The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample

Abstract

We present optical light curves, redshifts, and classifications for 365 spectroscopically confirmed Type Ia supernovae (SNe Ia) discovered by the Pan-STARRS1 (PS1) Medium Deep Survey. We detail improvements to the PS1 SN photometry, astrometry and calibration that reduce the systematic uncertainties in the PS1 SN Ia distances. We combine the subset of 279 PS1 SN Ia ($0.03<z<0.68$) with useful distance estimates of SN Ia from SDSS, SNLS, various low-z and HST samples to form the largest combined sample of SN Ia consisting of a total of 1048 SN Ia ranging from $0.01<z<2.3$, which we call the `Pantheon Sample'. When combining Planck 2015 CMB measurements with the Pantheon SN sample, we find ${\Omega }_m=0.307\pm 0.012$ and $w=-1.026\pm 0.041$ for the wCDM model. When the SN and CMB constraints are combined with constraints from BAO and local H0 measurements, the analysis yields the most precise measurement of dark energy to date: $w0=-1.007\pm 0.089$ and $wa=-0.222\pm 0.407$ for the w0waCDM model. Tension with a cosmological constant previously seen in an analysis of PS1 and low-z SNe has diminished after an increase of $2\times$ in the statistics of the PS1 sample, improved calibration and photometry, and stricter light-curve quality cuts. We find the systematic uncertainties in our measurements of dark energy are almost as large as the statistical uncertainties, primarily due to limitations of modeling the low-redshift sample. This must be addressed for future progress in using SN Ia to measure dark energy.

arXiv commentAccepted by ApJ. Data can be found here: http://dx.DOI.org/10.17909/T95Q4X

References in corpus (108)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
• Planck 2015 results. XIII. Cosmological parameters
• Measuring Reddening with SDSS Stellar Spectra and Recalibrating SFD
• Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
• Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
• Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
• Cosmological parameters from CMB and other data: a Monte-Carlo approach
• Correcting for the Effects of Interstellar Extinction
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
• The Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III
• The Supernova Legacy Survey: Measurement of Omega_M, Omega_Lambda and w from the First Year Data Set
• A 2.4% Determination of the Local Value of the Hubble Constant
• Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples
• The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
• New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy
• The Hubble Space Telescope Cluster Supernova Survey: V. Improving the Dark Energy Constraints Above z>1 and Building an Early-Type-Hosted Supernova Sample
• Wide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report
• The Pan-STARRS1 Photometric System
• Observational Constraints on the Nature of the Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey
• Improved Dark Energy Constraints from ~100 New CfA Supernova Type Ia Light Curves
• Supernova Constraints and Systematic Uncertainties from the First 3 Years of the Supernova Legacy Survey
• Improved Distances to Type Ia Supernovae with Multicolor Light Curve Shapes: MLCS2k2
• BVRI Light Curves for 22 Type Ia Supernovae
• The Pan-STARRS1 Surveys
• First-year Sloan Digital Sky Survey-II (SDSS-II) Supernova Results: Hubble Diagram and Cosmological Parameters
• The Supernova Legacy Survey 3-year sample: Type Ia Supernovae photometric distances and cosmological constraints
• CfA3: 185 Type Ia Supernova Light Curves from the CfA
• The Sloan Digital Sky Survey-II Supernova Survey: Technical Summary
• SNLS3: Constraints on Dark Energy Combining the Supernova Legacy Survey Three Year Data with Other Probes
• The Dependence of Type Ia Supernova Luminosities on their Host Galaxies
• Hectospec, the MMT's 300 Optical Fiber-Fed Spectrograph
• Photometric Calibration of the First 1.5 Years of the Pan-STARRS1 Survey
• UBVRI Light Curves of 44 Type Ia Supernovae
• Planck 2015 results. XIV. Dark energy and modified gravity
• Hubble Residuals of Nearby Type Ia Supernovae Are Correlated with Host Galaxy Masses
• The Carnegie Supernova Project: First Photometry Data Release of Low-Redshift Type Ia Supernovae
• Photometric Response Functions of the SDSS Imager
• Cosmological Constraints from Measurements of Type Ia Supernovae discovered during the first 1.5 years of the Pan-STARRS1 Survey
• The Carnegie Supernova Project: Analysis of the First Sample of Low-Redshift Type-Ia Supernovae
• The Pan-STARRS 1 Photometric Reference Ladder, Release 12.0
• SNANA: A Public Software Package for Supernova Analysis
• The ESSENCE Supernova Survey: Survey Optimization, Observations, and Supernova Photometry
• Pan-STARRS Photometric and Astrometric Calibration
• The Carnegie Supernova Project: Light Curve Fitting with SNooPy
• The Effect of Host Galaxies on Type Ia Supernovae in the SDSS-II Supernova Survey
• The Carnegie Supernova Project: Second Photometry Data Release of Low-Redshift Type Ia Supernovae
• Cosmological parameters from the comparison of peculiar velocities with predictions from the 2M++ density field
• Correcting Type Ia Supernova Distances for Selection Biases and Contamination in Photometrically Identified Samples
• Type Ia Supernova Distances at z > 1.5 from the Hubble Space Telescope Multi-Cycle Treasury Programs: The Early Expansion Rate
• Correlated Fluctuations in Luminosity Distance and the (Surprising) Importance of Peculiar Motion in Supernova Surveys
• CfA4: Light Curves for 94 Type Ia Supernovae
• Evidence of Environmental Dependencies of Type Ia Supernovae from the Nearby Supernova Factory indicated by Local Hα
• Testing LMC Microlensing Scenarios: The Discrimination Power of the SuperMACHO Microlensing Survey
• The Data Release of the Sloan Digital Sky Survey-II Supernova Survey
• Techniques and Review of Absolute Flux Calibration from the Ultraviolet to the Mid-Infrared
• The Sloan Digital Sky Survey-II: Photometry and Supernova Ia Light Curves from the 2005 data
• Simulations of the WFIRST Supernova Survey and Forecasts of Cosmological Constraints
• Type Ia Supernova Rate Measurements to Redshift 2.5 from CANDELS : Searching for Prompt Explosions in the Early Universe
• The MagE Spectrograph
• Type Ia Supernova Light Curve Inference: Hierarchical Models in the Optical and Near Infrared
• Nearby Supernova Rates from the Lick Observatory Supernova Search. I. The Methods and Database
• Type-Ia Supernova Rates to Redshift 2.4 from CLASH: the Cluster Lensing And Supernova survey with Hubble
• Systematic Uncertainties Associated with the Cosmological Analysis of the First Pan-STARRS1 Type Ia Supernova Sample
• The Difference Imaging Pipeline for the Transient Search in the Dark Energy Survey
• Streaming motions of galaxy clusters within 12000 km/s - V. The peculiar velocity field
• The Pan-STARRS Data Processing System
• Measuring Ejecta Velocity Improves Type Ia Supernova Distances
• An Early Warning System for Asteroid Impact
• Pan-STARRS Pixel Processing: Detrending, Warping, Stacking
• The Foundation Supernova Survey: Motivation, Design, Implementation, and First Data Release
• Testing $\Lambda$CDM at the lowest redshifts with SN Ia and galaxy velocities
• Photometric redshifts from evolutionary synthesis with PEGASE: the code ZPEG and the z=0 age constraint
• Measuring Dark Energy Properties with Photometrically Classified Pan-STARRS Supernovae. II. Cosmological Parameters
• The reddening law of Type Ia Supernovae: separating intrinsic variability from dust using equivalent widths
• Marginal evidence for cosmic acceleration from Type Ia supernovae
• Supercal: Cross-Calibration of Multiple Photometric Systems to Improve Cosmological Measurements with Type Ia Supernovae
• A Non Parametric Model for the Cosmic Velocity Field
• A blinded determination of $H_0$ from low-redshift Type Ia supernovae, calibrated by Cepheid variables
• Ages of Type Ia Supernovae Over Cosmic Time
• The Host Galaxies of Type Ia Supernovae Discovered by the Palomar Transient Factory
• Figure of Merit for Dark Energy Constraints from Current Observational Data
• Pan-STARRS Pixel Analysis : Source Detection and Characterization
• Improved Photometric Calibration of the SNLS and the SDSS Supernova Surveys
• A More General Model for the Intrinsic Scatter in Type Ia Supernova Distance Moduli
• Hypercalibration: A Pan-STARRS1-based recalibration of the Sloan Digital Sky Survey
• Measuring Type Ia Supernova Populations of Stretch and Color and Predicting Distance Biases
• Dependence of Type Ia supernova luminosities on their local environment
• Constraints on dark energy with the LOSS SN Ia sample
• Testing Models of Intrinsic Brightness Variations in Type Ia Supernovae, and their Impact on Measuring Cosmological Parameters
• Constraining dark matter halo properties using lensed SNLS supernovae
• Color Dispersion and Milky Way Reddening Among Type Ia Supernovae
• Apparent cosmic acceleration from type Ia supernovae
• Is the expansion of the universe accelerating? All signs point to yes
• Cosmological Parameter Uncertainties from SALT-II Type Ia Supernova Light Curve Models
• The Type Ia Supernova Color-Magnitude Relation and Host Galaxy Dust: A Simple Hierarchical Bayesian Model
• The Fundamental Metallicity Relation Reduces Type Ia SN Hubble Residuals More Than Host Mass Alone
• Measuring the Properties of Dark Energy with Photometrically Classified Pan-STARRS Supernovae. I. Systematic Uncertainty from Core-Collapse Supernova Contamination
• Photometry of supernovae in an image series : methods and application to the Supernova Legacy Survey (SNLS)
• Type Ia Supernova Colors and Ejecta Velocities: Hierarchical Bayesian Regression with Non-Gaussian Distributions
• The Changing Fractions of Type Ia Supernova NUV-Optical Subclasses with Redshift
• Assessment of Systematic Chromatic Errors that Impact Sub-1% Photometric Precision in Large-Area Sky Surveys
• Light Curves of 213 Type Ia Supernovae from the ESSENCE Survey
• Sampling the Probability Distribution of Type Ia Supernova Lightcurve Parameters in Cosmological Analysis
• Search For Type Ia Supernova NUV-Optical Subclasses

Cited by in corpus (1722)

• A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team
• In the Realm of the Hubble tension $-$ a Review of Solutions
• Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory
• The Pantheon+ Analysis: Cosmological Constraints
• Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
• H0LiCOW XIII. A 2.4% measurement of $H_0$ from lensed quasars: $5.3\sigma$ tension between early and late-Universe probes
• The Pantheon+ Analysis: The Full Dataset and Light-Curve Release
• Challenges for $\Lambda$CDM: An update
• The Zwicky Transient Facility: Science Objectives
• The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch
• Cosmic Distances Calibrated to 1% Precision with Gaia EDR3 Parallaxes and Hubble Space Telescope Photometry of 75 Milky Way Cepheids Confirm Tension with LambdaCDM
• KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints
• The Hubble Hunter's Guide
• 2020 Global reassessment of the neutrino oscillation picture
• Planck evidence for a closed Universe and a possible crisis for cosmology
• Measurements of the Hubble Constant: Tensions in Perspective
• On the Cosmological Implications of the String Swampland
• Cosmology Intertwined II: The Hubble Constant Tension
• Teleparallel Gravity: From Theory to Cosmology
• New physics in light of the $H_0$ tension: an alternative view
• The $H_0$ Olympics: A fair ranking of proposed models
• A 2 per cent Hubble constant measurement from standard sirens within 5 years
• Non-minimal dark sector physics and cosmological tensions
• Observational constraints of $f(Q)$ gravity
• Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Modeling Uncertainty
• On the Hubble constant tension in the SNe Ia Pantheon sample
• Dark Energy Survey Year 1 Results: Constraints on Extended Cosmological Models from Galaxy Clustering and Weak Lensing
• TDCOSMO IV: Hierarchical time-delay cosmography -- joint inference of the Hubble constant and galaxy density profiles
• Cluster Cosmology Constraints from the 2500 deg${}^2$ SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Baryon acoustic oscillations with Lyman-$\alpha$ forests
• Cosmology with the Laser Interferometer Space Antenna
• Oscillating scalar fields and the Hubble tension: a resolution with novel signatures
• Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension
• Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions
• Early Dark Energy Does Not Restore Cosmological Concordance
• The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
• Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances and Weak Lensing
• First Cosmology Results using Type Ia Supernovae from the Dark Energy Survey: Constraints on Cosmological Parameters
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from the anisotropic power spectrum of the Quasar sample between redshift 0.8 and 2.2
• To H0 or not to H0?
• Acoustic Dark Energy: Potential Conversion of the Hubble Tension
• Cosmic microwave background bounds on primordial black holes including dark matter halo accretion
• Is the Observable Universe Consistent with the Cosmological Principle?
• The First Three Seconds: a Review of Possible Expansion Histories of the Early Universe
• $H_0$ from cosmic chronometers and Type Ia supernovae, with Gaussian Processes and the novel Weighted Polynomial Regression method
• Baryon acoustic oscillations from the cross-correlation of Ly$\alpha$ absorption and quasars in eBOSS DR14
• Resolving the Hubble Tension with New Early Dark Energy
• Limits on stellar-mass compact objects as dark matter from gravitational lensing of type Ia supernovae
• Baryon acoustic oscillations at z = 2.34 from the correlations of Ly$\alpha$ absorption in eBOSS DR14
• Local determination of the Hubble constant and the deceleration parameter
• A standard siren measurement of the Hubble constant from GW170817 without the electromagnetic counterpart
• Sounds Discordant: Classical Distance Ladder & $\Lambda$CDM -based Determinations of the Cosmological Sound Horizon
• First Cosmological Results using Type Ia Supernovae from the Dark Energy Survey: Measurement of the Hubble Constant
• Is the Hubble tension a hint of AdS phase around recombination?
• On the evolution of the Hubble constant with the SNe Ia Pantheon Sample and Baryon Acoustic Oscillations: a feasibility study for GRB-cosmology in 2030
• The landscape, the swampland and the era of precision cosmology
• Prospects for resolving the Hubble constant tension with standard sirens
• New Early Dark Energy
• Planck 2018 results. VI. Cosmological parameters
• Relieving the Hubble tension with primordial magnetic fields
• Hyper Suprime-Cam Year 3 Results: Cosmology from Cosmic Shear Power Spectra
• Why reducing the cosmic sound horizon alone can not fully resolve the Hubble tension
• A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension
• Evidence for anisotropy of cosmic acceleration
• A buyer's guide to the Hubble Constant
• On the use of the local prior on the absolute magnitude of Type Ia supernovae in cosmological inference
• Hubble Sinks In The Low-Redshift Swampland
• Hubble Space Telescope Observations of Mira Variables in the Type Ia Supernova Host NGC 1559: An Alternative Candle to Measure the Hubble Constant
• Consistency tests of $\Lambda$CDM from the early integrated Sachs-Wolfe effect: Implications for early-time new physics and the Hubble tension
• A Future Percent-Level Measurement of the Hubble Expansion at Redshift 0.8 With Advanced LIGO
• Holographic dark energy through Tsallis entropy
• Can Late Dark Energy Transitions Raise the Hubble constant?
• Modified cosmology from extended entropy with varying exponent
• Revisiting a negative cosmological constant from low-redshift data
• Arbitrating the $S_8$ discrepancy with growth rate measurements from Redshift-Space Distortions
• Accelerated Expansion of the Universe in Non-minimally Coupled Gravity
• Simulations of the WFIRST Supernova Survey and Forecasts of Cosmological Constraints
• Cosmography in $f(Q)$ gravity
• Model-independent reconstruction of $f(Q)$ non-metric gravity
• A non-linear solution to the $S_8$ tension?
• Does Hubble Tension Signal a Breakdown in FLRW Cosmology?
• $H_0$ Tension, Phantom Dark Energy and Cosmological Parameter Degeneracies
• It's Dust: Solving the Mysteries of the Intrinsic Scatter and Host-Galaxy Dependence of Standardized Type Ia Supernova Brightnesses
• Quasars as standard candles III. Validation of a new sample for cosmological studies
• Early dark energy is not excluded by current large-scale structure data
• High-redshift cosmography: auxiliary variables versus Padé polynomials
• General Cosmography Model with Spatial Curvature
• Update on Coupled Dark Energy and the $H_0$ tension
• Limits on $w$CDM from the EFTofLSS with the PyBird code
• Primordial gravitational waves from NANOGrav: a broken power-law approach
• Is there an early Universe solution to Hubble tension?
• Strong gravitational lensing of explosive transients
• The Pantheon+ Analysis: SuperCal-Fragilistic Cross Calibration, Retrained SALT2 Light Curve Model, and Calibration Systematic Uncertainty
• Dark Energy with Phantom Crossing and the $H_0$ tension
• The Foundation Supernova Survey: Motivation, Design, Implementation, and First Data Release
• Updated results on neutrino mass and mass hierarchy from cosmology with Planck 2018 likelihoods
• Observational Properties of Thermonuclear Supernovae
• Robust Preference for Dynamical Dark Energy in DESI BAO and SN Measurements
• Tension with the flat ΛCDM model from a high redshift Hubble Diagram of supernovae, quasars and gamma-ray bursts
• Investigating Cosmic Discordance
• Observational constraints on cosmological solutions of $f(Q)$ theories
• The Local Perspective on the Hubble Tension: Local Structure Does Not Impact Measurement of the Hubble Constant
• Unifying Holographic Inflation with Holographic Dark Energy: a Covariant Approach
• Rock 'n' Roll Solutions to the Hubble Tension
• SALT3: An Improved Type Ia Supernova Model for Measuring Cosmic Distances
• Models and Simulations for the Photometric LSST Astronomical Time Series Classification Challenge (PLAsTiCC)
• Non-parametric spatial curvature inference using late-universe cosmological probes
• Dark Energy in the Swampland
• The Hubble Tension in Light of the Full-Shape Analysis of Large-Scale Structure Data
• Early modified gravity in light of the $H_0$ tension and LSS data
• Final Moments I: Precursor Emission, Envelope Inflation, and Enhanced Mass loss Preceding the Luminous Type II Supernova 2020tlf
• Non-Gaussianity and the induced gravitational wave background
• Holographic dark energy from nonadditive entropy: cosmological perturbations and observational constraints
• A rapid transition of $G_{\mathrm{eff}}$ at $z_t\simeq 0.01$ as a solution of the Hubble and growth tensions
• Relaxing cosmological tensions with a sign switching cosmological constant
• Cosmic acceleration with bulk viscosity in modified $f(Q)$ gravity
• KiDS-1000 Cosmology: constraints beyond flat $\Lambda$CDM
• Tensions in the dark: shedding light on Dark Matter-Dark Energy interactions
• Is Local $H_0$ At Odds With Dark Energy EFT?
