Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM

Abstract

We present an improved determination of the Hubble constant (H0) from Hubble Space Telescope (HST) observations of 70 long-period Cepheids in the Large Magellanic Cloud. These were obtained with the same WFC3 photometric system used to measure Cepheids in the hosts of Type Ia supernovae. Gyroscopic control of HST was employed to reduce overheads while collecting a large sample of widely-separated Cepheids. The Cepheid Period-Luminosity relation provides a zeropoint-free link with 0.4% precision between the new 1.2% geometric distance to the LMC from Detached Eclipsing Binaries (DEBs) measured by Pietrzynski et al (2019) and the luminosity of SNe Ia. Measurements and analysis of the LMC Cepheids were completed prior to knowledge of the new LMC distance. Combined with a refined calibration of the count-rate linearity of WFC3-IR with 0.1% precision (Riess et al 2019), these three improved elements together reduce the full uncertainty in the LMC geometric calibration of the Cepheid distance ladder from 2.5% to 1.3%. Using only the LMC DEBs to calibrate the ladder we find H0=74.22 +/- 1.82 km/s/Mpc including systematic uncertainties, 3% higher than before for this particular anchor. Combining the LMC DEBs, masers in NGC 4258 and Milky Way parallaxes yields our best estimate: H0 = 74.03 +/- 1.42 km/s/Mpc, including systematics, an uncertainty of 1.91%---15% lower than our best previous result. Removing any one of these anchors changes H0 by < 0.7%. The difference between H0 measured locally and the value inferred from Planck CMB+LCDM is 6.6+/-1.5 km/s/Mpc or 4.4 sigma (P=99.999% for Gaussian errors) in significance, raising the discrepancy beyond a plausible level of chance. We summarize independent tests which show this discrepancy is not readily attributable to an error in any one source or measurement, increasing the odds that it results from a cosmological feature beyond LambdaCDM.

arXiv commentaccepted by ApJ, replaced with accepted version, 25 pages, 5 figures

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• Could quasar lensing time delays hint to a core component in halos, instead of H0 tension?
• An Improved Calibration of the Wavelength Dependence of Metallicity on the Cepheid Leavitt law
• The Early Dark Sector, the Hubble Tension, and the Swampland
• Standard Siren Speeds: Improving velocities in gravitational-wave measurements of $H_0$
• Tomographic measurement of the intergalactic gas pressure through galaxy-tSZ cross-correlations
• Testing H0 in Acoustic Dark Energy Models with Planck and ACT Polarization
• Measuring cosmological parameters with a luminosity-time correlation of gamma-ray bursts
• Determining the Hubble Constant without the Sound Horizon Scale: Measurements from CMB Lensing
• Prospects for improving cosmological parameter estimation with gravitational-wave standard sirens from Taiji
• 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
• Addressing the cosmological $H_0$ tension by the Heisenberg uncertainty
• Explaining Cosmological Anisotropy: Evidence for Causal Horizons from CMB data
• Dark Neutrino interactions phase out the Hubble tension
• A Standard Ruler at Cosmic Dawn
• Rastall gravity extension of the standard $\Lambda$CDM model: theoretical features and observational constraints
• Cosmological constraints from HII starburst galaxy apparent magnitude and other cosmological measurements
• Incompleteness Matters Not: Inference of $H_0$ from BBH-galaxy cross-correlations
• Solar neutrino probes of the muon anomalous magnetic moment in the gauged $U(1{)}_{L_{\mu }-L_{\tau }}$
• Cosmology under the fractional calculus approach
• Unbiased Hubble constant estimation from binary neutron star mergers
• Asymmetric mass ratios for bright double neutron-star mergers
• The BINGO Project I: Baryon Acoustic Oscillations from Integrated Neutral Gas Observations
• Data-driven Reconstruction of the Late-time Cosmic Acceleration with f(T) Gravity
• 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
• Gamma-Ray Bursts, Quasars, Baryonic Acoustic Oscillations, and Supernovae Ia: new statistical insights and cosmological constraints
• Time-delay cosmographic forecasts with strong lensing and JWST stellar kinematics
• Testing AdS early dark energy with Planck, SPTpol and LSS data
• Constraining the Hubble constant to a precision of about 1% using multi-band dark standard siren detections
• Connecting early and late epochs by f(z)CDM cosmography
• Parametric and nonparametric methods hint dark energy evolution
• Model independent calibrations of gamma ray bursts using machine learning
• Strongly lensed SNe Ia in the era of LSST: observing cadence for lens discoveries and time-delay measurements
• Can $f(T)$ gravity resolve the $H_0$ tension?
• A Critique of Holographic Dark Energy
• Can scale-dependent cosmology alleviate the $H_0$ tension?
• The Hubble constant from eight time-delay galaxy lenses
• Dark degeneracy I: Dynamical or interacting dark energy?
• Unveiling dark fifth forces with linear cosmology
• Constraining Teleparallel Gravity through Gaussian Processes
• Generalized Emergent Dark Energy: observational Hubble data constraints and stability analysis
• Cosmology-insensitive estimate of IGM baryon mass fraction from five localized fast radio bursts
• Challenging bulk viscous unified scenarios with cosmological observations
• Self-interacting neutrinos: solution to Hubble tension versus experimental constraints
• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from multi-tracer BAO analysis with galaxies and voids
• A parallax distance to 3C 273 through spectroastrometry and reverberation mapping
• Empirical calibration of the reddening maps in the Magellanic Clouds
• Strongly Lensed Transient Sources: A Review
• Measurements of the Hubble constant and cosmic curvature with quasars: ultra-compact radio structure and strong gravitational lensing
• Resolving the $H_0$ tension with diffusion
• Quantifying concordance of correlated cosmological data sets
• The influence of metallicity on the Leavitt Law from geometrical distances of Milky Way and Magellanic Clouds Cepheids
• Systematic uncertainty of standard sirens from the viewing angle of binary neutron star inspirals
• A 0.9% Calibration of the Galactic Cepheid luminosity scale based on Gaia DR3 data of open clusters and Cepheids
• Probing elastic interactions in the dark sector and the role of $S_8$
• Cosmography approach to dark energy cosmologies: new constrains using the Hubble diagrams of supernovae, quasars and gamma-ray bursts
• CMB tensions with low-redshift $H_0$ and $S_8$ measurements: impact of a redshift-dependent type-Ia supernovae intrinsic luminosity
• Cosmological dynamics of dark energy in scalar-torsion $f(T,\varphi )$ gravity
• Can Non-standard Recombination Resolve the Hubble Tension?
• Constraints on interacting dark energy models from time-delay cosmography with seven lensed quasars
• The Hubble Constant determined through an inverse distance ladder including quasar time delays and Type Ia supernovae
• On the road to percent accuracy II: calibration of the non-linear matter power spectrum for arbitrary cosmologies
• Warm Decaying Dark Matter and the Hubble Tension
• Testing the Consistency of Dust Laws in SN Ia Host Galaxies: A BayeSN Examination of Foundation DR1
• Quantum Anomalies in String-Inspired Running Vacuum Universe: Inflation and Axion Dark Matter
• A fake Interacting Dark Energy detection?
• Matter Power Spectrum Emulator for f(R) Modified Gravity Cosmologies
• Non-parametric reconstruction of the cosmological \textit{jerk} parameter
• The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method
• Cosmological constraints from higher-redshift gamma-ray burst, HII starburst galaxy, and quasar (and other) data
• Cosmological model-independent constraints on spatial curvature from strong gravitational lensing and type Ia supernova observations
• Emergent Dark Energy, neutrinos and cosmological tensions
• Cosmographic parameters in model-independent approaches
• Constraining the cosmological parameters using gravitational wave observations of massive black hole binaries and statistical redshift information
• Sterile neutrino self-interactions: $H_0$ tension and short-baseline anomalies
• Euclid: impact of nonlinear prescriptions on cosmological parameter estimation from weak lensing cosmic shear
• Implications of the possible 21-cm line excess at cosmic dawn on dynamics of interacting dark energy
• TDCOSMO II: 6 new time delays in lensed quasars from high-cadence monitoring at the MPIA 2.2m telescope
• Comparison between different methods of model selection in cosmology
• Cosmic evolution and thermal stability of Barrow holographic dark energy in nonflat Friedmann-Robertson-Walker Universe
• The Cepheid Distance to the Seyfert 1 Galaxy NGC 4151
• Persistent homology in cosmic shear: constraining parameters with topological data analysis
• Simple-graduated dark energy and spatial curvature
• Is there really a Hubble tension?
