• New observational constraints on $f(T)$ cosmology from radio quasars
• Tracing the first stars and galaxies of the Milky Way
• Internal bremsstrahlung signatures in light of direct dark matter searches
• A description of the Galactic Center excess in the Minimal Supersymmetric Standard Model
• Viability of bouncing cosmology in energy-momentum-squared gravity
• DEMNUni: Massive neutrinos and the bispectrum of large scale structures
• Gamma-ray flaring activity from the gravitationally lensed blazar PKS 1830-211 observed by Fermi LAT
• Self-consistent Semi-analytic Modeling of Feedback During Primordial Star Formation and Reionization
• A No-Go Theorem for Direct Collapse Black Holes Without a Strong Ultraviolet Background
• Statistics of extreme objects in the Juropa Hubble Volume simulation
• Two component WIMP-FImP dark matter model with singlet fermion, scalar and pseudo scalar
• Predictions and sensitivity forecasts for reionization-era [C II] line intensity mapping
• The prevalence of pseudo-bulges in the Auriga simulations
• The effect of non-Gaussianity on error predictions for the Epoch of Reionization (EoR) 21-cm power spectrum
• Inflationary universe in terms of a van der Waals viscous fluid
• The Konus-Wind catalog of gamma-ray bursts with known redshifts. II. Waiting mode bursts simultaneously detected by Swift/BAT
• Warm Inflation in $f(\mathcal{G})$ Theory of Gravity
• Generalised uncertainty relations from superpositions of geometries
• A New Precision Measurement of the Small-Scale Line-of-Sight Power Spectrum of the Ly$\alpha$ Forest
• The Dekel-Zhao profile: A mass-dependent dark-matter density profile with flexible inner slope and analytic potential, velocity dispersion, and lensing properties
• Where does galactic dust come from?
• Banana Split: Testing the Dark Energy Consistency with Geometry and Growth
• Dark-Matter Harmonics Beyond Annual Modulation
• The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for the Quasar Sample
• Velocity dispersion in the interstellar medium of early galaxies
• Lyman-alpha emitters gone missing: the different evolution of the bright and faint populations
• EDGE: Two routes to dark matter core formation in ultra-faint dwarfs
• Improved constraints on lepton asymmetry from the cosmic microwave background
• Search for Gamma-ray Emission from Dark Matter Annihilation in the Large Magellanic Cloud with the Fermi Large Area Telescope
• The importance of black hole repositioning for galaxy formation simulations
• Model independent inference of the expansion history and implications for the growth of structure
• The short ionizing photon mean free path at z=6 in Cosmic Dawn III, a new fully-coupled radiation-hydrodynamical simulation of the Epoch of Reionization
• Hydrogen Reionization in the Illustris universe
• An evaluation of cosmological models from expansion and growth of structure measurements
• Broadband, radio spectro-polarimetric study of 100 radiative-mode and jet-mode AGN
• Changing the prior: absolute neutrino mass constraints in nonlocal gravity
• Absolute Ages and Distances of 22 GCs using Monte Carlo Main-Sequence Fitting
• Light axion-like dark matter must be present during inflation
• On the Evolution of the Cosmic Ionizing Background
• Soft X-ray Excess in the Coma Cluster from a Cosmic Axion Background
• Theoretical and observational constraints on the HI intensity power spectrum
• The Atacama Cosmology Telescope: Dynamical masses for 44 SZ-selected galaxy clusters over 755 square degrees
• B-modes and the Nature of Inflation
• Sensitivity to oscillation with a sterile fourth generation neutrino from ultra-low threshold neutrino-nucleus coherent scattering
• Model independent calibrations of gamma ray bursts using machine learning
• Intensity mapping with SDSS/BOSS Lyman-alpha emission, quasars and their Lyman-alpha forest
• Chiral Gravity Waves and Leptogenesis in Inflationary Models with non-Abelian Gauge Fields
• Alignments between galaxies, satellite systems and haloes
• 21-cm signal from cosmic dawn - II: Imprints of the light-cone effects
• The evolution of SMBH spin and AGN luminosities for $z<6$ within a semi-analytic model of galaxy formation
• Localized massive halo properties in Bahamas and Macsis simulations: scalings, log-normality, and covariance
• A Comprehensive Study of Detectability and Contamination in Deep Rapid Optical Searches for Gravitational Wave Counterparts
• Frame Covariant Nonminimal Multifield Inflation
• Excluding Black Hole Firewalls with Extreme Cosmic Censorship
• Improved Limits on Sterile Neutrino Dark Matter using Full-Sky Fermi Gamma-Ray Burst Monitor Data
• Galaxy merger histories and the role of merging in driving star formation at z>1
• On the shape of dark matter halos from MultiDark Planck simulations
• The Rise of Active Galactic Nuclei in the GAlaxy Evolution and Assembly semi-analytic model
• Can $f(T)$ gravity resolve the $H_0$ tension?
• Nonzero ${\theta }_{13}$ and Leptogenesis in a Type-I See-saw Model with $A_4$ Symmetry
• The SLUGGS Survey: Dark matter fractions at large radii and assembly epochs of early-type galaxies from globular cluster kinematics
• Cosmological implications of scale-independent energy-momentum squared gravity: Pseudo nonminimal interactions in dark matter and relativistic relics
• Constraints on a generalized deceleration parameter from cosmic chronometers
• A search for sterile neutrinos with the latest cosmological observations
• Simulations of the OzDES AGN Reverberation Mapping Project
• Mocking the Weak Lensing universe: the LensTools python computing package
• NIHAO XII: galactic uniformity in a ΛCDM universe
• Shaken, not stirred: kinetic mixing in scalar-tensor theories of gravity
• Galactic Scale Feedback Observed in the 3C 298 Quasar Host Galaxy
• Measurements of E-Mode Polarization and Temperature-E-Mode Correlation in the Cosmic Microwave Background from 100 Square Degrees of SPTpol Data
• First-order Cosmological Perturbations Engendered by Point-like Masses
• Acceleration of the universe: a reconstruction of the effective equation of state
• Addressing the too big to fail problem with baryon physics and sterile neutrino dark matter
• Efficient simulations of large scale structure in modified gravity cosmologies with comoving Lagrangian acceleration
• A parametric reconstruction of the cosmological jerk from diverse observational data sets
• Dwarf spheroidal galaxies as degenerate gas of free fermions
• Gravothermal solutions of SIDM halos: mapping from constant to velocity-dependent cross section
• LHC constraints on light neutralino dark matter in the MSSM
• Scalar Representations in the Light of Electroweak Phase Transition and Cold Dark Matter Phenomenology
• Robust model comparison disfavors power law cosmology
• Can primordial magnetic fields be the origin of the BICEP2 data?
• Constraints on secret neutrino interactions after Planck
• Mapping the Chevallier-Polarski-Linder parametrization onto Physical Dark Energy Models
• The effective field theory of inflation/dark energy and the Horndeski theory
• ColDICE: a parallel Vlasov-Poisson solver using moving adaptive simplicial tessellation
• Symmetry violations in nuclear and neutron $\beta$ decay
• Modelling the observed luminosity function and clustering evolution of Lyman-$\alpha$ emitters: growing evidence for late reionization
• Probing the intra-group medium of a z = 0.28 galaxy group
• CFHTLenS and RCSLenS: Testing Photometric Redshift Distributions Using Angular Cross-Correlations with Spectroscopic Galaxy Surveys
• Accurate Shear Measurement with Faint Sources
• Measurement of the halo bias from stacked shear profiles of galaxy clusters
• Explaining $B\to K^{(\ast )}{\ell }^{+}{\ell }^{-}$ anomaly by radiatively induced coupling in $U(1{)}_{\mu -\tau }$ gauge symmetry
• The origin of the $\alpha$-enhancement of massive galaxies
• Natural SUSY in Plain Sight
• Reconstruction of the Scalar Field Potential in Inflationary Models with a Gauss-Bonnet term
• Constraints on the Lyman continuum escape fraction for faint star forming galaxies
• Status of CMSSM in light of current LHC Run-2 and LUX data
• Universal features of quantum bounce in loop quantum cosmology
• Low Variance at large scales of WMAP 9 year data
• Cosmic acceleration without dark energy: Background tests and thermodynamic analysis
• Properties of Local Group galaxies in hydrodynamical simulations of sterile neutrino dark matter cosmologies
• A search for pair production of new light bosons decaying into muons in proton-proton collisions at 13 TeV
• Neutrinos in the holographic dark energy model: constraints from latest measurements of expansion history and growth of structure
• Towards simulating and quantifying the light-cone EoR 21-cm signal
• Comparing galaxy formation in semi-analytic models and hydrodynamical simulations
• Leptogenesis and Primordial Magnetic Fields
• Constraining the HI-Halo Mass Relation From Galaxy Clustering
• Nonthermal Two Component Dark Matter Model for Fermi-LAT $\gamma$-ray excess and 3.55 keV X-ray Line
• Discrimination of dark matter models in future experiments
• Search for a Variation of the Fine Structure around the Supermassive Black Hole in Our Galactic Center
• The faint radio sky: VLBA observations of the COSMOS field
• Simulating Neutron Star Mergers as r-process Sources in Ultra Faint Dwarf Galaxies
• ALMA and GMRT constraints on the off-axis gamma-ray burst 170817A from the binary neutron star merger GW170817
• Resolved galaxy scaling relations in the EAGLE simulation: star formation, metallicity and stellar mass on kpc scales
• Spectral Energy Distribution Fitting of HETDEX Pilot Survey Lyman-alpha Emitters in COSMOS and GOODS-N
• Dynamical Mass Measurements of Contaminated Galaxy Clusters Using Machine Learning
• Cosmic ray propagation and dark matter in light of the latest AMS-02 data
• Dark Energy and Dark Matter from an additional adiabatic fluid
• Electroweak breaking and Dark Matter from the common scale
• Dark matter substructure modelling and sensitivity of the Cherenkov Telescope Array to Galactic dark halos
• Distinguishing models of reionization using future radio observations of 21-cm 1-point statistics
• Towards a Supersymmetric Description of the Fermi Galactic Center Excess
• Constraining Non-thermal and Thermal properties of Dark Matter
• Post-ACME2013 CP-violation in Higgs Physics and Electroweak Baryogenesis
• Dark energy scenario consistent with GW170817 in theories beyond Horndeski gravity
• Searching for Oscillations in the Primordial Power Spectrum: Perturbative Approach (Paper I)
• Extragalactic Imprints in Galactic Dust Maps
• Possible Interpretations of IceCube High-Energy Neutrino Events
• GRB171205A/SN2017iuk: A local low-luminosity gamma-ray burst
• Dirac Neutrinos with $S_4$ Flavor Symmetry in Warped Extra Dimensions
• Introducing EMP-Pathfinder: modelling the simultaneous formation and evolution of stellar clusters in their host galaxies
• Cancellation mechanism for the electron electric dipole moment connected with the baryon asymmetry of the Universe
• The Linear Growth of Structure in the R_h=ct Universe
• The effects of dynamical substructure on Milky Way mass estimates from the high velocity tail of the local stellar halo
• Impact of neutrino flavor oscillations on the neutrino-driven wind nucleosynthesis of an electron-capture supernova
• The CTA aims at the Inert Doublet Model
• Propagation of Ultra High Energy Cosmic Rays in Extragalactic Magnetic Fields: A view from cosmological simulations
• Quantum cosmology and late-time singularities
• Neutrino Mixing and Geometric CP Violation with Delta(27) Symmetry
• Lepton flavor violating decays of vector quarkonia and of the $Z$ boson
• Unveiling secret interactions among sterile neutrinos with big-bang nucleosynthesis
• Hi intensity mapping with MeerKAT: Primary beam effects on foreground cleaning
• Stars behind bars I: The Milky Way's central stellar populations
• Properties of ionized outflows in MaNGA DR2 galaxies
• Dark matter halo shapes in the Auriga simulations
• Warm and cold fermionic dark matter via freeze-in
• Old-minimal supergravity models of inflation
• The Stellar Populations of Two Ultra-Diffuse Galaxies from Optical and Near-infrared Photometry
• An alternative to the LCDM model: the case of scale invariance
• Polyspectra searches for sharp oscillatory features in cosmic microwave sky data
• Kinematic constraints beyond $z\simeq 0$ using calibrated GRB correlations
• Reducing Noise in Cosmological N-body Simulations with Neutrinos
• Matter Power Spectrum Emulator for f(R) Modified Gravity Cosmologies
• Fermi-LAT Observations of the 2014 May-July outburst from 3C 454.3
• Protocluster Discovery in Tomographic Ly$\alpha$ Forest Flux Maps
• Cosmological bounds on dark matter-photon coupling
• Maximal compression of the redshift space galaxy power spectrum and bispectrum
• From a Bounce to the Dark Energy Era with $F(R)$ Gravity
• Mass and star formation rate of the host galaxies of compact binary mergers across cosmic time
• Properties of simulated galaxies and supermassive black holes in cosmic voids
• Mock catalogs for the extragalactic X-ray sky: simulating AGN surveys with Athena and with the AXIS probe
• On the stellar halo metallicity profile of Milky Way-like galaxies in the Auriga simulations
• Hybrid Inflation in the Complex Plane
• Evading Weinberg's no-go theorem to construct mass dimension one fermions: Constructing darkness
• Doublet-Triplet Fermionic Dark Matter
• Wormhole geometries in Eddington-inspired Born-Infeld gravity
• Anisotropic inflation reexamined: upper bound on broken rotational invariance during inflation
• CLASH: Accurate Photometric Redshifts with 14 HST bands in Massive Galaxy Cluster Cores
• General Dynamics of Varying-Alpha Universes
• The Hydrodynamic Feedback of Cosmic Reionization on Small-Scale Structures and Its Impact on Photon Consumption during the Epoch of Reionization
• RAyMOND: An N-body and hydrodynamics code for MOND
• Multi-wavelength constraints on the inflationary consistency relation
• Galactic inflow and wind recycling rates in the EAGLE simulations
• Neutrinoless Double Beta Decay in the Presence of Light Sterile Neutrinos
• Late-time decaying dark matter: constraints and implications for the $H_0$-tension
• Dynamics and cosmological evolution in Λ-varying cosmology
• The Splashback Radius of Planck-SZ clusters
• Measurement of the small-scale structure of the intergalactic medium using close quasar pairs
• A direct measurement of galaxy major and minor merger rates and stellar mass accretion histories at $z<3$ using galaxy pairs in the REFINE survey
• KASHz: No evidence for ionised outflows instantaneously suppressing star formation in moderate luminosity AGN at $z$$\sim$$1.4$-$2.6$
• Coupled Boltzmann computation of mixed axion neutralino dark matter in the SUSY DFSZ axion model
• Relating quarks and leptons with the T7 flavour group
• Dark matter and halo bispectrum in redshift space: theory and applications
• On the Bias of the Distance-Redshift Relation from Gravitational Lensing
• The ACS Survey of Galactic Globular Clusters XIV: Bayesian Single-Population Analysis of 69 Globular Clusters
• An analysis of the $H_0$ tension problem in a universe with a viscous dark fluid
• Galaxy Formation as a Cosmological Tool. I: The Galaxy Merger History as a Measure of Cosmological Parameters
• Cosmic shear full nulling: sorting out dynamics, geometry and systematics
• How an improved implementation of H2 self-shielding influences the formation of massive stars and black holes
• Accelerated and decelerated expansion in a causal dissipative cosmology
• Weak-Lensing Mass Calibration of the Atacama Cosmology Telescope Equatorial Sunyaev-Zeldovich Cluster Sample with the Canada-France-Hawaii Telescope Stripe 82 Survey
• Distinguishing interacting dark energy from wCDM with CMB, lensing, and baryon acoustic oscillation data
• The missing link: a nonlinear post-Friedmann framework for small and large scales
• Emergence of a Dark Force in Corpuscular Gravity
• Bianchi-V String Cosmological model with Dark Energy Anisotropy
• The Relationship Between Star-formation Activity and Galaxy Structural Properties in CANDELS and a Semi-analytic Model
• Test of parametrized post-Newtonian gravity with galaxy-scale strong lensing systems
• Accurate mass and velocity functions of dark matter halos
• Reduced LHC constraints for higgsino-like heavier electroweakinos
• Cosmological constraints from the BOSS DR12 void size function
• Searching for Secluded Dark Matter with H.E.S.S., Fermi-LAT, and Planck
• Update on Light WIMP Limits: LUX, lite and Light
• Cosmic microwave background constraints on secret interactions among sterile neutrinos
• Limits on the power-law mass and luminosity density profiles of elliptical galaxies from gravitational lensing systems
• Rapid early coeval star formation and assembly of the most massive galaxies in the universe
• Modelling the post-reionization neutral Hydrogen (\HI) bias
• Unified dark fluid in Brans-Dicke theory
• The Perils of Analytic Continuation
• Non-local gravity and comparison with observational datasets. II. Updated results and Bayesian model comparison with $\Lambda$CDM
• Gaugino coannihilations
• Hints, neutrino bounds and WDM constraints from SDSS DR14 Lyman-$\alpha$ and Planck full-survey data
• LoCuSS: The infall of X-ray groups onto massive clusters
• Probing cosmology with weak lensing selected clusters I: Halo approach and all-sky simulations
• Damping Wing-Like Features in the Stacked Ly$\alpha$ Forest: Potential Neutral Hydrogen Islands at $z<6$
• Self-Interacting Dark Matter and Small-Scale Gravitational Lenses in Galaxy Clusters
• Prediction of the 21-cm signal from reionization: comparison between 3D and 1D radiative transfer schemes
• Testing the equation of state for viscous dark energy
• Majorana dark matter in a classically scale invariant model
• Sterile neutrino Dark Matter production from scalar decay in a thermal bath
• Simulating the diversity of shapes of the Lyman-$\alpha$ line
• Cosmic evolution and thermal stability of Barrow holographic dark energy in nonflat Friedmann-Robertson-Walker Universe
• Observations of the Lyman series forest towards the redshift 7.1 quasar ULAS J1120+0641
• Observational selection biases in time-delay strong lensing and their impact on cosmography
• Search for a gamma-ray line feature from a group of nearby Galaxy clusters with Fermi LAT Pass 8 data
• Searching for metal-deficient emission-line galaxy candidates: the final sample of the SDSS DR12 galaxies
• Observations of a nearby filament of galaxy clusters with the Sardinia Radio Telescope
• First data from DM-Ice17
• Constraining anisotropic models of the early Universe with WMAP9 data
• Anomaly-free flavor models for Nambu-Goldstone bosons and the 3.5 keV X-ray line signal
• Graph Theoretical Analysis Reveals: Women's Brains are Better Connected than Men's
• Baryonic effects on the matter bispectrum
• Searching for Modified Gravity: Scale and Redshift Dependent Constraints from Galaxy Peculiar Velocities
• No excess of bright galaxies around the redshift 7.1 quasar ULAS J1120+0641
• 2HOT: An Improved Parallel Hashed Oct-Tree N-Body Algorithm for Cosmological Simulation
• Signatures of Horndeski gravity on the Dark Matter Bispectrum
• A KiDS weak lensing analysis of assembly bias in GAMA galaxy groups
• Dark matter and muon $(g-2)$ in local $U(1{)}_{L_{\mu }-L_{\tau }}$-extended Ma Model
• The connection between the radio jet and the gamma-ray emission in the radio galaxy 3C 120
• Light Dark Matter through Assisted Annihilation
• Photon number conservation and the large-scale 21 cm power spectrum in semi-numerical models of reionization
• Oscillation of heavy sterile neutrino in decay of $B\to \mu e\pi$
• Probing the diffuse baryon distribution with the lensing-tSZ cross-correlation
• A Hubble diagram from Type II Supernovae based solely on photometry: the Photometric-Colour Method
• EMMA: an AMR cosmological simulation code with radiative transfer
• Accelerating cosmological expansion from shear and bulk viscosity
• The SLUGGS Survey: A comparison of total-mass profiles of early-type galaxies from observations and cosmological simulations, to $\sim$4 effective radii
• Scalar-Fluid interacting dark energy: cosmological dynamics beyond the exponential potential
• Radio Galaxy Zoo: A Search for Hybrid Morphology Radio Galaxies
• On structure formation from a small-scales-interacting dark sector
• The diverse nature and formation paths of slow rotator galaxies in the EAGLE simulations
• The Knotted Sky II: Does BICEP2 require a nontrivial primordial power spectrum?
• Approximate Bayesian Computation in Large Scale Structure: constraining the galaxy-halo connection
• Constraining dark matter properties with Cosmic Microwave Background observations
• Here be Dragons: The Unexplored Continents of the CMSSM
• A New Statistical Model for Population III Supernova Rates: Discriminating Between $\Lambda$CDM and WDM Cosmologies
• J1234+3901: an extremely metal-deficient compact star-forming dwarf galaxy at redshift 0.133
• Simulating the growth of Intermediate Mass Black Holes
• Lepton Flavor Mixing and CP Symmetry
• Constraining the second half of reionization with the Lyman-$\beta$ forest
• Hemispherical Asymmetry and Local non-Gaussianity: a Consistency Condition
• CosmicGrowth Simulations---Cosmological simulations for structure growth studies
• EFTCAMB/EFTCosmoMC: massive neutrinos in dark cosmologies
• Accelerating Universe in Hybrid and Logarithmic Teleparallel Gravity
• Enhancing BOSS bispectrum cosmological constraints with maximal compression
• Dark Energy Survey Year 1 Results: Constraining Baryonic Physics in the Universe
• New Constraints on Higgs-portal Scalar Dark Matter
• HI-selected Galaxies in Hierarchical Models of Galaxy Formation and Evolution
• The dependence of the galaxy stellar-to-halo mass relation on galaxy morphology
• Constraining the Cosmic Baryon Distribution with Fast Radio Burst Foreground Mapping
• A New Approach to Cosmological Bulk Viscosity
• ETHOS -- an effective theory of structure formation: predictions for the high-redshift Universe -- abundance of galaxies and reionization
• A Relationship Between Halo Mass, Cooling, AGN Heating, and the Coevolution of Massive Black Holes
• Planck confronts large scale structure: methods to quantify discordance
• An improved measurement of baryon acoustic oscillations from the correlation function of galaxy clusters at $z\sim 0.3$
• Large-Scale Structure Observables in General Relativity
• Observational Constraints on Monomial Warm Inflation
• Constraints on hybrid metric-Palatini models from background evolution
• Real-space density profile reconstruction of stacked voids
• On the relative bias of void tracers in the Dark Energy Survey
• Direct collapse black hole formation via high-velocity collisions of protogalaxies
• Modelling and testing the equation of state for (Early) dark energy
• Growing a `Cosmic Beast': Observations and Simulations of MACS J0717.5+3745
• Bayesian 3d velocity field reconstruction with VIRBIuS
• Probing gravity with a joint analysis of galaxy and CMB lensing and SDSS spectroscopy
• Bouncing alternatives to inflation
• The chemical enrichment of long-GRB nurseries up to z=2
• On the universality of luminosity-metallicity and mass-metallicity relations for compact star-forming galaxies at redshifts 0 < z < 3
• Natural NMSSM after LHC Run I and the Higgsino dominated dark matter scenario
• Direct Measurement of the HI-Halo Mass Relation through Stacking
• Intergalactic magnetic field spectra from diffuse gamma rays
• Time Delay Lens Modelling Challenge
• The impact of stellar and AGN feedback on halo-scale baryonic and dark matter accretion in the EAGLE simulations
• The distribution and physical properties of high-redshift [OIII] emitters in a cosmological hydrodynamics simulation
• The Atacama Cosmology Telescope: measuring radio galaxy bias through cross-correlation with lensing
• Precise Measurements of Primordial Power Spectrum with 21 cm Fluctuations
• Cosmological Parameters from pre-Planck CMB Measurements: a 2017 Update
• Non-Universalities in Pure Gravity Mediation
• Radio Galaxy Zoo: The Distortion of Radio Galaxies by Galaxy Clusters
• On the Direct Detection of Dark Matter Annihilation
• Bayesian Evidence against Harrison-Zel'dovich spectrum in tension cosmology
• Observational evidence of galaxy assembly bias
• Impact of baryons on the cluster mass function and cosmological parameter determination
• Modelling high resolution ALMA observations of strongly lensed highly star forming galaxies detected by Herschel
• Reannihilation of self-interacting dark matter
• Dark Radiation or Warm Dark Matter from long lived particle decays in the light of Planck
• Early observations of the nearby type Ia supernova SN 2015F
• Lyman-Alpha Emitting Galaxies as a Probe of Reionization: Large-Scale Bubble Morphology and Small-Scale Absorbers
• Massive and supermassive black holes in the contemporary and early universe and the new problems of cosmology and astrophysics
• Hubble constant and dark energy inferred from free-form determined time delay distances
• An elliptical accretion disk following the tidal disruption event AT 2020zso
• Axion dark matter from Higgs inflation with an intermediate $H_{\ast }$
• Directional Sensitivity In Light-Mass Dark Matter Searches With Single-Electron Resolution Ionization Detectors
• Connecting neutrino physics with dark matter
• AGN feedback, quiescence and CGM metal enrichment in early-type galaxies
• Fits to the Fermi-LAT GeV excess with RH sneutrino dark matter: implications for direct and indirect dark matter searches and the LHC
• Cosmological constraints from Subaru weak lensing cluster counts
• Voids in Modified Gravity Reloaded: Eulerian Void Assignment
• Towards the statistical detection of the warm-hot intergalactic medium in inter-cluster filaments of the cosmic web
• Constrained realizations of 2MRS density and peculiar velocity fields: growth rate and local flow
• The Cosmic Microwave Background: The history of its experimental investigation and its significance for cosmology
• Constraints on neutrino mass from Cosmic Microwave Background and Large Scale Structure
• Neutrinos and dark energy after Planck and BICEP2: data consistency tests and cosmological parameter constraints
• The bursting nature of star formation in compact star-forming galaxies from the Sloan Digital Sky Survey
• $\Lambda (t)$ cosmology induced by a slowly varying Elko field
• 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
• Evidence of cross-correlation between the CMB lensing and the gamma-ray sky
• Subaru Telescope adaptive optics observations of gravitationally lensed quasars in the Sloan Digital Sky Survey
• Investigating Cepheid $\ell$ Carinae's Cycle-to-cycle Variations via Contemporaneous Velocimetry and Interferometry
• ${\varphi }^2$ Inflation at its Endpoint
• MultiModeCode: An efficient numerical solver for multifield inflation
• Accretion disc cooling and narrow absorption lines in the tidal disruption event AT 2019dsg
• Modified Gravity Constraints from the Full Shape Modeling of Clustering Measurements from DESI 2024
• The significance of anisotropic signals hiding in the type Ia supernovae
• Maximum redshift of gravitational wave merger events
• A loophole to the universal photon spectrum in electromagnetic cascades: application to the "cosmological lithium problem"
• A Detailed Look at the First Results from the Large Underground Xenon (LUX) Dark Matter Experiment
• Cosmological aspects of a hyperbolic solution in $f(R,T)$ gravity
• A quasar reddened by a sub-parsec sized, metal-rich and dusty cloud in a damped Lyman-alpha absorber at z=2.13
• Probing dark matter with star clusters: a dark matter core in the ultra-faint dwarf Eridanus II
• Deviation from Bimaximal Mixing and Leptonic CP Phases in $S_4$ Family Symmetry and Generalized CP
• Massive Photon and Dark Energy
• A light NMSSM pseudoscalar Higgs boson at the LHC redux
• Linking gas and galaxies at high redshift: MUSE surveys the environments of six damped Lyman alpha galaxies at z~3
• Galaxy evolution in protoclusters
• Relic Neutrino Freeze-out: Dependence on Natural Constants
• Testing deviations from $\Lambda$CDM with growth rate measurements from 6 Large Scale Structure Surveys at $\mathbf{z}=0.06$ to 1
• The better half -- Asymmetric star-formation due to ram pressure in the EAGLE simulations
• Low-redshift lowest-metallicity star-forming galaxies in the SDSS DR14
• Diagnosing galactic feedback with the line broadening in the low redshift Lyman-alpha forest
• Flavored Peccei-Quinn symmetry
• Formation of the first star clusters and massive star binaries by fragmentation of filamentary primordial gas clouds
• The Jubilee ISW Project II: observed and simulated imprints of voids and superclusters on the cosmic microwave background
• Evolution of Star-forming Galaxies from z = 0.7 to 1.2 with eBOSS Emission-line Galaxies
• Cosmic variance limited Baryon Acoustic Oscillations from the DEUS-FUR $\Lambda$CDM simulation
• The origin of the enhanced metallicity of satellite galaxies
• Minimal Vector-like leptonic Dark Matter and Signatures at the LHC
• Probing galaxy evolution in massive clusters using ACT and DES: splashback as a cosmic clock
• Figuring Out Gas & Galaxies in Enzo (FOGGIE). II. Emission from the z=3 Circumgalactic Medium
• Testing statistics of the CMB B-mode polarization toward unambiguously establishing quantum fluctuation of vacuum
• On the scalar consistency relation away from slow roll
• $Z$ boson mediated dark matter beyond the effective theory
• Exploring the nature of the Lyman-$\alpha$ emitter CR7
• The SCUBA-2 Cosmology Legacy Survey: The EGS deep field - II. Morphological transformation and multi-wavelength properties of faint submillimetre galaxies
• Evolution of galactic planes of satellites in the EAGLE simulation
• Principal Component Analysis of Modified Gravity using Weak Lensing and Peculiar Velocity Measurements
• Leptogenesis from left-handed neutrino production during axion inflation
• Adiabatic contraction revisited: implications for primordial black holes
• On the possibility of wormhole formation in the galactic halo due to dark matter Bose-Einstein condensates
• Eternal Higgs inflation and cosmological constant problem
• Simulated ΛCDM analogues of the thin Plane of Satellites around the Andromeda galaxy are not kinematically coherent structures
• Global stability analysis for cosmological models with non-minimally coupled scalar fields
• Three Loop Neutrino Model with Isolated $k^{\pm \pm }$
• Recycled stellar ejecta as fuel for star formation and implications for the origin of the galaxy mass-metallicity relation
• Neutrino mixing with non-zero ${\theta }_{13}$ and CP violation in the 3-3-1 model based on $A_4$ flavor symmetry
• Gravitationally induced adiabatic particle production: From Big Bang to de Sitter
• Comparing M31 and Milky Way Satellites: The Extended Star Formation Histories of Andromeda II and Andromeda XVI
• The Abundance and Structure of Subhaloes near the Free Streaming Scale and Their Impact on Indirect Dark Matter Searches
• Gravity at the horizon: on relativistic effects, CMB-LSS correlations and ultra-large scales in Horndeski's theory
• Suite of Hydrodynamical Simulations for the Lyman-Alpha Forest with Massive Neutrinos
• Probing the end of reionization with the near-zones of z > 6 QSOs
• Simplified Dirac Dark Matter Models and Gamma-Ray Lines
• Clustering of quasars in the First Year of the SDSS-IV eBOSS survey: Interpretation and halo occupation distribution
• Testing cosmic geometry without dynamic distortions using voids
• Detection of hot, metal-enriched outflowing gas around $z\approx$2.3 star-forming galaxies in the Keck Baryonic Structure Survey
• Implications of hydrodynamical simulations for the interpretation of direct dark matter searches
• The formation and coalescence sites of the first gravitational wave events
• A new test of $f(R)$ gravity with the cosmological standard rulers in radio quasars
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: combining correlated Gaussian posterior distributions
• Reionization on Large Scales IV: Predictions for the 21 cm signal incorporating the light cone effect
• Distinguishing between Neutrinos and time-varying Dark Energy through Cosmic Time
• Lyman-alpha opacities at z=4-6 require low mass, radiatively-suppressed galaxies to drive cosmic reionization
• Cosmology with Standard Sirens at Cosmic Noon
• The Sagittarius dwarf galaxy: Where did all the gas go?
• Tensions between direct measurements of the lens power spectrum from Planck data
• Top-philic Vector-Like Portal to Scalar Dark Matter
• Magnetogenesis around the first galaxies: the impact of different field seeding processes on galaxy formation
• Dynamics of a two scalar field cosmological model with phantom terms
• An SU(5) x A5 Golden Ratio Flavour Model
• Constraining interacting dark energy with CMB and BAO future surveys
• Modified Dust and the Small Scale Crisis in CDM
• Dark Radiation candidates after Planck
• What is parameterized $Om(z)$ diagnostics telling us in light of recent observations?
• Planck's Dusty GEMS. VII. Atomic carbon and molecular gas in dusty starburst galaxies at z=2 to 4
• Winds of change: reionization by starburst galaxies
• Weakening Gravity on Redshift-Survey Scales with Kinetic Matter Mixing
• Excluding the Light Dark Matter Window of a 331 Model Using LHC and Direct Dark Matter Detection Data
• The final SDSS-IV/SPIDERS X-ray point source spectroscopic catalogue
• Constraints and tensions in testing general relativity from Planck and CFHTLenS including intrinsic alignment systematics
• Search for supersymmetry in events with large missing transverse momentum, jets, and at least one tau lepton in 20 fb${}^{-1}$ of $\sqrt{s}$=8 TeV proton-proton collision data with the ATLAS detector
• Faint Submillimeter Galaxies identified through their optical/near-infrared colours I: spatial clustering and halo masses
• Singlet-Doublet Fermionic Dark Matter, Neutrino Mass and Collider Signatures
• Neutrino constraints: what large-scale structure and CMB data are telling us?
• Galactic structure explained with dissipative mirror dark matter
• Power Suppression at Large Scales in String Inflation
• Swampland criteria for a dark-energy dominated universe, ensuing from Gaussian process and H(z) data analysis
• Cosmological investigations of (extended) nonlinear massive gravity schemes with non-minimal coupling
• Lensed or not lensed: Determining lensing magnifications for binary neutron star mergers from a single detection
• Stellar 3-D kinematics in the Draco dwarf spheroidal galaxy
• Self-consistent semi-analytic models of the first stars
• Anisotropic cosmological solutions in massive vector theories
• The 21-cm BAO signature of enriched low-mass galaxies during cosmic reionization
• Alleviating the cosmological constant problem from particle production
• Reconstruction of broad features in the primordial spectrum and inflaton potential from Planck
• On the evidence for large-scale galactic conformity in the local Universe
• CoMaLit - II. The scaling relation between mass and Sunyaev-Zel'dovich signal for Planck selected galaxy clusters
• New constraints on ${\sigma }_8$ from a joint analysis of stacked gravitational lensing and clustering of galaxy clusters
• Dark matter, neutrino masses and high scale validity of an inert Higgs doublet model
• Weighing the Local Group in the Presence of Dark Energy
• On the local variation of the Hubble constant
• Primordial tensor modes of the early Universe
• One-loop Modified Gravity in de Sitter Universe, Quantum Corrected Inflation, and its Confrontation with the Planck Result
• Showcasing HH production: Benchmarks for the (HL-)LHC
• Primordial black holes as a novel probe of primordial gravitational waves. II: Detailed analysis
• Implications of Feebly Interacting Dark Sector on Neutron Star Properties and Constraints from GW170817
• Generalized Galilean Genesis
• Monitoring AGNs with H$\beta$ Asymmetry. III. Long-term Reverberation Mapping Results of 15 Palomar-Green Quasars
• A Hybrid Deep Learning Approach to Cosmological Constraints From Galaxy Redshift Surveys
• Flybys, orbits, splashback: subhalos and the importance of the halo boundary
• Resonant conversions of QCD axions into hidden axions and suppressed isocurvature perturbations
• On de Sitter solutions in asymptotically safe $f(R)$ theories
• Annihilating Asymmetric Dark Matter
• Generation of Neutrino mass from new physics at TeV scale and Multi-lepton Signatures at the LHC
• Black Hole Growth and Feedback in Isolated Romulus25 Dwarf Galaxies
• The Origin of r-process Enhanced Metal-Poor Halo Stars In Now-Destroyed Ultra-Faint Dwarf Galaxies
• Visible neutrino decay in the light of appearance and disappearance long baseline experiments
• Modelling and simulation of large-scale polarized dust emission over the southern Galactic cap using the GASS HI data
• Bulk viscous embedded hybrid dark energy models
• Statistics of the epoch of reionization 21-cm signal - I. Power spectrum error-covariance
• 3\%-accurate predictions for the clustering of dark matter, haloes and subhaloes, over a wide range of cosmologies and scales
• Towards Natural Inflation in String Theory
• Energy wrinkles and phase-space folds of the last major merger
• A rumble in the dark: signatures of self-interacting dark matter in Super-Massive Black Hole dynamics and galaxy density profiles
• The primordial matter power spectrum on sub-galactic scales
• Combining Universal and Odd RR Axions for Aligned Natural Inflation
• Neutrino Mixing from CP Symmetry
• How to relax the cosmological neutrino mass bound
• Testing Gravity on Cosmic Scales: A Case Study of Jordan-Brans-Dicke Theory
• The Extremely High Dark Matter Halo Concentration of the Relic Compact Elliptical Galaxy Mrk 1216
• The lopsided distribution of satellite galaxies
• Possibility of realizing weak gravity in redshift space distortion measurements
• Dark matter and U(1)' symmetry for the right-handed neutrinos
• Dark matter component decaying after recombination: Sensitivity to BAO and RSD probes
• Ruling out the power-law form of the scalar primordial spectrum
• Upper limits on DM annihilation cross sections from the first AMS-02 antiproton data
• Measurement of the expansion rate of the Universe from γ-ray attenuation
• The effect of Dark Matter and Dark Energy interactions on the peculiar velocity field and the kinetic Sunyaev-Zel'dovich effect
• One-loop corrections to neutralino-stop coannihilation revisited
• Low-l CMB Power Loss in String Inflation
• Update on Minimal Supersymmetric Hybrid Inflation in Light of PLANCK
• Extending Higgs Inflation with TeV Scale New Physics
• Dark Matter Detection in Focus Point Supersymmetry
• Age and metallicity gradients support hierarchical formation for M87
• Search for features in the spectrum of primordial perturbations using Planck and other datasets
• A new approach for detecting compressed bino/wino at the LHC
• Galaxies Probing Galaxies at High Resolution: Co-Rotating Gas Associated with a Milky Way Analog at z=0.4
• Precision modelling of the matter power spectrum in a Planck-like Universe
• The Imprint of f(R) Gravity on Non-Linear Structure Formation
• Stacking of large interferometric data sets in the image- and uv-domain -- a comparative study
• Effective equation of state for running vacuum: "mirage" quintessence and phantom dark energy
• Anisotropic cosmological reconstruction in $f(R,T)$ gravity
• Coupled dark energy: a dynamical analysis with complex scalar field
• Scale-invariance as the origin of dark radiation?