• New constraint on Early Dark Energy from Planck and BOSS data using the profile likelihood
• Unified framework for Early Dark Energy from $\alpha$-attractors
• First Cosmology Results Using Type Ia Supernovae From the Dark Energy Survey: Analysis, Systematic Uncertainties, and Validation
• The galaxy power spectrum take on spatial curvature and cosmic concordance
• Cosmological constraints in extended parameter space from the Planck 2018 Legacy release
• A new measurement of the Hubble constant using Type Ia supernovae calibrated with surface brightness fluctuations
• On the most constraining cosmological neutrino mass bounds
• KiDS-1000 Methodology: Modelling and inference for joint weak gravitational lensing and spectroscopic galaxy clustering analysis
• Model independent $H(z)$ reconstruction using the cosmic inverse distance ladder
• New Observational $H(z)$ Data from Full-Spectrum Fitting of Cosmic Chronometers in the LEGA-C Survey
• A larger value for $H_0$ by an evolving gravitational constant
• A model-independent determination of the Hubble constant from lensed quasars and supernovae using Gaussian process regression
• Should Type Ia Supernova Distances be Corrected for their Local Environments?
• Brans-Dicke gravity with a cosmological constant smoothes out $\Lambda$CDM tensions
• Scant evidence for thawing quintessence
• Updated Bounds on Sum of Neutrino Masses in Various Cosmological Scenarios
• PISCO: The Pmas/ppak Integral-field Supernova hosts COmpilation
• Constraints on a Bianchi type I spacetime extension of the standard $\Lambda$CDM model
• Revealing Intrinsic Flat $\Lambda$CDM Biases with Standardizable Candles
• The Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) Survey Design, Reductions, and Detections
• Observational constraints on sign-changeable interaction models and alleviation of the $H_0$ tension
• Dark Energy at early times and ACT: a larger Hubble constant without late-time priors
• The SRG/eROSITA all-sky survey: Cosmology constraints from cluster abundances in the western Galactic hemisphere
• Comparing Tip of the Red Giant Branch Distance Scales: An Independent Reduction of the Carnegie-Chicago Hubble Program and the Value of the Hubble Constant
• Avocado: Photometric Classification of Astronomical Transients with Gaussian Process Augmentation
• Baryon acoustic oscillation, Hubble parameter, and angular size measurement constraints on the Hubble constant, dark energy dynamics, and spatial curvature
• Implications for the Hubble tension from the ages of the oldest astrophysical objects
• Cosmic flows in the nearby Universe: new peculiar velocities from SNe and cosmological constraints
• Deep symbolic regression for physics guided by units constraints: toward the automated discovery of physical laws
• Early recombination as a solution to the $H_0$ tension
• Hints of FLRW Breakdown from Supernovae
• Renormalizing the vacuum energy in cosmological spacetime: implications for the cosmological constant problem
• Dependence of Type Ia supernova luminosities on their local environment
• The Pantheon+ Analysis: Evaluating Peculiar Velocity Corrections in Cosmological Analyses with Nearby Type Ia Supernovae
• Constraints on the curvature of the Universe and dynamical dark energy from the Full-shape and BAO data
• Updated constraints on massive neutrino self-interactions from cosmology in light of the $H_0$ tension
• Cosmological constraints from the tomographic cross-correlation of DESI Luminous Red Galaxies and Planck CMB lensing
• The Young Supernova Experiment: Survey Goals, Overview, and Operations
• Cosmological Constraints from Multiple Probes in the Dark Energy Survey
• Using Pantheon and DES supernova, baryon acoustic oscillation, and Hubble parameter data to constrain the Hubble constant, dark energy dynamics, and spatial curvature
• A new method to build the (inverse) distance ladder
• Analyzing the $H_0$ tension in $F(R)$ gravity models
• K2 Observations of SN 2018oh Reveal a Two-Component Rising Light Curve for a Type Ia Supernova
• Cosmology in $f(R,L_m)$ gravity
• A $w-M$ phantom transition at $z_t<0.1$ as a resolution of the Hubble tension
• GAIA Cepheid parallaxes and 'Local Hole' relieve $H_0$ tension
• Cosmography and flat $\Lambda$CDM tensions at high redshift
• Cosmological Perturbation Theory in $f(Q,T)$ Gravity
• Implications of a transition in the dark energy equation of state for the $H_0$ and ${\sigma }_8$ tensions
• First Cosmology Results using Type Ia Supernovae from the Dark Energy Survey: The Effect of Host Galaxy Properties on Supernova Luminosity
• A deep learning approach to cosmological dark energy models
• Density perturbations for running vacuum: a successful approach to structure formation and to the ${\sigma }_8$-tension
• Using quasar X-ray and UV flux measurements to constrain cosmological model parameters
• Negative cosmological constant in the dark sector?
• Relaxing cosmological tensions with a sign switching cosmological constant: Improved results with Planck, BAO, and Pantheon data
• 2021-$H_0$ Odyssey: Closed, Phantom and Interacting Dark Energy Cosmologies
• Hints of Early Dark Energy in Planck, SPT, and ACT data: new physics or systematics?
• Cosmic dissonance: new physics or systematics behind a short sound horizon?
• Bayesian analysis of $f(T)$ gravity using $f{\sigma }_8$ data
• BOSS Correlation Function Analysis from the Effective Field Theory of Large-Scale Structure
• The Foundation Supernova Survey: Measuring Cosmological Parameters with Supernovae from a Single Telescope
• Interacting Dark Energy in a closed universe
• Probing observational bounds on scalar-tensor theories from standard sirens
• On Larger $H_0$ Values in the CMB Dipole Direction
• The X-ray fundamental plane of the Platinum Sample, the Kilonovae and the SNe Ib/c associated with GRBs
• A Step in Understanding the Hubble Tension
• Quantifying the $S_8$ tension with the Redshift Space Distortion data set
• First Cosmology Results using Type Ia Supernova from the Dark Energy Survey: Simulations to Correct Supernova Distance Biases
• JWST early Universe observations and ΛCDM cosmology
• Can late-time extensions solve the $H_0$ and ${\sigma }_8$ tensions?
• Comparing early dark energy and extra radiation solutions to the Hubble tension with BBN
• First Cosmology Results Using Type Ia Supernovae From the Dark Energy Survey: Photometric Pipeline and Light Curve Data Release
• Do gamma-ray burst measurements provide a useful test of cosmological models?
• Strong lensing time-delay cosmography in the 2020s
• SuperRAENN: A Semi-supervised Supernova Photometric Classification Pipeline Trained on Pan-STARRS1 Medium Deep Survey Supernovae
• Reconstructing Gravity on Cosmological Scales
• Carnegie Supernova Project-II: Extending the Near-Infrared Hubble Diagram for Type Ia Supernovae to $z\sim 0.1$
• Hubble tension or a transition of the Cepheid SnIa calibrator parameters?
• Relieving the $H_0$ tension with a new interacting dark energy model
• Cosmological model insensitivity of local $H_0$ from the Cepheid distance ladder
• Cosmological viable models in $f(T,B)$ gravity as solutions to the $H_0$ tension
• Observational constraints on the tilted spatially-flat and the untilted nonflat $\varphi$CDM dynamical dark energy inflation models
• Implication of the Hubble tension for the primordial Universe in light of recent cosmological data
• Determining the range of validity of quasar X-ray and UV flux measurements for constraining cosmological model parameters
• Optical and X-ray GRB Fundamental Planes as Cosmological Distance Indicators
• Carnegie Supernova Project-II: The Near-infrared Spectroscopy Program
• Dark sectors with dynamical coupling
• Cosmology Intertwined IV: The Age of the Universe and its Curvature
• Cosmic chronometers to calibrate the ladders and measure the curvature of the Universe. A model-independent study
• Hints of a Local Matter Underdensity or Modified Gravity in the Low $z$ Pantheon data
• New Early Dark Energy is compatible with current LSS data
• Quasar X-ray and UV flux, baryon acoustic oscillation, and Hubble parameter measurement constraints on cosmological model parameters
• Post-Newtonian limit of generalized symmetric teleparallel gravity
• Unraveling the effective fluid approach for $f(R)$ models in the subhorizon approximation
• TDCOSMO V: strategies for precise and accurate measurements of the Hubble constant with strong lensing
• The LSST DESC DC2 Simulated Sky Survey
• Determining the Hubble Constant without the Sound Horizon: Measurements from Galaxy Surveys
• The impact of the cosmic variance on $H_0$ on cosmological analyses
• Evidence for Emergent Dark Energy
• Dark sector interaction and the supernova absolute magnitude tension
• Upper Bound of Neutrino Masses from Combined Cosmological Observations and Particle Physics Experiments
• All-inclusive interacting dark sector cosmologies
• Testing Late Time Cosmic Acceleration with uncorrelated Baryon Acoustic Oscillations dataset
• Cosmological Limits on the Neutrino Mass and Lifetime
• The Effect of Environment on Type Ia Supernovae in the Dark Energy Survey Three-Year Cosmological Sample
• Standardizing Platinum Dainotti-correlated gamma-ray bursts, and using them with standardized Amati-correlated gamma-ray bursts to constrain cosmological model parameters
• Late time approaches to the Hubble tension deforming $H(z)$, worsen the growth tension
• Reconciling $H_0$ tension in a six parameter space?
• Evidence of a decreasing trend for the Hubble constant
• Late-transition vs smooth $H(z)$ deformation models for the resolution of the Hubble crisis
• Can dark energy be dynamical?
• Can Conformally Coupled Modified Gravity Solve The Hubble Tension?
• Recombination-independent determination of the sound horizon and the Hubble constant from BAO
• Neutrino Mass Bounds in the era of Tension Cosmology
• Measurements of $H_0$ in modified gravity theories: The role of lensed quasars in the late-time Universe
• A Hierarchical Bayesian SED Model for Type Ia Supernovae in the Optical to Near-Infrared
• A fast test to assess the impact of marginalization in Monte Carlo analyses, and its application to cosmology
• Do cosmological observations allow a negative $\Lambda$?
• $H_0$ Tension, Swampland Conjectures and the Epoch of Fading Dark Matter
• Constraints on cosmological parameters from gamma-ray burst peak photon energy and bolometric fluence measurements and other data
• Dark Sector to Restore Cosmological Concordance
• The state of the dark energy equation of state circa 2023
• On the homogeneity of SnIa absolute magnitude in the Pantheon+ sample
• Applications and Techniques for Fast Machine Learning in Science
• Gaussian Process Estimation of Transition Redshift
• Brans-Dicke cosmology with a $\Lambda$- term: a possible solution to $\Lambda$CDM tensions
• What can Machine Learning tell us about the background expansion of the Universe?
• Determining Model-independent $H_0$ and Consistency Tests
• On the impact of $f(Q)$ gravity on the Large Scale Structure
• How Many Kilonovae Can Be Found in Past, Present, and Future Survey Datasets?
• Euclid: Forecast constraints on the cosmic distance duality relation with complementary external probes
• Omnipotent dark energy: A phenomenological answer to the Hubble tension
• Early mass varying neutrino dark energy: Nugget formation and Hubble anomaly
• Standardizing Dainotti-correlated gamma-ray bursts, and using them with standardized Amati-correlated gamma-ray bursts to constrain cosmological model parameters
• Towards early dark energy and $n_s$=1 with Planck, ACT and SPT
• Early-Universe-Physics Insensitive and Uncalibrated Cosmic Standards: Constraints on ${\Omega }_{\mathrm{m}}$ and Implications for the Hubble Tension
• ZTF Early Observations of Type Ia Supernovae II: First Light, the Initial Rise, and Time to Reach Maximum Brightness
• The $H_0$ tension: $\Delta G_N$ vs. $\Delta N_{\mathrm{eff}}$
• The Gamma-ray Bursts fundamental plane correlation as a cosmological tool
• Measuring the Hubble constant and spatial curvature from supernova apparent magnitude, baryon acoustic oscillation, and Hubble parameter data
• Updated constraints from the effective field theory analysis of BOSS power spectrum on Early Dark Energy
• Model-independent determination of $H_0$ and ${\Omega }_{K0}$ from strong lensing and type Ia supernovae
• A new parametrization of Hubble parameter in $f(Q)$ gravity
• Swampland Conjectures and Late-Time Cosmology
• How to use GP: Effects of the mean function and hyperparameter selection on Gaussian Process regression
• Constraints on barotropic dark energy models by a new phenomenological $q(z)$ parameterization
• The trouble beyond $H_0$ and the new cosmic triangles
• Observational constraints on interacting Tsallis holographic dark energy models
• Forecast for cosmological parameter estimation with gravitational-wave standard siren observation from the Cosmic Explorer
• No-go guide for the Hubble tension : Late-time solutions
• The local and distant Universe: stellar ages and $H_0$
• Observational constraints on the deceleration parameter in a tilted universe
• Addressing $H_0$ tension by means of VCDM
• Gravitational wave cosmology with extreme mass-ratio inspirals
• Think Global, Act Local: The Influence of Environment Age and Host Mass on Type Ia Supernova Light Curves
• Measurements of $H_0$ and reconstruction of the dark energy properties from a model-independent joint analysis
• Assessing the effect of lens mass model in cosmological application with updated galaxy-scale strong gravitational lensing sample
• Observational evidence for a local underdensity in the Universe and its effect on the measurement of the Hubble Constant
• Standardized long gamma-ray bursts as a cosmic distance indicator
• The evidence of cosmic acceleration and observational constraints
• ZTF 18aaqeasu (SN 2018byg): A Massive Helium-shell Double Detonation on a Sub-Chandrasekhar Mass White Dwarf
• Massive neutrinos and cosmic composition
• Multi-Dimensional Parameter Study of Double Detonation Type Ia Supernovae Originating from Thin-Helium-Shell White Dwarfs
• Can reverberation-measured quasars be used for cosmology?
• Late time transitions in the quintessence field and the $H_0$ tension
• Cosmological parameter estimation with future gravitational wave standard siren observation from the Einstein Telescope
• Soundness of Dark Energy properties
• Geometrical observational bounds on a fractal horizon holographic dark energy
• Can dark energy be expressed as a power series of the Hubble parameter?
• Quasar standardization: Overcoming Selection Biases and Redshift Evolution
• $f(R)$ gravity in the Jordan Frame as a Paradigm for the Hubble Tension
• Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies
• Cosmological constraints on late-universe decaying dark matter as a solution to the $H_0$ tension
• Looking for interactions in the cosmological dark sector
• Spectrophotometric templates for core collapse supernovae and their application in simulations of time-domain surveys
• Using SPTpol, Planck 2015, and non-CMB data to constrain tilted spatially-flat and untilted non-flat $\Lambda$CDM, XCDM, and $\varphi$CDM dark energy inflation cosmologies
• BAO+BBN revisited -- Growing the Hubble tension with a 0.7km/s/Mpc constraint
• Late time interacting cosmologies and the Hubble constant tension
• Testing Low-Redshift Cosmic Acceleration with Large-Scale Structure
• Falsifying $\Lambda$CDM: Model-independent tests of the concordance model with eBOSS DR14Q and Pantheon
• Revealing the effects of curvature on the cosmological models
• $T_0$ censorship of early dark energy and AdS vacua
• Redshift evolution of the underlying type Ia supernova stretch distribution
• Fitting $f(Q,T)$ gravity models with a $\Lambda$CDM limit using H(z) and Pantheon data
• Linear cosmological constraints on 2-body decaying dark matter scenarios and the $S_8$ tension
• Updating constraints on f(T) teleparallel cosmology and the consistency with Big Bang Nucleosynthesis
• Observational constraints on a logarithmic scalar field dark energy model and black hole mass evolution in the Universe
• The Carnegie Supernova Project-I: Correlation Between Type Ia Supernovae and Their Host Galaxies from Optical to Near-Infrared Bands
• hi_class: Background Evolution, Initial Conditions and Approximation Schemes
• Do quasar X-ray and UV flux measurements provide a useful test of cosmological models?
• The most luminous blue quasars at $3.0<z<3.3$. I. A tale of two X-ray populations
• Supernova Photometric Classification Pipelines Trained on Spectroscopically Classified Supernovae from the Pan-STARRS1 Medium-Deep Survey
• Einstein, Planck and Vera Rubin: relevant encounters between the Cosmological and the Quantum Worlds
• Robustness of baryon acoustic oscillation constraints for early-Universe modifications to $\Lambda$CDM
• Coupled and uncoupled early dark energy, massive neutrinos and the cosmological tensions
• The Early Dark Sector, the Hubble Tension, and the Swampland
• Cosmological Measurements from Angular Power Spectra Analysis of BOSS DR12 Tomography
• Testing H0 in Acoustic Dark Energy Models with Planck and ACT Polarization
• Cosmological observational constraints on the power law $f(Q)$ type modified gravity theory
• Constraining power of asymptotic safety for scalar fields
• Independent Cosmological Constraints from high-z HII Galaxies
• Prospects for improving cosmological parameter estimation with gravitational-wave standard sirens from Taiji
• Updated constraints on $f(T)$ models using direct and indirect measurements of the Hubble parameter
• Independent cosmological constraints from high-z HII galaxies: new results from VLT-KMOS data
• Determining the Hubble Constant without the Sound Horizon Scale: Measurements from CMB Lensing
• The Impact of Peculiar Velocities on the Estimation of the Hubble Constant from Gravitational Wave Standard Sirens
• Generalized Emergent Dark Energy Model and the Hubble Constant Tension
• Cosmological constraints from HII starburst galaxy apparent magnitude and other cosmological measurements
• Cosmology-independent estimate of the fraction of baryon mass in the IGM from fast radio burst observations
• Testing spatial curvature and anisotropic expansion on top of the $\Lambda$CDM model
• Cosmological Constraints from Gas Mass Fractions of Massive, Relaxed Galaxy Clusters
• Cosmology under the fractional calculus approach
• Gamma-Ray Bursts, Quasars, Baryonic Acoustic Oscillations, and Supernovae Ia: new statistical insights and cosmological constraints
• Parametric and nonparametric methods hint dark energy evolution
• Testing AdS early dark energy with Planck, SPTpol and LSS data
• Dark energy beyond quintessence: Constraints from the swampland
• Forecasting constraints on deviations from general relativity in $f(Q)$ gravity with standard sirens
• Model independent calibrations of gamma ray bursts using machine learning
• Connecting early and late epochs by f(z)CDM cosmography
• Dark degeneracy I: Dynamical or interacting dark energy?