• Mirror Twin Higgs Cosmology: Constraints and a Possible Resolution to the $H_0$ and $S_8$ Tensions
• Testing the effect of $H_0$ on $f{\sigma }_8$ tension using a Gaussian Process method
• Solving the curvature and Hubble parameter inconsistencies through structure formation-induced curvature
• Tracing dark energy history with gamma ray bursts
• Chain Early Dark Energy: Solving the Hubble Tension and Explaining Today's Dark Energy
• Neural Network Reconstruction of Late-Time Cosmology and Null Tests
• Ultralight Scalar Decay and the Hubble Tension
• Strong gravitational lensing and microlensing of supernovae
• COSMOGRAIL XVIII: time delays of the quadruply lensed quasar WFI2033-4723
• Modeling the Extragalactic Background Light and the Cosmic Star Formation History
• Reconstructing teleparallel gravity with cosmic structure growth and expansion rate data
• Screened fifth forces lower the TRGB-calibrated Hubble constant too
• Testing the Mutual Consistency of the Pantheon and SDSS/eBOSS BAO Data Sets with Gaussian Processes
• 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
• Model-independent measurement of cosmic curvature with the latest $H(z)$ and SNe Ia data: A comprehensive investigation
• Cosmological Constraints on First-Order Phase Transitions
• Hierarchical Inference With Bayesian Neural Networks: An Application to Strong Gravitational Lensing
• Intimate Relationship Between Sterile Neutrino Dark Matter and $\Delta N_{\mathrm{eff}}$
• Uncertain Times: The Redshift-Time Relation from Cosmology and Stars
• Current and future constraints on cosmology and modified gravitational wave friction from binary black holes
• Time Delay Lens Modelling Challenge
• Cosmography by orthogonalized logarithmic polynomials
• Observational constraints of a new unified dark fluid and the $H_0$ tension
• Modelling and testing the equation of state for (Early) dark energy
• Revealing the late-time transition of $H_0$: relieve the Hubble crisis
• A sub-2% Distance to M31 from Photometrically Homogeneous Near-Infrared Cepheid Period-Luminosity Relations Measured with the Hubble Space Telescope
• A sub-GeV dark matter model
• The Accuracy of the Hubble Constant Measurement Verified through Cepheid Amplitudes
• Multi-interacting dark energy and its cosmological implications
• Near-IR Type Ia SN distances: host galaxy extinction and mass-step corrections revisited
• Exploring Early Dark Energy solution to the Hubble tension with Planck and SPTPol data
• Measuring the Hubble Constant with a sample of kilonovae
• Strong detection of the CMB lensingxgalaxy weak lensingcross-correlation from ACT-DR4,PlanckLegacy and KiDS-1000
• Gravity in the infrared and effective nonlocal models
• Reconstruction of quintessence field for the THDE with swampland correspondence in $f(R,T)$ gravity
• The DFSZ axion in the CMB
• Neutrino Echoes from Multimessenger Transient Sources
• Bounds on neutrino-scalar nonstandard interactions from big bang nucleosynthesis
• Cosmology with Standard Sirens at Cosmic Noon
• Classical Cepheid period-Wesenheit-metallicity relation in the Gaia bands
• Infrared Surface Brightness Fluctuation Distances for MASSIVE and Type Ia Supernova Host Galaxies
• The full Boltzmann hierarchy for dark matter-massive neutrino interactions
• Survey of Gravitationally-lensed Objects in HSC Imaging (SuGOHI). IV. Lensed quasar search in the HSC survey
• The Hubble constant from strongly lensed supernovae with standardizable magnifications
• The Zwicky Transient Facility Type Ia supernova survey: first data release and results
• A Bayesian comparison between $\Lambda$CDM and phenomenologically emergent dark energy models
• Interacting dark energy: clarifying the cosmological implications and viability conditions
• Self-interacting dark matter from late decays and the $H_0$ tension
• Scaling solutions and weak gravity in dark energy with energy and momentum couplings
• Constraining the Baryonic Feedback with Cosmic Shear Using the DES Year-3 Small-Scale Measurements
• Addressing $H_0$ tension with emergent dark radiation in unitary gravity
• Precision cosmology and the stiff-amplified gravitational-wave background from inflation: NANOGrav, Advanced LIGO-Virgo and the Hubble tension
• Hints of dark energy anisotropic stress using Machine Learning
• On Neural Architectures for Astronomical Time-series Classification with Application to Variable Stars
• Dynamical Dark sectors and Neutrino masses and abundances
• Limits on primordial non-Gaussianities from BOSS galaxy-clustering data
• One spectrum to cure them all: Signature from early Universe solves major anomalies and tensions in cosmology
• The growth rate of cosmic structures in the local Universe with the ALFALFA survey
• Early dark energy in $k$-essence
• Consistency of the local Hubble constant with the cosmic microwave background
• Strengthening the bound on the mass of the lightest neutrino with terrestrial and cosmological experiments
• The Cosmic Expansion History from Line-Intensity Mapping
• Testing Gravity on Cosmic Scales: A Case Study of Jordan-Brans-Dicke Theory
• 3\%-accurate predictions for the clustering of dark matter, haloes and subhaloes, over a wide range of cosmologies and scales
• $H_0$ tension and the String Swampland
• Gravitational-Wave Detector Networks: Standard Sirens on Cosmology and Modified Gravity Theory
• TDCOSMO. VII. Boxyness/discyness in lensing galaxies : Detectability and impact on $H_0$
• Dark energy interactions near the galactic centre
• Towards a model-independent reconstruction approach for late-time Hubble data
• A New Method to Measure Hubble Parameter $H(z)$ using Fast Radio Bursts
• Neutrino non-standard interactions meet precision measurements of $N_{\mathrm{eff}}$
• Metastable dark energy models in light of Planck 2018: Alleviating the $H_0$ tension
• Accuracy of environmental tracers and consequence for determining the Type Ia Supernovae magnitude step
• Prospect for constraining holographic dark energy with gravitational wave standard sirens from the Einstein Telescope
• TDCOSMO III: Dark matter substructure meets dark energy -- the effects of (sub)halos on strong-lensing measurements of $H_0$
• High-precision distance measurements with classical pulsating stars
• Solving the Hubble tension without spoiling Big Bang Nucleosynthesis
• X-ray Plateaus in Gamma-Ray Burst Afterglows and Their Application in Cosmology
• The minimally extended Varying Speed of Light (meVSL)
• Determining the Hubble Constant without the Sound Horizon: Perspectives with Future Galaxy Surveys
• Impacts of gravitational-wave standard siren observations from Einstein Telescope and Cosmic Explorer on weighing neutrinos in interacting dark energy models
• Late time acceleration due to generic modification of gravity and Hubble tension
• Unveiling the Intrinsic Alignment of Galaxies with Self-Calibration and DECaLS DR3 data
• Ruling Out New Physics at Low Redshift as a solution to the $H_0$ Tension
• Berkeley Supernova Ia Program: Data Release of 637 Spectra from 247 Type Ia Supernovae
• A data-driven Reconstruction of Horndeski gravity via the Gaussian processes
• Cosmic Birefringence Test of the Hubble Tension
• Carbon stars as standard candles: I. The luminosity function of carbon stars in the Magellanic Clouds
• Constraints on the transition redshift from the calibrated Gamma-ray Burst $E_{\mathrm{p}}$-$E_{\mathrm{iso}}$ correlation
• Testing dark energy models with a new sample of strong-lensing systems
• GALLUMI: A Galaxy Luminosity Function Pipeline for Cosmology and Astrophysics
• Observational constraints of the modified cosmology through Barrow entropy
• Over-constrained Models of Time Delay Lenses Redux: How the Angular Tail Wags the Radial Dog
• On the halo-mass and radial scale dependence of the lensing is low effect
• Cross-correlating dark sirens and galaxies: constraints on $H_0$ from GWTC-3 of LIGO-Virgo-KAGRA
• Using the Tip of the Red Giant Branch as a Distance Indicator in the Near Infrared
• Beware of commonly used approximations II: estimating systematic biases in the best-fit parameters
• Dynamical dark energy models in the light of Gravitational-Wave Transient Catalogues
• HOLISMOKES -- IV. Efficient mass modeling of strong lenses through deep learning
• Cosmology with varying fundamental constants from hyperlight, coupled scalars
• Current and future applications of Reverberation-mapped quasars in Cosmology
• Astrometric requirements for strong lensing time-delay cosmography
• Hubble parameter estimation via dark sirens with the LISA-Taiji network
• Reconciling Hubble Constant Discrepancy from Holographic Dark Energy
• Revisiting a non-parametric reconstruction of the deceleration parameter from combined background and the growth rate data
• Intrinsic tension in the supernova sector of the local Hubble constant measurement and its implications
• Running vacuum in QFT in FLRW spacetime: The dynamics of ${\rho }_{\mathrm{vac}}(H)$ from the quantized matter fields
• Axi-Higgs Cosmology
• The first simultaneous measurement of Hubble constant and post-Newtonian parameter from Time-Delay Strong Lensing
• Cosmology-independent Estimate of the Hubble Constant and Spatial Curvature Using Time-delay Lenses and Quasars
• Constraints on dark matter to dark radiation conversion in the late universe with DES-Y1 and external data
• Dynamical dark energy in the light of DESI 2024 data
• Quantifying Suspiciousness Within Correlated Data Sets
• Screening anisotropy via energy-momentum squared gravity: $\Lambda$CDM model with hidden anisotropy
• Screened Fifth Forces Mediated by Dark Matter-Baryon Interactions: Theory and Astrophysical Probes
• Investigating the Hubble Constant Tension -- Two Numbers in the Standard Cosmological Model
• The Chandra view of the relation between X-ray and UV emission in quasars
• Revisiting Metastable Dark Energy and Tensions in the Estimation of Cosmological Parameters
• Lensing-like tensions in the Planck legacy release
• Touch of Neutrinos on the Vacuum Metamorphosis: is the $H_0$ Solution Back?
• The Local Distance Network: a community consensus report on the measurement of the Hubble constant at 1% precision
• Free-streaming and Coupled Dark Radiation Isocurvature Perturbations: Constraints and Application to the Hubble Tension
• The Carnegie Chicago Hubble Program X: Tip of the Red Giant Branch Distances to NGC 5643 and NGC 1404
• Non-minimal geometry-matter couplings in Weyl-Cartan space-times: $f(R,T,Q,T_m)$ gravity
• A measurement of the CMB E-mode angular power spectrum at subdegree scales from 670 square degrees of POLARBEAR data
• Model-independent Distance Calibration and Curvature Measurement using Quasars and Cosmic Chronometers
• Varying fundamental constants principal component analysis: additional hints about the Hubble tension
• Reducing the $H_0$ tension with generalized Proca theory
• Hubble tension vs two flows
• Prospects for Measuring the Hubble Constant with Neutron-Star-Black-Hole Mergers
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• Cosmological perturbations in modified teleparallel gravity models: Boundary term extension
• New Graviton Mass Bound from Binary Pulsars
• A Generalized Interacting Tsallis Holographic Dark Energy Model and its thermodynamic implications
• A new way to explore cosmological tensions using gravitational waves and strong gravitational lensing
• The Hubble Tension, The $M$ Crisis of Late Time $H(z)$ Deformation Models and the Reconstruction of Quintessence Lagrangians
• Evidence for a high-z ISW signal from supervoids in the distribution of eBOSS quasars
• Peculiar velocities in the local Universe: comparison of different models and the implications for $H_0$ and dark matter
• Weak cosmic growth in coupled dark energy with a Lagrangian formulation
• Resolving Hubble Tension by Self-Interacting Neutrinos with Dirac Seesaw
• An extended theoretical scenario for Classical Cepheids. I. Modeling Galactic Cepheids in the Gaia photometric system
• Hubble tension bounds the GUP and EUP parameters
• A hint of matter underdensity at low $z$?
