The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15

Abstract

We create a sample of spectroscopically identified galaxies with $z<0.2$ from the Sloan Digital Sky Survey (SDSS) Data Release 7, covering 6813 deg${}^2$. Galaxies are chosen to sample the highest mass haloes, with an effective bias of 1.5, allowing us to construct 1000 mock galaxy catalogs (described in Paper II), which we use to estimate statistical errors and test our methods. We use an estimate of the gravitational potential to "reconstruct" the linear density fluctuations, enhancing the Baryon Acoustic Oscillation (BAO) signal in the measured correlation function and power spectrum. Fitting to these measurements, we determine $D_V(z_{\mathrm{eff}}=0.15)=(664\pm 25)(r_d/r_{d,\mathrm{fid}})$ Mpc; this is a better than 4 per cent distance measurement. This "fills the gap" in BAO distance ladder between previously measured local and higher redshift measurements, and affords significant improvement in constraining the properties of dark energy. Combining our measurement with other BAO measurements from BOSS and 6dFGS galaxy samples provides a 15 per cent improvement in the determination of the equation of state of dark energy and the value of the Hubble parameter at $z=0$ ($H_0$). Our measurement is fully consistent with the Planck results and the $\Lambda$CDM concordance cosmology, but increases the tension between Planck$+$BAO $H_0$ determinations and direct $H_0$ measurements.

arXiv commentAccepted by MNRAS, distance likelihood is available in source files

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• Measuring the Hubble constant and spatial curvature from supernova apparent magnitude, baryon acoustic oscillation, and Hubble parameter data
• Cosmological Bound on the QCD Axion Mass, Redux
• Forecast for cosmological parameter estimation with gravitational-wave standard siren observation from the Cosmic Explorer
• Cosmological constraints from the power spectrum of eBOSS emission line galaxies
• Bounds on light sterile neutrino mass and mixing from cosmology and laboratory searches
• The trouble beyond $H_0$ and the new cosmic triangles
• CMB and BAO constraints for an induced gravity dark energy model with a quartic potential
• No-go guide for the Hubble tension : Late-time solutions
• The Hubble Tension as a Hint of Leptogenesis and Neutrino Mass Generation
• MGCAMB with massive neutrinos and dynamical dark energy
• Ups and Downs in Dark Energy: phase transition in dark sector as a proposal to lessen cosmological tensions
• Revisit of the interacting holographic dark energy model after Planck 2015
• The evidence of cosmic acceleration and observational constraints
• Symmetry of Cosmological Observables, and a High Hubble Constant as an Indicator of a Mirror World Dark Sector
• Cosmological discordances: a new measure, marginalization effects, and application to geometry vs growth current data sets
• Addressing $H_0$ tension by means of VCDM
• Constraints on non-flat cosmologies with massive neutrinos after Planck 2015
• Cosmological parameter estimation with future gravitational wave standard siren observation from the Einstein Telescope
• Impacts of dark energy on weighing neutrinos: mass hierarchies considered
• Soundness of Dark Energy properties
• Massive neutrinos and cosmic composition
• Cosmology from large scale galaxy clustering and galaxy-galaxy lensing with Dark Energy Survey Science Verification data
• Updated Constraints and Forecasts on Primordial Tensor Modes
• Late time transitions in the quintessence field and the $H_0$ tension
• Phenomenology of the generalized cubic covariant Galileon model and cosmological bounds
• $\Lambda$CDM or self-interacting neutrinos? - how CMB data can tell the two models apart
• Cosmological limits on neutrino unknowns versus low redshift priors
• Flavor-specific Interaction Favors Strong Neutrino Self-coupling in the Early Universe
• Can dark energy be expressed as a power series of the Hubble parameter?