• Barrow Entropy Cosmology: an observational approach with a hint of stability analysis
• A Critique of Holographic Dark Energy
• Robust and model-independent cosmological constraints from distance measurements
• Challenging bulk viscous unified scenarios with cosmological observations
• Constraining Teleparallel Gravity through Gaussian Processes
• Quantifying Scalar Field Dynamics with DESI 2024 Y1 BAO measurements
• Supernova Host Galaxies in the Dark Energy Survey: I. Deep Coadds, Photometry, and Stellar Masses
• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from multi-tracer BAO analysis with galaxies and voids
• Cosmology-insensitive estimate of IGM baryon mass fraction from five localized fast radio bursts
• Cosmological Results from the RAISIN Survey: Using Type Ia Supernovae in the Near Infrared as a Novel Path to Measure the Dark Energy Equation of State
• Quantifying concordance of correlated cosmological data sets
• Model-independent cosmological inference post DESI DR1 BAO measurements
• Constrained $f(Q,T)$ gravity accelerating cosmological model and its dynamical system analysis
• New Roads to the Small-Scale Universe: Measurements of the Clustering of Matter with the High-Redshift UV Galaxy Luminosity Function
• Strongly Lensed Transient Sources: A Review
• Health checkup test of the standard cosmological model in view of recent Cosmic Microwave Background Anisotropies experiments
• Probing elastic interactions in the dark sector and the role of $S_8$
• Unveiling cosmography from the dark energy equation of state
• Cosmography approach to dark energy cosmologies: new constrains using the Hubble diagrams of supernovae, quasars and gamma-ray bursts
• Euclid preparation: XIX. Impact of magnification on photometric galaxy clustering
• New cosmological bounds on hot relics: Axions $\&$ Neutrinos
• Towards hybrid inflation with $n_s=1$ in light of Hubble tension and primordial gravitational waves
• $H_0=69.8\pm 1.3$ $\mathrm{km}{\mathrm{s}}^{-1}\mathrm{Mp}{\mathrm{c}}^{-1}$, ${\Omega }_{m0}=0.288\pm 0.017$, and other constraints from lower-redshift, non-CMB, expansion-rate data
• CMB tensions with low-redshift $H_0$ and $S_8$ measurements: impact of a redshift-dependent type-Ia supernovae intrinsic luminosity
• SUGAR: An improved empirical model of Type Ia Supernovae based on spectral features
• Constraints on interacting dark energy models from time-delay cosmography with seven lensed quasars
• Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter
• Anisotropy of the Universe via the Pantheon supernovae sample revisited
• A Step in Understanding the $S_8$ Tension
• Testing the Consistency of Dust Laws in SN Ia Host Galaxies: A BayeSN Examination of Foundation DR1
• The Road to Precision Cosmology
• Multidimensionality of the Hubble tension: the roles of ${\Omega }_m$ and ${\omega }_c$
• Future Constraints on Dynamical Dark-Energy using Gravitational-Wave Standard Sirens
• The resilience of the Etherington-Hubble relation
• Determining the Hubble Constant without the Sound Horizon: A $3.6\%$ Constraint on $H_0$ from Galaxy Surveys, CMB Lensing and Supernovae
• Non-parametric reconstruction of the cosmological \textit{jerk} parameter
• Cosmological constraints from higher-redshift gamma-ray burst, HII starburst galaxy, and quasar (and other) data
• From a Bounce to the Dark Energy Era with $F(R)$ Gravity
• Kinematic constraints beyond $z\simeq 0$ using calibrated GRB correlations
• Rates and delay times of type Ia supernovae in the Dark Energy Survey
• Reheating in quintessential inflation via gravitational production of heavy massive particles: A detailed analysis
• Late-time decaying dark matter: constraints and implications for the $H_0$-tension
• Emergent Dark Energy, neutrinos and cosmological tensions
• Combining pre- and post-recombination new physics to address cosmological tensions: case study with varying electron mass and sign-switching cosmological constant
• Constant sound speed and its thermodynamical interpretation in $f(Q)$ gravity
• Cosmological model-independent constraints on spatial curvature from strong gravitational lensing and type Ia supernova observations
• Cosmographic parameters in model-independent approaches
• Designing Horndeski and the effective fluid approach
• Testing the equation of state for viscous dark energy
• First Cosmology Results Using Type Ia Supernovae From the Dark Energy Survey: Survey Overview and Supernova Spectroscopy
• Cosmological Constraint on ${\Omega }_m$ and ${\sigma }_8$ from Cluster Abundances using the $GalWCat19$ Optical-Spectroscopic SDSS Catalog
• Is there really a Hubble tension?
• Comparison between different methods of model selection in cosmology
• $\Lambda$CDM Tensions: Localising Missing Physics through Consistency Checks
• Cosmological constraints on decaying axion-like particles: a global analysis
• Testing the consistency between cosmological data: the impact of spatial curvature and the dark energy EoS
• Ultralight Scalar Decay and the Hubble Tension
• Observational constraints on Myrzakulov gravity
• Chain Early Dark Energy: Solving the Hubble Tension and Explaining Today's Dark Energy
• KiDS-1000: Combined halo-model cosmology constraints from galaxy abundance, galaxy clustering and galaxy-galaxy lensing
• Lensed Type Ia Supernova "Encore" at z=2: The First Instance of Two Multiply-Imaged Supernovae in the Same Host Galaxy
• Cosmological constraints of phantom dark energy models
• Gamma-ray burst data strongly favor the three-parameter fundamental plane (Dainotti) correlation relation over the two-parameter one
• Testing Dark energy models in the light of ${\sigma }_8$ tension
• Inferring $S_8(z)$ and $\gamma (z)$ with cosmic growth rate measurements using machine learning
• PELICAN: deeP architecturE for the LIght Curve ANalysis
• Hubble diagram at higher redshifts: Model independent calibration of quasars
• Accelerating expansion of the universe in modified symmetric teleparallel gravity
• Investigating the Diversity of Type Ia Supernova Spectra with the Open-Source Relational Database Kaepora
• Strong gravitational lensing and microlensing of supernovae
• Testing the Mutual Consistency of the Pantheon and SDSS/eBOSS BAO Data Sets with Gaussian Processes
• Reconstructing teleparallel gravity with cosmic structure growth and expansion rate data
• Strong Calcium Emission Indicates that the Ultraviolet-Flashing Type Ia SN 2019yvq was the Result of a Sub-Chandrasekhar Mass Double-Detonation Explosion
• A preliminary forecast for cosmological parameter estimation with gravitational-wave standard sirens from TianQin
• The Young Supernova Experiment Data Release 1 (YSE DR1): Light Curves and Photometric Classification of 1975 Supernovae
• Model-independent measurement of cosmic curvature with the latest $H(z)$ and SNe Ia data: A comprehensive investigation
• Observational constraints of a new unified dark fluid and the $H_0$ tension
• Cosmography by orthogonalized logarithmic polynomials
• Is the $H_0$ tension suggesting a 4th neutrino's generation?
• 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
• Ricci-inverse gravity: a novel alternative gravity, its flaws, and how to cure them
• Modelling and testing the equation of state for (Early) dark energy
• Finding the missing baryons in the intergalactic medium with localized fast radio bursts
• Multi-interacting dark energy and its cosmological implications
• Inference of the cosmic rest-frame from supernovae Ia
• Constrained realizations of 2MRS density and peculiar velocity fields: growth rate and local flow
• Assessment of the cosmic distance duality relation using Gaussian Process
• Revealing the late-time transition of $H_0$: relieve the Hubble crisis
• Cosmography with Supernova Refsdal through time-delay cluster lensing: independent measurements of the Hubble constant and geometry of the Universe
• Current Constraints on Anisotropic and Isotropic Dark Energy Models
• GHOST: Using Only Host Galaxy Information to Accurately Associate and Distinguish Supernovae
• Near-IR Type Ia SN distances: host galaxy extinction and mass-step corrections revisited
• Late-Time constraints on Interacting Dark Energy: Analysis independent of $H_0$, $r_d$ and $M_B$
• Return of Harrison-Zeldovich spectrum in light of recent cosmological tensions
• Gravity in the infrared and effective nonlocal models
• The DFSZ axion in the CMB
• KiDS & Euclid: Cosmological implications of a pseudo angular power spectrum analysis of KiDS-1000 cosmic shear tomography
• Testing interacting dark matter and dark energy model with cosmological data
• Out of the Swampland with Multifield Quintessence?
• Investigating the dark energy phenomenon in $f(R,L_m)$ cosmological models with observational constraints
• A Bayesian comparison between $\Lambda$CDM and phenomenologically emergent dark energy models
• Joint growth rate measurements from redshift-space distortions and peculiar velocities in the 6dF Galaxy Survey
• Quantifying the evidence for the current speed-up of the Universe with low and intermediate-redshift data. A more model-independent approach
• Null test for interactions in the dark sector
• High-redshift cosmography: Application and comparison with different methods
• The Hubble constant from strongly lensed supernovae with standardizable magnifications
• Consistency of Planck, ACT and SPT constraints on magnetically assisted recombination and forecasts for future experiments
• The Zwicky Transient Facility Type Ia supernova survey: first data release and results
• Viscous cosmology in the Weyl-type $f(Q,T)$ gravity
• TDCOSMO. IX. Systematic comparison between lens modelling software programs: time delay prediction for WGD 2038-4008
• SNR-calibrated Type Ia supernova models
• A Revised SALT2 Surface for Fitting Type Ia Supernova Light Curves
• One spectrum to cure them all: Signature from early Universe solves major anomalies and tensions in cosmology
• Hints of dark energy anisotropic stress using Machine Learning
• Early dark energy in $k$-essence
• Unified Dark Energy and Dark Matter from Dynamical Space Time
• Machine Learning the Cosmic Curvature in a Model-independent Way
• Towards a model-independent reconstruction approach for late-time Hubble data
• The Cosmic Expansion History from Line-Intensity Mapping
• Forecasting F(Q) cosmology with $\Lambda$CDM background using standard sirens
• Testing Gravity on Cosmic Scales: A Case Study of Jordan-Brans-Dicke Theory
• Model-independent constraints on cosmic curvature: implication from updated Hubble diagram of high-redshift standard candles
• Exploring the evidence for a large local void with supernovae Ia data
• Type Ia Supernovae are Excellent Standard Candles in the Near-Infrared
• Generalized tracker quintessence models for dark energy
• Inflation, the Hubble Tension and Early Dark Energy: an alternative overview
• Measuring the Hubble constant with black sirens
• Gravitational-Wave Detector Networks: Standard Sirens on Cosmology and Modified Gravity Theory
• Strengthening the bound on the mass of the lightest neutrino with terrestrial and cosmological experiments
• Concerning Colour: The Effect of Environment on Type Ia Supernova Colour in the Dark Energy Survey
• New accelerating solutions in late-time cosmology
• SALT3-NIR: Taking the Open-Source Type Ia Supernova Model to Longer Wavelengths for Next-Generation Cosmological Measurements
• Dark energy from $\alpha$-attractors: phenomenology and observational constraints
• Anomaly Detection in the Open Supernova Catalog
• Observational Constraints and Cosmological Implications of Scalar-Tensor $f(R,T)$ Gravity
• Prospect for constraining holographic dark energy with gravitational wave standard sirens from the Einstein Telescope
• Accuracy of environmental tracers and consequence for determining the Type Ia Supernovae magnitude step
• X-ray Plateaus in Gamma-Ray Burst Afterglows and Their Application in Cosmology
• Cannibalism hinders growth: Cannibal Dark Matter and the $S_8$ tension
• Early Dark Energy with Power-law F(R) Gravity
• Probing modified gravity theories with multiple measurements of high-redshift quasars
• Massive neutrino self-interactions and inflation
• Late time acceleration due to generic modification of gravity and Hubble tension
• Ruling Out New Physics at Low Redshift as a solution to the $H_0$ Tension
• Reconstruction of the neutrino mass as a function of redshift
• Calibrating Gamma-Ray Bursts by Using a Gaussian Process with Type Ia Supernovae
• Constraints on the Parameterized Deceleration Parameter in FLRW Universe
• The Dark Energy Survey Supernova Program: Modelling selection efficiency and observed core collapse supernova contamination
• Impacts of gravitational-wave standard siren observations from Einstein Telescope and Cosmic Explorer on weighing neutrinos in interacting dark energy models
• Determining the Hubble Constant without the Sound Horizon: Perspectives with Future Galaxy Surveys
• Berkeley Supernova Ia Program: Data Release of 637 Spectra from 247 Type Ia Supernovae
• Cosmological inference from the EFTofLSS: the eBOSS QSO full-shape analysis
• Cosmological perturbations in the Tsallis holographic dark energy scenarios
• Model-independent cosmic acceleration and type Ia supernovae intrinsic luminosity redshift dependence
• The Mira Distance to M101 and a 4% Measurement of H0
• On the dynamics of a dark sector coupling
• Metric $f(R)$ gravity with dynamical dark energy as a scenario for the Hubble tension
• GALLUMI: A Galaxy Luminosity Function Pipeline for Cosmology and Astrophysics
• An Axially Symmetric Transitioning models with Observational Constraints
• Constraints on the transition redshift from the calibrated Gamma-ray Burst $E_{\mathrm{p}}$-$E_{\mathrm{iso}}$ correlation
• New constraints on the distance duality relation from the local data
• Forecasting the Interaction in Dark Matter-Dark Energy Models with Standard Sirens From the Einstein Telescope
• A data-driven Reconstruction of Horndeski gravity via the Gaussian processes
• A galaxy-driven model of type Ia supernova luminosity variations
• Power-law cosmology in Weyl-type $f(Q,T)$ gravity
• Thermodynamical aspects of Bianchi type-I Universe in quadratic form of $f\left(Q\right)$ gravity and observational constraints
• Testing dark energy models with a new sample of strong-lensing systems
• Projected Cosmological Constraints from Strongly Lensed Supernovae with the Roman Space Telescope
• On the halo-mass and radial scale dependence of the lensing is low effect
• Revisiting a non-parametric reconstruction of the deceleration parameter from combined background and the growth rate data
• Galaxy cluster strong lensing cosmography: cosmological constraints from a sample of regular galaxy clusters
• Nebular Spectroscopy of Kepler's Brightest Supernova
• Dynamical dark energy models in the light of Gravitational-Wave Transient Catalogues
• Reconciling Hubble Constant Discrepancy from Holographic Dark Energy
• Observational constraints of the modified cosmology through Barrow entropy
• Testing Dark Energy Models with Gamma-Ray Bursts Calibrated from the Observational $H(z)$ Data through a Gaussian Process
• CMB distance priors revisited: effects of dark energy dynamics, spatial curvature, primordial power spectrum, and neutrino parameters
• Beware of commonly used approximations II: estimating systematic biases in the best-fit parameters
• Is the Hubble diagram of quasars in tension with concordance cosmology?
• Gamma ray burst constraints on cosmological models from the improved Amati correlation
• Direct Detection of Dark Matter Substructure in Strong Lens Images with Convolutional Neural Networks
• Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy
• Constraining the Asymptotically Safe Cosmology: cosmic acceleration without dark energy
• Current and future applications of Reverberation-mapped quasars in Cosmology
• Cosmology with varying fundamental constants from hyperlight, coupled scalars
• Viewing angle of binary neutron star mergers
• Constraints on dark matter to dark radiation conversion in the late universe with DES-Y1 and external data
• Phenomenological emergent dark energy in the light of DESI Data Release 1
• Intrinsic tension in the supernova sector of the local Hubble constant measurement and its implications
• Constraining the dark energy models using Baryon Acoustic Oscillations: An approach independent of $H_0\cdot r_d$
• Principal reconstructed modes of dark energy and gravity
• Unified early and late Universe cosmology through dissipative effects in steep quintessential inflation potential models
• Slow-rolling scalar dynamics and as solution for the Hubble tension
• Running vacuum in QFT in FLRW spacetime: The dynamics of ${\rho }_{\mathrm{vac}}(H)$ from the quantized matter fields
• Cosmology-independent Estimate of the Hubble Constant and Spatial Curvature Using Time-delay Lenses and Quasars
• Model selection applied to reconstructions of the Dark Energy
• Testing logarithmic corrections on $R^2$-exponential gravity by observational data
• Constraining the anisotropy of the Universe via Pantheon supernovae sample
• Revisiting Metastable Dark Energy and Tensions in the Estimation of Cosmological Parameters
• Cosmological tests of the osculating Barthel-Kropina dark energy model
• Forecasting Interacting Vacuum-Energy Models using Gravitational Waves
• Beyond $\Lambda$CDM constraints from the full shape clustering measurements from BOSS and eBOSS
• Investigating the Hubble Constant Tension -- Two Numbers in the Standard Cosmological Model
• Minimal dark energy: key to sterile neutrino and Hubble constant tensions?
• JWST Photometric Time-Delay and Magnification Measurements for the Triply-Imaged Type Ia "Supernova H0pe" at z = 1.78
• Cosmology with fast radio bursts in the era of SKA
• Touch of Neutrinos on the Vacuum Metamorphosis: is the $H_0$ Solution Back?
• Lensing-like tensions in the Planck legacy release
• ParSNIP: Generative Models of Transient Light Curves with Physics-Enabled Deep Learning
• The Chandra view of the relation between X-ray and UV emission in quasars
• Constraining Type Ia supernova explosions and early flux excesses with the Zwicky Transient Factory
• $E_{\mathrm{iso}}$-$E_{\mathrm{p}}$ correlation of gamma ray bursts: calibration and cosmological applications
• Machine learning constraints on deviations from general relativity from the large scale structure of the Universe
• Evidence for Cosmic Acceleration is Robust to Observed Correlations Between Type Ia Supernova Luminosity and Stellar Age
• Model-independent Distance Calibration and Curvature Measurement using Quasars and Cosmic Chronometers
• The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset
• Do supernovae indicate an accelerating universe?
• The Hubble Tension, The $M$ Crisis of Late Time $H(z)$ Deformation Models and the Reconstruction of Quintessence Lagrangians
• Cosmological constraints on the Generalized Uncertainty Principle from modified Friedmann equations
• Percent-Level Test of Isotropic Expansion Using Type Ia Supernovae
• Cosmic expansion parametrization: Implication for curvature and ${\text{H}}_0$ tension
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• No-go theorem for inflation in Ricci-inverse gravity
• Holographic dark energy from the laws of thermodynamics with Rényi entropy
• SNIa-Cosmology Analysis Results from Simulated LSST Images: from Difference Imaging to Constraints on Dark Energy
• Late-time constraints on modified Gauss-Bonnet cosmology
• Tensions with the flat $\mathbf{\Lambda }$CDM model from high-redshift cosmography
• Cosmological constraints on dark energy in $f(Q)$ gravity: A parametrized perspective
• Further evidence that galaxy age drives observed type Ia supernova luminosity differences
• Constraining Anisotropic Cosmological Model in $f(\mathcal{R},{\mathcal{L}}_m)$ Gravity
• Model-independent constraints on ${\Omega }_m$ and $H(z)$ from the link between geometry and growth
• CosmicNet II: Emulating extended cosmologies with efficient and accurate neural networks
• Pantheon update on a model-independent analysis of cosmological supernova data
• A hint of matter underdensity at low $z$?