• Dark Energy Survey internal consistency tests of the joint cosmological probes analysis with posterior predictive distributions
• Dynamical systems methods and statefinder diagnostic of interacting vacuum energy models
• Impact of $H_0$ priors on $f(T)$ late time cosmology
• Dark sector interactions and the curvature of the Universe in light of Planck's 2018 data
• Dark energy and accelerating cosmological evolution from osculating Barthel-Kropina geometry
• Constraining the curvature density parameter in cosmology
• Testing dark energy after pre-recombination early dark energy
• Minimally Modified Gravity fitting Planck data better than $\Lambda$CDM
• Toward a concordance teleparallel Cosmology I: Background Dynamics
• No-go guide for late-time solutions to the Hubble tension: Matter perturbations
• Astrophysical Distance Scale II. Application of the JAGB Method: A Nearby Galaxy Sample
• HOLISMOKES -- III. Achromatic Phase of Strongly Lensed Type Ia Supernovae
• No H_0 Assistance from Assisted Quintessence
• The Iron Yield of Normal Type II Supernovae
• Cosmology With Low-Redshift Observations: No Signal For New Physics
• A new coupled three-form dark energy model and implications for the $H_0$ tension
• Reconstruction of the dark sectors' interaction: A model-independent inference and forecast from GW standard sirens
• Exploration of interacting dynamical dark energy model with interaction term including the equation-of-state parameter: alleviation of the $H_0$ tension
• A Dark Matter Trigger for Early Dark Energy Coincidence
• Hubble tension in lepton asymmetric cosmology with an extra radiation
• Fitting string inflation to real cosmological data: the Fibre Inflation case
• $H_0$ Ex Machina: Vacuum Metamorphosis and Beyond $H_0$
• Dark Matter Halos in Interacting Dark Energy Models: Formation History, Density Profile, Spin and Shape
• Dynamical analysis of cosmological models with non-Abelian gauge vector fields
• MOG cosmology without dark matter and the cosmological constant
• Stability of scalar perturbations in scalar-torsion $f(T,\varphi )$ gravity theories in the presence of a matter fluid
• Effects of Supernova Redshift Uncertainties on the Determination of Cosmological Parameters
• Relativistic SZ temperature scaling relations of groups and clusters derived from the BAHAMAS and MACSIS simulations
• An updated measurement of the Hubble constant from near-infrared observations of Type Ia supernovae
• Luminosity distance and anisotropic sky-sampling at low redshifts: a numerical relativity study
• Entropic corrections to Friedmann equations and bouncing universe due to the zero-point length
• Hubble tension as a guide for refining the early Universe: Cosmologies with explicit local Lorentz and diffeomorphism violation
• Constraining early dark energy with gravitational waves before recombination
• Evolutionary tracks, ejecta, and ionizing photons from intermediate-mass to very massive stars with PARSEC
• Sterile Neutrino Searches with MicroBooNE: Electron Neutrino Disappearance
• Nonlocal gravity and gravitational-wave observations
• On cosmological signatures of baryons-dark energy elastic couplings
• The Twins Embedding of Type Ia Supernovae II: Improving Cosmological Distance Estimates
• GIGA-Lens: Fast Bayesian Inference for Strong Gravitational Lens Modeling
• Constraints on $f(T)$ Cosmology with Pantheon+
• Exploiting the Einstein Telescope to solve the Hubble tension
• Observational constraints and predictions of the interacting dark sector with field-fluid mapping
• Proca in the sky
• Multimessenger parameter estimation of GW170817: from jet structure to the Hubble constant
• Observational Constraints on $f(T)$ Gravity from Model-Independent Data
• Sources of $H_0$-tensions in dark energy scenarios
• The Astrophysical Distance Scale III: Distance to the Local Group Galaxy WLM using Multi-Wavelength Observations of the Tip of the Red Giant Branch, Cepheids, and JAGB Stars
• The ASKAP-EMU Early Science Project: 888 MHz Radio Continuum Survey of the Large Magellanic Cloud
• Observational constraints on Tsallis modified gravity
• SN 2021zny: an early flux excess combined with late-time oxygen emission suggests a double white dwarf merger event
• Latest evidence for a late time vacuum -- geodesic CDM interaction
• An exploration of an early gravity transition in light of cosmological tensions
• Dark Energy as a Critical Phenomenon: a Resolution for Hubble Tension
• Determination of the Local Hubble Constant from Virgo Infall Using TRGB Distances
• DES Y1 results: Splitting growth and geometry to test $\Lambda$CDM
• Evolutionary and pulsation properties of Type II Cepheids
• Neutrino Masses and Hubble Tension via a Majoron in MFV
• Linear Point and Sound Horizon as Purely Geometric standard rulers
• Backreaction in Cosmology
• Revisiting Fractional Cosmology
• Testing the violation of the equivalence principle in the electromagnetic sector and its consequences in $f(T)$ gravity
• Cosmicflows-4: The Baryonic Tully-Fisher Relation Providing ~10,000 Distances
• Gravitationally induced particle production in scalar-tensor $f(R,T)$ gravity
• A thin shell of ionized gas explaining the IR excess of classical Cepheids
• Inflation Wars: A New Hope
• Studying Type II supernovae as cosmological standard candles using the Dark Energy Survey
• Saez-Ballester gravity in Kantowski-Sachs Universe: a new reconstruction paradigm for Barrow Holographic Dark Energy
• Study of changes in the pulsation period of 148 Galactic Cepheid variables
• Sterile Neutrino Shape-shifting Caused by Dark Matter
• Dark energy by natural evolution: Constraining dark energy using Approximate Bayesian Computation
• RR Lyrae-based Distances for 39 Nearby Dwarf Galaxies Calibrated to Gaia eDR3
• On the Period--Luminosity--Metallicity relation of Classical Cepheids
• Exploring late-time cosmic acceleration: A study of a linear $f(T)$ cosmological model using observational data
• Constraining the dark-energy equation of state with cosmological data
• A new cosmological probe using super-massive black hole shadows
• Recent advances in cosmological singularities
• Luminosity distribution of Type II supernova progenitors
• Revising the Hubble constant, spatial curvature and dark energy dynamics with the latest observations of quasars
• Do the observational data favor a local void?
• Connecting Infrared Surface Brightness Fluctuation Distances to Type Ia Supernova Hosts: Testing the Top Rung of the Distance Ladder
• Using the cosmological recombination radiation to probe early dark energy and fundamental constant variations
• VLT/MUSE observations of SDSS J1029+2623: towards a high-precision strong lensing model
• A new and homogeneous metallicity scale for Galactic classical Cepheids II. The abundance of iron and alpha elements
• Classification of Teleparallel Horndeski Cosmology via Noether Symmetries
• On the (Lack of) Evolution of the Stellar Mass Function of Massive Galaxies from $z$=1.5 to 0.4
• Prospects for constraining interacting dark energy models from gravitational wave and gamma ray burst joint observation
• Can varying the gravitational constant alleviate the tensions ?
• Thermal Friction as a Solution to the Hubble and Large-Scale Structure Tensions
• Light gravitino dark matter: LHC searches and Hubble tension
• Velocity-dependent interacting dark energy and dark matter with a Lagrangian description of perfect fluids
• Observational constraints on Starobinsky $f(R)$ cosmology from cosmic expansion and structure growth data
• Gravitational wave populations and cosmology with neural posterior estimation
• Revisiting the Hubble constant, spatial curvature and cosmography with time-delay and cosmic chronometer observations
• Possible Hints of Sterile Neutrinos in Recent Measurements of the Hubble Parameter
• Superpotential method for chiral cosmological models connected with modified gravity
• Minimal theory of massive gravity in the light of CMB data and the $S_8$ tension
• A forecast of using fast radio burst observations to constrain holographic dark energy
• Constraining the Evolution of the Baryon Fraction in the IGM with FRB and H(z) data
• Modeling of accelerating Universe with bulk viscous fluid in Bianchi V space-time
• Neural Network Reconstruction of $H^{\prime }(z)$ and its application in Teleparallel Gravity
• A Cosmological Underdensity Does Not Solve the Hubble Tension
• Current Challenges in Cepheid Distance Calibrations Using Gaia EDR3
• Inflation model selection revisited after a 1.91% measurement of the Hubble constant
• Metallicities from high resolution spectra of 49 RR Lyrae Variables
• Hot thermal universe endowed with massive dark vector fields and the Hubble tension
• General formulation of cosmological perturbations in scalar-tensor dark energy coupled to dark matter
• Inspecting the Cepheid distance ladder: The Hubble Space Telescope distance to the SNIa host galaxy NGC 5584
• Implications of an extended dark energy model with massive neutrinos
• Massive neutrino self-interactions with a light mediator in cosmology
• Augmenting astrophysical scaling relations with machine learning: application to reducing the Sunyaev-Zeldovich flux-mass scatter
• Growth of matter perturbations in the extended viscous dark energy models
• Peculiar motion of Solar system from the Hubble diagram of supernovae Ia and its implications for cosmology
• Addressing the Hubble and $S_8$ Tensions with a Kinetically Mixed Dark Sector
• Diffusion in unimodular gravity: Analytical solutions, late-time acceleration, and cosmological constraints
• Sky localization of space-based gravitational wave detectors
• Carbon stars as standard candles: II. The median J magnitude as a distance indicator
• On the separation between RR Lyrae and Type II Cepheids and their importance for distance determination: the case of $\omega$ Cen
• Debiasing Cosmic Gravitational Wave Sirens
• Cosmological constraints on Hořava gravity revised in light of GW170817 and GRB170817A and the degeneracy with massive neutrinos
• Low-redshift estimates of the absolute scale of baryon acoustic oscillations
• Testing modified gravity via Yukawa potential in two body problem: Analytical solution and observational constraints
• Exact solutions and cosmological constraints in fractional cosmology
• The Scale-Invariant Vacuum (SIV) Theory: A Possible Origin of Dark Matter and Dark Energy
• When a Period Is Not a Full Stop: Light Curve Structure Reveals Fundamental Parameters of Cepheid and RR Lyrae Stars
• Reaffirming the Cosmic Acceleration without Supernova and CMB
• Multiwavelength Period-Luminosity and Period-Luminosity-Color relations at maximum-light for Mira variables in the Magellanic Clouds
• Next generation design and prospects for CANNEX
• The BINGO Project VII: Cosmological Forecasts from 21cm Intensity Mapping
• Minimal theory of massive gravity and constraints on the graviton mass
• Observational Constraints on Dynamical Dark Energy Models
• Cepheids with giant companions. I. Revealing a numerous population of double-lined binary Cepheids
• Linear stability of black holes with static scalar hair in full Horndeski theories: generic instabilities and surviving models
• Alleviating $H_0$ Tension with New Gravitational Scalar Tensor Theories
• Decaying dark matter, the $H_0$ tension, and the lithium problem
• Cepheid Metallicity in the Leavitt Law (C- MetaLL) survey: II.High-resolution spectroscopy of the most metal poor Galactic Cepheids
• Weakening gravity for dark matter in a type-II minimally modified gravity
• Super-CMB fluctuations and the Hubble tension
• Can the quantum vacuum fluctuations really solve the cosmological constant problem?
