The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics

Abstract

The standard model of cosmology has provided a good phenomenological description of a wide range of observations both at astrophysical and cosmological scales for several decades. This concordance model is constructed by a universal cosmological constant and supported by a matter sector described by the standard model of particle physics and a cold dark matter contribution, as well as very early-time inflationary physics, and underpinned by gravitation through general relativity. There have always been open questions about the soundness of the foundations of the standard model. However, recent years have shown that there may also be questions from the observational sector with the emergence of differences between certain cosmological probes. In this White Paper, we identify the key objectives that need to be addressed over the coming decade together with the core science projects that aim to meet these challenges. These discordances primarily rest on the divergence in the measurement of core cosmological parameters with varying levels of statistical confidence. These possible statistical tensions may be partially accounted for by systematics in various measurements or cosmological probes but there is also a growing indication of potential new physics beyond the standard model. After reviewing the principal probes used in the measurement of cosmological parameters, as well as potential systematics, we discuss the most promising array of potential new physics that may be observable in upcoming surveys. We also discuss the growing set of novel data analysis approaches that go beyond traditional methods to test physical models. [Abridged]

arXiv comment416 pages, 81 figures

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• Lyman-alpha constraints on warm and on warm-plus-cold dark matter models
• WMAP constraints on low redshift evolution of dark energy
• Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Modeling Uncertainty
• Shear calibration biases in weak lensing surveys
• Inflationary Universe with Anisotropic Hair
• Large-scale instability in interacting dark energy and dark matter fluids
• Big-Bang Nucleosynthesis After Planck
• Weak lensing for precision cosmology
• Suppressing the lower Multipoles in the CMB Anisotropies
• On the Hubble constant tension in the SNe Ia Pantheon sample
• Halo Properties in Cosmological Simulations of Self-Interacting Cold Dark Matter
• Future of the universe in modified gravitational theories: Approaching to the finite-time future singularity
• Early dark energy, the Hubble-parameter tension, and the string axiverse
• Cosmological Constraints on Late-time Entropy Production
• A Map of the Universe
• Fundamental Physics with the Square Kilometre Array
• An introduction to the Vainshtein mechanism
• A White Paper on keV Sterile Neutrino Dark Matter
• The Linear Theory Power Spectrum from the Lyman-alpha Forest in the Sloan Digital Sky Survey
• On initial conditions for the Hot Big Bang
• Towards a realistic population of simulated galaxy groups and clusters
• Curvature tension: evidence for a closed universe
• Planck 2018 results. III. High Frequency Instrument data processing and frequency maps
• The Quest for B Modes from Inflationary Gravitational Waves
• The TianQin project: current progress on science and technology
• The Hubble Diagram to Redshift >6 from 69 Gamma-Ray Bursts
• The halo mass function from the dark ages through the present day
• Any Light Particle Search II -- Technical Design Report
• Signatures of Relativistic Neutrinos in CMB Anisotropy and Matter Clustering
• TDCOSMO IV: Hierarchical time-delay cosmography -- joint inference of the Hubble constant and galaxy density profiles
• The $\nu$MSM, Inflation, and Dark Matter
• The intergalactic magnetic field constrained by Fermi/LAT observations of the TeV blazar 1ES 0229+200
• Extended Gravity Theories and the Einstein-Hilbert Action
• Lorentz violation at high energy: concepts, phenomena and astrophysical constraints
• The most metal-poor galaxies
• Hubble Space Telescope Fine Guidance Sensor Parallaxes of Galactic Cepheid Variable Stars: Period-Luminosity Relations
• Preheating in the Standard Model with the Higgs-Inflaton coupled to gravity
• ZOBOV: a parameter-free void-finding algorithm
• Cluster Cosmology Constraints from the 2500 deg${}^2$ SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Baryon acoustic oscillations with Lyman-$\alpha$ forests
• Sterile neutrinos, dark matter, and the pulsar velocities in models with a Higgs singlet
• A CEERS Discovery of an Accreting Supermassive Black Hole 570 Myr after the Big Bang: Identifying a Progenitor of Massive z > 6 Quasars
• Reconciling Planck with the local value of $H_0$ in extended parameter space
• Extended Gravity Cosmography
• The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
• Tsallis Holographic Dark Energy
• Third Data Release of the Hyper Suprime-Cam Subaru Strategic Program
• Shadow of a black hole surrounded by dark matter
• Dark matter production in the early Universe: beyond the thermal WIMP paradigm
• Tip of the Red Giant Branch Distances. II. Zero-Point Calibration
• Cosmography: Cosmology without the Einstein equations
• Cosmology with the Laser Interferometer Space Antenna
• Oscillating scalar fields and the Hubble tension: a resolution with novel signatures
• Gauge Fields and Inflation
• Strong coupling in Horava gravity
• Dark Matter and Collider Phenomenology of Universal Extra Dimensions
• Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension
• Evidence for Astrophysical Muon Neutrinos from the Northern Sky with IceCube
• Quantum escape of sudden future singularity
• KiDS+VIKING-450: Cosmic shear tomography with optical+infrared data
• The Neutrino Puzzle: Anomalies, Interactions, and Cosmological Tensions
• The population of galaxy-galaxy strong lenses in forthcoming optical imaging surveys
• Solutions to Horava Gravity
• The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters
• Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions
• Phenomenology of a realistic accelerating universe using only Planck-scale physics
• Dark Energy Anisotropic Stress and Large Scale Structure Formation
• Teleparallel Theories of Gravity: Illuminating a Fully Invariant Approach
• Tale of stable interacting dark energy, observational signatures, and the $H_0$ tension
• First results from a microwave cavity axion search at 24 micro-eV
• The International Pulsar Timing Array second data release: Search for an isotropic Gravitational Wave Background
• The Evolution of the Intergalactic Medium
• Early Dark Energy Does Not Restore Cosmological Concordance
• The Early Data Release of the Dark Energy Spectroscopic Instrument
• On the evidence for a common-spectrum process in the search for the nanohertz gravitational-wave background with the Parkes Pulsar Timing Array
• Lorentz-Violating Vector Fields Slow the Universe Down
• The Quijote simulations
• EGMF Constraints from Simultaneous GeV-TeV Observations of Blazars
• Early results from GLASS-JWST. III: Galaxy candidates at z$\sim$9-15
• Conditions for Reionizing the Universe with A Low Galaxy Ionizing Photon Escape Fraction
• Consistently Large Cosmic Flows on Scales of 100 Mpc/h: a Challenge for the Standard LCDM Cosmology
• ARCADE 2 Measurement of the Extra-Galactic Sky Temperature at 3-90 GHz
• Cosmological constant and vacuum energy: old and new ideas
• Baryons Matter: Why Luminous Satellite Galaxies Have Reduced Central Masses
• Imprints of a Primordial Preferred Direction on the Microwave Background
• Generalized entropy formalism and a new holographic dark energy model
• Axinos as Cold Dark Matter
• HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
• The Laniakea supercluster of galaxies
• Matter Bounce in Horava-Lifshitz Cosmology
• Thermal Gravitino Production and Collider Tests of Leptogenesis
• Large Nongaussianity in Axion Inflation
• Further matters in space-time geometry: $f(R,T,R_{\mu \nu }{T}^{\mu \nu })$ gravity
• Tests of Chameleon Gravity
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Testing gravity with redshift-space distortions using the power spectrum multipoles
• Primordial magnetic fields from pseudo-Goldstone bosons
• Galaxy Formation with BECDM: I. Turbulence and relaxation of idealised haloes
• Highest-frequency detection of FRB 121102 at 4-8 GHz using the Breakthrough Listen Digital Backend at the Green Bank Telescope
• Stress Testing $\Lambda$CDM with High-redshift Galaxy Candidates
• Leptogenesis from Gravity Waves in Models of Inflation
• The fourth data release of the Kilo-Degree Survey: ugri imaging and nine-band optical-IR photometry over 1000 square degrees
• Cosmological Model Predictions for Weak Lensing: Linear and Nonlinear Regimes
• Bounds on very low reheating scenarios after Planck
• Why Baryons Matter: The Kinematics of Dwarf Spheroidal Satellites
• The Cosmology of Modified Gauss-Bonnet Gravity
• The Dark Energy Survey Data Release 2
• Bayesian physical reconstruction of initial conditions from large scale structure surveys
• Core Formation in Dwarf Halos with Self Interacting Dark Matter: No Fine-Tuning Necessary
• Testing the Dark Matter Hypothesis with Low Surface Brightness Galaxies and Other Evidence
• The Physical Mechanisms of Fast Radio Bursts
• Hubble Parameter and Baryon Acoustic Oscillation Measurement Constraints on the Hubble Constant, the Deviation from the Spatially-Flat $\Lambda$cdm Model, The Deceleration-Acceleration Transition Redshift, and Spatial Curvature
• Strong bound on canonical ultra-light axion dark matter from the Lyman-alpha forest
• A measurement of large-scale peculiar velocities of clusters of galaxies: results and cosmological implications
• The Void Phenomenon
• Constraints on a Primordial Magnetic Field
• Multiple Images of a Highly Magnified Supernova Formed by an Early-Type Cluster Galaxy Lens
• Quantum gravity without Lorentz invariance
• One Channel to Rule Them All? Constraining the Origins of Binary Black Holes using Multiple Formation Pathways
• The Carnegie Supernova Project: Light Curve Fitting with SNooPy
• CosmoSIS: modular cosmological parameter estimation
• On the Accuracy of Weak Lensing Cluster Mass Reconstructions
• Planck intermediate results. LVII. Joint Planck LFI and HFI data processing
• Distinguishing Modified Gravity from Dark Energy
• The distribution of dark matter in galaxies
• Cosmological solutions and growth index of matter perturbations in $f(Q)$ gravity
• Dark-matter sterile neutrinos in models with a gauge singlet in the Higgs sector
• Lower limit on the strength and filling factor of extragalactic magnetic fields
• Weighing the Giants IV: Cosmology and Neutrino Mass
• $f(T,\mathcal{T})$ gravity and cosmology
• Constraining Dark Matter-Baryon Scattering with Linear Cosmology
• Towards a precision calculation of $N_{\mathrm{eff}}$ in the Standard Model II: Neutrino decoupling in the presence of flavour oscillations and finite-temperature QED
• Conceptual Design of the International Axion Observatory (IAXO)
• Dissipative hidden sector dark matter
• Particle production during inflation and gravitational waves detectable by ground-based interferometers
• Neutrino masses and cosmology with Lyman-alpha forest power spectrum
• The Atacama Cosmology Telescope: A Catalog of > 4000 Sunyaev-Zel'dovich Galaxy Clusters
• Measuring ${\Omega }_m$ with the ROSAT Deep Cluster Survey
• Cosmic homogeneity demonstrated with luminous red galaxies
• Cosmological implications of ultra-light axion-like fields
• How Massless Neutrinos Affect the Cosmic Microwave Background Damping Tail
• The HST Key Project on the Extragalactic Distance Scale XIII. The Metallicity Dependence of the Cepheid Distance Scale
• Crossing the Phantom Divide: Dark Energy Internal Degrees of Freedom
• Inferring the dark matter power spectrum from the Lyman-alpha forest in high-resolution QSO absorption spectra
• The Energy-Momentum Tensor for Cosmological Perturbations
• KiDS-450 + 2dFLenS: Cosmological parameter constraints from weak gravitational lensing tomography and overlapping redshift-space galaxy clustering
• Thermal production of gravitinos
• Neutrino decoupling including flavour oscillations and primordial nucleosynthesis
• Liquid Xenon Detectors for Particle Physics and Astrophysics
• On average properties of inhomogeneous fluids in general relativity II: perfect fluid cosmologies
• Core Cosmology Library: Precision Cosmological Predictions for LSST
• First measurement of the Hubble constant from a dark standard siren using the Dark Energy Survey galaxies and the LIGO/Virgo binary-black-hole merger GW170814
• Teleparallel equivalent of Gauss-Bonnet gravity and its modifications
• CMB polarization from secondary vector and tensor modes
• High-resolution dark matter density profiles of THINGS dwarf galaxies: Correcting for non-circular motions
• The halo mass function through the cosmic ages
• New constraints on cosmological parameters and neutrino properties using the expansion rate of the Universe to z~1.75
• Constraining the mass of light bosonic dark matter using SDSS Lyman-$\alpha$ forest
• Efficient Formation of Massive Galaxies at Cosmic Dawn by Feedback-Free Starbursts
• An Imprint of Super-Structures on the Microwave Background due to the Integrated Sachs-Wolfe Effect
• A precision calculation of relic neutrino decoupling
• Thermodynamic interpretation of the generalized gravity models with geometry - matter coupling
• Corrections to the Friedmann Equations from LQG for a Universe with a Free Scalar Field
• Gaussian Process Cosmography
• Evidence of vorticity and shear at large angular scales in the WMAP data: a violation of cosmological isotropy?
• Chromo-Natural Inflation: Natural inflation on a steep potential with classical non-Abelian gauge fields
• The central slope of dark matter cores in dwarf galaxies: Simulations vs. THINGS
• Calibrating Redshift Distributions Beyond Spectroscopic Limits with Cross-Correlations
• The small scatter of the baryonic Tully-Fisher relation
• An Improved Distance to NGC 4258 and its Implications for the Hubble Constant
• On the large-angle anomalies of the microwave sky
• The Cosmology of Atomic Dark Matter
• New Extraction of the Cosmic Birefringence from the Planck 2018 Polarization Data
• Axinos as Dark Matter
• Dynamics of scalar perturbations in f(R,T) gravity
• Common-red-signal analysis with 24-yr high-precision timing of the European Pulsar Timing Array: Inferences in the stochastic gravitational-wave background search
• Weakly Self-Interacting Dark Matter and the Structure of Dark Halos
• Parity violation in the Cosmic Microwave Background from a pseudoscalar inflaton
• A new Cepheid distance to the maser-host galaxy NGC 4258 and its implications for the Hubble Constant
• Does the Hubble constant tension call for new physics?
• Distances to Galaxies from the Correlation Between Luminosities and Linewidths. III. Cluster Template and Global Measurements of H0
• The Atacama Cosmology Telescope: A Measurement of the DR6 CMB Lensing Power Spectrum and its Implications for Structure Growth
• The Intrinsic Alignment of Galaxies and its Impact on Weak Gravitational Lensing in an Era of Precision Cosmology
• Effects of Scale-Dependent Non-Gaussianity on Cosmological Structures
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Analysis of potential systematics
• Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances and Weak Lensing
• Cosmological constraints from cosmic shear two-point correlation functions with HSC survey first-year data
• Effect of Photometric Redshift Uncertainties on Weak Lensing Tomography
• The GLASS James Webb Space Telescope Early Release Science Program. I. Survey Design and Release Plans
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Observational systematics and baryon acoustic oscillations in the correlation function
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from the anisotropic power spectrum of the Quasar sample between redshift 0.8 and 2.2
• The Clustering of the SDSS Main Galaxy Sample II: Mock galaxy catalogues and a measurement of the growth of structure from Redshift Space Distortions at $z=0.15$
• Double-Disk Dark Matter
• A Test of the Cosmological Principle with Quasars
• The Uncorrelated Universe: Statistical Anisotropy and the Vanishing Angular Correlation Function in WMAP Years 1-3
• Did Something Decay, Evaporate, or Annihilate during Big Bang Nucleosynthesis?
• Atomic Dark Matter
• Identification and properties of intense star-forming galaxies at redshifts z>10
• Setting the Stage for Cosmic Chronometers. II. Impact of Stellar Population Synthesis Models Systematics and Full Covariance Matrix
• Discovery and properties of ultra-high redshift galaxies ($9<z<12$) in the JWST ERO SMACS 0723 Field
• Barrow holographic dark energy
• Relativistic cosmology and large-scale structure
• First Results from ABRACADABRA-10 cm: A Search for Sub-$\mu$eV Axion Dark Matter
• TPZ : Photometric redshift PDFs and ancillary information by using prediction trees and random forests
• The Zurich Extragalactic Bayesian Redshift Analyzer (ZEBRA) and its first application: COSMOS
• The XXL Survey: I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme
• Extragalactic chemical abundances: do HII regions and young stars tell the same story? The case of the spiral galaxy NGC 300
• On the possible running of the cosmological "constant"
• The Atacama Cosmology Telescope: A Measurement of the Cosmic Microwave Background Power Spectra at 98 and 150 GHz
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in Fourier-space
• Towards a more realistic population of bright spiral galaxies in cosmological simulations
• Axion Cosmology and the Energy Scale of Inflation
• Model independent evidence for dark energy evolution from Baryon Acoustic Oscillations
• Evidence for massive neutrinos from CMB and lensing observations
• To H0 or not to H0?
• Measurement of Baryon Acoustic Oscillations in the Lyman-alpha Forest Fluctuations in BOSS Data Release 9
• Measurements of the E-Mode Polarization and Temperature-E-Mode Correlation of the CMB from SPT-3G 2018 Data
• Weighing the Giants - III. Methods and Measurements of Accurate Galaxy Cluster Weak-Lensing Masses
• The cosmological origin of the Tully-Fisher relation
• Is dark matter with long-range interactions a solution to all small-scale problems of ΛCDM cosmology?
• The universality of the virial halo mass function and models for non-universality of other halo definitions
• Cosmological Relic Density from Minimal Supergravity with Implications for Collider Physics
• Anomaly-Free Gauged R-Symmetry
• An SZ-selected sample of the most massive galaxy clusters in the 2500-square-degree South Pole Telescope survey
• N-flationary magnetic fields
• Correcting Type Ia Supernova Distances for Selection Biases and Contamination in Photometrically Identified Samples
• Spatial variation in the fine-structure constant -- new results from VLT/UVES
• Cosmology of the Lifshitz universe
• Early dark energy from massive neutrinos -- a natural resolution of the Hubble tension
• The Megamaser Cosmology Project. III. Accurate Masses of Seven Supermassive Black Holes in Active Galaxies with Circumnuclear Megamaser Disks
• Acoustic Dark Energy: Potential Conversion of the Hubble Tension
• DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars
• The scaling evolution of cosmological constant
• Phenomenological parameterization of quintessence
• General Constraints on Dark Matter Decay from the Cosmic Microwave Background
• Cosmological Constraints from Galaxy Clusters in the 2500 square-degree SPT-SZ Survey
• Topological Black Holes in Horava-Lifshitz Gravity
• Cosmological implications of Fast Radio Burst / Gamma-Ray Burst Associations
• The Representative XMM-Newton Cluster Structure Survey (REXCESS) of an X-ray Luminosity Selected Galaxy Cluster Sample
• CFHTLenS revisited: assessing concordance with Planck including astrophysical systematics
• The FLAMINGO project: cosmological hydrodynamical simulations for large-scale structure and galaxy cluster surveys
• Type II Supernovae as Standardized Candles
• Cosmic dynamics in the era of Extremely Large Telescopes
• A general test of the Copernican Principle
• Accurate halo-model matter power spectra with dark energy, massive neutrinos and modified gravitational forces
• ETHOS - An Effective Theory of Structure Formation: Dark matter physics as a possible explanation of the small-scale CDM problems
• LoCuSS: The slow quenching of star formation in cluster galaxies and the need for pre-processing
• Is the Observable Universe Consistent with the Cosmological Principle?
• Cosmological Evolution With Interaction Between Dark Energy And Dark Matter
• The International Pulsar Timing Array
• The Physics of Fast Radio Bursts
• DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha Forest
• A comparison of cosmological models using recent supernova data
• A redshift-independent efficiency model: star formation and stellar masses in dark matter halos at z>4
• The IR-resummed Effective Field Theory of Large Scale Structures
• Constraining Early Dark Energy with Large-Scale Structure
• $H_0$ from cosmic chronometers and Type Ia supernovae, with Gaussian Processes and the novel Weighted Polynomial Regression method
• Bayesian Galaxy Shape Measurement for Weak Lensing Surveys -I. Methodology and a Fast Fitting Algorithm
• Searching for WISPy Cold Dark Matter with a Dish Antenna
• ETHOS - An Effective Theory of Structure Formation: From dark particle physics to the matter distribution of the Universe
• Scale invariance, unimodular gravity and dark energy
• The Effective Theory of Quintessence: the w<-1 Side Unveiled
• Testing the stability of fundamental constants with the 199Hg+ single-ion optical clock
• Constraints on the cosmic expansion history from GWTC-3
• A new determination of the primordial He abundance using the HeI 10830A emission line: cosmological implications
• Inflation with a constant rate of roll
• Cosmology and Astrophysics from Relaxed Galaxy Clusters II: Cosmological Constraints
• iPTF16geu: A multiply imaged, gravitationally lensed type Ia supernova
• The pre-launch Planck Sky Model: a model of sky emission at submillimetre to centimetre wavelengths
• Halo mass function: Baryon impact, fitting formulae and implications for cluster cosmology
• Parameter inference with estimated covariance matrices
• Lensing of Fast Radio Bursts as a Probe of Compact Dark Matter
• ECOSMOG: An Efficient Code for Simulating Modified Gravity
• A gravitational-wave measurement of the Hubble constant following the second observing run of Advanced LIGO and Virgo
• Baryon acoustic oscillations from the cross-correlation of Ly$\alpha$ absorption and quasars in eBOSS DR14
• KiDS+GAMA: Cosmology constraints from a joint analysis of cosmic shear, galaxy-galaxy lensing and angular clustering
• Lyman-alpha Constraints on Ultralight Scalar Dark Matter: Implications for the Early and Late Universe
• Resolving the Hubble Tension with New Early Dark Energy
• Elucidating $\Lambda$CDM: Impact of Baryon Acoustic Oscillation Measurements on the Hubble Constant Discrepancy
• Baryon acoustic oscillations at z = 2.34 from the correlations of Ly$\alpha$ absorption in eBOSS DR14
• Planck 2013 results. XXVII. Doppler boosting of the CMB: Eppur si muove
• Dark Energy Survey Year 1 Results: Weak Lensing Mass Calibration of redMaPPer Galaxy Clusters
• Higgs-Dilaton Cosmology: From the Early to the Late Universe
• STRIDES: a 3.9 per cent measurement of the Hubble constant from the strong lens system DES J0408-5354
• Le Chatelier-Braun principle in cosmological physics
• Local determination of the Hubble constant and the deceleration parameter
• Time Delay Cosmography
• Spectroscopic confirmation of two luminous galaxies at $z\sim 14$
• Flux- and volume-limited groups/clusters for the SDSS galaxies: catalogues and mass estimation
• A new cosmic microwave background constraint to primordial gravitational waves
• A Hubble Diagram for Quasars
• Cosmological constraints on exotic injection of electromagnetic energy
• A Model For Halo Formation With Axion Mixed Dark Matter
• First Cosmological Results using Type Ia Supernovae from the Dark Energy Survey: Measurement of the Hubble Constant
• Cosmology from gravitational lens time delays and Planck data
• Is the Hubble tension a hint of AdS phase around recombination?
• On the evolution of the Hubble constant with the SNe Ia Pantheon Sample and Baryon Acoustic Oscillations: a feasibility study for GRB-cosmology in 2030
• Confirmation of a Star Formation Bias in Type Ia Supernova Distances and its Effect on Measurement of the Hubble Constant
• Evolution of the $f{\sigma }_8$ tension with the Planck15/$\Lambda$CDM determination and implications for modified gravity theories
• On the Trace-Free Einstein Equations as a Viable Alternative to General Relativity
• Cosmography and constraints on the equation of state of the Universe in various parametrizations
• Analysis of two-point statistics of cosmic shear: I. Estimators and covariances
• Heavy Sneutrinos as Dark Matter
• The Frontier Fields Lens Modeling Comparison Project
• Precision of Hubble constant derived using black hole binary absolute distances and statistical redshift information
• Science with the space-based interferometer eLISA. III: Probing the expansion of the Universe using gravitational wave standard sirens
• The Horizon-AGN simulation: evolution of galaxy properties over cosmic time
• TDCOSMO. I. An exploration of systematic uncertainties in the inference of $H_0$ from time-delay cosmography
• Concordance and Discordance in Cosmology
• Resolving the Radio Source Background: Deeper Understanding Through Confusion
• Thermodynamic approach to holographic dark energy and the Rényi entropy
• On the stunning abundance of super-early, massive galaxies revealed by JWST
• Probing quantum gravity using photons from a flare of the active galactic nucleus Markarian 501 observed by the MAGIC telescope
• WALLABY -- An SKA Pathfinder HI Survey
• Cosmographic analysis of the equation of state of the universe through Padé approximations
• Precision cosmography with stacked voids
• Entropic Accelerating Universe
• Cosmic clocks, cosmic variance and cosmic averages
• Testing modified gravity at cosmological distances with LISA standard sirens
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Measuring D_A and H at z=0.57 from the Baryon Acoustic Peak in the Data Release 9 Spectroscopic Galaxy Sample
• Revealing Galaxy Candidates out to $z\sim 16$ with JWST Observations of the Lensing Cluster SMACS0723
• Echo of interactions in the dark sector
• Prospects for resolving the Hubble constant tension with standard sirens
• Nonparametric Dark Energy Reconstruction from Supernova Data
• Dark Radiation constraints on minicharged particles in models with a hidden photon
• Current Direct Neutrino Mass Experiments
• Gravitational Rainbows: LIGO and Dark Energy at its Cutoff
• A time - luminosity correlation for Gamma Ray Bursts in the X - rays
• Formation and structure of ultralight bosonic dark matter halos
• The Visible and Infrared Survey Telescope for Astronomy (VISTA): Design, Technical Overview and Performance
• Phase-Space analysis of Teleparallel Dark Energy
• Dark energy as the weight of violating energy conservation
• The brightest galaxies at Cosmic Dawn
• Running Non-Gaussianities in DBI Inflation
• Metric-affine approach to teleparallel gravity
• Cosmic Microwave Weak lensing data as a test for the dark universe
• Sterile neutrinos in cosmology
• Entropy of Static Spacetimes and Microscopic Density of States
• Effects of cooling and star formation on the baryon fractions in clusters
• Astrophysical Probes of the Constancy of the Velocity of Light
• Planck Early Results XI: Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations
• The Effect of Metallicity on Cepheid-Based Distances
• Shadow and Deflection Angle of Rotating Black Holes in Perfect Fluid Dark Matter with a Cosmological Constant
• The non-Gaussian Cold Spot in the 3-year WMAP data
• CMB power spectra and cosmological parameters from Planck PR4 with CamSpec
• New Early Dark Energy
• Lorentz-violation-induced arrival delays of cosmological particles
• Beyond linear galaxy alignments
• Dark energy in Horndeski theories after GW170817: A review
• First evidence of running cosmic vacuum: challenging the concordance model
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: RSD measurement from the LOS-dependent power spectrum of DR12 BOSS galaxies
• Perturbations in generalized multi-field inflation
• Non-Abelian Gauge Field Inflation
• PRISM (Polarized Radiation Imaging and Spectroscopy Mission): An Extended White Paper
• JWST CEERS & JADES Active Galaxies at z = 4-7 Violate the Local $M_{\bullet }-M_{\star }$ Relation at $>3\sigma$: Implications for Low-Mass Black Holes and Seeding Models
• Relieving the Hubble tension with primordial magnetic fields
• Learning to Predict the Cosmological Structure Formation
• Eppur è piatto? The cosmic chronometer take on spatial curvature and cosmic concordance
• Astrophysics with the Spatially and Spectrally Resolved Sunyaev-Zeldovich Effects: A Millimetre/Submillimetre Probe of the Warm and Hot Universe
• The Effect of Physical Assumptions on the Calculation of Microwave Background Anisotropies
• Stellar Populations in the Large Magellanic Cloud from 2MASS
• The I-Band Tully-Fisher Relation for Cluster Galaxies: Data Presentation
• Interacting scenarios with dynamical dark energy: observational constraints and alleviation of the $H_0$ tension
• New Exclusion Limits for the Search of Scalar and Pseudoscalar Axion-Like Particles from "Light Shining Through a Wall"
• Quantifying discordance in the 2015 Planck CMB spectrum
• Hyper Suprime-Cam Year 3 Results: Cosmology from Cosmic Shear Power Spectra
• A distance determination to the Small Magellanic Cloud with an accuracy of better than 2 percent based on late-type eclipsing binary stars
• Reconciling CMB and structure growth measurements with dark energy interactions
• keV sterile neutrino dark matter in gauge extensions of the standard model
• Redefining the Axion Window
• Cosmological Limits on Slightly Skew Stresses
• The WiggleZ Dark Energy Survey: the transition to large-scale cosmic homogeneity
• Why reducing the cosmic sound horizon alone can not fully resolve the Hubble tension
• How well can we determine cluster mass profiles from weak lensing?