• Carnegie Supernova Project-II: A new method to photometrically identify sub-types of extreme Type Ia Supernovae
• A test of cosmic distance duality relation using SPT-SZ galaxy clusters, Type Ia supernovae, and cosmic chronometers
• Stepped Partially Acoustic Dark Matter, Large Scale Structure, and the Hubble Tension
• Phase space analysis and singularity classification for linearly interacting dark energy models
• Dynamical dark energy confronted with multiple CMB missions
• Exploration of interacting dynamical dark energy model with interaction term including the equation-of-state parameter: alleviation of the $H_0$ tension
• Cold New Early Dark Energy pulls the trigger on the $H_0$ and $S_8$ tensions: a simultaneous solution to both tensions without new ingredients
• Measuring the sound horizon and absolute magnitude of SNIa by maximizing the consistency between low-redshift data sets
• A New $Om(z)$ Diagnostic of Dark Energy in General Relativity Theory
• Analyzing the geometrical and dynamical parameters of modified Teleparallel-Gauss-Bonnet model
• Smoothing the $H_0$ tension with a dynamical dark energy model
• Observational constraints on Yukawa cosmology and connection with black hole shadows
• Gravitational wave propagation in $f(R)$ models: New parametrizations and observational constraints
• Imprints of an extended Chevallier-Polarski-Linder parametrization on the large scale of our universe
• Toward a concordance teleparallel Cosmology I: Background Dynamics
• Reconstruction of the dark sectors' interaction: A model-independent inference and forecast from GW standard sirens
• Are Type Ia Supernovae in Restframe $H$ Brighter in More Massive Galaxies?
• A new coupled three-form dark energy model and implications for the $H_0$ tension
• No-go guide for late-time solutions to the Hubble tension: Matter perturbations
• Impact of $H_0$ priors on $f(T)$ late time cosmology
• Bulk viscous matter and the cosmic acceleration of the universe in $f(Q,T)$ gravity
• Testing dark energy after pre-recombination early dark energy
• Constraining the curvature density parameter in cosmology
• SALT2 Versus SALT3: Updated Model Surfaces and Their Impacts on Type Ia Supernova Cosmology
• Can high-redshift Hubble diagrams rule out the standard model of cosmology in the context of cosmographic method?
• Effects of Supernova Redshift Uncertainties on the Determination of Cosmological Parameters
• CosmoBit: A GAMBIT module for computing cosmological observables and likelihoods
• $H_0$ Ex Machina: Vacuum Metamorphosis and Beyond $H_0$
• ECoPANN: A Framework for Estimating Cosmological Parameters using Artificial Neural Networks
• Fitting string inflation to real cosmological data: the Fibre Inflation case
• Hubble tension in lepton asymmetric cosmology with an extra radiation
• Impacts of dark energy on weighing neutrinos after DESI BAO
• Constraining $f(Q,L_m)$ gravity with bulk viscosity
• Constrained evolution of effective equation of state parameter in non-linear $f(R,L_m)$ dark energy model: Insights from Bayesian analysis of cosmic chronometers and Pantheon samples
• Tsallis holographic dark energy in Fractal Universe
• Model marginalized constraints on neutrino properties from cosmology
• A Dark Matter Trigger for Early Dark Energy Coincidence
• Cosmological Constraints on sub-horizon scales modified gravity theories with MGCLASS II
• Cosmic opacity: cosmological-model-independent tests from gravitational waves and Type Ia Supernova
• MOG cosmology without dark matter and the cosmological constant
• Microphysics of Early Dark Energy
• Quantifying the Line-of-Sight Halo Contribution to the Dark Matter Convergence Power Spectrum from Strong Gravitational Lenses
• Measurements of the Hubble Constant with a Two Rung Distance Ladder: Two Out of Three Ain't Bad
• Standardizing reverberation-measured C IV time-lag quasars, and using them with standardized Mg II quasars to constrain cosmological parameters
• Do you smell something decaying? Updated linear constraints on decaying dark matter scenarios
• Bayesian Comparison of Interacting Scenarios
• Testing the anisotropy of cosmic acceleration from Pantheon supernovae sample
• Testing cosmic anisotropy with Pantheon sample and quasars at high redshifts
• Constraints on $f(T)$ Cosmology with Pantheon+
• Exploring accelerated expansion in the universe: A study of $f(Q,T)$ gravity with parameterized EoS and cosmological constraints
• Cosmological constraints from HII starburst galaxy, quasar angular size, and other measurements
• Observational constraints and some toy models in $f(Q)$ gravity with bulk viscous fluid
• Cosmology with relativistically varying physical constants
• Measuring the reionization optical depth without large-scale CMB polarization
• The Impact of Observing Strategy on Cosmological Constraints with LSST
• Modeling Transit Dark Energy in $f(R,L_m)$-gravity
• Red and Reddened: Ultraviolet through Near-Infrared Observations of Type Ia Supernova 2017erp
• Proca in the sky
• Observational analysis of late-time acceleration in $f(Q,L_m)$ gravity
• Cosmographic view on the $H_0$ and ${\sigma }_8$ tensions
• Observational constraints and predictions of the interacting dark sector with field-fluid mapping
• The Twins Embedding of Type Ia Supernovae II: Improving Cosmological Distance Estimates
• The Copernican principle in light of the latest cosmological data
• Consistency of Modified Gravity with a decreasing $G_{\mathrm{eff}}(z)$ in a $\Lambda$CDM background
• A void in the Hubble tension? The end of the line for the Hubble bubble
• Measuring Cosmological Parameters with Type Ia Supernovae in redMaGiC galaxies
• Observational constraints on Tsallis modified gravity
• Thermodynamics of the viscous $f(T,B)$ gravity in the new agegraphic dark energy model
• The Hyper Suprime-Cam SSP Transient Survey in COSMOS: Overview
• Dark Energy as a Critical Phenomenon: a Resolution for Hubble Tension
• Magnification, dust and time-delay constraints from the first resolved strongly lensed Type Ia supernova
• Two Fluid Scenario in Bianchi Type-I Universe
• Model independent bounds on Type Ia supernova absolute peak magnitude
• Multiple transitions in vacuum dark energy and $H_0$ tension
• A grounded perspective on New Early Dark Energy using ACT, SPT, and BICEP/Keck
• SICRET: Supernova Ia Cosmology with truncated marginal neural Ratio EsTimation
• Latest evidence for a late time vacuum -- geodesic CDM interaction
• Observational constraints on the equation of state of viscous fluid in $f(R,T)$ gravity
• DES Y1 results: Splitting growth and geometry to test $\Lambda$CDM
• An exploration of an early gravity transition in light of cosmological tensions
• Sources of $H_0$-tensions in dark energy scenarios
• Observational Constraints on $f(T)$ Gravity from Model-Independent Data
• $H_0$ Tension in Torsion-based Modified Gravity
• Binning is Sinning (Supernova Version): The Impact of Self-Calibration in Cosmological Analyses with Type Ia Supernovae
• Generalized Chaplygin gas and accelerating universe in $f(Q,T)$ gravity
• LensWatch: I. Resolved HST Observations and Constraints on the Strongly-Lensed Type Ia Supernova 2022qmx ("SN Zwicky")
• A Carbon/Oxygen-dominated Atmosphere Days After Explosion for the "Super-Chandrasekhar" Type Ia SN 2020esm
• Inevitable manifestation of wiggles in the expansion of the late Universe
• Studying Type II supernovae as cosmological standard candles using the Dark Energy Survey
• Testing the violation of the equivalence principle in the electromagnetic sector and its consequences in $f(T)$ gravity
• Profiling Cold New Early Dark Energy
• A Model-independent Test of Cosmic Isotropy with Low-z Pantheon Supernovae
• Tomographic Alcock-Paczynski Test with Redshift-Space Correlation Function: Evidence for the Dark Energy Equation of State Parameter w>-1
• New MGCAMB tests of gravity with CosmoMC and Cobaya
• The period--luminosity relation for Mira variables in the Milky Way using Gaia DR3: a further distance anchor for $H_0$
• The weak, the strong and the ugly -- A comparative analysis of interacting stepped dark radiation
• Do the observational data favor a local void?
• The Reconstruction of Constant Jerk Parameter with $f(R,T)$ Gravity
• Exploring late-time cosmic acceleration: A study of a linear $f(T)$ cosmological model using observational data
• Observational constraints on bimetric gravity
• A new cosmological probe using super-massive black hole shadows
• Cosmological implications of the constant jerk parameter in $f(Q,T)$ gravity theory
• Constraining the $f(R,T)=R+2\lambda T$ cosmological model using recent observational data
• Quasar UV/X-ray relation luminosity distances are shorter than reverberation-measured radius-luminosity relation luminosity distances
• Observational constrained $F(R,\mathcal{G})$ gravity cosmological model and the dynamical system analysis
• The QCD phase transition behind a PBH origin of LIGO/Virgo events?
• The multipole expansion of the local expansion rate
• Exploring the Hubble tension with a late time Modified Gravity scenario
• An 8.0\% Determination of the Baryon Fraction in the Intergalactic Medium from Localized Fast Radio Bursts
• Bayesian evidence for $\alpha$-attractor dark energy models
• Strong Bounds on Sum of Neutrino Masses in a 12 Parameter Extended Scenario with Non-Phantom Dynamical Dark Energy ($w(z)\ge -1$)
• Quasars as high-redshift standard candles
• Challenging matter creation models in the phantom divide
• Likelihood-free Cosmological Constraints with Artificial Neural Networks: An Application on Hubble Parameters and SNe Ia
• The constrained cosmological model in Lyra geometry
• Is Dark Energy Dynamical in the DESI Era? A Critical Review
• Anisotropic Universe in $f(Q,T)$ gravity, a novel study
• The dependency of Type Ia Supernova parameters on host galaxy morphology for the Pantheon cosmological sample
• Current data are consistent with flat spatial hypersurfaces in the $\Lambda$CDM cosmological model but favor more lensing than the model predicts
• Steve: A hierarchical Bayesian model for Supernova Cosmology
• Model Independent Expansion History from Supernovae: Cosmology versus Systematics
• Modelling the Accelerating Universe with $f(Q)$ Gravity: Observational Consistency
• No rungs attached: A distance-ladder free determination of the Hubble constant through type II supernova spectral modelling
• The dark side of the torsion: Dark Energy from propagating torsion
• Testing $\Lambda$-Free f(Q) Cosmology
• Evaporating primordial black holes as varying dark energy
• KiDS-SBI: Simulation-based inference analysis of KiDS-1000 cosmic shear
• General cosmological perturbations in teleparallel gravity
• Effects of type Ia supernovae absolute magnitude priors on the Hubble constant value
• Effect of evolutionary physical constants on type-1a supernova luminosity
• Euclid: Forecast constraints on consistency tests of the $\Lambda$CDM model
• Thermal Friction as a Solution to the Hubble and Large-Scale Structure Tensions
• Limits on Clustering and Smooth Quintessence from the EFTofLSS
• Data Analysis of three parameter models of deceleration parameter in FRW Universe
• Dynamical Dark Energy Implies a Coupled Dark Sector: Insights from DESI DR2 via a Data-Driven Approach
• Probing the cosmic opacity from Future Gravitational Wave Standard Sirens
• Dark Energy, Extra Dimensions, and the Swampland
• Exploring the Hubble Tension and Spatial Curvature from the Ages of Old Astrophysical Objects
• Do reverberation-measured H$\beta$ quasars provide a useful test of cosmology?
• Constraining viscous dark energy equation of state in $f(R,L_m)$ gravity
• Phantom scalar-tensor models and cosmological tensions
• Cosmological parameter estimation with Genetic Algorithms
• Constraints on anisotropic primordial non-Gaussianity from intrinsic alignments of SDSS-III BOSS galaxies
• Dark energy and matter interacting scenario to relieve $H_0$ and $S_8$ tensions
• Using Host Galaxy Photometric Redshifts to Improve Cosmological Constraints with Type Ia Supernova in the LSST Era
• Forecast of Neutrino Cosmology from the CSST Photometric Galaxy Clustering and Cosmic Shear Surveys
• Implications of an extended dark energy model with massive neutrinos
• Massive neutrino self-interactions with a light mediator in cosmology
• Gaussian Processes Reconstruction of the Dark Energy Potential
• A Cosmological Underdensity Does Not Solve the Hubble Tension
• Minimal theory of massive gravity in the light of CMB data and the $S_8$ tension
• $\alpha$ attractors in Quintessential Inflation motivated by Supergravity
• Modeling of accelerating Universe with bulk viscous fluid in Bianchi V space-time
• Growth of matter perturbations in the extended viscous dark energy models
• The effects of varying colour-luminosity relations on supernova science
• On Problems with Cosmography in Cosmic Dark Ages
• Measurement on the cosmic curvature using the Gaussian process method
• Supernova Siblings: Assessing the Consistency of Properties of Type Ia Supernovae that Share the Same Parent Galaxies
• Horndeski in the Swampland
• New cosmological constraints on $f(T)$ gravity in light of full Planck-CMB and type Ia supernovae data
• Cosmological constraints on Hořava gravity revised in light of GW170817 and GRB170817A and the degeneracy with massive neutrinos
• Debiasing Cosmic Gravitational Wave Sirens
• Rapidly Descending Dark Energy and the End of Cosmic Expansion
• The Scale-Invariant Vacuum (SIV) Theory: A Possible Origin of Dark Matter and Dark Energy
• Peculiar motion of Solar system from the Hubble diagram of supernovae Ia and its implications for cosmology
• Constraining the cosmological model of modified $f(Q)$ gravity: Phantom dark energy and observational insights
• Testing modified gravity via Yukawa potential in two body problem: Analytical solution and observational constraints
• Towards a possible solution to the Hubble tension with Horndeski gravity
• Exact solutions and cosmological constraints in fractional cosmology
• Measuring the cosmic homogeneity scale with SDSS-IV DR16 Quasars
• Consistency study of high- and low-accreting Mg ii quasars: No significant effect of the Fe ii to Mg ii flux ratio on the radius-luminosity relation dispersion
• Defying the laws of Gravity I: model-independent reconstruction of the Universe expansion from growth data
• Reaffirming the Cosmic Acceleration without Supernova and CMB
• Diffusion in unimodular gravity: Analytical solutions, late-time acceleration, and cosmological constraints
• IWDM: The fate of an interacting non-cold dark matter $-$ vacuum scenario
• Low-redshift estimates of the absolute scale of baryon acoustic oscillations
• Cosmological perturbations in the interacting dark sector: Mapping fields and fluids
• Supernova Magnitude Evolution and PAge Approximation
• Quasars: standard candles up to z=7.5 with the precision of Supernovae Ia
• Minimal theory of massive gravity and constraints on the graviton mass
• Decaying dark matter, the $H_0$ tension, and the lithium problem
• The first Hubble diagram and cosmological constraints using superluminous supernova
• Dark Matter in Astrophysics/Cosmology
• Testing $\Lambda$CDM cosmology in a binned universe: anomalies in the deceleration parameter
• The dependence of intrinsic alignment of galaxies on wavelength using KiDS and GAMA
• Probing the interaction between dark energy and dark matter with future fast radio burst observations
• Cosmological constraints on dark energy models using DESI BAO 2024
• Improving sampling and calibration of GRBs as distance indicators
• Constraining the SN Ia Host Galaxy Dust Law Distribution and Mass Step: Hierarchical BayeSN Analysis of Optical and Near-Infrared Light Curves
• Bayesian model selection on Scalar $\epsilon$-Field Dark Energy
• Super-CMB fluctuations and the Hubble tension
• Improved constraint on primordial gravitational waves in light of the Hubble tension and BICEP/Keck
• The Dark Energy Survey Supernova Program: Cosmological biases from supernova photometric classification
• Analysis of galaxy kinematics based on Cepheids from the Gaia DR2 Catalogue
• A search for the variation of speed of light using galaxy cluster gas mass fraction measurements
• Observational Constraints on Dynamical Dark Energy Models
• Can the quantum vacuum fluctuations really solve the cosmological constant problem?
• Significant Luminosity Differences of Two Twin Type Ia Supernovae
• Cosmological Constraints on Non-flat Exponential $f(R)$ Gravity
• Transit String Dark Energy Models in $f(Q)$ Gravity
• Estimated Age of the Universe in Fractional Cosmology
• Quintessential inflation and cosmological seesaw Mechanism: reheating and observational constraints
• Questioning the $H_0$ tension via the look-back time
• Cosmological constraints on non-adiabatic dark energy perturbations
• Does $\Lambda$CDM really be in tension with the Hubble diagram data?
• Impacts of dark energy on constraining neutrino mass after Planck 2018
• Dark energy and dark matter unification from dynamical space time: observational constraints and cosmological implications
• Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension
• Galaxy-Scale Test of General Relativity with Strong Gravitational Lensing
• Quintessential Cosmological Tensions
• Constraining extra dimensions on cosmological scales with LISA future gravitational wave siren data
• Investigating the accelerated expansion of the Universe through updated constraints on viable $f(R)$ models within the metric formalism
• Hubble constant difference between CMB lensing and BAO measurements
• Forecast for weighing neutrinos in cosmology with SKA
• Toward a concordance teleparallel Cosmology II: Linear perturbation
• Brans-Dicke cosmology mimicking running vacuum
• The Integrated Sachs Wolfe effect: unWISE and Planck constraints on Dynamical Dark Energy
• Multiple measurements of quasars acting as standard probes: model independent calibration and exploring the Dark Energy Equation of States
• Concordance Cosmology?