• Galaxy-Scale Test of General Relativity with Strong Gravitational Lensing
• Phantom-like dark energy from quantum gravity
• Consequences of the lack of azimuthal freedom in the modeling of lensing galaxies
• The phantom dark matter halos of the Local Volume in the context of modified Newtonian dynamics
• The ultraluminous X-ray source bubble in NGC 5585
• Detecting the power spectrum turnover with HI intensity mapping
• Phantom braneworld and the Hubble tension
• Analysing the spectral energy distributions of Galactic classical Cepheids
• Quintessential inflation and cosmological seesaw Mechanism: reheating and observational constraints
• Fractional Holographic Dark Energy
• Cosmological Constraints on Non-flat Exponential $f(R)$ Gravity
• Hubble constant difference between CMB lensing and BAO measurements
• Multiple measurements of quasars acting as standard probes: model independent calibration and exploring the Dark Energy Equation of States
• Impacts of dark energy on constraining neutrino mass after Planck 2018
• An improved Tully-Fisher estimate of $H_0$
• Testing generalized logotropic models with cosmic growth
• Quintessential Cosmological Tensions
• Multiband gravitational wave cosmology with stellar origin black hole binaries
• No-go guide for the Hubble tension: late-time or local-scale new physics
• Current constraints on deviations from General Relativity using binning in redshift and scale
• Cosmological model-independent measurement of cosmic curvature using distance sum rule with the help of gravitational waves
• On Zero Point Calibration of the Red Giant Branch Tip in the Magellanic Clouds
• Viable Gauge Choices in Cosmologies with Non-Linear Structures
• TDCOSMO VI: Distance Measurements in Time-delay Cosmography under the Mass-sheet transformation
• Model-independent Estimations for the Cosmic Curvature from the Latest Strong Gravitational Lensing Systems
• 4D Gauss-Bonnet gravity: cosmological constraints, $H_0$ tension and large scale structure
• Organised Randoms: Learning and correcting for systematic galaxy clustering patterns in KiDS using self-organising maps
• Alleviating $H_0$ tension in Horndeski gravity
• Dynamical systems analysis of tachyon dark energy model from a new perspective
• HOLISMOKES -- VII. Time-delay measurement of strongly lensed Type Ia supernovae using machine learning
• Consequences of neutrino self interactions for weak decoupling and big bang nucleosynthesis
• New constraints on the mass bias of galaxy clusters from the power spectra of the thermal Sunyaev-Zeldovich effect and cosmic shear
• First Identification of a CMB Lensing Signal Produced by $1.5$ Million Galaxies at $z\sim$4: Constraints on Matter Density Fluctuations at High Redshift
• Coupled Multi-Proca Vector Dark Energy
• The Hubble constant tension with next-generation galaxy surveys
• Easing cosmic tensions with an open and hotter universe
• Qualitative Stability Analysis of Cosmological Parameters in $f(T,B)$ Gravity
• Hubble constant and sound horizon from the late-time Universe
• Late-time acceleration with a scalar field source: Observational constraints and statefinder diagnostics
• Testing f(R) gravity models with quasar X-ray and UV fluxes
• Analyzing the Hubble tension through hidden sector dynamics in the early universe
• J-PAS: forecasts on interacting vacuum energy models
• A gravitational constant transition within cepheids as supernovae calibrators can solve the Hubble tension
• The Twins Embedding of Type Ia Supernovae I: The Diversity of Spectra at Maximum Light
• A model independent comparison of supernova and strong lensing cosmography: implications for the Hubble constant tension
• Suppressed cosmic growth in coupled vector-tensor theories
• Resolving the Hubble tension in a U(1)${}_{L_{\mu }-L_{\tau }}$ model with Majoron
• Three open clusters containing Cepheids: NGC 6649, NGC 6664 and Berkeley 55
• A Measurement of the Hubble Constant using Gravitational Waves from the Binary Merger GW190814
• Anisotropic solid dark energy
• Revisiting Chaplygin gas cosmologies with the recent observations of high-redshfit quasars
• Viscous cosmology in $f(T)$ gravity
• High Redshift Long Gamma-Ray Bursts Hubble Diagram as a Test of Basic Cosmological Relations
• A Linear Formation Flying Astronomical Interferometer in Low Earth Orbit
• Constraining the Source of the High-velocity Ejecta in Type Ia SN 2019ein
• Flavour specific neutrino self-interaction: $H_0$ tension and IceCube
• The case for a Casimir cosmology
• Alleviating Cosmological Tensions with a Coupled Scalar Fields Model
• Constraints on neutrino mass in the scenario of vacuum energy interacting with cold dark matter after Planck 2018
• The cosmic neutrino background as a collection of fluids in large-scale structure simulations
• Investigating Dark Energy Equation of State With High Redshift Hubble Diagram
• Photometric Classification of Early-Time Supernova Lightcurves with SCONE
• Cascading Dark Energy
• Measuring $H_0$ using X-ray and SZ effect observations of dynamically relaxed galaxy clusters
• Kinematic Constraints on Spatial Curvature from Supernovae Ia and Cosmic Chronometers
• Hubble tension and absolute constraints on the local Hubble parameter
• Redshift drift cosmography for model-independent cosmological inference
• Constraints on Newton's Constant from Cosmological Observations
• A Dark Energy model from Generalized Proca Theory
• Cosmological discordances III: more on measure properties, Large-Scale-Structure constraints, the Hubble constant and Planck
• A testable hidden-sector model for Dark Matter and neutrino masses
• A common explanation of the Hubble tension and anomalous cold spots in the CMB
• Thermal Dark Energy
• The Carnegie Chicago Hubble Program VI: Tip of the Red Giant Branch Distances to M66 and M96 of the Leo I Group
• Cosmological search for sterile neutrinos after Planck 2018
• Completeness of the Gaia-verse V: Astrometry and Radial Velocity sample selection functions in Gaia EDR3
• On the Use of Field RR Lyrae as Galactic Probes. V. Optical and radial velocity curve templates
• Implications of a frame dependent dark energy for the spacetime metric, cosmography, and effective Hubble constant
• Updated theoretical Period-Age and Period-Age-Color relations for Galactic Classical Cepheids: an application to the Gaia DR2 sample
• Spatial Curvature in $f(R)$ Gravity
• Charged strange star coupled to anisotropic dark energy in Tolman-Kuchowicz spacetime
• Absolute Calibration of Cepheid Period-Luminosity Relations in NGC 4258
• Running vacuum versus Holographic dark energy: a cosmographic comparison
• The redshift dependence of the inferred $H_0$ in a local void solution to the Hubble tension
• Dynamical system analysis of scalar field cosmology in coincident $f(Q)$ gravity
• Environmental processing in cluster core galaxies at z=1.7
• The impact of line-of-sight structures on measuring $H_0$ with strong lensing time-delays
• Shedding Light on Dark Matter and Neutrino Interactions from Cosmology
• Hydrodynamical structure formation in Milgromian cosmology
• The Cepheid Distance to the Narrow-Line Seyfert 1 Galaxy NGC 4051
• IDECAMB: an implementation of interacting dark energy cosmology in CAMB
• Does non-stationary noise in LIGO and Virgo affect the estimation of $H_0$?
• Holographic dark energy in Rastall theory
• Constraining Dark Energy from Local Group dynamics
• Galaxy-lens determination of $H_0$: constraining density slope in the context of the mass sheet degeneracy
• Impact of symmetron screening on the Hubble tension: new constraints using cosmic distance ladder data
• Binary white dwarfs and decihertz gravitational wave observations: From the Hubble constant to supernova astrophysics
• Ultra-light axions and the kinetic Sunyaev-Zel'dovich Effect
• Cosmology with the sub-millimetre galaxies magnification bias: Tomographic Analysis
• Cosmological Perturbation Theory in Metric-Affine Gravity
• The Heisenberg limit at cosmological scales
• HOLISMOKES -- V. Microlensing of type II supernovae and time-delay inference through spectroscopic phase retrieval
• Oscillating dark energy in light of the latest observations and its impact on the Hubble tension
• Strongly lensed type Ia supernovae as a precise late-universe probe of measuring the Hubble constant and cosmic curvature
• Identification of Galaxy-Galaxy Strong Lens Candidates in the DECam Local Volume Exploration Survey Using Machine Learning
• Pseudoscalar sterile neutrino self-interactions in light of Planck, SPT and ACT data
• Resonant neutrino self-interactions and the $H_0$ tension
• On the Lambda-evolution of galaxy clusters
• The simplest parametrization of equation of state parameter in the scalar field Universe
• Consistent extinction model for type Ia supernovae in Cepheid-based calibration galaxies and its impact on $H_0$
• The BAHAMAS project: Effects of dynamical dark energy on large-scale structure
• Structure growth in $f(Q)$ cosmology
• Constraining Dark-Matter Ensembles with Supernova Data
• Cosmology from weak lensing alone and implications for the Hubble tension
• A critical discussion on the $H_0$ tension
• Combining cosmological and local bounds on bimetric theory
• Can the Hubble tension be resolved by bulk viscosity?
• A 4% measurement of $H_0$ using the cumulative distribution of strong-lensing time delays in doubly-imaged quasars
• Accounting for object detection bias in weak gravitational lensing studies
• Can $f(R)$ gravity relieve $H_0$ and ${\sigma }_8$ tensions?
• Prospects for multi-messenger extended emission from core-collapse supernovae in the Local Universe
• On the Color-Metallicity Relation of the Red Clump and the Reddening Toward the Magellanic Clouds
• Tully-Fisher Distances and Dynamical Mass Constraints for 24 Host Galaxies of Reverberation-Mapped AGN
• Scalar-Tensor Gravity and DESI 2024 BAO data
• Reconstructing Quintessence
• Theoretical and numerical perspectives on cosmic distance averages
• Cosmological constraints with the sub-millimetre galaxies Magnification Bias after large scale bias corrections
• Cosmological evolution with quadratic gravity and nonideal fluids
• Using 1991T/1999aa-like Type Ia Supernovae as Standardizable Candles
• Phase space analysis of the bouncing universe with stringy effects
• Noether Symmetry Approach in Scalar-Torsion $f(T,\varphi )$ Gravity
• Numerical solutions to Einstein's equations in a shearing-dust Universe: a code comparison
• Phenomenological Gravitational Phase Transition: Early and Late Modifications
• Cosmic expansion with matter creation and bulk viscosity
• Phenomenological Gravitational Phase Transition: Reconciliation between the Late and Early Universe
• The Exotic Type Ic Broad-Lined Supernova SN 2018gep: Blurring the Line Between Supernovae and Fast Optical Transients
• The Spectrum of Dark Radiation as a Probe of Reheating
• Breaking cosmic degeneracies: Disentangling neutrinos and modified gravity with kinematic information
• Observational constraints on the interacting dark energy - dark matter (IDM) cosmological models
• Relativistic corrections for measuring Hubble's constant to 1% using stellar standard candles
• Ghost and Laplacian Instabilities in the Teleparallel Horndeski Gravity
• Unitarity at the Late time Boundary of de Sitter
• On using inspiralling supermassive binary black holes in the PTA frequency band as standard sirens to constrain dark energy
• When tension is just a fluctuation: How noisy data affect model comparison
• Lanczos potential of Weyl field: interpretations and applications
• An exponential equation of state of dark energy in the light of 2018 CMB Planck data
• Stringent Pulsar Timing Bounds on Light Scalar Couplings to Matter
• The potential role of binary neutron star merger afterglows in multimessenger cosmology
• Modelling time delays from two reprocessors in active galactic nuclei
• HOLISMOKES -- IX. Neural network inference of strong-lens parameters and uncertainties from ground-based images
• The Halo Spin Transition as a Probe of Dark Energy
• Probing the Seesaw Mechanism with Cosmological Data
• Electron mass variation from dark sector interactions and compatibility with cosmological observations
• Baryon Acoustic Oscillations in the projected cross-correlation function between the eBOSS DR16 quasars and photometric galaxies from the DESI Legacy Imaging Surveys
• The SRG-eROSITA All-Sky Survey : Constraints on f(R) Gravity from Cluster Abundance
• A cosmic glitch in gravity
• Neutrino masses from large-scale structures: future sensitivity and theory dependence
• Updating constraints on phantom crossing $f(T)$ gravity
• Parameter estimation of eccentric gravitational waves with a decihertz observatory and its cosmological implications
• Prospects of Searching for Type Ia Supernovae with 2.5-m Wide Field Survey Telescope
• Differentiating dark interactions with perturbation
• Cosmological forecasts with the clustering of weak lensing peaks
• A Model-independent Method to Determine $H_0$ Using Time-Delay Lensing, Quasars and Type Ia Supernovae
• Open clusters housing classical Cepheids in Gaia DR3
• Model-independent $H_0$ within FLRW: Joint constraints from GWTC-3 standard sirens and strong lensing time delays
• Cosmology with the submillimetre galaxies magnification bias: Proof of concept
• Cuscuta-Galileon cosmology: Dynamics, gravitational "constant"s and the Hubble Constant
• Forecasts on interacting dark energy with standard sirens
• Designing an Optimal LSST Deep Drilling Program for Cosmology with Type Ia Supernovae
• Constraints on new physics around the MeV scale with cosmological observations
• Radiative stability and observational constraints on dark energy and modified gravity
• Probing Beyond the Standard Model Physics with Double-beta Decays
• Cosmological bound on neutrino masses in the light of $H_0$ tension
• Supernova Siblings and their Parent Galaxies in the Zwicky Transient Facility Bright Transient Surve
• The Legacy of Einstein's Eclipse, Gravitational Lensing
• Growth of structures using redshift space distortion in $f(T)$ Cosmology
• Can decaying dark matter scenarios alleviate both $H_0$ and ${\sigma }_8$ tensions?
