A 2.4% Determination of the Local Value of the Hubble Constant

Abstract

We use the Wide Field Camera 3 (WFC3) on the Hubble Space Telescope (HST) to reduce the uncertainty in the local value of the Hubble constant (H_0) from 3.3% to 2.4%. Improvements come from new, near-infrared observations of Cepheid variables in 11 new hosts of recent SNe~Ia, more than doubling the sample of SNe~Ia having a Cepheid-calibrated distance for a total of 19; these leverage the magnitude-z relation based on 300 SNe~Ia at z<0.15. All 19 hosts and the megamaser system NGC4258 were observed with WFC3, thus nullifying cross-instrument zeropoint errors. Other improvements include a 33% reduction in the systematic uncertainty in the maser distance to NGC4258, more Cepheids and a more robust distance to the LMC from late-type DEBs, HST observations of Cepheids in M31, and new HST-based trigonometric parallaxes for Milky Way (MW) Cepheids. We consider four geometric distance calibrations of Cepheids: (i) megamasers in NGC4258, (ii) 8 DEBs in the LMC, (iii) 15 MW Cepheids with parallaxes, and (iv) 2 DEBs in M31. H_0 from each is 72.25+/-2.51, 72.04+/-2.67, 76.18+/-2.37, and 74.50+/-3.27 km/sec/Mpc, respectively. Our best estimate of 73.24+/-1.74 km/sec/Mpc combines the anchors NGC4258, MW, and LMC, and includes systematic errors for a final uncertainty of 2.4%. This value is 3.4 sigma higher than 66.93+/-0.62 km/sec/Mpc predicted by LambdaCDM with 3 neutrinos with mass 0.06 eV and the Planck data, but reduces to 2.1 sigma relative to the prediction of 69.3+/-0.7 km/sec/Mpc with the combination of WMAP+ACT+SPT+BAO, suggesting systematic uncertainties in CMB measurements may play a role in the tension. If we take the conflict between Planck and H_0 at face value, one plausible explanation could involve an additional source of dark radiation in the early Universe in the range of Delta N_eff=0.4-1. We anticipate significant improvements in H_0 from upcoming parallax measurements.

accepted ApJ, includes proof corrections and edits, 63 pages, 16 figures, 8 tables. Table 4 available electronically by ApJ Revised since v1 to include one new supernova/calibrator and updated Planck constraints

References in corpus (16)

• New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy
• Improved Dark Energy Constraints from ~100 New CfA Supernova Type Ia Light Curves
• Improved Distances to Type Ia Supernovae with Multicolor Light Curve Shapes: MLCS2k2
• An eclipsing binary distance to the Large Magellanic Cloud accurate to 2 per cent
• CfA3: 185 Type Ia Supernova Light Curves from the CfA
• The 1% Concordance Hubble Constant
• The Hubble Constant: A Summary of the HST Program for the Luminosity Calibration of Type Ia Supernovae by Means of Cepheids
• A new Cepheid distance to the maser-host galaxy NGC 4258 and its implications for the Hubble Constant
• Cosmological parameters from the comparison of peculiar velocities with predictions from the 2M++ density field
• The influence of chemical composition on the properties of Cepheid stars. II-The iron content
• Cepheid Parallaxes and the Hubble Constant
• Cepheid Calibrations of Modern Type Ia Supernovae:Implications for the Hubble Constant
• Neutrinos help reconcile Planck measurements with both Early and Local Universe
• Toward a New Distance to the Active Galaxy NGC 4258: II. Centripetal Accelerations and Investigation of Spiral Structure
• No new cosmological concordance with massive sterile neutrinos
• The M31 Near-Infrared Period-Luminosity Relation and its non-linearity for $\delta$ Cep Variables with $0.5\le \log (P)\le 1.7$

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• Cosmological discordances: a new measure, marginalization effects, and application to geometry vs growth current data sets
• Think Global, Act Local: The Influence of Environment Age and Host Mass on Type Ia Supernova Light Curves
• Symmetry of Cosmological Observables, and a High Hubble Constant as an Indicator of a Mirror World Dark Sector
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• Dirac and Majorana neutrino signatures of primordial black holes
• Distance and properties of NGC 4993 as the host galaxy of a gravitational wave source, GW170817
• Phenomenology of the generalized cubic covariant Galileon model and cosmological bounds
• A Comparison of Cosmological Parameters Determined from CMB Temperature Power Spectra from the South Pole Telescope and the Planck Satellite
• Multi-Dimensional Parameter Study of Double Detonation Type Ia Supernovae Originating from Thin-Helium-Shell White Dwarfs
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• Flavor-specific Interaction Favors Strong Neutrino Self-coupling in the Early Universe
• Test of the cosmic evolution using Gaussian processes
• The effect of metallicity on Cepheid Period-Luminosity relations from a Baade-Wesselink analysis of Cepheids in the Milky Way and Magellanic Clouds
• Can redshift errors bias measurements of the Hubble Constant?
• BAO+BBN revisited -- Growing the Hubble tension with a 0.7km/s/Mpc constraint
• The SPIRITS sample of Luminous Infrared Transients: Uncovering Hidden Supernovae and Dusty Stellar Outbursts in Nearby Galaxies
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• COSMOGRAIL XVII: Time delays for the quadruply imaged quasar PG 1115+080
• Cosmological constraints on alternative model to Chaplygin fluid revisited
• Einstein's Universe: Cosmological structure formation in numerical relativity
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• Independent Cosmological Constraints from high-z HII Galaxies
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• Measuring the Hubble constant: Gravitational wave observations meet galaxy clustering
• Rastall gravity extension of the standard $\Lambda$CDM model: theoretical features and observational constraints
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• Incompleteness Matters Not: Inference of $H_0$ from BBH-galaxy cross-correlations
• A Standard Ruler at Cosmic Dawn
• Data-driven Reconstruction of the Late-time Cosmic Acceleration with f(T) Gravity
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• Quintessence Axion Dark Energy and a Solution to the Hubble Tension
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• Supernova Siblings: Assessing the Consistency of Properties of Type Ia Supernovae that Share the Same Parent Galaxies
• Augmenting astrophysical scaling relations with machine learning: application to reducing the Sunyaev-Zeldovich flux-mass scatter
• Modeling of accelerating Universe with bulk viscous fluid in Bianchi V space-time
• Probing Cosmology with Dark Matter Halo Sparsity Using X-ray Cluster Mass Measurements
• Inspecting the Cepheid distance ladder: The Hubble Space Telescope distance to the SNIa host galaxy NGC 5584
• Constraining viscous dark energy models with the latest cosmological data
• Does Quartessence Ease Tensions?