• FLRW cosmological models with quark and strange quark matters in f(R,T) gravity
• Using dark energy to suppress power at small scales
• Ultracompact minihalos as probes of inflationary cosmology
• Multipole analysis of IceCube data to search for dark matter accumulated in the Galactic halo
• Discrepancies between CFHTLenS cosmic shear & Planck: new physics or systematic effects?
• The efficiency of ionising photon production and the radiation energy balance in compact star-forming galaxies
• Color Breaking Baryogenesis
• Axion monodromy inflation with multi-natural modulations
• Cosmology in beyond-generalized Proca theories
• Model independent constraints on transition redshift
• Singlet-Doublet Dirac Dark Matter
• Cosmological Constraint Precision of the Photometric and Spectroscopic Multi-probe Surveys of China Space Station Telescope (CSST)
• A Fresh Look at keV Sterile Neutrino Dark Matter from Frozen-In Scalars
• Chemically Distinct Nuclei and Outflowing Shocked Molecular Gas in Arp 220
• Sterile neutrinos and right-handed currents in KATRIN
• Prospect for constraining holographic dark energy with gravitational wave standard sirens from the Einstein Telescope
• J2229+2725: an extremely low-metallicity dwarf compact star-forming galaxy with an exceptionally high [OIII]5007/[OII]3727 flux ratio of 53
• Characterizing hydrostatic mass bias with Mock-X
• Nature and statistical properties of quasar associated absorption systems in the XQ-100 Legacy Survey
• Eternal Universe
• CMB dipole asymmetry from a fast roll phase
• A Dark Census: Statistically Detecting the Satellite Populations of Distant Galaxies
• Cosmology Inference from Biased Tracers using the EFT-based Likelihood
• The challenge of simultaneously matching the observed diversity of chemical abundance patterns in cosmological hydrodynamical simulations
• Relativistic Interpretation of Newtonian Simulations for Cosmic Structure Formation
• Alleviating both $H_0$ and ${\sigma }_8$ tensions in Tsallis cosmology
• The diverse evolutionary pathways of post-starburst galaxies
• Probing the innermost regions of AGN jets and their magnetic fields with RadioAstron II. Observations of 3C 273 at minimum activity
• The Little Galaxies that Could (Reionize the Universe): Predicting Faint End Slopes & Escape Fractions at z > 4
• A self-consistent analytical magnetar model: The luminosity of $\gamma$-ray burst supernovae is powered by radioactivity
• AGN feedback on molecular gas reservoirs in quasars at $z\sim$2.4
• Cosmic equation of state from combined angular diameter distances: Does the tension with luminosity distances exist?
• Virialisation-induced curvature as a physical explanation for dark energy
• A New Method to Quantify Environment and Model Ram-Pressure Stripping in N-Body Simulations
• Consistent Modified Gravity Analysis of Anisotropic Galaxy Clustering Using BOSS DR11
• Host galaxies of SNe Ic-BL with and without long gamma-ray bursts
• Faint progenitors of luminous $z\sim 6$ quasars: why don't we see them?
• Cosmology with anisotropic galaxy clustering from the combination of power spectrum and bispectrum
• Reheating processes after Starobinsky inflation in old-minimal supergravity
• Effective photon mass and (dark) photon conversion in the inhomogeneous Universe
• X-ray Plateaus in Gamma-Ray Burst Afterglows and Their Application in Cosmology
• Dark matter in ghost-free bigravity theory: From a galaxy scale to the universe
• Galactic dark matter search via phenomenological astrophysics modeling
• Dark Radiation Constraints on Mixed Axion/Neutralino Dark Matter
• A Deep Search for Prompt Radio Emission from the Short GRB 150424A With The Murchison Widefield Array
• Gauge-Invariance and Infrared Divergences in the Luminosity Distance
• POLOCALC: a Novel Method to Measure the Absolute Polarization Orientation of the Cosmic Microwave Background
• The Jubilee ISW Project I: simulated ISW and weak lensing maps and initial power spectra results
• The origin of the red sequence galaxy population in the EAGLE simulation
• SUSY Implications from WIMP Annihilation into Scalars at the Galactic Centre
• Testing General Relativity with Growth rate measurement from Sloan Digital Sky Survey III Baryon Oscillations Spectroscopic Survey galaxies
• Prospects of discovering sub-solar primordial black holes using the stochastic gravitational wave background from third-generation detectors
• Higgs boson mass, neutrino masses and mixing and keV dark matter in an $U(1{)}_R-$ lepton number model
• Spectroscopy of Masses and Couplings during Inflation
• Searching for Dark Matter in the Galactic Halo with a Wide Field of View TeV Gamma-ray Observatory in the Southern Hemisphere
• An upper limit on the strength of the extragalactic magnetic field from ultra-high-energy cosmic-ray anisotropy
• The environment of the SN-less GRB 111005A at z = 0.0133
• Combined analysis of galaxy cluster number count, thermal Sunyaev-Zel'dovich power spectrum, and bispectrum
• Measuring growth index in a universe with massive neutrinos: A revisit of the general relativity test with the latest observations
• A Closer Look at Gaugino Masses in Pure Gravity Mediation Model/Minimal Split SUSY Model
• Thin accretion disk luminosity and its image around rotating black holes in perfect fluid dark matter
• Strongly first order phase transition in the singlet fermionic dark matter model after LUX
• Broadband Intensity Tomography: Spectral Tagging of the Cosmic UV Background
• Correlations between Triaxial Shapes and Formation History of Dark Matter Haloes
• Fermion and scalar phenomenology of a 2-Higgs doublet model with $S_3$
• Primordial black holes as a novel probe of primordial gravitational waves
• Creating a galaxy lacking dark matter in a dark matter dominated universe
• Higgs Chaotic Inflation and the Primordial B-mode Polarization Discovered by BICEP2
• Electroweak baryogenesis via bottom transport
• Anisotropic Inflation with the non-Vacuum Initial State
• The velocity anisotropy of the Milky Way satellite system
• Subhalo statistics of galactic halos: beyond the resolution limit
• Kinetic decoupling of WIMPs: analytic expressions
• Scalar Singlet Dark Matter and Gamma Lines
• Neutrino Masses and Scalar Singlet Dark Matter
• Perturbative Renormalization of Neutron-Antineutron Operators
• The challenge for single field inflation with BICEP2 result
• Hybrid Textures of Majorana Neutrino Mass Matrix and Current Experimental Tests
• Inflation in the closed FLRW model and the CMB
• Observational constraints on cosmological models with Chaplygin gas and quadratic equation of state
• 3.5 keV X-ray Line Signal from Decay of Right-Handed Neutrino due to Transition Magnetic Moment
• Constraints on dark radiation from cosmological probes
• Spectral distortions from the dissipation of tensor perturbations
• Dissecting the Gamma-Ray Background in Search of Dark Matter
• The first Super Massive Black Holes: indications from models for future observations
• Implications of an Improved Neutron-Antineutron Oscillation Search for Baryogenesis: A Minimal Effective Theory Analysis
• Bounce Loop Quantum Cosmology Corrected Gauss-Bonnet Gravity
• Growth of matter perturbations in clustered holographic dark energy cosmologies
• Baryon effects on void statistics in the EAGLE simulation
• The BaLROG project - I. Quantifying the influence of bars on the kinematics of nearby galaxies
• A predictive $331$ model with $A_4$ flavour symmetry
• SUSY-QCD corrections to stop annihilation into electroweak final states including Coulomb enhancement effects
• Forecasting the Interaction in Dark Matter-Dark Energy Models with Standard Sirens From the Einstein Telescope
• Does small scale structure significantly affect cosmological dynamics?
• Perspective of monochromatic gamma-ray line detection with the High Energy cosmic-Radiation Detection (HERD) facility onboard China's Space Station
• Friction in Gravitational Waves: a test for early-time modified gravity
• Evidence for Early Filamentary Accretion from the Andromeda Galaxy's Thin Plane of Satellites
• Measuring the 2D Baryon Acoustic Oscillation signal of galaxies in WiggleZ: Cosmological constraints
• A Trio of GRB-SNe: GRB 120729A, GRB 130215A / SN 2013ez and GRB 130831A / SN 2013fu
• Marked clustering statistics in $f(R)$ gravity cosmologies
• A universal relation between the properties of supermassive black holes, galaxies, and dark matter halos
• Chromo-Natural Inflation in the Axiverse
• Hydrostatic and Caustic Mass Profiles of Galaxy Clusters
• From inflation to recent cosmic acceleration: The fermionic Elko field driving the evolution of the universe
• Probing the jet base of the blazar PKS1830-211 from the chromatic variability of its lensed images. Serendipitous ALMA observations of a strong gamma-ray flare
• Search for dark matter and unparticles produced in association with a Z boson in proton-proton collisions at sqrt(s) = 8 TeV
• Probing cosmic opacity at high redshifts with gamma-ray bursts
• Neutrino Mass Priors for Cosmology from Random Matrices
• Foreground removal for Square Kilometre Array observations of the Epoch of Reionization with the Correlated Component Analysis
• The effect of massive neutrinos on the Sunyaev-Zeldovich and X-ray observables of galaxy clusters
• Planck's dusty GEMS. IV. Star formation and feedback in a maximum starburst at z=3 seen at 60-pc resolution
• Updated Results on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• Elementary Goldstone Higgs Boson and Dark Matter
• Eppur si muove: Positional and kinematic correlations of satellite pairs in the low Z universe
• X-rays from the redshift 7.1 quasar ULAS J1120+0641
• Simulating Momentum Exchange in the Dark Sector
• Rhapsody-G simulations: galaxy clusters as baryonic closed boxes and the covariance between hot gas and galaxies
• LUX likelihood and limits on spin-independent and spin-dependent WIMP couplings with LUXCalc
• HaloSat -- A CubeSat to Study the Hot Galactic Halo
• Near Maximal Atmospheric Neutrino Mixing in Neutrino Mass Models with Two Texture Zeros
• Search for Gamma-ray Emission from Dark Matter Annihilation in the Small Magellanic Cloud with the Fermi Large Area Telescope
• Stellar and AGN feedback in isolated early-type galaxies: the role in regulating star formation and ISM properties
• A sensitive APEX and ALMA CO(1-0), CO(2-1), CO(3-2), and [CI](1-0) spectral survey of 40 local (U)LIRGs
• Exploring MSSM for Charge and Color Breaking and Other Constraints in the Context of Higgs@125 GeV
• Search for a light charged Higgs boson in the H${}^{\pm }$ $\to$ cs channel in proton-proton collisions at $\sqrt{s}=$ 13 TeV
• Planck intermediate results. XVI. Profile likelihoods for cosmological parameters
• How Late can the Dark Matter form in our universe?
• Transition Redshift: New constraints from parametric and nonparametric methods
• Intensity Mapping Cross-Correlations: Connecting the Largest Scales to Galaxy Evolution
• A normal supermassive black hole in NGC 1277
• Reconstruction of the dark matter-vacuum energy interaction
• Constraining the Asymptotically Safe Cosmology: cosmic acceleration without dark energy
• Evolution of LMC/M33-mass dwarf galaxies in the EAGLE simulation
• Comprehensive Assessment of the Too-Big-to-Fail Problem
• Quintessence with Yukawa Interaction
• Indirect Detection of Dark Matter with gamma rays
• Early chemo-dynamical evolution of dwarf galaxies deduced from enrichment of r-process elements
• Natural MSSM after the LHC 8 TeV run
• Voronoi volume function: A new probe of cosmology and galaxy evolution
• Cosmology in scalar-vector-tensor theories
• CMB distance priors revisited: effects of dark energy dynamics, spatial curvature, primordial power spectrum, and neutrino parameters
• Majorana CP-violating phases in neutrino-antineutrino oscillations and other lepton-number-violating processes
• Kinematics of the intermediate mass black hole candidate HLX-1
• Deadly dark matter cusps vs faint and extended star clusters: Eridanus II and Andromeda XXV
• CFHTLenS and RCSLenS Cross-Correlation with Planck Lensing Detected in Fourier and Configuration Space
• Generalised teleparallel quintom dark energy non-minimally coupled with the scalar torsion and a boundary term
• Redshifted 21-cm Bispectrum I: Impact of the Redshift Space Distortions on the Signal from the Epoch of Reionization
• Evolution of the fine-structure constant in runaway dilaton models
• NIHAO XVIII: Origin of the MOND phenomenology of galactic rotation curves in a LCDM universe
• Modelling the luminosities and sizes of radio galaxies: radio luminosity function at z = 6
• The impact of feedback and the hot halo on the rates of gas accretion onto galaxies
• NIHAO XVI: The properties and evolution of kinematically selected discs, bulges and stellar haloes
• Holographic thermalization and gravitational collapse in the spacetime dominated by quintessence dark energy
• The offsets between galaxies and their dark matter in Lambda-CDM
• Saving Natural Inflation
• The BINGO telescope: a new instrument exploring the new 21-cm cosmology window
• NIHAO XXII: Introducing black hole formation, accretion and feedback into the NIHAO simulation suite
• Interacting viscous dark fluids
• The impact of inhomogeneous subgrid clumping on cosmic reionization
• Structural and Dynamical Properties of Galaxies in a Hierarchical Universe: Sizes and Specific Angular Momenta
• Reproducing the Universe: a comparison between the EAGLE simulations and the nearby DustPedia galaxy sample
• Sommerfeld enhancements with vector, scalar and pseudoscalar force-carriers
• The build-up of pseudobulges in a hierarchical universe
• How smooth are particle trajectories in a $\Lambda$CDM Universe?
• The semi-constrained NMSSM in light of muon g-2, LHC, and dark matter constraints
• The Magellanic Stream: break up and accretion onto the hot Galactic corona
• Stellar splashback: the edge of the intracluster light
• Dynamical mass inference of galaxy clusters with neural flows
• GRB 140606B / iPTF14bfu: Detection of shock-breakout emission from a cosmological gamma-ray burst?
• Constraints on the distance moduli, helium and metal abundances, and ages of globular clusters from their RR Lyrae and non-variable horizontal-branch stars. II. Multiple stellar populations in 47Tuc, M3, and M13
• Successful $N_2$ leptogenesis with flavour coupling effects in realistic unified models
• Multiple Point Principle of the Standard Model with Scalar Singlet Dark Matter and Right Handed Neutrinos
• Galaxy formation on the largest scales: The impact of astrophysics on the BAO peak
• Exploring scalar field dynamics with Gaussian processes
• Reconstructing inflationary potential from BICEP2 and running of tensor modes
• Shedding Light on Dark Matter at Colliders
• Cosmology with non-minimal derivative couplings: perturbation analysis and observational constraints
• The weak neutral Fe fluorescence line and long-term X-ray evolution of the Compton-thick AGN in NGC 7674
• Testing Fractional Action Cosmology
• Do model emission line galaxies live in filaments at z~1?
• Energy-momentum correlations for Abelian Higgs cosmic strings
• Constraining the dark energy models using Baryon Acoustic Oscillations: An approach independent of $H_0\cdot r_d$
• Dark Matter vs. Neutrinos: The effect of astrophysical uncertainties and timing information on the neutrino floor
• Toward a tomographic analysis of the cross-correlation between Planck CMB lensing and H-ATLAS galaxies
• Dependence of GAMA galaxy halo masses on the cosmic web environment from 100 square degrees of KiDS weak lensing data
• Looking for Population III stars with He II line intensity mapping
• The galaxy cluster outskirts probed by Chandra
• Dark Energy from graviton-mediated interactions in the QCD vacuum
• On the Quantum-To-Classical Transition for Ekpyrotic Perturbations
• Formation of Massive Population III Galaxies through Photoionization Feedback: A Possible Explanation for CR7
• The diverse galaxy counts in the environment of high-redshift massive black holes in Horizon-AGN
• Primordial $\alpha +d\to {}^6\mathrm{Li}+\gamma$ reaction and second Lithium puzzle
• Study of Electroweak Vacuum Stability from Extended Higgs Portal of Dark Matter and Neutrinos
• Black hole growth and AGN feedback under clumpy accretion
• Radiative neutrino mass generation linked to neutrino mixing and $0\nu \beta \beta$-decay predictions
• The Incomplete Conditional Stellar Mass Function: Unveiling the Stellar Mass Functions of Galaxies at 0.1 < Z < 0.8 from BOSS Observations
• Observational constraints on key-parameters of cosmic reionisation history
• Limits on the Neutrino Velocity, Lorentz Invariance, and the Weak Equivalence Principle with TeV Neutrinos from Gamma-Ray Bursts
• An alternate approach to measure specific star formation rates at 2<z<7
• Pionic Dark Matter
• Improved CMB anisotropy constraints on primordial magnetic fields from the post-recombination ionization history
• Indirect Search for Dark Matter from the Galactic Center and Halo with the Super-Kamiokande Detector
• Detecting the cosmological neutrino background in the CMB
• Constraining topological defects with temperature and polarization anisotropies
• Accounting for the time evolution of the equation of state parameter during reheating
• CP Symmetry and Lepton Mixing from a Scan of Finite Discrete Groups
• Nonlinear particle acceleration and thermal particles in GRB afterglows
• ALMA Imprint of Intergalactic Dark Structures in the Gravitational Lens SDP.81
• Cosmological Consequences of Initial State Entanglement
• Electroweakly-Interacting Dirac Dark Matter
• The $\text{Fermi}$-LAT gamma-ray excess at the Galactic Center in the singlet-doublet fermion dark matter model
• Gravitational wave consistency relations for multifield inflation
• Dark-Photon searches via Higgs-boson production at the LHC
• Cosmological dynamics of scalar fields with kinetic corrections: Beyond the exponential potential
• GRB/GW association: Long-short GRB candidates, time-lag, measuring gravitational wave velocity and testing Einstein's equivalence principle
• Testing the distance duality relation using type Ia supernovae and ultracompact radio sources
• Clustering of infrared-bright dust-obscured galaxies revealed by the Hyper Suprime-Cam and WISE
• JWST high-z galaxy constraints on warm and cold dark matter models
• Improved constraint on the primordial gravitational-wave density using recent cosmological data and its impact on cosmic string models
• No-Scale Inflation
• Higgs portals to pulsar collapse
• Holographic Dark Energy Models and Higher Order Generalizations in Dynamical Chern-Simons Modified Gravity
• Graviton Loop Corrections to Vacuum Polarization in de Sitter in a General Covariant Gauge
• Testing Inflation and Curvaton Scenarios with CMB Distortions
• Searches for massive neutrinos with mechanical quantum sensors
• Revisiting Metastable Dark Energy and Tensions in the Estimation of Cosmological Parameters
• Present and projected sensitivities of Dark Matter direct detection experiments to effective WIMP-nucleus couplings
• Testing logarithmic corrections on $R^2$-exponential gravity by observational data
• The Diphoton and Diboson Excesses in a Left-Right Symmetric Theory of Dark Matter
• Galaxy gas flows inferred from a detailed, spatially resolved metal budget
• $A_4$ and CP symmetry and a model with maximal CP violation
• DAMA/LIBRA-phase2 in WIMP effective models
• The Mass-Concentration Relation and the Stellar-to-Halo Mass Ratio in the CFHT Stripe 82 Survey
• The history of the dark and luminous side of Milky Way-like progenitors
• The optical identifcation of events with poorly defined locations: The case of the Fermi GBM GRB140801A
• Extreme submillimetre starburst galaxies
• Ring Galaxies in the EAGLE Hydrodynamical Simulations
• Inflation and Alternatives with Blue Tensor Spectra
• Effective Field Theory of Dark Matter: a Global Analysis
• The Radial Acceleration Relation in Disk Galaxies in the MassiveBlack-II Simulation
• The two-mode puzzle: Confronting self-interacting neutrinos with the full shape of the galaxy power spectrum
• Impact of sterile neutrinos on the early time flux from a galactic supernova
• Power-law cosmology, SN Ia, and BAO
• Effects of baryons on weak lensing peak statistics
• Constraints on mixed dark matter from anomalous strong lens systems
• Anisotropic inflation in Gauss-Bonnet gravity
• Correlating correlation functions of primordial perturbations
• Scalar triplet flavored leptogenesis: a systematic approach
• A multi-wavelength de-blended Herschel view of the statistical properties of dusty star-forming galaxies across cosmic time
• Axions and Axion-Like Particles
• Inflationary power asymmetry from primordial domain walls
• The use of low temperature detectors for direct measurements of the mass of the electron neutrino
• Large 21 cm signals from AGN-dominated reionization
• A flavor dependent gauge symmetry, Predictive radiative seesaw and LHCb anomalies
• Quiescent low-mass galaxies observed by JWST in the Epoch of Reionization
• New Limits on Coupled Dark Energy from Planck
• Neutron Stars in Screened Modified Gravity: Chameleon vs Dilaton
• NMSSM explanations of the Galactic center gamma ray excess and promising LHC searches
• Structural and photometric properties of barred galaxies from the Auriga cosmological simulations
• Lyman alpha and Lyman continuum emission of MgII-selected star-forming galaxies
• The simplest extension of Starobinsky inflation
• Dark energy with a gradient coupling to the dark matter fluid: cosmological dynamics and structure formation
• Search for Low-Mass Dark Matter with CsI(Tl) Crystal Detectors
• Constraints on the neutrino parameters by future cosmological 21cm line and precise CMB polarization observations
• The Pursuit of Dark Matter at Colliders - An Overview
• Oscillatory inflation in non-minimal derivative coupling model
• Hydrostatic mass estimates of massive galaxy clusters: a study with varying hydrodynamics flavours and non-thermal pressure support
• Compensated isocurvature perturbations in the curvaton model
• Rise of the First Super-Massive Stars
• 3D hydrodynamic simulations for the formation of the Local Group satellite planes
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• On the proper kinetic quadrupole CMB removal and the quadrupole anomalies
• Neutrino Mixing with Non-Zero ${\theta }_{13}$ and CP Violation in the 3-3-1 Model Based on $S_4$ Flavor Symmetry
• A weak gravitational lensing recalibration of the scaling relations linking the gas properties of dark halos to their mass
• Properties of the ionized CGM and IGM: a comparison of galaxy formation models via the Sunyaev-Zel'dovich effect
• Tracing galaxy populations through cosmic time: A critical test of methods for connecting the same galaxies between different redshifts at $z<3$
• The star-formation law at GMC scales in M33, the Triangulum Galaxy
• A Generalized Interacting Tsallis Holographic Dark Energy Model and its thermodynamic implications
• A long optical plateau in the afterglow of the Extended Emission short GRB 150424A: Evidence for energy injection by a magnetar?
• Deconstructing Thermal Sunyaev-Zel'dovich - Gravitational Lensing Cross-Correlations: Implications for the Intracluster Medium
• Towards a general parametrization of the warm dark matter halo mass function
• Exploring the properties of milliarcsecond radio sources
• Probing decaying heavy dark matter with the 4-year IceCube HESE data
• The radial acceleration relation in galaxy clusters
• Calibrated Ultra Fast Image Simulations for the Dark Energy Survey
• Deep Learning Based Detection of Cosmological Diffuse Radio Sources
• Leptogenesis in SO(10)
• Brans-Dicke theory and the emergence of ΛCDM model
• Non-Minimal Two-Loop Inflation
• NIHAO-XXIII: Dark Matter density shaped by Black Hole feedback
• How did the Virgo cluster form?
• Three-loop Neutrino Mass Model with Doubly Charged Particles from Iso-Doublets
• Alternative Schemes of Predicting Lepton Mixing Parameters from Discrete Flavor and CP Symmetry
• Quantifying Concordance in Cosmology
• VERITAS detection of $\gamma$-ray flaring activity from the BL Lac object 1ES 1727+502 during bright moonlight observations
• Constraints on a $\varphi$CDM model from strong gravitational lensing and updated Hubble parameter measurements
• Search for $\gamma$-ray emission from dark matter particle interactions from Andromeda and Triangulum Galaxies with the Fermi Large Area Telescope
• Globular clusters as tracers of the dark matter halo: insights from the E-MOSAICS simulations
• Ultra-bright CO and [CI] emission in a lensed z=2.04 submillimeter galaxy with extreme molecular gas properties
• Observations of metals in the $z\approx 3.5$ intergalactic medium and comparison to the EAGLE simulations
• Complementarity of the future $e^{+}{e}^{-}$ colliders and gravitational waves in the probe of complex singlet extension to the Standard Model
• Isospin-violating dark matter from a double portal
• Fast Gravitational Wave Radiometry using Data Folding
• Observational signatures of the theories beyond Horndeski
• Extension of warm inflation to noncanonical scalar fields
• Lyman-α Forest and Cosmic Weak Lensing in a Warm Dark Matter Universe
• Boosted Dark Matter and its implications for the features in IceCube HESE data
• Including birefringence into time evolution of CMB: current and future constraints
• CosmicNet II: Emulating extended cosmologies with efficient and accurate neural networks
• Post-Newtonian parameters and cosmological constant of screened modified gravity
• Long term variability and correlation study of the blazar 3C 454.3 in radio, NIR and optical wavebands
• Fermi-bounce Cosmology and scale invariant power-spectrum
• Forming Super-Massive Black Hole Seeds under the Influence of a Nearby Anisotropic Multi-Frequency Source
• A comparative study of satellite galaxies in Milky Way-like galaxies from HSC, DECaLS and SDSS
• Brane with variable tension as a possible solution to the problem of the late cosmic acceleration
• Extreme Supernova Models for the Superluminous Transient ASASSN-15lh
• Statistics of galaxy mergers: bridging the gap between theory and observation
• 10 GeV neutralino dark matter and light stau in the MSSM
• The supermassive black hole coincident with the luminous transient ASASSN-15lh
• CLASH-VLT: Constraints on the Dark Matter Equation of State from Accurate Measurements of Galaxy Cluster Mass Profiles
• BICEP / Keck XVII: Line of Sight Distortion Analysis: Estimates of Gravitational Lensing, Anisotropic Cosmic Birefringence, Patchy Reionization, and Systematic Errors
• Beyond Minimal Lepton Flavored Dark Matter
• Gravitational Redshift of Galaxies in Clusters from the Sloan Digital Sky Survey and the Baryon Oscillation Spectroscopic Survey
• Predictions for Ultra-Deep Radio Counts of Star-Forming Galaxies
• The New Numerical Galaxy Catalog (${\nu }^2$GC): An Updated Semi-analytic Model of Galaxy and AGN with Large Cosmological N-body Simulation
• Constraints on Gauge Field Production during Inflation
• Internal Delensing of Cosmic Microwave Background Acoustic Peaks
• Collimation of the relativistic jet in the quasar 3C 273
• Measuring the distance-redshift relation with the baryon acoustic oscillations of galaxy clusters
• Discovery of a z = 7.452 High Equivalent Width Lyman-α Emitter from the Hubble Space Telescope Faint Infrared Grism Survey
• Constraining Multiplicative Bias in CFHTLenS Weak Lensing Shear Data
• Warm Dark Matter in B-L Inverse Seesaw
• The interpretation for Galactic Center Excess and Electroweak Phase Transition in the NMSSM
• Modeling the JWST high-redshift galaxies with a general formation scenario and the consistency with the $\Lambda$CDM model
• Mapping metals at high redshift with far-infrared lines
• Crucial Factors for Lyα Transmission in the Reionizing Intergalactic Medium: Infall Motion, HII Bubble Size, and Self-shielded Systems
• Cosmology With Low-Redshift Observations: No Signal For New Physics
• Herschel reveals a molecular outflow in a z = 2.3 ULIRG
• Cosmology of F(R) nonlinear massive gravity
• SN 2016jhj at redshift 0.34: extending the Type II supernova Hubble diagram using the standard candle method
• The impact of early massive mergers on the chemical evolution of Milky Way-like galaxies: insights from NIHAO-UHD simulations
• Redshifted 21-cm bispectrum II: Impact of the spin temperature fluctuations and redshift space distortions on the signal from the Cosmic Dawn
• Black hole accretion disc impacts
• Dynamical analysis for a vector-like dark energy
• Bias-Hardened CMB Lensing with Polarization
• Primordial Statistical Anisotropies: The Effective Field Theory Approach
• The effects of AGN feedback on the structural and dynamical properties of Milky Way-mass galaxies in cosmological simulations
• Grand Unification, Axion, and Inflation in Intermediate Scale Supersymmetry
• Early Science with the Large Millimeter Telescope: Observations of dust continuum and CO emission lines of cluster-lensed submillimetre galaxies at z=2.0-4.7
• Search for gamma-ray emission from $p$-wave dark matter annihilation in the Galactic Center
• J-PLUS: On the identification of new cluster members in the double galaxy cluster A2589 & A2593 using PDFs
• Accuracy of the growth index in the presence of dark energy perturbations
• Hyperbolic Inflation in the Light of Planck 2015 data
• Qualitative analysis of Kantowski-Sachs metric in a generic class of $f(R)$ models
• A comparison of the Higgs sectors of the CMSSM and NMSSM for a 126 GeV Higgs boson
• CMB Hemispherical Asymmetry: Long Mode Modulation and non-Gaussianity
• A systematic halo-independent analysis of direct detection data within the framework of Inelastic Dark Matter
• Magnetic dark matter for the X-ray line at 3.55 keV
• The Fate of Gas rich Satellites in Clusters
• Constraining $f(Q,L_m)$ gravity with bulk viscosity
• First results on the cluster galaxy population from the Subaru Hyper Suprime-Cam survey. II. Faint end color-magnitude diagrams and radial profiles of red and blue galaxies at $0.1<z<1.1$
• Voids in cosmological simulations over cosmic time
• Cosmic Acceleration From Matter-Curvature Coupling
• The rise and fall of a challenger: the Bullet Cluster in $\Lambda$ Cold Dark Matter simulations
• The redshift distribution of submillimetre galaxies at different wavelengths
• Confronting Galactic and Extragalactic $\gamma$-ray observed by Fermi-LAT with Annihilating Dark Matter in Inert Higgs Doublet Model
• The Shape and Size distribution of HII Regions near the percolation transition
• Big Bang Nucleosynthesis constraints on $f(T,\mathcal{T})$ gravity
• Neutrinos secretly converting to lighter particles to please both KATRIN and the cosmos
• Small Field Coleman-Weinberg Inflation driven by Fermion Condensate
• Probing a Scalar Singlet-Catalyzed Electroweak Phase Transition with Resonant Di-Higgs Production in the $4b$ Channel
• Comparing Planck and WMAP: Maps, Spectra, and Parameters
• An accurate perturbative approach to redshift space clustering of biased tracers in modified gravity
• Evolution of CMB spectral distortion anisotropies and tests of primordial non-Gaussianity
• The impact of environment and mergers on the HI content of galaxies in hydrodynamic simulations
• The TT, TB, EB and BB correlations in anisotropic inflation
• Strong Far-IR Cooling Lines, Peculiar CO Kinematics and Possible Star Formation Suppression in Hickson Compact Group 57
• Irruption of massive particle species during inflation
• Holographic Dark Energy from Fluid/Gravity Duality Constraint by Cosmological Observations
• Gravitational imaging through a triple source plane lens: revisiting the $\Lambda$CDM-defying dark subhalo in SDSSJ0946+1006
• Complementarity of Dark Matter Searches at Resonance
• Explaining the DAMPE data with scalar dark matter and gauged $U(1{)}_{L_e-L_{\mu }}$ interaction
• Metals in the circumgalactic medium are out of ionization equilibrium due to fluctuating active galactic nuclei
• The Conditional Colour-Magnitude Distribution: I. A Comprehensive Model of the Colour-Magnitude-Halo Mass Distribution of Present-Day Galaxies
• A Family of WISPy Dark Matter Candidates
• Testing the electroweak phase transition in scalar extension models at lepton colliders
• Constraints on the temperature of the intergalactic medium at z=8.4 with 21-cm observations
• Holographic Dark Energy with Cosmological Constant
• Potential for Precision Measurement of Low-Energy Antiprotons with GAPS for Dark Matter and Primordial Black Hole Physics
• Testing Predictions of the Quantum Landscape Multiverse 2: The Exponential Inflationary Potential
• CMB $\mu$ distortion from primordial gravitational waves
• LHC search for di-Higgs decays of stoponium and other scalars in events with two photons and two bottom jets
• Detailed study of geodesics in the Kerr-Newman-(A)dS spactime and the rotating charged black hole spacetime in $f(R)$ gravity
• Predicting LyC emission of galaxies using their physical and Ly$\alpha$ emission properties
• Limits to Rest-Frame Ultraviolet Emission From Far-Infrared-Luminous z~6 Quasar Hosts
• Constraining Absolute Neutrino Masses via Detection of Galactic Supernova Neutrinos at JUNO
• Constraints on Lorentz Invariance Violation with gamma-ray bursts via a Markov Chain Monte Carlo approach
• Inert scalars and vacuum metastability around the electroweak scale
• Mock Quasar-Lyman-α Forest Data-sets for the SDSS-III Baryon Oscillation Spectroscopic Survey
• The Fast Radio Burst Dispersion Measure Distribution
• Search for dark matter and supersymmetry with a compressed mass spectrum in the vector boson fusion topology in proton-proton collisions at sqrt(s) = 8 TeV
• Inflation and leptogenesis in the 3-3-1-1 model
• Two-point Correlation Function of WMAP 9 year data
• An orbital perspective on the starvation, stripping, and quenching of satellite galaxies in the EAGLE simulations
• Beyond delta: Tailoring marked statistics to reveal modified gravity
• Towards Accurate Modelling of Galaxy Clustering on Small Scales: Testing the Standard $\Lambda \mathrm{CDM}$ + Halo Model
• Neutrino Masses and Mass Hierarchy: Evidence for the Normal Hierarchy
• Relieving tensions related to the lensing of CMB temperature power spectra
• Indirect and direct detection prospect for TeV dark matter in the MSSM-9
• Non-Standard Higgs Decays in U(1) Extensions of the MSSM
• EDGE: What shapes the relationship between HI and stellar observables in faint dwarf galaxies?
• An ever-present $Gaia$ snail shell triggered by a dark matter wake
• Can Cosmological Simulations Reproduce the Spectroscopically Confirmed Galaxies Seen at $z\ge 10$?
• Robustness of cosmic neutrino background detection in the cosmic microwave background
• Observational constraints on varying neutrino-mass cosmology
• Tachyon Inflation in Teleparallel Gravity
• Gravitational Lensing of Schwarzschild and Charged Black Holes Immersed in Perfect Fluid Dark Matter Halo
• Exploring compact binary merger host galaxies and environments with $\mathrm{zELDA}$
• Bayesian semi-blind component separation for foreground removal in interferometric 21-cm observations
• 21 cm intensity mapping with the Five hundred metre Aperture Spherical Telescope
• On the Topology of the Inflaton Field in Minimal Supergravity Models
• Simulating the LOcal Web (SLOW): I. Anomalies in the local density field
• Muon g-2 and Dark Matter suggest Non-Universal Gaugino Masses: $\mathbf{SU}(5)\times {\mathbf{A}}_4$ case study at the LHC
• Correction to Lagrangian for Bouncing Cosmologies in $f(Q)$ Gravity
• Precision CMB constraints on eV-scale bosons coupled to neutrinos
• Constraints on Cosmological Parameters from the Angular Power Spectrum of a Combined 2500 deg${}^2$ SPT-SZ and Planck Gravitational Lensing Map
• The SIBELIUS Project: E Pluribus Unum
• SEAGLE - I: A pipeline for simulating and modeling strong lenses from cosmological hydrodynamic simulations
• Revealing the physical properties of gas accreting to haloes in the EAGLE simulations
• Searching for primordial localized features with CMB and LSS spectra
• Constraining the mass of the Local Group
• Measuring the reionization optical depth without large-scale CMB polarization
• Semi-analytic galaxy formation in f(R)-gravity cosmologies
• Primordial Magnetic Helicity Constraints from WMAP Nine-Year Data
• Cosmic absorption of ultra high energy particles
• The splashback radius of halos from particle dynamics: III. Halo catalogs, merger trees, and host-subhalo relations
• Evidence for an environment-dependent shift in the baryon acoustic oscillation peak
• CMB power spectrum of Nambu-Goto cosmic strings
• Cosmological Constraint on the Light Gravitino Mass from CMB Lensing and Cosmic Shear
• Searching for scalar gravitational interactions in current and future cosmological data
• Analysis of the theoretical bias in dark matter direct detection
• Extracting cosmological information from the angular power spectrum of the 2MASS Photometric Redshift catalogue
• The COSINE-100 Liquid Scintillator Veto System
• Cosmological Implications of Light Sterile Neutrinos produced after the QCD Phase Transition
• Diffusion of cosmic rays at EeV energies in inhomogeneous extragalactic magnetic fields
• 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
• Cosmology with Superluminous Supernovae
• The role of CP violating scatterings in baryogenesis - case study of the neutron portal
• Figuring Out Gas & Galaxies in Enzo (FOGGIE). III. The Mocky Way: Investigating Biases in Observing the Milky Way's Circumgalactic Medium
• Spherically symmetric Einstein-aether perfect fluid models
• Observational analysis of late-time acceleration in $f(Q,L_m)$ gravity
• Exploring degeneracies in modified gravity with weak lensing
• Impact of anisotropic stress of free-streaming particles on gravitational waves induced by cosmological density perturbations
• Stellar and dark matter density in the Local Universe
• The stellar halo of isolated central galaxies in the Hyper Suprime-Cam imaging survey
• Strong Optimized Conservative Fermi-LAT Constraints on Dark Matter Models from the Inclusive Photon Spectrum
• Fermionic dark matter and neutrino masses in a $\mathcal{B}-\mathcal{L}$ model
• Testing Predictions of the Quantum Landscape Multiverse 1: The Starobinsky Inflationary Potential
• Hints of dark photon dark matter from observations and hydrodynamical simulations of the low-redshift Lyman-$\alpha$ forest
• Dark Energy Cosmological Models with General forms of Scale Factor
• Using the topology of large-scale structure in the WiggleZ Dark Energy Survey as a cosmological standard ruler
• Planck residuals anomaly as a fingerprint of alternative scenarios to inflation
• Information Gains from Cosmological Probes
• Dynamical stability of K-essence field interacting non-minimally with a perfect fluid
• A Compton thick AGN in the barred spiral NGC 4785
• Massive black hole and Population III galaxy formation in over-massive dark matter halos with violent merger histories
• The Signatures of Self-Interacting Dark Matter and Subhalo Disruption on Cluster Substructure
• Dissecting the thermal Sunyaev-Zeldovich-gravitational lensing cross-correlation with hydrodynamical simulations
• Anisotropy test of the axion-like particle Universe opacity effect: a case for the Cherenkov Telescope Array
• Neutrino Oscillation Probabilities in Matter with Direct and Indirect Unitarity Violation in the Lepton Mixing Matrix
• Timescape cosmology with radiation fluid
• Rotating and non-linear magnetic-charged black hole surrounded by quintessence
• Gamma rays from the Galactic Centre region: a review
• Revealing the z~2.5 Cosmic Web With 3D Lyman-Alpha Forest Tomography: A Deformation Tensor Approach
• WARPFIELD Population Synthesis: The physics of (extra-)Galactic star formation and feedback driven cloud structure and emission from sub-to-kpc scales
• LSP Squark Decays at the LHC and the Neutrino Mass Hierarchy
• Small-scale galaxy clustering in the EAGLE simulation
• Galaxy fields of LISA massive black hole mergers in a simulated Universe
• Inflation, String Theory and Cosmology
• The Mass Function of Unprocessed Dark Matter Halos and Merger Tree Branching Rates
• An $A_4$ realization of inverse seesaw: neutrino masses, ${\theta }_{13}$ and leptonic non-unitarity
• Metastable dark energy
• Early structure formation from primordial density fluctuations with a blue-tilted power spectrum
• Comparing the Galactic Bulge and Galactic Disk Millisecond Pulsars
• The best fit for the observed galaxy Counts-in-Cell distribution function
• Tomographic Intensity Mapping versus Galaxy Surveys: Observing the Universe in H-alpha emission with new generation instruments
• Strongly Interacting Light Dark Matter
• Cosmology in General Massive Gravity Theories
• A low pre-infall mass for the Carina dwarf galaxy from disequilibrium modelling
• Unified Treatment of the Luminosity Distance in Cosmology
• Modified Brans-Dicke Theory in Arbitrary Dimensions
• Hunting electroweakinos at future hadron colliders and direct detection experiments
• CMB Constraints On The Thermal WIMP Mass And Annihilation Cross Section
• Voids in Lyα Forest Tomographic Maps
• Sub-Planckian Two-Field Inflation Consistent with the Lyth Bound
• Dark Radiation and Inflationary Freedom after Planck 2015
• Mapping the Integrated Sachs-Wolfe Effect
• Constraining Anisotropic Lorentz Violation via the Spectral-Lag Transition of GRB 160625B
• Geodesic completeness and homogeneity condition for cosmic inflation
• What is the Maximum Mass of a Population III Galaxy?