• Testing $F(Q)$ gravity with redshift space distortions
• Early Dark Energy Cosmologies
• On the Stellar Populations of Galaxies at z=9-11: The Growth of Metals and Stellar Mass at Early Times
• Dark Matter Axions Revisited
• Standard Big-Bang Nucleosynthesis up to CNO with an improved extended nuclear network
• The Aspen--Amsterdam Void Finder Comparison Project
• Evidence for anisotropy of cosmic acceleration
• A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension
• Microwave Background Signatures of a Primordial Stochastic Magnetic Field
• A new method to quantify the effects of baryons on the matter power spectrum
• The Origin of the Extragalactic Gamma-Ray Background and Implications for Dark-Matter Annihilation
• Calibration of the galaxy cluster M_500-Y_X relation with XMM-Newton
• Axion Dark Matter Detection using an LC Circuit
• On the use of the local prior on the absolute magnitude of Type Ia supernovae in cosmological inference
• Bias in the Effective Field Theory of Large Scale Structures
• The evidence for a spatially flat Universe
• Dark Quest. I. Fast and Accurate Emulation of Halo Clustering Statistics and Its Application to Galaxy Clustering
• Non-linear electrodynamics and the acceleration of the universe
• Constraining the Self-Interacting Neutrino Interpretation of the Hubble Tension
• Smoothing Supernova Data to Reconstruct the Expansion History of the Universe and its Age
• A Novel Test of the Modified Newtonian Dynamics with Gas Rich Galaxies
• Estimating the Redshift Distribution of Faint Galaxy Samples
• An infrared background--TeV gamma-ray crisis?
• The I-Band Tully-Fisher Relation for Cluster Galaxies: a Template Relation, its Scatter and Bias Corrections
• The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Quasar Target Selection
• The Three-Point Correlation Function in Cosmology
• The Tully-Fisher relations of early-type spiral and S0 galaxies
• Mapping the Galaxy Color-Redshift Relation: Optimal Photometric Redshift Calibration Strategies for Cosmology Surveys
• Living beyond the edge: Higgs inflation and vacuum metastability
• Millicharged Atomic Dark Matter
• Hubble Space Telescope Observations of Mira Variables in the Type Ia Supernova Host NGC 1559: An Alternative Candle to Measure the Hubble Constant
• A Test of the Collisional Dark Matter Hypothesis from Cluster Lensing
• Bouncing Cosmology in f(Q) Symmetric Teleparallel Gravity
• Origins of weak lensing systematics, and requirements on future instrumentation (or knowledge of instrumentation)
• Cosmological parameters derived from the final (PR4) Planck data release
• The implications of an extended dark energy cosmology with massive neutrinos for cosmological tensions
• Sterile Neutrinos
• Dark Energy Survey Year 1 Results: Redshift distributions of the weak lensing source galaxies
• Consistency tests of $\Lambda$CDM from the early integrated Sachs-Wolfe effect: Implications for early-time new physics and the Hubble tension
• Red Giant Branch stars: the theoretical framework
• Cosmological Inference using Gravitational Wave Standard Sirens: A Mock Data Challenge
• The BAO+BBN take on the Hubble tension
• Relating gravitational wave constraints from primordial nucleosynthesis, pulsar timing, laser interferometers, and the CMB: implications for the early universe
• Nonminimal torsion-matter coupling extension of f(T) gravity
• A Future Percent-Level Measurement of the Hubble Expansion at Redshift 0.8 With Advanced LIGO
• The Lagrangian-space Effective Field Theory of Large Scale Structures
• Cosmological Solutions of $f(T)$ Gravity
• Higgs inflation
• KiDS-450: Testing extensions to the standard cosmological model
• Observational Evidence for Primordial Black Holes: A Positivist Perspective
• Dynamical Dark Matter: I. Theoretical Overview
• Deviations from the Local Hubble Flow. I. The Tip of the Red Giant Branch as a Distance Indicator
• Can the Acceleration of Our Universe Be Explained by the Effects of Inhomogeneities?
• Can Late Dark Energy Transitions Raise the Hubble constant?
• Dark coupling
• A JWST/NIRCam Study of Key Contributors to Reionization: The Star-forming and Ionizing Properties of UV-faint $z\sim 7-8$ Galaxies
• Baryon Acoustic Oscillations and the Hubble Constant: Past, Present and Future
• A new measurement of the bulk flow of X-ray luminous clusters of galaxies
• Constraints on Dark Matter Annihilation in Clusters of Galaxies with the Fermi Large Area Telescope
• Goldstone Bosons as Fractional Cosmic Neutrinos
• Inflationary interpretation of the stochastic gravitational wave background signal detected by pulsar timing array experiments
• A fresh look at linear cosmological constraints on a decaying dark matter component
• Dark Matter from an ultra-light pseudo-Goldsone-boson
• Distance determinations using type II supernovae and the expanding photosphere method
• Inflation from Warped Space
• Interacting dark energy with time varying equation of state and the $H_0$ tension
• Cepheid Calibrations from the Hubble Space Telescope of the Luminosity of Two Recent Type Ia Supernovae and a Re-determination of the Hubble Constant
• Revisiting a negative cosmological constant from low-redshift data
• Inflation Physics from the Cosmic Microwave Background and Large Scale Structure
• The Carnegie Supernova Project: Absolute Calibration and the Hubble Constant
• Next Generation Cosmology: Constraints from the Euclid Galaxy Cluster Survey
• Lyman-alpha Forest Constraints on the Mass of Warm Dark Matter and the Shape of the Linear Power Spectrum
• Late universe decaying dark matter can relieve the H_0 tension
• CMU DeepLens: Deep Learning For Automatic Image-based Galaxy-Galaxy Strong Lens Finding
• Signature of Excess Radio Background in the 21-cm Global Signal and Power Spectrum
• Galactic Rotation Curves vs. Ultra-Light Dark Matter: Implications of the Soliton -- Host Halo Relation
• Microwave Background Signals from Tangled Magnetic Fields
• Extreme TeV blazars and the intergalactic magnetic field
• Spectroscopic Confirmation of CEERS NIRCam-selected Galaxies at $\mathbf{z}\simeq 8-10$
• Energy-Momentum Squared Gravity
• Dark Energy Survey Year 1 Results: Measurement of the Baryon Acoustic Oscillation scale in the distribution of galaxies to redshift 1
• Evidence for dark matter in the inner Milky Way
• Quantifying baryon effects on the matter power spectrum and the weak lensing shear correlation
• A Hemispherical Power Asymmetry from Inflation
• "Expansion" around the vacuum equation of state - sudden future singularities and asymptotic behavior
• Nonmetricity formulation of general relativity and its scalar-tensor extension
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the emission line galaxy sample from the anisotropic power spectrum between redshift 0.6 and 1.1
• Reducing the $H_0$ and ${\sigma }_8$ tensions with Dark Matter-neutrino interactions
• Evidence for a ~300 Mpc Scale Under-density in the Local Galaxy Distribution
• Weak Lensing Measurement of the Mass--Richness Relation of SDSS redMaPPer Clusters
• The impact of baryons on the matter power spectrum from the Horizon-AGN cosmological hydrodynamical simulation
• Non-Abelian dark matter and dark radiation
• Mass Function Predictions Beyond LCDM
• Higgs-Palatini Inflation and Unitarity
• Sharpening the Weak Gravity Conjecture with Dimensional Reduction
• Tip of the Red Giant Branch Distances. I. Optimization of a Maximum Likelihood Algorithm
• Constraints on Cosmology and Gravity from the Dynamics of Voids
• Probing cosmic isotropy with a new X-ray galaxy cluster sample through the $L_{\text{X}}-T$ scaling relation
• Cosmological expansion and local physics
• Testing the Hypothesis of Modified Dynamics with Low Surface Brightness Galaxies and Other Evidence
• Cosmic Flows on 100 Mpc/h Scales: Standardized Minimum Variance Bulk Flow, Shear and Octupole Moments
• Modified Gravity-GADGET: A new code for cosmological hydrodynamical simulations of modified gravity models
• A Limit on Primordial Small-Scale Magnetic Fields from CMB Distortions
• Planck 2015 results. XXI. The integrated Sachs-Wolfe effect
• Low reheating temperature and the visible sterile neutrino
• Dark Energy Survey Year 3 Results: Weak Lensing Shape Catalogue
• On the Effect of Rotation on Populations of Classical Cepheids II. Pulsation Analysis for Metallicities 0.014, 0.006, and 0.002
• The structure and evolution of weakly self-interacting cold dark matter halos
• Type Ia Supernova Light Curve Inference: Hierarchical Models in the Optical and Near Infrared
• A cluster finding algorithm based on the multiband identification of red sequence galaxies
• COSMOPOWER: emulating cosmological power spectra for accelerated Bayesian inference from next-generation surveys
• A Horizon Study for Cosmic Explorer: Science, Observatories, and Community
• A non-linear solution to the $S_8$ tension?
• CMB anisotropies from primordial inhomogeneous magnetic fields
• LOFAR Detection of 110-188 MHz Emission and Frequency-Dependent Activity from FRB 20180916B
• Resolving the Extragalactic $\gamma$-ray Background above 50 GeV with Fermi-LAT
• A Cosmology-Independent Calibration of Gamma-Ray Burst Luminosity Relations and the Hubble Diagram
• The internal structure of the lens PG1115+080: breaking degeneracies in the value of the Hubble Constant
• Constraints on neutrino masses from Lyman-alpha forest power spectrum with BOSS and XQ-100
• The Hubble series: Convergence properties and redshift variables
• Dynamics of $k$-essence
• $H_0$ Tension, Phantom Dark Energy and Cosmological Parameter Degeneracies
• A new analysis of galaxy 2-point functions in the BOSS survey, including full-shape information and post-reconstruction BAO
• On the theory and applications of modern cosmography
• Planck intermediate results. LI. Features in the cosmic microwave background temperature power spectrum and shifts in cosmological parameters
• $f(R,T_{\mu \nu }{T}^{\mu \nu })$ gravity and Cardassian-like expansion as one of its consequences
• Cosmological simulations of galaxy clusters
• Quasars as standard candles III. Validation of a new sample for cosmological studies
• Dark Energy Survey Year 3 Results: Redshift Calibration of the Weak Lensing Source Galaxies
• Quantum cosmological perfect fluid models
• The Hubble Constant from Infrared Surface Brightness Fluctuation Distances
• Early dark energy is not excluded by current large-scale structure data
• An optically-selected cluster catalog at redshift 0.1<z<1.1 from the Hyper Suprime-Cam Subaru Strategic Program S16A data
• A New Shear Estimator for Weak Lensing Observations
• The non-Gaussian Cold Spot in WMAP: significance, morphology and foreground contribution
• Quantum-Gravity Analysis of Gamma-Ray Bursts using Wavelets
• Hot Axions and the $H_0$ tension
• The BAHAMAS project: the CMB--large-scale structure tension and the roles of massive neutrinos and galaxy formation
• Extremely energetic Fermi Gamma-Ray Bursts obey spectral energy correlations
• A $\gamma$-ray determination of the Universe's star-formation history
• Modelling baryonic feedback for survey cosmology
• How Dark Matter Came to Matter
• New physics from the polarised light of the cosmic microwave background
• Graduated dark energy: Observational hints of a spontaneous sign switch in the cosmological constant
• Extragalactic Radio Sources and the WMAP Cold Spot
• The Supercluster-Void Network I. The Supercluster Catalogue and Large-Scale Distribution
• Gravitational induced particle production through a nonminimal curvature-matter coupling
• Cosmic radio dipole from NVSS and WENSS
• High-redshift cosmography: auxiliary variables versus Padé polynomials
• Interacting Dark Sector and Precision Cosmology
• Measuring the Hubble constant with Type Ia supernovae as near-infrared standard candles
• The $H_0$ tension in light of vacuum dynamics in the Universe
• Running Hubble Tension and a H0 Diagnostic
• McVittie's Legacy: Black Holes in an Expanding Universe
• Detection of the velocity dipole in the radio galaxies of the NRAO VLA Sky Survey
• Exploring the effects of galaxy formation on matter clustering through a library of simulation power spectra
• The Matter Bounce Scenario in Loop Quantum Cosmology
• Primordial Gravitational Waves from Axion-Gauge Fields Dynamics
• Universality of galactic surface densities within one dark halo scale-length
• Dark Matter from Early Decays
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: BAO measurement from the LOS-dependent power spectrum of DR12 BOSS galaxies
• Non-Gaussianities and chiral gravitational waves in natural steep inflation
• Can the $H_0$ tension be resolved in extensions to $\Lambda$CDM cosmology?
• A CMB Search for the Neutrino Mass Mechanism and its Relation to the $H_0$ Tension
• String or M theory axion as a quintessence
• Phases of New Physics in the CMB
• Update on Coupled Dark Energy and the $H_0$ tension
• Does the small CMB quadrupole moment suggest new physics?
• Finsler geometric extension of Einstein gravity
• Euclid preparation: IX. EuclidEmulator2 -- Power spectrum emulation with massive neutrinos and self-consistent dark energy perturbations
• Implications of High-Resolution Simulations on Indirect Dark Matter Searches
• KiDS-1000 catalogue: Redshift distributions and their calibration
• Using the Full Power of the Cosmic Microwave Background to Probe Axion Dark Matter
• Primordial gravitational waves from NANOGrav: a broken power-law approach
• CEERS Spectroscopic Confirmation of NIRCam-Selected z > 8 Galaxy Candidates with JWST/NIRSpec: Initial Characterization of their Properties
• A First Detection of the Acoustic Oscillation Phase Shift Expected from the Cosmic Neutrino Background
• Fast radio bursts as a cosmic probe?
• Dark energy: a quantum fossil from the inflationary Universe?
• Derivation of a Vacuum Refractive Index in a Stringy Space-Time Foam Model
• Accelerated Universe from Modified Chaplygin Gas and Tachyonic Fluid
• A 120-Mpc Periodicity in the Three-Dimensional Distribution of Galaxy Superclusters
• Is there an early Universe solution to Hubble tension?
• Structure formation in $f(T)$ gravity and a solution for $H_0$ tension
• Mass Calibration and Cosmological Analysis of the SPT-SZ Galaxy Cluster Sample Using Velocity Dispersion ${\sigma }_v$ and X-ray $Y_{\text{X}}$ Measurements
• Cosmology Constraints from the Weak Lensing Peak Counts and the Power Spectrum in CFHTLenS
• A Vacuum Phase Transition Solves $H_0$ Tension
• Local Voids as the Origin of Large-angle Cosmic Microwave Background Anomalies I
• Cosmology with massive neutrinos I: towards a realistic modeling of the relation between matter, haloes and galaxies
• Model independent constraints on dark energy evolution from low-redshift observations
• The POLARBEAR-2 and the Simons Array Experiment
• Limits on Neutrino-Neutrino Scattering in the Early Universe
• The Pantheon+ Analysis: SuperCal-Fragilistic Cross Calibration, Retrained SALT2 Light Curve Model, and Calibration Systematic Uncertainty
• Dark sector interaction: a remedy of the tensions between CMB and LSS data
• The one-dimensional power spectrum from the SDSS DR14 Ly$\alpha$ forests
• Evolution of the UV LF from z~15 to z~8 Using New JWST NIRCam Medium-Band Observations over the HUDF/XDF
• Wormhole geometries in $f(Q)$ gravity and the energy conditions
• The radio emission from the Galaxy at 22 MHz
• Dark Energy with Phantom Crossing and the $H_0$ tension
• Relic Density of Neutralino Dark Matter in Supergravity Models
• Quantum-Gravitational Diffusion and Stochastic Fluctuations in the Velocity of Light
• First star-forming structures in fuzzy cosmic filaments
• How to optimally parametrize deviations from General Relativity in the evolution of cosmological perturbations
• DES Y3 + KiDS-1000: Consistent cosmology combining cosmic shear surveys
• Towards a Cosmological Hubble Diagram for Type II-P Supernovae
• Searching for a Cosmological Preferred Axis: Union2 Data Analysis and Comparison with Other Probes
• A New Target for Cosmic Axion Searches
• Quantitative Spectroscopy of Photospheric-Phase Type II Supernovae
• Large peculiar motion of the solar system from the dipole anisotropy in sky brightness due to distant radio sources
• Observational constraints on one-parameter dynamical dark-energy parametrizations and the $H_0$ tension
• The Bianchi IX attractor
• Nonlocal gravity. Conceptual aspects and cosmological predictions
• DESI 2024: Reconstructing Dark Energy using Crossing Statistics with DESI DR1 BAO data
• Constraints from Ly-$\alpha$ forests on non-thermal dark matter including resonantly-produced sterile neutrinos
• Observational Constraints on Teleparallel Dark Energy
• A Challenge to the Standard Cosmological Model
• Models of coupled dark matter to dark energy
• Accelerating Cosmologies with an Anisotropic Equation of State
• Stability analysis of chromo-natural inflation and possible evasion of Lyth's bound
• The Third Gravitational Lensing Accuracy Testing (GREAT3) Challenge Handbook
• Constraints on scattering of keV--TeV dark matter with protons in the early Universe
• Robust Preference for Dynamical Dark Energy in DESI BAO and SN Measurements
• Results of the GREAT08 Challenge: An image analysis competition for cosmological lensing
• Dipoles in the Sky
• GeV Gamma-Ray Attenuation and the High-Redshift UV Background
• SuperWIMP Solutions to Small Scale Structure Problems
• Tension with the flat ΛCDM model from a high redshift Hubble Diagram of supernovae, quasars and gamma-ray bursts
• Kaniadakis holographic dark energy and cosmology
• The Local Perspective on the Hubble Tension: Local Structure Does Not Impact Measurement of the Hubble Constant
• Comparing Equivalent Gravities: common features and differences
• Searching for galactic axions through magnetized media: the QUAX proposal
• Sneutrino cold dark matter, a new analysis: relic abundance and detection rates
• Fermi/LAT observations of 1ES 0229+200: implications for extragalactic magnetic fields and background light
• Strong constraints on self-interacting dark matter with light mediators
• Observational constraints on cosmological solutions of $f(Q)$ theories
• Strong Lens Time Delay Challenge: II. Results of TDC1
• Interpreting Cosmological Vacuum Decay
• Unifying Holographic Inflation with Holographic Dark Energy: a Covariant Approach
• Expansion History with Decaying Vacuum: A Complete Cosmological Scenario
• On the Mechanism of Gamma-Ray Burst Afterglows
• Updated constraints on non-standard neutrino interactions from Planck
• Physical Bayesian modelling of the non-linear matter distribution: new insights into the Nearby Universe
• Using Quantitative Spectroscopic Analysis to Determine the Properties and Distances of Type II-Plateau Supernovae: SNe 2005cs and 2006bp
• Tensor Microwave Anisotropies from a Stochastic Magnetic Field
• Bounds on the possible evolution of the Gravitational Constant from Cosmological Type-Ia Supernovae
• Dark energy and curvature from a future baryonic acoustic oscillation survey using the Lyman-alpha forest
• From Spitzer Galaxy Photometry to Tully-Fisher Distances
• Hints of dynamical vacuum energy in the expanding Universe
• Faraday Rotation of the Cosmic Microwave Background Polarization by a Stochastic Magnetic Field
• A Critical Assessment of CMB Limits on Dark Matter-Baryon Scattering: New Treatment of the Relative Bulk Velocity
• Constraining Dark Matter-Neutrino Interactions using the CMB and Large-Scale Structure
• A new cosmological distance measure using AGN
• Extreme Value Statistics of the Halo and Stellar Mass Distributions at High Redshift: are JWST Results in Tension with ΛCDM?
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Growth rate of structure measurement from anisotropic clustering analysis in configuration space between redshift 0.6 and 1.1 for the Emission Line Galaxy sample
• A Low CMB Quadrupole from Dark Energy Isocurvature Perturbations
• Varying-$\alpha$ Theories and Solutions to the Cosmological Problems
• Calibration of weak-lensing shear in the Kilo-Degree Survey
• SALT3: An Improved Type Ia Supernova Model for Measuring Cosmic Distances
• Rock 'n' Roll Solutions to the Hubble Tension
• New Physics in the Rayleigh-Jeans Tail of the CMB
• Prime Focus Spectrograph (PFS) for the Subaru Telescope: Overview, recent progress, and future perspectives
• Search for invisible axion dark matter of mass m${}_a=43\mu$eV with the QUAX--$a\gamma$ experiment
• CMB anisotropies seen by an off-center observer in a spherically symmetric inhomogeneous universe
• Dark Matter and Fundamental Physics with the Cherenkov Telescope Array
• Semi-Analytical Models for the Formation of Disk Galaxies: I. Constraints from the Tully-Fisher Relation
• Cosmicflows-4
• Possible signals of vacuum dynamics in the Universe
• Dynamical vacuum energy in the expanding Universe confronted with observations: a dedicated study
• Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
• Discovery of a tight correlation for gamma ray burst afterglows with `canonical' light curves
• An Analytical Model for the Triaxial Collapse of Cosmological Perturbations
• Evidence for dark matter interactions in cosmological precision data?
• Precision cosmology with Padé rational approximations: theoretical predictions versus observational limits
• Dark Energy Survey Year 1 Results: Methods for Cluster Cosmology and Application to the SDSS
• Asymptotically Safe Inflation
• Non-parametric spatial curvature inference using late-universe cosmological probes
• The abundance of voids and the excursion set formalism
• From galactic bars to the Hubble tension: weighing up the astrophysical evidence for Milgromian gravity
• SDSS DR7 superclusters. The catalogues
• The Carnegie Hubble Program: The Distance and Structure of the SMC as Revealed by Mid-infrared Observations of Cepheids
• Black Hole Space-time In Dark Matter Halo
• Constraining properties of GRB magnetar central engines using the observed plateau luminosity and duration correlation
• Entropic cosmology for a generalized black-hole entropy
• The lithium isotopic ratio in very metal-poor stars
• Fast-Roll Inflation
• Revealing reionization with the thermal history of the intergalactic medium: new constraints from the Lyman-$\alpha$ flux power spectrum
• Cosmological Models in Energy-Momentum-Squared Gravity
• The Hubble Tension in Light of the Full-Shape Analysis of Large-Scale Structure Data
• Searching for Primordial Black Holes in the radio and X-ray sky
• Alternative quantization of the Hamiltonian in loop quantum cosmology II: Including the Lorentz term
• OGLE-ing the Magellanic System: Optical Reddening Maps of the Large and Small Magellanic Cloud from Red Clump Stars
• The First DIRECT Distance Determination to a Detached Eclipsing Binary in M33
• Cosmic shear results from the deep lens survey - I: Joint constraints on omega_m and sigma_8 with a two-dimensional analysis
• Dark Matter from Split Seesaw
• Early modified gravity in light of the $H_0$ tension and LSS data
• Constraints on a New Post-General Relativity Cosmological Parameter
• Relic Dark energy from Trans-Planckian Regime
• Complete Cosmic History with a dynamical Lambda(H) term
• Black Hole Shadow of Sgr A${}^{\ast }$ in Dark Matter Halo
• Cosmographic analysis with Chebyshev polynomials
• No large-angle correlations on the non-Galactic microwave sky
• N-Body Simulations for Coupled Scalar Field Cosmology
• The Dark Dimension and the Swampland
• Cluster Cepheids with High Precision Gaia Parallaxes, Low Zeropoint Uncertainties, and Hubble Space Telescope Photometry
• Redshift-Space Distortions in Lagrangian Perturbation Theory
• Cluster-galaxy weak lensing
• UV Luminosity Density Results at z>8 from the First JWST/NIRCam Fields: Limitations of Early Data Sets and the Need for Spectroscopy
• The COpernicus COmplexio: Statistical Properties of Warm Dark Matter Haloes
• The Hubble flow around the Local Group
• Dusty Starbursts Masquerading as Ultra-high Redshift Galaxies in JWST CEERS Observations
• Robust Neutrino Constraints by Combining Low Redshift Observations with the CMB
• Model independent tests of the standard cosmological model
• The impact of intrinsic alignment on current and future cosmic shear surveys
• Determining neutrino oscillation parameters from atmospheric muon neutrino disappearance with three years of IceCube DeepCore data
• The zoo plot meets the swampland: mutual (in)consistency of single-field inflation, string conjectures, and cosmological data
• Generalized entropies and corresponding holographic dark energy models
• Early dark energy resolution to the Hubble tension in light of weak lensing surveys and lensing anomalies
• A measurement of the Hubble constant from Type II supernovae
• Relaxing cosmological tensions with a sign switching cosmological constant
• Updated fundamental constant constraints from Planck 2018 data and possible relations to the Hubble tension
• Modeling Quintessential Inflation
• Effect of baryonic feedback on two- and three-point shear statistics: prospects for detection and improved modelling
• Dark energy from the string axiverse
• A rapid transition of $G_{\mathrm{eff}}$ at $z_t\simeq 0.01$ as a solution of the Hubble and growth tensions
• Cosmological bounds on dark matter-neutrino interactions
• A First Attempt to Calibrate the Baryonic Tully-Fisher Relation with Gas Dominated Galaxies
• Quintessential Inflation with $\alpha$-attractors
• KiDS+VIKING-450 and DES-Y1 combined: Mitigating baryon feedback uncertainty with COSEBIs
• Tensions in the dark: shedding light on Dark Matter-Dark Energy interactions
• Determination of the intrinsic Luminosity Time Correlation in the X-ray Afterglows of GRBs
• An improved model-independent assessment of the late-time cosmic expansion
• Early-universe constraints on a time-varying fine structure constant
• New Light Species and the CMB
• The Atacama Cosmology Telescope: Constraints on Pre-Recombination Early Dark Energy
• The Megamaser Cosmology Project: IV. A Direct Measurement of the Hubble Constant from UGC 3789
• Scaling relations for galaxy clusters: properties and evolution
• CEERS Key Paper V: A triality on the nature of HST-dark galaxies
• Unified framework for Early Dark Energy from $\alpha$-attractors
• A local resolution of the Hubble tension: The impact of screened fifth forces on the cosmic distance ladder
• The ROSAT All-Sky Survey Bright Source Catalogue
• The Complete Calibration of the Color-Redshift Relation (C3R2) Survey: Survey Overview and Data Release 1
• A Quantitative Study of Interacting Dark Matter in Halos
• New constraint on Early Dark Energy from Planck and BOSS data using the profile likelihood
• Rotating Black Hole Shadow in Perfect Fluid Dark Matter
• Planck 2013 results. XXVI. Background geometry and topology of the Universe
• Fast Radio Burst/Gamma-Ray Burst Cosmography
• Solutions of the Einstein equations for a black hole surrounded by a galactic halo
• The Atacama Cosmology Telescope: Modeling the Gas Thermodynamics in BOSS CMASS galaxies from Kinematic and Thermal Sunyaev-Zel'dovich Measurements
• A tale of two modes: Neutrino free-streaming in the early universe
• The "Tip" of the Red Giant Branch as a distance indicator: results from evolutionary models
• The galaxy power spectrum take on spatial curvature and cosmic concordance
• A Detailed Description of the CamSpec Likelihood Pipeline and a Reanalysis of the Planck High Frequency Maps
• The Megamaser Cosmology Project: I. VLBI observations of UGC 3789
• Cosmological constraints in extended parameter space from the Planck 2018 Legacy release
• Constraints on the Hubble constant from Supernova Refsdal's reappearance
• Stringent Limit on Primordial Magnetic Fields from the Cosmic Microwave Background Radiation
• Progress on Cosmological Magnetic Fields
• Axion cold dark matter in non-standard cosmologies
• The VMC Survey. XXV. The 3D structure of the Small Magellanic Cloud from Classical Cepheids
• A new measurement of the Hubble constant using Type Ia supernovae calibrated with surface brightness fluctuations
• Examining the evidence for dynamical dark energy
• Average observational quantities in the timescape cosmology
• Constraining Variations in the Fine-Structure Constant with the Cosmic Microwave Background
• ArborZ: Photometric Redshifts Using Boosted Decision Trees
• On the most constraining cosmological neutrino mass bounds
• Model-independent reconstruction of $f(T)$ gravity from Gaussian Processes
• PArthENoPE reloaded
• Probing the thermal state of the intergalactic medium at $z>5$ with the transmission spikes in high-resolution Ly$\alpha$ forest spectra
• Bouncing Loop Quantum Cosmology from $F(T)$ gravity
• Dark matter halos of massive elliptical galaxies at $z\sim 0.2$ are well described by the Navarro-Frenk-White profile
• Nonparametric late-time expansion history reconstruction and implications for the Hubble tension in light of recent DESI and type Ia supernovae data
• Collisional versus Collisionless Dark Matter
• Quintessence and the Separation of CMB Peaks
• New classes of modified teleparallel gravity models
• CFHTLenS tomographic weak lensing: Quantifying accurate redshift distributions
• Small Magellanic Cloud Cepheids Observed with the Hubble Space Telescope Provide a New Anchor for the SH0ES Distance Ladder
• MassiveNuS: Cosmological Massive Neutrino Simulations
• Finding the chiral gravitational wave background of an axion-SU(2) inflationary model using CMB observations and laser interferometers
• LXCDM: a cosmon model solution to the cosmological coincidence problem?