• The shape of galaxy dark matter halos in massive galaxy clusters: Insights from strong gravitational lensing
• Degenerate Sub-keV Fermion Dark Matter from a Solution to the Hubble Tension
• Diffusion in unimodular gravity: Analytical solutions, late-time acceleration, and cosmological constraints
• A comment on power-law inflation with a dark radiation component
• Low-redshift estimates of the absolute scale of baryon acoustic oscillations
• Debiasing Cosmic Gravitational Wave Sirens
• The Scale-Invariant Vacuum (SIV) Theory: A Possible Origin of Dark Matter and Dark Energy
• The Intrinsic Scatter of the Radial Acceleration Relation
• Radial oscillations and tidal Love numbers of dark energy stars
• Constraining power of cosmological observables: blind redshift spots and optimal ranges
• A new measure of tension between experiments
• Isotropic vs. Anisotropic components of BAO data: a tool for model selection
• Carbon stars as standard candles: II. The median J magnitude as a distance indicator
• Cepheid Metallicity in the Leavitt Law (C- MetaLL) survey: II.High-resolution spectroscopy of the most metal poor Galactic Cepheids
• Dark energy in multi-fractional spacetimes
• Unified Dark Fluid and Cosmic Transit Models in Brans-Dicke Theory
• Using spatial curvature with HII galaxies and cosmic chronometers to explore the tension in $H_0$
• Breaking the Vainshtein screening in clusters of galaxies
• Luminosity functions of globular clusters in five nearby spiral galaxies using HST/ACS images
• Significant Luminosity Differences of Two Twin Type Ia Supernovae
• An accurate method to determine the systematics due to the peculiar velocities of galaxies in measuring the Hubble constant from gravitational wave standard sirens
• Torsion in string-inspired cosmologies and the universe dark sector
• On a new and homogeneous metallicity scale for Galactic classical Cepheids - I. Physical parameters
• Constraining the SN Ia Host Galaxy Dust Law Distribution and Mass Step: Hierarchical BayeSN Analysis of Optical and Near-Infrared Light Curves
• Can the quantum vacuum fluctuations really solve the cosmological constant problem?
• Multiwavelength Period-Luminosity and Period-Luminosity-Color relations at maximum-light for Mira variables in the Magellanic Clouds
• Anisotropic massive Brans-Dicke gravity extension of the standard $\Lambda$CDM model
• Phantom braneworld and the Hubble tension
• On the influence of the environment on galactic chemical abundances
• Does fractal Universe describe a complete cosmic scenario?
• Constraints on Lorentz Invariance and CPT Violation using Optical Photometry and Polarimetry of Active Galaxies BL Lacertae and S5 B0716+714
• Type II Supernovae as Distance Indicators at Near-IR Wavelengths
• Cepheids in M31 - The PAndromeda Cepheid sample
• Constraining light sterile neutrino mass with the BICEP2/Keck Array 2014 B-mode polarization data
• Isolating the Lyman Alpha Forest BAO Anomaly
• The Hubble-Lemaître constant and sound horizon from low-redshift probes
• Newest measurements of Hubble constant from DESI 2024 BAO observations
• Brans-Dicke cosmology mimicking running vacuum
• Luminous Type II supernovae for their low expansion velocities
• Testing the warmness of dark matter
• DustPedia - the relationships between stars, gas and dust for galaxies residing in different environments
• Multiple measurements of quasars acting as standard probes: model independent calibration and exploring the Dark Energy Equation of States
• x-cut Cosmic Shear: Optimally Removing Sensitivity to Baryonic and Nonlinear Physics with an Application to the Dark Energy Survey Year 1 Shear Data
• First cosmological constraints combining Planck with the recent gravitational-wave standard siren measurement of the Hubble constant
• No-go guide for the Hubble tension: late-time or local-scale new physics
• Probing a Steep EoS for Dark Energy with latest observations
• Constraints on the dark matter and dark energy interactions from weak lensing bispectrum tomography
• Electroweak Kaluza-Klein Dark Matter
• Clustering and redshift-space distortions in modified gravity models with massive neutrinos
• On Zero Point Calibration of the Red Giant Branch Tip in the Magellanic Clouds
• Dark energy in scalar-vector-tensor theories
• Improving the absolute accuracy of the gravitational wave detectors by combining the photon pressure and gravity field calibrators
• A revised lens time delay for JVAS B0218+357 from a reanalysis of VLA monitoring data
• An updated Type II supernova Hubble diagram
• HOLISMOKES -- VII. Time-delay measurement of strongly lensed Type Ia supernovae using machine learning
• Consistent radial velocities of classical Cepheids from the cross-correlation technique
• H0LiCOW XI. A weak lensing measurement of the external convergence in the field of the lensed quasar B1608+656 using HST and Subaru deep imaging
• The Hubble constant tension with next-generation galaxy surveys
• The supernova of the MAGIC GRB190114C
• Cosmological backreaction within the Szekeres model and emergence of spatial curvature
• Cosmological Tests of Everpresent $\Lambda$
• Gravitational Lenses as High-Resolution Telescopes
• The Twins Embedding of Type Ia Supernovae I: The Diversity of Spectra at Maximum Light
• The variance of the locally measured Hubble parameter explained with different estimators
• Does the second law hold at cosmic scales?
• The first constraint from SDSS galaxy-galaxy weak lensing measurements on interacting dark energy models
• Dynamical stability in models where dark matter and dark energy are non-minimally coupled to curvature
• Stability analysis and constraints on interacting viscous cosmology
• New cosmological constraints with extended-Baryon Oscillation Spectroscopic Survey DR14 quasar sample
• Suppressed cosmic growth in coupled vector-tensor theories
• A BayeSN Distance Ladder: $H_0$ from a consistent modelling of Type Ia supernovae from the optical to the near infrared
• The Araucaria Project. The Distance to the Sculptor Group Galaxy NGC 7793 from Near-Infrared Photometry of Cepheid Variables
• Astrophysical Signatures of Black holes in Generalized Proca Theories
• A gravitational constant transition within cepheids as supernovae calibrators can solve the Hubble tension
• Molecular gas in two companion cluster galaxies at z=1.2
• The Absolute Magnitudes of 1991T-like Supernovae
• Testing for New Physics: Neutrinos and the Primordial Power Spectrum
• A Comparison of Maps and Power Spectra Determined from South Pole Telescope and Planck Data
• K-mouflage Imprints on Cosmological Observables and Data Constraints
• Constraints on Steep Equation of State for the Dark Energy using BAO
• The Foundation Supernova Survey: Photospheric Velocity Correlations in Type Ia Supernovae
• Cosmological Constraints from Galaxy Cluster Sparsity, Cluster Gas Mass Fraction and Baryon Acoustic Oscillations Data
• Observational Constraints in Nonlocal Gravity: the Deser-Woodard Case
• Testing cosmic acceleration for $w(z)$ parameterizations using $f_{gas}$ measurements in galaxy clusters
• Emergent gravity in galaxies and in the Solar System
• Anisotropic solid dark energy
• Kinematic Constraints on Spatial Curvature from Supernovae Ia and Cosmic Chronometers
• The deceleration parameter in `tilted' universes: generalising the Friedmann background
• Enhancing the H2O Megamaser Detection Rate Using Optical and Mid-infrared Photometry
• Cepheid metallicity in the Leavitt law (C-MetaLL) survey -- III. Simultaneous derivation of the Gaia parallax offset and Period-Luminosity-Metallicity coefficients
• Non-parametric reconstruction of dark energy and cosmic expansion from the Pantheon compilation of type Ia supernovae
• Constraining Sterile Neutrino Cosmology with Terrestrial Oscillation Experiments
• Cosmological constraints and phenomenology of a beyond-Horndeski model
• Cascading Dark Energy