• Deconstructing the Planck TT Power Spectrum to Constrain Deviations from $\Lambda$CDM
• The stellar photosphere-hydrogen ionization front interaction in Classical Pulsators: a theoretical explanation for observed period-colour relations
• Reproductive Freeze-In of Self-Interacting Dark Matter
• Hidden Monopole Dark Matter via Axion Portal and its Implications for Direct Detection Searches, Beam-Dump Experiments, and the $H_0$ Tension
• Cosmological Probes of Structure Growth and Tests of Gravity
• Cosmic Growth in $f(T)$ Teleparallel Gravity
• SN 2018agk: A Prototypical Type Ia Supernova with a Smooth Power-law Rise in Kepler (K2)
• The effects of peculiar velocities in SN Ia environments on the local $H_0$ measurement
• Galaxy-lens determination of $H_0$: the effect of the ellipse+shear modeling assumption
• A Critique of the Spite Plateau, and the Astration of Primordial Lithium
• Interstellar communication network. I. Overview and assumptions
• The Spin Tensor of Dark Matter and the Hubble Parameter Tension
• Dark Lepton Superfluid in Proto-Neutron Stars
• SN 2017cfd: A Normal Type Ia Supernova Discovered Very Young
• Constraints from High-Precision Measurements of the Cosmic Microwave Background: The Case of Disintegrating Dark Matter with $\Lambda$ or Dynamical Dark Energy
• Discovering strongly lensed quasar candidates with catalogue-based methods from DESI Legacy Surveys
• Prospects of strongly lensed fast radio bursts: Simultaneous measurement of post-Newtonian parameter and Hubble constant
• A Preliminary Calibration of the JAGB Method Using Gaia EDR3
• Low-redshift measurement of the sound horizon through gravitational time-delays
• Investigating dark energy by electromagnetic frequency shifts
• Model-Independent Determination of $H_0$ and ${\Omega }_{K,0}$ using Time-Delay Galaxy Lenses and Gamma-Ray Bursts
• Optical follow-up of gravitational wave triggers with DECam during the first two LIGO/VIRGO observing runs
• The RayGalGroupSims cosmological simulation suite for the study of relativistic effects: an application to lensing-matter clustering statistics
• The Effect of Systematic Redshift Biases in BAO Cosmology
• A Sample of Dust Attenuation Laws for DES Supernova Host Galaxies
• A novel method of measuring cosmological distances using broad-line regions of quasars
• Constraining Cosmological and Galaxy Parameters using Strong Gravitational Lensing Systems
• The intrinsic reddening of the Magellanic Clouds as traced by background galaxies -- II. The Small Magellanic Cloud
• Early Dark Energy from a Higher-dimensional Gauge Theory
• A Cepheid-Based Distance to the Seyfert Galaxy NGC 6814
• Axion Dark Radiation: Hubble Tension and Hyper-kamiokande Neutrino Experiment
• A GREAT model comparison against the cosmological constant
• Measuring the speed of light with updated Hubble diagram of high-redshift standard candles
• $H_0$ tension without CMB data: beyond the $\Lambda$CDM
• Apparent dark matter as a non-local manifestation of emergent gravity
• Constraints on interacting dark energy revisited: implications for the Hubble tension
• The Integrated Sachs-Wolfe Effect in Interacting Dark Matter-Dark Energy Models
• A single parameterization for dark energy and modified gravity models
• Hubble tensions: a historical statistical analysis
• Generalized Brans-Dicke theories in light of evolving dark energy
• Reducing the $H_0$ Tension with Exponential Acoustic Dark Energy
• Finding Multiply-Lensed and Binary Quasars in the DESI Legacy Imaging Surveys
• Mapping Poincaré gauge cosmology to Horndeski theory for emergent dark energy
• Identifying lensed quasars and measuring their time-delays from unresolved light curves
• Unphysical properties in a class of interacting dark energy models
• Sensitivity reach of gamma-ray measurements for strong cosmological magnetic fields
• Noether Symmetries in $f(T,T_G)$ Cosmology
• A new Parametrization for Bulk Viscosity Cosmology as Extension of the $\Lambda$CDM Model
• An FLRW interacting dark energy model of the Universe
• Reeling in the Whirlpool: the distance to M 51 clarified by Cepheids and the Type IIP SN 2005cs
• Using machine learning to compress the matter transfer function $T(k)$
• Hubble distancing: Focusing on distance measurements in cosmology
• Dynamics of interacting scalar field model in the realm of chiral cosmology
• Discrepancy between cosmological and electroweak observables in Higgs Inflation
• Charged Dark Matter and the $H_0$ tension
• Discovering Strongly-lensed QSOs From Unresolved Light Curves
• Constraining properties of neutron star merger outflows with radio observations
• The impact of mass map truncation on strong lensing simulations
• Calibrating the cosmic distance ladder using gravitational-wave observations
• A low Hubble Constant from galaxy distribution observations
• An estimate of the dark matter density from galaxy clusters and supernovae data
• Frequency analysis of OGLE-IV photometry for classical Cepheids in Galactic fields: non-radial modes and modulations
• Cosmological study of a symmetric teleparallel gravity model
• Stability analysis of warm quintessential dark energy model
• Reconstructing a non-linear interaction in the dark sector with cosmological observations
• Cosmological constraints of Palatini $f(\mathcal{R})$ gravity
• Cosmological Parameter Estimation Using Current and Future Observations of Strong Gravitational Lensing
• The Hubble tension: Change in dark energy or a case for modified gravity?
• Robust Limits from Upcoming Neutrino Telescopes and Implications on Minimal Dark Matter Models
• Model-independent way to determine the Hubble constant and the curvature from phase shift of gravitational waves with DECIGO
• Manifesting hidden dynamics of a sub-component dark matter
• Exploring cosmological evolution and constraints in $f(T)$ teleparallel gravity
• Baryonic feedback measurement from KV450 cosmic shear analysis
• Holographic energy density, dark energy sound speed, and tensions in cosmological parameters: $H_0$ and $S_8$
• Multipole expansion for 21cm Intensity Mapping power spectrum: forecasted cosmological parameters estimation for the SKA Observatory
• Using Gravitational Wave Parallax to Measure the Hubble Parameter with Pulsar Timing Arrays
• Cosmological constraints on time-varying cosmological terms: A study of FLRW universe models with $\Lambda (t)$CDM cosmology
• Is gravity getting weaker at low z? Observational evidence and theoretical implications
• Dynamics and statefinder analysis of a class of sign-changeable interacting dark energy scenarios
• Non-thermal neutrino-like hot dark matter in light of the $S_8$ tension
• Constraints on the electron-to-proton mass ratio variation at the epoch of reionization
• Cosmological model-independent constraints on the baryon fraction in the IGM from fast radio bursts and supernovae data
• Beyond optical depth: Future determination of ionization history from the CMB
• Dark energy loopholes some time after GW170817
• Study of a viscous $\Lambda$WDM model: Near equilibrium condition, entropy production, and cosmological constraints
• Constraining a possible time-variation of the speed of light along with the fine-structure constant using strong gravitational lensing and Type Ia supernovae observations
• Empirical inference on the Majorana mass of the ordinary neutrinos
• Probing self-interacting sterile neutrino dark matter with the diffuse supernova neutrino background
• Observational constraints on varying fundamental constants in a minimal CPC model
• Band-limited Features in the Primordial Power Spectrum Do Not Resolve the Hubble Tension
• Joint Constraints on the Hubble Constant, Spatial Curvature, and Sound Horizon from the Late-time Universe with Cosmography
• Constraining the emergent dark energy models with observational data at intermediate redshift
• Geodesic Congruences and a Collapsing Stellar Distribution in f (T ) Theories
• The New SI and the Fundamental Constants of Nature
• Casimir Self-Interaction Energy Density of Quantum Electrodynamic Fields
• Measuring the Hubble constant from the cooling of the CMB monopole
• Distances to Local Group Galaxies via Population II, Stellar Distance Indicators. II. The Fornax Dwarf Spheroidal
• Variation of dust properties with cosmic time implied by radiative torque disruption
• Spatial curvature sensitivity to local $H_0$ from the Cepheid distance ladder
• Potential biases and prospects for the Hubble constant estimation via electromagnetic and gravitational-wave joint analyses
• Probing alternative cosmologies through the inverse distance ladder
• The local dark sector. Probing gravitation's low-acceleration frontier and dark matter in the Solar System neighborhood
• A tower of hidden sectors: a general treatment and physics implications
• Is "Dark Energy" a Quantum Vacuum Energy?
• A visual tool for assessing tension-resolving models in the $H_0$-${\sigma }_8$ plane
• Observational constraints on the fractal cosmology
• Quantum origin of dark energy and the Hubble tension
• Pseudo-Evolution of Galaxies in LCDM Cosmology
• Torsion driving cosmic expansion
• Metallicity estimation of MW, SMC and LMC classical Cepheids from the shape of the $V$- and $I$-band light curves
• Accuracy of estimation of parameters with space-borne gravitational wave observatory
• Holographic dark energy in Barrow cosmology with Granda-Oliveros IR cutoff
• Molecular gas in distant brightest cluster galaxies
• An Anisotropic Model for the Universe
• Towards a Solution to the H0 Tension: the Price to Pay
• CMB lensing in a modified $\Lambda$CDM model in light of the $H_0$ tension
• Testing the growth rate in homogeneous and inhomogeneous interacting vacuum models
• Einstein-Vlasov Calculations of Structure Formation
• Tsallis holographic dark energy with power law ansatz approach
• Fractional Einstein-Gauss-Bonnet scalar field cosmology
• Towards detecting super-GeV dark matter via annihilation to neutrinos
• Shan--Chen interacting vacuum cosmology
• Cosmological Distances And Hubble Tension In Einstein-Cartan Theory
• Resolving Hubble tension with the Milne model
• On the question of measuring spatial curvature in an inhomogeneous universe
• Investigating dark energy by electromagnetic frequency shifts II: the Pantheon+ sample
• Constraining Holographic Dark Energy and Analyzing Cosmological Tensions
• Dissecting kinetically coupled quintessence: phenomenology and observational tests
• A study on Cubic Galileon Gravity Using N-body Simulations
• Stochastic gravitational wave background: birth from string-wall death
• Anthropic Bound on Dark Radiation and its Implications for Reheating
• Possible Resolution of the Hubble Tension with Weyl Invariant Gravity
• Quantum Discrete Levels of the Universe from the Early Trans-Planckian Vacuum to the Late Dark Energy
• Interacting dark sector: a dynamical system perspective
• Will Gravitational Wave Sirens Determine the Hubble Constant?