• High redshift radio galaxies and divergence from the CMB dipole
• Addressing the circularity problem in the $E_{\text{p}}-E_{\text{iso}}$ correlation of Gamma-Ray Bursts
• New models and Big Bang Nucleosynthesis constraints in $f(Q)$ gravity
• Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data
• On the consistency of universally non-minimally coupled $f(R,T,R_{\mu \nu }{T}^{\mu \nu })$ theories
• Beyond $\Lambda$CDM with Low and High Redshift Data: Implications for Dark Energy
• Structure formation in large-volume cosmological simulations of fuzzy dark matter: Impact of the non-linear dynamics
• Converting non-relativistic dark matter to radiation
• New Observational $H(z)$ Data from Full-Spectrum Fitting of Cosmic Chronometers in the LEGA-C Survey
• Probing the Cosmological Principle in the counts of radio galaxies at different frequencies
• Evolution of dark energy reconstructed from the latest observations
• Should Type Ia Supernova Distances be Corrected for their Local Environments?
• The Radio Background Below 100 MHz
• Interacting neutrinos in cosmology: exact description and constraints
• Thermal Friction as a Solution to the Hubble Tension
• Type IIP Supernovae as Cosmological Probes: A SEAM Distance to SN 1999em
• Probing Primordial Gravitational Waves: Ali CMB Polarization Telescope
• The Complete Calibration of the Color-Redshift Relation (C3R2) Survey: Analysis and Data Release 2
• Cosmological Simulations of Normal-Branch Braneworld Gravity
• A model-independent determination of the Hubble constant from lensed quasars and supernovae using Gaussian process regression
• Cosmological constraints on Brans-Dicke theory
• A measurement of Hubble's Constant using Fast Radio Bursts
• Cosmological window onto the string axiverse and the supersymmetry breaking scale
• A statistical standard siren measurement of the Hubble constant from the LIGO/Virgo gravitational wave compact object merger GW190814 and Dark Energy Survey galaxies
• Brans-Dicke gravity with a cosmological constant smoothes out $\Lambda$CDM tensions
• DES Y3 results: Blending shear and redshift biases in image simulations
• Probing the cosmological viability of non-gaussian statistics
• Induced two-photon decay of the 2s level and the rate of cosmological hydrogen recombination
• Metacalibration: Direct Self-Calibration of Biases in Shear Measurement
• Polarization of gravitational waves in symmetric teleparallel theories of gravity and their modifications
• Cosmicflows 4: The Calibration of Optical and Infrared Tully-Fisher Relations
• Constraints on a Bianchi type I spacetime extension of the standard $\Lambda$CDM model
• Density split statistics: Cosmological constraints from counts and lensing in cells in DES Y1 and SDSS data
• Photometric Redshift Calibration with Self Organising Maps
• Revealing Intrinsic Flat $\Lambda$CDM Biases with Standardizable Candles
• Dynamical Dark Matter: II. An Explicit Model
• Information content of weak lensing power spectrum and bispectrum: including the non-Gaussian error covariance matrix
• Revisiting the NVSS number count dipole
• A Quintessential Axion
• CMB multipole measurements in the presence of foregrounds
• Constraints on dark matter scenarios from measurements of the galaxy luminosity function at high redshifts
• Spectral sirens: cosmology from the full mass distribution of compact binaries
• Using The Baryonic Tully-Fisher Relation to Measure $H_o$
• Shadows of Sgr A${}^{\ast }$ Black Hole Surrounded by Superfluid Dark Matter Halo
• Covariant Effective Action for Loop Quantum Cosmology a la Palatini
• Observational constraints on sign-changeable interaction models and alleviation of the $H_0$ tension
• Cosmological Effective Hamiltonian from full Loop Quantum Gravity Dynamics
• A new life for sterile neutrinos: resolving inconsistencies using hot dark matter
• Probing the isotropy of cosmic acceleration traced by Type Ia supernovae
• Cosmic Voids: structure, dynamics and galaxies
• From Big Bang to Asymptotic de Sitter: Complete Cosmologies in a Quantum Gravity Framework
• Are the ultra-high-redshift galaxies at z > 10 surprising in the context of standard galaxy formation models?
• Constraining Primordial Magnetism
• Cosmological implications of the anisotropy of ten galaxy cluster scaling relations
• Heavy spin-2 Dark Matter
• A dynamical model of the local cosmic expansion
• The Halo Mass Function from Excursion Set Theory. II. The Diffusing Barrier
• Strongly lensed repeating Fast Radio Bursts as precision probes of the universe
• CMB lensing tomography with the DES Science Verification galaxies
• First Batch of Candidate Galaxies at Redshifts 11 to 20 Revealed by the James Webb Space Telescope Early Release Observations
• Lorentz-covariant deformed algebra with minimal length and application to the 1+1-dimensional Dirac oscillator
• Blue-tilted Tensor Spectrum and Thermal History of the Universe
• Cosmological constraints from unWISE and Planck CMB lensing tomography
• Axion-Dilaton Destabilization and the Hubble Tension
• LoCuSS: Calibrating Mass-Observable Scaling Relations for Cluster Cosmology with Subaru Weak Lensing Observations
• The Parallax of Omega Centauri Measured from Gaia EDR3 and a Direct, Geometric Calibration of the Tip of the Red Giant Branch and the Hubble Constant
• Solving the small-scale structure puzzles with dissipative dark matter
• The Assembly History of Disk Galaxies: I - The Tully-Fisher Relation to z~1.3 from Deep Exposures with DEIMOS
• A fundamental plane for long gamma-ray bursts with X-ray plateaus
• Scalar-tensor theories of gravity, neutrino physics, and the $H_0$ tension
• Dark Energy at early times and ACT: a larger Hubble constant without late-time priors
• Three-Higgs-doublet models: symmetries, potentials and Higgs boson masses
• Collisional dark matter and the structure of dark halos
• Universe acceleration and nonlinear electrodynamics
• Preheating in Palatini Higgs inflation
• A More General Model for the Intrinsic Scatter in Type Ia Supernova Distance Moduli
• Cosmology with Void-Galaxy Correlations
• Variable gravity: A suitable framework for quintessential inflation
• The Hawaii K-Band Galaxy Survey. II. Bright K-band Imaging
• Modeling baryonic physics in future weak lensing surveys
• Effective Theory of Interacting Dark Energy
• The SRG/eROSITA all-sky survey: Cosmology constraints from cluster abundances in the western Galactic hemisphere
• First results from the OSQAR photon regeneration experiment: No light shining through a wall
• The Red Giant Branch in the Near-Infrared Colour-Magnitude Diagrams. I: The calibration of photometric indices
• Comparing Tip of the Red Giant Branch Distance Scales: An Independent Reduction of the Carnegie-Chicago Hubble Program and the Value of the Hubble Constant
• Direct neutrino-mass measurement based on 259 days of KATRIN data
• A Compendium of Chameleon Constraints
• The Relation between Stellar and Dynamical Surface Densities in the Central Regions of Disk Galaxies
• A Sudden Gravitational Transition
• Ultra-compact structure in intermediate-luminosity radio quasars: building a sample of standard cosmological rulers and improving the dark energy constraints up to $z\sim 3$
• An updated Gamma Ray Bursts Hubble diagram
• Effects of Cosmological Magnetic Helicity on the Cosmic Microwave Background
• The KBC void and Hubble tension contradict $\Lambda$CDM on a Gpc scale $-$ Milgromian dynamics as a possible solution
• The effects of baryons on the halo mass function
• Diurnal modulation signal from dissipative hidden sector dark matter
• On the cosmological constant problem
• The Pantheon+ Analysis: Improving the Redshifts and Peculiar Velocities of Type Ia Supernovae Used in Cosmological Analyses
• Improved constraints on H0 from a combined analysis of gravitational-wave and electromagnetic emission from GW170817
• Gravitational Waves in Modified Teleparallel Theories
• Quantifying tensions in cosmological parameters: Interpreting the DES evidence ratio
• Model Independent Reconstruction of the Expansion History of the Universe and the Properties of Dark Energy
• Reconciling Planck results with low redshift astronomical measurements
• Clues on void evolution II: Measuring density and velocity profiles on SDSS galaxy redshift space distortions
• Is there Correlation between Fine Structure and Dark Energy Cosmic Dipoles?
• Cepheid Calibrations of Modern Type Ia Supernovae:Implications for the Hubble Constant
• Imprints of Dark Matter on Black Hole Shadows using Spherical Accretions
• Measuring the Hubble constant with neutron star black hole mergers
• Cosmological Constraints from DES Y1 Cluster Abundances and SPT Multi-wavelength data
• Entropy signature of the running cosmological constant
• Resonant laser power build-up in ALPS -- a "light-shining-through-walls" experiment
• Cosmographic Hubble fits to the supernova data
• The halo model as a versatile tool to predict intrinsic alignments
• The baryonic Tully-Fisher relation and its implication for dark matter halos
• Restoring cosmological concordance with early dark energy and massive neutrinos?
• Cosmological Effects of Nonlinear Electrodynamics
• Neutralinos, Big Bang Nucleosynthesis and 6Li in Low-Metallicity Stars
• Towards Cosmological Dynamics from Loop Quantum Gravity
• Cosmology with self-interacting sterile neutrinos and dark matter - A pseudoscalar model
• Cosmological hydrodynamical simulations of galaxy clusters: X-ray scaling relations and their evolution
• Modelling the Sgr A* Black Hole Immersed in a Dark Matter Spike
• Evidence for a Lower Value for $H_0$ from Cosmic Chronometers Data?
• Running vacuum against the $H_0$ and ${\sigma }_8$ tensions
• Early recombination as a solution to the $H_0$ tension
• An 8\% Determination of the Hubble Constant from localized Fast Radio Bursts
• Analyzing the Large-Scale Bulk Flow using CosmicFlows4: Increasing Tension with the Standard Cosmological Model
• Small neutrino masses from gravitational $\theta$-term
• Stochastic star formation in early galaxies: JWST implications
• Hints of FLRW Breakdown from Supernovae
• Curvature vs Distances: testing the FLRW cosmology
• Photometric Redshifts for Next-Generation Surveys
• Nucleosynthesis Constraints on a Massive Gravitino in Neutralino Dark Matter Scenarios
• Phenomenology of D-Brane Inflation with General Speed of Sound
• The Pantheon+ Analysis: Evaluating Peculiar Velocity Corrections in Cosmological Analyses with Nearby Type Ia Supernovae
• Photon Mass Limits from Fast Radio Bursts
• Testing modified gravity with Planck: the case of coupled dark energy
• Cosmic microwave background and large scale structure limits on the interaction between dark matter and baryons
• Future Cosmological Constraints from Fast Radio Bursts
• Sample variance in the local measurements of the Hubble constant
• Emergent scale symmetry: Connecting inflation and dark energy
• Redshift-space distortions around voids
• Updated constraints on massive neutrino self-interactions from cosmology in light of the $H_0$ tension
• Gas dynamics in tidal dwarf galaxies: disc formation at z=0
• On the Dark Sector Interactions
• How early is early dark energy?
• Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances, Weak Lensing, and Galaxy Correlations
• Constraining Non-Cold Dark Matter Models with the Global 21-cm Signal
• The $\bar{\Lambda }CDM$ cosmology: from inflation to dark energy through running $\Lambda$
• The Young Supernova Experiment: Survey Goals, Overview, and Operations
• The Cosmic Radio Dipole: Estimators and Frequency Dependence
• Lensing Time Delays and Cosmological Complementarity
• The Cosmological Constant Problem and Running Vacuum in the Expanding Universe
• Star formation histories of UV-luminous galaxies at $z\simeq 6.8$: implications for stellar mass assembly at early cosmic times
• 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
• The Tully-Fisher relation for S0 galaxies
• Cosmological constraints from the tomographic cross-correlation of DESI Luminous Red Galaxies and Planck CMB lensing
• SWIFT: A modern highly-parallel gravity and smoothed particle hydrodynamics solver for astrophysical and cosmological applications
• Large Tensor Non-Gaussianity from Axion-Gauge Fields Dynamics
• A new method to build the (inverse) distance ladder
• Velocity correction for Hubble constant measurements from standard sirens
• Axion Gauge Field Inflation and Gravitational Leptogenesis: A Lower Bound on B Modes from the Matter-Antimatter Asymmetry of the Universe
• Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?
• Leptogenesis and tensor polarisation from a gravitational Chern-Simons term
• Decaying dark matter and the tension in ${\sigma }_8$
• A new tension in the cosmological model from primordial deuterium?
• Looking for a varying $\alpha$ in the Cosmic Microwave Background
• Full-shape cosmology analysis of SDSS-III BOSS galaxy power spectrum using emulator-based halo model: a $5\%$ determination of ${\sigma }_8$
• Dodelson-Widrow Mechanism In the Presence of Self-Interacting Neutrinos
• Resembling dark energy and modified gravity with Finsler-Randers cosmology
• The $L-\sigma$ relation for massive bursts of star formation
• Bayesian evidence as a tool for comparing datasets
• Fractal Dimension as a measure of the scale of Homogeneity
• The Chandra COSMOS legacy survey: Energy Spectrum of the Cosmic X-ray Background and constraints on undetected populations
• EMPRESS. VIII. A New Determination of Primordial He Abundance with Extremely Metal-Poor Galaxies: A Suggestion of the Lepton Asymmetry and Implications for the Hubble Tension
• Quintessential inflation with canonical and noncanonical scalar fields and Planck 2015 results
• Detection of the Gravitational Lens Magnifying a Type Ia Supernova
• A $w-M$ phantom transition at $z_t<0.1$ as a resolution of the Hubble tension
• GAIA Cepheid parallaxes and 'Local Hole' relieve $H_0$ tension
• Nonlinear interacting cosmological models after Planck 2018 legacy release and the $H_0$ tension
• Dehnen halo effect on a black hole in an ultra-faint dwarf galaxy
• Cosmography and flat $\Lambda$CDM tensions at high redshift
• Small-scale CMB polarization anisotropies due to tangled primordial magnetic fields
• Dynamical dark energy versus $\Lambda =$const. in light of observations
• TDCOSMO. XII. Improved Hubble constant measurement from lensing time delays using spatially resolved stellar kinematics of the lens galaxy
• Massive gravitons as dark matter and gravitational waves
• Interpreting cosmological tensions from the effective field theory of torsional gravity
• A deep learning approach to cosmological dark energy models
• The PHLEK Survey: A New Determination of the Primordial Helium Abundance
• Cosmological Constraints on Dark Matter Interactions with Ordinary Matter
• Density perturbations for running vacuum: a successful approach to structure formation and to the ${\sigma }_8$-tension
• On the robustness of the primordial power spectrum in renormalized Higgs inflation
• Cosmic concordance and the fine structure constant
• LoCuSS: The Sunyaev-Zel'dovich Effect and Weak Lensing Mass Scaling Relation
• Partially Acoustic Dark Matter, Interacting Dark Radiation, and Large Scale Structure
• Interacting radiation after Planck and its implications for the Hubble Tension
• Large Magellanic Cloud Near-Infrared Synoptic Survey. I. Cepheid variables and the calibration of the Leavitt Law
• Flat rotation curves and low velocity dispersions in KMOS star-forming galaxies at z~1
• Gravitational Origin of Dark Matter
• Cosmic Microwave Background Polarization Signals from Tangled Magnetic Fields
• Photometric AGN reverberation mapping - an efficient tool for BLR sizes, black hole masses and host-subtracted AGN luminosities
• DESI DR2 Results I: Baryon Acoustic Oscillations from the Lyman Alpha Forest
• Measurement of the Extragalactic Background Light using MAGIC and Fermi-LAT gamma-ray observations of blazars up to z = 1
• The Hobby-Eberly Telescope Dark Energy Experiment (HETDEX): Description and Early Pilot Survey Results
• Probing the Small-Scale Matter Power Spectrum with Large-Scale 21-cm Data
• Neutralino relic density in a Universe with a non-vanishing cosmological constant
• The Quasar Main Sequence explained by the combination of Eddington ratio, metallicity and orientation
• Dynamical dark energy after Planck CMB final release and $H_0$ tension
• Negative cosmological constant in the dark sector?
• Cores of Dark Matter Halos Correlate with Disk Scale Lengths
• Dirac Neutrinos and Dark Matter Stability from Lepton Quarticity
• The brightness of the Red Giant Branch tip: Theoretical framework, a set of reference models, and predicted observables
• Measuring Time-Dependence of Dark Energy Density from Type Ia Supernova Data
• 2021-$H_0$ Odyssey: Closed, Phantom and Interacting Dark Energy Cosmologies
• Planck 2018 results. II. Low Frequency Instrument data processing
• On the magnetar origin of the GRBs presenting X-ray afterglow plateaus
• Do we have any hope of detecting scattering between dark energy and baryons through cosmology?
• Dark matter effect on the weak deflection angle by black holes at the center of Milky Way and M87 galaxies
• Higgsed Chromo-Natural Inflation
• The Tip of the Red Giant Branch Distances to Type Ia Supernova Host Galaxies. IV. Color Dependence and Zero-Point Calibration
• Relaxing cosmological tensions with a sign switching cosmological constant: Improved results with Planck, BAO, and Pantheon data
• Cosmological parameter analyses using transversal BAO data
• Non-Thermal Dark Matter Mimicking An Additional Neutrino Species In The Early Universe
• Galaxy Build-up in the first 1.5 Gyr of Cosmic History: Insights from the Stellar Mass Function at $z\sim 4-9$ from JWST NIRCam Observations
• CMB bispectrum from primordial magnetic fields on large angular scales
• Improving Helium Abundance Determinations with Leo P as a Case Study
• Modelling the large scale structure of the Universe as a function of cosmology and baryonic physics
• Constraints on anisotropic cosmic expansion from supernovae
• Vector Curvaton with varying Kinetic Function
• Hints of Early Dark Energy in Planck, SPT, and ACT data: new physics or systematics?
• Cosmic dissonance: new physics or systematics behind a short sound horizon?
• Lorentz violation and generalized uncertainty principle
• Sunyaev-Zel'dovich Effect and X-ray Scaling Relations from Weak-Lensing Mass Calibration of 32 SPT Selected Galaxy Clusters
• Machine Learning-based Brokers for Real-time Classification of the LSST Alert Stream
• Spectroscopic Needs for Imaging Dark Energy Experiments: Photometric Redshift Training and Calibration
• Large-scale stable interacting dark energy model: Cosmological perturbations and observational constraints
• Insensitivity of The Distance Ladder Hubble Constant Determination to Cepheid Calibration Modeling Choices
• Parametrized Post-Friedmann Framework for Interacting Dark Energy
• Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements
• The MOSDEF Survey: Dynamical and Baryonic Masses and Kinematic Structures of Star-Forming Galaxies at $1.4\le z\le 2.6$
• Primordial Deuterium after LUNA: concordances and error budget
• Mock weak lensing analysis of simulated galaxy clusters: bias and scatter in mass and concentration
• Dark energy in light of the early JWST observations: case for a negative cosmological constant?
• The Horizon Run N-body Simulation: Baryon Acoustic Oscillations and Topology of Large Scale Structure of the Universe
• On Larger $H_0$ Values in the CMB Dipole Direction
• Probing observational bounds on scalar-tensor theories from standard sirens
• Effects of baryon removal on the structure of dwarf spheroidal galaxies
• Observational bounds on the cosmic radiation density
• Constraints and analytical solutions of $f(R)$ theories of gravity using Noether symmetries
• Shadow and weak deflection angle of extended uncertainty principle black hole surrounded with dark matter
• The Megamaser Cosmology Project VIII. A Geometric Distance to NGC 5765b
• SN2023ixf in Messier 101: A Variable Red Supergiant as the Progenitor Candidate to a Type II Supernova
• Cosmological Constraints from the ROSAT Deep Cluster Survey
• Future singularities and Teleparallelism in Loop Quantum Cosmology
• Improved constraints on cosmological parameters from SNIa data
• Self-interacting asymmetric dark matter coupled to a light massive dark photon
• The X-ray fundamental plane of the Platinum Sample, the Kilonovae and the SNe Ib/c associated with GRBs
• Direct Detection of the Wino- and Higgsino-like Neutralino Dark Matters at One-Loop Level
• Finite-time Cosmological Singularities and the Possible Fate of the Universe
• Dark matters on the scale of galaxies
• Charged-particle decay and suppression of small-scale power
• New constraints on time-dependent variations of fundamental constants using Planck data
• On the EFT of Large Scale Structures in Redshift Space
• Using Galaxy Two-point Correlation Functions to Determine the Redshift Distributions of Galaxies Binned by Photometric Redshift
• Dark Energy Survey Year 1 Results: Constraints on Intrinsic Alignments and their Colour Dependence from Galaxy Clustering and Weak Lensing
• New Constraints on Warm Dark Matter from the Lyman-$\alpha$ Forest Power Spectrum
• Quantum Horizons of the Standard Model Landscape
• Cosmic acceleration in dust only Universe via energy-momentum powered gravity
• The effect of a massive object on an expanding universe
• How to constrain warm dark matter with the Lyman $\alpha$ forest
• Gamma-ray induced cascades and magnetic fields in intergalactic medium
• The cosmic microwave background temperature bispectrum from scalar perturbations induced by primordial magnetic fields
• An independent determination of the local Hubble constant
• Has JWST already falsified dark-matter-driven galaxy formation?
• Slope evolution of GRB correlations and cosmology
• Can late-time extensions solve the $H_0$ and ${\sigma }_8$ tensions?
• CMB and BBN constraints on evaporating primordial black holes revisited
• The Novel Probes Project -- Tests of Gravity on Astrophysical Scales
• Dark calling Dark: Interaction in the dark sector in presence of neutrino properties after Planck CMB final release
• A Subaru Weak Lensing Survey I: Cluster Candidates and Spectroscopic Verification
• Thermal Dark Matter Below an MeV
• Signals From the Epoch of Cosmological Recombination
• Disformal couplings and the dark sector of the universe
• A light in the dark: searching for electromagnetic counterparts to black hole-black hole mergers in LIGO/Virgo O3 with the Zwicky Transient Facility
• Disformal Scalar Fields and the Dark Sector of the Universe
• Precise Time Delays from Strongly Gravitationally Lensed Type Ia Supernovae with Chromatically Microlensed Images
• Comparing early dark energy and extra radiation solutions to the Hubble tension with BBN
• UNCOVER: Illuminating the Early Universe -- JWST/NIRSpec Confirmation of $z>12$ Galaxies
• Finsler spacetime geometry in Physics
• Baryonic Tully-Fisher Relation for Extremely Low Mass Galaxies
• BICEP Array: a multi-frequency degree-scale CMB polarimeter
• Old-Aged Stellar Population Distance Indicators
• LRP 2020 Whitepaper: The Canadian Hydrogen Observatory and Radio-transient Detector (CHORD)
• Bayesian Lensing Shear Measurement
• Search for sterile neutrinos in holographic dark energy cosmology: Reconciling Planck observation with the local measurement of the Hubble constant
• Future Type Ia Supernova Data as Tests of Dark Energy from Modified Friedmann Equations
• Consistent lensing and clustering in a low-$S_8$ Universe with BOSS, DES Year 3, HSC Year 1 and KiDS-1000
• Strong lensing time-delay cosmography in the 2020s
• The OGLE View of Microlensing towards the Magellanic Clouds. III. Ruling out sub-solar MACHOs with the OGLE-III LMC data
• Testing Screened Modified Gravity
• AMICO galaxy clusters in KiDS-DR3: sample properties and selection function
• Matching current observational constraints with nonminimally coupled dark energy
• Recovering 3D clustering information with angular correlations
• Reconstructing Functions and Estimating Parameters with Artificial Neural Networks: A Test with the Hubble Parameter and SNe Ia
• Luminosity--time and luminosity--luminosity correlations for GRB prompt and afterglow plateau emissions
• The Baryonic Tully-Fisher Relationship for S${}^4$G Galaxies and the "Condensed" Baryon Fraction of Galaxies
• Modeling projection effects in optically-selected cluster catalogues
• Hubble tension or a transition of the Cepheid SnIa calibrator parameters?