• The Impact of the Fiducial Cosmology Assumption on BAO Cosmological Parameter Inference
• Late time interacting cosmologies and the Hubble constant tension
• Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies
• 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
• Testing Low-Redshift Cosmic Acceleration with Large-Scale Structure
• An Efficient and Accurate Hybrid Method for Simulating Non-Linear Neutrino Structure
• Cosmological constraints on late-universe decaying dark matter as a solution to the $H_0$ tension
• Revealing the effects of curvature on the cosmological models
• A Measurement of Gravitational Lensing of the Cosmic Microwave Background Using SPT-3G 2018 Data
• Cosmology and the neutrino mass ordering
• Constraints on the neutrino mass and mass hierarchy from cosmological observations
• Linear cosmological constraints on 2-body decaying dark matter scenarios and the $S_8$ tension
• $T_0$ censorship of early dark energy and AdS vacua
• Updating constraints on f(T) teleparallel cosmology and the consistency with Big Bang Nucleosynthesis
• Impacts of dark energy on weighing neutrinos after Planck 2015
• Long Range Interactions in Cosmology: Implications for Neutrinos
• Observational Constraints on Oscillating Dark-Energy Parametrizations
• 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
• The Early Dark Sector, the Hubble Tension, and the Swampland
• How predictions of cosmological models depend on Hubble parameter data sets
• Constraining Neutrino Mass with the Tomographic Weak Lensing Bispectrum
• Cosmological constraints on induced gravity dark energy models
• Testing H0 in Acoustic Dark Energy Models with Planck and ACT Polarization
• Coupled and uncoupled early dark energy, massive neutrinos and the cosmological tensions
• Neutrino masses and beyond-$\Lambda$CDM cosmology with LSST and future CMB experiments
• Generalized Emergent Dark Energy Model and the Hubble Constant Tension
• Prospects for improving cosmological parameter estimation with gravitational-wave standard sirens from Taiji
• Dark Neutrino interactions phase out the Hubble tension
• Cosmological Constraints from Gas Mass Fractions of Massive, Relaxed Galaxy Clusters
• Planck 2015 constraints on the non-flat $\varphi$CDM inflation model
• Rastall gravity extension of the standard $\Lambda$CDM model: theoretical features and observational constraints
• Improving cosmological parameter estimation with the future gravitational-wave standard siren observation from the Einstein Telescope
• SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field
• The Clustering of Galaxies in the Completed SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from DR12 galaxy clustering -- towards an accurate model
• H0LiCOW II. Spectroscopic survey and galaxy-group identification of the strong gravitational lens system HE0435-1223
• Weighing neutrinos in the scenario of vacuum energy interacting with cold dark matter: application of the parameterized post-Friedmann approach
• Gamma-Ray Bursts, Quasars, Baryonic Acoustic Oscillations, and Supernovae Ia: new statistical insights and cosmological constraints
• Prospects for Constraining Interacting Dark Energy Models with 21 cm Intensity Mapping Experiments
• Data-driven Reconstruction of the Late-time Cosmic Acceleration with f(T) Gravity
• The Price of Shifting the Hubble Constant
• An evaluation of cosmological models from expansion and growth of structure measurements
• Testing AdS early dark energy with Planck, SPTpol and LSS data
• Changing the prior: absolute neutrino mass constraints in nonlocal gravity
• Connecting early and late epochs by f(z)CDM cosmography
• Cosmological constraints on an exponential interaction in the dark sector
• Model independent calibrations of gamma ray bursts using machine learning
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR16 luminous red galaxy and emission line galaxy samples: cosmic distance and structure growth measurements using multiple tracers in configuration space
• Cosmological implications of scale-independent energy-momentum squared gravity: Pseudo nonminimal interactions in dark matter and relativistic relics
• Robust and model-independent cosmological constraints from distance measurements
• Unveiling dark fifth forces with linear cosmology
• A search for sterile neutrinos with the latest cosmological observations
• A Critique of Holographic Dark Energy
• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from multi-tracer BAO analysis with galaxies and voids
• Robust model comparison disfavors power law cosmology
• The $H_0$ and ${\sigma }_8$ tensions and the scale invariant spectrum
• Model-independent limits and constraints on extended theories of gravity from cosmic reconstruction techniques
• Partially Acoustic Dark Matter Cosmology and Cosmological Constraints
• Health checkup test of the standard cosmological model in view of recent Cosmic Microwave Background Anisotropies experiments