• Dark matter solution to the $H_0$ and $S_8$ tensions, and the integrated Sachs-Wolfe void anomaly
• Testing the cosmic opacity at higher redshifts: implication from quasars with available UV and X-ray observations
• New probe of gravity: strongly lensed gravitational wave multi-messenger approach
• The Araucaria Project. Multi-band calibrations of the TRGB absolute magnitude
• Coupled Multi Scalar Field Dark Energy
• Absolute Calibration of Cepheid Period-Luminosity Relations in NGC 4258
• Extended $\Lambda$CDM model
• The Unsettled Number: Hubble's Tension
• A common explanation of the Hubble tension and anomalous cold spots in the CMB
• {\it Gauging} the cosmic acceleration with recent type Ia supernovae data sets
• Spectroscopic properties of a two-dimensional time-dependent Cepheid model II. Determination of stellar parameters and abundances
• Constraining the interaction between dark sectors with future HI intensity mapping observations
• Gravitino/Axino as Decaying Dark Matter and Cosmological Tensions
• Probing dynamics of dark energy with latest observations
• A testable hidden-sector model for Dark Matter and neutrino masses
• The Carnegie Chicago Hubble Program VI: Tip of the Red Giant Branch Distances to M66 and M96 of the Leo I Group
• A comprehensive parametrization approach for the Hubble parameter in scalar field dark energy models
• SN 2015ba: A type IIP supernova with a long plateau
• A framework for the next generation of stationary cosmological models
• A new pressure-parametrization unified dark fluid model
• Swift UVOT Grism Observations of Nearby Type Ia Supernovae -- II. Probing the Progenitor Metallicity of SNe Ia with Ultraviolet Spectra
• Vacuum dynamics in the Universe versus a rigid $\Lambda =$const
• Searching for Signatures of Dark matter-Dark Radiation Interaction in Observations of Large-scale Structure
• Reddened, Redshifted, or Intrinsically Red? Understanding Near-Ultraviolet Colors of Type Ia Supernovae
• Universe opacity and Type Ia supernova dimming
• Impact of symmetron screening on the Hubble tension: new constraints using cosmic distance ladder data
• Molecular gas in radio galaxies in dense Mpc-scale environments at $z=0.4-2.6$
• A Tale of Two Type Ia Supernovae: The fast-declining siblings SNe 2015bo and 1997cn
• The Cepheid Distance to the Narrow-Line Seyfert 1 Galaxy NGC 4051
• Alleviating the Hubble-constant tension and the growth tension via a transition of absolute magnitude favored by the Pantheon+ sample
• The effect of dark matter-dark radiation interactions on halo abundance -- a Press-Schechter approach
• Ultra-compact structure in radio quasars as a cosmological probe: a revised study of the interaction between cosmic dark sectors
• Dark Energy and String Theory
• Testing a quintessence model with Yukawa interaction from cosmological observations and N-body simulations
• Backreaction and FRW consistency conditions
• Addressing Astrophysical and Cosmological Problems With Secretly Asymmetric Dark Matter
• $f(R)$ gravity modifications: from the action to the data
• Constraining cosmology with the cosmic microwave and infrared backgrounds correlation
• Late decaying 2-component dark matter scenario as an explanation of the AMS-02 positron excess
• Bayesian correction of $H(z)$ data uncertainties
• HOLISMOKES -- V. Microlensing of type II supernovae and time-delay inference through spectroscopic phase retrieval
• Cosmological acceleration
• Bulk Flow Motion Detection in the Local Universe with Pantheon$+$ Type Ia Supernovae
• Observations of the low-luminosity Type Iax supernova 2019gsc: a fainter clone of SN 2008ha?
• Galaxy-lens determination of $H_0$: constraining density slope in the context of the mass sheet degeneracy
• How does an incomplete sky coverage affect the Hubble Constant variance?
• How does the grouping scheme affect the Wiener Filter reconstruction of the local Universe?
• A Model of Interacting Dark Matter and Dark Radiation for $H_0$ and ${\sigma }_8$ Tensions
• Field Theories and Fluids for an Interacting Dark Sector
• Constraining Dark-Matter Ensembles with Supernova Data
• On the Color-Metallicity Relation of the Red Clump and the Reddening Toward the Magellanic Clouds
• Constraints on self-interacting Bose-Einstein condensate dark matter using large-scale observables
• Getting a THUMP from a WIMP
• Prospect for cosmological parameter estimation using future Hubble parameter measurements
• Redshift remapping and cosmic acceleration in dark-matter-dominated cosmological models
• Easily Interpretable Bulk Flows: Continuing Tension with the Standard Cosmological Model
• Cosmological signatures of torsion and how to distinguish torsion from the dark sector
• Consistent extinction model for type Ia supernovae in Cepheid-based calibration galaxies and its impact on $H_0$
• Hubble trouble or Hubble bubble?
• Constraining constant and tomographic coupled dark energy with low-redshift and high-redshift probes
• No evidence for dynamical dark energy in two models
• Probing $\Lambda$CDM cosmology with the Evolutionary Map of the Universe survey
• Extended $\Lambda$CDM model and viscous dark energy: A Bayesian analysis
• Probing the large scale structure using gravitational-wave observations of binary black holes
• Reassessing the Constraints from SH0ES Extragalactic Cepheid Amplitudes on Systematic Blending Bias
• Cosmological model with time varying deceleration parameter in $F(R,G)$ gravity
• Phenomenological Gravitational Phase Transition: Reconciliation between the Late and Early Universe
• Consistency of the Planck CMB data and $\Lambda$CDM cosmology
• An exponential equation of state of dark energy in the light of 2018 CMB Planck data
• Constraints on Early Dark Energy from the Axion Weak Gravity Conjecture
• On the impact of large angle CMB polarization data on cosmological parameters
• Precise Empirical Determination of Metallicity Dependence of Near-infrared Period-Luminosity Relations for RR Lyrae Variables
• Constraining Type Iax Supernova Progenitor Systems with Stellar Population Aging
• New observational limits on dark radiation in brane-world cosmology
• Dark energy versus modified gravity: Impacts on measuring neutrino mass
• Cosmological evolution with quadratic gravity and nonideal fluids
• Cosmological models with squared trace in modified gravity
• Frames of most uniform Hubble flow
• Modeling the large-scale power deficit with smooth and discontinuous primordial spectra
• Tully-Fisher Distances and Dynamical Mass Constraints for 24 Host Galaxies of Reverberation-Mapped AGN
• The unified history of the viscous accelerating universe and phase transitions
• Improving data-driven model-independent reconstructions and updated constraints on dark energy models from Horndeski cosmology
• Phenomenological Gravitational Phase Transition: Early and Late Modifications
• Probing Polaris' Puzzling Radial Velocity Signals - Pulsational (In-)Stability, Orbital Motion, and Bisector Variations
• Probing the Neutrino Mass Hierarchy beyond $\Lambda$CDM Model
• When tension is just a fluctuation: How noisy data affect model comparison
• Most general cubic-order Horndeski Lagrangian allowing for scaling solutions and the application to dark energy
• An Empirical Calibration of the Tip of the Red Giant Branch Distance Method in the Near Infrared. I. HST WFC3/IR F110W and F160W Filters
• Relativistic corrections for measuring Hubble's constant to 1% using stellar standard candles
• The arbitrariness of potentials in interacting quintessence models
• Arbitrarily coupled $p-$forms in cosmological backgrounds
• Thunder and Lightning: Using Neutron-Star Mergers as Simultaneous Standard Candles and Sirens to Measure Cosmological Parameters
• Constraints on the physical properties of Type Ia supernovae from photometry
• Cosmological simulations of self-interacting Bose-Einstein condensate dark matter
• Parameter estimation of eccentric gravitational waves with a decihertz observatory and its cosmological implications