• Gaia Data Release 3: The Galaxy in your preferred colours. Synthetic photometry from Gaia low-resolution spectra
• Constraining early and interacting dark energy with gravitational wave standard sirens: the potential of the eLISA mission
• Cosmological Applications of Pade Approximant
• The length of the low-redshift standard ruler
• Evidence for suppression of structure growth in the concordance cosmological model
• Slow-roll inflation in $f(Q)$ non-metric gravity
• Impact of neutrino properties on the estimation of inflationary parameters from current and future observations
• Relieving the $H_0$ tension with a new interacting dark energy model
• The Big-Bang Singularity in the framework of a Generalized Uncertainty Principle
• Unification of inflation and dark energy {\it à la} quintessential inflation
• Search for Dark Matter Axions with CAST-CAPP
• A new perspective on Dark Energy modeling via Genetic Algorithms
• The Case for an EeV Gravitino
• A new measurement of the Hubble constant and matter content of the Universe using extragalactic background light $\gamma$-ray attenuation
• The Challenge of the Largest Structures in the Universe to Cosmology
• Constraints on Cosmological Parameters from the 500 deg${}^2$ SPTpol Lensing Power Spectrum
• Standard rulers, candles, and clocks from the low-redshift Universe
• The Local Hole in the Galaxy Distribution: Evidence from 2MASS
• Post-Inflationary Gravitino Production Revisited
• Assessing the effects of foregrounds and sky removal in WMAP
• Detection of a Supervoid Aligned with the Cold Spot of the Cosmic Microwave Background
• Dark matter component decaying after recombination: lensing constraints with Planck data
• Tracing The Sound Horizon Scale With Photometric Redshift Surveys
• Quintom cosmology and modified gravity after DESI 2024
• Running vacuum in quantum field theory in curved spacetime: renormalizing ${\rho }_{vac}$ without $\sim m^4$ terms
• The HST/ACS Coma Cluster Survey: I - Survey Objectives and Design
• Cosmological model insensitivity of local $H_0$ from the Cepheid distance ladder
• Constraints on $\Lambda$CDM Extensions from the SPT-3G 2018 $EE$ and $TE$ Power Spectra
• A class of quintessential inflation models with parameter space consistent with BICEP2
• Light Neutralino Dark Matter: Direct/Indirect Detection and Collider Searches
• A study of gamma ray bursts with afterglow plateau phases associated with supernovae
• The Impact of New d(p,γ)He3 Rates on Big Bang Nucleosynthesis
• AX-GADGET: a new code for cosmological simulations of Fuzzy Dark Matter and Axion models
• Non-extensive Statistics Solution to the Cosmological Lithium Problem
• Toward a New Distance to the Active Galaxy NGC 4258: II. Centripetal Accelerations and Investigation of Spiral Structure
• Implication of the Hubble tension for the primordial Universe in light of recent cosmological data
• Dust in the Circumgalactic Medium of Low-Redshift Galaxies
• The Megamaser Cosmology Project. V. An Angular Diameter Distance to NGC 6264 at 140 Mpc
• Angular Baryon Acoustic Oscillation measure at z=2.225 from the SDSS quasar survey
• A designer approach to $f(Q)$ gravity and cosmological implications
• Dark Sirens to Resolve the Hubble-Lemaître Tension
• Small-scale microwave background anisotropies due to tangled primordial magnetic fields
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: theoretical systematics and Baryon Acoustic Oscillations in the galaxy correlation function
• Baryon Acoustic Oscillations from the SDSS DR10 galaxies angular correlation function
• A Study of the Gamma-Ray Burst Fundamental Plane
• Cosmology Intertwined IV: The Age of the Universe and its Curvature
• Inflation meets neutrinos
• Toward a standard Gamma Ray Burst: tight correlations between the prompt and the afterglow plateau phase emission
• Radiative Production of Non-thermal Dark Matter
• Constraining the GRB-magnetar model by means of the Galactic pulsar population
• CMB Constraints on a Stochastic Background of Primordial Magnetic Fields
• Cosmology with the EFTofLSS and BOSS: dark energy constraints and a note on priors
• Observational constraints on successful model of quintessential Inflation
• Cosmic chronometers to calibrate the ladders and measure the curvature of the Universe. A model-independent study
• New Early Dark Energy is compatible with current LSS data
• A Profile Likelihood Analysis of the Constrained MSSM with Genetic Algorithms
• On the baryonic, stellar, and luminous scaling relations of disk galaxies
• Quasar X-ray and UV flux, baryon acoustic oscillation, and Hubble parameter measurement constraints on cosmological model parameters
• An Extended Matter Bounce Scenario: current status and challenges
• The impact of feedback from galaxy formation on the Lyman-alpha transmitted flux
• Baryonic effects for weak lensing. Part I. Power spectrum and covariance matrix
• A detection of the integrated Sachs-Wolfe imprint of cosmic superstructures using a matched-filter approach
• Measuring $\alpha$ in the Early Universe: CMB Polarization, Reionization and the Fisher Matrix Analysis
• Hyper Suprime-Cam Year 3 Results: Cosmology from Galaxy Clustering and Weak Lensing with HSC and SDSS using the Minimal Bias Model
• Evidence for Emergent Dark Energy
• Determining the Hubble Constant without the Sound Horizon: Measurements from Galaxy Surveys
• Exploring the full parameter space for an interacting dark energy model with recent observations including redshift-space distortions: Application of the parametrized post-Friedmann approach
• Galaxy clustering in the DESI Legacy Survey and its imprint on the CMB
• The impact of the cosmic variance on $H_0$ on cosmological analyses
• TDCOSMO V: strategies for precise and accurate measurements of the Hubble constant with strong lensing
• Dark sector interaction and the supernova absolute magnitude tension
• Templates for Fitting Photometry of Ultra-High-Redshift Galaxies
• Sharpening the Tip of the Red Giant Branch
• The three-year shear catalog of the Subaru Hyper Suprime-Cam SSP Survey
• Galaxy Bias and its Effects on the Baryon Acoustic Oscillations Measurements
• The high mass end of the Tully-Fisher relation
• Testing Late Time Cosmic Acceleration with uncorrelated Baryon Acoustic Oscillations dataset
• Inhomogeneous vacuum energy
• Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations
• A massive blow for $\Lambda$CDM $-$ the high redshift, mass, and collision velocity of the interacting galaxy cluster El Gordo contradicts concordance cosmology
• Large-Scale Clustering of Cosmic Voids
• Anisotropic non-Gaussianity from vector field perturbations
• Precision cosmology with voids in the final BOSS data
• Cosmicflows-2: I-band Luminosity - HI Linewidth Calibration
• Model-independent test of the FLRW metric, the flatness of the Universe, and non-local measurement of $H_0{r}_{\mathrm{d}}$
• The Atacama Cosmology Telescope: Constraints on Cosmic Birefringence
• A standard siren measurement of the Hubble constant using gravitational wave events from the first three LIGO/Virgo observing runs and the DESI Legacy Survey
• A Model of Universe Anisotropization
• Cosmology with the Galaxy Bispectrum Multipoles: Optimal Estimation and Application to BOSS Data
• Constraints on coupled dark energy using CMB data from WMAP and SPT
• Assessing tension metrics with Dark Energy Survey and Planck data
• Spatially Resolved Properties of High Redshift Galaxies in the SMACS0723 JWST ERO Field
• The Megamaser Cosmology Project. VI. Observations of NGC 6323
• The Megamaser Cosmology Project. II. The Angular-Diameter Distance to UGC 3789
• Relaxing Cosmological Neutrino Mass Bounds with Unstable Neutrinos
• What are $Om{h}^2(z_1,z_2)$ and $Om(z_1,z_2)$ diagnostics telling us in light of $H(z)$ data?
• Arc sensitivity to cluster ellipticity, asymmetries and substructures
• ARCADE 2 Observations of Galactic Radio Emission
• The FAST all sky HI survey (FASHI): The first release of catalog
• Searching for dark matter - dark energy interactions: going beyond the conformal case
• Cosmology Intertwined I: Perspectives for the Next Decade
• M-flation: Inflation From Matrix Valued Scalar Fields
• AMICO galaxy clusters in KiDS-DR3: weak-lensing mass calibration
• Cepheids in Open Clusters: An 8-D All-sky Census
• Cosmological Limits on the Neutrino Mass and Lifetime
• Asymptotically safe inflation from quadratic gravity
• Late time approaches to the Hubble tension deforming $H(z)$, worsen the growth tension
• Reconciling $H_0$ tension in a six parameter space?
• An overview of what current data can (and cannot yet) say about evolving dark energy
• Arguments against using $h^{-1}\mathrm{Mpc}$ units in observational cosmology
• Evidence of a decreasing trend for the Hubble constant
• Testing models of vacuum energy interacting with cold dark matter
• Ultra-light axions and the $S_8$ tension: joint constraints from the cosmic microwave background and galaxy clustering
• Fuzzy Dark Matter and Dark Matter Halo Cores
• Possible structure in the GRB sky distribution at redshift two
• WMAP Constraints on varying $\alpha$ and the Promise of Reionization
• A measurement of large-scale peculiar velocities of clusters of galaxies: technical details
• Direct detection of dark energy: the XENON1T excess and future prospects
• Dark Matter Halos with Cores from Hierarchical Structure Formation
• A model independent null test on the cosmological constant
• Late-transition vs smooth $H(z)$ deformation models for the resolution of the Hubble crisis
• Dark Energy Survey Year 3 Results: Clustering Redshifts -- Calibration of the Weak Lensing Source Redshift Distributions with redMaGiC and BOSS/eBOSS
• The Sloan Great Wall. Morphology and galaxy content
• Fast cosmological parameter estimation using neural networks
• Do LIGO/Virgo black hole mergers produce AGN flares? The case of GW190521 and prospects for reaching a confident association
• Vacuum models with a linear and a quadratic term in H: structure formation and number counts analysis
• Effective Theory of Dark Energy at Redshift Survey Scales
• Dark Matter Halos of Disk Galaxies: Constraints from the Tully-Fisher Relation
• Distance estimates for AGB stars from parallax measurements
• Combined Preheating on the lattice with applications to Higgs inflation
• Resolved Near-Infrared Stellar Populations in Nearby Galaxies
• Phases of New Physics in the BAO Spectrum
• Reconstructing the dark sector interaction with LISA
• Recognising Axionic Dark Matter by Compton and de-Broglie Scale Modulation of Pulsar Timing
• CEERS Key Paper IV: Galaxies at $4<z<9$ are Bluer than They Appear -- Characterizing Galaxy Stellar Populations from Rest-Frame $\sim 1$ micron Imaging
• Black holes in galactic centers: quasinormal ringing, grey-body factors and Unruh temperature
• Testing GRBs as Standard Candles
• Ultra-light dark matter in disk galaxies
• Cosmic Shear Cosmology Beyond 2-Point Statistics: A Combined Peak Count and Correlation Function Analysis of DES-Y1
• Recombination-independent determination of the sound horizon and the Hubble constant from BAO
• Expanded haloes, abundance matching and too-big-to-fail in the Local Group
• Measurements of $H_0$ in modified gravity theories: The role of lensed quasars in the late-time Universe
• AMICO galaxy clusters in KiDS-DR3: cosmological constraints from counts and stacked weak-lensing
• B polarization of the CMB from Faraday rotation
• Early results from GLASS-JWST. XI: Stellar masses and mass-to-light ratio of z>7 galaxies
• Dark Radiation Emerging After Big Bang Nucleosynthesis?
• Gravitational and Chiral Anomalies in the Running Vacuum Universe and Matter-Antimatter Asymmetry
• High-Redshift Galaxies from Early JWST Observations: Constraints on Dark Energy Models
• Unveiling Dark Matter free-streaming at the smallest scales with high redshift Lyman-alpha forest
• The XXL Survey XXV. Cosmological analysis of the C1 cluster number counts
• The integrated Sachs-Wolfe imprints of cosmic superstructures: a problem for ΛCDM
• A fast test to assess the impact of marginalization in Monte Carlo analyses, and its application to cosmology
• On the impact of baryons on the halo mass function, bias, and cluster cosmology
• Do cosmological observations allow a negative $\Lambda$?
• Clustering and Halo Abundances in Early Dark Energy Cosmological Models
• Scattering of Dark Matter and Dark Energy
• The Tully-Fisher and mass-size relations from halo abundance matching
• Testing homogeneity on large scales in the Sloan Digital Sky Survey Data Release One
• $H_0$ Tension, Swampland Conjectures and the Epoch of Fading Dark Matter
• Constraining neutrino mass with tomographic weak lensing one-point probability distribution function and power spectrum
• Ginzburg-Landau Theory of Dark Energy: A Framework to Study Both Temporal and Spatial Cosmological Tensions Simultaneously
• A dark matter interpretation for the ARCADE excess?
• Bianchi Model CMB Polarization and its Implications for CMB Anomalies
• First Constraint on the Neutrino-Induced Phase Shift in the BAO Spectrum
• Non-Gaussianity from Cosmic Magnetic Fields
• The BOSS bispectrum analysis at one loop from the Effective Field Theory of Large-Scale Structure
• The slope of the Baryonic Tully-Fisher relation
• Multiplicity of Galactic Cepheids and RR Lyrae stars from Gaia DR2 - I. Binarity from proper motion anomaly
• The state of the dark energy equation of state circa 2023
• Integral constraints in spectroscopic surveys
• High-precision limit on variation in the fine-structure constant from a single quasar absorption system
• Constraining the time evolution of dark energy, curvature and neutrino properties with cosmic chronometers
• Relieving the Tension between Weak Lensing and Cosmic Microwave Background with Interacting Dark Matter and Dark Energy Models
• Numerical evolution of squeezed and non-Gaussian states in loop quantum cosmology
• Improving time-delay cosmography with spatially resolved kinematics
• Redshift Space Distortions in the Effective Field Theory of Large Scale Structures
• Coupled quintessence with a $\Lambda$CDM background: removing the ${\sigma }_8$ tension
• zeus: A Python implementation of Ensemble Slice Sampling for efficient Bayesian parameter inference
• The DIRECT Project: Influence of Blending on the Cepheid Distance Scale. I. Cepheids in M31
• Euclid: Forecast constraints on the cosmic distance duality relation with complementary external probes
• Constraining Gravity at the Largest Scales through CMB Lensing and Galaxy Velocities
• The past and future dynamics of quintom dark energy models
• Model-independent reconstruction of the Interacting Dark Energy Kernel: Binned and Gaussian process
• Type Ia supernovae, standardisable candles, and gravity
• A String and M-theory Origin for the Salam-Sezgin Model
• The Local Hole revealed by galaxy counts and redshifts
• Validation of the accuracy and precision of Gaia EDR3 parallaxes with globular clusters
• A Near-Infrared Period-Luminosity Relation for Miras in NGC 4258, an Anchor for a New Distance Ladder
• A Consistent View of Interacting Dark Energy from Multiple CMB Probes
• New Constraints on the Primordial Magnetic Field
• The Hitchhiker's guide to the galaxy catalog approach for gravitational wave cosmology
• Anisotropy in the Hubble constant as observed in the HST Extragalactic Distance Scale Key Project results
• Origin of Sterile Neutrino Dark Matter via Vector Secret Neutrino Interactions
• The eROSITA Final Equatorial-Depth Survey (eFEDS): X-ray Observable-to-Mass-and-Redshift Relations of Galaxy Clusters and Groups with Weak-Lensing Mass Calibration from the Hyper Suprime-Cam Subaru Strategic Program Survey
• Robustness of dark energy phenomenology across different parameterizations
• Omnipotent dark energy: A phenomenological answer to the Hubble tension
• Equivalent Neutrinos, Light WIMPs, and the Chimera of Dark Radiation
• Dark Energy Survey Year 3 results: cosmological constraints from the analysis of cosmic shear in harmonic space
• Higgs inflation in the Palatini formulation with kinetic terms for the metric
• Cosmological constraints from baryon acoustic oscillations and clustering of large-scale structure
• A 5% measurement of the Hubble constant from Type II supernovae
• NIHAO V: Too big doesn't fail -- reconciling the conflict between LCDM predictions and the circular velocities of nearby field galaxies
• Relativistic N-body simulations with massive neutrinos
• A new measurement of the expansion history of the Universe at z=1.26 with cosmic chronometers in VANDELS
• The Carnegie-Chicago Hubble Program. II. The Distance to IC 1613: The Tip of the Red Giant Branch and RR Lyrae Period-Luminosity Relations
• Using neural networks to estimate redshift distributions. An application to CFHTLenS
• DeepCMB: Lensing Reconstruction of the Cosmic Microwave Background with Deep Neural Networks
• Cosmology From CMB Lensing and Delensed EE Power Spectra Using 2019-2020 SPT-3G Polarization Data
• The baryonic content and Tully-Fisher relation at z~0.6
• Towards early dark energy and $n_s$=1 with Planck, ACT and SPT
• Toward a New Geometric Distance to the Active Galaxy NGC4258: I. VLBI Monitoring of Water Maser Emission
• On the Viability of Bianchi Type VIIh Models with Dark Energy
• The Gamma-ray Bursts fundamental plane correlation as a cosmological tool
• Magnetized CMB observables: a dedicated numerical approach
• Distance Determination To Eight Galaxies Using Expanding Photosphere Method
• Constraining the time variation of Newton's constant $G$ with gravitational-wave standard sirens and supernovae
• Primordial power spectrum in light of JWST observations of high redshift galaxies
• Did JWST observe imprints of axion miniclusters or primordial black holes?
• Resolving the Hubble tension with Early Dark Energy
• Qualitative dynamics and inflationary attractors in loop cosmology
• Measuring the Hubble constant and spatial curvature from supernova apparent magnitude, baryon acoustic oscillation, and Hubble parameter data
• Spherical collapse and halo mass function in f(R) theories
• Model-independent determination of $H_0$ and ${\Omega }_{K0}$ from strong lensing and type Ia supernovae
• Calibration of the Mid-Infrared Tully-Fisher Relation
• DES Y3 cosmic shear down to small scales: constraints on cosmology and baryons
• Consistency of effective field theory analyses of the BOSS power spectrum
• Constraining the range of Yukawa gravity interaction from S2 star orbits II: Bounds on graviton mass
• Constraining primordial magnetic fields with distortions of the black-body spectrum of the cosmic microwave background: pre- and post-decoupling contributions
• Cosmological Bound on the QCD Axion Mass, Redux
• Bounds on light sterile neutrino mass and mixing from cosmology and laboratory searches
• More out of less: an excess integrated Sachs-Wolfe signal from supervoids mapped out by the Dark Energy Survey
• Calibrating Dark Energy
• On the linearity of tracer bias around voids
• How to use GP: Effects of the mean function and hyperparameter selection on Gaussian Process regression
• The Hubble tension and a renormalizable model of gauged neutrino self-interactions
• New period-luminosity and period-color relations of classical Cepheids: III. Cepheids in SMC
• Rational approximations of $f(R)$ cosmography through Padé polynomials
• The Cosmic Microwave Background and the Ionization History of the Universe
• The Hubble Tension as a Hint of Leptogenesis and Neutrino Mass Generation
• CMB Anisotropy of the Poincare Dodecahedron
• The UTMOST: A hybrid digital signal processor transforms the MOST
• The IRAS PSCz Dipole
• Seeing patterns in noise: Gigaparsec-scale `structures' that do not violate homogeneity
• The Milky Way Cepheid Leavitt law based on Gaia DR2 parallaxes of companion stars and host open cluster populations
• The Type Ia Supernova Color-Magnitude Relation and Host Galaxy Dust: A Simple Hierarchical Bayesian Model
• Tight bonds between sterile neutrinos and dark matter
• Constraining the Dark Energy Equation of State with HII Galaxies
• Observational constraints on the deceleration parameter in a tilted universe
• Breaking degeneracies in modified gravity with higher (than 2nd) order weak-lensing statistics
• Measuring chiral gravitational waves in Chern-Simons gravity with CMB bispectra
• Further empirical evidence for the non-linearity of the period-luminosity relations as seen in the Large Magellanic Cloud Cepheids
• Running vacuum in the Universe: phenomenological status in light of the latest observations, and its impact on the ${\sigma }_8$ and $H_0$ tensions
• CMB Power Asymmetry from Non-Gaussian Modulation
• Revisit of the interacting holographic dark energy model after Planck 2015
• Gravitational wave cosmology with extreme mass-ratio inspirals
• Measurements of $H_0$ and reconstruction of the dark energy properties from a model-independent joint analysis
• Ups and Downs in Dark Energy: phase transition in dark sector as a proposal to lessen cosmological tensions
• Suppressing structure formation at dwarf galaxy scales and below: late kinetic decoupling as a compelling alternative to warm dark matter
• Observational evidence for a local underdensity in the Universe and its effect on the measurement of the Hubble Constant
• Screening $\Lambda$ in a new modified gravity model
• Observation of interstellar lithium in the low-metallicity Small Magellanic Cloud
• Lorentz-covariant deformed algebra with minimal length
• Addressing $H_0$ tension by means of VCDM
• Tidal Deformability of Dark Matter Admixed Neutron Stars
• Sources of the Radio Background Considered
• A giant ring-like structure at 0.78<z<0.86 displayed by GRBs
• Modulated Natural Inflation
• Accelerating astronomical and cosmological inference with Preconditioned Monte Carlo
• Cosmological constraints on multi-interacting dark matter
• Genetic Algorithms and Supernovae Type Ia Analysis
• Precision Scaling Relations for Disk Galaxies in the Local Universe
• Cosmology and modified gravitational wave propagation from binary black hole population models
• A Robust and Efficient Deep Learning Method for Dynamical Mass Measurements of Galaxy Clusters
• Late time transitions in the quintessence field and the $H_0$ tension
• Dawn of the dark: unified dark sectors and the EDGES Cosmic Dawn 21-cm signal
• Phenomenology of the generalized cubic covariant Galileon model and cosmological bounds
• Updated Constraints and Forecasts on Primordial Tensor Modes
• Modified Dispersion Relations from Closed Strings in Toroidal Cosmology
• The lensing and temperature imprints of voids on the Cosmic Microwave Background
• Distinguishing standard and modified gravity cosmologies with machine learning
• Implications of a Stochastic Microscopic Finsler Cosmology
• Observational constraints on braneworld inflation: the effect of a Gauss-Bonnet term
• Test of the cosmic evolution using Gaussian processes
• Euclid: Forecasts from redshift-space distortions and the Alcock-Paczynski test with cosmic voids
• The Impact of the Fiducial Cosmology Assumption on BAO Cosmological Parameter Inference
• The Nearby Supernova Factory
• Quasar standardization: Overcoming Selection Biases and Redshift Evolution
• Homogeneous and isotropic cosmologies with nonlinear electromagnetic radiation
• The halo model for cosmology: a pedagogical review
• Cosmological constraints on the neutrino mass including systematic uncertainties
• Flavor-specific Interaction Favors Strong Neutrino Self-coupling in the Early Universe
• Early galaxy formation in warm dark matter cosmologies
• Remedy of some cosmological tensions via effective phantom-like behavior of interacting vacuum energy
• BAO+BBN revisited -- Growing the Hubble tension with a 0.7km/s/Mpc constraint
• Cosmological constraints on late-universe decaying dark matter as a solution to the $H_0$ tension
• Falsifying $\Lambda$CDM: Model-independent tests of the concordance model with eBOSS DR14Q and Pantheon
• Black hole in quantum wave dark matter
• Dark energy, the electroweak vacua and collider phenomenology
• Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies
• Model-independent constraints on the cosmological anisotropic stress
• A Measurement of Gravitational Lensing of the Cosmic Microwave Background Using SPT-3G 2018 Data
• Are Cluster Magnetic Fields Primordial ?
• Infrared Tip of the Red Giant Branch and Distances to the Maffei/IC 342 Group
• The Radial Tully-Fisher relation for spiral galaxies I
• Cosmic rays and TeV photons as probes of quantum properties of space-time
• HICOSMO - Cosmology with a complete sample of galaxy clusters: I. Data analysis, sample selection and luminosity-mass scaling-relation
• Neutrino Self-Interactions and Double Beta Decay
• Constraints on Primordial Magnetic Fields from Planck combined with the South Pole Telescope CMB B-mode polarization measurements
• Additional Light Sterile Neutrinos and Cosmology
• $f(R)$ gravity in the Jordan Frame as a Paradigm for the Hubble Tension
• Baryon-driven growth of solitonic cores in fuzzy dark matter halos
• Time-delay Cosmography: Increased Leverage with Angular Diameter Distances
• Spectral analysis of Fermi-LAT gamma-ray bursts with known redshift and their potential use as cosmological standard candles
• Late time interacting cosmologies and the Hubble constant tension
• New quantum aspects of a vacuum-dominated universe
• KiDS-1000: cosmic shear with enhanced redshift calibration
• Model-agnostic assessment of dark energy after DESI DR1 BAO
• STRIDES: Automated uniform models for 30 quadruply imaged quasars
• A Stringent Limit on the Warm Dark Matter Particle Masses from the Abundance of z=6 Galaxies in the Hubble Frontier Fields
• Confronting Dark Energy Models using Galaxy Cluster Number Counts
• Redshift evolution of the underlying type Ia supernova stretch distribution
• Linear cosmological constraints on 2-body decaying dark matter scenarios and the $S_8$ tension
• Constraining the physical properties of the first lensed $z\sim 10-16$ galaxy candidates with JWST
• $T_0$ censorship of early dark energy and AdS vacua
• The Sherwood-Relics simulations: overview and impact of patchy reionization and pressure smoothing on the intergalactic medium
• Teleparallel theories of gravity as analogue of non-linear electrodynamics
• How unusual are the Shapley Supercluster and the Sloan Great Wall?
• Dynamical Dark Energy Beyond Planck? Constraints from multiple CMB probes, DESI BAO and Type-Ia Supernovae
• Hybrid cosmological attractors
• Cosmological equivalence principle and the weak-field limit
• Can Gravitational Instantons Really Constrain Axion Inflation?
• Determination of the primordial helium abundance based on NGC 346 an HII region of the Small Magellanic Cloud
• Long Range Interactions in Cosmology: Implications for Neutrinos
• Galactic Rotation Dynamics in f(T) gravity
• Non-Gaussian estimates of tensions in cosmological parameters
• Imprint of the seesaw mechanism on feebly interacting dark matter and the baryon asymmetry
• BAO angular scale at z_eff = 0.11 with the SDSS blue galaxies
• Exploring the high-redshift PBH-$\Lambda$CDM Universe: early black hole seeding, the first stars and cosmic radiation backgrounds
• Robustness of baryon acoustic oscillation constraints for early-Universe modifications to $\Lambda$CDM
• COMAP Early Science: I. Overview
• Mitigating Shear-dependent Object Detection Biases with Metacalibration
• What Can WMAP Tell Us About The Very Early Universe? New Physics as an Explanation of Suppressed Large Scale Power and Running Spectral Index
• Standard Siren Speeds: Improving velocities in gravitational-wave measurements of $H_0$
• Primordial Magnetic Field Limits from Cosmic Microwave Background Bispectrum of Magnetic Passive Scalar Modes
• Coupled and uncoupled early dark energy, massive neutrinos and the cosmological tensions
• Relaxing the ${\sigma }_8$-tension through running vacuum in the Universe
• Constraining Neutrino Mass with the Tomographic Weak Lensing Bispectrum
• Can a supervoid explain the Cold Spot?
• Model-independent reconstruction of the linear anisotropic stress $\eta$
• Dark Energy Constraints after Planck
• Model-independent reconstruction of $f(T)$ teleparallel cosmology
• Measuring the dark flow with public X-ray cluster data
• Dynamics and Afterglow Light Curves of GRB Blast Waves with a Long-lived Reverse Shock
• The Early Dark Sector, the Hubble Tension, and the Swampland
• An Improved Calibration of the Wavelength Dependence of Metallicity on the Cepheid Leavitt law
• Reconstruction of the Dark Energy equation of state
• Constraints on the Evolution of the Primordial Magnetic Field from the Small-Scale Cosmic Microwave Background Angular Anisotropy
• The Megamaser Cosmology Project.IX. Black hole masses for three maser galaxies
• A new cosmological distance measure using AGN X-ray variability
• The stacked ISW signal of rare superstructures in ΛCDM
• A theory of type-II minimally modified gravity
• Independent Cosmological Constraints from high-z HII Galaxies
• Addressing the cosmological $H_0$ tension by the Heisenberg uncertainty
• Determining the Hubble Constant without the Sound Horizon Scale: Measurements from CMB Lensing
• Phase Portraits of general f(T) Cosmology
• Dark energy from quantum gravity discreteness
• The baryonic Tully-Fisher relation and galactic outflows
• Generalized Emergent Dark Energy Model and the Hubble Constant Tension
• The Impact of Peculiar Velocities on the Estimation of the Hubble Constant from Gravitational Wave Standard Sirens
• Explaining Cosmological Anisotropy: Evidence for Causal Horizons from CMB data
• CMB anisotropies due to cosmological magnetosonic waves
• Cosmological Constraints from Galaxy Clusters and Groups in the eROSITA Final Equatorial Depth Survey
• Testing spatial curvature and anisotropic expansion on top of the $\Lambda$CDM model
• Massive black hole binaries in LISA: multimessenger prospects and electromagnetic counterparts
• Rastall gravity extension of the standard $\Lambda$CDM model: theoretical features and observational constraints
• Concordance cosmology without dark energy
• Cosmology under the fractional calculus approach
• Cosmological Constraints from Gas Mass Fractions of Massive, Relaxed Galaxy Clusters
• Gaussian processes and effective field theory of $f(T)$ gravity under the $H_0$ tension
• Parallax of Galactic Cepheids from Spatially Scanning the Wide Field Camera 3 on the Hubble Space Telescope: The Case of SS Canis Majoris
• Data-driven Reconstruction of the Late-time Cosmic Acceleration with f(T) Gravity
• Prospects for Constraining Interacting Dark Energy Models with 21 cm Intensity Mapping Experiments
• Dynamics of nonlinear interacting dark energy models
• Testing the Cosmological Principle with CatWISE Quasars: A Bayesian Analysis of the Number-Count Dipole
• The BINGO Project I: Baryon Acoustic Oscillations from Integrated Neutral Gas Observations
• A large sample of shear selected clusters from the Hyper Suprime-Cam Subaru Strategic Program S16A wide field mass maps
• BICEP2 / Keck Array IX: New Bounds on Anisotropies of CMB Polarization Rotation and Implications for Axion-Like Particles and Primordial Magnetic Fields
• Direct detection of dark matter: a critical review
• Neutrino-Assisted Early Dark Energy: Theory and Cosmology
• Gamma-Ray Bursts, Quasars, Baryonic Acoustic Oscillations, and Supernovae Ia: new statistical insights and cosmological constraints
• Multipole decomposition of the general luminosity distance 'Hubble law' -- a new framework for observational cosmology
• Listening to the Universe with Next Generation Ground-Based Gravitational-Wave Detectors
• The supercluster--void network II. An oscillating cluster correlation function
• Constraints on interacting dark energy models through cosmic chronometers and Gaussian process
• Cosmological constraints on an exponential interaction in the dark sector
• Quantifying the Effects of Known Unknowns on Inferred High-redshift Galaxy Properties: Burstiness, the IMF, and Nebular Physics
• EPOCHS IV: SED Modelling Assumptions and their impact on the Stellar Mass Function at 6.5 < z < 13.5 using PEARLS and public JWST observations
• Euclid Preparation. XXVIII. Forecasts for ten different higher-order weak lensing statistics
• Isotropic cosmic birefringence from early dark energy
• Time-delay cosmographic forecasts with strong lensing and JWST stellar kinematics
• Viability of the matter bounce scenario in Loop Quantum Cosmology for general potentials
• Parametric and nonparametric methods hint dark energy evolution
• Model independent inference of the expansion history and implications for the growth of structure
• Forecasting constraints on deviations from general relativity in $f(Q)$ gravity with standard sirens
• The ARCADE 2 Instrument
• Cosmological equivalence between the Finsler-Randers space-time and the DGP gravity model
• Dark Stars: a new look at the First Stars in the Universe
• Light axion-like dark matter must be present during inflation
• Do we Live in a "Small Universe"?