• A Possible Distance Bias for Type Ia Supernovae with Different Ejecta Velocities
• Parametrising non-linear dark energy perturbations
• Model-independent test for the cosmic distance duality relation with Pantheon and eBOSS DR16 quasar sample
• Testing generalized logotropic models with cosmic growth
• Model-independently calibrating the luminosity correlations of gamma-ray bursts using deep learning
• Prospects for measuring dark energy with 21 cm intensity mapping experiments: A joint survey strategy
• Newest measurements of Hubble constant from DESI 2024 BAO observations
• Kernel Selection for Gaussian Process in Cosmology: with Approximate Bayesian Computation Rejection and Nested Sampling
• Current constraints on deviations from General Relativity using binning in redshift and scale
• Model-independent study for a quintessence model of dark energy: Analysis and Observational constraints
• On An Interacting New Holographic Dark Energy Model: observational constraints
• No-go guide for the Hubble tension: late-time or local-scale new physics
• Perturbations in a scalar field model with virtues of $\Lambda$CDM
• Alleviating $H_0$ tension in Horndeski gravity
• TDCOSMO VI: Distance Measurements in Time-delay Cosmography under the Mass-sheet transformation
• Testing f(R) gravity with the simulated data of gravitational waves from the Einstein Telescope
• Reconstruction of an Observationally Constrained $f(R,T)$ gravity model
• Consistency testing for invariance of the speed of light at different redshifts: the newest results from strong lensing and type Ia supernovae observations
• A constrained cosmological model in $f(R,L_m)$ gravity
• Spectroscopic Studies of Type Ia Supernovae Using LSTM Neural Networks
• CSST Cosmological Emulator I: Matter Power Spectrum Emulation with one percent accuracy to k = 10 h/Mpc
• Constraints on field flows of quintessence dark energy
• Hints for possible low redshift oscillation around the best fit $\Lambda$CDM model in the expansion history of the Universe
• Can phantom transition at $z\sim 1$ restore the Cosmic concordance?
• Model-independent Estimations for the Cosmic Curvature from the Latest Strong Gravitational Lensing Systems
• The quadrupole in the local Hubble parameter: first constraints using Type Ia supernova data and forecasts for future surveys
• Late-time acceleration with a scalar field source: Observational constraints and statefinder diagnostics
• ZTF SN Ia DR2: Colour standardisation of Type Ia Supernovae and its dependence on environment
• Tsallis Holographic Dark Energy Reconsidered
• A model independent comparison of supernova and strong lensing cosmography: implications for the Hubble constant tension
• Cosmological constraints from the cross-correlation of DESI Luminous Red Galaxies with CMB lensing from Planck PR4 and ACT DR6
• Primordial black holes and gravitational waves in teleparallel Gravity
• New parametrization of the dark-energy equation of state with a single parameter
• Prospects for measuring dark energy with 21 cm intensity mapping experiments
• Observational Constraints on Warm Inflation in Loop Quantum Cosmology
• Acceleration in Friedmann cosmology with torsion
• R-band light-curve properties of Type Ia supernovae from the (intermediate) Palomar Transient Factory
• A thorough investigation of the prospects of eLISA in addressing the Hubble tension: Fisher Forecast, MCMC and Machine Learning
• Hint of a truncated primordial spectrum from the CMB large-scale anomalies
• A gravitational constant transition within cepheids as supernovae calibrators can solve the Hubble tension
• Analyzing the Hubble tension through hidden sector dynamics in the early universe
• The Twins Embedding of Type Ia Supernovae I: The Diversity of Spectra at Maximum Light
• Thermodynamically consistent entropic late-time cosmological acceleration
• Scrutinizing Various Phenomenological Interactions In The Context Of Holographic Ricci Dark Energy Models
• Hubble constant and sound horizon from the late-time Universe
• First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Effects of Chromatic Corrections to Supernova Photometry on Measurements of Cosmological Parameters
• Cosmological constraints on the Multi Scalar Field Dark Matter model
• Friedmann cosmology with decaying vacuum density in Brans-Dicke theory
• Testing f(R) gravity models with quasar X-ray and UV fluxes
• Cosmography with Standard Sirens from the Einstein Telescope
• Exploring new physics in the late Universe's expansion through non-parametric inference
• Constraints on $f(Q)$ logarithmic model using gravitational wave standard sirens
• High Redshift Long Gamma-Ray Bursts Hubble Diagram as a Test of Basic Cosmological Relations
• Non-Canonical Volume-Form Formulation of Modified Gravity Theories and Cosmology
• Alleviating Cosmological Tensions with a Coupled Scalar Fields Model
• Running vacuum in Brans-Dicke theory: a possible cure for the ${\sigma }_8$ and $H_0$ tensions
• Cosmological test on viscous bulk models using Hubble Parameter measurements and type Ia Supernovae data
• Non-parametric reconstruction of dark energy and cosmic expansion from the Pantheon compilation of type Ia supernovae
• Viscous cosmology in $f(T)$ gravity
• Testing the cosmic opacity at higher redshifts: implication from quasars with available UV and X-ray observations
• Revisiting Chaplygin gas cosmologies with the recent observations of high-redshfit quasars
• The role of CMB spectral distortions in the Hubble tension: a proof of principle
• Cascading Dark Energy
• Constraints on Newton's Constant from Cosmological Observations
• Constraints on anisotropic properties of the universe in $f(Q,T)$ gravity theory
• Modeling cosmic acceleration with a generalized varying deceleration parameter
• Kinematic Constraints on Spatial Curvature from Supernovae Ia and Cosmic Chronometers
• Cosmological constrains on minimally and non-minimally coupled scalar field models
• Local Hole revisited: evidence for bulk motions and self-consistent outflow
• Anisotropic f(Q) gravity model with bulk viscosity
• Probing Modified Gravity with Integrated Sachs-Wolfe CMB and Galaxy Cross-correlations
• Constraints on neutrino mass in the scenario of vacuum energy interacting with cold dark matter after Planck 2018
• Dark matter solution to the $H_0$ and $S_8$ tensions, and the integrated Sachs-Wolfe void anomaly
• Cosmological discordances III: more on measure properties, Large-Scale-Structure constraints, the Hubble constant and Planck
• Measuring the Hubble Constant with cosmic chronometers: a machine learning approach
• Null test for cosmic curvature using Gaussian process
• Neural networks and standard cosmography with newly calibrated high redshift GRB observations
• Update constraints on neutrino mass and mass hierarchy in light of dark energy models
• Swift UVOT Grism Observations of Nearby Type Ia Supernovae -- II. Probing the Progenitor Metallicity of SNe Ia with Ultraviolet Spectra
• PS15cey and PS17cke: prospective candidates from the Pan-STARRS Search for Kilonovae
• Imprints of interacting dark energy on cosmological perturbations
• A new $f(Q)$ cosmological model with $H(z)$ quadratic expansion
• $\Lambda$CDM is alive and well
• A model-independent characterisation of strong gravitational lensing by observables
• Exploring Universe acceleration through observational constraints via Hubble parameter reconstruction
• Running vacuum versus Holographic dark energy: a cosmographic comparison
• Spatial Curvature in $f(R)$ Gravity
• Gravitational-wave constraints on the cosmic opacity at $z\sim 5$: forecast from space gravitational-wave antenna DECIGO
• Extended $\Lambda$CDM model
• Generalised model-independent characterisation of strong gravitational lenses VI: the origin of the formalism intrinsic degeneracies and their influence on $H_0$
• Absolute Calibration of Cepheid Period-Luminosity Relations in NGC 4258
• Time-dependent $G$ in Einstein's equations as an alternative to the cosmological constant
• Vacuum Energy Density Measured from Cosmological Data
• Galaxy cluster Sunyaev-Zel'dovich effect scaling-relation and type Ia supernova observations as a test for the cosmic distance duality relation
• A comprehensive parametrization approach for the Hubble parameter in scalar field dark energy models
• Likelihood-free Inference with Mixture Density Network
• Theoretical priors in scalar-tensor cosmologies: Thawing quintessence
• Cosmological search for sterile neutrinos after Planck 2018
• Non-parametric Reconstruction of Growth Index via Gaussian Processes
• Forecast of Cosmological Constraints with Type Ia Supernovae from the Chinese Space Station Telescope
• The cosmological bulk flow in QCDM model: (In)consistency with $\Lambda CDM$
• Decay of multiple dark matter particles to dark radiation in different epochs does not alleviate the Hubble tension
• Reconstructing the Fraction of Baryons in the Intergalactic Medium with Fast Radio Bursts via Gaussian Processes
• Cosmological foundations revisited with Pantheon+
• Cosmological acceleration
• Cosmic Anisotropy and Fast Radio Bursts
• Neural network reconstruction of cosmology using the Pantheon compilation
• Constraints on Cosmological Parameters with a Sample of Type Ia Supernovae from JWST
• Planck-PR4 anisotropy spectra show (better) consistency with General Relativity
• Modified cosmology from quantum deformed entropy
• Dark Sectors with Mass Thresholds Face Cosmological Datasets
• IDECAMB: an implementation of interacting dark energy cosmology in CAMB
• HOD-Dependent Systematics in Emission Line Galaxies for the DESI 2024 BAO analysis
• A hybrid model of viscous and Chaplygin gas to tackle the Universe acceleration
• A Tale of Two Type Ia Supernovae: The fast-declining siblings SNe 2015bo and 1997cn
• Bulk Flow Motion Detection in the Local Universe with Pantheon$+$ Type Ia Supernovae
• Gamma Rays Bursts: A Viable Cosmological Probe?
• Universe opacity and Type Ia supernova dimming
• Testing cosmic anisotropy with Pade approximation and Pantheon+ sample
• Constraints on self-interacting Bose-Einstein condensate dark matter using large-scale observables
• The Large Array Survey Telescope -- Science Goals
• Running Hubble constant: evolutionary Dark Energy
• Sweeping Horndeski Canvas: New Growth-Rate Parameterization for Modified-Gravity Theories
• A New Test of Dynamical Dark Energy Models and Cosmic Tensions in Hořava Gravity
• Improving Bayesian posterior correlation analysis on Type Ia supernova luminosity evolution
• A non-parametric test of variability of Type Ia supernovae luminosity and CDDR
• A model-independent method with phantom divide line crossing in Weyl-type $f(Q,T)$ gravity
• Calibration of gamma-ray bursts luminosity correlations using gravitational waves as standard sirens
• Discordance of dipole asymmetries seen in recent large radio surveys with the Cosmological Principle
• Cosmological measurements from void-galaxy and galaxy-galaxy clustering in the Sloan Digital Sky Survey
• Transit cosmological models in Myrzakulov F(R,T) gravity theory
• New Early Dark Energy as a solution to the $H_0$ and $S_8$ tensions
• Redshift Evolution and Non-Universal Dispersion of Quasar Luminosity Correlation
• Modified gravity in the presence of matter creation: scenario for the late Universe
• Testing the $n_s-H_0$ scaling relation with Planck-independent CMB data
• ZTF SN Ia DR2: Environmental dependencies of stretch and luminosity of a volume limited sample of 1,000 Type Ia Supernovae
• A critical discussion on the $H_0$ tension
• The simplest parametrization of equation of state parameter in the scalar field Universe
• Testing MOdified Gravity (MOG) theory and dark matter model in Milky Way using the local observables
• Strongly lensed type Ia supernovae as a precise late-universe probe of measuring the Hubble constant and cosmic curvature
• Constraining constant and tomographic coupled dark energy with low-redshift and high-redshift probes
• The $S_8$ Tension in Light of Updated Redshift-Space Distortion Data and PAge Approximation
• Extended $\Lambda$CDM model and viscous dark energy: A Bayesian analysis
• Observational Constraints on Growth Index with Cosmography
• Consistent extinction model for type Ia supernovae in Cepheid-based calibration galaxies and its impact on $H_0$
• How does an incomplete sky coverage affect the Hubble Constant variance?
• Constraining Dark-Matter Ensembles with Supernova Data
• Interaction of divergence-free deceleration parameter in Weyl-type $f(Q,T)$ gravity
• Oscillating dark energy in light of the latest observations and its impact on the Hubble tension
• A Distance-Deviation Consistency and Model-Independent Method to Test the Cosmic Distance-Duality Relation
• Can $f(R)$ gravity relieve $H_0$ and ${\sigma }_8$ tensions?
• The observed number counts in luminosity distance space
• Pseudoscalar sterile neutrino self-interactions in light of Planck, SPT and ACT data
• Search for transient optical counterparts to high-energy IceCube neutrinos with Pan-STARRS1
• Phenomenological Gravitational Phase Transition: Early and Late Modifications
• Constraining the anisotropy of the Universe with the X-ray and UV fluxes of quasars
• Holographic and Gravity-Thermodynamic Approaches in Entropic Cosmology: Bayesian Assessment using late-time Data
• Model-independent constraints on Type Ia supernova light-curve hyper-parameters and reconstructions of the expansion history of the Universe
• CoLFI: Cosmological Likelihood-free Inference with Neural Density Estimators
• $f\left(R,{\nabla }_{{\mu }_1}R,\dots ,{\nabla }_{{\mu }_1}\dots {\nabla }_{{\mu }_n}R\right)$ theories of gravity in Einstein frame: A higher order modified Starobinsky inflation model in the Palatini approach
• The Dark Energy Survey Supernova Program: Cosmological Analysis and Systematic Uncertainties
• Unbiased Cosmic Opacity Constraints from Standard Sirens and Candles
• A brief review on cosmological analysis of galaxy surveys with multiple tracers
• The Oscillatory Universe, phantom crossing and the Hubble tension
• Cosmology-informed neural networks to solve the background dynamics of the Universe
• Multiple measurements of gravitational waves acting as standard probes: model-independent constraints on the cosmic curvature with DECIGO
• Unitarity at the Late time Boundary of de Sitter
• Observational constraints on the interacting dark energy - dark matter (IDM) cosmological models
• Detection and classification of supernovae beyond z~2 redshift with the James Webb Space Telescope
• Reconciling low and high redshift GRB luminosity correlations
• Theoretical and numerical perspectives on cosmic distance averages
• Reconstructing Quintessence
• Barrow Holographic Dark Energy Model with GO Cut-off -- An Alternative Perspective
• Generalised model-independent characterisation of strong gravitational lenses V: reconstructing the lensing distance ratio by supernovae for a general Friedmann universe
• Using newest VLT-KMOS HII Galaxies and other cosmic tracers to test the $\Lambda$CDM tension
• Latest data constraint of some parameterized dark energy models
• Improving cosmological parameter estimation with the future 21 cm observation from SKA
• Direct Estimate of the Post-Newtonian Parameter and Cosmic Curvature from Galaxy-scale Strong Gravitational Lensing
• Observable Predictions for Massive-Neutrino Cosmologies with Model-Independent Dark Energy
• Swampland Criteria in the Slotheon Field Dark Energy
• Cosmic expansion with matter creation and bulk viscosity
• An exponential equation of state of dark energy in the light of 2018 CMB Planck data
• Evidence for strong progenitor age dependence of type Ia supernova luminosity standardization process
• Cosmological Bounds on sub-GeV Dark Vector Bosons from Electromagnetic Energy Injection
• Constraints from Fermi observations of Long Gamma-Ray Bursts on cosmological parameters
• Constraints on dark energy models from the Horndeski theory
• Reconstruction of late-time cosmology using Principal Component Analysis
• Cosmography of the Local Universe by Multipole Analysis of the Expansion Rate Fluctuation Field
• Quintessence-like features in the late-time cosmological evolution of $f(Q)$ symmetric teleparallel gravity
• A null test of the Cosmological Principle with BAO measurements
• Cosmological Implications of $f(R,\Sigma ,T)$ Gravity: A Unified Approach Using OHD and SN Ia Data
• On sign-changeable interaction in FLRW cosmology
• Testing a varying-$\Lambda$ model for dark energy within Co-varying Physical Couplings framework
• Parameter estimation of eccentric gravitational waves with a decihertz observatory and its cosmological implications
• First study of reionization in tilted flat and untilted non-flat dynamical dark energy inflation models
• Updating constraints on phantom crossing $f(T)$ gravity
• Testing the cosmic distance duality relation with Type Ia supernova and transverse BAO measurements
• Differentiating dark interactions with perturbation
• Inverse Cosmography: testing the effectiveness of cosmographic polynomials using machine learning
• Addressing Cosmological Tensions by Non-Local Gravity
• Probing the Seesaw Mechanism with Cosmological Data
• Diagnostic and Comparative Analysis of Dark Energy Models with $q(z)$ Parametrizations
• Electron mass variation from dark sector interactions and compatibility with cosmological observations
• The growth factor parametrization versus numerical solutions in flat and non-flat dark energy models
• Constraining a causal dissipative cosmological model
• Observational Constraints on Hybrid Scale Factor in f(Q,T) Gravity with Anisotropic Space-Time
• Roles of Modified Chaplygin-Jacobi and Chaplygin-Abel Gases in FRW Universe
• f(T) cosmology against the cosmographic method: A new study using mock and observational data
• Observational constraints on soft dark energy and soft dark matter: challenging $\Lambda$CDM
• Anisotropy in Pantheon+ supernovae
• A cosmic glitch in gravity
• Hubble tension as a window on the gravitation of the dark matter sector
• Baryon acoustic oscillations in thin redshift shells from BOSS DR12 and eBOSS DR16 galaxies
• LADDER: Revisiting the Cosmic Distance Ladder with Deep Learning Approaches and Exploring its Applications
• The QCD Axion: Some Like It Hot
• DGP and DGPish cosmologies from $f(Q)$ actions
• Cosmic Growth in $f(T)$ Teleparallel Gravity
• Revisiting progenitor-age dependence of type Ia supernova luminosity standardization process
• Modified cosmology in $f(Q,L_m)$ gravity
• Cosmological bound on neutrino masses in the light of $H_0$ tension
• Forecasts on interacting dark energy with standard sirens
• Can decaying dark matter scenarios alleviate both $H_0$ and ${\sigma }_8$ tensions?
• The HST See Change Program: I. Survey Design, Pipeline, and Supernova Discoveries
• A Test of the Standard Cosmological Model with Geometry and Growth
• The effects of peculiar velocities in SN Ia environments on the local $H_0$ measurement
• Probing variation of the fine-structure constant in runaway dilaton models using Strong Gravitational Lensing and Type Ia Supernovae
• Forecast constraints on Anisotropic Stress in Dark Energy using gravitational-waves
• Designing an Optimal LSST Deep Drilling Program for Cosmology with Type Ia Supernovae
• Bayesian Comparison of the Cosmic Duality Scenarios
• FLRW Cosmology in Metric-Affine $F(R,Q)$ Gravity
• Using Host Galaxy Spectroscopy to Explore Systematics in the Standardisation of Type Ia Supernovae
• Analytic Solutions and Observational support: A study of $f(R,T)$ gravity with $f(R,T)=R+h(T)$
• New cosmological constraints on the evolution of dark matter energy density
• On the amount of peculiar velocity field information in supernovae from LSST and beyond
• Testing the Cosmic Distance Duality Relation Using Strong Gravitational Lensing Time Delays and Type Ia Supernovae
• Pre-explosive accretion and simmering phases of Type Ia Supernovae
• Observational constraints on interacting vacuum energy with linear interactions
• SN 2018agk: A Prototypical Type Ia Supernova with a Smooth Power-law Rise in Kepler (K2)
• The First Data Release from SweetSpot: 74 Supernovae in 36 Nights on WIYN+WHIRC
• Type Ia supernovae data with scalar-tensor gravity
• From Hubble to Snap Parameters: A Gaussian Process Reconstruction
• Recovering $\Lambda$CDM Model From a Cosmographic Study
• Momentum transfer in the dark sector and lensing convergence in upcoming galaxy surveys
• Cosmic acceleration with bulk viscosity in an anisotropic $f(R,L_m)$ background
• Low-redshift measurement of the sound horizon through gravitational time-delays
• Impact of the damping tail on neutrino mass constraints
• Gopakumar-Vafa Hierarchies in Winding Inflation and Uplifts
• Carnegie Supernova Project-II: Near-infrared spectral diversity and template of Type Ia Supernovae
• Dark energy, Ricci-nonflat spaces, and the Swampland
• Constraints from High-Precision Measurements of the Cosmic Microwave Background: The Case of Disintegrating Dark Matter with $\Lambda$ or Dynamical Dark Energy
• Constraining Cosmological and Galaxy Parameters using Strong Gravitational Lensing Systems
• Can dark matter-dark energy interaction alleviate the Cosmic Coincidence Problem?