• Can modified gravity models reconcile the tension between CMB anisotropy and lensing maps in Planck-like observations?
• Redshift-space distortions in massive neutrino and evolving dark energy cosmologies
• Fast and easy super-sample covariance of large scale structure observables
• Constraining spatial curvature with large-scale structure
• Scalar field and time varying Cosmological constant in $f(R,T)$ gravity for Bianchi type-I Universe
• Does Planck really rule out monomial inflation?
• Warm intermediate inflation in the Randall-Sundrum II model in the light of Planck 2015 and BICEP2 results: A general dissipative coefficient
• What $\xi$? Cosmological constraints on the non-minimal coupling constant
• Cosmic backgrounds due to the formation of the first generation of supermassive black holes
• Testing the gas mass density profile of galaxy clusters with distance duality relation
• Post-Newtonian Approximation of Teleparallel Gravity Coupled with a Scalar Field
• The VIMOS Ultra Deep Survey. Luminosity and stellar mass dependence of galaxy clustering at z~3
• Inflation Model Selection meets Dark Radiation
• Parameters of cosmological models and recent astronomical observations
• SO(10)-inspired solution to the problem of the initial conditions in leptogenesis
• Bridging Star-Forming Galaxy and AGN Ultraviolet Luminosity Functions at $z=4$ with the SHELA Wide-Field Survey
• A Bound Violation on the Galaxy Group Scale: The Turn-Around Radius of NGC 5353/4
• Comparison of weak lensing by NFW and Einasto halos and systematic errors
• Rapidly Evolving Transients from the Hyper Suprime-Cam SSP Transient Survey
• The quasi-linear nearby Universe
• Nebular line emission from z > 7 galaxies in cosmological simulations: rest-frame UV to Optical lines
• Confronting the Galactic Center Gamma Ray Excess With a Light Scalar Dark Matter
• Weak lensing induced by second-order vector mode
• NuSTAR observations of the powerful radio-galaxy Cygnus A
• The Old, Super-Metal-Rich Open Cluster, NGC 6791 - Elemental Abundances in Turn-off Stars from Keck/HIRES Spectra
• 750 GeV Di-photon excess at CERN LHC from a dark sector assisted scalar decay
• What's in a name? Quantifying the interplay between the Definition, Orientation, and Shape of Ultra-diffuse Galaxies Using the Romulus Simulations
• Cosmic CARNage I: on the calibration of galaxy formation models
• Is there evidence for additional neutrino species from cosmology?
• The impact of galactic feedback on the shapes of dark-matter haloes
• Weak Lensing Analysis of SPT selected Galaxy Clusters using Dark Energy Survey Science Verification Data
• The KBC Void: Consistency with Supernovae Type Ia and the Kinematic SZ Effect in a $\Lambda$LTB Model
• Feedback from low-luminosity radio galaxies: B2 0258+35
• Feeble DM-SM Interaction via New Scalar and Vector Mediators in Rotating Neutron Stars
• A search for faint high-redshift radio galaxy candidates at 150 MHz
• Saez-Ballester gravity in Kantowski-Sachs Universe: a new reconstruction paradigm for Barrow Holographic Dark Energy
• Evolution of Dark Matter Halos and their Radio Emissions
• Cosmological constraints to dark matter with two- and many-body decays
• Radiative transfer with POLARIS. II.: Modeling of synthetic Galactic synchrotron observations
• Simulation-based inference of dynamical galaxy cluster masses with 3D convolutional neural networks
• Dark matter scenarios in a constrained model with Dirac gauginos
• Galactic dynamics and long-range quantum gravity
• The need for obscured supermassive black hole growth to explain quasar proximity zones in the epoch of reionization
• Strongly Coupled Dark Energy Cosmologies: preserving LCDM success and easing low scale problems II - Cosmological simulations
• The effect of dust bias on the census of neutral gas and metals in the high-redshift Universe due to SDSS-II quasar colour selection
• Inflationary cosmology with Chaplygin gas in Palatini formalism
• 21-cm signature of the first sources in the Universe: Prospects of detection with SKA
• Scale-invariant helical magnetic field evolution and the duration of inflation
• What is the distance to the CMB?
• How to Optimally Constrain Galaxy Assembly Bias: Supplement Projected Correlation Functions with Count-in-cells Statistics
• The BOSS-WiggleZ overlap region II: dependence of cosmic growth on galaxy type
• Cosmic Microwave Background Acoustic Peak Locations
• Cosmological Evidence Modelling: a new simulation-based approach to constrain cosmology on non-linear scales
• Dwarfs walking in a row. The filamentary nature of the NGC3109 association
• IDMS: Inert Dark Matter Model with a complex singlet
• Matter effects in neutrino visible decay at future long-baseline experiments
• Post-Planck Dark Energy Constraints
• The physical origins of low-mass spin bias
• Vacuum structure in a chiral R+R^n modification of pure supergravity
• Brightest galaxies as halo centre tracers in SDSS DR7
• Strong Lensing by Galaxies
• Massive Low Surface Brightness Galaxies in the EAGLE Simulation
• On the initial conditions for inflation with plateau potentials: the $R+R^2$ (super)gravity case
• Disorder in the Early Universe
• Search for Gamma-ray Spectral Lines from Dark Matter Annihilation in Dwarf Galaxies with the High-Altitude Water Cherenkov Observatory
• Origin of inflation in CFT driven cosmology: $R^2$-gravity and non-minimally coupled inflaton models
• Fragmentation inside atomic cooling haloes exposed to Lyman-Werner radiation
• Leptogenesis from Heavy Right-Handed Neutrinos in CPT Violating Backgrounds
• IROCKS: Spatially resolved kinematics of z~1 star forming galaxies
• Herschel-ATLAS/GAMA: SDSS cross-correlation induced by weak lensing
• A minimal model of inflation and dark radiation
• DEMNUni: comparing nonlinear power spectra prescriptions in the presence of massive neutrinos and dynamical dark energy
• Cross-correlation of galaxies and galaxy clusters in the Sloan Digital Sky Survey and the importance of non-Poissonian shot noise
• Statistical uncertainties and systematic errors in weak lensing mass estimates of galaxy clusters
• Comparison between the Logotropic and $\Lambda$CDM models at the cosmological scale
• The twisted dark matter halo of the Milky Way
• Do the observational data favor a local void?
• Constraining the dynamical dark energy parameters: Planck-2013 vs WMAP9
• Distinguishing Inert Higgs Doublet and Inert Triplet Scenarios
• Graceful exit from Higgs G-inflation
• Constraining the $\Lambda$CDM and Galileon models with recent cosmological data
• Type Ia Supernovae: Colors, Rates, and Progenitors
• Stars behind bars II: A cosmological formation scenario for the Milky Way's central stellar structure
• Asymptotically Safe Dark Matter
• Measuring the X-ray Background in the Reionization Era with First Generation 21 cm Experiments
• I. Apples to apples $A^2$: realistic galaxy simulated catalogs and photometric redshift predictions for next-generation surveys
• Gas flows in the circumgalactic medium around simulated high-redshift galaxies
• An optimal estimator for resonance bispectra in the CMB
• Modelling of Lyman-alpha Emitting Galaxies and Ionized Bubbles at the Era of Reionization
• CMB lensing power spectrum estimation without instrument noise bias
• Cosmology with the CMB temperature-polarization correlation
• The extended High A(V) Quasar Survey: Searching for dusty absorbers toward mid-infrared selected quasars
• Subdominant Left-Right Scalar Dark Matter as Origin of the 750 GeV Di-photon Excess at LHC
• $\Lambda$CDM Predictions for the Satellite Population of M33
• Conditions for detecting lensed Population III galaxies in blind surveys with the James Webb Space Telescope, the Roman Space Telescope and Euclid
• Majorana Neutrino Magnetic Moment and Neutrino Decoupling in Big Bang Nucleosynthesis
• Cosmological investigation of multi-frequency VLBI observations of ultra-compact structure in $z\sim 3$ radio quasars
• Nonlocal Metric Realizations of MOND
• Examining the consistency relations describing the three-point functions involving tensors
• The period--luminosity relation for Mira variables in the Milky Way using Gaia DR3: a further distance anchor for $H_0$
• Inflation of universe due to nonlinear electrodynamics
• Helicitogenesis: WIMPy baryogenesis with sterile neutrinos and other realizations
• Fermi-bounce cosmology and the fermion curvaton mechanism
• Faraday rotation at low frequencies: magnetoionic material of the large FRII radio galaxy PKS J0636-2036
• The evolution of the UV-to-mm extragalactic background light: evidence for a top-heavy initial mass function?
• Parameter discordance in Planck CMB and low-redshift measurements: projection in the primordial power spectrum
• How gas flows shape the stellar-halo mass relation in the EAGLE simulation
• Power Spectra Based Planck Constraints on Compensated Isocurvature, and Forecasts for LiteBIRD and CORE Space Missions
• A Hydrogen-Poor Superluminous Supernova with Enhanced Iron-Group Absorption: A New Link Between SLSNe and Broad-Lined Type Ic SNe
• A giant Ly$\alpha$ nebula in the core of an X-ray cluster at $z=1.99$: implications for early energy injection
• A Spatially-Resolved Survey of Distant Quasar Host Galaxies: I. Dynamics of galactic outflows
• The extended epoch of galaxy formation: age dating of ~3600 galaxies with 2<z<6.5 in the VIMOS Ultra-Deep Survey
• The Ellipsoidal Universe in the Planck Satellite Era
• Simulation tests of galaxy cluster constraints on chameleon gravity
• Out of the White Hole: A Holographic Origin for the Big Bang
• Interpretation of Departure from the Broad Line Region Scaling in Active Galactic Nuclei
• The origin of the cosmic gamma-ray background in the MeV range
• The Entire Virial Radius of the Fossil Cluster RXJ1159+5531: I. Gas Properties
• Closing in on the Tip of the CMSSM Stau Coannihilation Strip
• NIHAO III: The constant disc gas mass conspiracy
• Two-portal Dark Matter
• Dark Matter and Collider Studies in the Left-Right Symmetric Model with Vector-Like Leptons
• On the consistency of $\Lambda$CDM with CMB measurements in light of the latest Planck, ACT, and SPT data
• Explaining the DAMPE $e^{+}{e}^{-}$ excess using the Higgs triplet model with a vector dark matter
• A dynamics-based density profile for dark haloes -- II. Fitting function
• Significant Enhancement of Neutralino Dark Matter Annihilation from Electroweak Bremsstrahlung
• Morphological and Rotation Structures of Circumgalactic Mg II Gas in the EAGLE Simulation and the Dependence on Galaxy Properties
• Stability analysis and future singularity of the $m^{2}R{\square }^{-2}R$ model of non-local gravity
• The Parametrized Post-Newtonian-Vainshteinian Formalism
• The role of self-interacting right-handed neutrinos in galactic structure
• Dwarf spheroidal galaxies and Bose-Einstein condensate dark matter
• The perspective of voids on rising cosmology tensions
• Cosmological Structure Formation in Decaying Dark Matter Models
• The Physical Origin of Galactic Conformity: From Theory to Observation
• The dispersion measure and scattering of FRBs: Contributions from the intergalactic medium, foreground halos, and hosts
• The ALMA Frontier Fields Survey III: 1.1 mm Emission Line Identifications in Abell 2744, MACSJ0416.1-2403, MACSJ1149.5+2223, Abell 370, and Abell S1063
• Strong stellar-driven outflows shape the evolution of galaxies at cosmic dawn
• Velocity-dependent interacting dark energy and dark matter with a Lagrangian description of perfect fluids
• Shadow of black hole surrounded by magnetized plasma: Axion-plasmon cloud
• Detecting quantum gravitational effects of loop quantum cosmology in the early universe?
• Effective field theory interpretation of searches for dark matter annihilation in the Sun with the IceCube Neutrino Observatory
• Effects of type Ia supernovae absolute magnitude priors on the Hubble constant value
• Semi-analytic galaxies -- III. The impact of supernova feedback on the mass-metallicity relation
• Radial oscillations of quark stars admixed with dark matter
• Reconstructing Small Scale Lenses from the Cosmic Microwave Background Temperature Fluctuations
• First experimental constraints on the disformally coupled Galileon model
• Understanding parameter differences between analyses employing nested data subsets
• Scalar and tensor perturbations in loop quantum cosmology: High-order corrections
• Early ultraviolet emission in the Type Ia supernova LSQ12gdj: No evidence for ongoing shock interaction
• Statistical tests of sterile neutrinos using cosmology and short-baseline data
• Dynamical analysis of interacting dark energy model in the framework of particle creation mechanism
• The distinctions between $\Lambda$CDM and $f(T)$ gravity according Noether symmetry
• The evolution of barred galaxies in the EAGLE simulations
• The 2QDES Pilot : The luminosity and redshift dependence of quasar clustering
• Parameter splitting in dark energy: is dark energy the same in the background and in the cosmic structures?
• Constraints on massive vector dark energy models from integrated Sachs-Wolfe-galaxy cross-correlations
• The Fundamental Relation between Halo Mass and Galaxy Group Properties
• Revisiting the Exclusion Limits from Direct Chargino-Neutralino Production at the LHC
• Challenging matter creation models in the phantom divide
• Study of galaxies on large-scale filaments in simulations
• Constraint on $f(R)$ Gravity through the Redshift Space Distortion
• The contribution of HI-bearing ultra-diffuse galaxies to the cosmic number density of galaxies
• Lithium in CEMP-no stars: A new constraint on the lithium depletion mechanism in the early universe
• The Massive and Distant Clusters of WISE Survey: MOO J1142+1527, A 10${}^{15}$ M${}_{\odot }$ Galaxy Cluster at z=1.19
• Inflation After False Vacuum Decay: New Evidence from BICEP2
• The SDSS-IV eBOSS: emission line galaxy catalogues at z=0.8 and study of systematic errors in the angular clustering
• The SLUGGS Survey: Multi-population dynamical modelling of the elliptical galaxy NGC 1407 from stars and globular clusters
• Simplified Models for Exotic BSM Searches
• Exploring the early dust-obscured phase of galaxy formation with blind mid-/far-IR spectroscopic surveys
• Neutron Stars and Dark Matter
• CosmicNet I: Physics-driven implementation of neural networks within Boltzmann-Einstein solvers
• Light mediators in dark matter direct detections
• Gravity Waves From Non-Minimal Quadratic Inflation
• The Structure of the Strongly Lensed Gamma-ray Source B2 0218+35
• Searching for features of a string-inspired inflationary model with cosmological observations
• The Cosmic Star Formation Rate from the Faintest Galaxies in the Unobservable Universe
• Boundary Localized Terms in Universal Extra-Dimensional Models through a Dark Matter perspective
• Dark matter interpretations of ATLAS searches for the electroweak production of supersymmetric particles in $\sqrt{s}=8$ TeV proton-proton collisions
• DEMNUni: disentangling dark energy from massive neutrinos with the void size function
• Strategies for Probing Non-Minimal Dark Sectors at Colliders: The Interplay Between Cuts and Kinematic Distributions
• Constraining neutrino properties with a Euclid-like galaxy cluster survey
• Dark Matter from Late Invisible Decays to/of Gravitinos
• Surrogate modelling the Baryonic Universe I: The colour of star formation
• The structural properties of classical bulges and discs from z~2
• 'Exotic vector-like pair' of color-triplet scalars
• IC 3639 - A new bona fide Compton thick AGN unveiled by NuSTAR
• Viscous Self Interacting Dark Matter and Cosmic Acceleration
• Measuring patchy reionisation with kSZ${}^2$-21 cm correlations
• Cosmological constraints on dark matter annihilation and decay: Cross-correlation analysis of the extragalactic $\gamma$-ray background and cosmic shear
• Active Galactic Nuclei with Ultra-fast Outflows Monitoring Project: The Broad-line Region of Mrk 79 as a Disk Wind
• The GOGREEN survey: Dependence of galaxy properties on halo mass at z > 1 and implications for environmental quenching
• Constraining Big Bang lithium production with recent solar neutrino data
• Flavor origin of dark matter and its relation with leptonic nonzero ${\theta }_{13}$ and Dirac CP phase $\delta$
• An Iwasawa-Taniguchi Effect for Compton-thick Active Galactic Nuclei
• Universality in Pure Gravity Mediation with Vector Multiplets
• How AGN feedback drives the size growth of the first quasars
• Statistical Anisotropies in Gravitational Waves in Solid Inflation
• Cosmological DCBH formation sites hostile for their growth
• The impact of ionised outflows from z$\sim$2.5 quasars is not through instantaneous in-situ quenching: the evidence from ALMA and VLT/SINFONI
• Galaxy clustering dependence on the $\left[\mathrm{O}\mathrm{II}\right]$ emission line luminosity in the local Universe
• Reconciling Planck cluster counts and cosmology? Chandra/XMM instrumental calibration and hydrostatic mass bias
• Contamination of early-type galaxy alignments to galaxy lensing-CMB lensing cross-correlation
• The Dynamical Mass of the Coma Cluster from Deep Learning
• Models of the Cosmological 21 cm Signal from the Epoch of Reionization Calibrated with Lyman-alpha and CMB Data
• The effects of a fast-turning trajectory in multiple-field inflation
• Evolution of spherical overdensities in holographic dark energy models
• A new approach to determine optically thick H2 cooling and its effect on primordial star formation
• Probing DAMA/LIBRA in the full parameter space of WIMP effective models of inelastic scattering
• SN2002es-like Supernovae From Different Viewing Angles
• Performance of a prototype active veto system using liquid scintillator for a dark matter search experiment
• Young, Star-forming Galaxies and their local Counterparts: the Evolving Relationship of Mass-SFR-Metallicity since z ~ 2.1
• Nonthermal production of dark radiation and dark matter
• An astrophysically motivated ranking criterion for low-latency electromagnetic follow-up of gravitational wave events
• Diagnostic of Horndeski Theories
• Leptogenesis with a dynamical seesaw scale
• Inflation beyond T-models and primordial B-modes
• Particle Spectroscopy of Supersymmetric SU(5) in Light of 125 GeV Higgs and Muon g-2 Data
• The physical drivers of gas turbulence in simulated disc galaxies
• The absolute age of the globular cluster M15 using near-infrared adaptive optics images from PISCES/LBT
• 3.5-keV X-ray line from nearly-degenerate WIMP dark matter decays
• The Scale-Invariant Vacuum (SIV) Theory: A Possible Origin of Dark Matter and Dark Energy
• The galaxy size to halo spin relation of disk galaxies in cosmological hydrodynamical simulations
• Cosmic microwave background radiation temperature in a dissipative universe
• Cosmological birefringence constraints from CMB and astrophysical polarization data
• A thermodynamics revision of Rastall gravity
• CMB anisotropies generated by a stochastic background of primordial magnetic fields with non-zero helicity
• Leptobaryons as Majorana Dark Matter
• Dynamics of non-minimally coupled perfect fluids
• Quantum Corrections in Galileons from Matter Loops
• Probing the physical and mathematical structure of $f(R)$ gravity by PSR $J0348+0432$
• Fermionic Light Dark Matter particles and the New Physics of Neutron Stars
• On the environmental influence of groups and clusters of galaxies beyond the virial radius: Galactic conformity at few Mpc scales
• Heavy quark-philic scalar dark matter with a vector-like fermion portal
• Deconvolving the Wedge: Maximum-Likelihood Power Spectra via Spherical-Wave Visibility Modeling
• Extended Axion Dark Matter Search Using the CAPP18T Haloscope
• How galaxies populate haloes in very low-density environments? An analysis of the Halo Occupation Distribution in cosmic voids
• Extended Phase Space Analysis of Interacting Dark Energy Models in Loop Quantum Cosmology
• NIHAO XXIV: Rotation or pressure supported systems? Simulated Ultra Diffuse Galaxies show a broad distribution in their stellar kinematics
• Clustering with JWST: Constraining Galaxy Host Halo Masses, Satellite Quenching Efficiencies, and Merger Rates at z=4-10
• Coupled tachyonic dark energy: a dynamical analysis
• Constraint on the time variation of the fine-structure constant with the SDSS-III/BOSS DR12 quasar sample
• Cross-correlation cosmic shear with the SDSS and VLA FIRST surveys
• Anatomy of a z=6 Lyman-α emitter down to parsec scales: extreme UV slopes, metal-poor regions and possibly leaking star clusters
• A magnified glance into the dark sector: probing cosmological models with strong lensing in A1689
• Searching for the Evidence of Dynamical Dark Energy
• Assessing the photometric redshift precision of the S-PLUS survey: the Stripe-82 as a test-case
• Cosmological dynamics with non-minimally coupled scalar field and a constant potential function
• Galaxy clusters in local Universe simulations without density constraints: a long uphill struggle
• DEMNUni: The imprint of massive neutrinos on the cross-correlation between cosmic voids and CMB lensing
• Polarization alignments of radio quasars in JVAS/CLASS surveys
• Constraining spatial variations of the fine structure constant using clusters of galaxies and Planck data
• A comment on power-law inflation with a dark radiation component
• Search for sharp and smooth spectral signatures of $\mu \nu$SSM gravitino dark matter with Fermi-LAT
• A multi-simulation study of relativistic SZ temperature scalings in galaxy clusters and groups
• The shape of galaxy dark matter halos in massive galaxy clusters: Insights from strong gravitational lensing
• Radio-Gamma-ray connection and spectral evolution in 4C +49.22 (S4 1150+49): the Fermi, Swift and Planck view
• Void profile from Planck lensing potential map
• Stability of Effective Thin-shell Wormholes Under Lorentz Symmetry Breaking Supported by Dark Matter and Dark Energy
• Large Scale Anisotropic Bias from Primordial non-Gaussianity
• Constrained Supersymmetry after the Higgs Boson Discovery: A global analysis with Fittino
• Shapes of Milky-Way-Mass Galaxies with Self-Interacting Dark Matter
• Viscosity, pressure, and support of the gas in simulations of merging cool-core clusters
• The halo bias inside cosmic voids
• The refractive index of relic gravitons
• Search for gamma-ray emission from super-luminous supernovae with the Fermi-LAT
• Galaxy clusters in simulations of the local Universe: a matter of constraints
• Confronting a New Three-loop Seesaw Model with the 750 GeV Diphoton Excess
• Hunting down systematics in baryon acoustic oscillations after cosmic high noon
• Measuring the evolution of intergalactic gas from z=0 to 5 using the kinematic Sunyaev-Zel'dovich effect
• BeyondPlanck I. Global Bayesian analysis of the Planck Low Frequency Instrument data
• Approximate Bayesian Uncertainties on Deep Learning Dynamical Mass Estimates of Galaxy Clusters
• The eventful life of GS-z14-0, the most distant galaxy at redshift $z=14.32$
• Galaxy bias from the Dark Energy Survey Science Verification data: combining galaxy density maps and weak lensing maps
• Probing galaxy assembly bias with LRG weak lensing observations
• Fast Bayesian inference for slow-roll inflation
• Gravitino LSP and leptogenesis after the first LHC results
• The stellar halo in Local Group Hestia simulations I. The in-situ component and the effect of mergers
• Linking the brightest stellar streams with the accretion history of Milky Way-like galaxies
• Parameter Inference for Weak Lensing using Gaussian Processes and MOPED
• Dark Supersymmetry
• Inflationary Features and Shifts in Cosmological Parameters from Planck 2015 Data
• Phenomenology of the Higgs sector of a Dimension-7 Neutrino Mass Generation Mechanism
• Inert Doublet Dark Matter with an additional scalar singlet and 125 GeV Higgs Boson
• The Type I Superluminous Supernova PS16aqv: Lightcurve Complexity and Deep Limits on Radioactive Ejecta in a Fast Event
• The Detection and Statistics of Giant Arcs Behind CLASH Clusters
• New thresholds for Primordial Black Hole formation during the QCD phase transition
• Thermodynamically allowed phantom cosmology with viscous fluid
• One-point fluctuation analysis of the high-energy neutrino sky
• Connecting inflation with late cosmic acceleration by particle production
• Dark Radiation in Anisotropic LARGE Volume Compactifications
• Effects of ghost dark energy perturbations on the evolution of spherical overdensities
• Criticality and Inflation of the Gauged B-L Model
• Cosmological model of the interaction between dark matter and dark energy
• Dynamics of Gauge Field Inflation
• Visible sector inflation and the right thermal history in light of Planck data
• Reheating temperature in non-minimal derivative coupling model
• Probing $f(R)$ cosmology with sterile neutrinos via measurements of scale-dependent growth rate of structure
• Leptogenesis in an SU(5) x A5 Golden Ratio Flavour Model
• Fully covering the MSSM Higgs sector at the LHC
• A divergence-free parametrization for dynamical dark energy
• How to Search for Islands of Neutral Hydrogen in the $z\sim 5.5$ IGM
• Multiple Lensing of the Cosmic Microwave Background anisotropies
• 3D Weak Gravitational Lensing of the CMB and Galaxies
• Dark Stars: Improved Models and First Pulsation Results
• Cosmological tests of modified gravity: constraints on $F(R)$ theories from the galaxy clustering ratio
• Power law Starobinsky model of inflation from no-scale SUGRA
• Phenomenological signatures of mixed complex scalar WIMP dark matter
• Search for Bosonic Super-WIMP Interactions with the XENON100 Experiment
• First star formation in ultra-light particle dark matter cosmology
• Cosmology of a generalised version of holographic dark energy in presence of bulk viscosity and its inflationary dynamics through slow roll parameters
• The role of AGN feedback on the evolution of dwarf galaxies from cosmological simulations: SMBHs suppress star formation in low-mass galaxies
• Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
• Constraints on Primordial Magnetic Fields from their impact on the ionization history with Planck 2018
• The impact of natal kicks on galactic r-process enrichment by neutron star mergers
• Probing the thermal history during reionization using a semi-numerical photon-conserving code SCRIPT
• The effect of inhomogeneous reionisation on the Lyman-$\alpha$ forest power spectrum at redshift $z>4$: implications for thermal parameter recovery
• Impact of internal-delensing biases on searches for primordial B-modes of CMB polarisation
• Unified Dark Fluid and Cosmic Transit Models in Brans-Dicke Theory
• Entropy Driven Winds: Outflows and Fountains Lifted Gently by Buoyancy
• Anisotropic massive Brans-Dicke gravity extension of the standard $\Lambda$CDM model
• The scattering of FRBs by the intergalactic medium: variations, strength and dependence on dispersion measures
• A Radial Measurement of the Galaxy Tidal Alignment Magnitude with BOSS Data
• Two Component Feebly Interacting Massive Particle (FIMP) Dark Matter
• Dynamics of warm power-law plateau inflation with a generalized inflaton decay rate: predicctions and constraints after Planck 2015
• Revealing modified gravity signal in matter and halo hierarchical clustering
• Cosmological Simulations of Dwarf Galaxies with Cosmic Ray Feedback
• One-loop renormalisation of the NMSSM in SloopS : 1. the neutralino-chargino and sfermion sectors
• Massive Gauge-flation
• Mass-concentration relation of clusters of galaxies from CFHTLenS
• General Analysis of Dark Radiation in Sequestered String Models
• Planck intermediate results. XXXIX. The Planck list of high-redshift source candidates
• Gravitino Dark Matter and low-scale Baryogenesis
• Coarse-grained description of cosmic structure from Szekeres models
• Planets in Other Universes: Habitability constraints on density fluctuations and galactic structure
• GARROTXA Cosmological Simulations of Milky Way-sized Galaxies: General Properties, Hot Gas Distribution, and Missing Baryons
• Diffuse coronae in cosmological simulations of Milky Way-sized galaxies
• Broadband distortion modeling in Lyman-$\alpha$ forest BAO fitting
• Cold imprint of supervoids in the Cosmic Microwave Background re-considered with Planck and BOSS DR10
• Testing Lambda CDM cosmology at turnaround: where to look for violations of the bound?
• Polarization Predictions for Inflationary CMB Power Spectrum Features
• More Viable Parameter Space for Leptogenesis
• Dark matter production from Goldstone boson interactions and implications for direct searches and dark radiation
• Cosmological evidence for leptonic asymmetry after Planck
• Targeting supermassive black hole binaries and gravitational wave sources for the pulsar timing array
• Supersymmetry at the LHC and The Theory of R-parity
• Fluid Inflation
• Implications of 98 GeV and 125 GeV Higgs scenario in non-decoupling SUSY with updated ATLAS, CMS and PLANCK data
• Generalized interacting Barrow Holographic Dark Energy: cosmological predictions and thermodynamic considerations
• Spontaneous CP Violation in Lepton-sector: a common origin for ${\theta }_{13}$, Dirac CP phase and leptogenesis
• Photon Number Conserving Models of H II Bubbles during Reionization
• A method to determine the evolution history of the mean neutral Hydrogen fraction
• RESOLVE and ECO: The Halo Mass-Dependent Shape of Galaxy Stellar and Baryonic Mass Functions
• Investigating the accelerated expansion of the Universe through updated constraints on viable $f(R)$ models within the metric formalism
• Phenomenology of Dark Matter via a Bimetric Extension of General Relativity
• Constraining the Nature of Two Ly-alpha Emitters detected by ALMA at z = 4.7
• Post LHC8 SUSY benchmark points for ILC physics
• The effective theory of fluids at NLO and implications for dark energy
• Quantifying resolution in cosmological N-body simulations using self-similarity
• Searching for primordial magnetism with multi-frequency CMB experiments
• Forecast for weighing neutrinos in cosmology with SKA
• Sound speed of scalar field dark energy: weak effects and large uncertainties
• The stellar halo in Local Group Hestia simulations II. The accreted component
• Life, the universe, and everything - 42 fundamental questions
• Effective Field Theory of non-Attractor Inflation
• Neutrino phenomenology and scalar Dark Matter with $A_4$ flavor symmetry in Inverse and type II seesaw
• Cyclic cosmology in modified gravity
• Prospects of type-II seesaw at future colliders in light of the DAMPE $e^{+}{e}^{-}$ excess
• The Herschel-ATLAS: magnifications and physical sizes of $500\mu$m-selected strongly lensed galaxies
• Probing the flavor violating scalar top quark signal at the LHC
• Effect of non-equilibrium ionization on derived physical conditions of the high-$z$ intergalactic medium
• Non-linear general relativistic effects in the observed redshift
• Accuracy of cosmological parameters using the baryon acoustic scale
• GOGREEN: a critical assessment of environmental trends in cosmological hydrodynamical simulations at z ~ 1
• Cosmological signatures of tilted isocurvature perturbations: reionization and 21cm fluctuations
• Modeling holographic dark energy with particle and future horizons
• Cosmological Evolution and Solar System Consistency of Massive Scalar-Tensor Gravity
• The detection of the imprint of filaments on cosmic microwave background lensing
• Precision growth index using the clustering of cosmic structures and growth data
• On the Interpretation of Far-infrared Spectral Energy Distributions. I: The 850 $\mu$m Molecular Mass Estimator
• Generation of large-scale magnetic fields, non-Gaussianity, and primordial gravitational waves in inflationary cosmology
• Covariant c-flation: a variational approach
• Joint Planck and WMAP Assessment of Low CMB Multipoles
• An embedded active nucleus in the OH megamaser galaxy IRAS16399-0937
• Finslerian Ressiner-Nordstrom spacetime
• No evidence for dust B-mode decorrelation in Planck data
• Two-loop Neutrino Model with Exotic Leptons
• Reconstruction of interaction rate in Holographic dark energy model with Hubble horizon as the infrared cut-off
• Light dark matter scattering in outer neutron star crusts
• On the influence of the environment on galactic chemical abundances
• High-resolution synthetic UV-submm images for Milky Way-mass simulated galaxies from the ARTEMIS project
• The Higgsino-Singlino World at the Large Hadron Collider
• Neutrino Masses and Deviation from Tri-bimaximal mixing in Δ(27) model with Inverse Seesaw Mechanism
• The Effect of Modified Gravity on the Odds of the Bound Violations of the Turn-Around Radii
• Multiply lensed star forming clumps in the A521-sys1 galaxy at redshift 1
• Lepton asymmetry, neutrino spectral distortions, and big bang nucleosynthesis
• Radiatively Induced Neutrino Mass Model with Flavor Dependent Gauge Symmetry
• The ultra-diffuse dwarf galaxies NGC 1052-DF2 and 1052-DF4 are in conflict with standard cosmology
• Confronting the concordance model of cosmology with Planck data
• Simulating cosmologies beyond $\Lambda$CDM with PINOCCHIO
• Spherical collapse and halo mass function in the symmetron model
• Optical & Sunyaev-Zel'dovich Observations of a New Sample of Distant Rich Galaxy Clusters in the ROSAT All Sky Survey
• Can phantom transition at $z\sim 1$ restore the Cosmic concordance?
• Expected dipole asymmetry in CMB polarization
• Leptophobic Dark Matter and the Baryon Number Violation Scale
• Modified Lyth bound and implications of BICEP2 results
• Semi-analytical description of clumping factor and CMB free-free distortions from reionization
• Hidden SUSY from precision gauge unification
• Fast $\gamma$-ray variability in blazars beyond redsift 3
• Gravitational Lensing of Cosmological 21cm Emission
• CMB constraints on mass and coupling constant of light pseudoscalar particles
• Studying Inflation with Future Space-Based Gravitational Wave Detectors
• Cluster counts: calibration issue or new physics?
• Light Higgsinos in Pure Gravity Mediation
• Unlocking the Full Potential of Extragalactic Ly$\alpha$ through Its Polarization Properties
• Subhalo accretion through filaments
• Satellite galaxies around present-day massive ellipticals
• A first estimate of the Milky Way dark matter halo spin
• Primordial Gravitational Waves with LISA
• Cosmic Reionization May Still Have Started Early and Ended Late: Confronting Early Onset with CMB Anisotropy and 21 cm Global Signals
• Inference from the small scales of cosmic shear with current and future Dark Energy Survey data
• Driving the Growth of the Earliest Supermassive Black Holes with Major Mergers of Host Galaxies
• Primordial Nucleosynthesis in the Rh = ct cosmology: Pouring cold water on the Simmering Universe
• Convolution Lagrangian perturbation theory for biased tracers beyond general relativity
• Preprocessing, mass loss and mass segregation of galaxies in DM simulations
• Dark-matter-deficient galaxies in hydrodynamical simulations
• Gamma-ray Signals from Dark Matter Annihilation Via Charged Mediators
• A Radio Quasi-periodic Oscillation of 176 day in the Radio-loud Narrow-line Seyfert 1 Galaxy J0849+5108
• Cosmological Constraints on the Gravitational Interactions of Matter and Dark Matter
• MeV-Scale Dark Matter Deep Underground
• A new calibration method of sub-halo orbital evolution for semi-analytic models
• Asymmetric Dark Matter, Inflation and Leptogenesis from B-L Symmetry Breaking
• Testing gravity at large scales with HI intensity mapping
• Cosmology with a successful Vainshtein screening in theories beyond Horndeski
• The stellar halo in Local Group Hestia simulations III. Chemical abundance relations for accreted and in-situ stars
• Probing neutrino physics with a self-consistent treatment of the weak decoupling, nucleosynthesis, and photon decoupling epochs
• The MBHBM${}^{\star }$ Project -- II. Molecular Gas Kinematics in the Lenticular Galaxy NGC 3593 Reveal a Supermassive Black Hole
• SKA-Phase 1 sensitivity for synchrotron radio emission from multi-TeV Dark Matter candidates
• Vacuum energy and the cosmological constant
• Accelerated expansion from cosmological holography
• Why Comparable? A Multiverse Explanation of the Dark Matter-Baryon Coincidence
• Energy and momentum of Bianchi Type VI_h Universes
• Spiral Inflation
• Gaussianisation for fast and accurate inference from cosmological data
• Cosmological simulations of Milky Way-sized galaxies
• No-go guide for the Hubble tension: late-time or local-scale new physics
• Observational Hints of a Pre--Inflationary Scale?