• CMB tensions with low-redshift $H_0$ and $S_8$ measurements: impact of a redshift-dependent type-Ia supernovae intrinsic luminosity
• Observational constraints on dark matter-dark energy scattering cross section
• Exploring neutrino mass and mass hierarchy in the scenario of vacuum energy interacting with cold dark matter
• Cosmological data favor Galileon ghost condensate over $\Lambda$CDM
• Primordial power spectra for curved inflating universes
• Cosmological constraints on slow-roll inflation: an update
• Probing elastic interactions in the dark sector and the role of $S_8$
• Novel null tests for the spatial curvature and homogeneity of the Universe and their machine learning reconstructions
• New cosmological bounds on hot relics: Axions $\&$ Neutrinos
• Planck 2015 constraints on the non-flat XCDM inflation model
• Positivity Bounds on Dark Energy: When Matter Matters
• A Step in Understanding the $S_8$ Tension
• Cosmological parameter estimation for dynamical dark energy models with future fast radio burst observations
• Novel cosmological bounds on thermally-produced axion-like particles
• The foreground wedge and 21 cm BAO surveys
• Constraints on interacting dark energy models from time-delay cosmography with seven lensed quasars
• Multidimensionality of the Hubble tension: the roles of ${\Omega }_m$ and ${\omega }_c$
• Fast and Credible Likelihood-Free Cosmology with Truncated Marginal Neural Ratio Estimation
• Warm Decaying Dark Matter and the Hubble Tension
• Effective field description of the Anton-Schmidt cosmic fluid
• Primordial gravitational waves and the H0-tension problem
• Gaussian processes reconstruction of modified gravitational wave propagation
• Cosmological constraints from higher-redshift gamma-ray burst, HII starburst galaxy, and quasar (and other) data
• Kinematic constraints beyond $z\simeq 0$ using calibrated GRB correlations
• Constraints on dark-matter properties from large-scale structure
• Cosmological bounds on dark matter-photon coupling
• Future Constraints on Dynamical Dark-Energy using Gravitational-Wave Standard Sirens
• Designing Horndeski and the effective fluid approach
• Cosmic microwave background constraints on secret interactions among sterile neutrinos
• Large-scale (in-) stability Analysis of an Exactly Solved Coupled Dark-Energy Model
• Emergent Dark Energy, neutrinos and cosmological tensions
• Reheating in quintessential inflation via gravitational production of heavy massive particles: A detailed analysis
• Combining pre- and post-recombination new physics to address cosmological tensions: case study with varying electron mass and sign-switching cosmological constant
• Is there a concordance value for $H_0$?
• Non-local gravity and comparison with observational datasets. II. Updated results and Bayesian model comparison with $\Lambda$CDM
• Higgs-Dilaton Cosmology: An inflation - dark energy connection and forecasts for future galaxy surveys
• Comparison between different methods of model selection in cosmology
• Constraints on active and sterile neutrinos in an interacting dark energy cosmology
• Mirror Twin Higgs Cosmology: Constraints and a Possible Resolution to the $H_0$ and $S_8$ Tensions
• Testing the equation of state for viscous dark energy
• Cosmological Constraint on ${\Omega }_m$ and ${\sigma }_8$ from Cluster Abundances using the $GalWCat19$ Optical-Spectroscopic SDSS Catalog
• Chain Early Dark Energy: Solving the Hubble Tension and Explaining Today's Dark Energy
• Planck 2015 constraints on spatially-flat dynamical dark energy models
• Testing Hu-Sawicki f(R) gravity with the Effective Field Theory approach
• Time-varying neutrino mass from a supercooled phase transition: current cosmological constraints and impact on the ${\Omega }_m$-${\sigma }_8$ plane
• Horava Gravity in the Effective Field Theory formalism: from cosmology to observational constraints
• Ultralight Scalar Decay and the Hubble Tension
• Testing the consistency between cosmological data: the impact of spatial curvature and the dark energy EoS
• Constraining dark matter properties with Cosmic Microwave Background observations
• Cosmological constraints on dark energy in light of gravitational wave bounds
• Testing the Mutual Consistency of the Pantheon and SDSS/eBOSS BAO Data Sets with Gaussian Processes
• Cosmological constraints of phantom dark energy models
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: a multi-tracer analysis in Fourier space for measuring the cosmic structure growth and expansion rate
• The Atacama Cosmology Telescope: Cosmology from cross-correlations of unWISE galaxies and ACT DR6 CMB lensing
• Testing Dark energy models in the light of ${\sigma }_8$ tension
• Dark Energy Survey Year 1 Results: Constraining Baryonic Physics in the Universe
• Screened fifth forces lower the TRGB-calibrated Hubble constant too