• CMB Maximum Temperature Asymmetry Axis: Alignment with Other Cosmic Asymmetries
• Gravitoelectromagnetism, Solar System Test and Weak-Field Solutions in $f(T,B)$ Gravity with Observational Constraints
• Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework
• A double take on early and interacting dark energy from JWST
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: constraining modified gravity
• Hot New Early Dark Energy
• Measuring the transverse baryonic acoustic scale from the SDSS DR11 galaxies
• The Parallax Zero-Point of Gaia Early Data Release 3 from LAMOST Primary Red Clump Stars
• Cosmological implications of scale-independent energy-momentum squared gravity: Pseudo nonminimal interactions in dark matter and relativistic relics
• Cosmic viscosity as a remedy for tension between PLANCK and LSS data
• Spin-Dependent WIMPs in DAMA?
• New NIR light-curve templates for classical Cepheids
• Gravitational Waves from Light Cosmic Strings: Backgrounds and Bursts with Large Loops
• Cosmological exploitation of the size function of cosmic voids identified in the distribution of biased tracers
• Generalized Emergent Dark Energy: observational Hubble data constraints and stability analysis
• Cosmic variance of the galaxy cluster weak lensing signal
• Dark Radiation from Particle Decays during Big Bang Nucleosynthesis
• Dynamical analysis on $f(R,\mathcal{G})$ cosmology
• Euclid: Cosmological forecasts from the void size function
• Simulating the 21-cm signal from reionisation including non-linear ionisations and inhomogeneous recombinations
• Resolving Cosmic Gamma Ray Anomalies with Dark Matter Decaying Now
• Right-Handed Neutrinos as the Dark Radiation: Status and Forecasts for the LHC
• Observable primordial vector modes
• A parallax distance to 3C 273 through spectroastrometry and reverberation mapping
• Quantifying Scalar Field Dynamics with DESI 2024 Y1 BAO measurements
• A tale of two (or more) $h$'s
• Anisotropic dark energy and CMB anomalies
• Resolving the $H_0$ tension with diffusion
• Calibration of bias and scatter involved in cluster mass measurements using optical weak gravitational lensing
• Primordial Magnetic Field Limits from CMB Trispectrum - Scalar Modes and Planck Constraints
• Model-independent cosmological inference post DESI DR1 BAO measurements
• Addressing the missing matter problem in galaxies through a new fundamental gravitational radius
• Gaia EDR3 Parallax Zero-point Offset based on W Ursae Majoris-type Eclipsing Binaries
• The $H_0$ and ${\sigma }_8$ tensions and the scale invariant spectrum
• Quantifying concordance of correlated cosmological data sets
• Heading Gaia to measure atmospheric dynamics in AGB stars
• SDSS DR7 superclusters. Morphology
• Alleviating the need for exponential evolution of JWST galaxies in 10${}^{10}{M}_{\odot }$ haloes at $z>10$ by a modified $\Lambda$CDM power spectrum
• Luminous superclusters: remnants from inflation
• Spectral modeling of type II supernovae. I. Dilution factors
• Cosmological Results from the RAISIN Survey: Using Type Ia Supernovae in the Near Infrared as a Novel Path to Measure the Dark Energy Equation of State
• Cosmological data favor Galileon ghost condensate over $\Lambda$CDM
• Observational constraints on Gauss-Bonnet cosmology
• Higher D or Li: Probes of Physics beyond the Standard Model
• Calibration of semi-analytic models of galaxy formation using Particle Swarm Optimization
• A Strategy to Measure the Dark Energy Equation of State using the HII galaxy Hubble Relation & X-ray AGN Clustering: Preliminary Results
• The impact of an evolving stellar initial mass function on early galaxies and reionisation
• Image Analysis for Cosmology: Results from the GREAT10 Star Challenge
• New Constraints on the Mass of Fermionic Dark Matter from Dwarf Spheroidal Galaxies
• Metastable Dark Energy with Radioactive-like Decay
• A 0.9% Calibration of the Galactic Cepheid luminosity scale based on Gaia DR3 data of open clusters and Cepheids
• Novel null tests for the spatial curvature and homogeneity of the Universe and their machine learning reconstructions
• Dark matter spike around Bumblebee black holes
• Testing the Quasar Hubble Diagram with LISA Standard Sirens
• Probing elastic interactions in the dark sector and the role of $S_8$
• Systematic uncertainty of standard sirens from the viewing angle of binary neutron star inspirals
• Towards hybrid inflation with $n_s=1$ in light of Hubble tension and primordial gravitational waves
• Peculiar motions, accelerated expansion and the cosmological axis
• Big Bang Nucleosynthesis constraints on higher-order modified gravities
• Multidimensionality of the Hubble tension: the roles of ${\Omega }_m$ and ${\omega }_c$
• Stringy-Running-Vacuum-Model Inflation: from primordial Gravitational Waves and stiff Axion Matter to Dynamical Dark Energy
• Dark Energy Survey Year 3 Results: Calibration of Lens Sample Redshift Distributions using Clustering Redshifts with BOSS/eBOSS
• A fresh look into the interacting dark matter scenario
• Galaxy Clusters Discovered via the Thermal Sunyaev-Zel'dovich Effect in the 500-square-degree SPTpol Survey
• Hierarchical Bayesian inference of galaxy redshift distributions from photometric surveys
• Anisotropy of the Universe via the Pantheon supernovae sample revisited
• Comparing inclination dependent analyses of kilonova transients
• A Step in Understanding the $S_8$ Tension
• JAX-COSMO: An End-to-End Differentiable and GPU Accelerated Cosmology Library
• Novel cosmological bounds on thermally-produced axion-like particles
• Schwinger Effect by an $SU(2)$ Gauge Field during Inflation
• Gaussian processes reconstruction of dark energy from observational data
• Artificial intelligence applied to the automatic analysis of absorption spectra. Objective measurement of the fine structure constant
• Quantum Anomalies in String-Inspired Running Vacuum Universe: Inflation and Axion Dark Matter
• The Local Hole in the Galaxy Distribution: New Optical Evidence
• Finsler-Randers Cosmology: dynamical analysis and growth of matter perturbations
• Dynamical system analysis for nonminimal torsion-matter coupled gravity
• The resilience of the Etherington-Hubble relation
• Constraints on Scalar and Tensor spectra from $N_{eff}$
• Determining the Hubble Constant without the Sound Horizon: A $3.6\%$ Constraint on $H_0$ from Galaxy Surveys, CMB Lensing and Supernovae
• Non-parametric reconstruction of the cosmological \textit{jerk} parameter
• Black hole surrounded by the pseudo-isothermal dark matter halo
• Realistic simulations of galaxy formation in f(R) modified gravity
• Gaussian processes reconstruction of modified gravitational wave propagation
• Kinematic constraints beyond $z\simeq 0$ using calibrated GRB correlations
• A new way to test the Cosmological Principle: measuring our peculiar velocity and the large scale anisotropy independently
• Improved constraints on the dark energy equation of state using Gaussian processes
• Improved Treatment of Dark Matter Capture in White Dwarfs
• Equation of state of the running vacuum
• Sterile neutrino self-interactions: $H_0$ tension and short-baseline anomalies
• Rotating black holes in three-dimensional Hořava gravity
• Towards a precision calculation of $N_{\mathrm{eff}}$ in the Standard Model III: Improved estimate of NLO contributions to the collision integral
• Search for GeV-scale Dark Matter Annihilation in the Sun with IceCube DeepCore
• Gravitino thermal production revisited
• Combining pre- and post-recombination new physics to address cosmological tensions: case study with varying electron mass and sign-switching cosmological constant
• Emergent Dark Energy, neutrinos and cosmological tensions
• Determining the Neutrino Lifetime from Cosmology
• Reheating in quintessential inflation via gravitational production of heavy massive particles: A detailed analysis
• Markov chain Monte Carlo analysis of Bianchi VII_h models
• Cosmic shear full nulling: sorting out dynamics, geometry and systematics
• Imprint of DES super-structures on the Cosmic Microwave Background
• Rates and delay times of type Ia supernovae in the Dark Energy Survey
• Stability Analysis in Tachyonic Potential Chameleon cosmology
• Running vacuum in the Universe and the time variation of the fundamental constants of Nature
• The universal rotation curve of low surface brightness galaxies IV: the interrelation between dark and luminous matter
• Cosmic microwave background constraints on secret interactions among sterile neutrinos
• Evolution of gravitational orbits in the expanding universe
• Non-Gaussianity from Axion-Gauge Fields Interactions during Inflation
• TDCOSMO II: 6 new time delays in lensed quasars from high-cadence monitoring at the MPIA 2.2m telescope
• Using Surface Brightness Fluctuations to Study Nearby Satellite Galaxy Systems: Calibration and Methodology
• Looking for Cosmological Alfven Waves in WMAP Data
• Cosmic Microwave Background Trispectrum and Primordial Magnetic Field Limits
• Evidence for extra radiation? Profile likelihood versus Bayesian posterior
• COLA with massive neutrinos
• Higgs-Dilaton Cosmology: An inflation - dark energy connection and forecasts for future galaxy surveys
• Big Bounce cosmology for Palatini $R^2$ gravity with a Nieh-Yan term
• Emergent de Sitter epoch of the Loop Quantum Cosmos: a detailed analysis
• The L-sigma Relation of Local HII Galaxies
• Constraints on active and sterile neutrinos in an interacting dark energy cosmology
• Is there really a Hubble tension?
• Solving the curvature and Hubble parameter inconsistencies through structure formation-induced curvature
• On average properties of inhomogeneous fluids in general relativity III: general fluid cosmologies
• Higgs inflation in Einstein-Cartan gravity
• A new determination of the primordial helium abundance using the analyses of HII region spectra from SDSS
• Simple-graduated dark energy and spatial curvature
• Earth as a transducer for dark-photon dark-matter detection
• Hints for a gravitational constant transition in Tully-Fisher data
• New constraint on the tensor-to-scalar ratio from the $Planck$ and BICEP/Keck Array data using the profile likelihood
• Uncovering a population of gravitational lens galaxies with magnified standard candle SN Zwicky
• White Paper and Roadmap for Quantum Gravity Phenomenology in the Multi-Messenger Era
• Taiji Data Challenge for Exploring Gravitational Wave Universe
• Neural Network Reconstruction of Late-Time Cosmology and Null Tests
• Lensed Type Ia Supernova "Encore" at z=2: The First Instance of Two Multiply-Imaged Supernovae in the Same Host Galaxy
• Directional Variations of Cosmological Parameters from the Planck CMB Data
• Time-varying neutrino mass from a supercooled phase transition: current cosmological constraints and impact on the ${\Omega }_m$-${\sigma }_8$ plane
• Dynamics of Nearby Groups of Galaxies: the role of the cosmological constant
• From inflation to dark energy through a dynamical Lambda: an attempt at alleviating fundamental cosmic puzzles
• Particle Dark Matter - A Theorist's Perspective
• Chain Early Dark Energy: Solving the Hubble Tension and Explaining Today's Dark Energy
• On structure formation from a small-scales-interacting dark sector
• A type of Born-Infeld regular gravity and its cosmological consequences
• Advances in Constraining Intrinsic Alignment Models with Hydrodynamic Simulations
• Pulsation Models for Ultra-Low (Z=0.0004) Metallicity Classical Cepheids
• Baryonic effects on the matter bispectrum
• Optical selection bias and projection effects in stacked galaxy cluster weak lensing
• Reconstructing teleparallel gravity with cosmic structure growth and expansion rate data
• Phantom matter: a challenging solution to the cosmological tensions
• How does the cosmic large-scale structure bias the Hubble diagram?
• Strong gravitational lensing and microlensing of supernovae
• Translation and Rotation Equivariant Normalizing Flow (TRENF) for Optimal Cosmological Analysis
• Probing the interaction between dark energy and dark matter with the parametrized post-Friedmann approach
• The ArDM Liquid Argon Time Projection Chamber at the Canfranc Underground Laboratory: a ton-scale detector for Dark Matter Searches
• Inferring $S_8(z)$ and $\gamma (z)$ with cosmic growth rate measurements using machine learning
• The Atacama Cosmology Telescope: Cosmology from cross-correlations of unWISE galaxies and ACT DR6 CMB lensing
• Supervoids in the WISE-2MASS catalogue imprinting Cold Spots in the Cosmic Microwave Background
• ETHOS -- an effective theory of structure formation: predictions for the high-redshift Universe -- abundance of galaxies and reionization
• Screened fifth forces lower the TRGB-calibrated Hubble constant too
• Constraining the Cosmic Baryon Distribution with Fast Radio Burst Foreground Mapping
• Can we predict $\Lambda$ for the Non-SUSY sector of the Landscape ?
• Testing Dark energy models in the light of ${\sigma }_8$ tension
• The Mira-Titan Universe IV. High Precision Power Spectrum Emulation
• Emerging chromo-natural inflation
• An improved measurement of baryon acoustic oscillations from the correlation function of galaxy clusters at $z\sim 0.3$
• High-redshift JWST Observations and Primordial Non-Gaussianity
• Acceleration of the universe, vacuum metamorphosis, and the large-time asymptotic form of the heat kernel
• Automated galaxy-galaxy strong lens modelling: no lens left behind
• Does the Universe Accelerate Equally in all Directions?
• CONNECT: A neural network based framework for emulating cosmological observables and cosmological parameter inference
• Joint Analysis of near-infrared properties and surface brightness fluctuations of LMC star clusters
• The 2MASS Tully-Fisher relation for flat edge-on galaxies
• Aspects of the Dark Dimension in Cosmology
• Model-independent measurement of cosmic curvature with the latest $H(z)$ and SNe Ia data: A comprehensive investigation
• The Dark Energy Survey Year 3 and eBOSS: constraining galaxy intrinsic alignments across luminosity and colour space
• The First Billion Years of a Warm Dark Matter Universe
• The Dark Energy Spectroscopic Instrument: One-dimensional power spectrum from first Lyman-$\alpha$ forest samples with Fast Fourier Transform
• The Baryonic Tully-Fisher relation revisited
• Modified big bang nucleosynthesis with non-standard neutron sources
• Probing the Dark Flow signal in WMAP 9 yr and PLANCK cosmic microwave background maps
• A simple nonsingular inflationary quintessential model
• Constraints on the Faint End of the Galaxy Stellar Mass Function at z ~ 4-8 from Deep JWST Data
• Current and future constraints on cosmology and modified gravitational wave friction from binary black holes
• Constraints on a Stochastic Background of Primordial Magnetic Fields with WMAP and South Pole Telescope data
• The XXL Survey: XVI. The clustering of X-ray selected galaxy clusters at z~0.3
• Uncertain Times: The Redshift-Time Relation from Cosmology and Stars
• Modelling and testing the equation of state for (Early) dark energy
• Cosmography by orthogonalized logarithmic polynomials
• Reducing the uncertainty on the Hubble constant up to 35\% with an improved statistical analysis: different best-fit likelihoods for Supernovae Ia, Baryon Acoustic Oscillations, Quasars, and Gamma-Ray Bursts
• The Radio Synchrotron Background: Conference Summary and Report
• Assessment of the cosmic distance duality relation using Gaussian Process
• A Bayesian direct method implementation to fit emission line spectra: Application to the primordial He abundance determination
• Large Magellanic Cloud Near-Infrared Synoptic Survey. V. Period-Luminosity Relations of Miras
• Probing nuclear rates with Planck and BICEP2
• On the signature of $z\sim 0.6$ superclusters and voids in the Integrated Sachs-Wolfe effect
• Modified Gravity Constraints from the Full Shape Modeling of Clustering Measurements from DESI 2024
• The Distance to the Coma Cluster from Surface Brightness Fluctuations
• A sub-2% Distance to M31 from Photometrically Homogeneous Near-Infrared Cepheid Period-Luminosity Relations Measured with the Hubble Space Telescope
• Cosmography with Supernova Refsdal through time-delay cluster lensing: independent measurements of the Hubble constant and geometry of the Universe
• Inference of the cosmic rest-frame from supernovae Ia
• Cosmic voids: a novel probe to shed light on our Universe
• The skewed weak lensing likelihood: why biases arise, despite data and theory being sound
• Updated constraints on decaying cold dark matter
• Primordial lepton asymmetries in the precision cosmology era: Current status and future sensitivities from BBN and the CMB
• The impact of spectroscopic incompleteness in direct calibration of redshift distributions for weak lensing surveys
• Out of the Swampland with Multifield Quintessence?
• Testing interacting dark matter and dark energy model with cosmological data
• Bayesian inflationary reconstructions from Planck 2018 data
• Baryon Acoustic Oscillation Theory and Modelling Systematics for the DESI 2024 results
• CP violating scalar Dark Matter
• Big-bounce and future time singularity resolution in Bianchi I: the projective invariant Nieh-Yan case
• Dark Energy Survey Year 3 Results: Exploiting small-scale information with lensing shear ratios
• Late-Time constraints on Interacting Dark Energy: Analysis independent of $H_0$, $r_d$ and $M_B$
• Cross-correlating the gamma-ray sky with catalogs of galaxy clusters
• Quasinormal modes of Schwarzschild black holes in projective invariant Chern-Simons modified gravity
• Optical Identification of Cepheids in 19 Host Galaxies of Type Ia Supernovae and NGC 4258 with the Hubble Space Telescope
• KiDS & Euclid: Cosmological implications of a pseudo angular power spectrum analysis of KiDS-1000 cosmic shear tomography
• Background history and cosmic perturbations for a general system of self-conserved dynamical dark energy and matter
• Isotropic Radio Background from Quark Nugget Dark Matter
• WALLABY Pilot Survey: Public release of HI data for almost 600 galaxies from phase 1 of ASKAP pilot observations
• Return of Harrison-Zeldovich spectrum in light of recent cosmological tensions
• Investigating effects of dark matter on photon orbits and black hole shadows
• Crossing Statistic: Reconstructing the Expansion History of the Universe
• Importance nested sampling with normalising flows
• The Knotted Sky I: Planck constraints on the primordial power spectrum
• Interacting dark energy: clarifying the cosmological implications and viability conditions
• Consistency of Planck, ACT and SPT constraints on magnetically assisted recombination and forecasts for future experiments
• Cosmology with matter diffusion
• Quantifying the evidence for the current speed-up of the Universe with low and intermediate-redshift data. A more model-independent approach
• The Hubble constant from strongly lensed supernovae with standardizable magnifications
• Game of cones: A nulling strategy for modelling lensing convergence in cones with large deviation theory
• New Interaction between Dark Energy and Dark Matter Changes Sign during Cosmological Evolution
• Evaluating bulk flow estimators for CosmicFlows-4 measurements
• The halo mass function and filaments in full cosmological simulations with fuzzy dark matter
• Redshift-space effects in voids and their impact on cosmological tests. Part I: the void size function
• Integral $F(R)$ Gravity and Saddle Point Condition as a Remedy for the $H_0$-tension
• A model-based approach to the spatial and spectral calibration of NIRSpec onboard JWST
• A Bayesian comparison between $\Lambda$CDM and phenomenologically emergent dark energy models
• Wide-area tomography of CMB lensing and the growth of cosmological density fluctuations
• Blinding multi-probe cosmological experiments
• Infrared Surface Brightness Fluctuation Distances for MASSIVE and Type Ia Supernova Host Galaxies
• Toward a Better Understanding of Cosmic Chronometers: Stellar Population Properties of Passive Galaxies at Intermediate Redshift
• The Baryonic Tully Fisher Relation
• Reconstruction of the Dark Energy equation of state from latest data: the impact of theoretical priors
• LISA Definition Study Report
• The SRG/eROSITA All-Sky Survey: Dark Energy Survey Year 3 Weak Gravitational Lensing by eRASS1 selected Galaxy Clusters
• Dark energy, the colored anti-de Sitter vacuum, and LHC phenomenology
• Astrophysical Distance Scale The JAGB Method: I. Calibration and a First Application
• Thermodynamical aspects of running vacuum models
• Tightening the reins on non-minimal dark sector physics: Interacting Dark Energy with dynamical and non-dynamical equation of state
• Constraints on Pre-Recombination Early Dark Energy from SPT-3G Public Data
• One spectrum to cure them all: Signature from early Universe solves major anomalies and tensions in cosmology
• Machine Learning the Cosmic Curvature in a Model-independent Way
• Flavor versus mass eigenstates in neutrino asymmetries: implications for cosmology
• Evidence against a supervoid causing the CMB Cold Spot
• Cosmic troublemakers: the Cold Spot, the Eridanus Supervoid, and the Great Walls
• Black holes surrounded by Einstein clusters as models of dark matter fluid
• QUBIC I: Overview and ScienceProgram
• Reconstruction of broad features in the primordial spectrum and inflaton potential from Planck
• A Giant Arc on the Sky
• Starobinsky-type Inflation in Dynamical Supergravity Breaking Scenarios
• New constraints on ${\sigma }_8$ from a joint analysis of stacked gravitational lensing and clustering of galaxy clusters
• Differential cosmic expansion and the Hubble flow anisotropy
• Early dark energy in $k$-essence
• Composite Dark Energy and the Cosmological Tensions
• Rapidly growing primordial black holes as seeds of the massive high-redshift JWST Galaxies
• Hints of dark matter-neutrino interactions in Lyman-$\alpha$ data
• What it takes to solve the Hubble tension through modifications of cosmological recombination
• Joint halo mass function for modified gravity and massive neutrinos I: simulations and cosmological forecasts
• Late time cosmology with LISA: probing the cosmic expansion with massive black hole binary mergers as standard sirens
• Shock cooling of a red-supergiant supernova at redshift 3 in lensed images
• Towards a model-independent reconstruction approach for late-time Hubble data
• Chemical abundances in 7 metal-poor HII regions and a determination of the primordial helium abundance
• Discovery of a massive supercluster system at $z\sim 0.47$
• Structure formation simulations with momentum exchange: alleviating tensions between high-redshift and low-redshift cosmological probes
• $H_0$ tension and the String Swampland
• Neutrino Cosmology after WMAP and LHC7
• Falsifying cosmological models based on a non-linear electrodynamics
• The part and the whole: voids, supervoids, and their ISW imprint
• Testing chirality of primordial gravitational waves with Planck and future CMB data: no hope from angular power spectra
• Darwin Meets Einstein: LISA Data Analysis Using Genetic Algorithms
• Exploring the evidence for a large local void with supernovae Ia data
• Missing Power vs low-l Alignments in the Cosmic Microwave Background: No Correlation in the Standard Cosmological Model
• Nonparametric reconstruction of the cosmic expansion with local regression smoothing and simulation extrapolation
• Quintessential inflation: A tale of emergent and broken symmetries
• Clues on void evolution III: Structure and dynamics in void shells
• An Infrared Census of DUST in Nearby Galaxies with Spitzer (DUSTiNGS). IV. Discovery of High-Redshift AGB Analogs
• Dark matter component decaying after recombination: Sensitivity to BAO and RSD probes
• Cosmic shear with small scales: DES-Y3, KiDS-1000 and HSC-DR1
• Model-independent cosmological constraints from growth and expansion
• How to relax the cosmological neutrino mass bound
• An updated metal-dependent theoretical scenario for Classical Cepheids
• Lensing of fast radio bursts: future constraints on primordial black hole density with an extended mass function and a new probe of exotic compact fermion and boson stars
• Model-independent constraints on cosmic curvature: implication from updated Hubble diagram of high-redshift standard candles
• The fifth data release of the Kilo Degree Survey: Multi-epoch optical/NIR imaging covering wide and legacy-calibration fields
• Testing Gravity on Cosmic Scales: A Case Study of Jordan-Brans-Dicke Theory
• Inflation, the Hubble Tension and Early Dark Energy: an alternative overview
• $k$-evolution: a relativistic N-body code for clustering dark energy
• Constraining the dark energy equation of state using Bayes theorem and the Kullback-Leibler divergence
• Is there a need and another way to measure the Cosmic Microwave Background temperature more accurately?
• k-cut Cosmic Shear: Tunable Power Spectrum Sensitivity to Test Gravity
• Alleviating both $H_0$ and ${\sigma }_8$ tensions in Tsallis cosmology
• Black Hole Shadows in Verlinde's Emergent Gravity
• KiDS-1000: Cosmology with improved cosmic shear measurements
• Is the dark energy equation of state parameter singular?
• Constructing a cosmological model-independent Hubble diagram of type Ia supernovae with cosmic chronometers
• Using Ultra Long Period Cepheids to Extend the Cosmic Distance Ladder to 100 Mpc and Beyond
• Metastable dark energy models in light of Planck 2018: Alleviating the $H_0$ tension
• A light particle solution to the cosmic lithium problem
• Optimal 1D Ly$\alpha$ Forest Power Spectrum Estimation -- II. KODIAQ, SQUAD & XQ-100
• Unbiased Estimate of Dark Energy Density from Type Ia Supernova Data
• Early Structure Formation from Cosmic String Loops in Light of Early JWST Observations
• Dark Energy Survey: A 2.1% measurement of the angular Baryonic Acoustic Oscillation scale at redshift $z_{\mathrm{eff}}$=0.85 from the final dataset
• New accelerating solutions in late-time cosmology
• Cepheid Metallicity in the Leavitt Law (C-MetaLL) survey: I. HARPS-N@TNG spectroscopy of 47 Classical Cepheid and 1 BL Her variables
• Hot New Early Dark Energy: Towards a Unified Dark Sector of Neutrinos, Dark Energy and Dark Matter
• Baryon Asymmetry from the Generalized Uncertainty Principle
• Baryogenesis in Nonminimally Coupled $f(R)$ Theories
• Cosmology beyond BAO from the 3D distribution of the Lyman-$\alpha$ forest
• Cannibal Dark Matter and Large Scale Structure
• The Near-Infrared Tip of the Red Giant Branch. II. An Absolute Calibration in the Large Magellanic Cloud
• Reconstruction of the neutrino mass as a function of redshift
• Model-independent cosmic acceleration and type Ia supernovae intrinsic luminosity redshift dependence
• Dark matter in ghost-free bigravity theory: From a galaxy scale to the universe
• The Mira Distance to M101 and a 4% Measurement of H0
• Multi-Epoch HST Observations of IZw18: Characterization of Variable Stars at Ultra-Low Metallicities
• Massive neutrino self-interactions and inflation
• Calibrating Gamma-Ray Bursts by Using a Gaussian Process with Type Ia Supernovae
• General framework for cosmological dark matter bounds using $N$-body simulations
• A simultaneous solution to the Hubble tension and observed bulk flow within 250 $h^{-1}$ Mpc
• Determining the Hubble Constant without the Sound Horizon: Perspectives with Future Galaxy Surveys
• Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions
• A large disparity in cosmic reference frames determined from the sky distributions of radio sources and the microwave background radiation
• Testing General Relativity with Growth rate measurement from Sloan Digital Sky Survey III Baryon Oscillations Spectroscopic Survey galaxies
• Cosmological inference from the EFTofLSS: the eBOSS QSO full-shape analysis
• Solving the Hubble tension without spoiling Big Bang Nucleosynthesis
• Metric $f(R)$ gravity with dynamical dark energy as a scenario for the Hubble tension
• The integrated 3-point correlation function of cosmic shear
• Constraints on compact dark matter with fast radio burst observations
• Reconnaissance with JWST of the J-region Asymptotic Giant Branch in Distance Ladder Galaxies: From Irregular Luminosity Functions to Approximation of the Hubble Constant
• Cosmological distance indicators
• Cosmological perturbations in the Tsallis holographic dark energy scenarios
• Ruling Out New Physics at Low Redshift as a solution to the $H_0$ Tension
• Testing dynamical vacuum models with CMB power spectrum from Planck
• Cosmology with clustering anisotropies: disentangling dynamic and geometric distortions in galaxy redshift surveys
• A persistent excess of galaxy-galaxy strong lensing observed in galaxy clusters
• On the faint-end of the galaxy luminosity function in the Epoch of Reionization: updated constraints from the HST Frontier Fields
• BAO signatures in the 2-point angular correlations and the Hubble tension
• Target Selection for the DESI Peculiar Velocity Survey
• A bias in cosmic shear from galaxy selection: results from ray-tracing simulations
• Higgs inflation and teleparallel gravity
• Unbiased clustering estimates with the DESI fibre assignment
• The GALAH Survey: A new constraint on cosmological lithium and Galactic lithium evolution from warm dwarf stars
• The cosmic radio dipole: Bayesian estimators on new and old radio surveys
• Sloan Great Wall as a complex of superclusters with collapsing cores
• Cold or Warm? Constraining Dark Matter with Primeval Galaxies and Cosmic Reionization after Planck
• Carbon stars as standard candles: I. The luminosity function of carbon stars in the Magellanic Clouds
• The X-ray Cluster Dipole
• Cosmological gravitational particle production of massive spin-2 particles
• Cosmic microwave background bispectrum of tensor passive modes induced from primordial magnetic fields
• Is Cosmic Parity Violation Responsible for the Anomalies in the WMAP Data?