• Addressing Cosmological Tensions by Non-Local Gravity
• Hubble tension as a window on the gravitation of the dark matter sector
• Tight $H_0$ constraint from galaxy redshfit surveys: combining baryon acoustic osillation measurements and Alcock-Paczynski test
• Weak lensing probe of cubic Galileon model
• Dark Energy Constraints in light of Pantheon SNe Ia, BAO, Cosmic Chronometers and CMB Polarization and Lensing Data
• Phantom crossing dark energy in Horndeski's theory
• Dynamical friction in Bose-Einstein condensed self-interacting dark matter at finite temperatures, and the Fornax dwarf spheroidal
• On sign-changeable interaction in FLRW cosmology
• Observed galaxy power spectrum in cubic Galileon model
• Prospects of the local Hubble parameter measurement using gravitational waves from double neutron stars
• The stellar photosphere-hydrogen ionization front interaction in Classical Pulsators: a theoretical explanation for observed period-colour relations
• Forecasts on interacting dark energy with standard sirens
• SN 2018agk: A Prototypical Type Ia Supernova with a Smooth Power-law Rise in Kepler (K2)
• Spectroscopic properties of a two-dimensional time-dependent Cepheid model I. Description and validation of the model
• From Hubble to Snap Parameters: A Gaussian Process Reconstruction
• Absolute Distances to Nearby Type Ia Supernovae via Light Curve Fitting Methods
• Nebular-Phase Spectra of Type Ia Supernovae from the Las Cumbres Observatory Global Supernova Project
• Photometry of Type II Supernova SN 2023ixf with a Worldwide Citizen Science Network
• Gravitational Wave Opacity from Gauge Field Dark Energy
• SN 2012ij: A low-luminosity type Ia supernova and evidence for continuous distribution from 91bg-like explosion to normal ones
• Geometrical origins of the Universe dark sector: string-inspired torsion and anomalies as seeds for inflation and dark matter
• Determining $H_0$ with the latest HII galaxy measurements
• Testing averaged cosmology with type Ia supernovae and BAO data
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). The matter density and baryon fraction from the galaxy power spectrum at redshift $0.6<z<1.1$
• Using Host Galaxy Spectroscopy to Explore Systematics in the Standardisation of Type Ia Supernovae
• Light deflection angle through velocity profile of galaxies in $f(R)$ model
• The effects of peculiar velocities in SN Ia environments on the local $H_0$ measurement
• Cepheid Metallicity in the Leavitt Law (C- MetaLL) survey: VI: Radial abundance gradients of 29 chemical species in the Milky Way Disk
• Baryon Physics and Tight Coupling Approximation in Boltzmann Codes
• Mapping Circumstellar Matter with Polarized Light - The Case of Supernova 2014J in M82
• On Estimating the Mass of Keplerian Accretion Disks in H2O Maser Galaxies
• Ultralight dark photon as a model for early universe dark matter
• Precise Clustering and Density Evolution of redMaPPer Galaxy Clusters versus MXXL Simulation
• ASASSN-15no: The Supernova that plays hide-and-seek
• A new parametrization for dark energy density and future deceleration
• A Test of MONDian Gravity in $\sim$300 pressure supported elliptical galaxies from the MaNGA survey
• Big Bang Nucleosynthesis Limits and Relic Gravitational Waves Detection Prospects
• Thomson scattering: One rate to rule them all
• A Preliminary Calibration of the JAGB Method Using Gaia EDR3
• Early Dark Energy from a Higher-dimensional Gauge Theory
• Recovering $\Lambda$CDM Model From a Cosmographic Study
• Studying the Intervention of an Unusual Term in $f(T)$ Gravity via Noether Symmetry
• Model-Independent Determination of $H_0$ and ${\Omega }_{K,0}$ using Time-Delay Galaxy Lenses and Gamma-Ray Bursts
• Contributions to $\Delta N_{eff}$ from the dark photon of $U(1{)}_{T3R}$
• Prospects of strongly lensed fast radio bursts: Simultaneous measurement of post-Newtonian parameter and Hubble constant
• The L - σ relation for HII galaxies in green
• Growth of structures and redshift-space distortion data in scale-dependent gravity
• Limits on Brane-World and Particle Dark Radiation from Big Bang Nucleosynthesis and the CMB
• $H_0$ tension without CMB data: beyond the $\Lambda$CDM
• Generalized Brans-Dicke theories in light of evolving dark energy
• Rapidly-Declining Hostless Type Ia Supernova KSP-OT-201509b from the KMTNet Supernova Program: Transitional Nature and Constraint on ${}^{56}$Ni Distribution and Progenitor Type
• First comprehensive constraints on the Finslerian models using cosmological observations
• HARPS-N high spectral resolution observations of Cepheids II. The impact of the surface-brightness color relation on the Baade-Wesselink projection factor of eta Aql
• Scalar Field Theory Description of the Running Vacuum Model: the Vacuumon
• Mean Estimate Distances for Galaxies with Multiple Estimates in NED-D
• Cosmological constraints from low-redshift data
• The Interaction of Supernova 2018evt with a Substantial Amount of Circumstellar Matter -- An SN1997cy-like Event
• Cosmologically viable generalized Einstein-Aether theories
• Calibrating the cosmic distance ladder using gravitational-wave observations
• Hubble distancing: Focusing on distance measurements in cosmology
• Potential Black Hole Seeding of the Spiral Galaxy NGC 4424 via an Infalling Star Cluster
• Cosmological constraints on sterile neutrino oscillations from Planck
• Supernovae and Weinberg's Higgs Portal Dark Radiation and Dark Matter
• Using Rest-Frame Optical and NIR Data from the RAISIN Survey to Explore the Redshift Evolution of Dust Laws in SN Ia Host Galaxies
• The Peculiar Velocity Correlation Function
• A model independent parametrization of the late time cosmic acceleration: constraints on the parameters from recent observations
• Vainshtein Screening in Bimetric Cosmology
• Consistency of local and astrophysical tests of the stability of fundamental constants
• ZTF SN Ia DR2: The spectral diversity of Type Ia supernovae in a volume-limited sample
• A possible solution to the Hubble constant discrepancy -- Cosmology where the local volume expansion is driven by the domain average density
• Origin of high-velocity ejecta and early red excess emission in the infant Type Ia supernova 2021aefx
• Horizon thermodynamics in holographic cosmological models with a power-law term
• Modelling of SN2013dx associated with the low-redshift GRB130702A points to diversity in GRB/SN properties
• Frequency analysis of OGLE-IV photometry for classical Cepheids in Galactic fields: non-radial modes and modulations
• Local probes strongly favor $\Lambda$CDM against power-law and $R_h=ct$ universe
• Hubble Constant from LSST Strong lens time delays with microlensing systematics
• Non-thermal Hot Dark Matter from Inflaton/Moduli Decay: The Momentum Distribution and Relaxing the Cosmological Mass Bound
• Robust Limits from Upcoming Neutrino Telescopes and Implications on Minimal Dark Matter Models
• Cosmological implications of the Weyl geometric gravity theory
• Model-Independent Predictions for Smooth Cosmic Acceleration Scenarios
• Cosmic expansion history from SNe Ia data via information field theory -- the charm code
• Is gravity getting weaker at low z? Observational evidence and theoretical implications
• Observing the dark sector
• Investigating The Hubble Tension Through Hubble Parameter Data
• Probing a light dark sector at future lepton colliders via invisible decays of the SM-like and dark Higgs bosons
• Environmental Dependence of Type Ia Supernovae in Low-Redshift Galaxy Clusters
• Cosmology with Galaxy Cluster Phase Spaces
• Using Gravitational Wave Parallax to Measure the Hubble Parameter with Pulsar Timing Arrays
• Constraining dynamical neutrino mass generation with cosmological data
• Calibrating gravitational-wave detectors with GW170817
• The Hubble tension: Change in dark energy or a case for modified gravity?