• Cosmological Constraints on First-Order Phase Transitions
• Forecast for FAST: from Galaxies Survey to Intensity Mapping
• Cosmological parameter forecasts for HI intensity mapping experiments using the angular power spectrum
• Latest astronomical constraints on some nonlinear parametric dark energy models
• A preliminary forecast for cosmological parameter estimation with gravitational-wave standard sirens from TianQin
• Cosmological constraints with self-interacting sterile neutrinos
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: application to the SDSS-III BOSS DR12 galaxies
• Modelling and testing the equation of state for (Early) dark energy
• Constraints on quintessence scalar field models using cosmological observations
• Assessment of the cosmic distance duality relation using Gaussian Process
• Modified gravity for surveys
• Some like it hot: $R^2$ heals Higgs inflation, but does not cool it
• Multi-interacting dark energy and its cosmological implications
• Constraining neutrino mass and extra relativistic degrees of freedom in dynamical dark energy models using Planck 2015 data in combination with low-redshift cosmological probes: basic extensions to $\Lambda$CDM cosmology
• Search for sterile neutrinos in a universe of vacuum energy interacting with cold dark matter
• The DFSZ axion in the CMB
• Gravity in the infrared and effective nonlocal models
• Return of Harrison-Zeldovich spectrum in light of recent cosmological tensions
• Testing interacting dark matter and dark energy model with cosmological data
• Efficient Computation of Galaxy Bias with Neutrinos and Other Relics
• A measurement of the Hubble constant using galaxy redshift surveys
• Probing Dark Matter with Future CMB Measurements
• Quantifying Tensions between CMB and Distance Datasets in Models with Free Curvature or Lensing Amplitude
• Dark Catalysis
• The full Boltzmann hierarchy for dark matter-massive neutrino interactions
• Self-interacting dark matter from late decays and the $H_0$ tension
• Distinguishing between Neutrinos and time-varying Dark Energy through Cosmic Time
• Consistency of Planck, ACT and SPT constraints on magnetically assisted recombination and forecasts for future experiments
• A Bayesian comparison between $\Lambda$CDM and phenomenologically emergent dark energy models
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: combining correlated Gaussian posterior distributions
• Running the running
• Constraints on Pre-Recombination Early Dark Energy from SPT-3G Public Data
• Reconstruction of the Dark Energy equation of state from latest data: the impact of theoretical priors
• Hints of dark matter-neutrino interactions in Lyman-$\alpha$ data
• One spectrum to cure them all: Signature from early Universe solves major anomalies and tensions in cosmology
• Unified Dark Energy and Dark Matter from Dynamical Space Time
• Hints of dark energy anisotropic stress using Machine Learning
• Neutron star merger GW170817 strongly constrains doubly coupled bigravity
• Dynamical Dark sectors and Neutrino masses and abundances
• Sterile neutrinos with pseudoscalar self-interactions and cosmology
• The Cosmic Expansion History from Line-Intensity Mapping
• How to relax the cosmological neutrino mass bound
• Dark matter component decaying after recombination: Sensitivity to BAO and RSD probes
• Strengthening the bound on the mass of the lightest neutrino with terrestrial and cosmological experiments
• Cold dark matter plus not-so-clumpy dark relics
• Generalized tracker quintessence models for dark energy
• Bayesian Evidences for Dark Energy models in light of current obsevational data
• Updated observational constraints on quintessence dark energy models
• Inflation model constraints from data released in 2015
• Gravitational-Wave Detector Networks: Standard Sirens on Cosmology and Modified Gravity Theory
• Testing Gravity on Cosmic Scales: A Case Study of Jordan-Brans-Dicke Theory
• Metastable dark energy models in light of Planck 2018: Alleviating the $H_0$ tension
• Dark Energy Survey: A 2.1% measurement of the angular Baryonic Acoustic Oscillation scale at redshift $z_{\mathrm{eff}}$=0.85 from the final dataset
• Prospect for constraining holographic dark energy with gravitational wave standard sirens from the Einstein Telescope
• Using dark energy to suppress power at small scales
• Cannibalism hinders growth: Cannibal Dark Matter and the $S_8$ tension
• Nonlocal Teleparallel Cosmology
• On the dynamics of a dark sector coupling
• Natural Inflation After Planck 2018
• Impacts of gravitational-wave standard siren observations from Einstein Telescope and Cosmic Explorer on weighing neutrinos in interacting dark energy models
• Constraints on the Parameterized Deceleration Parameter in FLRW Universe
• Model-independent cosmic acceleration and type Ia supernovae intrinsic luminosity redshift dependence