• The bulk flow motion and the Hubble-Lema\^ıtre law in the Local Universe with the ALFALFA survey
• A study of interacting scalar field model from the perspective of the dynamical systems theory
• Viewing angle observations and effects of evolution with redshift, black hole mass, and Eddington ratio in quasar based cosmology
• On The Distribution of Bayesian Evidences
• The Hubble tension in the non-flat Super-$\Lambda \mathrm{CDM}$ model
• Reply to: Overconfidence in Bayesian analyses of galaxy rotation curves
• Self-interacting neutrinos, the Hubble parameter tension, and the Cosmic Microwave Background
• Late-time acceleration by a residual cosmological constant from sequestering vacuum energy in ultimate collapsed structures
• Source localizations with the network of space-based gravitational wave detectors
• Model-Independent Perspectives on Coupled Dark Energy and the Swampland
• A segmented period-luminosity relation for nearby extragalactic $\delta$ Scuti stars
• Lessons from the first multiply imaged supernova II: A parametric strong-lensing model for the galaxy cluster MACS J1149.5+2223
• Probing cosmic anisotropy with GW/FRB as upgraded standard sirens
• Constraining deviations from $\Lambda$CDM in the Hubble expansion rate
• Observational constraints in Delta Gravity: CMB and supernovas
• Cosmological framework for renormalization group extended gravity at the action level
• SEEDisCS I. Molecular gas in galaxy clusters and their large scale structure: the case of CL1411.1$-$1148 at $z\sim 0.5$
• Coupled dark energy model inspired from general conformal transformation
• Investigating the Hubble Tension: Effect of Cepheid Calibration
• Scaling solutions as Early Dark Energy resolutions to the Hubble tension
• Constraining cosmological parameters from strong lensing with DECIGO and B-DECIGO sources
• Dark-siren Cosmology with Decihertz Gravitational-wave Detectors
• Prospects of calibrating afterglow modeling of short GRBs with gravitational wave inclination angle measurements and resolving the Hubble tension with a GW-GRB association event
• The role of $T_0$ in CMB anisotropy measurements
• Dark Matter Cosmology with Varying Viscosity: a Possible Resolution to the $S_8$ Tension
• Cosmological constraints with the Effective Fluid approach for Modified Gravity
• Relic Neutrino Degeneracies and Their Impact on Cosmological Parameters
• Cosmological Fisher forecasts for next-generation spectroscopic surveys
• A study of Si II and S II features in spectra of Type Ia supernova
• 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
• Dark Energy From Dynamical Projective Connections
• N-body simulations, halo mass functions, and halo density profile in $f(T)$ gravity
• Towards a 1% Measurement of the Hubble Constant: Accounting for Time Dilation in Variable Star Light Curves
• Searching for local features in primordial power spectrum using genetic algorithms
• The Logotropic Dark Fluid: Observational and Thermodynamic Constraints
• A Standard Siren Cosmological Measurement from the Potential GW190521 Electromagnetic Counterpart ZTF19abanrhr
• Dark photon bursts from compact binary systems and constraints
• Reference level of the vacuum energy density of the Universe and astrophysical data
• Inflaton-driven early dark energy
• Cosmology from multimeasure multifield model
• Calibrating the Galactic Cepheid Period-Luminosity relation from the maximum-likelihood technique
• Predicted masses of Galactic Cepheids in the Gaia Data Release 2
• Possible formation of ring galaxies by torus-shaped magnetic wormholes
• Testing the Equivalence Principle with Strong Lensing Time Delay Variations
• Turnaround density as a probe of the cosmological constant
• Low-Redshift Constraints on Covariant Canonical Gauge Theory of Gravity
• Search for line-like and box-shaped spectral features from nearby galaxy clusters with 11.4 years of Fermi LAT data
• Point-spread function reconstruction of adaptive-optics imaging: Meeting the astrometric requirements for time-delay cosmography
• Modified Equations of State for Dark Energy and Observational Limitations
• Phenomenological Dark Energy model with hybrid dynamic Cosmological Constant
• Galaxy flows within 8,000 km/s from Numerical Action methods
• Extended Uncertainty Principle: A Deeper Insight into the Hubble Tension?
• Effects of a local physics change on the SH0ES determination of $H_0$
• A search for the fine-structure constant evolution from fast radio bursts and type Ia supernovae data
• Multi-spectral Sirens: Gravitational-wave Cosmology with (Multi-) Sub-populations of Binary Black Holes
• Reconstructions of $f(\mathcal{P})$ and $f(\mathcal{Q})$ gravity models from $(m,n)$-type Barrow Holographic Dark Energy: Analysis and Observational Constraints
• Enhanced power spectra from multi-field inflation
• First Overtone Cepheids of the OGLE Magellanic Cloud Collection -- beyond radial modes
• Domain Wall Network: A Dual Solution for Gravitational Waves and Hubble Tension?
• Period Change Rates of Large Magellanic Cloud Cepheids using MESA
• 21 cm power spectrum in interacting cubic Galileon model
• Dirac dark matter, dark radiation, and the type-II seesaw mechanism in alternative $U(1{)}_X$ standard model
• A Measurement of the Cosmic Expansion Within our Lifetime
• Probing Gravitational Slip with Strongly Lensed Fast Radio Bursts
• Detecting Baryon Acoustic Oscillations with third generation gravitational wave observatories
• Covariant formulation of refracted gravity
• Tests of Standard Cosmology in Horava Gravity and Bayesian Evidence for a Closed Universe, and the Hubble Tension
• Fast radio bursts at the dawn of the 2020s
• Non-parametric modeling of the cosmological data, base on the ${\chi }^2$ distribution
• Measuring Cosmological Distances Using Cluster Edges as a Standard Ruler
• The mid-infrared Leavitt Law for Classical Cepheids in the Magellanic Clouds
• Interplay of CMB Temperature, Space Curvature, and Expansion Rate Parameters
• Interpreting Internal Consistency of DES Measurements
• Model selection and parameter estimation using the iterative smoothing method
• Determining the Hubble Constant with AGN-assisted Black Hole Mergers
• Thermodynamic Constraints on the Dark Sector
• Screening away the $H_0$ tension
• Bayesian Comparison of Interacting Modified Holographic Ricci Dark Energy Scenarios
• Constraints on the Spacetime Dynamics of an Early Dark Energy Component
• Gravitational waves, CMB polarization, and the Hubble tension
• Non-particle dark matter from Hubble parameter
• Model-independent measurement of the absolute magnitude of Type Ia Supernovae with gravitational-wave sources
• Radio Continuum Sources behind the Large Magellanic Cloud
• Probing Interacting Dark Sector with the next generation of gravitational-wave detectors
• A convenient approach to characterizing model uncertainty with application to early dark energy solutions of the Hubble tension
• Astrophysical Distance Scale IV. Preliminary Zero-Point Calibration of the JAGB Method in the HST/WFC3-IR Broad J-Band (F110W) Filter
• Forays into the dark side of the swamp
• Determining Cosmological-model-independent $H_0$ with Gravitationally Lensed Supernova Refsdal
• Tracking the validity of the quasi-static and sub-horizon approximations in modified gravity
• Forecasting constraints on the baryon mass fraction in the IGM from fast radio bursts and type Ia supernovae
• Early Light Curve Excess in Type IIb Supernovae Observed by the ATLAS Survey: Qualitative Constraints on Progenitor Systems
• Simultaneous measurements on cosmic curvature and opacity using latest HII regions and $H(z)$ observations
• Consequences of using a smooth cosmic distance in a lumpy universe: I
• Confronting quantum-corrected teleparallel cosmology with observations
• Eliminating the Hubble Tension in the Presence of the Interconnection between Dark Energy and Matter in the Modern Universe
• The proper motion of stars in dwarf galaxies: distinguishing central density cusps from cores
• SN 2019ein: A Type Ia Supernova Likely Originated from a Sub-Chandrasekhar-Mass Explosion
• Can acoustic and axion-like early dark energy still resolve the Hubble tension?