• Finding structure in the dark: coupled dark energy, weak lensing, and the mildly nonlinear regime
• Imprint of thawing scalar fields on large scale galaxy overdensity
• Stability analysis of warm quintessential dark energy model
• Integrated cosmological probes: Concordance quantified
• Observational status of the Galileon model general solution from cosmological data and gravitational waves
• Forecast on lepton asymmetry from future CMB experiments
• Distances to Local Group Galaxies via Population II, Stellar Distance Indicators. II. The Fornax Dwarf Spheroidal
• Thermonuclear Supernovae: Prospecting in the Age of Time-Domain and Multi-Wavelength Astronomy
• Cosmological Constraints on Scalar Field Dark Matter
• 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
• Calibrating Long Period Variables as Standard Candles with Machine Learning
• Unveiling the Hubble Constant through Galaxy Cluster Gas Mass Fractions
• Ensemble Average Theory of Gravity
• The cosmology dependence of the concentration-mass-redshift relation
• Probing alternative cosmologies through the inverse distance ladder
• Constraints on interacting dynamical dark energy and a new test for $\Lambda$CDM
• Structure Formation in Nonlocal MOND
• Modified majoron model for cosmological anomalies
• Predictions for the sky-averaged depth of the 21cm absorption signal at high redshift in cosmologies with and without non-baryonic cold dark matter
• Constraints on brane inflation after Planck 2015: Impacts of the latest local measurement of the Hubble constant
• Revisiting the epoch of cosmic acceleration
• Theoretical analysis of surface brightness-colour relations for late-type stars using MARCS model atmospheres
• Impact of the latest measurement of Hubble constant on constraining inflation models
• Cosmic Time Slip: Testing Gravity on Supergalactic Scales with Strong-Lensing Time Delays
• Observational constraints on the fractal cosmology
• Imprint of a Steep Equation of State in the growth of structure
• Band-limited Features in the Primordial Power Spectrum Do Not Resolve the Hubble Tension
• Cosmological phase transitions, gravitational waves and self-interacting dark matter in the singlet extension of MSSM
• AlFoCS + F3D II: unexpectedly low gas-to-dust ratios in the Fornax galaxy cluster
• Constraining the emergent dark energy models with observational data at intermediate redshift
• Resolving the Excess of Long GRBs at low redshift in the Swift Era
• Comparing the luminosity distance for gravitational waves and electromagnetic signals in a simple model of quadratic gravity
• Non-thermally trapped inflation by tachyonic dark photon production
• Brightest stars of irregular and low-massive spiral galaxies
• The Integrated Sachs-Wolfe Effect in the Bulk Viscous Dark Energy Model
• Will Gravitational Wave Sirens Determine the Hubble Constant?
• The background Friedmannian Hubble constant in relativistic inhomogeneous cosmology and the age of the Universe
• Towards detecting super-GeV dark matter via annihilation to neutrinos
• Wolf-Rayet stars in the Antennae unveiled by MUSE
• SU(2)${}_{\mathrm{CMB}}$ and the cosmological model: angular power spectra
• Young and Intermediate-age Distance Indicators
• Decaying dark energy in light of the latest cosmological dataset
• Mitigating the binary viewing angle bias for standard sirens
• Coordinated JWST Imaging of Three Distance Indicators in a SN Host Galaxy and an Estimate of the TRGB Color Dependence
• Prospects for observing strongly lensed supernovae behind Hubble Frontier Fields galaxy clusters with the James Webb Space Telescope
• Impact of distance determinations on Galactic structure. II. Old tracers
• Mathematical Underpinnings of the Multi-Wavelength Structure of the TRGB
• On the cosmological performance of photometrically classified supernovae with machine learning
• Weak gravity on a $\Lambda$CDM background
• Quantum gravity phenomenology at the dawn of the multi-messenger era -- A review
• A modified Friedmann equation for a system with varying gravitational mass
• Interacting dark energy in the dark $SU(2{)}_R$ model
• Cosmological tests of gravity with latest observations
• The interacting vacuum and tensions: a comparison of theoretical models
• Investigating the Hubble Tension: Effect of Cepheid Calibration
• Self-interacting neutrinos, the Hubble parameter tension, and the Cosmic Microwave Background
• Imprint of Early Dark Energy in Stochastic Gravitational Wave Background
• Hubble tension as a window on the gravitation of the dark matter sector: Exploration of a family of models
• Constraints on Dark Matter-Photon Coupling in the Presence of Time-Varying Dark Energy
• Testing backreaction effects with observational Hubble parameter data
• Observational constraints in Delta Gravity: CMB and supernovas
• Probing cosmic anisotropy with GW/FRB as upgraded standard sirens
• Optical Observations of the Nearby Type Ia Supernova 2021hpr
• Simulating time-varying strong lenses
• Constraints on kinematic parameters at $z\ne 0$
• Dark matter perturbations and viscosity: a causal approach
• A study of Si II and S II features in spectra of Type Ia supernova
• Late-time acceleration with steep exponential potentials
• The effective running Hubble constant in SNe Ia as a marker for the dark energy nature
• How to Detect Inclined Water Maser Disks (and Possibly Measure Black Hole Masses)
• New observational constraints on interacting dark energy using galaxy clusters virial equilibrium states
• On the concordance of cosmological data in the case of the generalized Chaplygin gas
• Forecasts for interacting dark energy with time-dependent momentum exchange
• $H_0$ tension or $M$ overestimation?
• Cosmography using strong lensing systems and cosmic chronometers
• An SU(6) GUT Origin of the TeV-Scale Vector-like Particles Associated with the 750 GeV Diphoton Resonance
• Late-time acceleration by a residual cosmological constant from sequestering vacuum energy in ultimate collapsed structures
• One Year of SN 2023ixf: Breaking Through the Degenerate Parameter Space in Light-Curve Models with Pulsating Progenitors
• Dynamical System Analysis of Quintessence Models with Exponential Potential -- Revisited
• Roles of sterile neutrinos in particle physics and cosmology
• Physical condition for the slowing down of cosmic acceleration
• Multistate scalar field dark matter and its correlation with galactic properties
• Diffuse neutrino supernova background as a cosmological test
• A Standard Siren Cosmological Measurement from the Potential GW190521 Electromagnetic Counterpart ZTF19abanrhr
• Towards a 1% Measurement of the Hubble Constant: Accounting for Time Dilation in Variable Star Light Curves
• ASASSN-14lp: two possible solutions for the observed UV suppression
• Covariant formulation of refracted gravity
• PTF11rka: an interacting supernova at the crossroads of stripped-envelope and H-poor super-luminous stellar core collapses
• Gravitational waves, CMB polarization, and the Hubble tension
• Interplay of CMB Temperature, Space Curvature, and Expansion Rate Parameters
• Bound Dark Energy: towards understanding the nature of the Dark Energy
• X-ray Limits on the Progenitor System of the Type Ia Supernova 2017ejb
• Perturbation level interacting dark energy model and its consequence on late-time cosmological parameters
• Reconstructing the Hubble diagram of gamma-ray bursts using deep learning
• Effects of a local physics change on the SH0ES determination of $H_0$
• Rapid onset of the 21-cm signal suggests a preferred mass range for dark matter particle
• Large-Distance Lens Uncertainties and Time-Delay Measurements of $H_0$
• The Hubble constant from two sibling Type Ia supernovae in the nearby galaxy NGC 4414: SN 1974G and SN 2021J
• Accurate spectroscopic redshift of the multiply lensed quasar PSOJ0147 from the Pan-STARRS survey
• The gravitational and lensing-ISW bispectrum of 21cm radiation
• Constraining neutrino mass and dark energy with peculiar velocities and lensing dispersions of Type Ia supernovae
• A Non-parametric Reconstruction of the Hubble Parameter $H(z)$ Based on Radial Basis Function Neural Networks
• Bayesian Comparison of Interacting Modified Holographic Ricci Dark Energy Scenarios
• A Geometric Calibration of the Tip of the Red Giant Branch in the Milky Way using Gaia DR3
• Cosmological surveys with multi-object spectrographs
• Photometric study of the late-time near-infrared plateau in Type Ia supernovae
• Lagrangian formulation for an extended cosmological equation-of-state
• The dynamics of three nearby E0 galaxies in refracted gravity
• Stress testing the dark energy equation of state imprint on supernova data
• Spatially Homogeneous Teleparallel Gravity: Bianchi I
• Optical photometry and spectroscopy of the low-luminosity, broad-lined Ic supernova iPTF15dld
• The massive star population of the Virgo Cluster galaxy NGC 4535
• Application of Convolutional Neural Networks to time domain astrophysics. 2D image analysis of OGLE light curves
• Constraining Temporal Oscillations of Cosmological Parameters Using Type Ia Supernovae
• Fundamental Physics and Cosmology with TianQin
• A hierarchical Bayesian model to infer PL(Z) relations using Gaia parallaxes
• Are quasars reliable standard candles?