• Investigating the relationship between cosmic curvature and dark energy models with the latest supernova sample
• Cosmological model with linear equation of state parameter in f(R, Lm) gravity
• Observational Constraints and Cosmographic Analysis of $f(T,T_G)$ Gravity and Cosmology
• Cosmology with viscous generalized Chaplygin gas in $f(Q)$ gravity
• Model-Independent Determination of $H_0$ and ${\Omega }_{K,0}$ using Time-Delay Galaxy Lenses and Gamma-Ray Bursts
• Bayesian analysis of a Unified Dark Matter model with transition: can it alleviate the $H_0$ tension?
• Investigating dark energy by electromagnetic frequency shifts
• Consistency of Pantheon+ supernovae with a large-scale isotropic universe
• A Sample of Dust Attenuation Laws for DES Supernova Host Galaxies
• Inflation and the cosmological (not-so) constant in unimodular gravity
• Toward a direct measurement of the cosmic acceleration: the first preparation with FAST
• Time-averaging axion-like interacting scalar fields models
• Pantheon+ constraints on dark energy and modified gravity: An evidence of dynamical dark energy
• Hints of Neutrino Dark Matter scattering in the CMB? Constraints from the Marginalized and Profile Distributions
• A single parameterization for dark energy and modified gravity models
• Constrained cosmological model in $f(Q,T)$ gravity with non-linear non-metricity
• Quantifying the CMB Degeneracy Between the Matter Density and Hubble Constant in Current Experiments
• Cosmography from well-localized Fast Radio Bursts
• The DEHVILS Survey Overview and Initial Data Release: High-Quality Near-Infrared Type Ia Supernova Light Curves at Low Redshift
• Using Rest-Frame Optical and NIR Data from the RAISIN Survey to Explore the Redshift Evolution of Dust Laws in SN Ia Host Galaxies
• Chasing cosmic inflation: constraints for inflationary models and reheating insights
• A GREAT model comparison against the cosmological constant
• Measuring the speed of light with updated Hubble diagram of high-redshift standard candles
• Quantifying the tension between cosmological models and JWST red candidate massive galaxies
• Unphysical properties in a class of interacting dark energy models
• GRB Redshift Estimation using Machine Learning and the Associated Web-App
• Constraints on Dark Energy Models Using Late Universe Probes
• Quasars as Standard Candles IV. Analysis of the X-ray and UV indicators of the disc-corona relation
• Prospects of constraining $f(T)$ gravity with the third-generation gravitational-wave detectors
• Cosmological Tests of $f(R,G,T)$ Dark Energy Model in FRW Universe
• Dark Energy Nature in Logarithmic $f(R,T)$ Cosmology
• Hubble distancing: Focusing on distance measurements in cosmology
• $H_0$ tension without CMB data: beyond the $\Lambda$CDM
• Model-independent estimation of the cosmography parameters using cosmic chronometers
• Constraints from observational data for a running cosmological constant and warm dark matter with curvature
• Correcting for peculiar velocities of Type Ia Supernovae in clusters of galaxies
• ZTF SN Ia DR2: Study of Type Ia Supernova lightcurve fits
• Reducing the $H_0$ Tension with Exponential Acoustic Dark Energy
• A new Parametrization for Bulk Viscosity Cosmology as Extension of the $\Lambda$CDM Model
• Measurement of the matter-radiation equality scale using the extended Baryon Oscillation Spectroscopic Survey Quasar Sample
• An estimate of the dark matter density from galaxy clusters and supernovae data
• Calibrating the cosmic distance ladder using gravitational-wave observations
• Lifshitz cosmology: quantum vacuum and Hubble tension
• TiDES: The 4MOST Time Domain Extragalactic Survey
• A Dark Energy Quintessence Model of the Universe
• Discrepancy between cosmological and electroweak observables in Higgs Inflation
• Kinetically Coupled Scalar Fields Model and Cosmological Tensions
• Strongly lensed gravitational waves as the probes to test the cosmic distance duality relation
• Null tests of the concordance model in the era of Euclid and the SKA
• Dynamical analysis in regularized $4D$ Einstein-Gauss-Bonnet gravity with non-minimal coupling
• The cosmic transparency measured with Type Ia supernovae: implications for intergalactic dust
• The cross-correlation of galaxies in absorption with the Lyman $\alpha$ forest
• Holographic energy density, dark energy sound speed, and tensions in cosmological parameters: $H_0$ and $S_8$
• Does the fraction of dark matter diminish with early dark energy?
• Testing cosmic opacity with the combination of strongly lensed and unlensed supernova Ia
• Environmental Dependence of Type Ia Supernovae in Low-Redshift Galaxy Clusters
• Photometric classification of HSC transients using machine learning
• The Simulated Catalogue of Optical Transients and Correlated Hosts (SCOTCH)
• Screening Mechanism and Late-time Cosmology: Role of a Chameleon-Brans-Dicke Scalar Field
• Cosmological model-independent constraints on the baryon fraction in the IGM from fast radio bursts and supernovae data
• Lensing impact on cosmic relics and tensions
• Early dark energy constraints with late-time expansion marginalization
• $f(T)$ cosmology in the regime of quasar observations
• Dynamics and statefinder analysis of a class of sign-changeable interacting dark energy scenarios
• f(R) Gravity in an Ellipsoidal Universe
• DE models with combined $H_0\cdot r_d$ from BAO and CMB dataset and friends
• Observing the dark sector
• Dark matter from torsion in Friedmann cosmology
• Thermodynamically consistent entropic-force cosmology
• Cosmological constraints on time-varying cosmological terms: A study of FLRW universe models with $\Lambda (t)$CDM cosmology
• Space-borne atom interferometric gravitational wave detections. Part I. The forecast of bright sirens on cosmology
• Photometric Supernovae Redshift Systematics Requirements
• Redshift-evolutionary X-ray and UV luminosity relation of quasars from Gaussian copula
• Inferring dark energy properties from the scale factor parametrisation
• Third-order corrections to the slow-roll expansion: calculation and constraints with Planck, ACT, SPT, and BICEP/Keck
• The impact of the Universe's expansion rate on constraints on modified growth of structure
• Non-thermal neutrino-like hot dark matter in light of the $S_8$ tension
• On the cosmic distance duality relation and the strong gravitational lens power law density profile
• Is gravity getting weaker at low z? Observational evidence and theoretical implications
• A Probabilistic Autoencoder for Type Ia Supernovae Spectral Time Series
• ISiTGR: Testing deviations from GR at cosmological scales including dynamical dark energy, massive neutrinos, functional or binned parametrizations, and spatial curvature
• Reconstructing a non-linear interaction in the dark sector with cosmological observations
• Cosmological fluids in the equivalence between Rastall and Einstein gravity
• A Photometric Analysis of the Relationship Between Type Ia Supernova UV Flux and Host Galaxy Metallicity
• Model Independent Analysis of Supernova Data, Dark Energy, Trans-Planckian Censorship and the Swampland
• $H_0$ Tension on the Light of Supermassive Black Hole Shadows Data
• Exploring cosmological evolution and constraints in $f(T)$ teleparallel gravity
• First constraints on non-minimally coupled Natural and Coleman-Weinberg inflation and massive neutrino self-interactions with Planck+BICEP/Keck
• Reconstructing the Hubble parameter with future Gravitational Wave missions using Machine Learning
• Probing the Progenitors of Type Ia Supernovae using Circumstellar Material Interaction Signatures
• Low-energy modified gravity signatures on the large-scale structures
• Analytical Gaussian Process Cosmography: Unveiling Insights into Matter-Energy Density Parameter at Present
• A visual tool for assessing tension-resolving models in the $H_0$-${\sigma }_8$ plane
• Standardizing the Gamma-ray burst as a standard candle and applying to the cosmological probes: constraints on the two-component dark energy model
• The Reconstruction of Constant Jerk Parameter with $f(R,T)$ Gravity in Bianchi-I spacetime
• Deep learning method in testing the cosmic distance duality relation
• Constraints on interacting dynamical dark energy and a new test for $\Lambda$CDM
• A More Accurate Parameterization based on cosmic Age (MAPAge)
• Is there evidence for a hotter Universe?
• Testing the growth rate in homogeneous and inhomogeneous interacting vacuum models
• Squared torsion $f(T,\mathcal{T})$ gravity and its cosmological implications
• Dark Matter in Fractional Gravity I: Astrophysical Tests on Galactic Scales
• Direct tests of General Relativity under screening effect with galaxy-scale strong lensing systems
• The Dark Energy Survey Supernova Program: Corrections on photometry due to wavelength-dependent atmospheric effects
• Minimal model dependent constraints on cosmological nuisance parameters and cosmic curvature from combinations of cosmological data
• Constraining the emergent dark energy models with observational data at intermediate redshift
• Constraining R${}_V$ Variation Using Highly Reddened Type Ia Supernovae from the Pantheon+ Sample
• $f(T,B)$ Gravity in the late Universe in the context of local measurements
• Imprint of a Steep Equation of State in the growth of structure
• Spatial curvature sensitivity to local $H_0$ from the Cepheid distance ladder
• Bulk viscous cosmological model in $f(T,\mathcal{T})$ modified gravity
• Reconstructing the extended structure of multiple sources strongly lensed by the ultra-massive elliptical galaxy SDSS J0100+1818
• Observational constraints on the fractal cosmology
• Binning is Sinning: Redemption for Hubble Diagram using Photometrically Classified Type Ia Supernovae
• Exploring the Cosmological Model in $f(R,T^{\varphi })$ Gravity with Observational Constraints
• Curvature dominance DE-model in $f(R)$-gravity
• HI intensity mapping correlation function from UNIT simulations: BAO and observationally induced anisotropy
• 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
• Observation constraints on scalar field cosmological model in Anisotropic universe
• Cosmology in Brans-Dicke-de Rham-Gabadadze-Tolley massive gravity
• Quasars as standard candles VI: spectroscopic validation of the cosmological sample
• Band-limited Features in the Primordial Power Spectrum Do Not Resolve the Hubble Tension
• Observational constraints on varying fundamental constants in a minimal CPC model
• Exploring bulk viscous unified scenarios with Gravitational Waves Standard Sirens
• Unveiling the Hubble Constant through Galaxy Cluster Gas Mass Fractions
• Cosmological Constraints on Scalar Field Dark Matter
• Study of a viscous $\Lambda$WDM model: Near equilibrium condition, entropy production, and cosmological constraints
• The tension in the absolute magnitude of Type Ia supernovae
• Shan--Chen interacting vacuum cosmology
• Prospects for weighing neutrinos in interacting dark energy models using joint observations of gravitational waves and $\gamma$-ray bursts
• Kerr-NUT-de Sitter as an Inhomogeneous Non-Singular Bouncing Cosmology
• Observational Constraints on the Dark Energy with a Quadratic Equation of State
• A unified geometric description of the Universe: from inflation to late-time acceleration without an inflaton nor a cosmological constant
• Constraining Holographic Dark Energy and Analyzing Cosmological Tensions
• Constraints on Cosmographic Functions of Cosmic Chronometers Data Using Gaussian Processes
• Do we need wavelets in the late Universe?
• The Hubble tension in the non-flat Super-$\Lambda \mathrm{CDM}$ model
• Dissecting kinetically coupled quintessence: phenomenology and observational tests
• Narrowing down the Hubble tension to the first two rungs of distance ladders
• On The Distribution of Bayesian Evidences
• On the cosmological performance of photometrically classified supernovae with machine learning
• Comprehensive Constraints on Dark Radiation Injection After BBN
• The H0 trouble: Confronting Non-thermal Dark Matter and Phantom Cosmology with the CMB, BAO, and Type Ia Supernovae data
• Will Gravitational Wave Sirens Determine the Hubble Constant?
• Terrestrial Probes of Electromagnetically Interacting Dark Radiation
• Evidence of dark energy in different cosmological observations
• Dark energy constraint on equation of state parameter in the Weyl type $f(Q,T)$ gravity
• Resolving Hubble tension with the Milne model
• Can the Universe decelerate in the future?
• asevolution: a relativistic N-body implementation of the (a)symmetron
• Weak gravity on a $\Lambda$CDM background
• Systematic errors on optical-SED stellar mass estimates for galaxies across cosmic time and their impact on cosmology
• Signatures of Light Massive Relics on nonlinear structure formation
• Observational constraints on interactions between dark energy and dark matter with momentum and energy transfers
• Constraints on the speed of sound in the k-essence model of dark energy
• IR quantum gravity solves naturally cosmic acceleration and its coincidence problem
• Dissipative Unified Dark Fluid Model
• Parameter inference and model comparison using theoretical predictions from noisy simulations
• On the question of measuring spatial curvature in an inhomogeneous universe
• Constraints on the Transition Redshift using Hubble Phase Space Portrait
• Probing Weyl-type $f(Q,T)$ gravity: Cosmological implications and constraints
• Cosmological effects of the Galileon term in Scalar-Tensor Theories
• Cosmological Constraints on Entropic Cosmology with Matter Creation
• The failure of testing for cosmic opacity via the distance-duality relation
• One-parameter dynamical dark-energy from the generalized Chaplygin gas
• Investigating dark energy by electromagnetic frequency shifts II: the Pantheon+ sample
• A generalized $\Lambda$CDM model with parameterized Hubble parameter in particle creation, viscous and $f(R)$ model framework
• The cosmology of $f(R,L_m)$ gravity: constraining the background and perturbed dynamics
• No evidence for EDE from Planck data in extended scenarios
• Cosmography using strong lensing systems and cosmic chronometers
• Distance-duality in theories with a nonminimal coupling to gravity
• Scaling solutions as Early Dark Energy resolutions to the Hubble tension
• Blast From the Past: Constraining Progenitor Models of SN 1972E
• Minihalos as probes of the inflationary spectrum: accurate boost factor calculation and new CMB constraints
• Breaking the baryon-dark matter degeneracy in a model-independent way through the Sunyaev-Zeldovich effect
• The DESI One-Percent Survey: Modelling the clustering and halo occupation of all four DESI tracers with Uchuu
• A study of Si II and S II features in spectra of Type Ia supernova
• Reference level of the vacuum energy density of the Universe and astrophysical data
• Viscous fluid cosmology in symmetric teleparallel gravity
• Testing Modified Gravity theory (MOG) with Type Ia Supernovae, Cosmic Chronometers and Baryon Acoustic Oscillations
• Real-time cosmology with SKA
• Signature flips in time-varying $\Lambda (t)$ cosmological models with observational data
• Self-interacting neutrinos, the Hubble parameter tension, and the Cosmic Microwave Background
• Bulk viscous fluid in symmetric teleparallel cosmology: theory versus experiment
• SN Ia Standardization on the Rise: Evidence for the Cosmological Importance of Pre-Maximum Measurements
• The effective running Hubble constant in SNe Ia as a marker for the dark energy nature
• Initial Evaluation of SNEMO2 and SNEMO7 Standardization Derived From Current Light Curves of Type Ia Supernovae
• 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 Logotropic Dark Fluid: Observational and Thermodynamic Constraints
• Constraints on sterile neutrinos and the cosmological tensions
• Going Forward with the Nancy Grace Roman Space Telescope Transient Survey: Validation of Precision Forward-Modeling Photometry for Undersampled Imaging
• Observational constraints in Delta Gravity: CMB and supernovas
• Cosmological constraints with the Effective Fluid approach for Modified Gravity
• Testing the Homogeneity of Type Ia Supernovae in the Near-Infrared for Accurate Distance Estimations
• Dark energy reconstruction analysis with artificial neural networks: Application on simulated Supernova Ia data from Rubin Observatory
• Dark Matter Cosmology with Varying Viscosity: a Possible Resolution to the $S_8$ Tension
• Hubble tension as a window on the gravitation of the dark matter sector: Exploration of a family of models
• Joint Analysis of Constraints on f(R) Parametrization from Recent Cosmological Observations
• Cosmological Boundary Flux Parameter
• Coupled Dark Sector Models and Cosmological Tensions
• Interacting quintessence cosmology from Noether symmetries: comparing theoretical predictions with observational data
• $H_0$ tension or $M$ overestimation?
• The interacting vacuum and tensions: a comparison of theoretical models
• A Spectroscopic Model of the Type Ia Supernova--Host Galaxy Mass Correlation from SALT3
• Interacting Models of Dark Energy and Dark Matter in Einstein scalar Gauss Bonnet Gravity
• Resolving FLRW cosmology through effective equations of state in $f(T)$ gravity
• Square-Root parametrization of dark energy in $f(Q)$ cosmology
• Constraints on the Spacetime Dynamics of an Early Dark Energy Component
• X-ray Limits on the Progenitor System of the Type Ia Supernova 2017ejb
• Forecasts of cosmological constraints from Type Ia supernovae including the weak-lensing convergence
• Test of Artificial Neural Networks in Likelihood-free Cosmological Constraints: A Comparison of IMNN and DAE
• Bayesian Comparison of Interacting Modified Holographic Ricci Dark Energy Scenarios
• Constraining the Dimensionality of SN Ia Spectral Variation with Twins
• Cosmological constraints on $f(Q)$ gravity models in the non-coincident formalism
• Measuring Cosmological Distances Using Cluster Edges as a Standard Ruler
• Is there a dynamical tendency in H0 with late time measurements?