• The DESI PRObabilistic Value-Added Bright Galaxy Survey (PROVABGS) Mock Challenge
• Study of diphoton decays of the lightest scalar Higgs boson in the Next-to-Minimal Supersymmetric Standard Model
• Panchromatic Hubble Andromeda Treasury XIII: The Cepheid period-luminosity relation in M31
• Cosmic metal density evolution in neutral gas: insights from observations and cosmological simulations
• Testing Metal Poor Stellar Models and Isochrones with HST Parallaxes of Metal Poor Stars
• Statistical Isotropy violation of CMB polarization sky due to Lorentz boost
• Physics of the cosmic microwave background anisotropy
• How to obtain a cosmological constant from small exotic R^4
• Non-abelian Dark Matter Solutions for Galactic Gamma-ray Excess and Perseus 3.5 keV X-ray Line
• ZOMG III: The effect of Halo Assembly on the Satellite Population
• New cosmological constraints with extended-Baryon Oscillation Spectroscopic Survey DR14 quasar sample
• Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XI. Proximity Zone Analysis for Faint Quasar Spectra at z~6
• Slowly decaying resonances of massive scalar fields around Schwarzschild-de Sitter black holes
• The phenomenology of beyond Horndeski gravity
• Assessing Consistency Between WMAP 9-year and Planck 2015 Temperature Power Spectra
• Hidden Superconformal Symmetry of the Cosmological Evolution
• Dark Matter, Muon $g-2$, Electric Dipole Moments and $Z\to {\ell }_i^{+}{\ell }_j^{-}$ in a One-Loop Induced Neutrino Model
• What sets the splashback radius of dark matter haloes: accretion history or other properties?
• The impact of two massive early accretion events in a Milky Way-like galaxy: repercussions for the buildup of the stellar disc and halo
• Geometry of the effective Majorana neutrino mass in the neutrinoless double-beta decay
• The origin of spin in galaxies: clues from simulations of atomic cooling halos
• Baryonic mass budgets for haloes in the EAGLE simulation, including ejected and prevented gas
• $\bar{T}$: A New Cosmological Parameter?
• Component Separation of a Isotropic Gravitational Wave Background
• Dark radiation and dark matter in supersymmetric axion models with high reheating temperature
• Helical cosmological magnetic fields from extra-dimensions
• Orbit optimization and time delay interferometry for inclined ASTROD-GW formation with half-year precession-period
• Gravitational wave signatures from an extended inert doublet dark matter model
• Cosmological parameter constraints from CMB lensing with cosmic voids
• Dark Energy: The Shadowy Reflection of Dark Matter?
• Hot and Turbulent Gas in Clusters
• Catalog of Long-Term Transient Sources in the First 10 Years of Fermi-LAT Data
• Charged Higgs boson in the $W^{\pm }$ Higgs channel at the Large Hadron Collider
• Gravitational waves from the remnants of the first stars in nuclear star clusters
• Planck's Dusty GEMS. III. A massive lensing galaxy with a bottom-heavy stellar initial mass function at z=1.5
• Lensing Model of MACS J1149.5+2223 - I. Cluster mass reconstruction
• An Ultimate Target for Dark Matter Searches
• Cosmological dynamics of brane gravity: A global dynamical system perspective
• First order electroweak phase transition triggered by the Higgs portal vector dark matter
• 3.55 keV line in Minimal Decaying Dark Matter scenarios
• The "Missing Mass Problem" in Astronomy and the Need for a Modified Law of Gravity
• A Measurement of Atomic X-ray Yields in Exotic Atoms and Implications for an Antideuteron-Based Dark Matter Search
• Constraining the propagation speed of gravitational waves with compact binaries at cosmological distances
• The galaxy luminosity function and the Local Hole
• Growth Rate in the Dynamical Dark Energy Models
• Cosmic variance in the nanohertz gravitational wave background
• Non-Gaussianity excess problem in classical bouncing cosmologies
• Gamma Lines from Majorana Dark Matter
• A hidden population of massive black holes in simulated dwarf galaxies
• Coupled vector dark energy
• Dark energy survivals in massive gravity after GW170817: SO(3) invariant
• Asymptotically Safe Higgs Inflation
• Strong thermal leptogenesis and the absolute neutrino mass scale
• Exploring the diversity and similarity of radially anisotropic Milky Way-like stellar haloes: implications for disrupted dwarf galaxy searches
• Dark Matter Superfluidity
• Electroweak baryogenesis in the framework of the effective field theory
• An extended size-luminosity relation for the reverberation-mapped AGNs: the role of the accretion rate
• Dynamics of Einstein-Aether Scalar field Cosmology
• Exploring the Milky Way Circumgalactic Medium in a Cosmological Context with a Semi-Analytic Model
• Type Ib SN 1999dn as an example of the thoroughly mixed ejecta of Ib supernovae
• Cosmological consequences of classical flavor-space locked gauge field radiation
• Dark matter relic density in Gauss-Bonnet braneworld cosmology
• Tensor to scalar ratio and large scale power suppression from pre-slow roll initial conditions
• Dynamical Fractional Chaotic Inflation -- Dynamical Generation of a Fractional Power-Law Potential for Chaotic Inflation
• A new fast radio burst in the datasets containing the Lorimer burst
• Late-time acceleration with a scalar field source: Observational constraints and statefinder diagnostics
• Hubble constant and sound horizon from the late-time Universe
• A Comparison of Maps and Power Spectra Determined from South Pole Telescope and Planck Data
• Dynamical Systems Analysis of K-essence Model
• Sky reconstruction for the Tianlai cylinder array
• ALMA observations of lensed Herschel sources : Testing the dark-matter halo paradigm
• Heavy colored SUSY partners from deflected anomaly mediation
• CMB constraints on a physical model of reionization
• Constraints on sneutrino dark matter from LHC Run 1
• Disformally coupled inflation
• New constraints on Lorentz invariance violation with polarized gamma-ray bursts
• Revisiting a pre-inflationary radiation era and its effect on the CMB power spectrum
• Les Houches lectures on inflationary observables and string theory
• The structure and evolution of a forming galaxy cluster at z = 1.62
• Mixed (Cold+Warm) Dark Matter in the Bino-Wino co-annihilation scenario
• Mono-Higgs signature in fermionic dark matter model
• Spectroscopy of Scalar Mediators to Dark Matter at the LHC and at 100 TeV
• Models of Distorted and Evolving Dark Matter Halos
• Dark Matter Simulations with Primordial Black Holes in the Early Universe
• Interpretation of the Cosmological Constant Problem within the Framework of Generalized Uncertainty Principle
• Vector theory of gravity: Universe without black holes and solution of dark energy problem
• Probing Modified Gravity with Integrated Sachs-Wolfe CMB and Galaxy Cross-correlations
• Limits on optical polarization during the prompt phase of GRB 140430A
• RAY-RAMSES: a code for ray tracing on the fly in N-body simulations
• Non-linearities in the Lyman-$\alpha$ forest and in its cross-correlation with dark matter halos
• The metal enrichment of passive galaxies in cosmological simulations of galaxy formation
• Cascading Dark Energy
• Direct dark matter searches - Test of the Big Bounce Cosmology
• Constraint on Primordial Magnetic Fields In the Light of ARCADE 2 and EDGES Observations
• I- A hydrodynamical CLONE of the Virgo cluster of galaxies to confirm observationally-driven formation scenarios
• Excess of high-$z$ galaxies as a test for bumpy power spectrum of density perturbations
• Neutrinoless Double Beta Decay in LRSM with Natural Type-II seesaw Dominance
• Subaru Hyper Suprime-Cam Survey for An Optical Counterpart of GW170817
• Consistency relation in power law G-inflation
• Cross-correlating 21 cm and galaxy surveys: implications for cosmology and astrophysics
• Asymmetric Dark Matter and CP Violating Scatterings in a UV Complete Model
• Constraints on a seesaw model leading to quasidegenerate neutrinos and signatures at the LHC
• Gas inflow and outflow in an interacting high-redshift galaxy: The remarkable host environment of GRB 080810 at $z=3.35$
• A dynamics-free lower bound on the mass of our galaxy
• AMS-02 Positron Excess and Indirect Detection of Three-body Decaying Dark Matter
• Mass-Temperature relation in $\Lambda$CDM and modified gravity
• Dark matter origins of neutrino masses
• Reconstruction of interaction rate in Holographic dark energy
• Dwarf Spheroidal Satellite Formation in a Reionized Local Group
• Cosmic Infrared Background anisotropies as a window into primordial non-Gaussianity
• The $Z_3$ symmetric I(2+1)HDM
• Known Unknowns of Dark Matter Annihilation over Cosmic Time
• Unifying the flavor origin of dark matter with leptonic nonzero ${\theta }_{13}$
• UV-extending Ghost Inflation
• Gaussian Approximation of Peak Values in the Integrated Sachs-Wolfe Effect
• Multipolar moments of weak lensing signal around clusters. Weighing filaments in harmonic space
• The Epoch of Reionization 21-cm Bispectrum: The impact of light-cone effects and detectability
• Running with BICEP2: Implications for Small-Scale Problems in CDM
• Galaxy and Mass Assembly (GAMA): Formation and Growth of Elliptical Galaxies in the Group Environment
• The hierarchy problem of the electroweak Standard Model revisited
• Chiral Imprint of a Cosmic Gauge Field on Primordial Gravitational Waves
• Fluctuations of the gravitational field generated by a random population of extended substructures
• Detecting strongly lensed supernovae at z ~ 5-7 with LSST
• Neutrinophilic two Higgs doublet model with dark matter under an alternative $U(1{)}_{B-L}$ gauge symmetry
• Origins of carbon-enhanced metal-poor stars
• Generalized spin-dependent WIMP-nucleus interactions and the DAMA modulation effect
• The universal multiplicity function: counting halos and voids
• Decoupling and de Sitter Vacua in Approximate No-Scale Supergravities
• The growth index of matter perturbations using the clustering of dark energy
• Explain DAMPE Results by Dark Matter With Hierarchical Lepton-Specific Yukawa Interactions
• Testing Vector Gravity with Gravitational Wave Interferometers
• Possibilities and Limitations of Kinematically Identifying Stars from Accreted Ultra-Faint Dwarf Galaxies
• The VLT LBG Redshift Survey - IV. Gas and galaxies at z ~ 3 in observations and simulations
• The Eccentric and Accelerating Stellar Binary Black Hole Mergers in Galactic Nuclei: Observing in Ground and Space Gravitational Wave Observatories
• Probing large-scale magnetism with the Cosmic Microwave Background
• The Magnetic Field and Polarization Properties of Radio Galaxies in Different Accretion States
• Cosmic CARNage II: the evolution of the galaxy stellar mass function in observations and galaxy formation models
• Cosmological singularities and analytical solutions in varying vacuum cosmologies
• Direction dependence of cosmological parameters due to cosmic hemispherical asymmetry
• Dark Energy: A Short Review
• Higher derivatives and power spectrum in effective single field inflation
• The impact of non-Gaussianity on the Epoch of Reionization parameter forecast using 21-cm power spectrum measurements
• Not a Copernican observer: biased peculiar velocity statistics in the local Universe
• Kinematic Constraints on Spatial Curvature from Supernovae Ia and Cosmic Chronometers
• The Impact of Neutral Intergalactic Gas on Lyman-$\alpha$ Intensity Mapping During Reionization
• Kinematics of the molecular interstellar medium probed by Gaia: steep velocity dispersion-size relation, isotropic turbulence, and location-dependent energy dissipation
• Dark matter and $B$-meson anomalies in a flavor dependent gauge symmetry
• Cosmic Polarization Rotation: an Astrophysical Test of Fundamental Physics
• Galaxy formation in the Planck cosmology II. Star formation histories and post-processing magnitude reconstruction
• Testing cosmic acceleration for $w(z)$ parameterizations using $f_{gas}$ measurements in galaxy clusters
• Observational Constraints in Nonlocal Gravity: the Deser-Woodard Case
• Can the 21 cm signal probe Population III and II star formation?
• Cosmological forecasts for future galaxy surveys with the linear point standard ruler: Toward consistent BAO analyses far from a fiducial cosmology
• The halo mass function in alternative dark matter models
• Reconciling galaxy cluster shapes, measured by theorists vs observers
• Galaxy halo expansions: a new biorthogonal family of potential-density pairs
• Higgs-portal Scalar Dark Matter: Scattering Cross Section and Observable Limits
• Looking for hints of a reconstructible seesaw model at the Large Hadron Collider
• Euclid: Effect of sample covariance on the number counts of galaxy clusters
• New quasar proximity zone size measurements at $z\sim 6$ using the enlarged XQR-30 sample
• Orbit-Superposition Dynamical Modeling of Barred Galaxies
• Evidence for non-axisymmetry in M31 from wide-field kinematics of stars and gas
• Confronting the neutralino and chargino sector of the NMSSM to the multi-lepton searches at the LHC
• A solution of the dark energy and its coincidence problem based on local antigravity sources without fine-tuning or new scales
• Correlation function of the luminosity distances
• A comparison of CMB Angular Power Spectrum Estimators at Large Scales: the TT case
• Simulations of the Galaxy Cluster CIZA J2242.8+5301 I: Thermal Model and Shock Properties
• Vacuum energy as dark matter
• A Neural-Network based estimator to search for primordial non-Gaussianity in Planck CMB maps
• North-South non-Gaussian asymmetry in PLANCK CMB maps
• Testing the mapping between redshift and cosmic scale factor
• The assembly of spheroid-dominated galaxies in the EAGLE simulation
• Antiproton Limits on Decaying Gravitino Dark Matter
• Doublet-singlet model and unitarity
• Leptogenesis in an SU(5) x A5 Golden Ratio Flavour Model: Addendum
• Interpreting broad emission-line variations II: Tensions between luminosity, characteristic size and responsivity
• PeV-EeV neutrinos from GRB blastwave in IceCube and future neutrino telescopes
• On the connection between the metal-enriched intergalactic medium and galaxies: an OVI-galaxy cross-correlation study at $z<1$
• RedMaPPer: Evolution and Mass Dependence of the Conditional Luminosity Functions of Red Galaxies in Galaxy Clusters
• Primordial features from ekpyrotic bounces
• Multiwavelength Study of the Quiescent States of Six Brightest Flat Spectrum Radio Quasars detected by Fermi-LAT
• Ly-alpha emission in low-redshift most metal-deficient compact star-forming galaxies
• Theoretical priors in scalar-tensor cosmologies: Thawing quintessence
• Long gamma-ray burst rate at very high redshift
• Microwave Background Polarization as a Probe of Large-Angle Correlations
• CFHTLenS: A Gaussian likelihood is a sufficient approximation for a cosmological analysis of third-order cosmic shear statistics
• Inevitable imprints of patchy reionization on the cosmic microwave background anisotropy
• Cosmological Consequences of a Variable Cosmological Constant Model
• Probing the statistical properties of CMB $B$-mode polarization through Minkowski Functionals
• Non-Gaussian Structure of B-mode Polarization after Delensing
• A Two-Dimensional Spectroscopic Study of Emission Line Galaxies in the Faint Infrared Grism Survey (FIGS) I: Detection Method and Catalog
• A new type of Neutrino Detector for Sterile Neutrino Search at Nuclear Reactors and Nuclear Nonproliferation Applications
• Higgs mass 125 GeV and g-2 of the muon in Gaugino Mediation Model
• The cancellation mechanism in the predictions of electric dipole moments
• What galaxy masses perturb the local cosmic expansion?
• Review on Effects of Long-lived Negatively Charged Massive Particles on Big Bang Nucleosynthesis
• Traversable $\ell$-wormholes supported by ghost scalar fields
• Observational constraints on quintessence models of dark energy
• Constraining the mass of fermionic dark matter from its feeble interaction with hadronic matter via dark mediators in neutron stars
• A quasar hiding behind two dusty absorbers. Quantifying the selection bias of metal-rich, damped Lyman-alpha absorption systems
• Gravitational waves carry information beyond effective spin parameters but it is hard to extract
• Cosmic clocks: A Tight Radius - Velocity Relationship for HI-Selected Galaxies
• Empirical multi-wavelength prediction method for very high energy gamma-ray emitting BL Lacs
• Understanding large-scale structure in the SSA22 protocluster region using cosmological simulations
• GRB 110715A: The peculiar multiwavelength evolution of the first afterglow detected by ALMA
• An accurate determination of the Hubble constant from Baryon Acoustic Oscillation datasets
• The impact of ionizing radiation on the formation of a supermassive star in the early Universe
• Median statistics cosmological parameter values
• Scalar and vector perturbations in a universe with discrete and continuous matter sources
• Detection prospects of light NMSSM Higgs pseudoscalar via cascades of heavier scalars from vector boson fusion and Higgs-strahlung
• Holographic approach for dark energy - dark matter interaction in curved FLRW spacetime
• Probing Large Extra Dimensions With IceCube
• Dark sectors of the Universe: A Euclid survey approach
• The stellar mass function and star formation rate-stellar mass relation of galaxies at z ~ 4 - 7
• The NEWFIRM HETDEX Survey: Photometric Catalog and a Conservative Sample of Massive Quiescent Galaxies at z=3-5 over 17.5 deg^2 in the SHELA Field
• The stellar mass in and around isolated central galaxies: connections to the total mass distribution through galaxy-galaxy lensing in the Hyper Suprime-Cam survey
• SUSY-QCD corrections for the direct detection of neutralino dark matter and correlations with the relic density
• Constraining Inert Triplet Dark Matter by the LHC and FermiLAT
• Weak lensing calibration of mass bias in the REFLEX+BCS X-ray galaxy cluster catalogue
• Practical Cosmology with Lenses
• Black hole accretion discs and screened scalar hair
• Galaxy Formation Efficiency and the Multiverse Explanation of the Cosmological Constant with EAGLE Simulations
• Estimating sizes of faint, distant galaxies in the submillimetre regime
• On the radial acceleration relation of $\Lambda$CDM satellite galaxies
• Velocity dispersion and dynamical mass for 270 galaxy clusters in the Planck PSZ1 catalogue
• A new pressure-parametrization unified dark fluid model
• Lepton-portal Dark Matter in Hidden Valley model and the DAMPE recent results
• The interconnection between galaxy mergers, AGN activity and rapid quenching of star formation in simulated post-merger galaxies
• A Three-loop Neutrino Mass Model with a Colored Triplet Scalar
• Limits on non-canonical heating and turbulence in the intergalactic medium from the low redshift Lyman-alpha forest
• The galaxy morphology-density relation in the EAGLE simulation
• Heavy dark matter particle annihilation in dwarf spheroidal galaxies: radio signals at the SKA telescope
• Predictions of a model of weak scale from dynamical breaking of scale invariance
• Cosmological dynamics of gravitating hadron matter
• A Multiwavelength Study of ELAN Environments (AMUSE${}^2$): Detection of a dusty star-forming galaxy within the enormous Lyman $\alpha$ nebula at $z=2.3$ sheds light on its origin
• Early dark energy and its interaction with dark matter
• Dark Matter on Top
• DESCQA: An Automated Validation Framework for Synthetic Sky Catalogs
• Dark-photon searches via $ZH$ production at $e^{+}{e}^{-}$ colliders
• Testing CPT Symmetry with Current and Future CMB Measurements
• Ghost condensates and pure kinetic $k$-essence condensates in presence of field-fluid non-minimal coupling in the dark sector
• EDGE: The emergence of dwarf galaxy scaling relations from cosmological radiation-hydrodynamics simulations
• Constraint on the primordial gravitational waves from the joint analysis of BICEP2 and Planck HFI 353 GHz dust polarization data
• A cosmological exclusion plot: Towards model-independent constraints on modified gravity from current and future growth rate data
• Central Mass Profiles of the Nearby Cool-core Galaxy Clusters Hydra A and A478
• Pulse-wise Amati correlation in Fermi GRBs
• 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
• Shedding Light on Dark Matter and Neutrino Interactions from Cosmology
• LEKID sensitivity for space applications between 80 and 600 GHz
• Euler-Heisenberg black hole surrounded by quintessence in the background of perfect fluid dark matter: Thermodynamics, Shadows and Quasinormal modes
• Dark Matter in the Higgs Triplet Model
• Cosmological Constant Problem and Renormalized Vacuum Energy Density in Curved Background
• Partitioning the universe into gravitational basins using the cosmic velocity field
• From dwarf galaxies to galaxy clusters: Self-Interacting Dark Matter over 7 orders of magnitude in halo mass
• KiDS+GAMA: The weak lensing calibrated stellar-to-halo mass relation of central and satellite galaxies
• Litmus Test for Cosmic Hemispherical Asymmetry in the Cosmic Microwave Background B-mode polarization
• Cosmology with non-minimal coupled gravity: inflation and perturbation analysis
• Is the baryon acoustic oscillation peak a cosmological standard ruler?
• Survival of pq-superstrings in field theory simulations
• Surrogate modelling the Baryonic Universe II: on forward modelling the colours of individual and populations of galaxies
• Minimal plateau inflationary cosmologies and constraints from reheating
• Skewon field and cosmic wave propagation
• IceCube potential for detecting Q-ball dark matter in gauge mediation
• Constraining gravity at large scales with the 2MASS Photometric Redshift catalogue and Planck lensing
• Charm decay in slow-jet supernovae as the origin of the IceCube ultra-high energy neutrino events
• The Supersymmetric Standard Models with a Pseudo-Dirac Gluino from Hybrid $F-$ and $D-$Term Supersymmetry Breakings
• The mass-metallicity relation as a ruler for galaxy evolution: insights from the James Webb Space Telescope
• The Astrophysics of the Intracluster Plasma
• On the Prevalence of Super-Massive Black Holes over Cosmic Time
• Galaxies with monstrous black holes in galaxy cluster environments
• 3.5 keV X-ray line and R-Parity Conserving Supersymmetry
• Matter Quantum Corrections to the Graviton Self-Energy and the Newtonian Potential
• Disformal vectors and anisotropies on a warped brane
• Exploring extensions to the standard cosmological model and the impact of baryons on small scales
• H-ATLAS/GAMA: Quantifying the Morphological Evolution of the Galaxy Population Using Cosmic Calorimetry
• SEAGLE--II: Constraints on feedback models in galaxy formation from massive early type strong lens galaxies
• DAMPE Electron-Positron Excess in Leptophilic $Z^{\prime }$ model
• Black hole formation and growth with non-Gaussian primordial density perturbations
• Effective equation of state in modified gravity and observational constraints
• Joint Analysis of Galaxy-Galaxy Lensing and Galaxy Clustering: Methodology and Forecasts for DES
• Observational Constraints on Varying-alpha Domain Walls
• Planck-PR4 anisotropy spectra show (better) consistency with General Relativity
• Graviton Creation by Small Scale Factor Oscillations in an Expanding Universe
• Multicomponent Dark Matter in Radiative Seesaw Models
• Jet-accretion system in the nearby mJy Radio Galaxies
• How identifying circumgalactic gas by line-of-sight velocity instead of the location in 3D space affects O VI measurements
• The impact of filamentary accretion of subhaloes on the shape and orientation of haloes
• Cosmological acceleration
• Status of Neutrino Mass and Mixing
• Looking for dark matter trails in colliding galaxy clusters
• Delay Spectrum with Phase-Tracking Arrays: Extracting the HI power spectrum from the Epoch of Reionization
• Kasner solutions, climbing scalars and big-bang singularity
• Connecting cosmological accretion to strong Lyman-alpha absorbers
• Evidence of extended cold molecular gas and dust halos around $\mathbf{z}\sim 2.3$ Extremely Red Quasars with ALMA
• Loop suppressed light fermion masses with $U(1{)}_R$ gauge symmetry
• Impact of Charge Trapping on the Energy Resolution of Ge Detectors for Rare-Event Physics Searches
• Constraints on Majorana Dark Matter from the LHC and IceCube
• Correspondence of I- and Q-balls as Non-relativistic Condensates
• Exploiting synergies between JWST and cosmic 21-cm observations to uncover star formation in the early Universe
• Accelerating anisotropic cosmologies in Brans-Dicke gravity coupled to a mass-varying vector field
• ROGER: Reconstructing Orbits of Galaxies in Extreme Regions using machine learning techniques
• The survival of globular clusters in a cuspy Fornax
• The assembly bias of emission line galaxies
• Cosmological foundations revisited with Pantheon+
• Cosmic flow around local massive galaxies
• Gamma-ray constraints on dark-matter annihilation to electroweak gauge and Higgs bosons
• Neutralino Dark Matter with Light Staus
• S-PLUS DR1 galaxy clusters and groups catalogue using PzWav
• Axions as Hot and Cold Dark Matter
• Assembly of the Intracluster Light in the Horizon-AGN Simulation
• Steep extinction towards GRB 140506A reconciled from host galaxy observations: Evidence that steep reddening laws are local
• Two radiative inverse seesaw models, dark matter, and baryogenesis
• EDGE: A new approach to suppressing numerical diffusion in adaptive mesh simulations of galaxy formation
• Observational constraints on the generalized $\alpha$ attractor model
• A scale dependent bias on linear scales: the case for HI intensity mapping at z=1
• A stable flat universe with variable Cosmological constant in f(R,T) Gravity
• Cosmology with velocity dispersion counts: an alternative to measuring cluster halo masses
• Constraints on the exponential $f(R)$ model from latest Hubble parameter measurements
• Phenomenology of neutrinoless double beta decay
• Discovery of $\gamma$-ray emission from the radio-intermediate quasar III Zw 2: violent jet activity with intraday $\gamma$-ray variability
• Cold dark energy constraints from the abundance of galaxy clusters
• Dark Matter 2014
• Neutrino mass sensitivity by MAC-E-Filter based time-of-flight spectroscopy with the example of KATRIN
• Extreme value statistics of weak lensing shear peak counts
• Vector Boson Fusion Searches for Dark Matter at the LHC
• Cosmology with decaying cosmological constant -- exact solutions and model testing
• No evidence for dynamical dark energy in two models
• Late time sky as a probe of steps and oscillations in primordial Universe
• Improving Hickson-like compact group finders in redshift surveys: an implementation in the SDSS
• Inflationary gravitational waves in the effective field theory of modified gravity
• The large-scale 21-cm power spectrum from reionization
• The general property of dynamical quintessence field
• On the change of old neutron star masses with galactocentric distance
• Compactly supported linearised observables in single-field inflation
• Protocluster detection in simulations of HSC-SSP and the 10-year LSST forecast, using PCcones
• Scalar perturbation in warm tachyon inflation in LQC in light of Plank and BICEP2
• Improving models of the cosmic infrared background using CMB lensing mass maps
• The galaxy-galaxy strong lensing cross-sections of simulated LCDM galaxy clusters
• Effect of asphericity in caustic mass estimates of galaxy clusters
• Universe acceleration in modified gravities: $F(R)$ and $F(T)$ cases
• Little Blue Dots in the Hubble Space Telescope Frontier Fields: Precursors to Globular Clusters?
• Turning Around along the Cosmic Web
• The Kiselev solution in power-Maxwell electrodynamics
• 21cm Signal Recovery via the Robust Principle Component Analysis
• Common Origin of 3.55 keV X-Ray Line and Galactic Center Gamma Ray Excess in a Radiative Neutrino Mass Model
• A separate universe view of the asymmetric sky
• Testing $f(R)$ Gravity With Scale Dependent Cosmic Void Velocity Profiles
• Hybrid Textures of the Right-Handed Majorana Neutrino Mass Matrix
• Elementary Theorems Regarding Blue Isocurvature Perturbations
• Schwarzschild Black Hole Surrounded by Perfect Fluid Dark Matter in the presence of Quintessence Matter Field
• Phenomenological study of neutrino mass, dark matter and baryogenesis within the framework of minimal extended seesaw
• Toward an Optimal Sampling of Peculiar Velocity Surveys For Wiener Filter Reconstructions
• Cosmic microwave background anisotropies in the timescape cosmology
• Suzaku X-ray Observations of the Nearest Non-Cool Core Cluster, Antlia: Dynamically Young but with Remarkably Relaxed Outskirts
• How does the grouping scheme affect the Wiener Filter reconstruction of the local Universe?
• Higher order statistics of shear field: a machine learning approach
• The Fornax3D project: Environmental effects on the assembly of dynamically cold disks in Fornax cluster galaxies
• GB6 J2113+1121: A multi-wavelength flaring gamma-ray blazar temporally and spatially coincident with the neutrino event IceCube-191001A
• Radio Galaxy Zoo: Observational evidence for environment as the cause of radio source asymmetry
• A fully-spectroscopic triple-source-plane lens: the Jackpot completed
• Perspectives of direct Detection of supersymmetric Dark Matter in the NMSSM
• Towards resolving strongly-interacting dark sectors at colliders
• Power radiated by a binary system in a de Sitter Universe
• The late Universe with non-linear interaction in the dark sector: the coincidence problem
• Age Problem in Lemaitre-Tolman-Bondi Void Models
• Testing supersymmetric Higgs inflation with non-Gaussianity
• Solving the muon g-2 anomaly in deflected AMSB with messenger-matter interactions
• Light Sterile Neutrinos and Inflationary Freedom
• Distortion of the luminosity function of high-redshift galaxies by gravitational lensing
• Tachyon-Warm Intermediate and Logamediate Inflation in the Brane-World Model in the Light of Planck Data
• Strong gravitational lensing as a tool to investigate the structure of jets at high energies
• An Improved Diffuse Foreground Subtraction by ILC method: CMB Map and Angular Power Spectrum using Planck and WMAP Observations
• Pushing down the low-mass halo concentration frontier with the Lomonosov cosmological simulations
• Dissipative dark matter and the rotation curves of dwarf galaxies
• Starobinsky Model in N=2 Supergravity
• A search for low-energy neutrino and antineutrino signals correlated with gamma-ray bursts with Borexino
• Partially Composite Dark Matter
• Does jackknife scale really matter for accurate large-scale structure covariances?
• The buildup of galaxies and their spheroids: the contributions of mergers, disc instabilities and star formation
• Precise probing of the inert Higgs-doublet model at the LHC
• Higgsino Dark Matter in Nonuniversal Gaugino Mass Models
• What is the amplitude of the Gravitational Waves background expected in the Starobinsky model ?
• Radio Polarization Properties of Quasars and Active Galaxies at High Redshifts
• Linear perturbations in K-mouflage cosmologies with massive neutrinos
• MultiDark-Clusters: Galaxy Cluster Mock Light-Cones, eROSITA and the Cluster Power Spectrum
• A case study for measuring the relativistic dipole of a galaxy cross-correlation with the Dark Energy Spectroscopic Instrument
• Properties and merger signatures of galaxies hosting LISA coalescing massive black hole binaries
• SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES) IV: Spatial clustering and halo masses of 450-$\mu$m-selected sub-millimeter galaxies
• Baryon Number as the Fourth Color
• The stepping-stone sampling algorithm for calculating the evidence of gravitational wave models
• Analysis of Sunyaev-Zel'dovich Effect Mass-Observable Relations using South Pole Telescope Observations of an X-ray Selected Sample of Low Mass Galaxy Clusters and Groups
• The HI absorption zoo: JVLA extension to $z\sim 0.4$
• Tracing stars in Milky Way satellites with A-SLOTH
• Testing Lambda and the Limits of Cosmography with the Union2.1 Supernova Compilation
• Production of heavy sterile neutrinos from vector boson decay at electroweak temperatures
• Constraints on features in the inflationary potential from future Euclid data
• ETHOS - an effective theory of structure formation: formation of the first haloes and their stars
• Halo models of HI selected galaxies
• Dark Matter Signals in Dilepton Production at Hadron Colliders
• Models with Extended Higgs Sectors at Future $e^{+}{e}^{-}$ Colliders
• Conformal Standard Model, Leptogenesis and Dark Matter
• Generating the cosmic microwave background power asymmetry with $g_{NL}$
• Resonant bar detector constraints on macro dark matter
• Maturing Satellite Kinematics into a Competitive Probe of the Galaxy-Halo Connection
• Discriminating Majorana Neutrino Textures in the light of Baryon Asymmetry
• Unraveling the interplay between SIDM and baryons in MW halos: defining where baryons dictate heat transfer
• Magneto-optic effects of the Cosmic Microwave Background
• Standard Big-Bang Nucleosynthesis after Planck
• Mass and size growth of early-type galaxies by dry mergers in cluster environments
• Designing and testing inflationary models with Bayesian networks
• High-scale validity of a model with Three-Higgs-doublets
• The $z\lesssim 1$ drop of cosmic dust abundance in a semi-analytic framework
• Freeze-in production of Fermionic Dark Matter with Pseudo-scalar and Phenomenological Aspects
• Fermionic influence (action) on inflationary fluctuations
• Planck intermediate results. XLI. A map of lensing-induced B-modes
• The mass-size plane of EAGLE galaxies
• The trajectories of galaxies in groups: mass loss and preprocessing
• Improving cosmological parameter estimation with the future 21 cm observation from SKA
• Minimal predictive see-saw model with normal neutrino mass hierarchy
• Grand Unification and Subcritical Hybrid Inflation
• Electroweak versus high scale finetuning in the 19-parameter SUGRA model
• Detection and classification of supernovae beyond z~2 redshift with the James Webb Space Telescope
• Dark energy versus modified gravity: Impacts on measuring neutrino mass
• Local photoionization feedback effects on galaxies
• Seeding supermassive black holes with a non-vortical dark-matter subcomponent
• Geodesic "curve"-of-sight formulae for the cosmic microwave background: a unified treatment of redshift, time delay, and lensing
• Unified Framework for Matter, Dark Matter, and Radiative Neutrino Mass
• Distinctive 21 cm structures of the first stars, galaxies, and quasars
• Inert doublet as multicomponent dark matter
• The dearth of difference between central and satellite galaxies II. Comparison of observations with L-GALAXIES and EAGLE in star formation quenching
• Reconstructing G-inflation: From the attractors $n_S(N)$ and $r(N)$
• A novel CMB polarization likelihood package for large angular scales built from combined WMAP and Planck LFI legacy maps
• The changing circumgalactic medium over the last 10 Gyr I: physical and dynamical properties
• Reconciling low multipole anomalies and reheating in single field inflationary models
• The evolution of the baryon fraction in halos as a cause of scatter in the galaxy stellar mass in the EAGLE simulation
• $Fermi$-LAT detection of a transient $\gamma$-ray source in the direction of a distant blazar B3 1428+422 at $z=4.72$
• External Enrichment of Minihalos by the First Supernovae
• Inflation that runs naturally: Gravitational waves and suppression of power at large and small scales
• CMB hemispherical asymmetry from non-linear isocurvature perturbations
• The QuaStar Survey: Detecting Hidden Low-Velocity Gas in the Milky Way's Circumgalactic Medium
• Magnification bias as a novel probe for primordial magnetic fields
• Indirect Probes of Dark Matter and Globular Cluster Properties From Dark Matter Annihilation within the Coolest White Dwarfs
• Lack-of-correlation anomaly in CMB large scale polarisation maps
• Origin and growth of primordial black holes
• The HI-halo mass relation at redshift $z\sim 1$ from the Minkowski functionals of 21 cm intensity maps
• Structure Growth and the CMB in Modified Gravity (MOG)
• Statistics of Anisotropies in Inflation with Spectator Vector Fields
• Raytracing simulations of coupled dark energy models
• Scalar dark matter explanation of the DAMPE data in the minimal Left-Right symmetric model
• Modeling the large-scale power deficit with smooth and discontinuous primordial spectra
• Effects of Curvature-Higgs Coupling on Electroweak Fine-Tuning
• Hidden $U(1)$ gauge symmetry realizing a neutrinophilic two-Higgs-doublet model with dark matter
• Structure and dynamics in low density regions: galaxy-galaxy correlations inside cosmic voids
• Little composite dark matter
• Cosmological observables in multi-field inflation with a non-flat field space
• Compensation for large tensor modes with iso-curvature perturbations in CMB anisotropies
• Model-Independent Measurements of Cosmic Expansion and Growth at z=0.57 Using the Anisotropic Clustering of CMASS Galaxies From the Sloan Digital Sky Survey Data Release 9
• Is the CNMSSM more credible than the CMSSM?