• Cosmological bounds on neutrino statistics
• Determining Cosmological-model-independent $H_0$ with Gravitationally Lensed Supernova Refsdal
• 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
• Eliminating the Hubble Tension in the Presence of the Interconnection between Dark Energy and Matter in the Modern Universe
• Observational Constraint on Spherical Inhomogeneity with CMB and Local Hubble Parameter
• The proper motion of stars in dwarf galaxies: distinguishing central density cusps from cores
• Stephani Cosmology: Entropically Viable But Observationally Challenged
• Astrophysical Distance Scale IV. Preliminary Zero-Point Calibration of the JAGB Method in the HST/WFC3-IR Broad J-Band (F110W) Filter
• Type Ia Supernova Magnitude Step from the local Dark Matter Environment
• The DIVING${}^{3D}$ Survey -- Deep IFS View of Nuclei of Galaxies -- I. Definition and Sample Presentation
• Cosmological Constraints using the newest VLT-KMOS HII Galaxies and the full Planck CMB spectrum
• RAiSERed: radio continuum redshifts for lobed AGNs
• Evolution of dissipative and non-dissipative universes in holographic cosmological models with a power-law term
• New insights into the use of Ultra Long Period Cepheids as cosmological standard candles
• Identifying Candidate Optical Variables Using Gaia Data Release 2
• de Sitter duality and logarithmic decay of dark energy
• Light curve properties of SN 2017fgc and HV SNe Ia
• New classical Cepheids in the inner part of the northern Galactic disk and their kinematics
• Probing dark energy using convergence power spectrum and bi-spectrum
• High-velocity feature as the indicator of the stellar population of Type Ia supernovae
• Parameters of the Link between the Optical and Radio Frames from Gaia DR2 Data and VLBI Measurements
• High accuracy on $H_0$ constraints from gravitational wave lensing events
• Dust Extinction towards the Type Ia Supernova 2012cu in NGC 4772
• SU(2)$_{\tiny\mbox{CMB}}$ at high redshifts and the value of $H_0$
• Hubble law: measure and interpretation
• A Search for Mass Loss on the Cepheid Instability Strip using HI 21-cm Line Observations
• Toward a more stringent test of gravity with redshift space power spectrum: simultaneous probe of growth and amplitude of large-scale structure
• Precise peculiar velocities from gravitational waves accompanied by electromagnetic signals and cosmological applications
• Early dark energy constraints on growing neutrino quintessence cosmologies
• Unveiling the Universe with Emerging Cosmological Probes
• Clifford algebra Cl(0,6) approach to beyond the standard model and naturalness problems
• On Dark Energy and Quantum Gravity
• Statistical analysis with cosmic-expansion-rate measurements and two-point diagnostics
• Dark matter physics in neutrino specific two Higgs doublet model
• A closer look at the quadruply lensed quasar PSOJ0147: spectroscopic redshifts and microlensing effect
• Emergent gravity fails to explain color-dependent galaxy-galaxy lensing signals from SDSS Dr7
• Degeneracy between nonadiabatic dark energy models and $\Lambda$CDM: ISW effect and the cross correlation of CMB with galaxy clustering data
• Covariant Decomposition of The Non-Linear Galaxy Number Counts and Their Monopole
• Revisiting model-independent constraints on spatial curvature and cosmic ladders calibration: updated and forecast analyses
• Exploring the distance-redshift relation with gravitational wave standard sirens and tomographic weak lensing
• Testing the phenomenological interacting dark energy model with gamma-ray bursts and Pantheon+ type Ia supernovae
• Impact of calibration uncertainties on Hubble constant measurements from gravitational-wave sources
• Calibrating the surface brightness - color relation for late-type red giants stars in the visible domain using VEGA/CHARA interferometric observations
• Variability in Quasar Light Curves: using quasars as standard candles
• The Observable Supernova Rate in Galaxy-Galaxy Lensing Systems with the TESS Satellite
• Non-linear Structure Formation for Dark Energy Models with a Steep Equation of State
• An Informational Approach to Cosmological Parameter Estimation
• Strongly Lensed Supernovae in Well-Studied Galaxy Clusters with the Vera C. Rubin Observatory
• Tests of photometry: the case of the NGC 3370 ACS field
• A More Accurate and Competitive Estimative of $H_0$ in Intermediate Redshifts
• SN 2016B a.k.a ASASSN-16ab: a transitional type II supernova
• Revealing the progenitor of SN 2021zby through analysis of the $TESS$ shock-cooling light curve
• Hubble tension and matter inhomogeneities: a theoretical perspective
• The Galaxy Halo Connection in Modified Gravity Cosmologies: Environment Dependence of Galaxy Luminosity function
• Scalar-tensor extension of the $\Lambda$CDM model
• Non-parametric Cosmology with Cosmic Shear
• Application of the FRADO model of BLR formation to the Seyfert galaxy NGC 5548 and the first step toward determining the Hubble constant
• Thermodynamic and observational constraints on black holes with primary hair in Beyond Horndeski Gravity: Stability and shadows
• Cosmological Dynamics in Interacting Scalar-Torsion f(T,$\varphi$) Gravity: Investigating Energy and Momentum Couplings
• Synthetic Population of Binary Cepheids. II. The effect of companion light on the extragalactic distance scale
• H-band light curves of Milky Way Cepheids via Difference Imaging
• Evaluating backreaction with the ellipsoidal collapse model
• Model-Independent Reconstruction of Quintessence Potential and Kinetic Energy from DESI DR2 and Pantheon+ Supernovae
• Revisiting kink-like parametrization and constraints using OHD/Pantheon+/BAO samples
• Holographic dark energy satisfying the energy conditions in Lovelock gravity
• A New Parameterized Interacting Holographic Dark Energy
• On the cosmological gravitational waves and cosmological distances
• Dynamic Dark Energy Equation of State (EoS) and Hubble Constant analysis using type Ia supernovae from Union 2.1 dataset
• Galaxy rotation curves and the deceleration parameter in weak gravity
• Estimating Hubble Constant with Gravitational Observations: A Concise Review
• Stellar photometry with Multi Conjugate Adaptive Optics
• Phantom Dirac-Born-Infeld Dark Energy
• How are Lyman $\alpha$ absorbers in the cosmic web related to gas-rich galaxies?