• Spectroscopic failures in photometric redshift calibration: cosmological biases and survey requirements
• Bayesian forward modelling of cosmic shear data
• Projected Cosmological Constraints from Strongly Lensed Supernovae with the Roman Space Telescope
• Exploring neutrino mass and mass hierarchy in interacting dark energy models
• Accelerations of Water Masers in NGC4258
• An Infrared Census Of Dust In Nearby Galaxies With Spitzer (DUSTiNGS): V. The Period-luminosity Relation For Dusty Metal-Poor AGB Stars
• Precise cosmological parameter estimation using CosmoRec
• Noether Symmetries and Quantum Cosmology in Extended Teleparallel Gravity
• Using the Tip of the Red Giant Branch as a Distance Indicator in the Near Infrared
• The Infrared Surface Brightness Fluctuation Distances to the Hydra and Coma Clusters
• Resolving conclusions about the early Universe requires accurate nuclear measurements
• Dark Matter microphysics and 21 cm observations
• Multiple Images and Flux Ratio Anomaly of Fuzzy Gravitational Lenses
• Self-Interacting Neutrinos in Light of Large-Scale Structure Data
• Near-infrared Mira Period-Luminosity Relations in M33
• Are $H_0$ and ${\sigma }_8$ tensions generic to present cosmological data?
• Constraining the observer angle of the kilonova AT2017gfo associated with GW170817: Implications for the Hubble constant
• The contribution of discrete sources to the sky temperature at 144 MHz
• Redshift and lateshift from homogeneous and isotropic modified dispersion relations
• Unusual A2142 supercluster with a collapsing core: distribution of light and mass
• Early and late time cosmology: the $f(R)$ gravity perspective
• The Isotropic Radio Background and Annihilating Dark Matter
• Parque Astronómico de Atacama: An ideal site for millimeter, submillimeter, and mid-infrared astronomy
• Evolution of the fine-structure constant in runaway dilaton models
• Revisiting a non-parametric reconstruction of the deceleration parameter from combined background and the growth rate data
• Planck-scale-modified dispersion relations in homogeneous and isotropic spacetimes
• A Consistent Theory of Decaying Dark Matter Connecting IceCube to the Sesame Street
• Transition Redshift: New constraints from parametric and nonparametric methods
• Large Magellanic Cloud Near-Infrared Synoptic Survey. III. A Statistical Study of Non-Linearity in the Leavitt Laws
• Stochastic optimization methods for extracting cosmological parameters from CMBR power spectra
• 6Li/7Li estimates for metal-poor stars
• The integrated Sachs-Wolfe effect in the AvERA cosmology
• Modelling Long-Period Variables -- II. Fundamental mode pulsation in the nonlinear regime
• New H-band Galaxy Number Counts: A Large Local Hole in the Galaxy Distribution?
• Dynamics in Varying vacuum Finsler-Randers Cosmology
• Simple inflationary quintessential model II: Power law potentials
• Model selection applied to reconstructions of the Dark Energy
• Testing dark matter interactions with CMB spectral distortions
• Mathematical foundations for field theories on Finsler spacetimes
• Snowmass2021 CMB-HD White Paper
• Phenomenological emergent dark energy in the light of DESI Data Release 1
• Optical appearance of black holes surrounded by a dark matter halo
• Constraining the dark energy models using Baryon Acoustic Oscillations: An approach independent of $H_0\cdot r_d$
• Probing the sign-changeable interaction between dark energy and dark matter with current observations
• Cosmic Explorer: A Submission to the NSF MPSAC ngGW Subcommittee
• Weak Lensing Tomographic Redshift Distribution Inference for the Hyper Suprime-Cam Subaru Strategic Program three-year shape catalogue
• Principal reconstructed modes of dark energy and gravity
• Generalised model-independent characterisation of strong gravitational lenses IV: formalism-intrinsic degeneracies
• Spectral modeling of type II supernovae II. A machine learning approach to quantitative spectroscopic analysis
• Six Puzzles for LCDM Cosmology
• Slow-rolling scalar dynamics and as solution for the Hubble tension
• Constraints on dark matter to dark radiation conversion in the late universe with DES-Y1 and external data
• Bianchi I Model: An Alternative Way To Model The Presentday Universe
• Cosmological-model-independent determination of Hubble constant from fast radio bursts and Hubble parameter measurements
• Running vacuum in QFT in FLRW spacetime: The dynamics of ${\rho }_{\mathrm{vac}}(H)$ from the quantized matter fields
• Constraints on warm dark matter from UV luminosity functions of high-z galaxies with Bayesian model comparison
• Nonlinear Evolution of Cosmic Magnetic Fields and Cosmic Microwave Background Anisotropies
• Minimal dark energy: key to sterile neutrino and Hubble constant tensions?
• Measuring Infrared Surface Brightness Fluctuation Distances with HST WFC3: Calibration and Advice
• The Near-Infrared Tip of the Red Giant Branch. I. A Calibration in the Isolated Dwarf Galaxy IC 1613
• Mass Determination of Groups of Galaxies: Effects of the Cosmological Constant
• The future search for low-frequency axions and new physics with the FLASH resonant cavity experiment at Frascati National Laboratories
• Cosmological constraints on ${\Lambda }_{\mathrm{s}}$CDM scenario in a type II minimally modified gravity
• KiDS-Legacy calibration: unifying shear and redshift calibration with the SKiLLS multi-band image simulations
• The DES view of the Eridanus supervoid and the CMB Cold Spot
• Isotropy of low redshift type Ia Supernovae: A Bayesian analysis
• Quantum Gravity Corrections and Entropy at the Planck time
• Screened Fifth Forces Mediated by Dark Matter-Baryon Interactions: Theory and Astrophysical Probes
• Full-shape BOSS constraints on dark matter interacting with dark radiation and lifting the $S_8$ tension
• Dwarf galaxies imply dark matter is heavier than $2.2\times 10^{-21}\mathbf{eV}$
• Axionic dark energy and a composite QCD axion
• Updated Constraints on Primordial Black Hole Evaporation
• Thermalizing sterile neutrino dark matter
• Back-Reaction of Super-Hubble Cosmological Perturbations Beyond Perturbation Theory
• Revisiting Metastable Dark Energy and Tensions in the Estimation of Cosmological Parameters
• JWST Photometric Time-Delay and Magnification Measurements for the Triply-Imaged Type Ia "Supernova H0pe" at z = 1.78
• Cosmological perturbations in an effective and genuinely phantom dark energy Universe
• A Fully Self-Consistent Cosmological Simulation Pipeline for Interacting Dark Energy Models
• Bianchi I meets the Hubble diagram
• JWST high-z galaxy constraints on warm and cold dark matter models
• Probing the properties of relic neutrinos using the cosmic microwave background, the Hubble Space Telescope and galaxy clusters
• The Globular Cluster Systems in the Coma Ellipticals. I: The Luminosity Function in NGC 4874, and Implications for Hubble's Constant
• Can small-scale baryon inhomogeneities resolve the Hubble tension? An investigation with ACT DR4
• Varying fundamental constants principal component analysis: additional hints about the Hubble tension
• CMB anisotropies in the presence of a stochastic magnetic field
• Evidence for a high-z ISW signal from supervoids in the distribution of eBOSS quasars
• Impact of local structure on the cosmic radio dipole
• Small-scale clumping at recombination and the Hubble tension
• The Hubble Tension, The $M$ Crisis of Late Time $H(z)$ Deformation Models and the Reconstruction of Quintessence Lagrangians
• Ionized gas kinematics and chemical abundances of low-mass star-forming galaxies at $z\sim 3$
• Relativistic kinetic gases as direct sources of gravity
• Towards a reliable calculation of relic radiation from primordial gravitational waves
• Hubble tension vs two flows
• Do supernovae indicate an accelerating universe?
• Machine learning constraints on deviations from general relativity from the large scale structure of the Universe
• On Cepheid Distance Scale Bias due to Stellar Companions and Cluster Populations
• The Fine Structure Constant and the CMB Damping Scale
• Model-independent Distance Calibration and Curvature Measurement using Quasars and Cosmic Chronometers
• The two-mode puzzle: Confronting self-interacting neutrinos with the full shape of the galaxy power spectrum
• The Tully-Fisher Relation for 25,000 SDSS Galaxies as Function of Environment
• Sterile Neutrino Dark Matter in Left-Right Theories
• Multi-field dark energy: cosmic acceleration on a steep potential
• Observational constraints on early dark energy
• FLIMFLAM DR1: The First Constraints on the Cosmic Baryon Distribution from 8 FRB sightlines
• Unification of Dark Matter - Dark Energy in Generalized Galileon Theories
• Forecasts on the speed of gravitational waves at high $z$
• Testing the standard model of cosmology with the SKA: the cosmic radio dipole
• First measurement of the Hubble parameter from bright binary black hole GW190521
• Generalized Uncertainty Principle Impact on Nonextensive Black Hole Thermodynamics
• Machine Learning improved fits of the sound horizon at the baryon drag epoch
• Dynamical dark energy confronted with multiple CMB missions
• Stepped Partially Acoustic Dark Matter, Large Scale Structure, and the Hubble Tension
• Gravitational ringing and superradiant instabilities of the Kerr-like black holes in a dark matter halo
• Hubble tension bounds the GUP and EUP parameters
• The XXL survey: XLVI. Forward cosmological analysis of the C1 cluster sample
• Extreme quasars at high redshift
• An Effective Sign Switching Dark Energy: Lotka-Volterra Model of Two Interacting Fluids
• Tensions with the flat $\mathbf{\Lambda }$CDM model from high-redshift cosmography
• Dynamical Supergravity Breaking via the Super-Higgs Effect Revisited
• Joint analysis of DES Year 3 data and CMB lensing from SPT and Planck II: Cross-correlation measurements and cosmological constraints
• Tsallis and Kaniadakis statistics from the viewpoint of entropic gravity formalism
• CosmicNet II: Emulating extended cosmologies with efficient and accurate neural networks
• Further evidence that galaxy age drives observed type Ia supernova luminosity differences
• Measuring the distance-redshift relation with the baryon acoustic oscillations of galaxy clusters
• Cold New Early Dark Energy pulls the trigger on the $H_0$ and $S_8$ tensions: a simultaneous solution to both tensions without new ingredients
• Redshift-space effects in voids and their impact on cosmological tests. Part II: the void-galaxy cross-correlation function
• The deceleration parameter in `tilted' Friedmann universes
• Impact of $H_0$ priors on $f(T)$ late time cosmology
• Astrophysical Distance Scale II. Application of the JAGB Method: A Nearby Galaxy Sample
• Landau damping for gravitational waves in parity-violating theories
• Measuring the sound horizon and absolute magnitude of SNIa by maximizing the consistency between low-redshift data sets
• Reconstructing Positions and Peculiar Velocities of Galaxy Clusters within 20000 km/sec. I: The Cluster 3D Dipole
• Science with the Murchison Widefield Array: Phase I Results and Phase II Opportunities
• CosmoPower-JAX: high-dimensional Bayesian inference with differentiable cosmological emulators
• Toward a concordance teleparallel Cosmology I: Background Dynamics
• Probing Cosmic Inflation with the LiteBIRD Cosmic Microwave Background Polarization Survey
• Constraints on photoionization feedback from number counts of ultra-faint high-redshift galaxies in the Frontier Fields
• Constraints on $\gamma$-CDM interactions matching the Planck data precision
• Constraining the curvature density parameter in cosmology
• Modified gravity and massive neutrinos: constraints from the full shape analysis of BOSS galaxies and forecasts for Stage IV surveys
• Confronting interacting dark radiation scenarios with cosmological data
• Exploration of interacting dynamical dark energy model with interaction term including the equation-of-state parameter: alleviation of the $H_0$ tension
• Model marginalized constraints on neutrino properties from cosmology
• A Dark Matter Trigger for Early Dark Energy Coincidence
• Machine Learning for Observational Cosmology
• A Model for Dark Energy decay
• A Universe Without Dark Energy: Cosmic Acceleration from Dark Matter-Baryon Interactions
• Euclid: Forecasts from the void-lensing cross-correlation
• Time variation of proton-electron mass ratio and fine structure constant with runaway dilaton
• BAO from angular clustering: optimization and mitigation of theoretical systematics
• Hubble tension in lepton asymmetric cosmology with an extra radiation
• Testing Predictions of the Quantum Landscape Multiverse 2: The Exponential Inflationary Potential
• Cosmological singularities in Born-Infeld determinantal gravity
• MIGHTEE: Deep 1.4 GHz Source Counts and the Sky Temperature Contribution of Star Forming Galaxies and Active Galactic Nuclei
• The Local Hole: a galaxy under-density covering 90% of sky to ~200 Mpc
• Fourier-series expansion of the dark-energy equation of state
• Inflation in non-minimal matter-curvature coupling theories
• Observational Constraints on Axion(s) Dark Energy with a Cosmological Constant
• ECoPANN: A Framework for Estimating Cosmological Parameters using Artificial Neural Networks
• The baryonic mass-velocity relation; clues to feedback processes during structure formation and the cosmic baryon inventory
• An updated measurement of the Hubble constant from near-infrared observations of Type Ia supernovae
• $H_0$ Ex Machina: Vacuum Metamorphosis and Beyond $H_0$
• Probing Diffuse Gas with Fast Radio Bursts
• Mild Non-Gaussianities under Perturbative Control from Rapid-Turn Inflation Models
• Gamma-ray burst supernovae as standardizable candles
• Standardizing reverberation-measured C IV time-lag quasars, and using them with standardized Mg II quasars to constrain cosmological parameters
• Finding the brightest cosmic beacons in the Southern Hemisphere
• Fuzzy Dark Matter as a Solution to Reconcile the Stellar Mass Density of High-z Massive Galaxies and Reionization History
• Relieving tensions related to the lensing of CMB temperature power spectra
• Measuring the reionization optical depth without large-scale CMB polarization
• Spacetime and dark matter from spontaneous breaking of Lorentz symmetry
• Acoustic signatures in the Cosmic Microwave Background bispectrum from primordial magnetic fields
• The Copernican principle in light of the latest cosmological data
• $S_8$ Tension in the Context of Dark Matter-Baryon Scattering
• 2MASS Constraints on the Local Large-Scale Structure: A Challenge to LCDM?
• Tsallis cosmology and its applications in dark matter physics with focus on IceCube high-energy neutrino data
• Anti-de Sitter $\to$ de Sitter transition driven by Casimir forces and mitigating tensions in cosmological parameters
• Influence of the Bounds of the Hyperparameters on the Reconstruction of Hubble Constant with Gaussian Process
• Exploiting the Einstein Telescope to solve the Hubble tension
• Gravitational Lensing of Schwarzschild and Charged Black Holes Immersed in Perfect Fluid Dark Matter Halo
• $5\sigma$ tension between Planck cosmic microwave background and eBOSS Lyman-alpha forest and constraints on physics beyond $\Lambda$CDM
• Hints of dark photon dark matter from observations and hydrodynamical simulations of the low-redshift Lyman-$\alpha$ forest
• Simulating the LOcal Web (SLOW): I. Anomalies in the local density field
• Cosmology and Astrophysics with Standard Sirens and Galaxy Catalogs in View of Future Gravitational Wave Observations
• Primordial Magnetic Helicity Constraints from WMAP Nine-Year Data
• Cosmographic view on the $H_0$ and ${\sigma }_8$ tensions
• Generalized LTB model with Inhomogeneous Isotropic Dark Energy: Observational Constraints
• Cosmological Constraints on Higgs-Dilaton Inflation
• Neural network reconstructions for the Hubble parameter, growth rate and distance modulus
• The IA Guide: A Breakdown of Intrinsic Alignment Formalisms
• Testing cosmic anisotropy with Pantheon sample and quasars at high redshifts
• Dark radiation and small-scale structure problems with decaying particles
• Testing Predictions of the Quantum Landscape Multiverse 1: The Starobinsky Inflationary Potential
• Searching for primordial localized features with CMB and LSS spectra
• Cosmography with next-generation gravitational wave detectors
• Dipole Cosmology: The Copernican Paradigm Beyond FLRW
• Cosmic microwave background bispectrum of vector modes induced from primordial magnetic fields
• An effective description of Laniakea: impact on cosmology and the local determination of the Hubble constant
• Capse.jl: efficient and auto-differentiable CMB power spectra emulation
• Origin of Delta N_eff as a Result of an Interaction between Dark Radiation and Dark Matter
• Cosmic voids detection without density measurements
• The Megamaser Cosmology Project. VII. Investigating disk physics using spectral monitoring observations
• Model independent bounds on Type Ia supernova absolute peak magnitude
• Stellar prospects for FRB gravitational lensing
• Multiple transitions in vacuum dark energy and $H_0$ tension
• Theoretical systematics in testing the Cosmological Principle with the kinematic quasar dipole
• Cosmic backgrounds due to the formation of the first generation of supermassive black holes
• Probing gravity and growth of structure with gravitational waves and galaxies' peculiar velocity
• Metastable dark energy
• Direct and indirect probes of Goldstone dark matter
• An exploration of an early gravity transition in light of cosmological tensions
• Mixed Non-Gaussianity from Axion-Gauge Field Dynamics
• Cosmology from weak lensing peaks and minima with Subaru Hyper Suprime-Cam survey first-year data
• Cosmological parameter estimation using Particle Swarm Optimization (PSO)
• Constant roll inflation in multifield models
• Inflation via Gravitino Condensation in Dynamically Broken Supergravity
• Microlensing of the X-ray, UV and optical emission regions of quasars: Simulations of the time-scales and amplitude variations of microlensing events
• Observational constraints on Tsallis modified gravity
• First Constraints on Compact Dark Matter from Fast Radio Burst Microstructure
• TDCOSMO X. Automated Modeling of 9 Strongly Lensed Quasars and Comparison Between Lens Modeling Software
• A grounded perspective on New Early Dark Energy using ACT, SPT, and BICEP/Keck
• Dark Energy as a Critical Phenomenon: a Resolution for Hubble Tension
• Why the Universe Started from a Low Entropy State
• Cosmological Avatars of the Landscape II: CMB and LSS Signatures
• Evolution of Dark Energy Perturbations in Scalar-Tensor Cosmologies
• Timescape cosmology with radiation fluid
• Exploring interacting holographic dark energy in a perturbed universe with parameterized post-Friedmann approach
• Evolution of the cluster optical galaxy luminosity function in the CFHTLS : breaking the degeneracy between mass and redshift
• Large-Scale Gravitational Lens Modeling with Bayesian Neural Networks for Accurate and Precise Inference of the Hubble Constant
• Quintessential $\alpha$-attractor inflation: forecasts for Stage IV galaxy surveys
• Equivalence of non-minimally coupled cosmologies by Noether symmetries
• Properties of M31. II: A Cepheid disk sample derived from the first year of PS1 PAndromeda data
• Constraints on Tsallis Cosmology from Big Bang Nucleosynthesis and the Relic Abundance of Cold Dark Matter Particles
• Torsional birefringence in metric-affine Chern-Simons gravity: gravitational waves in late-time cosmology
• Cosmicflows-3: Cold Spot Repeller?
• Transition dynamics in the ${\Lambda }_{\mathrm{s}}$CDM model: Implications for bound cosmic structures
• Cosmicflows-4: The Baryonic Tully-Fisher Relation Providing ~10,000 Distances
• A model-independent reconstruction of dark sector interactions
• Constraints on Yukawa gravity parameters from observations of bright stars
• Cosmology of $f(R,\square R)$ gravity
• From infinite to infinitesimal: Using the Universe as a dataset to probe Casimir corrections to the vacuum energy from fields inhabiting the dark dimension
• Baryon acoustic oscillations reconstruction using convolutional neural networks
• Theoretical Aspects of Quintom Models
• Stasis in an Expanding Universe: A Recipe for Stable Mixed-Component Cosmological Eras
• Evidence for cosmic acceleration with next-generation surveys: A model-independent approach
• Gravitationally induced particle production in scalar-tensor $f(R,T)$ gravity
• Tomographic Alcock-Paczynski Test with Redshift-Space Correlation Function: Evidence for the Dark Energy Equation of State Parameter w>-1
• The Gravitational Lensing Signatures of BOSS Voids in the Cosmic Microwave Background
• Non-parametric reconstruction of interaction in the cosmic dark sector
• KiDS-1000 cosmology: Combined second- and third-order shear statistics
• Profiling Cold New Early Dark Energy
• The Second Radio Synchrotron Background Workshop: Conference Summary and Report
• D-Foam Phenomenology: Dark Energy, the Velocity of Light and a Possible D-Void
• A new life for sterile neutrino dark matter after the pandemic
• ZFIRE: The Evolution of the Stellar Mass Tully-Fisher Relation to Redshift 2.0 < Z < 2.5 with MOSFIRE
• Bounding the mass of ultralight bosonic Dark Matter particles with the motion of the S2 star around Sgr A*
• Early Dark Energy in Type IIB String Theory
• Inflation and Acceleration of the Universe by Nonlinear Magnetic Monopole Fields
• Current and Future Constraints on Primordial Magnetic Fields
• Cross-correlation of galaxies and galaxy clusters in the Sloan Digital Sky Survey and the importance of non-Poissonian shot noise
• Exploring the Hubble tension with a late time Modified Gravity scenario
• Deciphering the Archaeological Record: Cosmological Imprints of Non-Minimal Dark Sectors
• Dark energy and Dark matter interaction in light of the second law of thermodynamics
• J-PAS: Forecasts for dark matter - dark energy elastic couplings
• GroundBIRD : A CMB polarization experiment with MKID arrays
• Scale-invariant alternatives to general relativity. III. The inflation--dark-energy connection
• Observational constraints on bimetric gravity
• Euclid: constraining dark energy coupled to electromagnetism using astrophysical and laboratory data
• The weak, the strong and the ugly -- A comparative analysis of interacting stepped dark radiation
• The Araucaria Project. Distances to Nine Galaxies Based on a Statistical Analysis of their Carbon Stars (JAGB Method)
• Constraining cosmological extra dimensions with gravitational wave standard sirens: from theory to current and future multi-messenger observations
• The TRGB-SBF Project. III. Refining the HST Surface Brightness Fluctuation Distance Scale Calibration with JWST
• Calibration of the Fundamental Plane Zero-point in the Leo-I Group and an Estimate of the Hubble Constant
• Evidence for galaxy dynamics tracing background cosmology below the de Sitter scale of acceleration
• Recent advances in cosmological singularities
• Quasars as high-redshift standard candles
• The sparkling Universe: the coherent motions of cosmic voids
• The multipole expansion of the local expansion rate
• Using the cosmological recombination radiation to probe early dark energy and fundamental constant variations
• The Ellipsoidal Universe in the Planck Satellite Era
• Connecting Infrared Surface Brightness Fluctuation Distances to Type Ia Supernova Hosts: Testing the Top Rung of the Distance Ladder
• Dark energy by natural evolution: Constraining dark energy using Approximate Bayesian Computation
• Quasar UV/X-ray relation luminosity distances are shorter than reverberation-measured radius-luminosity relation luminosity distances
• No rungs attached: A distance-ladder free determination of the Hubble constant through type II supernova spectral modelling
• Why Cosmic Voids Matter: Nonlinear Structure & Linear Dynamics
• The perspective of voids on rising cosmology tensions
• Cosmic Birefringence: Cross-Spectra and Cross-Bispectra with CMB Anisotropies
• First observational constraints on tensor non-Gaussianity sourced by primordial magnetic fields from cosmic microwave background
• Likelihood-free Cosmological Constraints with Artificial Neural Networks: An Application on Hubble Parameters and SNe Ia
• Extended phase-space analysis of the Horava-Lifshitz cosmology
• Teleparallel axions and cosmology
• Euclid preparation. XXXII. Evaluating the weak lensing cluster mass biases using the Three Hundred Project hydrodynamical simulations
• Constraining cosmology with shear peak statistics: tomographic analysis
• Discordances in cosmology and the violation of slow-roll inflationary dynamics
• Investigation of Redshift- and Duration-Dependent Clustering of Gamma-ray Bursts
• Revisiting the Hubble constant, spatial curvature and cosmography with time-delay and cosmic chronometer observations
• Euclid: Forecast constraints on consistency tests of the $\Lambda$CDM model
• Redshift-dependent galaxy formation efficiency at $z=5-13$ in the FirstLight simulations
• Reconstruction of the primordial power spectrum from CMB data
• A comparison of template vs. direct model fitting for redshift-space distortions in BOSS
• Effect of evolutionary physical constants on type-1a supernova luminosity
• KiDS-SBI: Simulation-based inference analysis of KiDS-1000 cosmic shear
• Axiverse cosmology and the energy scale of inflation
• A Cosmological Underdensity Does Not Solve the Hubble Tension
• Gaussian Processes Reconstruction of the Dark Energy Potential
• ${\Lambda }_{\mathrm{s}}$CDM cosmology: Alleviating major cosmological tensions by predicting standard neutrino properties
• Non-fiducial cosmological test from geometrical and dynamical distortions around voids
• Noncommutative minisuperspace, gravity-driven acceleration and kinetic inflation
• CosmicNet I: Physics-driven implementation of neural networks within Boltzmann-Einstein solvers
• Big-Bounce cosmology in the presence of Immirzi field
• Dynamics of the diffusive DM-DE interaction--dynamical system approach
• Revisiting the distance duality relation using a non-parametric regression method
• Phantom scalar-tensor models and cosmological tensions
• Quantifying the tension between cosmological and terrestrial constraints on neutrino masses
• Constraining neutrino properties with a Euclid-like galaxy cluster survey
• Hot thermal universe endowed with massive dark vector fields and the Hubble tension
• Anisotropic k-essence cosmologies
• Dark energy and matter interacting scenario to relieve $H_0$ and $S_8$ tensions
• Fundamental constants and cosmic vacuum: the micro and macro connection
• Observational cosmology with Artificial Neural Networks
• $\alpha$ attractors in Quintessential Inflation motivated by Supergravity
• The Impact of Baryons on Cosmological Inference from Weak Lensing Statistics
• Measurement on the cosmic curvature using the Gaussian process method
• Constraining cosmological parameters with the clustering properties of galaxy clusters in optical and X-ray bands
• Promise of Future Searches for Cosmic Topology
• Cosmological parameter estimation with Genetic Algorithms
• Neural Network Reconstruction of $H^{\prime }(z)$ and its application in Teleparallel Gravity
• PRIYA: A New Suite of Lyman-alpha Forest Simulations for Cosmology
• Gravitational transitions via the explicitly broken symmetron screening mechanism
• S0 galaxies in the Coma cluster: Environmental dependence of the S0 offset from the Tully-Fisher relation
• Cosmological Constraints from the eBOSS Lyman-$\alpha$ Forest using the PRIYA Simulations
• Inflation from a nonlinear magnetic monopole field nonminimally coupled to curvature
• Towards a possible solution to the Hubble tension with Horndeski gravity
• The formation and survival of the Milky Way's oldest stellar disk
• Diffusion in unimodular gravity: Analytical solutions, late-time acceleration, and cosmological constraints
• Cosmological constraints on early dark energy from the full shape analysis of eBOSS DR16
• The metallicity and distance of NGC 2403 from blue supergiants
• A comparison of optimisation algorithms for high-dimensional particle and astrophysics applications
• Axiology
• ETHOS -- An effective parametrization and classification for structure formation: the non-linear regime at $z\gtrsim 5$
• Peculiar motion of Solar system from the Hubble diagram of supernovae Ia and its implications for cosmology
• Can a dust dominated universe have accelerated expansion?