• High accuracy on $H_0$ constraints from gravitational wave lensing events
• Upper Limit on the Dissipation of Gravitational Waves in Gravitationally Bound Systems
• Direct geometrical measurement of the Hubble constant from galaxy parallax: predictions for the Vera C. Rubin Observatory and Nancy Grace Roman Space Telescope
• Pinpointing coalescing binary neutron star sources with the IGWN, including LIGO-Aundha
• First all-flavor search for transient neutrino emission using 3-years of IceCube DeepCore data
• Implications for cosmology from Ground-based Cosmic Microwave Background observations
• Scalar field evolution at background and perturbation levels for a broad class of potentials
• Geometric Distances of Quasars Measured by Spectroastrometry and Reverberation Mapping:Monte Carlo Simulations
• Impact of Microlensing on Observational Strategies for Gravitational Time Delay Measurements
• Application of Convolutional Neural Networks to time domain astrophysics. 2D image analysis of OGLE light curves
• Solar System-scale interferometry on fast radio bursts could measure cosmic distances with sub-percent precision
• New insights into the use of Ultra Long Period Cepheids as cosmological standard candles
• The progenitors of Type Ia supernovae with asymptotic giant branch donors
• Evolution of dissipative and non-dissipative universes in holographic cosmological models with a power-law term
• RAiSERed: radio continuum redshifts for lobed AGNs
• Results from the Pan-STARRS Search for Kilonovae: Contamination by Massive Stellar Outbursts
• Consistency of Cubic Galileon Cosmology: Model-Independent Bounds from Background Expansion and Perturbative Analyses
• Revisiting Friedmann-like cosmology with torsion: newest constraints from high-redshift observations
• Spherical collapse in coupled quintessence with a $\Lambda$CDM background
• Spectral energy distributions of classical cepheids in the Magellanic Clouds
• Impact of gravitational waveform model systematics on the measurement of the Hubble constant
• Calibrating the surface brightness - color relation for late-type red giants stars in the visible domain using VEGA/CHARA interferometric observations
• New perspectives on future rip scenarios with holographic dark energy
• Cosmological horizons radiate
• Cosmology with LIGO/Virgo dark sirens: Hubble parameter and modified gravitational wave propagation
• Effects of the Hubble Parameter on the Cosmic Growth of the First Quasars
• Strongly Lensed Supernovae in Well-Studied Galaxy Clusters with the Vera C. Rubin Observatory
• Surface Tension: Accelerated Expansion, Coincidence Problem & Hubble Tension
• SEEDisCS II. Molecular gas in galaxy clusters and their large scale structure: low gas fraction galaxies, the case of CL1301.7$-$1139
• On Dark Gravitational Wave Standard Sirens as Cosmological Inference and Forecasting the Constraint on Hubble Constant using Binary Black Holes Detected by Deci-hertz Observatory
• Chameleon Early Dark Energy and the Hubble Tension
• Consistency of CMB experiments beyond cosmic variance
• Testing consistency of ${\Omega }_b{h}^2$ in the Planck data
• An Informational Approach to Cosmological Parameter Estimation
• Singling out modified gravity parameters and datasets reveals a dichotomy between Planck and lensing
• A model-independent constraint on the Hubble constant with gravitational waves from the Einstein Telescope
• More on Emergent Dark Energy from Unparticles
• Axi-Higgs cosmology: Cosmic Microwave Background and cosmological tensions
• A targeted search for strongly lensed supernovae with the Las Cumbres Observatory
• Magrathea-Pathfinder: A 3D adaptive-mesh code for geodesic ray tracing in $N$-body simulations
• Constraining cosmological scaling solutions of a Galileon field
• Unveiling the Universe with Emerging Cosmological Probes
• Multiple measurements on the cosmic curvature using Gaussian process regression without calibration and a cosmological model
• Unveiling the Effects of Coupling Extended Proca-Nuevo Gravity on Cosmic Expansion with Recent Observations
• The intrinsic reddening of the Magellanic Clouds as traced by background galaxies -- III. The Large Magellanic Cloud
• Dark Energy from the Fifth Dimension
• Analytic Calculation of Covariance between Cosmological Parameters from Correlated Data Sets, with an Application to SPTpol
• Growth and Geometry Split in Light of the DES-Y3 Survey
• Measuring the distances to quasars at high redshifts with strong lensing
• Unveiling the quasar main sequence: illuminating the complexity of active galactic nuclei and their evolution
• Synergy Between Hubble Tension Motivated Self-Interacting Neutrino and KeV-Sterile Neutrino Dark Matter
• Testing the phenomenological interacting dark energy model with gamma-ray bursts and Pantheon+ type Ia supernovae
• The flux-weighted gravity-luminosity relation of Galactic classical Cepheids
• Constraints on Lorentz invariance violation from the extraordinary Mrk 421 flare of 2014 using a novel analysis method
• Climbing out of the shadows: building the distance ladder with black hole images
• The Deviation of the Broad-line Region Size Between Reverberation Mapping and Spectroastrometry
• Estimating Hubble Constant with Gravitational Observations: A Concise Review
• Dynamic Dark Energy Equation of State (EoS) and Hubble Constant analysis using type Ia supernovae from Union 2.1 dataset
• Generalized phenomenological models of dark energy
• Coupling quintessence kinetics to electromagnetism
• Perturbations and the Future Conformal Boundary
• Broadband study and the discovery of pulsations from the Be/X-ray binary eRASSU J052914.9-662446 in the Large Magellanic Cloud
• Gravitational wave signatures from dark sector interactions
• Using simulated Tianqin gravitational wave data and electromagnetic wave data to study the coincidence problem and Hubble tension problem
• The stellar evolution perspective on the metallicity dependence of classical Cepheid Leavitt laws
• Constraining neutrino mass in dynamical dark energy cosmologies with the logarithm parametrization and the oscillating parametrization
• On the Paradoxical Impact of Blending by Red Clump Giants
• Dark sector production and baryogenesis from not quite black holes
• HOLISMOKES -- XII. Time-delay Measurements of Strongly Lensed Type Ia Supernovae using a Long Short-Term Memory Network
• Gravitational lens time-delay as a probe of a possible time variation of the fine-structure constant
• Scrutinizing coupled vector dark energy in light of data
• An SU(2) gauge principle for the Cosmic Microwave Background: Perspectives on the Dark Sector of the Cosmological Model
• Cosmological Dynamics in Interacting Scalar-Torsion f(T,$\varphi$) Gravity: Investigating Energy and Momentum Couplings
• Parameterized Deceleration in $f(Q,C)$ Gravity: A Logarithmic Approach
• New simple and accurate quintessence approximations
• A Multi-messenger view of Cosmic Dawn: Conquering the Final Frontier
• Period-Colour and Amplitude-Colour relations for OGLE-$\delta$ Scuti stars in the Galactic Bulge and LMC
• Fundamental physical constants: current results in search for variations and their description
• H-band light curves of Milky Way Cepheids via Difference Imaging
• Probing extra dimensions through cosmological observations of dark energy
• Scalar field dark energy: Insights into cosmological evolution and black hole accretion
• Studies on dark energy evolution
• Linking the $R_{K^{(\ast )}}$ anomalies to the Hubble tension via a single right-handed neutrino
• Gravitational Interactions and Neutrino Masses
• Quantum Trans-Planckian Physics inside Black Holes and its Spectrum
• The HI Structure of the Local Volume Dwarf Galaxy Pisces A
• Multi-field TDiff theories for cosmology
• Hubble tension and matter inhomogeneities: a theoretical perspective
• Do current observations support transient acceleration of our universe?
• Cluster Assembly Times as a Cosmological Test
• From Barthel Randers Kropina Geometries to the Accelerating Universe: A Brief Review of Recent Advances in Finslerian Cosmology
• Model Selection using Baryon Acoustic Oscillations in the Final SDSS-IV Release
• Cosmology of fermionic dark energy coupled to curvature
• The maximum turnaround radius for axisymmetric cosmic structures
• Quintessence scalar field and cosmological constant: Dynamics of a multi-component dark energy model
• Dark Energy: is it `just' Einstein's Cosmological Constant Lambda?
• Signatures of Very Early Dark Energy in the Matter Power Spectrum
• Cosmological signatures of a Rapid Diluted Energy Density
• Effects of Dark Energy anisotropic stress on the matter power spectrum
• Testing Lambert$W$ equation of state with observational Hubble parameter data
• Spectroscopic study of the [OIII]$\lambda$5007 profile in Seyfert 1 galaxies
• Growth of cosmic perturbations in the modified $f(R,T)$ gravity
• The T-E correlation coefficient of Planck legacy data
• Inverse Seesaw, dark matter and the Hubble tension
• Emergent universe revisited through the CSL theory
• Redshift evolution of the X-ray and UV luminosity relation of quasars: calibrated results from SNe Ia
• Testing the coincidence problem with strong gravitational lens, Type Ia supernovae and Hubble parameter observational data
• Thermodynamics of Modified Chaplygin-Jacobi Gas and Modified Chaplygin-Abel Gas: Stability Analysis and Observational Constraints
• A scalar field inducing a non-metrical contribution to gravitational acceleration and a compatible add-on to light deflection
• Coherent states of quantum spacetimes for black holes and de Sitter spacetime
• 2D BAO vs 3D BAO: Hints for new physics?
• Helium abundance (and $H_0$) in X-COP galaxy clusters
• Accelerating behavior from dynamical system analysis parameters
• Relaxing cosmological constraints on current neutrino masses
• Another look on the connections of Hubble tension with the Heisenberg Uncertainty Principle
• An independent determination of the distance to supernova SN 1987A by means of the light echo AT 2019xis
• Emergent universe: tensor perturbations within the CSL framework
• A new way to test the WIMP dark matter models
• Einstein clusters as models of inhomogeneous spacetimes
• Prospects of observation of gravitationally lensed sources by space submillimeter telescopes
• Spatial correlations of dark energy from quantum fluctuations in inflation
• Gravitational wave probes of Barrow cosmology with LISA standard sirens
• Axion-philic cosmological moduli
• Clustering of Local Group distances: publication bias or correlated measurements? VII. A distance framework out to 100 Mpc
• Black hole and cosmological analysis of BF sequestered gravity
• Using Neutrino Oscillations to Measure $H_0$
• Structure Formation in Dark Matter Particle Production Cosmology
• Optimizing Gravitational-Wave Detector Design for Squeezed Light
• Voids and Halos in Voids statistics as a probe of the Expansion History of the Universe
• Modified propagation of gravitational waves from the early radiation era
• Local Limit of Nonlocal Gravity: A Teleparallel Extension of General Relativity
• Probing Cosmology beyond $\Lambda$CDM using the SKA
• Peculiar velocity effects on the Hubble constant from time-delay cosmography
• The establishment of the Standard Cosmological Model through observations
• Anisotropic power-law inflation for a generalized model of two scalar and two vector fields
• Host group degeneracy in gravitational lensing time delay determination of $H_0$
• Angular Correlation Function from sample covariance with BOSS and eBOSS LRG
• Local Limit of Nonlocal Gravity: Cosmological Perturbations
• Dynamical systems analysis of a cosmological model with interacting Umami Chaplygin fluid in adiabatic particle creation mechanism: Some bouncing features
• Modified $f(R,T)$ theory in light of gravitational wave standard sirens
• Reconstructions of Einstein-Aether Gravity from Barrow Agegraphic and New Barrow Agegraphic Dark Energy models: Examinations and Observational Limits
• Rips and regular future scenario with Holographic Dark Energy: A comprehensive look
• A glitch in gravity: cosmic Lorentz-violation from fiery Big Bang to glacial heat death
• A Bright Future? Prospects for Cosmological Tests of GR with Multimessenger Gravitational Wave Events
• TDCOSMO: XX. WFI2033--4723, the First Quadruply-Imaged Quasar Modeled with JWST Imaging
• The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch
• Can Hubble tension be eased by invoking a finite range for gravity?
• The Uplifting of AdS Type to Quintessence Like Potential Induced by Frozen Large Scale Lorentz Violation
• LeMMINGs. VI. Connecting nuclear activity to bulge properties of active and inactive galaxies: radio scaling relations and galaxy environment
• Early dark energy in the pre- and post-recombination epochs
• Sparse formulae for the distance modulus in cosmology
• Viewing angle effects in quasar application to cosmology
• Mass assembly history of dark matter halos in the light of $H_0$ tension
• Probing Cosmology with Baryon Acoustic Oscillations using Gravitational Waves
• Time delay estimation in unresolved lensed quasars
• Sky localization of space-based detectors with time-delay interferometry
• Confronting dark energy in Harada's Conformal Killing Gravity with observational data
• Late Time Phenomena in $f(T,\mathcal{T})$ Gravity Framework: Role of $H_0$ Priors
• Evidence for possible systematic underestimation of uncertainties in extragalactic distances and its cosmological implications
• Analytic Solutions of Scalar Field Cosmology, Mathematical Structures for Early Inflation and Late Time Accelerated Expansion
• On the Field Theoretical Description of an Alternative Model to Generalized Chaplygin Gas and its Thermodynamic Behaviour
• Non-linear saturation and energy transport in global simulations of magneto-thermal turbulence in the stratified intracluster medium
• Construction of the cosmological model with periodically distributed inhomogeneities with growing amplitude
• The Gravitational Lensing Imprints of DES Y3 Superstructures on the CMB: A Matched Filtering Approach
• Vainshtein screening in Horndeski theories nonminimally and kinetically coupled to ordinary matter
• Beyond self-acceleration: force- and fluid-acceleration
• Can the angular scale of cosmic homogeneity be used as a cosmological test?