• A comprehensive data-driven odyssey to explore the equation of state of dark energy
• Cosmography of the minimally extended Varying Speed of Light Model
• Traversable wormholes in bi-metric gravity
• Radio Observations of Six Young Type Ia Supernovae
• The time delay of JVAS B1030+074 from VLA polarization monitoring
• Global asymptotic dynamics of the cubic galileon interacting with dark matter
• On the Paradoxical Impact of Blending by Red Clump Giants
• ZTF SN Ia DR2: Properties of the low-mass host galaxies of Type Ia supernovae in a volume-limited sample
• An SU(2) gauge principle for the Cosmic Microwave Background: Perspectives on the Dark Sector of the Cosmological Model
• Climbing out of the shadows: building the distance ladder with black hole images
• Time-Series Surveys and Pulsating Stars: The Near-Infrared Perspective
• M31 PAndromeda Cepheid sample observed in four HST bands
• All-sky angular power spectra from cleaned WISE$\times$SuperCOSMOS galaxy number counts
• Period-Colour and Amplitude-Colour relations for OGLE-$\delta$ Scuti stars in the Galactic Bulge and LMC
• Prospects of probing dark energy with eLISA: Standard versus null diagnostics
• Intensity mapping of post-reionization 21-cm signal and its cross-correlations as a probe of $f(R)$ gravity
• Observational constraints on viscous cosmology in $f(T,L_m)$ gravity
• Dynamics of cosmological perturbations in modified Brans-Dicke cosmology with matter-scalar field interaction
• Fluctuating Dark Energy and the Luminosity Distance
• Impact of AGN and nuclear star formation on the ISM turbulence of galaxies: Insights from JWST/MIRI spectroscopy
• Constraining late-time transitions in the dark energy equation of state
• Bayesian analysis of running holographic Ricci dark energy
• A Hubble Constant Determination Through Quasar Time Delays and Type Ia Supernovae
• The Carnegie-Chicago Hubble Program: Calibration of the Near-Infrared RR Lyrae Period-Luminosity Relation With HST
• Sub-MeV Bosonic Dark Matter, Misalignment Mechanism and Galactic Dark Matter Halo Luminosities
• Gravitational wave probes of Barrow cosmology with LISA standard sirens
• Growth of cosmic perturbations in the modified $f(R,T)$ gravity
• Dequantization of electric charge: Probing scenarios of cosmological multi-component dark matter
• Locally-homogeneous Riemann-Cartan geometries with the largest symmetry group
• Probing Quintessence using BAO imprint on the cross-correlation of weak lensing and post-reionization HI 21 cm signal
• Signature of the interaction between dark sectors in the reionization process
• Observational tests of the Glavan, Prokopec and Starobinsky model of dark energy
• Barrow holographic dark energy interacting model in the presence of radiation and matter
• Measuring the velocity field from type Ia supernovae in an LSST-like sky survey
• The art of building a smooth cosmic distance ladder in a perturbed universe
• On the convergence of cosmographic expansions in Lemaitre-Tolman-Bondi models
• Fine-structure constant constraints on late-time dark energy transitions
• Voids and Halos in Voids statistics as a probe of the Expansion History of the Universe
• An Accelerating Universe without Lambda: Delta~Gravity Using Monte Carlo
• Performance of Non-Parametric Reconstruction Techniques in the Late-Time Universe
• The $\Lambda$ to zero limit of spacetimes and its physical interpretation
• Measuring neutrino mass imprinted on the anisotropic galaxy clustering
• On the Metric $f(R)$ gravity Viability in Accounting for the Binned Supernovae Data
• A multiwavelength study of the flat spectrum radio-quasar NVSS J141922-083830 covering four flaring episodes
• Local Limit of Nonlocal Gravity: Cosmological Perturbations
• Predicting extragalactic distance errors using Bayesian inference in multi-measurement catalogs
• Period Variations for the Cepheid VZ Cyg
• New active galactic nuclei science cases with interferometry: An incomplete preview
• Using Neutrino Oscillations to Measure $H_0$
• New measures to test modified gravity cosmologies
• The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch
• Modified $f(R,T)$ theory in light of gravitational wave standard sirens
• Anisotropic power-law inflation for a generalized model of two scalar and two vector fields
• Dynamical System Analysis for Scalar Field Potential in Teleparallel Gravity
• Reconstruction of energy conditions from observations and implications for extended theories of gravity
• Non-Parametric Analysis for the Dark Matter Density Evolution
• Data Analysis and Phenomenological Cosmology
• Clustering of Local Group distances: publication bias or correlated measurements? VII. A distance framework out to 100 Mpc
• On the intrinsically flat cosmological models in a lattice
• A quintessence dynamical dark energy model from ratio gravity
• Towards a new proposal for the time delay in gravitational lensing
• Perspectives of a visible instrument on the VLTI
• Cosmological Standard Timers from Unstable Primordial Relics
• Interacting dark sector with quadratic coupling: theoretical and observational viability
• Considering light-matter interactions in the Friedmann equations
• Projected two- and three-point statistics: Forecasts and mitigation of non-linear RSDs
• Influence of the correlation prior on reconstruction of the dark energy equation of state
• Testing the coupling of dark radiations in light of the Hubble tension
• Cosmic acceleration in asymptotically Ricci flat Universe
• Dynamical Symmetry Breaking and Negative Cosmological Constant
• Deep Extragalactic VIsible Legacy Survey (DEVILS): DR1 Blended Spectra Search for Candidate Strong Gravitational Lenses
• Cosmic Kite: Auto-encoding the Cosmic Microwave Background
• A joint 1% calibration of the RR Lyrae & type-II Cepheid Leavitt laws yields homogeneous distances to 93 Galactic globular clusters
• Tracking Pre-inflation Era from density perturbation spectra
• Probing the independence within the dark sector in the fluid approximation
• Dynamics and chaos in the unified scalar field cosmology II. System in a finite box
• The Use of Binary Black Holes Merging in AGN Disks for Hubble Constant Measurements
• Inflation of the Universe by the Non-minimal $Y(R)F^2$ Models
• Long Journey toward the Detection of Gravitational Waves and New Era of Gravitational Wave Astrophysics
• The Ambiguity in the Definition and Behavior of the Gravitational and Cosmological `Coupling Constants' in the Theory of Induced Gravity
• Thermo-Coupled Early Dark Energy
• Ultra Long Period Cepheids as standard candles from Gaia to Rubin-LSST
• Unified Dark Energy and Dark Matter from Dynamical Spacetime Cosmology
• Binary Neutron Star (BNS) merger: What we learned from relativistic ejecta of GW/GRB~170817A
• Exploring thermodynamics inconsistencies in unimodular gravity: a comparative study of two energy diffusion functions
• Wormholes in a viscous universe
• An Introduction to the Planck Mission
• Observational Constraints on the Cosmology with Holographic Dark Fluid
• Reconciling cosmic dipolar tensions with a gigaparsec void
• Vainshtein screening in Horndeski theories nonminimally and kinetically coupled to ordinary matter
• First Detection of Radio Emission Associated with a Classical Cepheid
• Uncovering the truth about M101, NGC 3938, and their significant others through radiative transfer
• Emergence of smooth distance and apparent magnitude in a lumpy Universe
• A MUSE view of the multiple interacting system HCG 31
• Unimodular Theory of Gravity in Light of the Latest Cosmological Data
• Six Maxims of Statistical Acumen for Astronomical Data Analysis
• Testing Exponential $f(R)$ Gravity with CMB, DESI-DR2, and Supernova Data
• A Joint Analysis of Strong Lensing and Type Ia Supernovae to Determine the Hubble Constant
• Cepheid Metallicity in the Leavitt Law (C-MetaLL) survey: IX. Metallicity dependence of Period-Wesenheit relations based on a homogeneous spectroscopic sample
• Observational constraints on generic models of non-minimal curvature-matter coupling
• A Review on Resolving the Hubble Tension via Late-Universe Physics
• Testing Lens Models of PLCK G165.7+67.0 Using Lensed SN H0pe
• Observational tests of the conformal osculating Barthel-Kropina cosmological model
• Is the Hubble Constant Scale-dependent?