• Singlet extension of the MSSM as a solution to the small cosmological scale anomalies
• Lightness of Higgs Boson and Spontaneous CP Violation in Lee Model
• Dynamics of viscous cosmologies in the full Israel-Stewart formalism
• Patient Observers and Non-perturbative Infrared Dynamics in Inflation
• Small scale clustering of late forming dark matter
• General dynamical properties of cosmological models with nonminimal kinetic coupling
• New constraints on cosmic polarization rotation from the ACTPol cosmic microwave background B-Mode polarization observation and the BICEP2 constraint update
• Measuring weak lensing correlations of Type Ia Supernovae
• On the impact of large angle CMB polarization data on cosmological parameters
• Spiral Inflation with Coleman-Weinberg Potential
• More Is Different: Reconciling eV Sterile Neutrinos with Cosmological Mass Bounds
• The impact of protocluster environments at z = 1.6
• Astrophysical interpretation of the anisotropies in the unresolved gamma-ray background
• Testing Type II Radiative Seesaw Model: from Dark Matter Detection to LHC Signatures
• Some observational tests of a minimal galaxy formation model
• Constraints on the cosmological parameters with three-parameter correlation of Gamma-ray bursts
• On the consistency of tachyon warm inflation with viscous pressure
• Imprint of Inhomogeneous and Anisotropic Primordial Power Spectrum on CMB Polarization
• Two fluid anisotropic dark energy models in a scale invariant theory
• Consistency of the Planck CMB data and $\Lambda$CDM cosmology
• Muon g-2 in Anomaly Mediated SUSY Breaking
• Anisotropic cosmological models with two fluids
• Insights into neutrino decoupling gleaned from considerations of the role of electron mass
• A Non-minimally Coupled Potential for Inflation and Dark Energy after Planck 2015: A Comprehensive Study
• Cosmological implications of the composite spectra of galactic X-ray binaries constructed using MAXI data
• Fruitbat: A Python Package for Estimating Redshifts of Fast Radio Bursts
• What do the cosmological supernova data really tell us?
• Primordial Power Spectrum features and $f_{NL}$ constraints
• Dark matter protohalos in MSSM-9 and implications for direct and indirect detection
• The cosmic spectral energy distribution in the EAGLE simulation
• Testing a model for subphotospheric dissipation in GRBs: fits to Fermi data constrain the dissipation scenario
• Recent results in nuclear astrophysics
• Constraining the mass density of free-floating black holes using razor-thin lensing arcs
• Rational nonlinear electrodynamics causes the inflation of the universe
• SImulator of GAlaxy Millimetre/submillimetre Emission (SIGAME): CO emission from massive z=2 main-sequence galaxies
• A Complete Cosmological Scenario in Teleparallel Gravity
• Improving spectroscopic lithium abundances. Fitting functions for 3D non-LTE corrections in FGK stars of different metallicity
• A Proposed Experimental Search for Chameleons using Asymmetric Parallel Plates
• Light Higgs Bosons in NMSSM at the LHC
• Scaling relations for globular cluster systems in early-type galaxies. II. Is there an environmental dependence?
• Cold and Hot gas distribution around the Milky-Way-M31 system in the HESTIA simulations
• Positive or Negative? The Impact of X-ray Feedback on the Formation of Direct Collapse Black Hole Seeds
• Bouncing Universes in Scalar-Tensor Gravity Around Conformal Invariance
• A no-go theorem for monodromy inflation
• An Intermediate Type Ia Supernova Between Normal And Super-Chandrasekhar
• Dark matter candidates in the constrained Exceptional Supersymmetric Standard Model
• Sharp inflaton potentials and bi-spectra: Effects of smoothening the discontinuity
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• Quasar clustering in a galaxy and quasar formation model based on ultra high-resolution N-body simulations
• Scalar Field as a Bose-Einstein Condensate?
• Snowmass-2013 Cosmic Frontier 3 (CF3) Working Group Summary: Non-WIMP dark matter
• Primordial non-Gaussianities in single field inflationary models with non-trivial initial states
• Magnetic reheating
• Universe opacity and CMB
• Structure formation in a mixed dark matter model with decaying sterile neutrino: the 3.5 keV X-ray line and the Galactic substructure
• Discovery of a lensed ultrabright submillimeter galaxy at z=2.0439
• Constraints on a possible evolution of mass density power-law index in strong gravitational lensing from cosmological data
• Dirac field as a source of the inflation in 2+1 dimensional Teleparallel gravity
• Casting Light on BSM Physics with SM Standard Candles
• Large tensor-to-scalar ratio and running of the scalar spectral index with Instep Inflation
• Perfect fluid and F(T) gravity descriptions of inflationary universe and comparison with obervational data
• From Cosmicflows distance moduli to unbiased distances and peculiar velocities
• Measurement of Muon Annual Modulation and Muon-Induced Phosphorescence in NaI(Tl) Crystals with DM-Ice17
• The impact of dark energy on galaxy formation. What does the future of our Universe hold?
• Relationship between the CMB, SZ Cluster Counts, and Local Hubble Parameter Measurements in a Simple Void Model
• Majorana Dark Matter in a new B-L model
• MaNGA galaxy properties -- II. A detailed comparison of observed and simulated spiral galaxy scaling relations
• The Diversity of Growth Histories of Milky Way-mass Galaxies
• Evolution of vacuum fluctuations generated during and before inflation
• On Nonlocal Modified Gravity and its Cosmological Solutions
• Constraining Type I Seesaw with $A_4$ Flavor Symmetry From Neutrino Data and Leptogenesis
• An accurate method of modeling cluster scaling relations in modified gravity
• Proton decay and new contribution to neutrino-less double beta decay in SO(10) with low-mass Z-prime boson, observable n-nbar oscillation, lepton flavor violation, and rare kaon decay
• Dynamical D-Terms in Supergravity
• Natural Inflation from Near Alignment in Heterotic String Theory
• Searching for primordial black holes with stochastic gravitational-wave background in the space-based detector frequency band
• 1000 days of lowest frequency emission from the low-luminosity GRB 171205A
• Revisiting the [C II]${}_{158\mu \text{m}}$ line-intensity mapping power spectrum from the EoR using non-uniform line-luminosity scatter
• Current constraints on early and stressed dark energy models and future 21 cm perspectives
• Clumpy galaxies in cosmological simulations: The effect of ISM model
• Tidal Stripping and Post-Merger Relaxation of Dark Matter Halos: Causes and Consequences of Mass Loss
• The Kullback-Leibler Divergence as an Estimator of the Statistical Properties of CMB Maps
• The SRG/eROSITA All-Sky Survey : Constraints on the structure growth from cluster number counts
• Faint Satellite Population of the NGC-3175 Group - a Local Group Analogue
• The Swampland Conjectures and Slow-Roll Thawing Quintessence
• Phantom crossing dark energy in Horndeski's theory
• G-Warm inflation
• Virial halo mass function in the $Planck$ cosmology
• The cosmic web around the Coma cluster from constrained cosmological simulations: I. Filaments connected to Coma at $z=0$
• The supermassive black hole masses of reverberation-mapped active galactic nuclei
• Comparison of cosmological models using standard rulers and candles
• Validation of Selection Function, Sample Contamination and Mass Calibration in Galaxy Cluster Samples
• Revisiting the Galaxy Shape and Spin Alignments with the Large-Scale Tidal Field: An Effective Practical Model
• Scalar coupling limits and diphoton Higgs decay from LHC in an $U(1{)}^{\prime }$ model with scalar dark matter
• Dark Energy Constraints in light of Pantheon SNe Ia, BAO, Cosmic Chronometers and CMB Polarization and Lensing Data
• Cepheid Variables in the Maser-Host Galaxy NGC 4258
• Flavored leptogenesis with quasi degenerate neutrinos in a broken cyclic symmetric model
• A Model-independent Method to Determine $H_0$ Using Time-Delay Lensing, Quasars and Type Ia Supernovae
• The Not-So-Sterile 4th Neutrino: Constraints on New Gauge Interactions from Neutrino Oscillation Experiments
• Spectral distortions in the cosmic microwave background polarization
• Planck Trispectrum Constraints on Primordial Non-Gaussianity at Cubic Order
• Combined constraints on deviations of dark energy from an ideal fluid from Euclid and Planck
• BeyondPlanck XII. Cosmological parameter constraints with end-to-end error propagation
• Effective Theories with Dark Matter Applications
• Probing the NMSSM via Higgs boson signatures from stop cascade decays at the LHC
• The abundance of dark matter haloes down to Earth mass
• Measuring Linear and Non-linear Galaxy Bias Using Counts-in-Cells in the Dark Energy Survey Science Verification Data
• Torsion as a Dark Matter Candidate from the Higgs Portal
• Neutron Beam Tests of $CsI(Na)$ and $Ca{F}_2(Eu)$ Crystals for Dark Matter Direct Search
• Direct-collapse black hole formation induced by internal radiation of host halos
• Constraints on dark energy models from the Horndeski theory
• A study on a minimally broken residual TBM-Klein symmetry with its implications on flavoured leptogenesis and ultra high energy neutrino flux ratios
• FERMI transient J1544-0649: a flaring radio-weak BL Lac
• Breaking through the high redshift bottleneck of Observational Hubble parameter Data: The Sandage-Loeb signal Scheme
• The Smith Cloud: surviving a high speed transit of the Galactic disc
• Stability of the Einstein static Universe in Einstein-Cartan-Brans-Dicke gravity
• Scaling ansatz with texture zeros in linear seesaw
• EDGE: Dark matter core creation depends on the timing of star formation
• Naturalness redux
• Deriving the star formation histories of galaxies from spectra with simulation-based inference
• Dynamical system approach to running $\Lambda$ cosmological models
• On Scale-Dependent Cosmic Shear Systematic Effects
• EDGE: The shape of dark matter haloes in the faintest galaxies
• Hunting for Metals Using XQ-100 Legacy Survey Composite Spectra
• Testing distance duality with CMB anisotropies
• $f(T)$ non-linear massive gravity and the cosmic acceleration
• Reconstructing the Local Potential of Inflation with BICEP2 data
• Bubble mapping with the Square Kilometer Array -- I. Detecting galaxies with Euclid, JWST, WFIRST and ELT within ionized bubbles in the intergalactic medium at z>6
• A unified composite model of inflation and dark matter in the Nambu-Jona-Lasinio theory
• The XXL Survey: XXXVII. The role of the environment in shaping the stellar population properties of galaxies at 0.1<z<0.5
• HAT-TR-318-007: a double-lined M-dwarf binary with total secondary eclipses discovered by HATNet and observed by K2
• Reducing the Variance of Redshift Space Distortion Measurements from Mock Galaxy Catalogues with Different Lines of Sight
• Beyond the growth rate of cosmic structure: Testing modified gravity models with an extra degree of freedom
• Revised estimates of CMB $B$-mode polarization induced by patchy reionization
• The Radcliffe Wave as the gas spine of the Orion Arm
• Example of an inhomogeneous cosmological model in the context of backreaction
• Generating $\fnl$ at $\ell\lsim 60$
• The XXL Survey XIX. A realistic population of simulated X-ray AGN: Comparison of models with observations
• Gravitational Waves: A Test for Modified Gravity
• Cosmology through arc statistics I: sensitivity to ${\Omega }_m$ and ${\sigma }_8$
• The Origin of Lopsided Satellite Galaxy Distribution in Galaxy Pairs
• Finite time future singularities in the interacting dark sector
• Dark Matter Annihilation into Four-Body Final States and Implications for the AMS Antiproton Excess
• Unveiling the hosts of parsec-scale massive black hole binaries: morphology and electromagnetic signatures
• Determining $H_0$ with the latest HII galaxy measurements
• Cosmological Constraints on Ghost Dark Energy in the Brans-Dicke Theory by Using MCMC Approach
• Strong Hydrogen Absorption at Cosmic Dawn: the Signature of a Baryonic Universe
• Late-end reionization with ATON-HE: towards constraints from Lyman-$\alpha$ emitters observed with JWST
• Constraints on the dark matter sound speed from galactic scales: the cases of the Modified and Extended Chaplygin Gas
• Non-Canonical Inflation in Supergravity
• Gravitational, shear and matter waves in Kantowski-Sachs cosmologies
• Generic inference of inflation models by non-Gaussianity and primordial power spectrum reconstruction
• Growth of perturbations in nonlocal gravity with non-$\Lambda$CDM background
• Can SKA--Phase 1 go much beyond the LHC in supersymmetry search?
• The stellar mass function and evolution of the density profile of galaxy clusters from the Hydrangea simulations at $0<z<1.5$
• Exact Scalar-Tensor Cosmological Models
• Absolute Distances to Nearby Type Ia Supernovae via Light Curve Fitting Methods
• Rosella: A mock catalogue from the P-Millennium simulation
• Galaxy clustering at cosmic dawn from JWST/NIRCam observations to redshift z$\sim$11
• Simulating the LOcal Web (SLOW) II: Properties of local galaxy clusters
• The Ultraviolet Detection of Diffuse Gas in Galaxy Groups
• Internal dark matter structure of the most massive galaxy clusters
• Galaxy bias from galaxy-galaxy lensing in the DES Science Verification Data
• Estimating the Turn-Around Radii of Six Isolated Galaxy Groups in the Local Universe
• Constraints on $f(R)$ and nDGP Modified Gravity Model Parameters with Cluster Abundances and Galaxy Clustering
• Resolving the issue of branched Hamiltonian in modified Lanczos-Lovelock gravity
• Type Ia supernovae data with scalar-tensor gravity
• CMB probes on the correlated axion isocurvature perturbation
• Chaotic inflation with curvaton induced running
• Cuscuta-Galileon cosmology: Dynamics, gravitational "constant"s and the Hubble Constant
• Reduced Lagrangians and analytic solutions in Einstein-æther Cosmology
• The Tiered Radio Extragalactic Continuum (T-RECS) simulation II: HI emission and continuum-HI cross-correlation
• Hybrid Textures of Neutrino Mass Matrix under the Lamppost of Latest Neutrino and Cosmology Data
• The phenomenological MSSM in view of the 125 GeV Higgs data
• Statistical recovery of the BAO scale from multipoles of the beam-convolved 21cm correlation function
• The Baryonic Collapse Efficiency of Galaxy Groups in the RESOLVE and ECO Surveys
• Initializing adaptive importance sampling with Markov chains
• The Inert Doublet Model and its extensions
• A Novel Statistical Method for Measuring the Temperature-Density Relation in the IGM Using the $b$-$N_{\text{HI}}$ Distribution of Absorbers in the Ly$\alpha$ Forest
• Higgs Coupling Measurements and Direct Searches as Complementary Probes of the pMSSM
• The Dearth of Difference between Central and Satellite Galaxies III. Environmental Dependence of Mass-Size and Mass-Structure Relations
• Higgs vacuum stability and inflationary dynamics after BICEP2 and PLANCK dust polarisation data
• The potential role of NGC 205 in generating Andromeda's vast thin co-rotating plane of satellite galaxies
• The cross-correlation between 3d cosmic shear and the integrated Sachs-Wolfe effect
• The edge of galaxy formation III: The effects of warm dark matter on Milky Way satellites and field dwarfs
• Red, Straight, no bends: primordial power spectrum reconstruction from CMB and large-scale structure
• Dark Matter in Split SUSY with Intermediate Higgses
• The mass profile and dynamical status of the z~0.8 galaxy cluster LCDCS 0504
• Effective Dark Matter Halo catalog in $f(R)$ gravity
• A Semi-blind PCA-based Foreground Subtraction Method for 21 cm Intensity Mapping
• Constraining particle dark matter using local galaxy distribution
• MgII 2797, 2803 emission in a large sample of low-metallicity star-forming galaxies from SDSS DR14
• The quest for neutrinoless double beta decay: Pseudo-Dirac, Majorana and sterile neutrinos
• Cosmologically probing ultra-light particle dark matter using 21 cm signals
• Dark Matter from a Vector Field in the Fundamental Representation of $SU(2{)}_L$
• Vector dark energy models with quadratic terms in the Maxwell tensor derivatives
• The Robustness of Cosmological Hydrodynamic Simulation Predictions to Changes in Numerics and Cooling Physics
• Stochastic background of gravitational waves from cosmological sources
• Gravitational Wave Opacity from Gauge Field Dark Energy
• Mass Functions, Luminosity Functions, and Completeness Measurements from Clustering Redshifts
• Inflation including collapse of the wave function: The quasi-de Sitter case
• The Hidden Flat Like Universe II: Quasi inverse power law inflation by $f(T)$ gravity
• A comparison between axion-like and power law potentials in cosmological background
• Cosmological perturbations on the Phantom brane
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). The matter density and baryon fraction from the galaxy power spectrum at redshift $0.6<z<1.1$
• Extragalactic sources in Cosmic Microwave Background maps
• Confirmation of a cluster of galaxies hidden behind the Galactic bulge using the VVV Survey
• On the Trispectrum of Galileon Inflation
• Super-Natural MSSM
• The compatibility of LHC Run 1 data with a heavy scalar of mass around 270\,GeV
• Baryonic effects in cosmic shear tomography: PCA parametrization and importance of extreme baryonic models
• A split SUSY model from SUSY GUT
• Oscillation characteristics of active and sterile neutrinos and neutrino anomalies at shot distances
• Quasi Static Evolution of Compact Objects in Modified Gravity
• Testing the tensor-vector-scalar Theory with the latest cosmological observations
• Statistical properties of dark matter mini-haloes at z >= 15
• Linking the BICEP2 result and the hemispherical power asymmetry through spatial variation of $r$
• New model of axion monodromy inflation and its cosmological implications
• Halo Mass Definition and Multiplicity Function
• A new parametrization for dark energy density and future deceleration
• Multiscale mass transport in z~6 galactic discs: fueling black holes
• Rotation curves in Bose-Einstein Condensate Dark Matter Halos
• Dark matter in the $SO(5)\times U(1)$ gauge-Higgs unification
• Spatially resolved mock observations of stellar kinematics: full radiative transfer treatment of simulated galaxies
• Chameleon Field Dynamics During Inflation
• Instability in interacting dark sector: An appropriate Holographic Ricci dark energy model
• Bayesian analysis of CCDM Models
• Are dark energy models with variable EoS parameter $w$ compatible with the late inhomogeneous Universe?
• On dataset tensions and signatures of new cosmological physics
• Lower Bound on the Garvitino Mass $m_{3/2}>O(100)$ TeV in $R$-Symmetry Breaking New Inflation
• Prospects of Establishing the Origin of Cosmic Neutrinos using Source Catalogs
• Gravitational-wave constraints on scalar-tensor gravity from a neutron star and black-hole binary GW200115
• Can galaxy clusters, type Ia supernovae and cosmic microwave background rule out a class of modified gravity theories?
• Searching for a possible dipole anisotropy on acceleration scale with 147 rotationally supported galaxies
• Kinetic mixing and symmetry breaking dependent interactions of the dark photon
• Higgs Mass and Muon $g-2$ Anomaly in MSSM with Gauge-Gravity hybrid Mediation
• Axionic Dark Radiation and the Milky Way's Magnetic Field
• Predicting Structures in the Zone of Avoidance
• Neutrinoless double beta decay and lepton flavour violation in broken $\mu -\tau$ symmetric neutrino mass models
• Reconstructing k-essence: Unifying the attractor $n_S(N)$ and the swampland criteria
• On the kinetic Sunyaev-Zel'dovich effect as an observational probe for halo spin bias
• Stop Co-Annihilation in the Minimal Supersymmetric Standard Model Revisited
• Prospects of strongly lensed fast radio bursts: Simultaneous measurement of post-Newtonian parameter and Hubble constant
• Modelling the star-formation activity and ionizing properties of high-redshift galaxies
• Neutrino mass matrices with one texture equality and one vanishing neutrino mass
• LHC constraints on Gravitino Dark Matter
• Searching for Dark Matter Annihilation into Neutrinos with Super-Kamiokande
• Consistency of Pantheon+ supernovae with a large-scale isotropic universe
• On self-gravitating strange dark matter halos around galaxies
• Building a digital twin of a luminous red galaxy spectroscopic survey: galaxy properties and clustering covariance
• Probing CP-violating $h\bar{t}t$ coupling in $e^{+}{e}^{-}\to h\gamma$
• Target Neutrino Mass Precision for Determining the Neutrino Hierarchy
• CMB low multipole alignments in the $\mathbf{\Lambda }$CDM and Dipolar models
• The effect of secular galactic growth on the evolution of star clusters
• Fast magnetic field amplification in the early Universe: growth of collisionless plasma instabilities in turbulent media
• Is it possible to discover a dark matter particle with an accelerator?
• ALMA observations of super-early galaxies: attenuation-free model predictions
• Late time accelerated scaling attractors in DGP (Dvali-Gabadadze-Porrati) braneworld
• Test of consistency between Planck and WMAP
• Precision Predictions for the Primordial Power Spectra of Scalar Potential Models of Inflation
• Lyman-tomography of cosmic infrared background fluctuations with Euclid: probing emissions and baryonic acoustic oscillations at z>10
• Chemical analysis of very metal-poor turn-off stars from SDSS-DR12
• Pantheon+ constraints on dark energy and modified gravity: An evidence of dynamical dark energy
• Constraint on the radius of five-dimensional dS spacetime with GW170817 and GRB 170817A
• Effect of supersonic relative motion between baryons and dark matter on collapsed objects
• Diagnosing the interstellar medium of galaxies with far-infrared emission lines I. The [C II] 158 microns line at z~0
• Gamma-ray triangles: a possible signature of asymmetric dark matter in indirect searches
• Baryogenesis via Mesino Oscillations
• Size-Luminosity Scaling Relations of Local and Distant Star Forming Regions
• Viscous Self Interacting Dark Matter Cosmology For Small Redshift
• On the Form of the Spitzer Leavitt Law and its Dependence on Metallicity
• Supernova constraints on Multi-coupled Dark Energy
• Axially magnetized Dark Energy cosmological model
• How feedback shapes galaxies: an analytic model
• Cosmological tracking solution and the Super-Higgs mechanism
• Cosmological reconstruction and {\it Om} diagnostic analysis of Einstein-Aether Theory
• CFT driven cosmology and conformal higher spin fields
• Isocurvature perturbations and tensor mode in light of Planck and BICEP2
• Was Entropy Conserved between BBN and Recombination?
• Semi-blind Bayesian inference of CMB map and power spectrum
• Long-Lived stop at the LHC with or without R-parity
• Negative running prevents eternal inflation
• Momentum transfer in the dark sector and lensing convergence in upcoming galaxy surveys
• How gravitational lensing helps gamma-ray photons avoid $\gamma -\gamma$ absorption
• Development of a low-$\alpha$-emitting $\mu$-PIC as a readout device for direction-sensitive dark matter detectors
• Neutrino masses, the $\mu$-term and ${\mathcal{P}\mathcal{SL}}_2(7)$
• Supersymmetric Left-Right Model of Radiative Neutrino Mass with Multipartite Dark Matter
• Fermionic Dark Matter through a Light Pseudoscalar Portal: Hints from the DAMA Results
• Minimal Asymmetric Dark Matter
• Scalar Field Theory Description of the Running Vacuum Model: the Vacuumon
• Multi-fluid cosmology in Einstein gravity: analytical solutions
• Direct searches of Type III seesaw triplet fermions at high energy $e^{+}{e}^{-}$ collider
• Two-loop Induced Majorana Neutrino Mass in a Radiatively Induced Quark and Lepton Mass Model
• Constraining warm dark matter mass with cosmic reionization and gravitational wave
• Superconducting dark energy
• A novel approach to reconstructing signals of isotropy violation from a masked CMB sky
• Properties and observables of massive galaxies in self-interacting dark matter cosmologies
• Testing galaxy formation models with galaxy stellar mass functions
• New physics effects on neutrinoless double beta decay from right-handed current
• The Peculiar Velocity Correlation Function
• Modelling the next-to-leading order matter three-point correlation function using FFTLog
• Mass characteristics of active and sterile neutrinos in a phenomenological (3+1+2)-model
• Thawing quintessence from the inflationary epoch to today
• Turbulence in the SuperModel: Mass Reconstruction with Nonthermal Pressure for Abell 1835
• Smooth deformations and cosmic statefinders
• A giant galaxy in the young Universe with a massive ring
• Cross-Correlation of Near and Far-Infrared Background Anisotropies as Traced by Spitzer and Herschel
• 21 cm line signal from magnetic modes
• Cosmology based on $f(R)$ gravity with $\mathcal{O}(1)$ eV sterile neutrino
• Revised cosmological parameters after BICEP 2 and BOSS
• Hidden Local Symmetry and Beyond
• A Cosmic ALP Background and the Cluster Soft X-ray Excess in A665, A2199 and A2255
• The impact of baryons on the internal structure of dark matter haloes from dwarf galaxies to superclusters in the redshift range 0<z<7
• Testing Cosmology with Double Source Lensing
• Emulation of the Cosmic Dawn 21-cm Power Spectrum and Classification of Excess Radio Models Using an Artificial Neural Network
• Number Counts and Dynamical Vacuum Cosmologies
• Parkes transient events: I. Database of single pulses, initial results and missing FRBs
• Non-virialised clusters for detection of Dark Energy-Dark Matter interaction
• Luminosity Ratio between [O IV] 25.89 um Line and Nuclear Continuum 12 um as Diagnostic for "Buried" AGN
• Estimation of the masses in the Local Group by Gradient Boosted Decision Trees
• Possible evidence for a large-scale enhancement in the Lyman-$\alpha$ forest power spectrum at redshift $\text{z}\ge 4$
• Fast Radio Bursts and Artificial Neural Networks: a cosmological-model-independent estimation of the Hubble Constant
• Bayesian evidence of non-standard inflation: isocurvature perturbations and running spectral index
• Neutrino electromagnetic interactions: a window to new physics
• First comprehensive constraints on the Finslerian models using cosmological observations
• Perfect fluids with $\omega =\mathrm{const}$ as sources of scalar cosmological perturbations
• Anapole Dark Matter after DAMA/LIBRA-phase2
• Barrow entropic Quintessence and Dilation dark energy Models with Generalized HDE cut-off
• The simplest origin of the big bounce and inflation
• Constraints on small-scale cosmological fluctuations from SNe lensing dispersion
• The impact of temperature fluctuations on the large-scale clustering of the Ly$\alpha$ forest
• Probing the innermost regions of AGN jets and their magnetic fields with RadioAstron IV. The quasar 3C 345 at 18 cm: Magnetic field structure and brightness temperature
• Probing texture zeros with scaling ansatz in inverse seesaw
• Search for Dark Matter Gamma-ray Emission from the Andromeda Galaxy with the High-Altitude Water Cherenkov Observatory
• Non-oscillating Early Dark Energy and Quintessence from Alpha-Attractors
• Providing stringent star formation rate limits of z$\sim$2 QSO host galaxies at high angular resolution
• Loop induced type-II seesaw model and GeV dark matter with $U(1{)}_{B-L}$ gauge symmetry
• Consistency of cosmic microwave background temperature measurements in three frequency bands in the 2500-square-degree SPT-SZ survey
• Towards realistic $f(T)$ models with nonminimal torsion-matter coupling extension
• Differentiable Predictions for Large Scale Structure with SHAMNet
• Towards a realistic model of quarks and leptons, leptonic CP violation and neutrinoless $\beta \beta$-decay
• Corrected constraints on big bang nucleosynthesis in a modified gravity model of $f(R)\propto R^n$
• Reconstruction of the null-test for the matter density perturbations
• Lifshitz cosmology: quantum vacuum and Hubble tension
• Local Group Analogs in $\Lambda$CDM cosmological simulations
• Asteroseismic and orbital analysis of the triple star system HD 188753 observed by Kepler
• Plasma dark matter direct detection
• Simulating the Anisotropic Clustering of Luminous Red Galaxies with Subhalos: A Direct Confrontation with Observation and Cosmological Implications
• Anisotropic cosmology and inflation from tilted Bianchi IX model
• Pseudoscalar N-flation and axial coupling revisited
• Role of ionizing background on the statistics of metal absorbers in hydrodynamical simulations
• Mass models of gas-rich void dwarf galaxies
• Galaxy clustering measurements out to redshift z$\sim$8 from Hubble Legacy Fields
• Merger types forming the Virgo cluster in recent gigayears
• Future sensitivity of neutrino telescopes to dark matter annihilations from the cosmic diffuse neutrino signal
• Small field models with gravitational wave signature supported by CMB data
• Implications of the $z>5$ Lyman-$\alpha$ forest for the 21-cm power spectrum from the epoch of reionization
• Fractional chaotic inflation in the lights of PLANCK and BICEP2
• Spatial Curvature and Thermodynamics
• Clustering tomography: measuring cosmological distances through angular clustering in thin redshift shells
• Redshift evolution of the hot intracluster gas metallicity in the C-EAGLE cluster simulations
• Dark matter annihilation and the Galactic Centre Excess
• Probing Hot Gas Components of Circumgalactic Medium in Cosmological Simulations with the Thermal Sunyaev-Zel'dovich Effect
• Footprint of Triplet Scalar Dark Matter in Direct, Indirect Search and Invisible Higgs Decay
• Globular cluster metallicity distributions in the E-MOSAICS simulations
• Statistical Anisotropic Gaussian Simulations of the CMB Temperature Field
• On the sensitivity of present direct detection experiments to WIMP-quark and WIMP-gluon effective interactions: a systematic assessment and new model-independent approaches
• Eddington's Gravity in Immersed Spacetime
• Higgs inflation and cosmological electroweak phase transition with N scalars in the post-Higgs era
• Bayesian approach to constraining the properties of ionized bubbles during reionization
• Impact of cosmic filaments on the gas accretion rate of dark matter halos
• Constraining dark sector perturbations I: cosmic shear and CMB lensing
• 21-cm signatures of residual HI inside cosmic HII regions during reionization
• The effect of dark matter resolution on the collapse of baryons in high redshift numerical simulations
• Mapping the low surface brightness Universe in the UV band with Lya emission from IGM filaments
• Clustering in the Simulated H$\alpha$ Galaxy Redshift Survey from Nancy Grace Roman Space Telescope
• Theoretical direct WIMP detection rates for transitions to nuclear excited states
• Ram pressure statistics for bent tail radio galaxies
• Non-commutative effects on gravitational measurements
• Odd-parity stability of hairy black holes in $U(1)$ gauge-invariant scalar-vector-tensor theories
• Axial Symmetric Kahler manifolds, the D-map of Inflaton Potentials and the Picard-Fuchs Equation
• Stellar migration in the Auriga simulations
• Probing a panoply of curvaton-decay scenarios using CMB data
• XMM-Newton observation of the ultraluminous quasar SDSS J010013.02+280225.8 at redshift 6.326
• Gravitational lens optical scalars in terms of energy-momentum distributions in the cosmological framework
• $\alpha$-attractor dark energy in view of next-generation cosmological surveys
• Dark Matter from the Supersymmetric Custodial Triplet Model
• Dynamics of Merging Galaxy Clusters from Simulated Analogs
• Cosmological constraints on time-varying cosmological terms: A study of FLRW universe models with $\Lambda (t)$CDM cosmology
• Is patchy reionization an obstacle in detecting the primordial gravitational wave signal?
• Quantum cosmological consistency condition for inflation
• Revised Mass-to-Light Ratios For Nearby Galaxy Groups and Clusters
• On the Uncertainties of Results Derived from HI Spectral Line Stacking Experiments
• ISW-Galaxy Cross Correlation:A probe of Dark Energy clustering and distribution of Dark Matter tracers
• Triplet Leptogenesis, Type-II Seesaw Dominance, Intrinsic Dark Matter, Vacuum Stability and Proton Decay in Minimal SO(10) Breakings
• Constraining the baryon fraction in the Warm Hot Intergalactic Medium at low redshifts with PLANCK data
• Semi-Analytic Galaxy Formation in Massive Neutrino Cosmologies
• Inflationary magnetogenesis, derivative couplings and relativistic Van der Waals interactions
• A Smooth Landscape: Ending Saddle Point Inflation Requires Features to be Shallow
• Euclid preparation. Modelling spectroscopic clustering on mildly nonlinear scales in beyond-$\Lambda$CDM models
• Investigating The Hubble Tension Through Hubble Parameter Data
• Isotropic extragalactic flux from dark matter annihilations: lessons from interacting dark matter scenarios
• Impact of generalized dissipative coefficient on warm inflationary dynamics in the light of latest Planck data
• Inflation without self-reproduction in $F(R)$ gravity
• On Detecting Stellar Binary Black Holes via the LISA-Taiji Network
• Constraining dark sector perturbations II: ISW and CMB lensing tomography
• High Redshift Investigation On The Dark Energy Equation of State
• The impact of spurious shear on cosmological parameter estimates from weak lensing observables
• Creation of entangled universes avoids the big bang singularity
• A Search for an N=2 Inflaton Potential
• Bayesian evidence and predictivity of the inflationary paradigm
• Effects of Lens Motion and Uneven Magnification on Image Spectra
• Whether Lyra's Manifold Itself is a Hidden Source of Dark Energy
• Supernovae as probes of cosmic parameters: estimating the bias from under-dense lines of sight
• Constraints on Lepton Asymmetry from Nucleosynthesis in a Linearly Coasting Cosmology
• Synthetic data products for future HI galaxy surveys: a tool for characterising source confusion in spectral line stacking experiments
• Combined cosmological tests of a bivalent tachyonic dark energy scalar field model
• Starobinsky inflation with a quadratic Weyl tensor
• Cosmic expansion history from SNe Ia data via information field theory -- the charm code
• Culminating the peak CUSP to descry the dark side of halos
• Diagnosing the interstellar medium of galaxies with far-infrared emission lines II. [C II], [O I], [O III], [N II] and [N III] up to z=6
• Lensing impact on cosmic relics and tensions
• Prospects for Observing the low-density Cosmic Web in Lyman-alpha Emission
• Galaxy-Galaxy Lensing in EAGLE: comparison with data from 180 square degrees of the KiDS and GAMA surveys
• How to Interpret Measurements of Diffuse Light in Stacked Observations of Groups and Clusters of Galaxies
• Cosmo++: An Object-Oriented C++ Library for Cosmology
• Axino dark matter with low reheating temperature
• Light WIMP searches involving electron scattering
• Ram pressure stripping in the EAGLE simulation
• Primordial gravitational waves in a quantum model of big bounce
• Maximal CP Violation in Minimal Seesaw Model
• Depth profile study of ${}^{210}$Pb in the surface of an NaI(Tl) crystal
• Cosmology: the search for twenty-four (or more) functions
• Redshifted 21-cm bispectrum: Impact of the source models on the signal and the IGM physics from the Cosmic Dawn
• Interacting holographic Ricci dark energy as running vacuum
• Nonthermal dark matter models and signals
• Constraints on modified Gauss-Bonnet gravity during big bang nucleosynthesis
• Supersymmetric Partially Interacting Dark Matter
• Measuring the Energy Scale of Inflation with Large Scale Structures
• Cosmic Acceleration and Anisotropic models with Magnetic field
• Removing beam asymmetry bias in precision CMB temperature and polarisation experiments
• Optical follow-up observation for GW event S190510g using Subaru/Hyper Suprime-Cam
• Cosmic reionization by primordial cosmic rays
• MIND THE GAP: Is The Too Big To Fail Problem Resolved?