• CMB anisotropies generated by a stochastic background of primordial magnetic fields with non-zero helicity
• Debiasing Cosmic Gravitational Wave Sirens
• Rapidly Descending Dark Energy and the End of Cosmic Expansion
• Searching for the Evidence of Dynamical Dark Energy
• Particle Swarm Optimization: An efficient method for tracing periodic orbits in 3D galactic potentials
• The prompt-early afterglow connection in gamma-ray bursts: implications for the early afterglow physics
• MCR-TRGB: A Multiwavelength-Covariant, Robust Tip of the Red Giant Branch Measurement Method
• Carbon stars as standard candles: II. The median J magnitude as a distance indicator
• Evolution of superclusters in the cosmic web
• Anisotropic massive Brans-Dicke gravity extension of the standard $\Lambda$CDM model
• ETpathfinder: a cryogenic testbed for interferometric gravitational-wave detectors
• candl: Cosmic Microwave Background Analysis with a Differentiable Likelihood
• Model-independent determination of the cosmic expansion rate. I. Application to type-Ia supernovae
• Bayesian model selection on Scalar $\epsilon$-Field Dark Energy
• Impact of the Hubble tension on the $r$-$n_s$ contour
• Exact Solutions in Higher-Dimensional Lovelock and $Ad{S}_5$ Chern-Simons Gravity
• Backreaction of axion-SU(2) dynamics during inflation
• Searching for Primordial Magnetic Fields with CMB B-modes
• A possible common explanation for several cosmic microwave background (CMB) anomalies: A strong impact of nearby galaxies on observed large-scale CMB fluctuations
• Non-Local Curvature and Gauss-Bonnet Cosmologies by Noether Symmetries
• Birth of the Universe from the Landscape of String Theory
• A three-dimensional map of the Milky Way using 66,000 Mira variable stars
• Revised constraints on the photon mass from well-localized fast radio bursts
• The Corona Borealis supercluster: connectivity, collapse, and evolution
• Quasars: standard candles up to z=7.5 with the precision of Supernovae Ia
• Tracing high redshift cosmic web with quasar systems
• Testing $\Lambda$CDM cosmology in a binned universe: anomalies in the deceleration parameter
• Quantum Genetic Algorithm with Individuals in Multiple Registers
• Euclid preparation III. Galaxy cluster detection in the wide photometric survey, performance and algorithm selection
• Alleviating $H_0$ Tension with New Gravitational Scalar Tensor Theories
• New late-time constraints on $f(R)$ gravity
• Decaying dark matter, the $H_0$ tension, and the lithium problem
• C${}^3$-Cluster Clustering Cosmology I. New constraints on the cosmic growth rate at z~0.3 from redshift-space clustering anisotropies
• Fractional Holographic Dark Energy
• A solution of the strong CP problem via the Peccei-Quinn mechanism through the Nieh-Yan modified gravity and cosmological implications
• ETHOS -- An Effective Theory of Structure Formation: Impact of Dark Acoustic Oscillations on Cosmic Dawn
• Gaussian Process Approach for Model-Independent Reconstruction of $f(Q)$ Gravity with Direct Hubble Measurements
• Observational test for $f(Q)$ gravity with weak gravitational lensing
• Model-independently calibrating the luminosity correlations of gamma-ray bursts using deep learning
• Kernel Selection for Gaussian Process in Cosmology: with Approximate Bayesian Computation Rejection and Nested Sampling
• Dark Matter Candidates of a Very Low Mass
• Constraints via the Event Horizon Telescope for Black Hole Solutions with Dark Matter under the Generalized Uncertainty Principle Minimal Length Scale Effect
• Properties of self-excited pulsations in 3D simulations of AGB stars and red supergiants
• Constraining light sterile neutrino mass with the BICEP2/Keck Array 2014 B-mode polarization data
• Torsion-induced gravitational $\theta$ term and gravitoelectromagnetism
• Probing correlations of early magnetic fields using mu-distortion
• Quintessential inflation and cosmological seesaw Mechanism: reheating and observational constraints
• Clusters of galaxies up to z=1.5 identified from photometric data of the Dark Energy Survey and unWISE
• Gravitational Redshift Constraints on the Effective Theory of Interacting Dark Energy
• The quest for new correlations in the realm of the Gamma-Ray Burst -- Supernova connection
• NoSOCS in SDSS. IV. The Role of Environment Beyond the Extent of Galaxy Clusters
• Testing an oscillatory behavior of dark energy
• New integrable models and analytical solutions in $f(R)$~cosmology with an ideal gas
• Starlet l1-norm for weak lensing cosmology
• H_0 tension: clue to common nature of dark sector?
• Profile Likelihoods in Cosmology: When, Why and How illustrated with $\Lambda$CDM, Massive Neutrinos and Dark Energy
• Toward a concordance teleparallel Cosmology II: Linear perturbation
• Quintessential Cosmological Tensions
• Brans-Dicke cosmology mimicking running vacuum
• Quadratic curvature theories formulated as Covariant Canonical Gauge theories of Gravity
• Observational constraints on conformal time symmetry, missing matter and double dark energy
• Newest measurements of Hubble constant from DESI 2024 BAO observations
• Fundamental constants and high resolution spectroscopy
• Lorentzian Quintessential Inflation
• New general parametrization of quintessence fields and its observational constraints
• Holographic dark energy: constraints on the interaction from diverse observational data sets
• An improved Tully-Fisher estimate of $H_0$
• Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension
• A roadmap to cosmological parameter analysis with third-order shear statistics I: Modelling and validation
• Cluster Mergers and the Origin of the ARCADE-2 Excess
• LiteBIRD Science Goals and Forecasts. A Case Study of the Origin of Primordial Gravitational Waves using Large-Scale CMB Polarization
• Strong lensing selection effects
• 4D Gauss-Bonnet gravity: cosmological constraints, $H_0$ tension and large scale structure
• Modeling Intrinsic Galaxy Alignment in the MICE Simulation
• The 3D Lyman-$\alpha$ Forest Power Spectrum from eBOSS DR16
• Analysis of Unified Galaxy Power Spectrum Multipole Measurements
• An updated Type II supernova Hubble diagram
• Compressing the cosmological information in one-dimensional correlations of the Lyman-$\alpha$ forest
• A Stochastic Approach To Reconstruct Gamma Ray Burst Lightcurves
• No-go guide for the Hubble tension: late-time or local-scale new physics
• The Cosmic Dipole in the Quaia Sample of Quasars: A Bayesian Analysis
• A short review on clustering dark energy
• A Maximum Likelihood Calibration of the Tip of the Red Giant Branch Luminosity from High Latitude Field Giants using Gaia Early Data Release 3 Parallaxes
• Scalar perturbations from inflation in the presence of gauge fields
• Dark Radiation from Neutrino Mixing after Big Bang Nucleosynthesis
• Wave Dark Matter and Ultra Diffuse Galaxies
• Alleviating $H_0$ tension in Horndeski gravity
• Testing f(R) gravity with the simulated data of gravitational waves from the Einstein Telescope
• Searching for dark energy with the Sun
• Massive Dark Matter Halos at High Redshift: Implications for Observations in the JWST Era
• Supernovae evidence for foundational change to cosmological models
• Apparent and emergent dark matter around a Schwarzschild black hole
• Progress on the calibration of surface brightness-color relations for early- and late-type stars
• Cosmological model-independent measurement of cosmic curvature using distance sum rule with the help of gravitational waves
• Do we need soft cosmology?
• Peculiar motion of the solar system derived from a dipole anisotropy in the redshift distribution of distant quasars
• Gamma-ray Bursts as Distance Indicators by a Statistical Learning Approach
• Impact of inhomogeneous reionization on the Lyman-α forest
• Bayesian reconstruction of the inflaton's speed of sound using CMB data
• ATLAS Probe: Breakthrough Science of Galaxy Evolution, Cosmology, Milky Way, and the Solar System
• X-ray scaling relations from a complete sample of the richest maxBCG clusters
• Solving the $H_0$ tension in $f(T)$ Gravity through Bayesian Machine Learning
• Large-scale motions and growth rate from forward-modelling Tully-Fisher peculiar velocities
• Strong constraints on a simple self-interacting neutrino cosmology
• Revisiting the impact of neutrino mass hierarchies on neutrino mass constraints in light of recent DESI data
• Large extra dimensions from higher-dimensional inflation
• Extracting cosmological parameters from N-body simulations using machine learning techniques
• Constraining interacting dark energy models with the halo concentration-mass relation
• Big-Bang nucleosynthyesis: constraints on nuclear reaction rates, neutrino degeneracy, inhomogeneous and Brans-Dicke models
• Mapping the ${\Lambda }_{\mathrm{s}}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate
• A BayeSN Distance Ladder: $H_0$ from a consistent modelling of Type Ia supernovae from the optical to the near infrared
• A gravitational constant transition within cepheids as supernovae calibrators can solve the Hubble tension
• A thorough investigation of the prospects of eLISA in addressing the Hubble tension: Fisher Forecast, MCMC and Machine Learning
• Exploring new physics in the late Universe's expansion through non-parametric inference
• Quintessential Inflation from Lorentzian Slow Roll
• The expected kinematic matter dipole is robust against source evolution
• The galaxy luminosity function and the Local Hole
• Nonparametric reconstruction of the Om diagnostic to test LCDM
• Exploring hints for dark energy density evolution in light of recent data
• Dark Radiation and Decaying Matter
• On the Statistical Significance of the Bulk Flow Measured by the PLANCK Satellite
• Constraining a late time transition of $G_{\mathrm{eff}}$ using low-z galaxy survey data
• Testing f(R) gravity models with quasar X-ray and UV fluxes
• Galaxy Formation in Sterile Neutrino Dark Matter Models
• Local Hole revisited: evidence for bulk motions and self-consistent outflow
• Running vacuum in Brans-Dicke theory: a possible cure for the ${\sigma }_8$ and $H_0$ tensions
• Alleviating Cosmological Tensions with a Coupled Scalar Fields Model
• Interpreting the CMB aberration and Doppler measurements: boost or intrinsic dipole?
• Sensitivity forecasts for the cosmological recombination radiation in the presence of foregrounds
• Two sides of the same coin: sterile neutrinos and dark radiation. Status and perspectives
• The El Gordo galaxy cluster challenges ΛCDM for any plausible collision velocity
• The deceleration parameter in `tilted' universes: generalising the Friedmann background
• Cascading Dark Energy
• Gaussian Approximation of Peak Values in the Integrated Sachs-Wolfe Effect
• Coupled Multi Scalar Field Dark Energy
• Scalar field dark matter and dark energy: a hybrid model for the dark sector
• The universal multiplicity function: counting halos and voids
• Hubble tension and absolute constraints on the local Hubble parameter
• Artificial intelligence and quasar absorption system modelling; application to fundamental constants at high redshift
• Observational Evidence of Evolving Dark Matter Profiles at $z\le 1$
• Cosmological Avatars of the Landscape I: Bracketing the SUSY Breaking Scale
• Dark energy perturbations in $N$-body simulations
• Equation of State of the Transplanckian Dark Energy and the Coincidence Problem
• Reexploration of interacting holographic dark energy model: Cases of interaction term excluding the Hubble parameter
• On chromonatural inflation in string theory
• Enhancing the H2O Megamaser Detection Rate Using Optical and Mid-infrared Photometry
• The Peebles -- Vilenkin quintessential inflation model revisited
• Neutrino mass bounds from confronting an effective model with BOSS Lyman-alpha data
• Absolute Calibration of Cepheid Period-Luminosity Relations in NGC 4258
• Neural Networks Optimized by Genetic Algorithms in Cosmology
• Gravitational Lensing in Modified Gravity: A case study for Fast Radio Bursts
• Optical and X-ray clusters as tracers of the supercluster-void network. II The spatial correlation function
• Update constraints on neutrino mass and mass hierarchy in light of dark energy models
• The redshift dependence of the inferred $H_0$ in a local void solution to the Hubble tension
• Gravitational-wave dark siren cosmology systematics from galaxy weighting
• Null test for cosmic curvature using Gaussian process
• Discreteness of Space from GUP in Strong Gravitational Fields
• Beyond the Boost: Measuring the intrinsic dipole of the CMB using the spectral distortions of the monopole and quadrupole
• Testing the Cosmological Principle in the radio sky
• TDCOSMO VIII: Cosmological distance measurements in light of the mass-sheet degeneracy -- forecasts from strong lensing and IFU stellar kinematics
• The kinetic gas universe
• Model-independent constraints on cosmic curvature: implication from the future gravitational wave observation DECIGO
• Intrinsic Bispectra of Cosmic Magnetic Fields
• Impact of baryons in cosmic shear analyses with tomographic aperture mass statistics
• Rescuing constraints on modified gravity using gravitational redshift in large-scale structure
• Measuring Hubble constant in an anisotropic extension of $\Lambda$CDM model
• Guess the cheese flavour by the size of its holes: A cosmological test using the abundance of Popcorn voids
• A model-independent characterisation of strong gravitational lensing by observables
• PeV IceCube signals and Dark Matter relic abundance in modified cosmologies
• The contribution of ultracompact dark matter minihalos to the isotropic radio background
• Bounce Models within Teleparallel modified gravity
• High Eddington quasars as discovery tools: current state and challenges
• Constraining f(R) models with cosmic chronometers and the HII galaxy Hubble diagram
• Strong Evidence Against a Statistically Isotropic Universe
• Neural networks and standard cosmography with newly calibrated high redshift GRB observations
• S-dual Inflation: BICEP2 data without unlikeliness
• Redshift-space distortions of galaxies, clusters and AGN: testing how the accuracy of growth rate measurements depends on scales and sample selections
• LiteBIRD Science Goals and Forecasts: Improving Sensitivity to Inflationary Gravitational Waves with Multitracer Delensing
• HOLISMOKES -- V. Microlensing of type II supernovae and time-delay inference through spectroscopic phase retrieval
• A note on the relations between thermodynamics, energy definitions and Friedmann equations
• Joint reconstructions of growth and expansion histories from stage-IV surveys with minimal assumptions. II. Modified gravity and massive neutrinos
• Applying the expanding photosphere and standardized candle methods to Type II-Plateau supernovae at cosmologically significant redshifts: the distance to SN 2013eq
• Cosmological foundations revisited with Pantheon+
• Impact of symmetron screening on the Hubble tension: new constraints using cosmic distance ladder data
• Cosmic Anisotropy and Fast Radio Bursts
• Reconciling $S_8$: Insights from Interacting Dark Sectors
• Non-detection of ${}^6$Li in Spite plateau stars with ESPRESSO
• Constraints on Cosmological Parameters with a Sample of Type Ia Supernovae from JWST
• Photometric Redshift Uncertainties in Weak Gravitational Lensing Shear Analysis: Models and Marginalization
• The cosmic shallows I: interaction of CMB photons in extended galaxy halos
• Probing spatial variation of the fine-structure constant using the CMB
• The evolution of Lithium: implications of a universal Spite plateau
• The Noether Bessel Hagen Symmetry Approach for Dynamical Systems
• Alleviating $H_0$ tension in scalar-tensor and bi-scalar-tensor theories
• Covariant cosmography: the observer-dependence of the Hubble parameter
• Comparative Analysis of TRGBs (CATs) from Unsupervised, Multi-Halo-Field Measurements: Contrast is Key
• Dynamics in interacting scalar-torsion theory
• Unifying Inflation with early and late Dark Energy in Multi-Fields: Spontaneously broken scale invariant TMT
• Neural network reconstruction of cosmology using the Pantheon compilation
• Bulk Flow Motion Detection in the Local Universe with Pantheon$+$ Type Ia Supernovae
• Cross-correlation of Planck CMB lensing with DESI galaxy groups
• Enhancing cosmic shear with the multi-scale lensing PDF
• IDECAMB: an implementation of interacting dark energy cosmology in CAMB
• Effects of Baryonic Feedback on the Cosmic Web
• C${}^3$-Cluster Clustering Cosmology II. First detection of the BAO peak in the three-point correlation function of galaxy clusters
• Big Bang Nucleosynthesis constraints on varying electron mass solution to the Hubble tension
• The clustering of baryonic matter. I: a halo-model approach
• A New Test of Dynamical Dark Energy Models and Cosmic Tensions in Hořava Gravity
• Nonminimally Coupled Boltzmann Equation I: Foundations
• Accounting for object detection bias in weak gravitational lensing studies
• A Model of Interacting Dark Matter and Dark Radiation for $H_0$ and ${\sigma }_8$ Tensions
• Constraining Dark-Matter Ensembles with Supernova Data
• MG-MAMPOSSt: A code to test modifications of gravity with the dynamics of galaxy clusters
• Non-comoving Cosmology
• Easily Interpretable Bulk Flows: Continuing Tension with the Standard Cosmological Model
• Pseudoscalar sterile neutrino self-interactions in light of Planck, SPT and ACT data
• Field Theories and Fluids for an Interacting Dark Sector
• Measurement of Redshift Space Power Spectrum for BOSS galaxies and the Growth Rate at redshift 0.57
• Dark Stars Powered by Self-Interacting Dark Matter
• Interacting dark sector from the trace-free Einstein equations: cosmological perturbations with no instability
• Zwicky Transient Facility and Globular Clusters: The Period-Luminosity and Period-Wesenheit Relations for Type II Cepheids
• Constraining constant and tomographic coupled dark energy with low-redshift and high-redshift probes
• The Hubble diagram for a system within dark energy: the location of the zero-gravity radius and the global Hubble rate
• Discordance of dipole asymmetries seen in recent large radio surveys with the Cosmological Principle
• Testing the $n_s-H_0$ scaling relation with Planck-independent CMB data
• Testing the isotropy of cosmic acceleration with Pantheon+ and SH0ES: A cosmographic analysis
• Gravitationally induced matter creation in scalar-tensor $f(R,T_{\mu \nu }{T}^{\mu \nu })$ gravity
• A critical discussion on the $H_0$ tension
• Compatibility of JWST results with exotic halos
• Testing cosmic anisotropy with Pade approximation and Pantheon+ sample
• New Early Dark Energy as a solution to the $H_0$ and $S_8$ tensions
• Modified gravity in the presence of matter creation: scenario for the late Universe
• Consistent extinction model for type Ia supernovae in Cepheid-based calibration galaxies and its impact on $H_0$
• Running Hubble constant: evolutionary Dark Energy
• Constraints on running vacuum model with $H(z)$ and $f{\sigma }_8$
• Evaluating the New Automatic Method for the Analysis of Absorption Spectra Using Synthetic Spectra
• Scalar-Tensor Gravity and DESI 2024 BAO data
• The Tully-Fisher relations for Hickson Compact Group galaxies
• Carbon stars as standard candles -- III. Un-binned maximum likelihood fitting and comparison with TRGB estimations
• Disformally Coupled Quintessence
• Constraints on the cosmological parameters with three-parameter correlation of Gamma-ray bursts
• Mass Bias of Weak Lensing Shear-selected Galaxy Cluster Samples
• Generalised model-independent characterisation of strong gravitational lenses V: reconstructing the lensing distance ratio by supernovae for a general Friedmann universe
• CoLFI: Cosmological Likelihood-free Inference with Neural Density Estimators
• Detecting Features in the Dark Energy Equation of State: A Wavelet Approach
• Scaling solutions in quintessential inflation
• Reconstructing Quintessence
• Status Report on the Chicago-Carnegie Hubble Program (CCHP): Measurement of the Hubble Constant Using the Hubble and James Webb Space Telescopes
• Holographic and Gravity-Thermodynamic Approaches in Entropic Cosmology: Bayesian Assessment using late-time Data
• Cluster cosmology with anisotropic boosts: Validation of a novel forward modeling analysis and application on SDSS redMaPPer clusters
• $f\left(R,{\nabla }_{{\mu }_1}R,\dots ,{\nabla }_{{\mu }_1}\dots {\nabla }_{{\mu }_n}R\right)$ theories of gravity in Einstein frame: A higher order modified Starobinsky inflation model in the Palatini approach
• Compressed baryon acoustic oscillation analysis is robust to modified-gravity models
• Gravitational wave birefringence in spatially curved teleparallel cosmology
• Tracking the Multifield Dynamics with Cosmological Data: A Monte Carlo approach
• Bounds on Neutrino Mass in Viscous Cosmology
• The Layzer-Irvine equation in theories with non-minimal coupling between matter and curvature
• Dark Energy from Inspiraling in Field Space
• Jeans Instability in Non-Minimal Matter-Curvature Coupling Gravity
• Dynamic cosmography of the local Universe: Laniakea and five more watershed superclusters
• Effect of extinction on quasar luminosity distances determined from UV and X-ray flux measurements
• Dark Matter Line Searches with the Cherenkov Telescope Array
• An Empirical Calibration of the Tip of the Red Giant Branch Distance Method in the Near Infrared. I. HST WFC3/IR F110W and F160W Filters
• Global dynamics in Einstein-Gauss-Bonnet scalar field cosmology with matter
• Observational constraints on soft dark energy and soft dark matter: challenging $\Lambda$CDM
• NIR Tully-Fisher in the Zone of Avoidance. -- III. Deep NIR catalogue of the HIZOA galaxies
• Dark D-Brane Cosmology: from background evolution to cosmological perturbations
• f(T) cosmology against the cosmographic method: A new study using mock and observational data
• Differentiating dark interactions with perturbation
• Measuring anisotropic stress with relativistic effects
• D-term inflation in braneworld models: Consistency with cosmic-string bounds and early-time Hubble tension resolving models
• A Stimulating Explanation of the Extragalactic Radio Background
• A simple parametrisation for coupled dark energy
• Wavelet analysis of baryon acoustic structures in the galaxy distribution
• Constraints on the axial-vector and pseudo-scalar mediated WIMP-nucleus interactions from PandaX-4T experiment
• Can accreting primordial black holes explain the excess radio background?
• HOLISMOKES -- IX. Neural network inference of strong-lens parameters and uncertainties from ground-based images
• Precision cosmology with time delay lenses: high resolution imaging requirements
• The SRG/eROSITA All-Sky Survey: Weak-Lensing of eRASS1 Galaxy Clusters in KiDS-1000 and Consistency Checks with DES Y3 & HSC-Y3
• Electron mass variation from dark sector interactions and compatibility with cosmological observations
• Deviation from $\Lambda$CDM: Pressure Parametrization
• Baryon acoustic oscillations in thin redshift shells from BOSS DR12 and eBOSS DR16 galaxies
• A cosmic glitch in gravity
• Observational bounds on extended minimal theories of massive gravity: New limits on the graviton mass
• Hubble tension in a nonminimally coupled curvature-matter gravity model
• Getting the model right; an information criterion for spectroscopy
• Inverse Cosmography: testing the effectiveness of cosmographic polynomials using machine learning
• Extended Analysis of Neutrino-Dark Matter Interactions with Small-Scale CMB Experiments
• Constraining $\Lambda$CDM cosmological parameters with Einstein Telescope mock data
• The future of cosmological likelihood-based inference: accelerated high-dimensional parameter estimation and model comparison
• Cosmological constraints from weak lensing scattering transform using HSC Y1 data
• Testing the $\Lambda$CDM paradigm with growth rate data and machine learning
• Red, Straight, no bends: primordial power spectrum reconstruction from CMB and large-scale structure
• Dynamics and constraints of the dissipative Liouville cosmology
• A comparison between axion-like and power law potentials in cosmological background
• Baryon acoustic oscillation methods for generic curvature: Application to the SDSS-III Baryon Oscillation Spectroscopic Survey
• Future Constraints on Dark Matter with Gravitationally Lensed Fast Radio Bursts Detected by BURSTT
• On the Evolution of Cosmological Type Ia Supernovae and the Gravitational Constant
• A general study of decaying scalar dark matter: existing limits and projected radio signals at the SKA
• Velocity Dispersions of Clusters in the Dark Energy Survey Y3 redMaPPer Catalog
• Probing modified gravitational-wave propagation with extreme mass-ratio inspirals
• Which Fundamental Constants for CMB and BAO?
• A Gaia Data Release 3 View on the Tip of the Red Giant Branch Luminosity
• The Structure of Supervoids -- I: Void Hierarchy in the Northern Local Supervoid
• LADDER: Revisiting the Cosmic Distance Ladder with Deep Learning Approaches and Exploring its Applications
• Dark CP-violation through the $Z$-portal
• Primordial brusque bounce in Born-Infeld determinantal gravity
• Cosmic Growth in $f(T)$ Teleparallel Gravity
• Hamilton's Object -- a clumpy galaxy straddling the gravitational caustic of a galaxy cluster : Constraints on dark matter clumping
• Exploring Mirror Twin Higgs Cosmology with Present and Future Weak Lensing Surveys
• Geometrical origins of the Universe dark sector: string-inspired torsion and anomalies as seeds for inflation and dark matter
• Can decaying dark matter scenarios alleviate both $H_0$ and ${\sigma }_8$ tensions?
• Sunyaev-Zel'dovich effect and X-ray scaling relations of galaxies, groups and clusters in the IllustrisTNG simulations
• Calibration of Surface Brightness Fluctuations for Dwarf Galaxies in the Hyper Suprime-Cam $gi$ Filter System
• Scalar perturbations in the late Universe: viability of the Chaplygin gas models
• Cosmic Reionization History and Dark Matter Scenarios
• A roadmap to cosmological parameter analysis with third-order shear statistics III: Efficient estimation of third-order shear correlation functions and an application to the KiDS-1000 data
• Pantheon+ constraints on dark energy and modified gravity: An evidence of dynamical dark energy
• Finding origins of CMB anomalies in the inflationary quantum fluctuations
• Refined modelling of the radio SZ signal: kinematic terms, relativistic temperature corrections and anisotropies in the radio background
• Analysis of the apparent lack of power in the cosmic microwave background anisotropy at large angular scales
• The Atacama Cosmology Telescope: limits on dark matter-baryon interactions from DR4 power spectra
• Probing the two-body decaying dark matter scenario with weak lensing and the cosmic microwave background
• The eROSITA Final Equatorial-Depth Survey (eFEDS): A complete census of X-ray properties of Subaru Hyper Suprime-Cam weak lensing shear-selected clusters in the eFEDS footprint
• Ultralight dark photon as a model for early universe dark matter
• Cosmology in the Lorentz gauge theory
• Testing the parametric model for self-interacting dark matter using matched halos in cosmological simulations
• Consistency of Pantheon+ supernovae with a large-scale isotropic universe
• Enhanced Early Galaxy Formation in JWST from Axion Dark Matter?
• Field-level inference of cosmic shear with intrinsic alignments and baryons
• Dynamical consistency conditions for rapid turn inflation
• Dark energy, Ricci-nonflat spaces, and the Swampland
• The Spin Tensor of Dark Matter and the Hubble Parameter Tension
• Family dispute: do Type IIP supernova siblings agree on their distance?
• Bayesian analysis of a Unified Dark Matter model with transition: can it alleviate the $H_0$ tension?