• Binary Neutron Star (BNS) merger: What we learned from relativistic ejecta of GW/GRB~170817A
• Observational constraints and dynamical analysis of Kaniadakis horizon-entropy cosmology
• Determining $H_0$ from distance sum rule combining gamma-ray bursts with observational Hubble data and strong gravitational lensing
• The Djorgovski-Gurzadyan dark energy integral equation and the Hubble diagram
• The Use of Binary Black Holes Merging in AGN Disks for Hubble Constant Measurements
• Common Origin of Warm Dark Matter and Dark Radiation
• ParamANN: A Neural Network to Estimate Cosmological Parameters for $\Lambda$CDM Universe Using Hubble Measurements
• A New Period Determination Method for Periodic Variable Stars
• Charged analog of anisotropic dark energy star in Rastall gravity
• Special cases of the Multi-Measure Model -- understanding the prolonged inflation
• Logarithmic and Strong Coupling Models in Weyl-Type $f(Q,T)$ Gravity
• Observational Constraints on the Cosmology with Holographic Dark Fluid
• Probing the independence within the dark sector in the fluid approximation
• Inhomogeneous Hubble diagram from vector K-mouflage
• Re-evaluation of ${\Omega }_k$ of the normalised Friedmann-Lema\^ıtre-Robertson-Walker model: Implications for Hubble constant determinations
• The Host Galaxy of the Dwarf Seyfert UGC 06728
• Quintom Dark Energy: Future Attractor and Phantom Crossing in Light of DESI DR2 Observation
• Exploring thermodynamics inconsistencies in unimodular gravity: a comparative study of two energy diffusion functions
• Constraining H0 Via Extragalactic Parallax
• A Geometric Probe of Cosmology: I. Gravitational Lensing Time Delays and Quasar Reverberation Mapping
• Revisiting Ryskin's Model of Cosmic Acceleration
• Determining Cosmological Constant Using Gravitational Wave Information
• Time behaviour of Hubble parameter by torsion
• A Review on Resolving the Hubble Tension via Late-Universe Physics
• A new pressure-parametric cosmological model
• Mapping the cosmic expansion history from LIGO-Virgo-KAGRA in synergy with DESI and SPHEREx
• Constraints on Multicomponent Dark Energy from Cosmological Observations
• KiDS-Legacy: Constraining dark energy, neutrino mass, and curvature
• From oversimplified to overlooked: the case for exploring Rich Dark Sectors
• LeMMINGs. V. Nuclear activity and bulge properties: a detailed multi-component decomposition of $e$-MERLIN Palomar galaxies with $HST$
• Scalar-tensor cosmologies in a minisuperspace formulation: a case study
• Parameter free Hubble constant from the quadruply lensed quasar SDSS J1004 + 4112
• Primordial nucleosynthesis constraints on high-z energy releases
• A new experiment for the gravitational waves detection
• The Anomalous 21-cm Absorption at High Redshifts
• Gaussian discriminators between $\Lambda$CDM and wCDM cosmologies using expansion data
• Cosmology of Single Species Hidden Dark Matter
• Large, fast and accurate HI intensity maps with latent overlap diffusion
• Testing Exponential $f(R)$ Gravity with CMB, DESI-DR2, and Supernova Data
• Degrees of Freedom of New General Relativity I: Type 2, Type 3, Type 5, and Type 8
• The snapshot distance method: estimating the distance to a Type Ia supernova from minimal observations
• Multifield theories invariant under transverse diffeomorphisms: The mixed regime case
• Coordinate independent approach to the calculation of the effects of local structure on the luminosity distance
• Alleviating the Hubble tension with Torsion Condensation (TorC)
• Biases in velocity reconstruction: investigating the effects on growth rate and expansion measurements in the local universe
• Magellanic System Stars Identified in SMACS J0723.3-7327 James Webb Space Telescope Early Release Observations Images
• Second-order dust perturbations of the non-flat FLRW model with the positive cosmological constant
• Neutrino Interactions with perturbed Rastall Gravity: A Novel Approach to Reducing the Hubble Tension
• H0 tension in Tsallis and Renyi statistics
• An Alcock-Paczynski Test on Reionization Bubbles for Cosmology
• Can cosmic rotation resolve the Hubble tension? Constraints from CMB and large-scale structure
• Space-based Gravitational Wave Observatories
• ECHO21: a tool for modelling global 21-cm signal from dark ages to reionization
• Accounting for Correlations When Fitting Extra Cosmological Parameters
• Model independent calibration for sound horizon combining observations of supernovae and transversal BAO measurements
• Flat Space, Dark Energy, and the Cosmic Microwave Background
• The Hubble Tension: Relativistic Dark Matter Production from Long-lived Particles
• Assessing the potential of cluster edges as a standard ruler
• Dark sector interactions in light of weak lensing data
• Reference frame dependence of the local measurement of the Hubble constant
• Testing Linearly Coasting Cosmology by Strong Lensing System and Pantheon+ Data
• Local dark energy in the Sculptor Filament of galaxies
• Impact of a Rapid Diluted Energy Density on the halo mass function
• Thermodynamics of sign-switching dark energy models
• Results from Hubble parameter data: oscillating dark energy?
• Testing $\Lambda$CDM with eBOSS data using a model independent diagnostic
• Understanding CMB physics through the exploration of exotic cosmological models: a classroom study using CLASS
• On observational signatures of multi-fractional theory
• Cosmological Frequency Combs
• Stealth black hole solutions in higher-order Maxwell-Einstein theories
• The impact of precession and higher-order multipoles for gravitational wave cosmological inference
• Cosmological Dynamics of Exponential Quintessence Constrained by BAO, Cosmic Chronometers, and DES-SN5YR/Pantheon+ Data
• Polytropic $f(Q)$ cosmology and its implications for the $H_0$ tension
• Constraining nonminimal f(T) gravity from Primordial Nucleosynthesis to Late-Universe observations
• The Forward Physics Facility at the High-Luminosity LHC
• Puzzling High-Velocity Calcium Absorption Features Of Type Ia Supernovae
• Kinematical models of latetime cosmology and the statefinder diagnostic
• Vector dark radiation and gravitational-wave polarization
• Early dark energy triggered by spacetime dynamics that encodes cosmic radiation-matter transition
• Evidence against Ryskin's model of cosmic acceleration
• Kaniadakis holographic dark energy: observational constraints and global dynamics
• Correlation of structure growth index with current cosmic acceleration: constraints on dark energy models
• Scalar field dark matter with two components: combined approach from particle physics and cosmology
• The SNIa Runaway LP 398-9: Detection of Circumstellar Material and Surface Rotation
• The CUBES Science Case
• Dissecting the $H_0$ and $S_8$ tensions with Planck + BAO + supernova type Ia in multi-parameter cosmologies
• Thermodynamic parametrization of dark energy
• Dependence of pulsation mode of Cepheids on metallicity
• The cosmological constant vs adiabatic invariance
• Robustness of the Cosmological Constant Damping Mechanism Through Matter Eras
• Ricci cosmology in light of astronomical data
• Hunting for the nature of the enigmatic narrow-line Seyfert 1 galaxy PKS 2004-447
• Decaying Dark Matter: Simulations and Weak-Lensing Forecast
• Cosmic tango between the very small and the very large: Addressing CMB anomalies through Loop Quantum Cosmology
• Optical design of a multi-object fiber-fed spectrograph system for Southern Spectroscopic Survey Telescope
• Improving NASA/IPAC Extragalactic Database Redshift Calculations
• Simultaneous inference of periods and period-luminosity relations for Mira variable stars
• Spatial Dependence of the Growth Factor in Scalar-Tensor Cosmology
• Turnaround Radius for charged particles in the Reissner-Nordström deSitter spacetime
• On rips and cosmological singularities in a universe merging with baby universes
• Structure of cosmic web in non-linear regime: the nearest neighbour and spherical contact distributions
• Application of the space-based optical interferometer towards measuring cosmological distances of quasars
• Validating the Angular Sizes of Red Clump Stars with Intensity Interferometry
• Local environmental dependence on weak-lensing shear statistics
• Addressing the too-big-to-fail problem and the void phenomenon through a modified initial power spectrum
• Energy conditions and entropy density of the universe
• Detectability of the Phase Transition Gravitational Waves in the DFSZ axion Model
• Yellow Post-Asymptotic-Giant-Branch Stars as Standard Candles. I. Calibration of the Luminosity Function in Galactic Globular Clusters
• Searching for a signature of turnaround in galaxy clusters with convolutional neural networks
• Cosmological perturbations on an averaged background
• Probing modified gravitational wave propagation with strongly lensed coalescing binaries
• Confusing dark matter particle properties with modifications to General Relativity
• OGLE-IV Period-Luminosity relation of the LMC: an analysis using mean and median magnitudes
• Spectral distortions in the decaying QCD dark matter scenario
• Parameter estimation for space-based gravitational wave detectors with ringdown signals
• The Astrophysical Distance Scale: V. A 2% Distance to the Local Group Spiral M33 via the JAGB Method, Tip of the Red Giant Branch, and Leavitt Law
• Extending the cosmic distance ladder two orders of magnitude with strongly lensed Cepheids, carbon AGB, and RGB stars
• Dynamics of tachyon dark energy on large scales and its imprint on observed galaxy power spectrum
• Active galactic nuclei and gravitational redshifts
• Holographic dark energy in modified Kaniadakis cosmology
• A Robust Bayesian Meta-Analysis for Estimating the Hubble Constant via Time Delay Cosmography
• An effective fluid description of scalar-vector-tensor theories under the sub-horizon and quasi-static approximations
• Cosmological implications of the full shape of anisotropic clustering measurements in BOSS and eBOSS
• NuAncestor: an artificial satellite-borne star for accurate frequency calibration of ground-based EPRV spectrographs
• The long freeze: an asymptotically static universe from holographic dark energy
• Luminosity-Temperature Relation as a Probe for Modified Gravity
• Bayesian vs Frequentist: Comparing Bayesian model selection with a frequentist approach using the iterative smoothing method
• Signatures of Extended Dark Energy Parametrisations in Structure Formation under Background Constraints
• Impact of the calibration of the Halo Mass Function on galaxy cluster number count cosmology
• Gamma-Ray Bursts, Supernovae Ia and Baryon Acoustic Oscillations: a binned cosmological analysis
• Systematic Light Propagation Bias from the Heliosphere and Its Impact on the Hubble Tension
• Possible evidences for physics beyond $\Lambda$CDM from DESI DR2 data
• Analytical solution of traversable wormholes in the presence of positive cosmological constant
• SDSS-IV MaNGA: A Catalogue of Spectroscopically Detected Strong Galaxy-Galaxy Lens Candidates
• Beyond the Cosmological Constant: Breaking the Geometric Degeneracy of $f(Q)$ cosmology via Redshift-Space Distortions
• Cosmology of Cubic Poincaré Gauge gravity
• SHARP VIII: J0924+0219 lens mass distribution and time-delay prediction through adaptive-optics imaging
• On the Orbital Velocity of Isolated Galaxy Pairs: a test of gravity in the low acceleration regime
• New Constraint of the Hubble Constant by Proper Motions of Radio Components Observed in AGN Twin-jets
• Observational Constraints and Geometric Diagnostics of Barboza-Alcaniz and Logarithmic Dark Energy Parametrizations
• Saving CNB assisted EDE model at the expense of quantum corrections?