• Baryonic matter perturbations in decaying vacuum cosmology
• First emergence of cold accretion and supermassive star formation in the early universe
• Proton-philic spin-dependent inelastic Dark Matter (pSIDM) as a viable explanation of DAMA/LIBRA-phase2
• ALP Conversion and the Soft X-ray Excess in the Outskirts of the Coma Cluster
• Searching for the shadows of giants: characterising protoclusters with line of sight Lyman-α absorption
• Local probes strongly favor $\Lambda$CDM against power-law and $R_h=ct$ universe
• The Q/U Imaging ExperimenT: Polarization Measurements of the Galactic Plane at 43 and 95 GHz
• Large Scale Suppression of Scalar Power on a Spatial Condensation
• Hardness of ionizing radiation fields in MaNGA star-forming galaxies
• The Unusually High Halo Concentration of the Fossil Group NGC 6482: Evidence for Weak Adiabatic Contraction
• The fall of CSS100217: a tidal disruption-induced low state in an apparently hostless active galactic nucleus
• Screening Mechanism and Late-time Cosmology: Role of a Chameleon-Brans-Dicke Scalar Field
• CII and HI 21-cm line intensity mapping from the EoR: Impact of the light-cone effect on auto and cross-power spectra
• Evolution of the gas mass fraction in galaxy clusters
• Large Molecular Gas Reservoirs in Star Forming Cluster Galaxies
• Discerning Singlet and Triplet scalars at the electroweak phase transition and Gravitational Wave
• On Nonlocal Modified Gravity and Cosmology
• Mass assembly history and infall time of the Fornax dwarf spheroidal galaxy
• Negative Running of the Spectral Index, Hemispherical Asymmetry and the Consistency of Planck with Large $r$
• Halo-independent comparison of direct dark matter detection data: a review
• Investigating subphotospheric dissipation in gamma-ray bursts using joint Fermi-Swift observations
• Hilltop inflation with preinflation from coupling to matter fields
• Galaxy chemical evolution models: The role of molecular gas formation
• Holographic energy density, dark energy sound speed, and tensions in cosmological parameters: $H_0$ and $S_8$
• Cosmic Voids in Evolving Dark Sector Cosmologies: the Low Redshift Universe
• Dark matter implications of the WMAP-Planck Haze
• MSSM Dark Matter in Light of Higgs and LUX Results
• Cold Mode Gas Accretion on Two Galaxy Groups at z$\sim$2
• AGNs at the cosmic dawn: predictions for future surveys from a $\Lambda$CDM cosmological model
• New Interpretation of the Recent Result of AMS-02 and Multi-component Decaying Dark Matters with non-Abelian Discrete Flavor Symmetry
• Period-Luminosity relations derived from the OGLE-III First-overtone mode Cepheids in the Magellanic Clouds
• Multipole expansion for 21cm Intensity Mapping power spectrum: forecasted cosmological parameters estimation for the SKA Observatory
• Galaxy cluster scaling relations measured with APEX-SZ
• Quark-Gluon Plasma as the Possible Source of Cosmological Dark Radiation
• On the coverage of neutralino dark matter in coannihilations at the upgraded LHC
• Constraining Majorana CP Phase in Precision Era of Cosmology and Double Beta Decay Experiment
• Mirror Symmetry of quantum Yang-Mills vacua and cosmological implications
• Constraints on tachyon inflationary models with an AdS/CFT correspondence
• Time Delay of Light in the Gravitational lensing of Supermassive Black Holes in Dark Matter Halos
• Radiative natural SUSY spectrum from deflected AMSB scenario with messenger-matter interactions
• Baryon asymmetry and lower bound on right handed neutrino mass in fast expanding Universe: an analytical approach
• Fragmentation in Population III Galaxies formed through Ionizing Radiation
• Forecasts of cosmological constraints from HI intensity mapping with FAST, BINGO & SKA-I
• Probing delayed-end reionization histories with the 21cm-LAE cross-power spectrum
• EDGES signal in presence of magnetic fields
• A high dust emissivity index beta for a CO-faint galaxy in a filamentary Lyman-alpha nebula at z=3.1
• Cosmic Voids in Evolving Dark Sector Cosmologies: the High Redshift Universe
• Thermodynamics of Shearing Massless Scalar Field Spacetimes is Inconsistent With the Weyl Curvature Hypothesis
• Self-Interacting Dark Matter and the Delay of Super-Massive Black Hole Growth
• Quantifying the abundance of faint, low-redshift satellite galaxies in the COSMOS survey
• Constraining the reionization history with CMB and spectroscopic observations
• Dynamic analysis of noncanonical warm inflation
• Non-linear dynamics of the minimal theory of massive gravity
• Clustering of CODEX clusters
• Uneven flows: On cosmic bulk flows, local observers, and gravity
• Recovering 21-cm signal from simulated FAST intensity maps
• A More Accurate Parameterization based on cosmic Age (MAPAge)
• Drivers of asymmetry in synthetic H I emission-line profiles of galaxies in the EAGLE simulation
• Selecting ultra-faint dwarf candidate progenitors in cosmological N-body simulations at high redshifts
• An Analytic Formulation of 21-cm Signal from Early Phase of Epoch of Reionization
• A radiative seesaw model with higher order terms under an alternative $U(1{)}_{B-L}$
• Imprints of the large-scale structure on AGN formation and evolution
• Some Recent Results on Ricci-Based Gravity Theories
• Observational constraints on the fractal cosmology
• Metallicity profiles of Ultra Diffuse Galaxies in NIHAO simulations
• Minimal model dependent constraints on cosmological nuisance parameters and cosmic curvature from combinations of cosmological data
• Testing the accuracy of likelihoods for cluster abundance cosmology
• Fermionic triplet dark matter in an $SO(10)$-inspired left right model
• Neutron star mass in dark matter clumps
• Low-$\ell$ power suppression in punctuated inflation
• Mirror QCD and Cosmological Constant
• Constraining the history of reheating with the NANOGrav 15-year data
• LiteBIRD Science Goals and Forecasts: Primordial Magnetic Fields
• Interpreting the cosmic far-infrared background anisotropies using a gas regulator model
• Standardizing the Gamma-ray burst as a standard candle and applying to the cosmological probes: constraints on the two-component dark energy model
• Vector Dark Matter Detection using the Quantum Jump of Atoms
• Molecular gas and dust properties in $z>7$ quasar hosts
• Linear matter density perturbations in the ${\Lambda }_{\mathrm{s}}$CDM model: Examining growth dynamics and addressing the $S_8$ tension
• Lepton mass and mixing in a Neutrino Mass Model based on $S_4$ flavor symmetry
• Improving naturalness in Gauge Mediation with non-unified messenger sectors
• Probing dark energy via galaxy cluster outskirts
• Exact Cosmological Solutions in Modified Brans-Dicke Theory
• Separate Einstein-Eddington Spaces and the Cosmological Constant
• The XMM Cluster Survey: evolution of the velocity dispersion -- temperature relation over half a Hubble time
• Constraining SN feedback: a tug of war between reionization and the Milky Way satellites
• Dark matter, lepton and baryon number, and left-right symmetric theories
• The Effect of Cosmic Rays on the Observational Properties of the CGM
• The Cosmological Parameters (2023)
• Photometric and Spectroscopic Observations of GRB 190106A: Emission from Reverse and Forward Shocks with Late-time Energy Injection
• Dark Matter in Fractional Gravity I: Astrophysical Tests on Galactic Scales
• Supersymmetry Searches in GUT Models with Non-Universal Scalar Masses
• Reionization time of the Local Group and Local-Group-like halo pairs
• Galactic Observatory Science with the ASTRI Mini-Array at the Observatorio del Teide
• Large Blue Spectral Isocurvature Spectral Index Signals Time-Dependent Mass
• Distances to Local Group Galaxies via Population II, Stellar Distance Indicators. II. The Fornax Dwarf Spheroidal
• Merging timescale for supermassive black hole binary in interacting galaxy NGC 6240
• Cosmic Variation of Proton to Electron Mass Ratio with an interacting Higgs Scalar Field
• Primordial power spectrum of tensor perturbations in Finsler spacetime
• On the importance of direct detection combined limits for spin independent and spin dependent dark matter interactions
• Interacting realization of cosmological singularities with variable vacuum energy
• Qualitative description of the universe in the interacting fluids scheme
• How CMB and large-scale structure constrain chameleon interacting dark energy
• Is there a connection between "dark" and "light" physics?
• Cosmological constraints on a unified dark matter-energy scalar field model with fast transition
• Exploring Charge and Color Breaking vacuum in Non-Holomorphic MSSM
• Unusual Flaring Activity in the Blazar PKS 1424-418 during 2008-2011
• Uncovering Mass Segregation with Galaxy Analogues in Dark Matter Simulations
• Higgs sector extension of the neutrino minimal standard model with thermal freeze-in production mechanism
• Phenomenological constraints on light mixed sneutrino dark matter scenarios
• Glauber theory and the quantum coherence of curvature inhomogeneities
• Constraining the growth of perturbations with lensing of supernovae
• Simple inflationary models in Gauss-Bonnet brane-world cosmology
• Measurements of the Sunyaev-Zel'dovich Effect in MACS J0647.7+7015 and MACS J1206.2-0847 at High Angular Resolution with MUSTANG
• Maximally localized states and quantum corrections of black hole thermodynamics in the framework of a new generalized uncertainty principle
• Relic density calculations beyond tree-level, exact calculations versus effective couplings: the ZZ final state
• Tensors, BICEP2, prior dependence, and dust
• Observational tests of backreaction with recent data
• Probing reionization using quasar near-zones at redshift z ~ 6
• Scale-dependent hemispherical asymmetry from general initial state during inflation
• The impact of a 126 GeV Higgs on the neutralino mass
• Out-of-equilibrium Baryogenesis and SuperWIMP Dark Matter
• Relic photon temperature versus redshift and the cosmic neutrino background
• CMB distortion from circumgalactic gas
• Detectability of Weak Lensing Modifications under Galileon Theories
• Maximal zero textures of the inverse seesaw with broken $\mu \tau$ symmetry
• A Reconstruction of Quintessence Dark Energy
• Constraining the Higgs-Dilaton with LHC and Dark Matter Searches
• On the Anisotropy of Nuclei Mid-Infrared Radiation in Nearby Active Galactic Nuclei
• Cosmological Tests of Coupled Galileons
• Super cosmic variance from mode-coupling: A worked example
• Top Quark as a Dark Portal and Neutrino Mass Generation
• Probing Gravitational Dark Matter
• Hemispherical asymmetry from an isotropy violating stochastic gravitational wave background
• Neglecting Primordial non-Gaussianity Threatens Future Cosmological Experiment Accuracy
• CP-violating Phases in Active-Sterile Solar Neutrino Oscillations
• Axino LSP Baryogenesis and Dark Matter
• Optimizing parameter constraints: a new tool for Fisher matrix forecasts
• Effective dark matter power spectra in $f(R)$ gravity
• SU(2) Yang-Mills Theory: Waves, Particles, and Quantum Thermodynamics
• The Uchuu-GLAM BOSS and eBOSS LRG lightcones: Exploring clustering and covariance errors
• Fisher Matrix Based Predictions for Measuring the z = 3.35 Binned 21-cm Power Spectrum using the Ooty Wide Field Array (OWFA)
• Evolution of Vacuum Fluctuations of an Ultra-Light Massive Scalar Field generated during and before Inflation
• Quintessential early dark energy
• Radiative Seesaw Model with Degenerate Majorana Dark Matter
• Bianchi type-V Transitioning model in Brans-Dicke theory with Observational Constraint
• SDSS J1138+3517: A quasar showing remarkably variable broad absorption lines
• Temporal variability and estimation of jet parameters for Ton 599
• Constraints on neutrino masses from the lensing dispersion of Type Ia supernovae
• High resolution study of the abundance pattern of the heavy elements in very metal-poor field stars
• Lopsided Satellite Distributions around Isolated Host Galaxies in a LCDM Universe
• Enhancement of Majorana Dark Matter Annihilation Through Higgs Bremsstrahlung
• Neutrino Anarchy and Renormalization Group Evolution
• On the luminosity distance and the epoch of acceleration
• Effect of interstellar objects on metallicity of low-mass first stars formed in a cosmological model
• MAHGIC: A Model Adapter for the Halo-Galaxy Inter-Connection
• Constraining Holographic Dark Energy and Analyzing Cosmological Tensions
• Dark matter imprint on ${}^8$B neutrino spectrum
• Anisotropic satellite accretion onto the Local Group with HESTIA
• The H$\alpha$ broadband photometric reverberation mapping of four Seyfert 1 galaxies
• Fluid phonons, protoinflationary dynamics and large-scale gravitational fluctuations
• The effect of interacting dark energy on local measurements of the Hubble constant
• Joint Suzaku and Chandra observations of the MKW4 galaxy group out to the virial radius
• Impact of the ${}^7$Be($\alpha ,\gamma$)${}^{11}$C reaction on the primordial abundance of ${}^7$Li
• Bogoliubov Excited States and the Lyth Bound
• Equivalence Principles, Spacetime Structure and the Cosmic Connection
• Cosmological effects of the Galileon term in Scalar-Tensor Theories
• Reducing cosmological small scale structure via a large dark matter-neutrino interaction: constraints and consequences
• No Naturalness or Fine-tuning Problems from No-Scale Supergravity
• Realising Interactions Between Dark Matter and Dark Energy Using $k$-essence Cosmology
• Majorana neutrinos with point interactions
• Future detectability of gravitational-wave induced lensing from high-sensitivity CMB experiments
• Reconstructing Orbits of Galaxies in Extreme Regions (ROGER) II: reliability of projected phase-space in our understanding of galaxy populations
• Singlino Resonant Dark Matter and 125 GeV Higgs Boson in High-Scale Supersymmetry
• Dark matter, a new proof of the predictive power of general relativity
• Resolving the nano-Hz gravitational wave sky: the detectability of eccentric binaries with PTA experiments
• The History of Inflation from Microwave Background Polarimetry and Laser Interferometry
• Machine learning synthetic spectra for probabilistic redshift estimation: SYTH-Z
• Study of electron anti-neutrinos associated with gamma-ray bursts using KamLAND
• New type of hill-top inflation
• Dark Matter 2013
• Accretion of satellites onto central galaxies in clusters: merger mass ratios and orbital parameters
• Pitfalls of a power-law parameterization of the primordial power spectrum for Primordial Black Hole formation
• Stars or gas? Constraining the hardening processes of massive black-hole binaries with LISA
• Cosmic Strings and the Origin of Globular Clusters
• Common Origin of $3.55$ keV X-ray line and Gauge Coupling Unification with Left-Right Dark Matter
• Fluid inflation with brane correction
• Implications of JLA data for $k-$essence model of dark energy with given equation of state
• The Past History of Galaxy Clusters told by their present neighbors
• A search for H$\alpha$ emission in high-metallicity damped Lyman-$\alpha$ systems at $z\sim 2.4$
• Exploring Flavor-Dependent Long-Range Forces in Long-Baseline Neutrino Oscillation Experiments
• Coevolution of broad emission lines and X-ray spectrum in changing-look AGNs
• Leptogenesis via the 750 GeV pseudoscalar
• Charged Q-ball Dark Matter from $B$ and $L$ direction
• Weak Lensing Skew-Spectrum
• Examining the Viability of Phantom Dark Energy
• Probing cosmology with weak lensing selected clusters II: Dark energy and f(R) gravity models
• Sunyaev-Zel'dovich Signal from Quasar Hosts: Implications for Detection of Quasar Feedback
• Light stop in the MSSM after LHC Run 1
• Gravitational Waves in Locally Rotationally Symmetric (LRS) Class II Cosmologies
• Angular momentum evolution of bulge stars in disc galaxies in NIHAO
• Eddington accreting Black Holes in the Epoch of Reionization
• The Lambda CDM-model in quantum field theory on curved spacetime and Dark Radiation
• 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
• The XXL Survey: XXX. Characterisation of the XLSSsC N01 supercluster and analysis of the galaxy stellar populations
• A Further Study of the Frampton-Glashow-Yanagida Model for Neutrino Masses, Flavor Mixing and Baryon Number Asymmetry
• Dissecting kinetically coupled quintessence: phenomenology and observational tests
• Weather Forecast of the Milky Way: Shear and Stellar feedback determine the lives of Galactic-scale filaments
• Lepton Number Violation, Lepton Flavour Violation and Baryogenesis in Left-Right Symmetric Model
• The tangential velocity of M31: CLUES from constrained simulations
• Is the core-cusp problem a matter of perspective: Jeans Anisotropic Modeling against numerical simulations
• Big Data in HEP: A comprehensive use case study
• A Novel CMB Component Separation Method: Hierarchical Generalized Morphological Component Analysis
• Cosmology with a Decaying Vacuum Energy Parametrization Derived from Quantum Mechanics
• Coupling between Ion-Acoustic Waves and Neutrino Oscillations
• Validating the methodology for constraining the linear growth rate from clustering anisotropies
• The 21-cm bispectrum from neutral hydrogen islands at z < 6
• Interacting dark energy in the dark $SU(2{)}_R$ model
• Probing Radiative Neutrino Mass Generation through Monotop Production
• Dark matter candidate in an extended type III seesaw scenario
• Universe Inflation Based on Nonlinear Electrodynamics
• Neutrino Fluxes from a Core-Collapse Supernova in a Model with Three Sterile Neutrinos
• A thermodynamic point of view on dark energy models
• Hidden Photons in connection to Dark Matter
• Modeling effective FRW cosmologies with perfect fluids from states of the hybrid quantum Gowdy model
• Star-formation rate in compact star-forming galaxies
• Direct reconstruction of dynamical dark energy from observational Hubble parameter data
• Late-time acceleration driven by shift-symmetric Galileon in the presence of Torsion
• The age gradients of galaxies in EAGLE: outside-in quenching as the origin of young bulges in cluster galaxies
• Probing quasar lifetimes with proximate $21$-centimetre absorption in the diffuse intergalactic medium at redshifts $z\ge 6$
• Can the splashback radius be an observable boundary of galaxy clusters?
• Greybody factor and perturbation of a Schwarzschild black hole with string clouds and quintessence
• Auriga Streams I: disrupting satellites surrounding Milky Way-mass haloes at multiple resolutions
• Prospects of probing quintessence with HI 21-cm intensity mapping survey
• Light Neutralino Dark Matter in $U(1{)}^{\prime }$ models
• Signatures of top flavour-changing dark matter
• The undiscovered ultra-diffuse galaxies of the Local Group
• Resurrecting Sneutrino (${\tilde{\nu }}_L$) Dark Matter in light of Neutrino Mass and LUX
• Explaining Low Energy $\gamma$-ray Excess from the Galactic Centre using a Two Component Dark Matter Model
• Detecting Ancient Supernovae at z ~ 5 - 12 with CLASH
• Cosmic structure, averaging and dark energy
• Statistics of Dark Matter Halos in the Excursion Set Peak Framework
• The Hot and Energetic Universe: The missing baryons and the warm-hot intergalactic medium
• Cosmological models with running cosmological term and decaying dark matter
• The local dark matter distribution in self-interacting dark matter halos
• BASILISK: Bayesian Hierarchical Inference of the Galaxy-Halo Connection using Satellite Kinematics--I. Method and Validation
• The Darkness of Spin-0 Dark Radiation
• Relation between halo spin and cosmic web filaments at z=3
• Accuracy of power spectra in dissipationless cosmological simulations
• Lithium in the lower red giant branch of 5 Galactic globular clusters
• Alternate Definitions of Loop Corrections to the Primordial Power Spectra
• How alive is constrained SUSY really?
• Background Subtraction Uncertainty from Submillimetre to Millimetre Wavelengths
• Probing the fluctuating Ultra-violet background using the Hubble Frontier Fields
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Constraining the Galaxy-Halo Connection with Optimal Statistics
• Non-local bispectra from super cosmic variance
• An environment-dependent halo mass function as a driver for the early quenching of $z\ge 1.5$ cluster galaxies
• Observational constraints on warm quasi-exponential inflation
• Modeling the cross power spectrum of Sunyaev-Zel'dovich and X-ray surveys
• Time-dependent diffusive interactions between dark matter and dark energy in the context of $k-$essence cosmology
• Holographic Ricci dark energy as running vacuum
• General parametrization for energy density of quintessence field
• Connecting Primordial Star Forming Regions and Second Generation Star Formation in the Phoenix Simulations
• Fingerprints of Anomalous Primordial Universe on the Abundance of Large Scale Structures
• Coupling structure of multi-field primordial perturbations
• Dark energy and dark matter perturbations in singular universes
• New Horizons in Cosmology with Spectral Distortions of the Cosmic Microwave Background
• Analysis of the Bounds on Dark Matter Models from Monojet Searches at the LHC
• Daughters mimic sterile neutrinos (almost!) perfectly
• Overdensity of VVV galaxies behind the Galactic bulge
• Constraining the physics of star formation from CIB-cosmic shear cross-correlations
• Naturalness, dark matter, and the muon anomalous magnetic moment in supersymmetric extensions of the standard model with a pseudo-Dirac gluino
• A Spatially-Resolved Survey of Distant Quasar Host Galaxies: II. Photoionization and Kinematics of the ISM
• Testing backreaction effects with observational Hubble parameter data
• A smuon in the NMSSM confronted with the muon g-2 and SUSY searches
• Theoretical implications of detecting gravitational waves
• EDGE: the puzzling ellipticity of Eridanus II's star cluster and its implications for dark matter at the heart of an ultra-faint dwarf
• Single Field Inflation in Supergravity with a $U(1)$ Gauge Symmetry
• Can Stellar Discs in a Cosmological Setting Avoid Forming Strong Bars?
• Statistical properties of filaments in weak gravitational lensing
• TD-CARMA: Painless, accurate, and scalable estimates of gravitational-lens time delays with flexible CARMA processes
• An SU(6) GUT Origin of the TeV-Scale Vector-like Particles Associated with the 750 GeV Diphoton Resonance
• Hubble diagrams of relativistic broad-lined type Ic supernovae
• The power spectrum of systematics in cosmic shear tomography and the bias on cosmological parameters
• Cosmological implications of tracker scalar fields: Testing the evidence for dynamical dark energy with recent data
• Boltzmann Equation Solver Adapted to Emergent Chemical Non-equilibrium
• Differentiating $U(1{)}^{\prime }$ supersymmetric models with right sneutrino and neutralino dark matter
• Robustness of $H_0$ determination at intermediate redshifts
• Bound on photon circular orbits in general relativity and beyond
• Testing core creation in hydrodynamical simulations using the HI kinematics of field dwarfs
• The case for mixed dark matter from sterile neutrinos
• Present status and future perspectives of the NEXT experiment
• Roles of sterile neutrinos in particle physics and cosmology
• The Square Kilometer Array: cosmology, pulsars and other physics with the SKA
• The Dark Energy Cosmic Clock: A New Way to Parametrise the Equation of State
• Cosmological Perturbations and Quasi-Static Assumption in $f(R)$ Theories
• Gemini IFU, VLA, and HST observation of the OH Megamaser Galaxy IRAS17526+3253
• Phenomenology of dark matter in chiral U(1)${}_X$ dark sector
• New observational constraints on interacting dark energy using galaxy clusters virial equilibrium states
• A Cosmological Study in Massive Gravity theory
• Simulating the LOcal Web (SLOW) -- III: Synchrotron emission from the local cosmic web
• Constraining Neutrino mass using the large scale HI distribution in the Post-reionization epoch
• Natural SUSY from SU(5) Orbifold GUT
• Galactic black hole immersed in a dark halo with its surrounding thin accretion disk
• Measuring the temperature and profiles of Lyman-$\alpha$ absorbers
• Dynamic equilibrium sets atomic content of galaxies across cosmic time
• The Logotropic Dark Fluid: Observational and Thermodynamic Constraints
• Constraints on sterile neutrinos and the cosmological tensions
• Locating Bound Structure in an Accelerating Universe
• Recovering the Tidal Field in the Projected Galaxy Distribution
• Relaxation of dark matter halos: how to match observational data?
• Discriminating the HTM and MLRSM models in collider studies via doubly charged Higgs boson pair production and the subsequent leptonic decays
• Mass-Varying Massive Gravity with k-essence
• An analytical method to simulate the HI 21-cm visibility signal for intensity mapping experiments
• Can a void mimic the $\Lambda$ in $\Lambda$CDM?
• On the primordial origin of the smoothing excess in the $Planck$ temperature power spectrum in light of LSS data
• Hamilton-Jacobi approach for quasi-exponential inflation: predictions and constraints after Planck 2015 results
• Averaged Energy Conditions and Bouncing Universes
• A common origin for the Fundamental Plane of quiescent and star-forming galaxies in the EAGLE simulations
• The signal of decaying dark matter with hydrodynamical simulations
• A Catalog of Emission-Line Galaxies from the Faint Infrared Grism Survey: Studying Environmental Influence on Star Formation
• The impact of faint AGN discovered by JWST on reionization
• Extended FLRW Models: dynamical cancellation of cosmological anisotropies
• The bispectrum of matter perturbations from cosmic strings
• Dynamical friction in the primordial neutrino sea
• X-ray lines and self-interacting dark matter
• Cosmological effects of coupled dark matter
• Average Dark Matter Halo Sparsity Relations as Consistency Check of Mass Estimates in Galaxy Cluster Samples
• Constraints on Dark Matter-Photon Coupling in the Presence of Time-Varying Dark Energy
• Predictions for measuring the cross power spectrum of the HI 21-cm signal and the Lyman-$\alpha$ forest using OWFA
• An Optical Analysis of the Merging Cluster Abell 3888
• Observational constraints in Delta Gravity: CMB and supernovas
• Morphology of Weak Lensing Convergence Maps
• The interacting vacuum and tensions: a comparison of theoretical models
• Relationship between Bondi-Sachs quantities and source of gravitational radiation in asymptotically de Sitter spacetime
• CMS kinematic edge from s-bottoms
• The role of $T_0$ in CMB anisotropy measurements
• Relativistic and nonrelativistic annihilation of dark matter: a sanity check using an effective field theory approach
• Dark Matter and The Seesaw Scale
• Prospects for higgsino-singlino dark matter detection at IceCube and PINGU
• Cosmological constraints with the Effective Fluid approach for Modified Gravity
• Traveling Through the Universe: Back in Time to the Quark-Gluon Plasma Era
• CDM/baryon isocurvature perturbations in a sneutrino curvaton model
• Gravitational Lensing of Spherically Symmetric Black Holes in Dark Matter Halos
• Higgs Inflation and General Initial Conditions
• Interpreting the Fermi-LAT gamma ray excess in the simplified framework
• Testing theories of Gravity and Supergravity with inflation and observations of the cosmic microwave background
• The Entire Virial Radius of the Fossil Cluster RXJ1159+5531: II. Dark Matter and Baryon Fraction
• Can the Baryon Asymmetry Arise From Initial Conditions?
• Unveiling the 100 pc scale nuclear radio structure of NGC 6217 with e-MERLIN and the VLA
• Revisiting the large-scale CMB anomalies: The impact of the SZ signal from the Local Universe
• Semi-analytic galaxy formation in coupled dark energy cosmologies
• Classifying the behavior of noncanonical quintessence
• Dark Matter from Unification of Color and Baryon Number
• Evolution of velocity dispersion along cold collisionless flows
• Investigating early-type galaxy evolution with a multi-wavelength approach. III. Insights from SPH simulations with chemo-photometric implementation
• Multimessenger TeV Dark Matter: a mini review
• Estimation of Inflation parameters for Perturbed Power Law model using recent CMB measurements
• Investigating time variability of X-ray absorption in Swift GRBs
• Two-Loop Quantum Gravity Corrections to Cosmological Constant in Landau Gauge
• Do the Spirits Rise?
• The Isaac Newton Telescope Monitoring Survey of Local Group Dwarf Galaxies. VI. The Star Formation History and Dust Production in Andromeda IX
• Identifying Active Galactic Nuclei at $z\sim 3$ from the HETDEX Survey Using Machine Learning
• Photo-z Quality Cuts and their Effect on the Measured Galaxy Clustering
• Diffusive dark matter and dark energy scenario and $k-$essence in the context of Supernova Ia observations
• Testing a dissipative kinetic k-essence model
• Testing the ABS method with the simulated Planck temperature maps
• Radiative Corrections from Heavy Fast-Roll Fields during Inflation
• Is there a connection between Broad Absorption Line Quasars and Narrow Line Seyfert 1 galaxies?
• Lightcone Averaging and Precision Cosmology
• Cosmic acceleration and ekpyrotic bounce with Chameleon field
• Probing the epoch of pre-reionization by cross-correlating cosmic microwave and infrared background anisotropies
• Biased cosmological parameter estimation with galaxy cluster counts in the presence of primordial non-Gaussianities
• GW170817 event rules out general relativity in favor of vector gravity
• Probing Dark-ALP Portals at Future $e^{+}{e}^{-}$ Colliders
• An SO(10) \times SO(10)' model for common origin of neutrino masses, ordinary and dark matter-antimatter asymmetries
• Nonthermal $CP$ violation in soft leptogenesis
• Very metal-poor stars in the solar vicinity: age determination
• Exploring the supersymmetric U(1)${}_{B-L}\times$ U(1)${}_R$ model with dark matter, muon $g-2$ and $Z^{\prime }$ mass limits
• Constraints on electromagnetic form factors of sub-GeV dark matter from the Cosmic Microwave Background anisotropy
• Redshift evolution of the HI detection rate in radio-loud active galactic nuclei
• Constraining $U(1{)}_{L_{\mu }-L_{\tau }}$ charged dark matter model for muon $g-2$ anomaly with AMS-02 electron and positron data
• Modified Baryonic Dynamics: two-component cosmological simulations with light sterile neutrinos
• The Subaru HSC weak lensing mass-observable scaling relations of spectroscopic galaxy groups from the GAMA survey
• Chameleon Fragmentation
• Upper Bound on the First Star Formation History
• Dark side of the universe in the Stephani cosmology
• Understanding the nature of the blazar CGRaBS~J0211$+$1051
• A Universal Bound on Excitations of Heavy Fields during Inflation
• CMB statistical anisotropy from noncommutative gravitational waves
• The Herschel Virgo Cluster Survey. XV. Planck submillimetre sources in the Virgo Cluster
• Modified Equations of State for Dark Energy and Observational Limitations
• Black hole virial masses from single-epoch photometry: the miniJPAS test case
• How well can we unravel the accreted constituents of the Milky Way stellar halo? A test on cosmological hydrodynamical simulations
• Gravitational Waves from Direct Collapse Black Holes Formation
• The influence of Hickson-like compact group environment on galaxy luminosities
• SEAGLE--III: Towards resolving the mismatch in the dark-matter fraction in early-type galaxies between simulations and observations
• Reconstructing the Hubble diagram of gamma-ray bursts using deep learning
• How does pressure gravitate? Cosmological constant problem confronts observational cosmology
• Bound Dark Energy: towards understanding the nature of the Dark Energy
• Science with CMB spectral distortions
• The QUIJOTE CMB Experiment: status and first results with the multi-frequency instrument
• Is there supercurvature mode of massive vector field in open inflation?
• The evolution of the galaxy and the birth of the solar system: The short-lived nuclides connection
• A Universal Profile for Stacked Filaments from Cold Dark Matter Simulations
• Potentialities of Hubble parameter and expansion rate function data to alleviate Hubble tension
• Some First Stars Were Red: Detecting Signatures of Massive Population III Formation Through Long-Term Stochastic Color Variations
• Inflation with $f(R,\varphi )$ in Jordan frame
• First polarised light with the NIKA camera
• Thermodynamic aspects of entropic cosmology with viscosity
• Ghost dark energy with sign-changeable interaction term
• Non-linear matter bispectrum in general relativity
• The halo bias for number counts on the light cone from relativistic N-body simulations
• R-Parity Conservation from a Top Down Perspective
• Compact objects and the swampland
• Anisotopic inflation with a non-abelian gauge field in Gauss-Bonnet gravity
• Intracluster light is a biased tracer of the dark matter distribution in clusters
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions and Lingering Tension
• The Coincidence Problem and the Swampland Conjectures in the Ijjas-Steinhardt Cyclic Model of the Universe
• Dark against luminous matter around isolated central galaxies: a comparative study between modern surveys and Illustris-TNG
• Testing CP-Violation in the Scalar Sector at Future $e^{+}{e}^{-}$ Colliders
• AKARI near-infrared background fluctuations arise from normal galaxy populations
• Challenges in Constraining Gravity with Cosmic Voids
• The signatures of the new particles $h_2$ and $Z_{\mu \tau }$ at e-p colliders in the $U(1{)}_{L_{\mu }-L_{\tau }}$ model
• Hemispherical Power Asymmetry of the Cosmic Microwave Background from a Remnant of a pre-Inflationary Topological Defect
• Confronting Four Zero Neutrino Yukawa Textures with $N_2^{}$-dominated Leptogenesis
• Absence of solid angle deficit singularities in beyond-generalized Proca theories
• Stringy bounces and gradient instabilities
• Dark matter halos and the M-σrelation for supermassive black holes
• Early Science with the Large Millimeter Telescope: Dust constraints in a z~9.6 galaxy
• High purity NaI(Tl) scintillator to search for dark matter
• Cluster-lensing: A Python Package for Galaxy Clusters & Miscentering
• Perturbation level interacting dark energy model and its consequence on late-time cosmological parameters
• External priors for the next generation of CMB experiments
• A Solution to Lithium Problem by Long-Lived Stau
• Effective Theory for Electroweak Doublet Dark Matter
• Effects of sterile neutrino and extra-dimension on big bang nucleosynthesis
• Multiple Field Inflation and Signatures of Heavy Physics in the CMB
• From Halos to Galaxies. VI. Improved halo mass estimation for SDSS groups and measurement of the halo mass function
• Thermal components in the early X-ray afterglows of GRBs: likely cocoon emission and constraints on the progenitors
• Backsplash galaxies and their impact on galaxy evolution: a three-stage, four-type perspective
• Szekeres models: a covariant approach
• Optimized Large-Scale CMB Likelihood And Quadratic Maximum Likelihood Power Spectrum Estimation
• Can power spectrum observations rule out slow-roll inflation?
• Two-body orbit expansion due to time-dependent relative acceleration rate of the cosmological scale factor
• Condensation of Galactic Cold Dark Matter
• Graviton mass due to dark energy as a superconducting medium: theoretical and phenomenological aspects
• Galaxy cluster optical mass proxies from probabilistic memberships
• Testing New Ideas Regarding the Nature of Interstellar Extinction
• Choice of vacuum state and the relation between inflationary and Planck scales
• Molecules in the early Universe
• RG Analysis for Quantum Gravity with A Single Dimensionless Coupling
• Galaxy populations in haloes in high-density environments
• Cosmology In Terms Of The Deceleration Parameter. Part II
• Cosmology of the interacting Tsallis holographic dark energy in $f(R,T)$ gravity framework
• On the dwarf galaxies rotation curves diversity problem
• On Weak Lensing Shape Noise
• Can we distinguish early dark energy from a cosmological constant?
• Foreground Removal of CO Intensity Mapping Using Deep Learning
• The parametrization of gas flows in discs in the Auriga simulations
• Astrophysical Tests of Kinematical Conformal Cosmology in Fourth-Order Conformal Weyl Gravity
• Phenomenology of $keV$ sterile neutrino in minimal extended seesaw
• Continuous Flavor Symmetries and the Stability of Asymmetric Dark Matter
• Panchromatic Spectral Energy Distributions of simulated galaxies: results at redshift $z=0$
• Variation of the stellar initial mass function in semi-analytical models III: testing the cosmic ray regulated integrated galaxy-wide initial mass function
• Cosmological evolution of the gravitational entropy of the large-scale structure
• ARTEMIS emulator: exploring the effect of cosmology and galaxy formation physics on Milky Way-mass haloes and their satellites
• Dynamics of Mixed Dark Energy Domination in Teleparallel Gravity and Phase-Space Analysis
• CALSAGOS: Clustering ALgorithmS Applied to Galaxies in Overdense Systems
• Enhanced lines and box-shaped features in the gamma-ray spectrum from annihilating dark matter in the NMSSM
• The Lyman-beta forest as a cosmic thermometer
• Determining $H_0$ using a model-independent method
• A radiative neutrino mass model in light of DAMPE excess with hidden gauged $U(1)$ symmetry
• The mass accretion history of dark matter haloes down to Earth mass
• HSC-CLAUDS survey: The star formation rate functions since z ~ 2 and comparison with hydrodynamical simulations
• Early formation of supermassive black holes from the collapse of strongly self-interacting dark matter
• Do bulges stop stars forming?
• A Local Universe model for constrained simulations
• Exploring the relationship between black hole accretion and star formation with blind mid-/far-infrared spectroscopic surveys
• Possible explanation of indirect gamma ray signatures from hidden sector fermionic dark matter
• Higgsino Asymmetry and Direct-Detection Constraints of Light Dark Matter in the NMSSM with Non-Universal Higgs Masses
• Discrimination of heavy elements originating from Pop III stars in z = 3 intergalactic medium
• A search for Population III galaxies in CLASH. I. Singly-imaged candidates at high redshift
• Characterizing galaxy clusters by their gravitational potential: systematics of cluster potential reconstruction
• Aspects of Some New Versions of Pilgrim Dark Energy in DGP Braneworld
• Predictive neutrino mass textures with origin of flavor symmetries
• J1046+4047: an extremely low-metallicity dwarf star-forming galaxy with O32 = 57
• SU(2)$_{\tiny\mbox{CMB}}$ at high redshifts and the value of $H_0$
• Constraining the host galaxy halos of massive black holes from LISA event rates
• Reconstruction of $f(T,\mathcal{T})$ Lagrangian for various cosmological scenarios
• Measuring the thermal and ionization state of the low-$z$ IGM using likelihood free inference
• Perturbations in Bouncing and Cyclic Models, a General Study
• Cosmic evolution in the background of non-minimal coupling in $f(R,T,R_{\mu \nu }{T}^{\mu \nu })$ Gravity
• Stability of neutron stars in Horndeski theories with Gauss-Bonnet couplings
• The Velocity Distribution Function of Galaxy Clusters as a Cosmological Probe
• Noncommutative Universe and Chameleon Field Dynamics
• How to confirm the existence of population III stars by observations of gravitational waves
• An i2HDM Strongly Coupled to a non-Abelian Vector Resonance
• SZ/X-ray scaling relations using X-ray data and Planck Nominal maps
• The effect of quantum decoherence on inflationary gravitational waves
• Dark Matter with multi-annihilation channels and AMS-02 positron excess and antiproton
• Constraints on just enough inflation preceded by a thermal era
• Amplification of Magnetic Fields in a Primordial HII Region and Supernova
• Co-Evolution vs. Co-existence: The Effect of Accretion Modelling on the Evolution of Black Holes and Host Galaxies
• Reassessing Dust's Role in Forming the CMB
• Does the chemothermal instability have any role in the fragmentation of primordial gas
• Phantom of the Hartle-Hawking instanton: connecting inflation with dark energy
• Direct geometrical measurement of the Hubble constant from galaxy parallax: predictions for the Vera C. Rubin Observatory and Nancy Grace Roman Space Telescope
• A new generic evolution for $k$-essence dark energy with $w\approx -1$
• Lightness of a Higgs Boson and Spontaneous CP-violation in the Lee Model: An Alternative Scenario
• How do baryonic effects on the cosmic matter distribution vary with scale and local density environment?
• The viable f(G) gravity models via reconstruction from the observations
• Deciphering the Milky Way disc formation time encrypted in the bar chrono-kinematics
• Probing departures from $\Lambda$CDM by late-time datasets
• Cosmological implications of shift symmetric Galileon field
• Interacting parametrized post-Friedmann method
• Circumnuclear Medium around the Central AGN in a Cool-Core Cluster, Abell 1644-South
• A new estimator of the deceleration parameter from galaxy rotation curves
• Coupling Unification and Dark Matter in a Standard Model Extension with Adjoint Majorana Fermions
• Clustering GCG: a viable option for unified dark matter-dark energy?
• Scale and shape dependent non-Gaussianity in the presence of inflationary vector fields
• The AGN Hubble Diagram and Its Implications for Cosmology
• Constraining Warm Dark Matter with high-$z$ supernova lensing
• The CIB-lensing bispectrum: impact on primordial non-Gaussianity and detectability for the Planck mission
• Revisiting Discrete Dark Matter Model:θ_{13}\neq0 and ν_{R} Dark Matter
• Quantifying the Impact of Cosmological Parameter Uncertainties on Strong Lensing Models With an Eye Toward the Frontier Fields
• A combined study of thermohaline mixing and envelope overshooting with PARSEC: Calibration to NGC 6397 and M4
• The strongest gravitational lenses: III. The order statistics of the largest Einstein radii
• Towards conformal cosmology
• SN 2016hil-- a Type II supernova in the remote outskirts of an elliptical host and its origin
• Particle initialization effects on Lyman-$\alpha$ forest statistics in cosmological SPH simulations
• The role of accreted and in situ populations in shaping the stellar halos of low-mass galaxies
• Probing the dark matter-electron interactions via hydrogen-atmosphere pulsating white dwarfs
• Cosmological constraints on superconducting dark energy models
• Constraining the mass-concentration relation through weak lensing peak function
• BICEP2, the curvature perturbation and supersymmetry
• Hidden from view: Coupled Dark Sector Physics and Small Scales
• Follow-up survey for the binary black hole merger GW200224_222234 using Subaru/HSC and GTC/OSIRIS
• Non minimally coupled condensate cosmologies: matching observational data with phase space
• Radiative Light Dark Matter
• Cosmological Constraints using the newest VLT-KMOS HII Galaxies and the full Planck CMB spectrum
• An observational testbed for cosmological zoom-in simulations: constraining stellar migration in the solar cylinder using asteroseismology
• How Slowly can the Early Universe Expand?