• Reconstruction of the neutrino mass as a function of redshift
• Cosmological inference from the EFTofLSS: the eBOSS QSO full-shape analysis
• Massive neutrino self-interactions and inflation
• Early Dark Energy with Power-law F(R) Gravity
• Measuring growth index in a universe with massive neutrinos: A revisit of the general relativity test with the latest observations
• Cosmology beyond BAO from the 3D distribution of the Lyman-$\alpha$ forest
• Constraints on the sum of neutrino masses using cosmological data including the latest extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample
• Observational constraints on cosmological models with Chaplygin gas and quadratic equation of state
• Forecasting the Interaction in Dark Matter-Dark Energy Models with Standard Sirens From the Einstein Telescope
• Exploring neutrino mass and mass hierarchy in interacting dark energy models
• Searching for sterile neutrinos in dynamical dark energy cosmologies
• Reconciling Hubble Constant Discrepancy from Holographic Dark Energy
• Quantifying the global "CMB tension" between the Atacama Cosmology Telescope and the Planck satellite in extended models of cosmology
• Revisiting a non-parametric reconstruction of the deceleration parameter from combined background and the growth rate data
• Cosmology with varying fundamental constants from hyperlight, coupled scalars
• Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy
• Principal reconstructed modes of dark energy and gravity
• Constraints on dark matter to dark radiation conversion in the late universe with DES-Y1 and external data
• Axi-Higgs Cosmology
• Prospects for probing the interaction between dark energy and dark matter using gravitational-wave dark sirens with neutron star tidal deformation
• Probing the sign-changeable interaction between dark energy and dark matter with current observations
• The Redshift-Space Momentum Power Spectrum I: Optimal Estimation From Peculiar Velocity Surveys
• Limits on the cosmic neutrino background
• Power law cosmology model comparison with CMB scale information
• Cosmological constraints on the gravitational constant
• Lensing-like tensions in the Planck legacy release
• Revisiting CMB constraints on dark matter annihilation
• What can CMB observations tell us about the neutrino distribution function?
• Revisiting Metastable Dark Energy and Tensions in the Estimation of Cosmological Parameters
• Full-shape BOSS constraints on dark matter interacting with dark radiation and lifting the $S_8$ tension
• Testing logarithmic corrections on $R^2$-exponential gravity by observational data
• Forecasting Interacting Vacuum-Energy Models using Gravitational Waves
• Investigating the Hubble Constant Tension -- Two Numbers in the Standard Cosmological Model
• Free-streaming and Coupled Dark Radiation Isocurvature Perturbations: Constraints and Application to the Hubble Tension
• Touch of Neutrinos on the Vacuum Metamorphosis: is the $H_0$ Solution Back?
• Cosmology with fast radio bursts in the era of SKA
• Minimal dark energy: key to sterile neutrino and Hubble constant tensions?
• New method for initial density reconstruction
• A measurement of the CMB E-mode angular power spectrum at subdegree scales from 670 square degrees of POLARBEAR data
• Probing the properties of relic neutrinos using the cosmic microwave background, the Hubble Space Telescope and galaxy clusters
• The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset
• Information Content of Higher-Order Galaxy Correlation Functions
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: Measuring the anisotropic Baryon Acoustic Oscillations with redshift weights
• Testing Einstein's gravity and dark energy with growth of matter perturbations: Indications for new Physics?
• The Hubble Tension, The $M$ Crisis of Late Time $H(z)$ Deformation Models and the Reconstruction of Quintessence Lagrangians
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• Reducing the $H_0$ tension with generalized Proca theory
• Can small-scale baryon inhomogeneities resolve the Hubble tension? An investigation with ACT DR4
• The XXL survey: XLVI. Forward cosmological analysis of the C1 cluster sample
• Towards a self-consistent analysis of the anisotropic galaxy two- and three-point correlation functions on large scales: application to mock galaxy catalogues
• Asymmetric Dark Matter Models in SO(10)
• $H_0$ Tension and the Phantom Regime: A Case Study In Terms of an Infrared $f(T)$ Gravity
• Estimating the galaxy two-point correlation function using a split random catalog
• Theoretical and observational bounds on some interacting vacuum energy scenarios
• Dark Energy Survey Year 1 Results: Galaxy Sample for BAO Measurement
• Distance Priors from \emph{Planck} 2015 data
• CosmicNet II: Emulating extended cosmologies with efficient and accurate neural networks
• Stepped Partially Acoustic Dark Matter, Large Scale Structure, and the Hubble Tension