• Constraining Exponential f(Q) Gravity with Cosmic Chronometers and Supernovae: A Data-Driven Analysis
• The Hubble constant from two sibling Type Ia supernovae in the nearby galaxy NGC 4414: SN 1974G and SN 2021J
• Potentialities of Hubble parameter and expansion rate function data to alleviate Hubble tension
• Reconstructing the Hubble diagram of gamma-ray bursts using deep learning
• Dark energy with the help of interacting dark sectors
• Modified Equations of State for Dark Energy and Observational Limitations
• Effect of low anisotropy on cosmological models by using supernova data
• Distinguish the $f(T)$ model from $\Lambda$CDM model with Gravitational Wave observations
• Impact of Rubin Observatory cadence choices on supernovae photometric classification
• On the relationship between Type Ia supernova luminosity and host-galaxy properties
• Emergence of space and expansion of universe
• Low-Redshift Constraints on Covariant Canonical Gauge Theory of Gravity
• Phenomenological Dark Energy model with hybrid dynamic Cosmological Constant
• Non-parametric modeling of the cosmological data, base on the ${\chi }^2$ distribution
• Addressing the Hubble tension in Yukawa cosmology?
• Interpreting Internal Consistency of DES Measurements
• Cosmological constraints on ultra-light axion fields
• Cosmological Constraints on Thermal Friction of Axion Dark Matter
• Model selection and parameter estimation using the iterative smoothing method
• Domain Wall Network: A Dual Solution for Gravitational Waves and Hubble Tension?
• A search for the fine-structure constant evolution from fast radio bursts and type Ia supernovae data
• Compact objects and the swampland
• Tests of Standard Cosmology in Horava Gravity and Bayesian Evidence for a Closed Universe, and the Hubble Tension
• A convenient approach to characterizing model uncertainty with application to early dark energy solutions of the Hubble tension
• Constraining Coupling Constants' Variation with Supernovae, Quasars, and GRBs
• Confronting quantum-corrected teleparallel cosmology with observations
• Understanding Type Ia Supernova Distance Biases by Simulating Spectral Variations
• The interaction of extended Bose-Einstein condensate dark matter with viscous $f(T,B)$ gravity
• Casimir cosmology
• Exploring Modified Gravity: Constraints on the $\mu$ and $\Sigma$ Parametrization with WMAP, ACT, and SPT
• Constraining Cosmological Parameters with Viscous Modified Chaplygin Gas and Generalized Cosmic Chaplygin Gas Models in Horava-Lifshitz Gravity: Utilizing Late-time Datasets
• Extended Bose-Einstein condensate dark matter in viscous Gauss-Bonnet gravity
• Photometric Data-driven Classification of Type Ia Supernovae in the Open Supernova Catalog
• Cosmological Constraints on the Phenomenological Interacting Dark Energy Model with Fermi Gamma-Ray Bursts and DESI DR2
• Implications for cosmology from Ground-based Cosmic Microwave Background observations
• Luminosity distance uncertainties from gravitational wave detections by third generation observatories
• Testing the consistency of early and late cosmological parameters with BAO and CMB data
• Constraints on Cosmological Models with Gamma-Ray Bursts in Cosmology-Independent Way
• Forecasting constraints on the baryon mass fraction in the IGM from fast radio bursts and type Ia supernovae
• Specific Effect of Peculiar Velocities on Dark-Energy Constraints from Type Ia Supernovae
• Forays into the dark side of the swamp
• FREmu: Power Spectrum Emulator for $f(R)$ Gravity
• Deep Learning and genetic algorithms for cosmological Bayesian inference speed-up
• See Change: VLT spectroscopy of a sample of high-redshift Type Ia supernova host galaxies
• Exploring the potentiality of standard sirens to probe cosmic opacity at high redshifts
• Exploring Alternative Cosmologies with the LSST: Simulated Forecasts and Current Observational Constraints
• Cosmological-model-independent tests of cosmic distance duality relation with Type Ia supernovae and radio quasars
• Two Dynamical Scenarios for Binned Master Sample Interpretation
• Consistency of Cubic Galileon Cosmology: Model-Independent Bounds from Background Expansion and Perturbative Analyses
• Euclid: Testing the Copernican principle with next-generation surveys
• Constraining Temporal Oscillations of Cosmological Parameters Using Type Ia Supernovae
• SN 2019ein: A Type Ia Supernova Likely Originated from a Sub-Chandrasekhar-Mass Explosion
• Simultaneous measurements on cosmic curvature and opacity using latest HII regions and $H(z)$ observations
• The viable f(G) gravity models via reconstruction from the observations
• Observational Hubble parameter data constraints on the interactive model of $f(T)$ gravity with particle creation
• Model-independent determination of cosmic curvature based on Padé approximation
• Impact of Cosmology on Lorentz Invariance Violation Constraints from GRB Time-Delays
• Spherical Collapse Approach for Non-standard Dark Matter Models and Enhanced Early Galaxy Formation in JWST
• Symbolic Implementation of Extensions of the $\text{PyCosmo}$ Boltzmann Solver
• Cosmological Constraints using the newest VLT-KMOS HII Galaxies and the full Planck CMB spectrum
• Stress testing the dark energy equation of state imprint on supernova data
• Can acoustic and axion-like early dark energy still resolve the Hubble tension?
• Constraining cosmological scaling solutions of a Galileon field
• StarDICE I: sensor calibration bench and absolute photometric calibration of a Sony IMX411 sensor
• Constraints on Late Time Violations of the Equivalence Principle in the Dark Sector
• Statistical and Observation Comparison of Weyl-Type $f(Q,T)$ Models with the $\Lambda$CDM Paradigm
• Effects of a Late Gravitational Transition on Gravitational Waves and Anticipated Constraints
• High-Precision Redshifts for Type Ia Supernovae with the Nancy Grace Roman Space Telescope P127 Prism
• Confronting the Galactic 511 keV emission with $B-L$ gauge boson dark matter
• Thawing k-essence dark energy in the PAge space
• Impact of calibration uncertainties on Hubble constant measurements from gravitational-wave sources
• Flatness without CMB - the Entanglement of Spatial Curvature and Dark Energy Equation of State
• Magnification and evolution bias of transient sources: GWs and SNIa
• Constraints on dark energy from TDCOSMO & SLACS lenses
• Unveiling the Universe with Emerging Cosmological Probes
• Investigating the dynamical models of cosmology with recent observations and upcoming gravitational-wave data
• Magrathea-Pathfinder: A 3D adaptive-mesh code for geodesic ray tracing in $N$-body simulations
• Axi-Higgs cosmology: Cosmic Microwave Background and cosmological tensions
• More on Emergent Dark Energy from Unparticles
• Variability in Quasar Light Curves: using quasars as standard candles
• A new nonlinear instability for scalar fields
• Chameleon Early Dark Energy and the Hubble Tension
• Testing the phenomenological interacting dark energy model with gamma-ray bursts and Pantheon+ type Ia supernovae
• Difficulties in reconciling non-negligible differences between the local and cosmological values of the gravitational coupling in extended Brans-Dicke theories
• Litmus tests of the flat $\Lambda$CDM model and model-independent measurement of $H_0{r}_{\mathrm{d}}$ with LSST and DESI
• Late-time dynamics of dark energy EoS in symmetric teleparallel gravity
• Combining strongly lensed and unlensed fast radio bursts: To be a more precise late-universe probe
• Revisiting holographic dark energy from the perspective of multi-messenger gravitational wave astronomy: future joint observations with short gamma-ray bursts
• Interacting Barrow Holographic Dark Energy in Non-flat Universe
• Alleviating the Hubble Tension with a Local Void and Transitions of the Absolute Magnitude
• Uncalibrated Cosmic Standards as a Robust Test on Late-Time Cosmological Models
• Singling out modified gravity parameters and datasets reveals a dichotomy between Planck and lensing
• The impact of 2D and 3D BAO measurements on the Cosmic Distance Duality Relation with HII galaxies
• Concerns about the reliability of publicly available SNe Ia data
• Observational constraints on complex quintessence with attractive self-interaction
• Testing $f(T)$ Gravity with Cosmological Observations: Confronting the Hubble Tension and Implications for the Late-Time Universe
• Unveiling the Effects of Coupling Extended Proca-Nuevo Gravity on Cosmic Expansion with Recent Observations
• Constraining modified gravity scenarios with the 6dFGS and SDSS galaxy peculiar velocity datasets
• Analytic Calculation of Covariance between Cosmological Parameters from Correlated Data Sets, with an Application to SPTpol
• Fitting of supernovae without dark energy
• Cosmological model selection from standard siren detections by third-generation gravitational wave obervatories
• Surface Tension: Accelerated Expansion, Coincidence Problem & Hubble Tension
• Magnification bias in the shear-ratio test: a viable mitigation strategy
• Maximum Cosmological Information from Type-Ia Supernova Observations
• Growth and Geometry Split in Light of the DES-Y3 Survey
• Examining the validity of the minimal varying speed of light model through cosmological observations: relaxing the null curvature constraint
• Extended Bose-Einstein condensate dark matter in $f(Q)$ gravity
• Constraining neutrino mass in dynamical dark energy cosmologies with the logarithm parametrization and the oscillating parametrization
• Constraints on the minimally extended varying speed of light model using the Pantheon+ dataset
• Parameterized Deceleration in $f(Q,C)$ Gravity: A Logarithmic Approach
• Instabilities Appearing in Cosmological Effective Field theories: When and How?
• Climbing out of the shadows: building the distance ladder with black hole images
• Studies on dark energy evolution
• Scalar field dark energy: Insights into cosmological evolution and black hole accretion
• Do current observations support transient acceleration of our universe?
• Using simulated Tianqin gravitational wave data and electromagnetic wave data to study the coincidence problem and Hubble tension problem
• Expanding covariant cosmography of the local Universe: incorporating the snap and axial symmetry
• Investigating the cosmic distance duality relation with gamma-ray bursts
• Exploring parametrized dark energy models in interacting scenario
• Non-parametric reconstruction of the fine structure constant with galaxy clusters
• What does a cosmological experiment really measure? Covariant posterior decomposition with normalizing flows
• Decay of dark energy into dark matter in a metric $f(R)$ gravity: effective running Hubble constant
• Distinguishing freezing and thawing dark energy models through measurements of the fine-structure constant
• Cosmological implications of non-minimally coupled f(Q) gravity
• Observational backreaction in discrete black holes lattice cosmological models
• Cosmological impact of microwave background temperature measurements
• Cosmological constraints on $R^2$-corrected Appleby-Battye model
• Prospects for searching for sterile neutrinos with gravitational wave and $\gamma$-ray burst joint observations
• Variable Chaplygin Gas: Constraints from Supernovae, GRB and Gravitational Wave Merger Events
• Stellar Populations in type Ia supernova host galaxies at intermediate-high redshift: Star formation and metallicity enrichment histories
• Dark energy-dark matter interactions as a solution to the $S_8$ tension
• Model-independent Gamma-Ray Bursts Constraints on Cosmological Models Using Machine Learning
• Observational constraints on Tsallis holographic dark energy with Ricci horizon cutoff
• On the consistency of the expansion with the perturbations
• Model-Independent Reconstruction of Quintessence Potential and Kinetic Energy from DESI DR2 and Pantheon+ Supernovae
• Measuring the speed of light with cosmological observations: current constraints and forecasts
• LensWatch. II. Improved Photometry and Time-delay Constraints on the Strongly Lensed Type Ia Supernova 2022qmx ("SN Zwicky") with HST Template Observations
• Coupling quintessence kinetics to electromagnetism
• Scrutinizing coupled vector dark energy in light of data
• Quantum signatures from Horava-Lifshitz cosmography
• Beyond dark energy Fisher forecasts: how DESI will constrain LCDM and quintessence models
• Euclid: Relativistic effects in the dipole of the 2-point correlation function
• A New Parameterized Interacting Holographic Dark Energy
• Holographic Dark Energy from the Anti-de Sitter Black Hole
• Dynamical system analysis in modified Galileon cosmology
• Statistics of Thawing K-essence Dark Energy Models
• Higgs Inflation: constraining the top quark mass and breaking the $H_0$-${\sigma }_8$ correlation
• Interacting Dark Energy: New parametrization and observational constraints
• Phase-space analysis of torsion-coupled dilatonic ghost condensate
• An Analysis of Variance of the Pantheon+ Dataset: Systematics in the Covariance Matrix?
• Gravitational lens time-delay as a probe of a possible time variation of the fine-structure constant
• A new parametrization of Hubble function and Hubble tension
• Constraints on Bianchi-I type universe with SH0ES anchored Pantheon+ SNIa data
• Possible Impact of non-Gaussianities on cosmological constraints in neutrino physics
• Effects of Dark Energy anisotropic stress on the matter power spectrum
• Thermodynamics of Modified Chaplygin-Jacobi Gas and Modified Chaplygin-Abel Gas: Stability Analysis and Observational Constraints
• Fluctuating Dark Energy and the Luminosity Distance
• Fast Radio Bursts as Standard Candles for Cosmology
• Constraining late-time transitions in the dark energy equation of state
• Testing time-delayed cosmology
• Cosmological inference from within the peculiar local universe
• A new way to test the WIMP dark matter models
• Reconstruction of a kinetic k--essence Lagrangian from a modified of dark energy equation of state
• The impact of weak lensing on Type Ia supernovae luminosity distances
• Gamma-Ray Bursts Calibrated from the Observational $H(z)$ Data in Artificial Neural Network Framework
• The first direct measurement of gravitational potential decay rate at cosmological scales and improved dark energy constraint
• Cosmic curvature on large-scale structures with homogeneous dark energy
• Towards a sound massive cosmology
• Observational constraints using Bayesian statistics and Deep Learning in $f(Q)$ gravity
• Constraints on Metastable Dark Energy Decaying into Dark Matter
• Hawai'i Supernova Flows: A Peculiar Velocity Survey Using Over a Thousand Supernovae in the Near-Infrared
• Tilted non-spatially-flat inflation
• Dark Matter Subhalos, Strong Lensing and Machine Learning
• Gravitational wave probes of Barrow cosmology with LISA standard sirens
• SN 2023adsy: A normal type Ia Supernova at z=2.9
• The Dependence of the Type Ia Supernova Host Bias on Observation or Fitting Technique
• Redshift evolution of the Hubble constant: Constraints and new insights from an interacting dark energy model
• Redshift-space distortion constraints on the neutrino mass and models to alleviate the Hubble tension
• Observational constraints on inflection point quintessence with a cubic potential
• Addressing the DESI DR2 Phantom-Crossing Anomaly and Enhanced $H_0$ Tension with Reconstructed Scalar-Tensor Gravity
• Bias of reconstructing the dark energy equation of state from the Pad$\acute{e}$ cosmography
• Emergent universe revisited through the CSL theory
• Impact of dark energy on the equation of state in light of the latest cosmological data
• Galaxy groups in the presence of Cosmological Constant: Increasing the Masses of Groups
• Dark matter or strong gravity?
• Testing CCC+TL Cosmology with Galaxy Rotation Curves
• Can an Anti-de Sitter Vacuum in the Dark Energy Sector Explain JWST High-Redshift Galaxy and Reionization Observations?
• Fast and Not-so-Furious: Case Study of the Fast and Faint Type IIb SN 2021bxu
• Constraining Cosmology with Double-source-plane Strong Gravitational Lenses from the AGEL Survey
• Dark matter deficient galaxies in the Illustris flat-$\Lambda$CDM model structure formation simulation
• Growth of cosmic perturbations in the modified $f(R,T)$ gravity
• The Hubble constant from galaxy cluster scaling-relation and SNe Ia observations: a consistency test
• Gravitational Wave luminosity distance in viscous cosmological models
• 2D BAO vs 3D BAO: Hints for new physics?
• Weak lensing magnification of Type Ia Supernovae from the Pantheon sample
• Cosmological Study in Myrzakulov $F(R,T)$ Quasi-dilaton Massive Gravity
• Testing the coincidence problem with strong gravitational lens, Type Ia supernovae and Hubble parameter observational data
• Constraining hybrid potential scalar field cosmological model in Lyra's geometry with recent observational data
• Cosmological signatures of a Rapid Diluted Energy Density
• High precision measurement of cosmic curvature: from gravitational waves and cosmic chronometer
• Equality scale-based and sound horizon-based analysis of the Hubble tension
• The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar and APOGEE-2 Data
• Cosmology of fermionic dark energy coupled to curvature
• Biases from Non-Simultaneous Regression with Correlated Covariates: A Case Study from Supernova Cosmology
• Modified $f(R,T)$ theory in light of gravitational wave standard sirens
• Viscous interacting and stability on dark matter Bose-Einstein condensation with modified Chaplygin gas
• Time dilation observed in Type Ia supernova light curves and its cosmological consequences
• Generalized Ghost Pilgrim Dark Energy Fractal Cosmology with Observational Constraint
• Propagating Uncertainties in the SALT3 Model Training Process to Cosmological Constraints
• Teleparallel Gravity and Quintessence: The Role of Nonminimal Boundary Couplings
• Diagnostic Approaches for Interacting generalized holographic Ricci Dark Energy Models
• Performance of Non-Parametric Reconstruction Techniques in the Late-Time Universe
• Role of Future SNIa Data from Rubin LSST in Reinvestigating Cosmological Models
• On the Metric $f(R)$ gravity Viability in Accounting for the Binned Supernovae Data
• Anisotropy in the cosmic acceleration inferred from supernovae
• On a possible cosmological evolution of galaxy cluster $Y_{\mathrm{X}}-Y_{\mathrm{SZE}}$ scaling relation
• The reconstruction of dark energy with Ridge Regression Approach
• A measure of cosmological distance using the \civ\ Baldwin effect in quasars
• THESEUS$-$BTA cosmological tests using Multimessenger Gamma-Ray Bursts observations
• Exploring the Evolution of Nonlinear Electrodynamics in the Universe: A Dynamical Systems Approach
• The Dawn of Black Holes
• [O II] as an Effective Indicator of the Dependence Between the Standardised Luminosities of Type Ia Supernovae and the Properties of their Host Galaxies
• Slitless spectrophotometry with forward modelling: principles and application to atmospheric transmission measurement
• A new instability in clustering dark energy?