• Reconstruction of CMB Temperature Anisotropies with Primordial CMB Induced Polarization in Galaxy Clusters
• Classification of static black holes in Einstein phantom/dilaton Maxwell/anti-Maxwell gravity systems
• Gravitational Waves in G4v
• Features in single field slow-roll inflation
• Setting the scene for BUFFALO: A study of the matter distribution in the HFF galaxy cluster MACS J0416.1-2403 and its parallel field
• Scalar Dark Energy Models and Scalar-Tensor Gravity: Theoretical Explanations for the Accelerated Expansion of Present Universe
• Angular distribution of cosmological parameters as a probe of space-time inhomogeneities
• Modified Teleparallel $f(T)$ Gravity, DESI BAO and the $H_0$ Tension
• Darkening the Little Higgs
• Simple brane-world inflationary models in light of BICEP2
• A possible role for the merger of clusters/voids in the cosmological expansion
• Monitoring broad emission-line components in spectra of the two low-metallicity dwarf compact star-forming galaxies SBS 1420+540 and J1444+4840
• Nonthermal radiation of evaporating black holes
• Accurate Analytic Mass-Scale Relations for Dark Matter Haloes of all Masses and Redshifts
• Probing the Nature of the First Galaxies with JWST and ALMA
• A deep learning approach to halo merger tree construction
• Cosmological constrains on fast transition Unified Dark Energy/Matter models
• Fitting of supernovae without dark energy
• Primordial Power Spectrum and Bispectrum from Lattice Simulations of Axion-U(1) Inflation
• The SCUBA-2 Cosmology Legacy Survey: The EGS deep field -- III. The evolution of faint submillimeter galaxies at $z<4$
• Cosmic evolution of grain size distribution in galaxies using the ${\nu }^2$GC semi-analytic model
• On Dark Gravitational Wave Standard Sirens as Cosmological Inference and Forecasting the Constraint on Hubble Constant using Binary Black Holes Detected by Deci-hertz Observatory
• A WHIM origin for the soft excess emission in the Coma cluster
• Intra-Cluster Light as a Dynamical Clock for Galaxy Clusters: Insights from the MAGNETICUM, IllustrisTNG, Hydrangea and Horizon-AGN Simulations
• Probing Reionization-Era Galaxies with JWST UV Luminosity Functions and Large-Scale Clustering
• Neutral meson mixing induced by box diagrams in the 3-3-1 model with heavy leptons
• Dark Matter in Leptophilic Higgs Models After the LHC Run-I
• Purely Triplet Seesaw and Leptogenesis within Cosmological Bound, Dark Matter and Vacuum Stability
• Modeling the Cosmic Dispersion Measure in the D < 120 Mpc Local Universe
• Three- and two-point spatial correlations of IGM at $z\sim 2$: Cloud based analysis using simulations
• Abundance matching tested on small scales with galaxy dynamics
• Basis invariant description of chemical equilibrium with implications for a recent axionic leptogenesis model
• The Gas Accretion History of Low Mass Halos within the Cosmic Web from Cosmological Simulations
• The supernova cosmology cookbook: Bayesian numerical recipes
• Globular Cluster Counts around 700 Nearby Galaxies
• A general approach to quenching and galactic conformity
• Constraints on the Combined Models with $R^{2-q}$ Inflation and Viable $f(R)$ Dark Energy
• Geometrical measures of non-Gaussianity generated from single field Inflationary models
• Fluorescent rings in star-free dark matter haloes
• Self-Interacting Dark Matter Scattering Rates Through Cosmic Time
• On the Hubble expansion in a Big Bang quantum cosmology
• Electromagnetic vacuum fluctuations around a cosmic string in de Sitter spacetime
• The $m$-$z$ relation for type Ia supernovae, locally inhomogeneous cosmological models, and the nature of dark matter
• Physics of the Cosmic Microwave Background Radiation
• Measurement of the quenching and channeling effects in a CsI crystal used for a WIMP search
• Can Dark Matter be a Scalar Field?
• Hubble flow variations as a test for inhomogeneous cosmology
• CCDM Model with Spatial Curvature and The Breaking of "Dark Degeneracy"
• Reheating constraints on modified quadratic chaotic inflation
• DEMNUni: cross-correlating the nonlinear ISWRS effect with CMB-lensing and galaxies in the presence of massive neutrinos
• Cosmic Acceleration from Varying Masses in Five Dimensions
• Cosmological Constant Implementing Mach Principle in General Relativity
• Isolating the linear signal when making redshift space distortion measurements
• The phase transition of Rastall AdS black hole with cloud of strings and quintessence
• New-Type Charged Q-ball Dark Matter in Gauge Mediated SUSY Breaking Models
• A γ-ray emitting NLS1 galaxy SDSS J095909.51+460014.3 identified by multiwavelength contemporaneous brightening
• Contribution of the first galaxies to the cosmic far-infrared/sub-millimeter background - I. Mean background level
• Spontaneous CP-violation in the Simplest Little Higgs Model and its Future Collider Tests: the Scalar Sector
• Universal dark halo scaling relation for the dwarf spheroidal satellites
• Methanol absorption in PKS B1830-211 at milliarcsecond scales
• Warm Modified Chaplygin Gas Shaft Inflation
• Simulating the z = 3.35 HI 21-cm visibility signal for the Ooty Wide Field Array(OWFA)
• Doublet-triplet dark matter with neutrino masses
• A framework to mitigate patchy reionization contamination on the primordial gravitational wave signal
• Electroweak Baryogenesis in the Exceptional Supersymmetric Standard Model
• The $c$-map, Tits Satake subalgebras and the search for $\mathcal{N}=2$ inflaton potentials
• Cosmological constraints on galaxy cluster structure
• Interactions in the dark sector of the Universe
• NIHAO XXVIII: Collateral effects of AGN on dark matter concentration and stellar kinematics
• Running of the Spectral index in Deformed Matter Bounce Scenarios with Hubble-rate-dependent Dark Energy
• Testing the anisotropy of the Universe with the distance duality relation
• Supergravity Model of Inflation and Explaining IceCube HESE Data via PeV Dark Matter Decay
• Differentiating small-scale subhalo distributions in CDM and WDM models using persistent homology
• Scalar quadratic maximum likelihood estimators for the CMB cross power spectrum
• Unveiling the Universe with Emerging Cosmological Probes
• Moduli inflation in five-dimensional supergravity models
• The impact of filaments on dwarf galaxy properties in the Auriga simulations
• Cosmological Analysis of Reconstructed $\mathcal{F}(T,T_{\mathcal{G}})$ Models
• Gauss-Bonnet dark energy on Hořava-Lifshitz cosmology
• Direct Detection with Dark Mediators
• Sub-horizon evolution of cold dark matter perturbations through dark matter-dark energy equivalence epoch
• The Redshift Dependence of the Radio Flux of Gamma-Ray Bursts and Their Host Galaxies
• Simiplified textures of the seesaw model for the trimaximal neutrino mixings
• Fast scalar quadratic maximum likelihood estimators for the CMB B-mode power spectrum
• The morphology of star-forming gas and its alignment with galaxies and dark matter haloes in the EAGLE simulations
• The mass-size relation of LRGs from BOSS and DECaLS
• Running of scalar spectral index in multi-field inflation
• Anti-screening of the Galileon force around a disk center hole
• Modulated Inflation Models and Primordial Black Holes
• N-body lensed CMB maps: lensing extraction and characterization
• Statistical analysis with cosmic-expansion-rate measurements and two-point diagnostics
• A numerical approach to model independently reconstruct $f(R)$ functions through cosmographic data
• Radiative Emission of Neutrino Pairs in Atoms and Light Sterile Neutrinos
• Corrections to Scaling Neutrino Mixing: Non-zero ${\theta }_{13},{\delta }_{CP}$ and Baryon Asymmetry
• A More Accurate and Competitive Estimative of $H_0$ in Intermediate Redshifts
• Studying galaxy cluster morphological metrics with Mock-X
• Covariant evolution of perturbations during reheating in two-field inflation
• Leptophobic $Z^{\prime }$ bosons in the secluded UMSSM
• A comparison of ${\text{H}}_2$ formation models at high redshift
• Bayesian model selection for dark energy using weak lensing forecasts
• Stochastic determination of matrix determinants
• Stochastic Gravitational Wave Background from Exoplanets
• Simplified equations for gravitational field in the vector theory of gravity and new insights into dark energy
• Dark Sector Coupling Bends the Superclusters
• The WIMP-induced Gamma Ray Spectrum of Active Galactic Nuclei
• On The Role of Supermassive Black Holes in Quenching Star Formation in Local Central Galaxies
• Intrinsic size correlations in weak lensing
• Analytic Calculation of Covariance between Cosmological Parameters from Correlated Data Sets, with an Application to SPTpol
• Fully renormalized stress tensor correlator in flat space
• Resolving primordial physics through correlated signatures
• Inhomogeneous and anisotropic Universe and apparent acceleration
• Radiative generation of neutrino mixing: degenerate masses and threshold corrections
• Cosmic Acceleration in an Extended Brans-Dicke-Higgs Theory
• Dark Matter as gravitational solitons in the weak field limit
• Search for Scalar Dark Matter via Pseudoscalar Portal Interactions: In Light of the Galactic Center Gamma-Ray Excess
• Dark matter in Inert Doublet Model with one scalar singlet and $U(1{)}_X$ gauge symmetry
• Dynamical model for primordial black holes
• Electroweak Naturalness and Deflected Mirage Mediation
• Thermodynamics of interacting holographic dark energy
• Ultra High Energy Neutrinos: Absorption, Thermal Effects and Signatures
• Can non-local or higher derivative theories provide alternatives to inflation?
• Generalized Interacting Dark Energy Model and Loop Quantum Cosmology
• The VIMOS VLT Deep Survey: the redshift distribution N(z) of magnitude-limited samples down to iAB=24.75 and KsAB=22
• Supersymmetric hybrid inflation with non-minimal coupling to gravity
• Imprints of the super-Eddington accretion on the quasar clustering
• Higher moments of primordial non-Gaussianity and N-body simulations
• A solution to the baryon-DM coincidence problem in the CMSSM with a 126-GeV Higgs boson
• Generalised Uncertainty Relations from Finite-Accuracy Measurements
• Signal of Cosmic Strings in Cross-Correlation of 21-cm Redshift and CMB Polarization Maps
• Subaru HSC weak lensing of SDSS redMaPPer cluster satellite galaxies: Empirical upper limit on orphan fractions
• HELLO project: High-$z$ Evolution of Large and Luminous Objects
• The Lyman-limit photon mean free path at the end of late reionisation in the Sherwood-Relics simulations
• Probing Lepton Asymmetry with 21 cm Fluctuations
• Neutrino Experiments and the LHC: Friends Across 14 Orders of Magnitude
• GRB 221009A and the Apparently Most Energetic Gamma-Ray Bursts
• Probing galaxy cluster and intra-cluster gas with luminous red galaxies
• The Swift X-ray Telescope Cluster Survey II. X-ray spectral analysis
• On galaxy rotation curves from a continuum mechanics approach to modified gravity
• Void alignment and density profile applied to measuring cosmological parameters
• NIHAO XXVII: Crossing the green valley
• Initial Li Abundances in the Protogalaxy and Globular Clusters Based upon the Chemical Separation and Hierarchical Structure Formation
• Some Phenomenologies of a Simple Scotogenic Inverse Seesaw Model
• The Glow of Axion Quark Nugget Dark Matter: (II) Galaxy Clusters
• Inflaton fluctuations in the presence of cosmological defects
• Impact of astrophysical scatter on the Epoch of Reionization [H I]${}_{21cm}$ bispectrum
• Active Dirac Neutrinos via $SU(2{)}_L$ Doublets in 5d
• Emission Line Metallicities From The Faint Infrared Grism Survey and VLT/MUSE
• Qualitative evolution in f(R) cosmologies
• Characterizing the Best Cosmic Telescopes with the Millennium Simulations
• Measuring the reionization 21 cm fluctuations using clustering wedges
• The effect of three matters on KSS bound
• The Double-Dark Portal
• Non-collider searches for stable massive particles
• One Extension to Explain Them All, One Scale-Invariant Spectrum to Test Them All, and in One Model Bind Them
• Distinguishing Neutrino Mass Hierarchies using Dark Matter Annihilation Signals at IceCube
• Testing kinetically coupled inflation models with CMB distortions
• Role of polarizations and spin-spin correlations of $W^{\prime }s$ in $e^{-}{e}^{+}\to W^{-}{W}^{+}$ at $\sqrt{s}=250$ GeV to probe anomalous $W^{-}{W}^{+}Z/\gamma$ couplings
• Decelerating cosmologies are de-scramblers
• Towards a Scale Free Electroweak Baryogenesis
• Hubble Space Telescope Astrometry of the Metal-Poor Visual Binary $\mu$ Cassiopeiae: Dynamical Masses, Helium Content, and Age
• Low-mass neutralino dark matter in supergravity scenarios: phenomenology and naturalness
• Fast and Flexible Neutrino Decoupling Part I: The Standard Model
• The Sun and stars: Giving light to dark matter
• Accommodation of the Dirac Phase in the Krauss-Nasri-Trodden Model
• The impact of environmental effects on AGN: a decline in the incidence of ionized outflows
• Quasi-spherical superclusters
• Thermal gravitational-wave background in the general pre-inflationary scenario
• Quantum Smearing in Hybrid Inflation with Chaotic Potentials
• G-Warm inflation: Intermediate model
• The hierarchy problem and the vacuum stability in two-scalar dark matter model
• Consistency of the nonflat $\Lambda$CDM model with the new result from BOSS
• Reconstructing thawing quintessence with multiple datasets
• Massive Gravity wrapped in the Cosmic Web
• Dynamical Properties of Molecular-forming Gas Clumps in Galaxies at the Epoch of Reionization
• Study of Majorana Fermionic Dark Matter
• Renormalization group equation analysis of a pseudoscalar portal dark matter model
• Reheating, thermalization and non-thermal gravitino production in MSSM inflation
• More about a successful vector-tensor theory of gravitation
• Inflationary buildup of a vector field condensate and its cosmological consequences
• Impact of Low ell's on Large Scale Structure Anomalies
• keV Sterile Neutrino Dark Matter and Low Scale Leptogenesis
• A Heavy "Neutralino" in Warped Extra dimensions
• Inflation in de Sitter spacetime and CMB large scales anomaly
• The relationship between cluster environment and molecular gas content of star-forming galaxies in the EAGLE simulation
• On the variation in stellar $\alpha$-enhancements of star-forming galaxies in the EAGLE simulation
• Phenomenology of Colored Radiative Neutrino Mass Model and Its Implications on the Cosmic-ray Observations
• Primordial magnetic fields from self-ordering scalar fields
• The Superhorizon Test of Future B-mode Experiments
• SN 2018gk Revisited: the Photosphere, the Central Engine, And the Putative Dust
• Population modelling of FRBs from intrinsic properties
• Analytic Formulation of 21 cm Signal from Cosmic Dawn: Ly$\alpha$ Fluctuations
• Using simulated Tianqin gravitational wave data and electromagnetic wave data to study the coincidence problem and Hubble tension problem
• Anisotropic power spectrum and the observed low-l power in PLANCK CMB data
• Biparametric complexities and the generalized Planck radiation law
• Statistical imprints of CMB B-type polarization leakage in an incomplete sky survey analysis
• The $\gamma$-ray emitting region in low synchrotron peak blazars. Testing self-synchrotron Compton and external Compton scenarios
• Studying neutral hydrogen structures during the epoch of reionization using fractal dimensions
• Improved cosmological fits with quantized primordial power spectra
• Cosmological Particle Decays at Finite Temperature
• Black Strings and String Clouds Embedded in Anisotropic Quintessence: Solutions for Scalar Particles and Implications
• Mirage Models Confront the LHC: III. Deflected Mirage Mediation
• Spatial and temporal variations of the fine-structure constant in the Finslerian universe
• Accelerated Expansion of the Universe in a Higher Dimensional Modified Gravity with Euler-Poincaré Terms
• Inner structure of dark matter halos at high $z$ in cosmological models with non-power-law primordial spectra
• Cluster Cosmology with the Velocity Distribution Function of the HeCS-SZ Sample
• Initial Mass Function Variation in two Elliptical Galaxies using Near-Infrared Tracers
• Global monopoles can change Universe's topology
• Disc-Halo Interactions in ΛCDM
• Explaining the Fermi Galactic Centre Excess in the CMSSM
• Scrutinizing coupled vector dark energy in light of data
• Anamorphic Quasiperiodic Universes in Modified and Einstein Gravity with Loop Quantum Gravity Corrections
• Extracting constraints from direct detection searches of supersymmetric dark matter in the light of null results from the LHC in the squark sector
• Three-body gravitino decays in the MSSM
• Revisiting kink-like parametrization and constraints using OHD/Pantheon+/BAO samples
• Observations of Galactic star-forming regions with the Cosmic Background Imager at 31 GHz
• Lowering threshold of NaI(Tl) scintillator to 0.7 keV in the COSINE-100 experiment
• Improving the Single Scalar Consistency Relation
• Milestones of general relativity: Hubble's law (1929) and the expansion of the universe
• Improved selection of extremely red quasars with boxy CIV lines in BOSS
• Towards Machine-assisted Meta-Studies: The Hubble Constant
• Status of the 98 - 125 GeV Higgs scenario with updated LHC-8 data
• A comprehensive view of blackbody components in the X-ray spectra of GRBs
• Principal component analysis of the reionization history from Planck 2015 data
• Fugacity and Reheating of Primordial Neutrinos
• Dark Matter Annihilation in the Universe
• Joint Constraints on Neutrinos and Dynamical Dark Energy in Minimally Modified Gravity
• The Shared Causal Pasts and Futures of Cosmological Events
• Decadal Mission for the New Physics Higgs/Flavor Era
• Probing spatial orientability of Friedmann--Robertson--Walker spatially flat spacetime
• Observational constraints on the unified dark matter and dark energy model based on the quark bag model
• CP violation in the extension of SM with a complex singlet scalar and vector quarks
• HESS J1943+213: a non-classical high-frequency-peaked BL Lac object
• Taylor expansion of luminosity distance in Szekeres cosmological models: Effects of local structures evolution on cosmographic parameters
• Higgsino-like Dark Matter From Sneutrino Late Decays
• Dark Photon as Fractional Cosmic Neutrino Masquerader
• Possible Impact of non-Gaussianities on cosmological constraints in neutrino physics
• Measuring the growth of structure by matching dark matter haloes to galaxies with VIPERS and SDSS
• Cosmic Variance and the Inhomogeneous UV Luminosity Function of Galaxies During Reionization
• A Simple Gravitational Lens Model For Cosmic Voids
• Cloud access to interoperable IVOA-compliant VOSpace storage
• Improving Constraint on ${\Omega }_m$ from SDSS Using Marked Correlation Functions
• Electromagnetic Casimir densities for a cylindrical shell on de Sitter space
• Axion-like Particles from String Compactifications
• Cosmological Parameter Estimation with a Joint-Likelihood Analysis of the Cosmic Microwave Background and Big Bang Nucleosynthesis
• Effective Field Theory of Majorana Dark Matter
• LSP baryogenesis and neutron-antineutron oscillations from R-parity violation
• The kinetic Sunyaev-Zel'dovich effect from the diffuse gas in the Local Group
• Low Energy Gamma Ray Excess Confronting a Singlet Scalar Extended Inert Doublet Dark Matter Model
• Does nonlocal gravity yield divergent gravitational energy-momentum fluxes?
• Another coincidence problem for $\Lambda$CDM?
• Physical Cosmological Constant in Asymptotically Background Free Quantum Gravity
• Growth of cosmic perturbations in the modified $f(R,T)$ gravity
• The Physical Nature of the Most Metal-Poor Damped Lyman Alpha Systems
• Distinguishing between inhomogeneous model and $\Lambda \text{CDM}$ model with the cosmic age method
• Dynamical evolution of quintessence cosmology in a physical phase space
• Dwarf Galaxy $\gamma$-excess and 3.55 keV X-ray Line In A Nonthermal Dark Matter Model
• Dual models of the neutrino mass spectrum
• Interacting dark energy: the role of microscopic feedback in the dark sector
• Power spectrum oscillations from Planck-suppressed operators in effective field theory motivated monodromy inflation
• Spatial variation of fundamental constants: testing models with thermonuclear supernovae
• The case for two-dimensional galaxy-galaxy lensing
• Light WIMPs, Equivalent Neutrinos, BBN, and the CMB
• Can supermassive stars form in protogalaxies due to internal Lyman-Werner feedback?
• CMB Cold Spot from Inflationary Feature Scattering
• Dark photon - dark energy stationary axisymmetric black holes
• The galaxy power spectrum on the lightcone: deep, wide-angle redshift surveys and the turnover scale
• Contamination of Dark Matter Experiments from Atmospheric Magnetic Dipoles
• The luminosity of cluster galaxies in the Cluster-EAGLE simulations
• NIHAO-RiNG: A Comparison of Simulated Disc Galaxies from GASOLINE and GIZMO
• Detections of simultaneous brightening of gamma-ray and optical emissions of a distant blazar GB 1508+5714 at redshift 4.3
• LHC and dark matter phenomenology of the NUGHM
• Can an Anti-de Sitter Vacuum in the Dark Energy Sector Explain JWST High-Redshift Galaxy and Reionization Observations?
• Using Artificial Intelligence and real galaxy images to constrain parameters in galaxy formation simulations
• Weak lensing corrections to tSZ-lensing cross correlation
• Effects of chemically homogeneous evolution of the first stars on the 21-cm signal and reionization
• Accurate renormalization group analyses in neutrino sector
• What is the optimal way to measure the galaxy power spectrum?
• On the recovery of ISW fluctuations using large-scale structure tracers and CMB temperature and polarization anisotropies
• ICE: a scalable, low-cost FPGA-based telescope signal processing and networking system
• Observational constraints on inflection point quintessence with a cubic potential
• Exact SU(5) Yukawa matrix unification in the General Flavour Violating MSSM
• A model with isospin doublet $U(1{)}_D$ gauge symmetry
• Direct detection of dark matter with resonant annihilation
• Right-handed sneutrinos as asymmetric DM and neutrino masses from neutrinophilic Higgs bosons
• BICEP's acceleration
• Simple brane-world inflationary models: an update
• Dark matter component decaying after recombination: constraints from diffuse gamma-ray and neutrino flux measurements
• Comparison of results on $N_{\mathrm{eff}}$ from various Planck likelihoods
• Emergent D-instanton as a source of Dark Energy
• The effects of environment on galaxies' dynamical structures: From simulations to observations
• Energy injection in pre-recombination era and EDGES detection
• Constraints on Dark Energy from New Observations including Pan-STARRS
• The influence of weak lensing on measurements of the Hubble constant with quad-image gravitational lenses
• Ellipticity and prolaticity of the initial gravitational-shear field at the position of density maxima
• Inflation as de Sitter instability
• Beyond boundaries of redshift surveys: assessing mass fluctuations on "super-survey" scales
• Disc galaxy resolved in HI absorption against the radio lobe of 3C 433: Case study for future surveys
• Constraining Neutrinos and Dark Energy with Galaxy Clustering in the Dark Energy Survey
• The fate of the interstellar medium in early-type galaxies. IV. The impact of stellar feedback, mergers, and black holes on the cold ISM in simulated galaxies
• A lower bound on light neutralino dark matter from LHC data
• Enhancing CMB map reconstruction and power spectrum estimation with convolutional neural networks
• Weak Lensing by Minifilament or Minivoid as the Origin of Flux-ratio Anomalies in Lensed Quasar MG0414+0534
• Early formed astrophysical objects and cosmological antimatter
• Three-stage Collapse of the Long Gamma-Ray Burst from GRB 160625B Prompt Multiwavelength Observations
• Local variations of the Stellar Velocity Ellipsoid-I: the disc of galaxies in the Auriga simulations
• Updated Constraints on Large Field Hybrid Inflation
• Measuring the velocity field from type Ia supernovae in an LSST-like sky survey
• Reconstruction of the scalar field potential in nonmetricity gravity through Gaussian processes
• Next to new minimal standard model
• Non-Virialized Axion Search Sensitive to Doppler Effects in the Milky Way Halo
• Constraining cosmology with the velocity function of low-mass galaxies
• The Texture One Zero Neutrino Mass Matrix With Vanishing Trace
• Nonlinear evolution of density and flow perturbations on a Bjorken background
• The Thermal Sunyaev-Zeldovich Effect of Primordial Recombination Radiation
• Holography and matter creation revisited
• Compton Scattering Energy Spectrum for Si and Ge Systems
• Efficiently estimating mean, uncertainty and unconstrained large scale fraction of local Universe simulations with paired fixed fields
• Dark photon production via $\gamma \gamma \to \gamma A^{\prime }$
• Null geodesic structure for the Barriola-Vilenkin spacetime via $k$-essence
• Prospects of a statistical detection of the 21-cm forest and its potential to constrain the thermal state of the neutral IGM during reionization
• The Diffusion Coefficient of the Splashback Mass Function as a Probe of Cosmology
• The internal metallicity distributions of simulated galaxies from EAGLE, Illustris, and IllustrisTNG at z=1.8-4 as probed by Gamma Ray Burst hosts
• VLA detects CO(1-0) emission in the z=3.65 quasar SDSS J160705+533558
• Non-Linear Resonance in Relativistic Preheating
• Cosmological inference including massive neutrinos from the matter power spectrum: biases induced by uncertainties in the covariance matrix
• Cosmology with Recombination Spectrum
• Effect of neutrino rest mass on ionization equilibrium freeze-out
• The maximum mass of dark matter existing in compact stars based on the self-interacting fermionic model
• Scale invariance of the primordial tensor power spectrum
• The history of the universe is an elliptic curve
• An $S_4$ model inspired from self-complementary neutrino mixing
• Temporal and Spectral Study of PKS B1222+216 Flares in 2014
• The Linear Perturbation Theory of Reionization in Position-Space: Cosmological Radiative Transfer Along the Light-Cone
• Ultralocal nature of geometrogenesis
• Lyman-alpha Heating of Inhomogeneous High-redshift Intergalactic Medium
• Mimicking the LCDM model with Stealths
• Experimental nuclear astrophysics in Italy
• Neutrino masses and ordering via multimessenger astronomy
• Cosmic Acceleration in a Model of Fourth Order Gravity
• Simulating the dark matter decay signal from the Perseus galaxy cluster
• Non-universal SUGRA at LHC: Prospects and Discovery Potential
• Universe in the light of LHC
• Cosmic-Ray Signatures of Dark Matter from a Flavor Dependent Gauge Symmetry Model with Neutrino Mass Mechanism
• Bose-Einstein condensate and degenerate Fermi cored dark matter halos
• Cosmic curvature on large-scale structures with homogeneous dark energy
• Searching for new physics in the solar system with tetrahedral spacecraft formations
• Bright but slow - Type II supernovae from OGLE-IV - Implications for magnitude limited surveys
• The emergence of globular clusters and globular-cluster-like dwarfs
• Detecting high-$z$ galaxies in the Near Infrared Background
• Constraining hybrid potential scalar field cosmological model in Lyra's geometry with recent observational data
• The correlation of high-redshift galaxies with the thermal Sunyaev-Zel'dovich effect traces reionization
• WHIM-hunting through cross-correlation of optical and SZ effect data in the Virgo cluster filaments
• Star formation and stellar & AGN feedback in the absence of accretion, not gas stripping, set the quenching timescale in satellite galaxies
• Early-Matter-Like Dark Energy and the Cosmic Microwave Background
• Oscillating solutions of the matter density contrast in Horndeski's theory
• Nonparametric test of consistency between cosmological models and multiband CMB measurements
• Inflation in maximal gauged supergravities
• Environmental effects on associations of dwarf galaxies
• Effective scalar four-fermion interaction for Ge-phobic exothermic dark matter and the CDMS-II Silicon excess
• The extent of gravitationally bound structure in a ΛCDM universe
• Non-Equilibrium Aspects of Relic Neutrinos: From Freeze-out to the Present Day
• Helium diffusion during formation of the first galaxies
• Constraining gas metal mixing strength in simulations using observations of the Milky Way's disc
• Higgs Inflation, Seesaw Physics and Fermion Dark Matter
• Implications of mixed axion/neutralino dark matter for the Cosmic Frontier: a Snowmass whitepaper
• Unification Predictions With or Without Supersymmetry
• Commissioning of a dual-phase xenon TPC at Nikhef
• Predictions for surveys with the SPICA Mid-infrared Instrument
• Scale-invariant scalar spectrum from the nonminimal derivative coupling with fourth-order term
• Neutrino oscillations in the presence of super-light sterile neutrinos
• A Framework for Measuring Weak-Lensing Magnification Using the Fundamental Plane
• New near-infrared observations and lens-model constraints for UM673
• Glow in the Dark Matter: Observing galactic halos with scattered light
• SUSY effects in Higgs productions at high energy $e^{+}{e}^{-}$ colliders
• From Peccei Quinn symmetry to mass hierarchy problem
• Semi analytical description of formation of galaxies and clusters of galaxies
• Sensitivity analysis of a galaxy formation model
• Modified $f(R,T)$ theory in light of gravitational wave standard sirens
• Origin Of The Cosmic Ray Positrons Observed Near Earth- Meson Decay Or Dark Matter Decay?
• Thawing vs. Tracker Solutions: A Dynamical Systems Approach
• Exploring CP-violation in $Y=0$ inert triplet with real singlet
• Probing Electroweak Phase Transition in Extended Singlet Scalar Model with Resonant $HH$ production in $bbZZ$ Channel using Parameterized Machine Learning
• Spectator Higgs, large-scale gauge fields and the non-minimal coupling to gravity
• Distribution of fast radio burst dispersion measures in CHIME/FRB Catalog 1: implications on the origin of FRBs
• Hypermagnetic knots and gravitational radiation at intermediate frequencies
• De Sitter Vacua from a D-term Generated Racetrack Uplift
• The strongest gravitational lenses: IV. The order statistics of the largest Einstein radii with cluster mergers
• Confronting Dirac Fermionic Dark Matter with Recent Data
• Effect of noncircularity of experimental beam on CMB parameter estimation
• A non-perturbative study of the evolution of cosmic magnetised sources
• Relativistic matter bispectrum of cosmic structures on the light cone
• Awakening of two $\gamma$-ray high redshift flat-spectrum radio quasars in the southern hemisphere
• Affleck-Dine baryogenesis after D-term inflation and solutions to the baryon-DM coincidence problem
• New measures to test modified gravity cosmologies
• A Pop III generated dust screen at z~16
• Vacuum energy, the Casimir effect, and Newton's non-constant
• The north-south asymmetry of the ALFALFA HI velocity width function
• Degeneracy in the spectrum and bispectrum among featured inflaton potentials
• Extreme gas kinematics in an off-nuclear HII region of SDSS J143245.98+404300.3
• Constraining ultra light fermionic dark matter with Milky-Way observations
• Soft Gamma Rays from Heavy WIMPs
• Higher-Order Spectra of Weak Lensing Convergence Maps in Parameterized Theories of Modified Gravity
• Constraining stochastic gravitational wave background from weak lensing of CMB B-modes
• Phenomenology of Baryogenesis from Lepton-Doublet Mixing
• Bandpass mismatch error for satellite CMB experiments II: Correcting for the spurious signal
• The Value of $H_0$ from Gaussian Processes
• Geometric phases and cyclic isotropic cosmologies
• Mass content of UGC 6446 and UGC 7524 through HI rotation curves: deriving the stellar discs from stellar population synthesis models
• Muon anomalous magnetic moment and positron excess at AMS-02 in a gauged horizontal symmetric model
• Buchdahl bound, photon ring, ISCO and radial acceleration in Einstein-æther theory
• Preliminary test results of LAr prototype detector
• Simulating the collapse of rotating primordial gas clouds to study the survival possibility of Pop III protostars
• Bouncing cosmological model with general relativistic hydrodynamics in extended gravity
• Neutrino Physics Now and in the Near Future
• Results and prospects of dark matter searches with ANTARES
• A possible relation between global CO excitation and massive molecular outflows in local ULIRGs
• Stability of small-scale baryon perturbations during cosmological recombination
• Leptogenesis in GeV scale seesaw models
• Modelling the impact of intrinsic size and luminosity correlations on magnification estimation
• Lognormal semi-numerical simulations of the Lyman-$\alpha$ forest: comparison with full hydrodynamic simulations
• Properties of Central Regions of the Dark Matter Halos in the Model with a Bump in the Power Spectrum of Density Perturbations
• The influence of baryons on low-mass haloes
• Conversations in the dark: cross-correlating birefringence and LSS to constrain axions
• Ether and Relativity
• The Formation and Evolution of Massive Galaxies
• Beginning of Universe through large field hybrid inflation
• C2-GaMe: Classification of Cluster Galaxy Membership with Machine Learning
• All Fermion Masses and Mixings in an Intersecting D-brane World
• Accurate halo mass functions from the simplest excursion set theory
• Detection of the Intrinsic Spin Alignments in Isolated Spiral Pairs
• Constraining primordial vector mode from B-mode polarization
• Massive neutrinos in nonlinear large scale structure: A consistent perturbation theory
• Dynamical systems analysis of a cosmological model with interacting Umami Chaplygin fluid in adiabatic particle creation mechanism: Some bouncing features
• Exploring the deviation of cosmological constant by a generalized pressure dark energy model
• The consistency test on the cosmic evolution
• Effect of a partial coverage of quasar broad-line regions by intervening H${}_2$-bearing clouds
• D = 1 supergravity and quantum cosmology
• Reionization and CMB non-Gaussianity
• Varying linear polarisation in the dust-free GRB 210610B
• The evolution of low-mass central galaxies in the vicinity of massive structures and its impact on the two-halo conformity
• Effect of Priomordial non-Gaussianities on Galaxy Clusters Scaling Relations
• Constraints on cosmological parameters from Planck and BICEP2 data
• SUSY SU(5) $\times S_4$ GUT Flavor Model for Fermion Masses and Mixings with Adjoint, Large ${\theta }_{13}^{PMNS}$
• A class of regular bouncing cosmologies
• Modeling the Multi-band Light Curves of the Afterglows of Three Gamma-Ray Bursts and Their Associated Supernovae
• Compact groups of galaxies in GAMA -- Probing the densest minor systems at intermediate redshifts
• Perturbative interaction approach to cosmological structure formation
• Effective field theory of coupled dark energy and dark matter
• Relation between the local width and linear halo mass density of cosmic filaments
• Clues to the nature of dark matter from first galaxies
• Structure and Kinematics of Star-forming Elliptical Galaxies in SDSS-MaNGA
• Phenomenology in supersymmetric neutrinophilic Higgs model with sneutrino dark matter
• Pseudo Newtonian Potential For a Rotating Kerr Black Hole Embedded in Quintessence
• Relativistic second-order initial conditions for simulations of large-scale structure
• The Quadratic Approximation for Quintessence with Arbitrary Initial Conditions
• Local variations of the Stellar Velocity Ellipsoid-II: the effect of the bar in the inner regions of Auriga galaxies
• Axions and Dark Matter
• Effects of Angular Momentum on Halo Profiles
• Scalar Dark Matter Candidates in Two Inert Higgs Doublet Model
• Planck and WMAP constraints on generalised Hubble flow inflationary trajectories
• Cosmic Microwave Background Dipole Asymmetry could be explained by Axion Monodromy Cosmic Strings
• Measurement of redshift-space two- and three-point correlation of Ly$\alpha$ absorbers at $1.7<z<3.5$: Implications on evolution of the physical properties of IGM
• Optical dispersion of composite particles consisting of millicharged constituents
• Probing the hyperbolic branch/focus point region of the constrained minimal supersymmetric standard model with generalized Yukawa quasi-unification
• Measurement of low-energy background events due to ${}^{222}$Rn contamination on the surface of a NaI(Tl) crystal
• Precision Experiments at LEP
• Non-linear curvature inhomogeneities and backreaction for relativistic viscous fluids
• Neutrino Mixing and Leptogenesis in $\mu -\tau$ Symmetry
• Magnetic contributions in Bekenstein type models
• Intrinsic alignments of the extended radio continuum emission of galaxies in the EAGLE simulations
• Insights into the evolution of five isolated galaxies
• Analytic Study of Cosmological Perturbations in a Unified Model of Dark Matter and Dark Energy with a Sharp Transition
• Spinning Toroidal Brane Cosmology; A Classical and Quantum Survey
• Extension of Minimal Fermionic Dark Matter Model : A Study with Two Higgs Doublet Model
• Investigating higgsino dark matter in the semi-constrained NMSSM
• The Milky Way in context: The formation of galactic discs and chemical sequences from a cosmological perspective
• Cosmography from accurate mass modeling of the lens group SDSS J0100+1818: five sources at three different redshifts
• Characterising galaxy clusters' completeness function in Planck with hydrodynamical simulations
• Study of thermal stability for different dark energy models
• Low scale leptogenesis under neutrino $\mu$-$\tau$ reflection symmetry
• The Low Redshift survey at Calar Alto (LoRCA)
• From Causal Dynamical Triangulations To Astronomical Observations
• String Theory clues for the low-$\ell$ CMB ?
• Predicting Localized Primordial Star Formation with Deep Convolutional Neural Networks
• Naturally large tensor-to-scalar ratio in inflation
• Comment on "Hubble flow variations as a test for inhomogeneous cosmology"
• Inflation of Universe by Nonlinear Electrodynamics
• NMSSM with generalized deflected mirage mediation
• Superclustering with the Atacama Cosmology Telescope and Dark Energy Survey: II. Anisotropic large-scale coherence in hot gas, galaxies, and dark matter
• Constraints on the varying electron mass and early dark energy in light of ACT DR6 and DESI DR2 and the implications for inflation
• Galaxy Assembly and Evolution in the P-Millennium simulation: galaxy clustering
• Can the NANOGrav observations constrain the geometry of the universe?