• Accounting for Correlations When Fitting Extra Cosmological Parameters
• Constraining disformal couplings with Redshift Space Distortion
• Toward a Measurement of the Transverse Peculiar Velocity of Galaxy Pairs
• Evolution of perturbations in a universe with exotic solid-like matter
• The snapshot distance method: estimating the distance to a Type Ia supernova from minimal observations
• An Alcock-Paczynski Test on Reionization Bubbles for Cosmology
• Coordinate independent approach to the calculation of the effects of local structure on the luminosity distance
• Constraining Violations of the Weak Equivalence Principle in the Dark Sector
• Space-based Gravitational Wave Observatories
• Toward Cosmological Standard Timers in Primordial Black Hole Binaries
• Multiwavelength Light Curve Parameters of Cepheid Variables
• Cepheids with the eyes of photometric space telescopes
• Vacuum arbitrariness and the Hubble tension
• Momentum transfer models of interacting dark energy
• Interacting Quintessence and Growth of Structure
• Reference frame dependence of the local measurement of the Hubble constant
• Impact of Large-Scale Structure along Line-of-Sight on Time-Delay Cosmography
• On observational signatures of multi-fractional theory
• A semi-cosmographic approach to study cosmological evolution in phase space
• Large-Scale Surveys of Pulsating Stars for Studying Stellar Populations in the Inner Galaxy
• Forecasts on Interacting Dark Energy from 21-cm Angular Power Spectrum with BINGO and SKA observations
• Nuclear fission reaction simulations in compact stars
• Does History Repeat Itself? Periodic Time Cosmology
• Faint galaxies in the Zone of Avoidance revealed by JWST/NIRCam
• Correlation of structure growth index with current cosmic acceleration: constraints on dark energy models
• Cosmological constant as a finite temperature effect
• Multiwavelength light curve analysis of Cepheid variables
• Testing $\Lambda$CDM with eBOSS data using a model independent diagnostic
• Analysis of the angular dependence of time delay in gravitational lensing
• Normal or transitional? The evolution and properties of two type Ia supernovae in the Virgo cluster
• The DESI DR1 Peculiar Velocity Survey: global zero-point and $H_0$ constraints
• Dark sector interactions in the $w\to -1$ limit: velocity locking in pure momentum exchange models
• Toward a renewed Galactic Cepheid distance scale from Gaia and optical interferometry
• Getting the Most Neutrinos out of IsoDAR
• Thermodynamics of sign-switching dark energy models
• Forward-modelling Milky Way Cepheids: selection effects and physical priors in the Gaia-HST calibration
• Constraint on Neutrino Statistics from Cosmological Data
• Study of Integrated Spectra of Four Globular Clusters in M31
• Kinematical models of latetime cosmology and the statefinder diagnostic
• Implications of single field inflation in general cosmological scenarios on the nature of dark energy given the swampland conjectures
• Observational constraints on the free parameters of an interacting Bose-Einstein gas as a dark-energy model
• Decaying Dark Matter: Simulations and Weak-Lensing Forecast
• Cosmic Microwave Background as a thermal gas of SU(2) photons: Implications for the high-z cosmological model and the value of $H_0$
• Hubble Tension and Gravitational Self-Interaction
• SU(2) Yang-Mills thermodynamics: a priori estimate and radiative corrections
• Correlated gravitational wave and microlensing signals of macroscopic dark matter
• Cepheid Metallicity in the Leavitt Law (C--MetaLL) survey: VIII. High-Resolution IGRINS Spectroscopy of 23 Classical Cepheids: Validating NIR Abundances
• Near-infrared observations of OGLE classical and type II Cepheid variables in the LMC
• Holographic dark energy in Einstein-Cartan spin cosmology
• Void spin distribution as a powerful probe of ${\sigma }_8$
• Finding Fast Transients in Real Time Using Novel Light Curve Analysis Algorithm
• San Pedro Meeting on Wide Field Variability Surveys: Some Concluding Comments
• Extragalactic Supergiants
• Variable stars in the Gaia era: Mira, RR Lyrae, delta and Type-II Cepheids
• Sample Variance for Supernovae Distance Measurements and the Hubble tension
• Effect of primary scalar hair on black hole's strong lensing in Beyond Horndeski Gravity
• Probing dark energy using anisotropies in the clustering of post-EoR HI distribution
• Fully Relativistic Derivation of the Thermal Sunyaev-Zel'dovich Effect
• 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
• Constraining runaway dilaton models using joint gravitational-wave and electromagnetic observations
• Genetic algorithm demystified for cosmological parameter estimation
• The dynamics of background evolution and structure formation in phase space: a semi-cosmographic reconstruction
• Systematic and Statistical Uncertainties in Cepheid PL Relations: Incorporating a Cross-Filter Random-Phase Mitigation Approach
• Evolution of superhorizon perturbations in early Universe with anisotropic solid remnant
• Cosmological evolution driven by polytropic fluids in an inhomogeneous spacetime
• Extra-galactic distances with massive stars: the role of stellar variability in the case of M33
• Yellow Post-Asymptotic-Giant-Branch Stars as Standard Candles. I. Calibration of the Luminosity Function in Galactic Globular Clusters
• Dark Matter profiles of "in silico" galaxies: deep learning inference
• Solid matter with zero shear modulus in flat universe
• Time Delay Cosmography: Analysis of Quadruply Lensed QSO SDSSJ1433 from Wendelstein Observatory
• Asymptotic Giant Branch Variables in Nearby Galaxies
• Exploring the constraints on cosmological models with CosmoEJS
• The BINGO project X. Cosmological parameter constraints from HI Intensity Mapping lognormal simulations
• Universality of the halo mass function in modified gravity cosmologies
• The Role of Gravitational Energy Flux in Cosmic Acceleration
• Prospects of the multi-channel photometric survey telescope in the cosmological application of Type Ia supernovae
• Evolution of matter perturbations in the context of cosmic slowing down
• Shadows of naked singularities and superspinars related to the revisited Kerr-de Sitter spacetimes
• Redshift Duality with Pantheon+SH0ES in a Planck-anchored Flat $\Lambda$CDM Framework: Implications for Hubble Tension and Observational Inference
• SN 2021pfs: A Type Ia Supernova Likely Affected by Progenitor Metallicity, as Revealed by Comparison with Its Twin Counterpart
• Primordial gravitational waves spectrum in the interacting Bose-Einstein gas model
• Hubble tension problem encompassed by phase-space quantum cosmology
• Constraints on energy scales from dark matter decay in a gauged $B-L$ model
• Observations of Field and Cluster RR Lyrae with Spitzer. Towards High Precision Distances with Population II Stellar Tracers
• Running Einstein Constant and a Possible Vacuum State of the Universe
• The impact of the locally measured Hubble parameter on the mass of Sterile neutrino