• Constraints on the varying electron mass and early dark energy in light of ACT DR6 and DESI DR2 and the implications for inflation
• Perturbation in an interacting dark universe
• Non-Parametric Analysis for the Dark Matter Density Evolution
• Solving the Hubble tension à la Ellis & Stoeger 1987
• A new analytical approximation of luminosity distance by optimal HPM-Padé technique
• An Accelerating Universe without Lambda: Delta~Gravity Using Monte Carlo
• The optimal Padé polynomial for reconstruction of luminosity distance based on 10-fold cross-validation
• The establishment of the Standard Cosmological Model through observations
• Probing General Relativity in galactic scales at z $\sim 0.3$
• Structure Formation in Dark Matter Particle Production Cosmology
• The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch
• Cosmological Standard Timers from Unstable Primordial Relics
• Sparse formulae for the distance modulus in cosmology
• An exact solution of the observable universe in Bianchi V space-time
• Early dark energy in the pre- and post-recombination epochs
• Linear growth of structure in projected massive gravity
• Constraints on the phase transition of Early Dark Energy with the CMB anisotropies
• Reaffirmation of Cosmological Oscillations in the Scale Factor from the Pantheon Compilation of 1048 Type Ia Supernovae
• Hints of the $H_0-r_d$ tension in uncorrelated Baryon Acoustic Oscillations dataset
• Standardizing reverberation-measured Mg II time-lag quasars, by using the radius-luminosity relation, and constraining cosmological model parameters
• Misinterpreting Modified Gravity as Dark Energy: a Quantitative Study
• The Hubble Diagram: Jump from Supernovae to Gamma-Ray Bursts
• Cosmological model with Gong-Zong Parametrization in $f(R,L_m)$ gravity
• Implications of Dynamical Dark Energy in the expansion of the Universe and the Structure Formation
• Does fractal Universe favour warm inflation: Observational support?
• An Information Theory Approach on Deciding Spectroscopic Follow Ups
• Generalized Holographic Cosmology: low-redshift observational constraint
• Sound Horizon Independent Constraints on Early Dark Energy: The Role of Supernova Data
• Cosmological Evolution of Viscous Dark Energy in f(Q,C) Gravity: Two-Fluid Approach
• Reconstructions of Einstein-Aether Gravity from Barrow Agegraphic and New Barrow Agegraphic Dark Energy models: Examinations and Observational Limits
• Stellar Profile Independent Determination of the Dark Matter Distribution of the Fornax Local Group Dwarf Spheroidal Galaxy
• Equivalence of Dark Energy Models: A Theoretical and Bayesian Perspective
• Linear perturbations spectra for dynamical dark energy inspired by modified gravity
• An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$
• Observational constraints in late time for an axially symmetric transitioning model with bulk viscous fluid
• Revisiting the Hubble constant, sound horizon and cosmography from late-time Universe observations
• Dark energy explained by a bias in the measurements
• Cosmological constraints in symmetric teleparallel gravity with bulk viscosity
• Is Dark Energy Changing? Probing the Universe's Expansion with present and future astronomical probes
• No evidence for local $H_0$ anisotropy from Tully--Fisher or supernova distances
• Forecasting Cosmological Constraints from the Weak Lensing Magnification of Type Ia Supernovae Measured by the Nancy Grace Roman Space Telescope
• Cosmic expansion beyond $\Lambda$CDM: Investigating power-law and logarithmic corrections
• Stretch to stretch, dust to dust: lower-value local $H_0$ measurement from two-population modelling of type Ia supernovae
• Exact Solutions and Constraints on the Dark Energy Model in FRW Universe
• Common Origin of Warm Dark Matter and Dark Radiation
• Constraints on Axions from Cosmic Distance Measurements
• Redshift drift effect through the observation of HI 21cm signal with SKA
• Model-Agnostic Cosmological Inference with SDSS-IV eBOSS: Simultaneous Probing for Background and Perturbed Universe
• Characterizing the equivalence between dark energy and radiation using gamma-ray bursts
• Interacting dark sector with quadratic coupling: theoretical and observational viability
• On the Field Theoretical Description of an Alternative Model to Generalized Chaplygin Gas and its Thermodynamic Behaviour
• Late Time Phenomena in $f(T,\mathcal{T})$ Gravity Framework: Role of $H_0$ Priors
• Quantitative constraints on modified gravity paradigms
• Observational constraints on cosmological parameters in the Bianchi type III Universe with f(R,T) gravity theory
• Probing the independence within the dark sector in the fluid approximation
• Comparison of $f(R,T)$ Gravity with Type Ia Supernovae Data
• Lensing convergence and anisotropic dark energy in galaxy redshift surveys
• Unified Dark Energy and Dark Matter from Dynamical Spacetime Cosmology
• Anisotropic cosmology in Bumblebee gravity theory
• Effect of lensing magnification on type Ia supernova cosmology
• Deep learning reconstruction of the large scale structure of the Universe from luminosity distance observations
• Is warm inflation quasi-stable?
• A Tale of Three Dust Populations: Variable $R_{\mathrm{V}}$ and Extreme Polarization Along Sightlines Toward $\zeta$ Ophiuchi
• New Constraints on Anisotropic Expansion from Supernovae Type Ia
• Observational constraints on the massive neutrinos induced late-time cosmic acceleration
• The Hydrogen Intensity and Real-time Analysis eXperiment: 256-Element Array Status and Overview
• Constraints on Tsallis cosmology using recent low and high redshift measurements
• Hubble Tension in Power-Law f(R) Gravity and Generalized Brans-Dicke Theory
• The DEHVILS in the Details: Type Ia Supernova Hubble Residual Comparisons and Mass Step Analysis in the Near-Infrared
• Observational constraints and dynamical analysis of Kaniadakis horizon-entropy cosmology
• Constraining the swiss-cheese IR-fixed point cosmology with cosmic expansion
• Viscous fluid dynamics with decaying vacuum energy density
• Analytic Solutions of Scalar Field Cosmology, Mathematical Structures for Early Inflation and Late Time Accelerated Expansion
• Testing the coupling of dark radiations in light of the Hubble tension
• $\Lambda CDM$ periodic cosmology
• Quintessence and tachyon dark energy in interaction with dark matter: Observational constraints and model selection
• Is the large-scale structure traced by the BOSS LOWZ galaxies consistent with $\text{Planck}$?
• Boosting MonteCarlo sampling with a non-Gaussian fit
• A cosmological distance measure using radio-loud quasars
• Pantheon+ tomography and Hubble tension
• Cosmological models, observational data and tension in Hubble constant
• Can cosmic rotation resolve the Hubble tension? Constraints from CMB and large-scale structure
• Calibrating the effective magnitudes of type Ia supernovae with a model-independent method
• ZTF SN Ia DR2: Improved SN Ia colors through expanded dimensionality with SALT3+
• Investigating the compatibility of exact solutions in Weyl-type $f(Q,T)$ gravity with observational data
• Reconstructing cosmic evolution with a density parametrization
• Probing stellar-mass primordial black holes with type Ia supernova microlensing
• Constraining Axially Symmetric Bianchi Type I Model with Self-Consistent Recombination History and Observables
• Model independent calibration for sound horizon combining observations of supernovae and transversal BAO measurements
• Reconstructing the weak lensing magnification distribution of Type Ia supernovae
• Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints
• Bounding the Cosmological Constant using Galactic Rotation Curves from the SPARC Dataset
• Revisiting cosmological diffusion models in Unimodular Gravity and the $H_0$ tension
• The BINGO/ABDUS Project: Forecast for cosmological parameters from a mock Fast Radio Bursts survey
• Assessing the Robustness of the CPL Parametrization to Basis and Prior Variations: Insights from DESI DR2 BAO Data
• Prospects of Cosmic Superstring Detection through Microlensing of Extragalactic Point-Like Sources
• Dynamical Dark Energy Signatures from a New Transition $Om(z)$ Parametrization in Flat FLRW Cosmology
• Low redshift constraints on scale-covariant models
• Calibration of luminosity correlations of gamma-ray bursts using quasars
• Holographic Principle and the Second Law in Stephani Cosmology Revisited
• Phantom scalar field cosmologies constrained by early cosmic measurements
• ZTF SN Ia DR2: Impact of the galaxy cluster environment on the stretch distribution of Type Ia supernovae
• The snapshot distance method: estimating the distance to a Type Ia supernova from minimal observations
• Accounting for Correlations When Fitting Extra Cosmological Parameters
• New analysis of SNeIa Pantheon Catalog: Variable speed of light as an alternative to dark energy
• Theoretical priors in scalar-tensor cosmologies: Shift-symmetric Horndeski models
• Observational constraints on generic models of non-minimal curvature-matter coupling
• Type Ia Supernovae from First-generation Stars
• Matter production effects and interacting scenario within a reconstructed mimetic cosmology for late times
• Domain Wall Bianchi Type $V{I}_0$ Universe in $f(R,T)$ Gravity
• Observational constraints on thawing quintessence scalar field model
• Constraints on Multicomponent Dark Energy from Cosmological Observations
• Ultra-compact Objects of Non-minimally Coupled Dark Matter
• Probing gravity with the DES-CMASS sample and BOSS spectroscopy
• Unimodular Theory of Gravity in Light of the Latest Cosmological Data
• Bohmian Quantum Cosmology from the Wheeler-DeWitt Equation
• The string theory swampland in the Euclid, SKA and Vera Rubin observatory era
• A mechanism to generate varying speed of light via Higgs-dilaton coupling: Theory and cosmological applications
• Mimetic Tensor-Vector-Scalar Cosmology: Incorporating Dark Matter, Dark Energy and Stiff Matter
• Toward Cosmological Standard Timers in Primordial Black Hole Binaries
• Testing the Constancy of Type Ia Supernova Luminosities with Gaussian Process
• Observational constraint on Dark Energy from Quantum Uncertainty
• Cosmological viability of a double field unified model from warm inflation
• Solving the inverse cosmological calibration problem of gamma-ray bursts
• Two c's in a pod: Cosmology independent measurement of the Type Ia supernova colour-luminosity relation with a sibling pair
• A fractal LTB model cannot explain Dark Energy
• Towards a Composite Framework for Simultaneous Exploration of New Physics in Background and Perturbed Universe
• ZTF SN Ia DR2 follow-up: Exploring the origin of the Type Ia supernova host galaxy step through Si II velocities
• Analysis of Pantheon+ supernova data suggests evidence of sign-changing pressure of the cosmological fluid
• A Template-Based Approach to the Photometric Classification of SN 1991bg-like Supernovae in the SDSS-II Supernova Survey
• Cosmic expansion history analysis with Hubble parametrization in $Q^n$ gravity
• A Bayesian approach to truncated data sets: An application to Malmquist bias in Supernova Cosmology
• Artificial Neural Network Spectral Light Curve Template for Type Ia Supernovae and its Cosmological Constraints
• Accelerating Kaluza-Klein Universe in Modified Theory of Gravitation
• Thermodynamic parametrization of dark energy
• Dark energy with oscillatory tracking potential: Observational Constraints and Perturbative effects
• A Relativistic Tensorial Model for Fractional Interaction between Dark Matter and Gravity
• Detection of Unresolved Strongly Lensed Supernovae with 7-Dimensional Telescope
• Kaniadakis holographic dark energy: observational constraints and global dynamics
• Cosmological implications and causality in $f(R,L_m,T)$ gravity theory with observational constraints
• Assessing the potential of cluster edges as a standard ruler
• SN 2017fgc: A Fast-Expanding Type Ia Supernova Exploded in Massive Shell Galaxy NGC 474
• Accelerating Universe with binary mixture of bulk viscous fluid and dark energy
• Addressing type Ia supernova color variability with a linear spectral template
• Probing Time-Varying Dark Energy with DESI: The Crucial Role of Precision Matter Density (Ω_{m0}) Measurements
• Development of a model to investigate the effect of the bias in SNIa measurements related to the inhomogeneity of space
• Holographic Ricci DE as running vacuum with nonlinear interactions
• Exploring the Latest Pantheon SNIa Dataset by Using Three Kinds of Statistics Techniques
• Dark energy constraints in light of theoretical priors
• Fermionic wave functions and Grassmann fields as possible sources of dark energy
• Probing Systematic Bias in Low-Redshift Type Ia Supernova Measurements by Cross Analyzing Surface Brightness and Hubble Residuals
• Reconstruction of Tsallis Holographic Dark Energy via Modified Non-Metric Gravity: An $f(Q,C)$ Approach
• Constraining decaying dark matter with BOSS data and the effective field theory of large-scale structures
• The X-ray$-$UV Luminosity Relation of eROSITA Quasars
• Cosmological constraints on the big bang quantum cosmology model
• The New Status Qvo? SN 2021qvo is Another 2003fg-like Type Ia Supernova with a Rising Light-Curve Bump
• A step in the right direction? Analyzing the Wess Zumino Dark Radiation solution to the Hubble tension
• The Dark Energy Survey Supernova Program results: Type Ia Supernova brightness correlates with host galaxy dust
• Local dark energy in the Sculptor Filament of galaxies
• Testing the Distance Duality Relation with Cosmological Observations at high Redshift using Artificial Neural Network
• Cosmological Constraints on f(T,B) Gravity from Observations of Early and Late Universe
• Electromagnetic Waves in Cosmological Space-Time II. Luminosity Distance
• SN 2025ogs: A Spectroscopically-Normal Type Ia Supernova at z = 2 as a Benchmark for Redshift Evolution
• Forecasting the Constraint on the Hu-Sawicki $f(R)$ Modified Gravity in the CSST $3\times 2$pt Photometric Survey
• Time delay measurements with Broken Power Law model
• On observational signatures of multi-fractional theory
• Ricci cosmology in light of astronomical data
• Model independent reconstruction of cosmological accelerated-decelerated phase
• Confronting Einstein Yang Mills Higgs Dark Energy in light of observations
• Does the Reionization Model Influence the Constraints on Dark Matter Decay or Annihilation?
• Sub-percentage measure of distances to redshift of 0.1 by a new cosmic ruler
• Dissecting the $H_0$ and $S_8$ tensions with Planck + BAO + supernova type Ia in multi-parameter cosmologies
• Momentum transfer models of interacting dark energy
• Cosmology in energy-momentum squared symmetric teleparallel gravity
• From Nonparametric Distance Reconstruction to Testing the Etherington Relation and Cosmic Curvature Using 2D and 3D BAO Measurements
• Diversity of Type Ia supernova optical light curves among different spectroscopic subclasses
• A Bayesian estimator for peculiar velocity correction in cosmological inference from supernovae data
• Measurements of cosmic expansion and growth rate of structure from voids in the Sloan Digital Sky Survey between redshift 0.07 and 1.0
• $f(T,B)$ cosmography for high redshifts
• Blueshift of light rays induced by gravitational wave memory effect
• Cosmography via stellar archaeology of low-redshift early-type galaxies from SDSS
• Cosmology in the presence of diffeomorphism-violating, nondynamical background fields
• Euclid: Optimising tomographic redshift binning for 3$\times$2pt power spectrum constraints on dark energy
• Running Hubble Constant with the Redshift as a Marker of Evolutionary Dark Energy
• Spectral distortions in the decaying QCD dark matter scenario
• Cosmological Constraints on the DGP Model in light of DESI DR2 2025 Data
• Aletheia: Emulating the non-linear matter power spectrum in the context of evolution mapping
• Windowing Artifacts Likely Account for Recent Claimed Detection of Oscillating Cosmic Scale Factor
• Running Einstein Constant and a Possible Vacuum State of the Universe
• A comparative study of emergent dark energy models
• Design and performance of a Collimated Beam Projector for telescope transmission measurement using a broadband light source
• Viscous effect in the late time evolution of phantom universe
• Testing the CCC+TL cosmology with cosmic-chronometer measurements of the Hubble parameter
• Intermediate redshift calibration of Gamma-ray Bursts and cosmic constraints in non-flat cosmology
• Cosmic acceleration driven by dark matter self-interactions: a phenomenological treatment
• Bayesian vs Frequentist: Comparing Bayesian model selection with a frequentist approach using the iterative smoothing method
• Systematic Light Propagation Bias from the Heliosphere and Its Impact on the Hubble Tension
• Stringy multifield quintessence and the Swampland
• The influence of environmental effects on Type Ia Supernovae Standardization
• The Effects of the Gravitational Coupling Variation on the Local $H_0$ Estimation
• Constraining Dark Energy Perturbations: the Role of Early Dark Energy
• Kinematic reconstruction of torsion as dark energy in Friedmann cosmology
• Primordial gravitational waves: Model effects on time evolution and spectrum
• Sample Variance for Supernovae Distance Measurements and the Hubble tension
• Observational Constraints and Geometric Diagnostics of Barboza-Alcaniz and Logarithmic Dark Energy Parametrizations
• Joint Curvature and Growth Rate measurements with Supernova Peculiar Velocities and the CMB
• Genetic algorithm demystified for cosmological parameter estimation
• Dipole of the luminosity distance as a test for dark energy models
• Joint analysis of EDGES $21$-cm line observations with standard candles and rulers in $\Lambda$CDM and non-adiabatic gCg models
• Perturbations In Some Dark Energy Models
• The Influence of the Peculiar Velocities of SNe Ia in Clusters of Galaxies on the Redshift Measurements
• The $H_0$ and $S_8$ tensions necessitate early and late time changes to $\Lambda$CDM
• PISCOLA: a data-driven transient light-curve fitter
• Effective $\Lambda$CDM model emerging from $f(Q,T)$ under a special EOS limit in symmetric cosmology with Bayesian and ANN observational constraints
• A new magnitude--redshift relation based on Type Ia supernovae
• Freeze-in Dark Matter via Lepton Portal: Hubble Tension and Stellar Cooling
• Optimizing Gaussian Process Kernels Using Nested Sampling and ABC Rejection for H(z) Reconstruction
• Current constraints on the minimally extended varying speed of light model through the cosmic distance duality relation
• Late-Time Cosmic Acceleration from QCD Confinement Dynamics
• Correspondence between particle creation and dark components interaction in the context of $f(\mathcal{G})$ gravity
• Comparative Study of $f(T)$ Gravity Models with Observational Constraints from \textit{OHD} and \textit{Pantheon+ datasets}
• Confusing dark matter particle properties with modifications to General Relativity
• Halos of dark energy
• The BINGO project X. Cosmological parameter constraints from HI Intensity Mapping lognormal simulations
• The $f(Q)$ gravity and affine EoS: Compatibility and observational constraints
• An Agnostic Approach to Building Empirical Type Ia Supernova Light Curves: Evidence for Intrinsic Chromatic Flux Variation Using Nearby Supernova Factory Data
• Bayesian evidence and model selection approach for time-dependent dark energy
• Training Custom Light Curve Models of SN Ia Sub-Populations Selected According to Host Galaxy Properties
• Gamma-Ray Bursts, Supernovae Ia and Baryon Acoustic Oscillations: a binned cosmological analysis
• Improved cosmological constraints on the neutrino mass and lifetime
• Accelerated expansion as manifestation of gravity: when Dark Energy belongs to the left
• Measurement of telescope transmission using a Collimated Beam Projector
• Non-local Interactions are Essential Elements for Dark Matter Halo Stability: A Cross-Model Study
• A model-independent test of speed of light variability with cosmological observations
• Running vacuum model versus $\Lambda$CDM -- a Bayesian analysis
• Model-independent reconstruction of cosmic thermodynamics and dark energy dynamics
• Exploration of Parameters in f(R,T) Gravity and Comparison with Type Ia Supernovae Data