• Role of ionizing background on the non-thermal broadening inferred for the aligned absorbers
• Dark energy with $w\to -1$: Asymptotic $\Lambda$ versus pseudo-$\Lambda$
• Reaching small scales with low frequency imaging: applications to the Dark Ages
• Unveiling acoustic physics of the CMB using nonparametric estimation of the temperature angular power spectrum for Planck
• Constraints on primordial magnetic fields from the optical depth of the cosmic microwave background
• Lyra's cosmology of homogeneous and isotropic universe in Brans-Dicke theory
• Assembly Conformity of Structure Growth: Fossil versus Normal Groups of Galaxies
• Evolution of the spectral index after inflation
• Distinguishing between inflationary models from cosmic microwave background
• Cosmological perturbation theory using generalized Einstein de Sitter cosmologies
• Probing the matter and dark energy sources in a viable Big Rip model of the Universe
• Dark energy with rigid voids versus relativistic voids alone
• Lensing convergence and anisotropic dark energy in galaxy redshift surveys
• FLORAH: A generative model for halo assembly histories
• HI absorption from the epoch of reionization and primordial magnetic fields
• Redshift Horizon for Detecting the First Galaxies in Far-Infared Surveys
• Critical points of the cosmic velocity field and the uncertainties in the value of the Hubble constant
• The Effect of Primordial Anti-Biasing on the Local Measurement of the Key Cosmological Parameters
• Coupling q-deformed dark energy to dark matter
• Galactic chimney sweeping: the effect of 'gradual' stellar feedback mechanisms on the evolution of dwarf galaxies
• The weak connection between the stellar haloes and merger histories of Milky Way-mass galaxies
• Bayesian analysis of multiple direct detection experiments
• Evaluating a Sigmoid Dark Energy Model to Explain the Hubble Tension
• Radio Observations of Star Forming Galaxies in the SKA era
• kSZ Pairwise Velocity Reconstruction with Machine Learning
• Impact of Cosmic Variance on the Galaxy-Halo Connection for Lyman-$\alpha$ Emitters
• The shape of relaxed galaxy clusters and the public release of a HST shape measurement code, pyRRG
• 'Constraint consistency' at all orders in Cosmological perturbation theory
• Can Higgs Inflation be Saved with High-scale Supersymmetry ?
• Enhanced Higgs Mass in Compact Supersymmetry
• DEAP-3600 dark matter experiment
• N-body self-consistent stars-halo modeling of the Fornax dwarf galaxy
• Detecting the relic gravitational wave from the electroweak phase transition at SKA
• A comparison of cosmological models with high-redshift quasars
• Constraining the Higgs portal with antiprotons
• Generalized Conformal Transformation and Inflationary Attractors
• Constraining blazar heating with the 2<z<3 Lyman-$\alpha$ forest
• CMB anisotropies from patchy reionisation and diffuse Sunyaev-Zel'dovich effects
• Constraining the Fast Radio Burst (FRB) properties using the joint distributions of dispersion measure and fluence of the events detected at Parkes, ASKAP, CHIME and UTMOST
• BASILISK II. Improved Constraints on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• Detecting anomalies in CMB maps: a new method
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• NESSiE: The Experimental Sterile Neutrino Search in Short-Base-Line at CERN
• Formation of globular clusters induced by external ultraviolet radiation II: Three-dimensional radiation hydrodynamics simulations
• Dust sub-millimetre emission in green valley galaxies
• Quantifying the effect of field variance on the H$\alpha$ luminosity function with the New Numerical Galaxy Catalogue (${\nu }^2$GC)
• A model with flavor-dependent gauged $U(1{)}_{B-L_1}\times U(1{)}_{B-L_2-L_3}$ symmetry
• Tensor to scalar ratio from single field magnetogenesis
• Heavy neutralino relic abundance with Sommerfeld enhancements - a study of pMSSM scenarios
• Scalar field vs hydrodynamic models in the homogeneous isotropic cosmology
• Late Time Phenomena in $f(T,\mathcal{T})$ Gravity Framework: Role of $H_0$ Priors
• Bounds from multi-messenger astronomy on the Super Heavy Dark Matter
• Sensing and vetoing loud transient noises for the gravitational-wave detection
• Analytical solutions for cosmological perturbations in a one-component universe with shear stress
• The gamma-ray spectral feature from Kaluza-Klein dark matter annihilation and its observability
• Turbulence in Simulated Local Cluster Analogs: One-to-one comparisons between SLOW and XRISM/Hitomi
• The isolated elliptical galaxy NGC 5812 -- MOND or Dark Matter?
• Associations of dwarf galaxies in a $\Lambda$CDM Universe
• Thermodynamics of scalar field models with kinetic corrections
• Inflation of the Universe by the Non-minimal $Y(R)F^2$ Models
• Testing the coupling of dark radiations in light of the Hubble tension
• The Dilaton-like Higgs boson with scalar singlet dark matter
• New Geometric Representations of the CMB 2pcf
• Light Higgsino Dark Matter in the MSSM on D-branes
• The prospects of gravitational waves on constraining the anisotropy of the Universe
• Composite dark matter and direct-search experiments
• A Flaring AGN In a ULIRG candidate in Stripe 82
• Cluster density slopes from Dark Matter-Baryons Energy Transfer
• Baryon Asymmetries in the Natural Inflation Model
• Superluminal Gravitational Waves
• Shadow of quadrupole-deformed compact objects in a local dark matter shell
• Einstein's cosmological considerations
• Quantifying the 'naturalness' of the curvaton model
• The $m$-$z$ relation for Type Ia supernovae: safety in numbers or safely without worry?
• Einstein-aether models III: conformally static metrics, perfect fluid and scalar fields
• From particles to orbits: precise dark matter density profiles using dynamical information
• Neutrino mass in flavor dependent gauged lepton model
• Superconformal generalizations of auxiliary vector modified polynomial f(R) theories
• Dark Matter and Lepton Flavour Violation in a Hybrid Neutrino Mass Model
• GUT-scale inflation with sizeable tensor modes
• End of a Dark Age?
• Exact Solutions and Constraints on the Dark Energy Model in FRW Universe
• Simulations of cm-wavelength Sunyaev-Zel'dovich galaxy cluster and point source blind sky surveys and predictions for the RT32/OCRA-f and the Hevelius 100-m radio telescope
• Effects of high-order operators in non-relativistic Lifshitz holography
• Interpreting gravitational-wave burst detections: constraining source properties without astrophysical models
• The temperature of IGM at high redshifts: shock heating and high mach problem
• Status after the first LHC run: Looking for new directions in the physics landscape
• Auriga Streams II: orbital properties of tidally disrupting satellites of Milky Way-mass galaxies
• The Splashback Mass Function in the Presence of Massive Neutrinos
• Testing extensions to LCDM on small scales with forthcoming cosmic shear surveys
• Hidden Figures in the Sky: Evolution of low-surface brightness galaxies from a hydro-dynamical perspective
• Tsunamis and Ripples: Effects of Scalar Waves on Screening in the Milky Way
• Family Non-Universal U(1)${}^{\prime }$ Model with Minimal Number of Exotics
• Is non-particle dark matter equation of state parameter evolving with time?
• The dynamics of the parsec-scale jet in the neutrino blazar PKS 0735+178
• Probability of Vacuum Stability in Type IIB Multi-Kähler Moduli Models
• Quasiadiabatic modes from viscous inhomogeneities
• Signatures of Synchrotron Radiation from the Annihilation of Dark Matter at the Galactic Centre
• The role of magnetic fields in ram pressure stripping of satellite galaxies in the circumgalactic medium around massive galaxies
• The CMB Derivatives of Planck's Beam Asymmetry
• Deep Extragalactic VIsible Legacy Survey (DEVILS): DR1 Blended Spectra Search for Candidate Strong Gravitational Lenses
• Search for GeV-scale Dark Matter from the Galactic Center with IceCube-DeepCore
• Galaxy mass profiles with convolutional neural networks
• Lithium evolution in the Galactic thin disc from Main-Sequence and early Red-Giant-Branch stars
• Non-linear coupling in the dark sector as a running vacuum model
• Constraining violations of the Weak Equivalence Principle Using CHIME FRBs
• Constraints on millicharged particles by neutron stars
• Power of the redshift drift on cosmological models and expansion history
• Quantum origin of suppression for vacuum fluctuations of energy
• Cosmological blueshifting may explain the gamma ray bursts
• Quantifying the sensitivity of Big Bang Nucleosynthesis to isospin breaking with input from lattice QCD
• A new model of arcsin-gravity
• Radiative corrections to $M_h$ from three generations of Majorana neutrinos and sneutrinos
• Improving photometric redshifts with Ly$\alpha$ tomography
• Detecting deviations from Gaussianity in high-redshift CMB lensing maps
• Large-scale structure power spectrum from scalar-tensor gravity
• Time-like geodesic structure for the K-essence Emergent Barriola-Vilenkin type spacetime
• Multiple solutions in supersymmetry and the Higgs
• Bottom quark contribution to spin-dependent dark matter detection
• Comparison of the Parkes and FAST FRB DM Distribution
• Inflation after Planck: and the winners are
• A Singlet Extension of the MSSM with a Dark Matter Portal
• Inflaton as a pseudo-Goldstone boson of vacuum energy shift symmetry
• All-sky reconstruction of the primordial scalar potential from WMAP temperature data
• Dynamical analysis for a scalar-tensor model with Gauss-Bonnet and non-minimal couplings
• Massive Scalar Field Quantum Cosmology
• Low-$\ell$ CMB from String-Scale SUSY Breaking?
• Cosmic acceleration sourced by modification of gravity without extra degrees of freedom
• Vector-like Sneutrino Dark Matter
• The Early Universe with High-Scale Supersymmetry
• Dynamics of clusters of galaxies with extended $f(\chi )$ gravity
• Evolution of gravity-dark energy coupled expanding universe
• Detecting CMB modulations and non-Gaussianities from power multipoles
• Constraints on Multicomponent Dark Energy from Cosmological Observations
• K-essential covariant holography
• Solar neutrinos as background in dark matter searches involving electron detection
• Quantifying the detection likelihood of faint peaks in interferometric data through jackknifing: Test application on finding $z>10$ galaxy candidates
• Search for cosmic dark matter by means of ultra high purity NaI(Tl) scintillator
• Simultaneously Modelling Dusty Star Forming Galaxies and Massive Quiescents: A Calibration Framework for Galaxy Formation Models
• Foreground removal and angular power spectrum estimation of 21 cm signal using harmonic space ILC method
• H0 tension in Tsallis and Renyi statistics
• Inert scalar dark matter in an extra dimension inspired model
• Classical, quantum, and phenomenological aspects of dark energy models
• Generalized Slow-roll Inflation in Non-minimally Coupled Theories
• Formation and evolution of boxy/peanut bulges in the Auriga cosmological simulations
• Signatures of Solar Chameleons in the Earth's Magnetic Field
• Cosmology from weak lensing of CMB
• Confronting Grand Unification with Lepton Flavour Violation, Dark Matter and LHC Data
• Properties of blueshifted light rays in quasispherical Szekeres metrics
• Supersymmetry with a Heavy Lightest Supersymmetric Particle
• Evolution of the star formation rate surface density main sequence. Insights from a semi-analytic simulation since $z=12$
• A new experiment for the gravitational waves detection
• Mapping the cosmic expansion history from LIGO-Virgo-KAGRA in synergy with DESI and SPHEREx
• On the tomographic cluster clustering as a cosmological probe
• Scrutinizing a di-photon resonance at the LHC through Moscow zero
• The presence of a Phantom field in a Randall-Sundrum scenario
• Dispersion Measures of Fast Radio Bursts through the Epoch of Reionization
• The environment of QSO triplets at 1 $\lesssim$ z $\lesssim$ 1.5
• Accounting for Correlations When Fitting Extra Cosmological Parameters
• A new mechanism for dark energy: the adaptive screening
• Cosmic Dawn II (CoDa II): a new radiation-hydrodynamics simulation of the self-consistent coupling of galaxy formation and reionization
• Deprojecting beam systematics for next-generation CMB B-mode searches
• Pre-heating of the intergalactic medium by gravitational collapse and ultraviolet background
• Imprints of Non-Symmetric Dark Matter Halos on Magnetars: A Two-Fluid Perspective
• Assessing the connection between galactic conformity and assembly-type bias
• The Majorana neutrino mass matrix indicated by the current data
• Stability of HDE model with sign-changeable interaction in Brans-Dicke theory
• Neutrino Interactions with perturbed Rastall Gravity: A Novel Approach to Reducing the Hubble Tension
• General relativity and cosmology
• Calculation of primordial abundances of light nuclei including a heavy sterile neutrino
• Planck's Constant as a Dynamical Field & Path Integral
• The Effects of Dark Matter Annihilation and Dark Matter-Baryon Velocity Offsets at Cosmic Dawn
• Viscous modes, isocurvature perturbations and CMB initial conditions
• Independent Measurements of the Dynamical Masses of Six Galaxy Clusters in the Local Universe
• Numerical effects on the stripping of dark matter and stars in IllustrisTNG galaxy groups and clusters
• Imprints of the redshift evolution of double neutron star merger rate on the signal to noise ratio distribution
• Study of dependence of ram pressure stripping on the orbital parameters of the galaxies
• Systematic Study of the Inner Structure of Molecular Tori in Nearby U/LIRGs using Velocity Decomposition of CO Rovibrational Absorption Lines
• Natural Inflation from 5D SUGRA and Low Reheat Temperature
• Gravitational entropy of cosmic expansion
• The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: Growth rate of structure measurement from cosmic voids
• Barboza-Alcaniz Equation of State Parametrization : Constraining the Parameters in Different Gravity Theories
• Searching for light WIMPS in view of neutron decay to dark matter
• Geometric sigma model of the Universe
• One String to Rule Them All: Neutrino Masses and Mixing Angles
• The electron plus positron spectrum from annihilation of Kaluza-Klein dark matter in the Galaxy
• Subdominant Dark Matter sterile neutrino resonant production in the light of Planck
• Primordial fluctuations from deformed quantum algebras
• Observational constraints on generic models of non-minimal curvature-matter coupling
• SU(5) unification of two triplet seesaw and leptogenesis with dark matter and vacuum stability
• A Homogeneous and Isotropic Universe in Lorentz Gauge Theory of Gravity
• Reconstructing galaxy star formation histories from COSMOS2020 photometry using simulation-based inference
• Degenerate spectrum in the neutrino mass anarchy with Wishart matrices and implications for $0\nu \beta \beta$ and ${\delta }_{\mathrm{CP}}$
• Distinguishing Orbiting and Infalling Dark Matter Particles with Machine Learning
• Minimal Fine Tuning in Supersymmetric Higgs Inflation
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• Identifying massive black hole binaries via light curve variability in optical time-domain surveys
• Quantitatively rating galaxy simulations against real observations with anomaly detection
• Hypergeometric viable models in $f(R)$ gravity
• Galaxy Cluster Mass Estimation Through The Splashback Radius
• HI-bearing dark galaxies predictions from constrained Local Group simulations: how many and where to find them
• Probing $f(R)$ gravity with PLANCK data on cluster pressure profiles
• The signature of galaxy formation models in the power spectrum of the hydrogen 21cm line during reionization
• Quenching Global Star Formation: Dominance of Gravitational Shock Heating at z<2
• Imprints of relic gravitational waves on pulsar timing
• Prospects for detecting the circum- and intergalactic medium in X-ray absorption using the extended intracluster medium as a backlight
• All one-loop scalar vertices in the effective potential approach
• A note on dark matter and dark energy
• Dark matter and the neutrino portal paradigm
• Collins in Wonderland
• Cornering top-philic dark matter with colliders and cosmology: the importance of QCD corrections
• Chameleon Gravity as an Alternative to Dark Matter
• Constraining Axially Symmetric Bianchi Type I Model with Self-Consistent Recombination History and Observables
• Cosmological parameter fittings with the BICEP2 data
• Landscape View at the Edge of a Mystery
• Xenon Bubble Chambers for Direct Dark Matter Detection
• LHC Dark Matter Signals from Vector Resonances and Top Partners
• Influence of dark photon on magnetized and charged particle orbits around static spherically symmetric black hole
• Supersymmetry - When Theory Inspires Experimental Searches
• A possible geometrical origin of the accelerated expansion of the universe
• Build-up and survival of the disc: From numerical models of galaxy formation to the Milky Way
• Hidden photons with Kaluza-Klein towers
• On Direct Estimation of Density Parameters and Hubble Constant for $\Lambda$CDM Universe using Hubble Measurements
• Measuring photo-ionization rate and mean free path of HeII ionizing photons at $2.5\le z\le 3.6$: Evidence for late and rapid HeII reionization Part-II
• A new perspective on galactic dynamics
• Holographic dark energy reconstruction of $f(T,\mathcal{T})$ gravity
• Relationship between the $\gamma -$ray variability and the pc-scale jet in the blazar 3C 454.3
• Aeos: The Impact of Population III Initial Mass Function and Star-by-Star Models in Galaxy Simulations
• An Optimally Weighted Estimator of the Linear Power Spectrum Disentangling the Growth of Density Perturbations Across Galaxy Surveys
• Exploring the outskirts of the EAGLE disc galaxies
• CMB delensing with deep learning
• A New f(R) Model in the Light of Local Gravity Test and Late-time Cosmology
• Neutrino mass and the Higgs portal dark matter in the ESSFSM
• Peculiar dark matter halos inferred from gravitational lensing as a manifestation of modified gravity
• Cosmic microwave background constraints on coupled dark matter
• Degeneracy and Discreteness in Cosmological Model Fitting
• The frozen vanilla model: Exploring dark sector interactions with delta effective theories
• Exploring Milky Way rotation curves with Gaia DR3: a comparison between $\Lambda$CDM, MOND, and General Relativistic approaches
• Quantum hoop conjecture and a natural cutoff for vacuum energy of a scalar field
• Emergent Universe as an interaction in the dark sector
• Natural Inflation on the brane with a TeV-scale gravity: Parameter constraints after Planck 2015
• Super-horizon second-order perturbations for cosmological random fluctuations and the Hubble-constant problem
• Mapping AdS to dS spaces and back
• The Cosmological Effect of CMB/BAO Measurements
• Primordial magnetogenesis before recombination
• How the Coherent Tides Obstruct the Radial Infalls of Satellite Galaxies onto Clusters
• Lepton Number and Expansion of the Universe
• Forecasting constraints from the cosmic microwave background on eternal inflation
• On the morphology of $\gamma -$ray emission induced by $e^{\pm }$ from annihilating self-interacting dark matter
• Primordial Gravitational Waves and Rescattered Electromagnetic Radiation in the Cosmic Microwave Background
• Flat Space, Dark Energy, and the Cosmic Microwave Background
• Testing the thermal Sunyaev-Zel'dovich power spectrum of a halo model using hydrodynamical simulations
• Astrophysical and Cosmological Relevance of the High-Frequency Features in the Stochastic Gravitational-Wave Background
• Electroweak phase transition with radiative symmetry breaking in Type-II seesaw with inert doublet
• Determining the primordial helium abundance and UV background using fluorescent emission in star-free dark matter haloes
• Blois 2019: highlights and outlook
• ngravs: Distinct gravitational interactions in GADGET-2
• Decoupled Sectors and Wolf-Rayet Galaxies
• Renormalization group invariant of lepton Yukawa couplings
• Quarks to Cosmos: Particles and Plasma in Cosmological evolution
• Effects of transient non-thermal particles on the big bang nucleosynthesis
• Spectator fields and their imprints on the Cosmic Microwave Background
• Bridging Simulations and Observations: New Insights into Galaxy Formation Simulations via Out-of-Distribution Detection and Bayesian Model Comparison
• ATCA detections of massive molecular gas reservoirs in dusty, high-z radio galaxies
• AMiBA: Cluster Sunyaev-Zel'dovich Effect Observations with the Expanded 13-Element Array
• Probing time orientability of spacetime
• Solar System Tests of a New Class of $f(z)$ Theory
• ARCHITECTS I: Impact of subgrid physics on the simulated properties of the circumgalactic medium
• Perspectives for studying the dark energy at z>2 with galaxy surveys
• Impact of Lepton Number Violation at the LHC on Models of Leptogenesis
• On the universality of the halo mass function beyond $\Lambda$CDM cosmology
• On observational signatures of multi-fractional theory
• The S-PLUS Fornax Project (S+FP): An extragalactic catalog covering $\sim$ 5 virial radii around NGC 1399 with galaxy properties
• The hot Hagedorn Universe
• Detection of Unresolved Strongly Lensed Supernovae with 7-Dimensional Telescope
• Constraint on Neutrino Statistics from Cosmological Data
• Uncertainty and bias of cosmology and astrophysical population model from statistical dark sirens
• The Effect of Interstellar Absorption on Measurements of the Baryon Acoustic Peak in the Lyman-α Forest
• Cosmological Dynamics of Exponential Quintessence Constrained by BAO, Cosmic Chronometers, and DES-SN5YR/Pantheon+ Data
• The expansion rate of the intermediate Universe in light of Planck
• Cosmological solutions and observational constraints on 5-dimensional braneworld cosmology with gravitating Nambu-Goto matching conditions
• Triplet fermion WIMP dark matter in the general supersymmetric Georgi-Machacek model
• Effects on sinθ_{12} from perturbation of the neutrino mixing matrix with the partially degenerated neutrino masses
• Theoretical and phenomenological consequences of active and sterile neutrino within Beyond Standard Model framework
• Investigative Study on Preprint Journal Club as an Effective Method of Teaching Latest Knowledge in Astronomy
• A Test for the Zero Mean Hypothesis in Cosmology
• Massive Star Clusters in the Semi-Analytical Galaxy Formation Model L-Galaxies 2020
• On the baryon acoustic oscillation amplitude as a probe of radiation density
• A Jacobian generalization of the pseudo Nambu-Goldstone bosons potential
• Covariant holography of a tachyonic accelerating universe
• Galaxy Velocity Bias in Cosmological Simulations: Towards Percent-level Calibration
• NIHAO-LG: The uniqueness of Local Group dwarf galaxies
• The mass profile of NGC 3377 from a Bayesian approach
• Probe $CP$-violating $H\gamma \gamma$ coupling through interferometry
• Cluster optical depth and pairwise velocity estimation using machine learning
• Halo Merger Tree Comparison: Impact on Galaxy Formation Models
• The Origin of the Orbital Parameter Distribution of Merging Halos
• A New Wavelet Scattering Transform-Based Statistic for Cosmological Analysis of Large-Scale Structure
• Late-Time Hubble Space Telescope Observations of a Hydrogen-Poor Superluminous Supernova Reveal the Power-Law Decline of a Magnetar Central Engine
• Constraining cosmic ray transport models using circumgalactic medium properties and observables
• Overmassive and Undermassive Massive Black Holes: The Role of Environment and Gravitational-Wave Recoils
• Emergence of red, star-forming galaxies (red misfits) in a ΛCDM universe
• Neutrino masses from CMB B-mode polarization and cosmic growth rate
• Absorption in the 21 cm Hydrogen Line at $z>10$ as a Sensitive Tool for the Construction of a Cosmological Model on Small Scales
• Impact of anisotropic photon emission from sources during the epoch of reionisation
• Impact on Astrophysics and Elementary Particle Physics of recent and future solar neutrino data
• Gravitational potential wells and the cosmic bulk flow
• The Effect of Large Optical Depths on the Non-Gaussian 21-cm signal from Cosmic Dawn
• Stirring Things Up: Bar-induced substructures in the stellar halo of a cosmological Milky Way analogue
• A new unified model of dark matter and dark energy in 5-dimensional $f(R,\varphi )$ gravity
• Impact of small scale inhomogeneities on observations of standard candles
• Modeling the Cosmological Lyman-$\alpha$ Forest at the Field Level
• Isochronous solutions of Einstein's equations and their Newtonian limit
• From $U(1)\times U(1)$ Symmetry Breaking to Majoron Cosmology: Insights from NANOGrav 15-year Data
• Searching for X-ray sources in nearby late-type galaxies with low star formation rates
• Cosmology with Type II Supernovae
• Selecting Clusters and Protoclusters via Stellar Mass Density: II. Application to HSC-SSP Observations
• Tight correlation of star formation with [Ci] and CO lines across cosmic time
• Cosmological solutions with time-delay
• Cosmological Simulations of Satellites around Isolated Dwarf Galaxies
• Star formation efficiency and flattened gradients in M31
• Observational constraints on inflation with the nonlinear sigma fields in light of Plank 2015
• Does History Repeat Itself? Periodic Time Cosmology
• Confronting Einstein Yang Mills Higgs Dark Energy in light of observations
• Selecting Clusters and Protoclusters via Stellar Mass Density: I. Method and tests on Mock HSC-SSP catalogs
• Dark Energy and CMB
• Modified scaling in $k$-essence model in interacting dark energy - dark matter scenario
• Deciphering galaxy images using machine vision -- Combining variational autoencoder and principal component analysis for feature extraction
• Softly Fine-Tuned Standard Model and the Scale of Inflation
• Fisher Matrix Optimization of Cosmic Microwave Background Interferometers
• The Connection between Dusty Star-Forming Galaxies and the First Massive Quenched Galaxies
• Using MiniBooNE neutral current elastic cross section results to constrain 3+1 sterile neutrino models
• Relations between physical observables: what is better?
• Quantum field theory on curved spacetime and the standard cosmological model
• Confronting SUSY GUT with Dark Matter, Sparticle Spectroscopy and Muon $(g-2)$
• Accelerating Kaluza-Klein Universe in Modified Theory of Gravitation
• Robustness of cosmological axion mass limits
• Constraints on the generalized natural inflation after Planck 2018
• Zooming into the neutrino-associated blazar candidate J1718+4239
• Correlations in the matter distribution in CLASH galaxy clusters
• Revisiting Agegraphic Dark Energy in Brans-Dicke Cosmology
• The Formation of Dwarf Galaxy Disks
• Fluids in cosmology
• Euclid: Exploring observational systematics in cluster cosmology -- a comprehensive analysis of cluster counts and clustering
• Local Group timing in Milgromian dynamics. A past Milky Way-Andromeda encounter at z>0.8
• Supermassive Black Hole Binaries: Environment and Galaxy Host Properties of PTA and eLISA sources
• Cosmological implications of electromagnetically interacting dark matter: milli-charged particles and atoms with singly and doubly charged dark matter
• Cold-electron bolometers for future mm and sub-mm sky surveys
• The effect of helium reionization on the Lyman-alpha forest hydrogen flux statistics
• Viscous Cold Dark Matter in agreement with observations
• Stars older than the universe and possible mechanism of their creation
• Dynamical Mass Determinations and Scaling Relations of Early-Type Galaxies
• Cosmology and Quantum Field Theory II: Study of an extended Nambu-Jona-Lasinio model with a Dynamical Coupling
• Complementarity of direct and indirect searches in the pMSSM
• Cosmological Perturbations in Inflationary Models with Anisotropic Space-Time Scaling in Lifshitz Background
• Back to basics: Little Red Dots as galaxies and dust-obscured AGNs in a synthetic NIRCam sky simulated with L-GalaxiesBH
• Radiative transfer of 21-cm line through ionised cavities in an expanding universe
• Parameter estimation from Ly$\alpha$ forest in Fourier space using Information Maximising Neural Network
• Probing Time-Dependent Dark Energy with the Flux Power Spectrum of the Lyman $\alpha$ Forest
• Interacting tachyon with varying mass dark matter
• Cosmological measurements from the CMB and BAO are insensitive to the tail probability in the assumed likelihood
• Refitting cosmological data with neutrino mass and degeneracy
• Modified Compton Effect and CMB Anisotropy
• Implications of the Fermi-LAT Pass 8 Galactic Center Excess on Supersymmetric Dark Matter
• Off-center black hole seed formation? Implications for high and low redshift massive black holes
• Cosmography via stellar archaeology of low-redshift early-type galaxies from SDSS
• Reionization in HESTIA: Studying reionization in the LG through zoom simulations
• $G_3$ -- interacting scalar tensor dark energy
• EDGE-INFERNO: How chemical enrichment assumptions impact the individual stars of a simulated ultra-faint dwarf galaxy
• The formation of blue cluster in local Universe
• Asymmetry and non-random orientation of the inflight effective beam pattern in the WMAP Data
• A radiative Type-II seesaw model with broken Symmetry Ansatz
• Radio constraints on Galactic WIMP dark matter
• Confronting the Inert Doublet Model with results from Run 1 of the LHC
• Using diffuse radio emission in clusters of galaxies to probe the cosmic web, cosmic rays and dark matter
• Axions/Axion like particles and the CMB asymmetric dipole
• Dipole Modulation in Tensor Modes: Signatures in CMB Polarization
• Machine Learning for Galactic Archaeology: A chemistry-based neural network method for identification of accreted disc stars
• Experimental constraints on anti-gravity and antimatter, in the context of dark energy
• Searching for Vector-Like Quarks in a Fermionic Dark Matter Model with Pseudoscalar: A Resonance Case
• Electromagnetic vacuum stresses and energy fluxes induced by a cosmic string in de Sitter spacetime
• Recent Progress in Cosmology and Particle Astrophysics
• On Quantum Contributions to Black Hole Growth
• Unbinned halo-independent methods for emerging dark matter signals
• Efficient neutral-IGM inference from noisy 21-cm forest spectra with latent-space U-Net encoding and XGBoost
• Size-scaling of clump instabilities in turbulent, feedback regulated disks
• Searching for light WIMPS via their interaction with electrons
• Non-thermal Dark Matter: A Selective Apercu
• Cosmological constraints on sterile neutrino Dark Matter production mechanisms
• Can accelerated expansion of the universe be due to spacetime vorticity?
• Confronting phantom inflation with Planck data
• Power-law and Logarithmic Entropy Corrected Holographic Dark Energy Models in Brans-Dicke Cosmology with Granda-Oliveros Cut-Off
• Spherically Symmetric Potentials in Quadratic $f(R)$ Gravity
• A dynamics-based density profile for dark haloes. I. Algorithm and basic results
• Timing the last major merger of galaxy clusters with large halo sparsity
• Observed structural parameters of EAGLE galaxies: reconciling the mass-size relation in simulations with local observations
• Neutrino physics from Cosmology
• The need to refine the standard recombination theory and the Hubble tension problem
• High redshift constraints on dark energy models from the $E_{\mathrm{p},\mathrm{i}}$ -- $E_{\mathrm{iso}}$ correlation in GRBs
• Aspects of $(d+D)$-dimensional Anisotropic Conformal Gravity
• High-Energy Neutrino Production in Clusters of Galaxies
• Siblings, friends and acquaintances: Testing galaxy association methods
• Cosmology with Coupled Gravity and Dark Energy
• Time Evolution of Optical Darkness in GRB Afterglow: The Case of GRB 240825A
• KURVS: chemical properties from multiple strong line calibrations for star-forming galaxies at $z\sim 1.5$
• The Impact of Star Formation Histories on the Inner Dark Matter Density Slopes of Galaxies
• Exploring the constraints on cosmological models with CosmoEJS
• The Journey to Dominance: How BCGs Evolve Differently from Other Massive Galaxies
• Fitting BICEP2 with defects, primordial gravitational waves and dust
• Revisiting the equation of state of dark energy from DESI BAO with SNe Ia and CMB
• Nearly scale-invariant power spectrum and quantum cosmological perturbations in the gravity's rainbow scenario
• Structure of cosmic web in non-linear regime: the nearest neighbour and spherical contact distributions
• Axion production and CMB spectral distortion in cosmological tangled magnetic field
• No-Scale Supergravity in the Light of LHC and Planck
• Measuring neutrino dynamics in NMSSM with a right-handed sneutrino LSP at the ILC
• Spin-density and Vorticity Contribution to the Cosmological Background
• The Primordial Magnetic Field (PMF) Generated in Large Field Inflation (LFI), Natural Inflation (NI) and $R^2$-Inflation by $f^{2}FF$ Model
• AMICO galaxy clusters in KiDS-DR3: the impact of estimator statistics on the luminosity-mass scaling relation
• Random walks around black holes and low-frequency X-ray variability
• GRB 160410A: the first Chemical Study of the Interstellar Medium of a Short GRB
• The effects of self-interacting dark matter on the stripping of galaxies that fall into clusters
• On Generalized Theories of Varying Fine Structure Constant
• Dwarf stellar haloes: a powerful probe of small-scale galaxy formation and the nature of dark matter
• Nuclear Physics and Astrophysics of Neutrino Oscillations
• Eclipsing negative-parity image of gravitational microlensing by a giant-lens star
• On the Formation of Warped Gas Disks in Galaxies
• Effect of the cosmological transition to metal-enriched star-formation on the hydrogen 21-cm signal
• SKA studies of nearby galaxies: star-formation, accretion processes and molecular gas across all environments
• Star-forming S0 Galaxies in SDSS-MaNGA: fading spirals or rejuvenated S0s?
• Inflationary epoch in the presence of holographic dark energy
• Impact of LHC Run-1 on particle astrophysics
• The Scaling Relation between Galaxy Luminosity and WHIM Density from EAGLE Simulations with application to SDSS data
• Flavor Mixing Phenomenology in Supersymmetric Models
• Maximally localized states and quantum corrections of black hole thermodynamics in the extreme case with an improved exponential GUP
• SUSY Dark Matter: Beyond the Standard Paradigm
• Profiles of cosmic filaments since z=4.0 in cosmological hydrodynamical simulation
• Fermion Masses and Mixings from a Minimum Principle
• Interacting dark matter and q-deformed dark energy non-minimally coupled to gravity
• Large-scale structure with superhorizon isocurvature dark energy
• Gravitino DM and high reheating temperatures after LHC 7/8
• How many new particles do we need after the Higgs boson?
• Turbulence in the intragroup and circumgalactic medium
• Exploring Heavy Higgs Bosons at a 100 TeV Hadron Collider within the Semi-Constrained NMSSM
• On the material origin of the cosmological constant
• Asymmetric Velocity Distributions from Halo Density Profiles in the Eddington Approach
• Antihelium-3 Sensitivity for the GRAMS Experiment
• Controlled Tension Forecasting: Quantifying Cross-Probe Biases in ${\omega }_0{\omega }_a$CDM
• Convergence and shear statistics in galaxy clusters as a result of Monte Carlo simulations
• Unveiling the properties of galaxy cores excavated by supermassive black hole binaries with SHARP
• Dark energy model selection with current and future data
• Prospects for Slepton Searches in Future Experiments
• Influence from cosmological uncertainties on galaxy number count at faint limit
• Improved Methods for Estimating Peculiar Velocity Correlation Functions Using Volume Weighting
• Gaia-Sausage-Enceladus: Lithium evolution from early red-giant-branch and main-sequence stars
• The Splashback Mass Function of Galaxy Clusters from Photometric Data
• Nearest Neighbour-Based Statistics for 21cm-Galaxy Cross-Correlations in the Epoch of Reionization
• Using the EAGLE simulations to elucidate the origin of disc surface brightness profile breaks as a function of mass and environment
• Model-independent reconstruction of cosmic thermodynamics and dark energy dynamics
• Unified Dark Matter from a Simple Gauge Group on a Domain-Wall Brane
• Finite inflation in curved space
• Interpretability of deep-learning methods applied to large-scale structure surveys
• Nonlinear Lattice Framework for Inflation: Bridging stochastic inflation and the $\delta N$ formalism
• Using Mineral Oil to Improve the Performance of Multi-Crystal Detector for Dark Matter Searching
• Fluctuation of the Hubble parameter
• Gravitational Wave Measurement of the $M_{\mathrm{BH}}$-$M_{\mathrm{bulge}}$ Intrinsic Scatter at High Redshift
• Higgs, di-Higgs and tri-Higgs production via SUSY processes at the LHC with 14 TeV
• Recent results and perspectives on cosmology and fundamental physics from microwave surveys
• Probing dark energy with braneworld cosmology in the light of recent cosmological data
• A Mass Dependent Density Profile from Dwarfs to Clusters
• D-brane Standard Model-Like and Scalar Dark Matter in Type IIA Superstring Theory
• Void spin distribution as a powerful probe of ${\sigma }_8$
• Searching for a signature of turnaround in galaxy clusters with convolutional neural networks
• Extreme value statistics of CMB lensing deflection angles
• Optimizing Foreground Modelling for Global 21cm Cosmology with GPU-Accelerated Nested Sampling
• BICEP/Keck XXI: Constraints on Early-Universe Parity Violation from Multipole-Dependent Birefringence
• The optical-infrared relation for active galactic nuclei: The role of contaminations
• Place of the Radcliffe Wave in the Local System
• A first linear cosmological structure formation scenario under extended gravity
• Noether gauge symmetry of Dirac field in $2+1$ dimensional gravity
• Uniformity of Cosmic Microwave Background as a Non-Inflationary Geometrical Effect
• The LHC upper bounds for $pp\to \text{diboson}$, $t\bar{t}$ cross section on fermionic dark matter
• Classification of Radio Backgrounds at Cosmic Dawn and 21 cm Signal Confirmation Using Neural Networks
• One-dimension quantum systems in the framework of the most general deformation GUP form
• Unweaving the Fabric of the Universe: The Interplay between Mathematics and Physics
• Analytically expressed constraint on two Majorana phases in neutrinoless double beta decay
• The chemodynamical memory of a major merger in a NIHAO-UHD Milky Way analogue -- I. A golden thread through time and space
• On the absence of a universal surface density, and a maximum Newtonian acceleration in dark matter haloes: consequences for MOND
• Bimetric Gravity, Variable Speed of Light Cosmology and Planck2013
• Shape, alignment, and mass distribution of baryonic and dark-matter halos in one EAGLE simulation
• Criticality and Big Brake singularities in the tachyonic evolutions of closed Friedmann universes with cold dark matter
• Extended H$\alpha$ over compact far-infrared continuum in dusty submillimeter galaxies -- Insights into dust distributions and star-formation rates at $z\sim 2$
• Stochastic gravitational wave background from the collisions of dark matter halos
• Hybrid Anomaly and Gravity Mediation for Electroweak Supersymmetry
• Implications of correlations and fluctuations in small systems
• Inflationary study of non-Gaussianity using two-dimensional geometrical measures of CMB temperature maps