• Impact of the damping tail on neutrino mass constraints
• Structure Formation Paradigm and Axion Quark Nugget dark matter model
• Constraints from High-Precision Measurements of the Cosmic Microwave Background: The Case of Disintegrating Dark Matter with $\Lambda$ or Dynamical Dark Energy
• On the interacting dark energy scenarios $-$ the case for Hubble constant tension
• On the effect of cyclotron emission on the spectral distortions of the cosmic microwave background
• Probing Small Scale Primordial Power Spectrum with 21cm Line Global Signal
• Investigating Gaia EDR3 parallax systematics using asteroseismology of Cool Giant Stars observed by Kepler, K2, and TESS II. Deciphering Gaia parallax systematics using red clump stars
• Hints of Neutrino Dark Matter scattering in the CMB? Constraints from the Marginalized and Profile Distributions
• The evolution of high-density cores of the BOSS Great Wall superclusters
• Spatial Curvature and Thermodynamics
• Optical interferometry and Gaia measurement uncertainties reveal the physics of asymptotic giant branch stars
• An empirical approach to model selection: weak lensing and intrinsic alignments
• BAO cosmology in non-spatially flat background geometry from BOSS+eBOSS and lessons for future surveys
• Scalar Field Theory Description of the Running Vacuum Model: the Vacuumon
• The FLAMINGO project: Baryonic impact on weak gravitational lensing convergence peak counts
• 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
• Reeling in the Whirlpool: the distance to M 51 clarified by Cepheids and the Type IIP SN 2005cs
• Fast Radio Bursts as probes of the late-time universe: a new insight on the Hubble tension
• Cosmological Implications of the String Theory Landscape
• A Framework for Obtaining Accurate Posteriors of Strong Gravitational Lensing Parameters with Flexible Priors and Implicit Likelihoods using Density Estimation
• Galaxy rotation curves using a non-parametric regression method: core, cusp and fuzzy scalar field dark matter models
• Reducing the $H_0$ Tension with Exponential Acoustic Dark Energy
• Thin-wall vacuum decay in the presence of a compact dimension meets the $H_0$ and $S_8$ tensions
• The Integrated Sachs-Wolfe Effect in Interacting Dark Matter-Dark Energy Models
• Sensitivity reach of gamma-ray measurements for strong cosmological magnetic fields
• Topological Quintessence
• Measuring the distortion of time with relativistic effects in large-scale structure
• Observational Evidence for Negative-Energy Dust in Late-Times Cosmology
• The CMB Cold Spot as predicted by foregrounds around nearby galaxies
• Primordial Bispectrum and Trispectrum Contributions to the Non-Gaussian Excursion Set Halo Mass Function with Diffusive Drifting Barrier
• A multitracer analysis for the eBOSS galaxy sample based on the effective field theory of large-scale structure
• Constraining Self-interacting Scalar Field Dark Matter From the Black Hole Shadow of the Event Horizon Telescope
• Stochastic star formation and the abundance of $z>10$ UV-bright galaxies
• Disentangling Doppler modulation, aberration and the temperature dipole in the CMB
• A generalized mass-to-horizon relation: a new global approach to entropic cosmologies and its connection to $\Lambda$CDM
• Photometric redshifts and intrinsic alignments: degeneracies and biases in 3$\times$2pt analysis
• Viability of the Matter Bounce Scenario
• Quantifying the tension between cosmological models and JWST red candidate massive galaxies
• Cosmological constraints using Minkowski functionals from the first year data of the Hyper Suprime-Cam
• Inflation Driven by Non-Linear Electrodynamics
• Discrepancy between cosmological and electroweak observables in Higgs Inflation
• Role of the Hubble Scale in the Weak Lensing vs. CMB Tension
• Gravitational Wave from Axion-SU(2) Gauge Fields: Effective Field Theory for Kinetically Driven Inflation
• Testing anisotropic Hubble expansion
• Non-oscillating Early Dark Energy and Quintessence from Alpha-Attractors
• Bayesian methods for fitting Baryon Acoustic Oscillations in the Lyman-$\alpha$ forest
• A theoretical estimate of intrinsic ellipticity bispectra induced by angular momenta alignments
• Interacting Scalar fields: Dark matter and early dark energy
• Unveiling the largest structures in the nearby Universe: Discovery of the Quipu superstructure
• Paths to gravitation via the gauging of parameterized field theories
• DE models with combined $H_0\cdot r_d$ from BAO and CMB dataset and friends
• The Anisotropy of the Extragalactic Radio Background from Dark Matter Annihilation
• A More Efficient Search for H2O Megamaser Galaxies : The Power of the X-ray and Mid-infrared Photometry
• Shell-like structures in our cosmic neighbourhood
• On How to Extend the NIR Tully-Fisher Relation to be Truly All-Sky
• Cosmology in a reduced Born-Infeld--$f(T)$ theory of gravity
• Quark stars with isotropic matter in Hořava gravity and Einstein-æther theory
• How much primordial tensor mode is allowed?
• Time Delay of Light in the Gravitational lensing of Supermassive Black Holes in Dark Matter Halos
• Search for the $f(R,T)$ gravity functional form via gaussian processes
• Integrated photometry of multiple stellar populations in Globular Clusters
• $f(T)$ cosmology in the regime of quasar observations
• Investigating the impact of galaxies' compact binary hosting probability for gravitational-wave cosmology
• Tachyon inflation in an AdS braneworld with back-reaction
• Quantum kinetic theory of Jeans instability in non-minimal matter-curvature coupling gravity
• Apercal -- The Apertif Calibration Pipeline
• AMICO galaxy clusters in KiDS-DR3: Cosmological constraints from angular power spectrum and correlation function
• Forecast on lepton asymmetry from future CMB experiments
• Big bang nucleosynthesis and early dark energy in light of the EMPRESS $Y_p$ results and the $H_0$ tension
• A MeerKAT, e-MERLIN, H.E.S.S. and Swift search for persistent and transient emission associated with three localised FRBs
• Pixelated Reconstruction of Foreground Density and Background Surface Brightness in Gravitational Lensing Systems using Recurrent Inference Machines
• The IC133 Water Vapor Maser in the Galaxy M33: A Geometric Distance
• Scalar induced gravitational waves in symmetric teleparallel gravity with a parity-violating term
• Neutrino astronomy as a probe of physics beyond the Standard Model: decay of sub-MeV $B$-$L$ gauge boson dark matter
• Axial Ratio of Edge-On Spiral Galaxies as a Test For Extended Bright Radio Halos
• The Cosmic Large-Scale Structure in X-rays (CLASSIX) Cluster Survey II: Unveiling a pancake structure with a 100 Mpc radius in the local Universe
• Reconstructing the Hubble parameter with future Gravitational Wave missions using Machine Learning
• Potential biases and prospects for the Hubble constant estimation via electromagnetic and gravitational-wave joint analyses
• Axion gravitodynamics, Lense-Thirring effect, and gravitational waves
• Effects of heterogeneous data sets and time-lag measurement techniques on cosmological parameter constraints from MgII and CIV reverberation-mapped quasar data
• Deep Neural Networks for Estimation of Gamma-Ray Burst Redshifts
• Dissecting a miniature universe: A multi-wavelength view of galaxy quenching in the Shapley supercluster
• Consistency of nonlinear interacting ghost dark energy with recent observations
• The Wide-field Spectroscopic Telescope (WST) Science White Paper
• $f(T)$ Cosmology with Nonzero Curvature
• Structure Formation in Various Dynamical Dark Energy Scenarios
• Tsallis holographic dark energy with power law ansatz approach
• A visual tool for assessing tension-resolving models in the $H_0$-${\sigma }_8$ plane
• Modified majoron model for cosmological anomalies
• DISCO-DJ I: a differentiable Einstein-Boltzmann solver for cosmology
• First constraints on non-minimally coupled Natural and Coleman-Weinberg inflation and massive neutrino self-interactions with Planck+BICEP/Keck
• LiteBIRD Science Goals and Forecasts: Primordial Magnetic Fields
• Dark Energy Survey: Galaxy Sample for the Baryonic Acoustic Oscillation Measurement from the Final Dataset
• Clustering of CODEX clusters
• Reassessment of the dipole in the distribution of quasars on the sky
• How accurately can we measure the baryon acoustic oscillation feature?
• Deviation From ΛCDM With Cosmic Strings Networks
• Consistent Constraints on the Equivalence Principle from localised Fast Radio Bursts
• Primordial Magnetism in CMB B-modes
• Post-reionization HI 21-cm signal: A probe of negative cosmological constant
• New insights on $\nu$-DM Interactions
• Period-Luminosity Relations for Galactic classical Cepheids in the Sloan bands
• Cosmological Distances And Hubble Tension In Einstein-Cartan Theory
• The H0 trouble: Confronting Non-thermal Dark Matter and Phantom Cosmology with the CMB, BAO, and Type Ia Supernovae data
• A comparison of Bayesian sampling algorithms for high-dimensional particle physics and cosmology applications
• Solar chameleons: Novel channels
• A generalized uncertainty-inspired quantum black hole
• Surface Tension of Cosmic Voids as a Possible Source for Dark Energy
• Standardized Luminosity of the Tip of the Red Giant Branch utilizing Multiple Fields in NGC 4258 and the CATs Algorithm
• Fundamental Physics with ESPRESSO, Constraining a simple parametrisation for varying $\alpha$
• Warm inflation with non-comoving scalar field and radiation fluid
• Irreversible Geometrothermodynamics of Open Systems in Modified Gravity
• A possible late-time transition of $M_B$ inferred via neural networks
• Explanation of high redshift luminous galaxies from JWST by early dark energy model
• Reconstructing the growth index $\gamma$ with Gaussian Processes
• Rhapsody-C simulations -- Anisotropic thermal conduction, black hole physics, and the robustness of massive galaxy cluster scaling relations
• Improving Photometric Redshift Estimates with Training Sample Augmentation
• Dark Energy Survey Year 3: Blue Shear
• The supercluster-void network V. Alternative evidence for its regularity
• Be careful in multi-messenger inference of the Hubble constant: A path forward for robust inference
• Viewing angle observations and effects of evolution with redshift, black hole mass, and Eddington ratio in quasar based cosmology
• Observational Constraints on the Dark Energy with a Quadratic Equation of State
• Can the Local Bubble explain the radio background?
• The contribution of star-forming galaxies to the cosmic radio background
• Checking the second law at cosmic scales
• Fast and effortless computation of profile likelihoods using CONNECT
• Continuous gravitational wave detection to understand the generation mechanism of fast radio bursts
• JWST high redshift galaxy observations have a strong tension with Planck CMB measurements
• Cosmological effects of the Galileon term in Scalar-Tensor Theories
• Testing $\alpha$-attractor quintessential inflation against CMB and low-redshift data
• Detection of ${}^7$Be II in the Small Magellanic Cloud
• Cosmology from LOFAR Two-metre Sky Survey Data Release 2: Cross-correlation with the cosmic microwave background
• LimberJack.jl: auto-differentiable methods for angular power spectra analyses
• Constraints on the speed of sound in the k-essence model of dark energy
• Complementary Probes of Two-component Dark Matter
• Cosmological Constraints on Entropic Cosmology with Matter Creation
• Robust constraints on tensor perturbations from cosmological data: a comparative analysis from Bayesian and frequentist perspectives
• Is cosmological data suggesting a nonminimal coupling between matter and gravity?
• Interacting dark energy in the dark $SU(2{)}_R$ model
• New calibrated models for the TRGB luminosity and a thorough analysis of theoretical uncertainties
• A Cosmological Unicorn Solution to Finsler Gravity
• Weak-Lensing Shear-Selected Galaxy Clusters from the Hyper Suprime-Cam Subaru Strategic Program: II. Cosmological Constraints from the Cluster Abundance
• Tomographic redshift dipole: Testing the cosmological principle
• Impact of baryonic feedback on HSC Y1 weak lensing non-Gaussian statistics
• A closer look at dark photon explanations of the excess radio background
• Chameleon Mechanism in Scalar Nonmetricity Cosmology
• The biasing phenomenon
• PROBES-I: A Compendium of Deep Rotation Curves and Matched multiband Photometry
• Dark energy reconstruction analysis with artificial neural networks: Application on simulated Supernova Ia data from Rubin Observatory
• Probing the anisotropic distribution of baryon matter in the Universe using fast radio bursts
• Constraints on extended Bekenstein models from cosmological, astrophysical, and local data
• The interacting vacuum and tensions: a comparison of theoretical models
• Data-driven and Almost Model-independent Reconstruction of Modified Gravity
• Searching for TeV Dark Matter in Irregular dwarf galaxies with HAWC Observatory
• Towards early-type eclipsing binaries as extragalactic milestones: II. NLTE spectral analysis and stellar parameters of the detached O-type system OGLE-LMC-ECL-06782 in the LMC
• What if Newton's Gravitational Constant was negative?
• Cross-correlation between $Planck$ CMB lensing potential and galaxy catalogues from HELP
• Generalised model-independent characterisation of strong gravitational lenses VIII. automated multi-band feature detection to constrain local lens properties
• Scaling solutions as Early Dark Energy resolutions to the Hubble tension
• Searching for local features in primordial power spectrum using genetic algorithms
• Can Early Dark Energy be Probed by the High-Redshift Galaxy Abundance?
• Particle creation and reheating in a braneworld inflationary scenario
• Revisiting dark energy models using differential ages of galaxies
• Stellar Neutrino Emission Across The Mass-Metallicity Plane
• Runaway dilaton models: improved constraints from the full cosmological evolution
• The low multipoles in the Pantheon+SH0ES data
• Exploiting the diversity of modeling methods to probe systematic biases in strong lensing analyses
• Einstein-aether theory in Weyl integrable geometry
• Potentialities of Hubble parameter and expansion rate function data to alleviate Hubble tension
• Gravitational wave cosmology and astrophysics with large spectroscopic galaxy surveys
• KiDS-Legacy: Covariance validation and the unified OneCovariance framework for projected large-scale structure observables
• Detection of Dipole Modulation in CMB Temperature Anisotropy Maps from WMAP and Planck using Artificial Intelligence
• Hamiltonian formulation of gravity as a spontaneously-broken gauge theory of the Lorentz group
• Hubble constant by natural selection: Evolution chips in the Hubble tension
• Model selection and parameter estimation using the iterative smoothing method
• Relic neutrino decay solution to the excess radio background
• A search for the fine-structure constant evolution from fast radio bursts and type Ia supernovae data
• Exploring evidence of interaction between dark energy and dark matter
• Cosmic voids and the kinetic analysis. III. Hubble tension and structure formation in the late Universe
• A local infall from a cosmographic analysis of Pantheon+
• Disentangling modified gravity from a dark force with gravitational redshift
• Determining the Hubble Constant with AGN-assisted Black Hole Mergers
• Gravitational particle production and the Hubble tension
• A study of Dipolar Signal in distant Quasars with various observables
• A Non-parametric Reconstruction of the Hubble Parameter $H(z)$ Based on Radial Basis Function Neural Networks
• Gravitational Lensing of Spherically Symmetric Black Holes in Dark Matter Halos
• Isotropic non-Gaussian $g_{\mathrm{NL}}$-like toy models that reproduce the cosmic microwave background anomalies
• 6Li in metal-poor halo stars: real or spurious?
• Modelling the emergence of cosmic anisotropy from non-linear structures
• Calibration of the Tully-Fisher relation in the WISE W1 ($3.4\mu \mathrm{m}$) and W2 ($4.6\mu \mathrm{m}$) Bands
• Anisotropic fluid spheres in Hořava gravity and Einstein-æther theory with a non-static æther
• Non-particle dark matter from Hubble parameter
• Oscillations of sterile neutrinos from dark matter decay eliminates the IceCube-Fermi tension
• The Coma - Leo I Distance Ratio and the Hubble Constant
• The End for Extended Inflation?
• Testing the Cosmological Principle: On the Time Dilation of Distant Sources
• Resolution of the incongruency of dipole asymmetries within various large radio surveys -- implications for the Cosmological Principle
• Tensions in cosmology: a discussion of statistical tools to determine inconsistencies
• New insights into the use of Ultra Long Period Cepheids as cosmological standard candles
• Quintessential Implications of the presence of AdS in the Dark Energy sector
• VI-Band Follow-Up Observations of Ultra-Long-Period Cepheid Candidates in M31
• Cosmological tensions in the birthplace of the heliocentric model
• Constraining Coupling Constants' Variation with Supernovae, Quasars, and GRBs
• Euclid and KiDS-1000: Quantifying the impact of source-lens clustering on cosmic shear analyses
• Simultaneous measurements on cosmic curvature and opacity using latest HII regions and $H(z)$ observations
• Small-scale CMB anisotropies induced by the primordial magnetic fields
• Deep Learning and genetic algorithms for cosmological Bayesian inference speed-up
• Symbolic Implementation of Extensions of the $\text{PyCosmo}$ Boltzmann Solver
• Spherical Collapse Approach for Non-standard Dark Matter Models and Enhanced Early Galaxy Formation in JWST
• Consistent first order action functional for gauge theories
• Constraints on Cosmological Models with Gamma-Ray Bursts in Cosmology-Independent Way
• Impact of Cosmology on Lorentz Invariance Violation Constraints from GRB Time-Delays
• S-dual Inflation and the String Swampland
• Self-similar galaxy dynamics below the de Sitter scale of acceleration
• A Snowmass Whitepaper: Dark Matter Production at Intensity-Frontier Experiments
• Episodic super-Eddington accretion as a clue to Overmassive Black Holes in the early Universe
• Diffusion-HMC: Parameter Inference with Diffusion-model-driven Hamiltonian Monte Carlo
• Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations?
• Scrutinizing Early Dark Energy models through CMB lensing
• Stability and pulsation of the first dark stars
• Agnostic cosmology in the CAMEL framework
• Lower tensor-to-scalar ratio as possible signature of modified gravity
• Difficulties in reconciling non-negligible differences between the local and cosmological values of the gravitational coupling in extended Brans-Dicke theories
• Probing Ultra-light Axion Dark Matter from 21cm Tomography using Convolutional Neural Networks
• Statistical analysis with cosmic-expansion-rate measurements and two-point diagnostics
• Model-independent approach to effective sound speed in multi-field inflation
• Effects of a Late Gravitational Transition on Gravitational Waves and Anticipated Constraints
• Examining the validity of the minimal varying speed of light model through cosmological observations: relaxing the null curvature constraint
• The ups and downs of inferred cosmological lithium
• ISW in $\Lambda$CDM or something else?
• The CMB lensing imprint of cosmic voids detected in the WISE-Pan-STARRS luminous red galaxy catalog
• Cosmology Large Angular Scale Surveyor (CLASS): 90 GHz Telescope Pointing, Beam Profile, Window Function, and Polarization Performance
• A diffeomorphism invariant family of metric-affine actions for loop cosmologies
• Is there evidence for CIDER in the Universe?
• Examining the local Universe isotropy with galaxy cluster velocity dispersion scaling relations
• Towards primordial gravitational waves and $n_s=1$ in light of BICEP/Keck, DESI BAO and Hubble tension
• CMB sky for an off-center observer in a local void I: framework for forecasts
• A possible role for the merger of clusters/voids in the cosmological expansion
• Strongly Lensed Supernovae in Well-Studied Galaxy Clusters with the Vera C. Rubin Observatory
• Diffuse Sources, Clustering and the Excess Anisotropy of the Radio Synchrotron Background
• Spherical collapse of non-top-hat profiles in the presence of dark energy with arbitrary sound speed
• On the Hubble expansion in a Big Bang quantum cosmology
• First investigation of void statistics in numerical relativity simulations
• Tutorial on ABC rejection and ABC SMC for parameter estimation and model selection
• Cosmic voids and the kinetic analysis. II. Link to Hubble tension
• Big Bang in Dipole Cosmology
• The catalog-to-cosmology framework for weak lensing and galaxy clustering for LSST
• Yonsei Evolutionary Population Synthesis (YEPS) Model. III. Surface Brightness Fluctuation of Normal and Helium-enhanced Simple Stellar Populations
• On the thermodynamics of reconciling quantum and gravity
• Incompatibility of fine-structure constant variations at recombination with local observations
• On Evidence for Elastic Interactions in the Dark Sector
• Limit on the dark matter mass from its interaction with photons
• Bianchi type II,III and V diagonal Einstein metrics re-visited
• Studies on dark energy evolution
• Procoli: Profiles of cosmological likelihoods
• An Analysis of Variance of the Pantheon+ Dataset: Systematics in the Covariance Matrix?
• The Tip of the Red Giant Branch Distance Ladder and the Hubble Constant
• Improved Lemaitre-Tolman model and the mass and turn-around radius in group of galaxies II: the role of dark energy
• Calibrating and standardizing the Tip of the Red Giant Branch in the Small Magellanic Cloud using small-amplitude red giants
• Early dark energy induced by non-linear electrodynamics
• Weak Primordial Magnetic Fields and Anisotropies in the Cosmic Microwave Background Radiation
• Impact of Low ell's on Large Scale Structure Anomalies
• Higgs Inflation: constraining the top quark mass and breaking the $H_0$-${\sigma }_8$ correlation
• Synthetic Population of Binary Cepheids. II. The effect of companion light on the extragalactic distance scale
• Constraining Fundamental Constants with Fast Radio Bursts: Unveiling the Role of Energy Scale
• Quasi-spherical superclusters
• Gravitational Slip parameter and Gravitational Waves in Einstein-Cartan theory
• Tully-Fisher Relation of Late-type Galaxies at $0.6\le z\le 2.5$
• Coupling quintessence kinetics to electromagnetism
• Cosmological Principle in Newtonian Dynamics
• An Analytic Formula for the Supercluster Mass Function
• Model-independent Gamma-Ray Bursts Constraints on Cosmological Models Using Machine Learning
• Cosmic voids and the kinetic analysis. IV. Hubble tension and the cosmological constant
• Beyond dark energy Fisher forecasts: how DESI will constrain LCDM and quintessence models
• Effort: a fast and differentiable emulator for the Effective Field Theory of the Large Scale Structure of the Universe
• A doublet of cosmological models to challenge the H0 tension in the Pantheon Supernovae Ia catalog
• Hubble tension and matter inhomogeneities: a theoretical perspective
• Signatures of Recent Cosmic-Ray Acceleration in the High-Latitude $\gamma$-Ray Sky
• Stage IV baryonic feedback correction for non-Gaussianity inference
• Nucleation regions in the Large-Scale Structure I. A catalogue of cores in nearby rich superclusters
• Growth of cosmic perturbations in the modified $f(R,T)$ gravity
• New high S/N observations of the Li-6/Li-7 blend in HD 84937 and two other metal-poor stars
• Cosmological constraints on light flavons
• Unexplained correlation between the Cosmic Microwave Background temperature and the local matter density distribution
• SN 2023adsy: A normal type Ia Supernova at z=2.9
• Investigating cosmic strings using large-volume hydrodynamical simulations in the context of JWST's massive UV-bright galaxies
• Comparison of results on $N_{\mathrm{eff}}$ from various Planck likelihoods
• Calibrating the Tully-Fisher Relation to Measure the Hubble Constant
• Tomographic cross correlations between galaxy surveys and the CMB gravitational lensing potential. Effect of the redshift bin mismatch
• Neutrino-Assisted Early Dark Energy is a Natural Resolution of the Hubble Tension
• Cosmological inference from within the peculiar local universe
• 2D BAO vs 3D BAO: Hints for new physics?
• Cosmology from UNIONS weak lensing profiles of galaxy clusters
• Joint Modelling of Astrophysical Systematics for Cosmology with LSST Cosmic Shear
• Dynamics of Inspiraling Dark Energy
• Dynamical dark energy with AdS-to-dS and dS-to-dS transitions: Implications for the $H_0$ tension
• Fast multiscale galaxy cluster detection with weak lensing: towards a mass-selected sample
• Mass bias and cosmological constraints from Planck cluster clustering
• Fundamental cosmology from ANDES precision spectroscopy
• Bayesian deep learning for dark energy
• Galaxy groups in the presence of Cosmological Constant: Increasing the Masses of Groups
• Constraints on Metastable Dark Energy Decaying into Dark Matter
• Investigating the Origin of CMB Large-Scale Features Using LiteBIRD and CMB-S4
• Galaxy dynamics tracing quantum cosmology beyond $\Lambda$CDM below the de Sitter scale of acceleration
• Hybrid Summary Statistics
• The Simons Observatory: impact of bandpass, polarization angle and calibration uncertainties on small-scale power spectrum analysis
• Primordial Power Spectrum of Five Dimensional Uniform Inflation
• Improved Lemaitre-Tolman model and the mass and turn-around radius in group of galaxies
• Inflation in Symmergent Metric-Palatini Gravity
• Impact of Neutrino Properties and Dark Matter on the Primordial Lithium Production
• Challenges to a sharp change in $G$ as a solution to the Hubble tension
• Perturbation in an interacting dark universe
• Clustering of Local Group distances: publication bias or correlated measurements? VII. A distance framework out to 100 Mpc
• Probing for Lorentz Invariance Violation in Pantheon Plus Dominated Cosmology
• Tracker behaviour of quintom dark energy and the Hubble tension
• Constraints on Primordial Magnetic Fields from High Redshift Stellar Mass Density
• A Measurement of Hubble Constant Using Cosmographic Approach from Fast Radio Bursts and SNe Ia
• HIGlow: Conditional Normalizing Flows for High-Fidelity HI Map Modeling
• The radio SZ effect as a probe of the cosmological radio background
• The imprint of primordial gravitational waves on the CMB intensity profile
• Metric-Affine Gauge theories of gravity: Foundations and new insights
• The Epoch of Reionization in Warm Dark Matter Scenarios
• $\Lambda$CDM and early dark energy in latent space: a data-driven parametrization of the CMB temperature power spectrum
• Weak Gravitational Lensing
• A universe born in a metastable false vacuum state needs not die
• Non-linear coupling in the dark sector as a running vacuum model
• Efficiency of weak lensing surveys to probe cosmological models
• Effect of redshift bin mismatch on cross correlation between DESI Legacy Imaging Survey and Planck CMB lensing potential
• A New Robust Partial $p$-Wasserstein-Based Metric for Comparing Distributions
• Timelike vs null deceleration parameter in tilted Friedmann universes
• The OGLE Collection of Variable Stars. Classical Cepheids in the Magellanic System
• Key early science with MANIFEST on GMT
• On the degeneracy between $f{\sigma }_8$ tension and its Gaussian process forecasting
• Constraining broad photon spectrum injections from exotic and astrophysical sources
• On priors and scale cuts in EFT-based full-shape analyses
• Non-parametric Reconstruction Of Some Cosmological Parameters
• Scalar field dark matter with time-varying equation of state
• The Gravitational Lensing Imprints of DES Y3 Superstructures on the CMB: A Matched Filtering Approach
• In search for the Local Universe dynamical homogeneity scale with CF4++ peculiar velocities
• Solution to the cosmological constant problem
• Modern Bayesian Sampling Methods for Cosmological Inference: A Comparative Study
• Evidence for dynamical dark energy from DESI-DR2 and SN data? A symbolic regression analysis
• Some Implications of the Leptonic Annihilation of Dark Matter: Possible Galactic Radio Emission Signatures and the Excess Radio Flux of Extragalactic Origin
• Non-linear Eulerian Hydrodynamics of Dark Energy: Riemann problem and Finite Volume Schemes
• The Chicago-Carnegie Hubble Program: The JWST J-region Asymptotic Giant Branch (JAGB) Extragalactic Distance Scale
• Ultra Long Period Cepheids as standard candles from Gaia to Rubin-LSST
• Asymptotic Giant Branch Variables as Extragalactic Distance Indicators
• When to interfere with dark matter? The impact of wave dynamics on statistics
• Outliers in DESI BAO: robustness and cosmological implications
• Reconciling Cosmological Tensions with Inelastic Dark Matter and Dark Radiation in a $\mathbf{U}(1{)}_{\mathbf{D}}$ Framework
• Non-minimal scalar-tensor theories
• Special cases of the Multi-Measure Model -- understanding the prolonged inflation
• The dynamics of vacuum, gravity and matter: Implications on the fundamental constants
• Weak Lensing by Galaxy Clusters
• Phantom scalar field cosmologies constrained by early cosmic measurements
• A cosmographic outlook on dark energy and modified gravity
• Gravitational Merging as a Possible Source for the Cosmological Accelerating
• Analytical constraints on bimetric gravity
• Alleviating cosmological tensions with a hybrid dark sector
• Constraining Co-Varying Coupling Constants from Globular Cluster Age
• Early Galaxies from Rare Inflationary Processes and JWST Observations
• Search for dark matter with IACTs and the Cherenkov Telescope Array
• Supermassive primordial black holes for the GHZ9 and UHZ1 observed by the JWST
• Discreteness effects in $N$-body simulations of warm dark matter
• Does the Low CMB Quadrupole Provide a New Cosmic Coincidence Problem ?
• Deep Learning Based Recalibration of SDSS and DESI BAO Alleviates Hubble and Clustering Tensions
• A Quadratic Equation of State to Cosmic Acceleration: Entropy Evolution and Phantom Crossing
• Structure formation in the local Universe and the cosmological constant
• Data-driven modeling of rotation curves with artificial neural networks
• Discovery of a likely Type II SN at $z$=3.6 with JWST
• CONCERTO: instrument and status
• Primordial Cosmology of an Emergent-like Universe from Modified Gravity: Reconstruction and Phenomenology Optimization with a Genetic Algorithm
• Cosmic shear beyond 2-point statistics: Accounting for galaxy intrinsic alignment with projected tidal fields
• Is it possible to separate baryonic from dark matter within the $\Lambda$-CDM formalism?
• The imprint of cosmic voids from the DESI Legacy Survey DR9 LRGs in the Planck 2018 lensing map through spectroscopically calibrated mocks
• Late-time data require smaller sound horizon at recombination
• Did the Big Bang and cosmic inflation really happen? (A tale of alternative cosmological models)
• Electromagnetic Waves in Cosmological Space-Time II. Luminosity Distance