• Brane with variable tension as a possible solution to the problem of the late cosmic acceleration
• Measuring the distance-redshift relation with the baryon acoustic oscillations of galaxy clusters
• CMB Constraint on Dark Matter Annihilation after Planck 2015
• Dark Energy Survey Year 1 Results: Measurement of the Galaxy Angular Power Spectrum
• Impact of $H_0$ priors on $f(T)$ late time cosmology
• Imprints of an extended Chevallier-Polarski-Linder parametrization on the large scale of our universe
• Cosmology With Low-Redshift Observations: No Signal For New Physics
• Minimally Modified Gravity fitting Planck data better than $\Lambda$CDM
• Confronting interacting dark radiation scenarios with cosmological data
• A new coupled three-form dark energy model and implications for the $H_0$ tension
• Measuring the sound horizon and absolute magnitude of SNIa by maximizing the consistency between low-redshift data sets
• Testing dark energy after pre-recombination early dark energy
• Cross-correlation of weak lensing and gamma rays: implications for the nature of dark matter
• 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
• Constraining the spatial curvature with cosmic expansion history in a cosmological model with a non-standard sound horizon
• Smoothing the $H_0$ tension with a dynamical dark energy model
• A Zeldovich reconstruction method for measuring redshift space distortions using cosmic voids
• No H_0 Assistance from Assisted Quintessence
• No-go guide for late-time solutions to the Hubble tension: Matter perturbations
• Toward a concordance teleparallel Cosmology I: Background Dynamics
• Modified gravity and massive neutrinos: constraints from the full shape analysis of BOSS galaxies and forecasts for Stage IV surveys
• BAO from angular clustering: optimization and mitigation of theoretical systematics
• A Dark Matter Trigger for Early Dark Energy Coincidence
• Testing Predictions of the Quantum Landscape Multiverse 2: The Exponential Inflationary Potential
• Do you smell something decaying? Updated linear constraints on decaying dark matter scenarios
• Bayesian Comparison of Interacting Scenarios
• Fractional Dark Matter decay: cosmological imprints and observational constraints
• Microphysics of Early Dark Energy
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: Dynamical dark energy
• Constraining An Exact Brans-Dicke gravity theory with Recent Observations
• Conservative cosmology: combining data with allowance for unknown systematics
• Impacts of dark energy on weighing neutrinos after DESI BAO
• Cosmological Constraints on sub-horizon scales modified gravity theories with MGCLASS II
• Theoretical Accuracy in Cosmological Growth Estimation
• MOG cosmology without dark matter and the cosmological constant
• Hubble tension in lepton asymmetric cosmology with an extra radiation
• Neutrinos secretly converting to lighter particles to please both KATRIN and the cosmos
• Fitting string inflation to real cosmological data: the Fibre Inflation case
• Observational Constraints on Axion(s) Dark Energy with a Cosmological Constant
• $H_0$ Ex Machina: Vacuum Metamorphosis and Beyond $H_0$
• CosmoBit: A GAMBIT module for computing cosmological observables and likelihoods
• A void in the Hubble tension? The end of the line for the Hubble bubble
• Galaxy 2-Point Covariance Matrix Estimation for Next Generation Surveys
• Constraints on $f(T)$ Cosmology with Pantheon+
• $5\sigma$ tension between Planck cosmic microwave background and eBOSS Lyman-alpha forest and constraints on physics beyond $\Lambda$CDM
• Wandering in the Lyman-alpha Forest: A Study of Dark Matter-Dark Radiation Interactions
• The Copernican principle in light of the latest cosmological data
• Searching for scalar gravitational interactions in current and future cosmological data
• Observational constraints and predictions of the interacting dark sector with field-fluid mapping
• ICE-COLA: fast simulations for weak lensing observables
• Testing Predictions of the Quantum Landscape Multiverse 1: The Starobinsky Inflationary Potential
• Cosmological Constraints on Higgs-Dilaton Inflation
• On cosmological signatures of baryons-dark energy elastic couplings
• Precision CMB constraints on eV-scale bosons coupled to neutrinos
• Extracting cosmological information from the angular power spectrum of the 2MASS Photometric Redshift catalogue
• Constraining the dark matter-vacuum energy interaction using the EDGES 21-cm absorption signal
• An exploration of an early gravity transition in light of cosmological tensions
• Dark Radiation and Inflationary Freedom after Planck 2015
• Halo nonlinear reconstruction
• A grounded perspective on New Early Dark Energy using ACT, SPT, and BICEP/Keck
• Multiple transitions in vacuum dark energy and $H_0$ tension
• Models of vacuum energy interacting with cold dark matter: Constraints and comparison
• Information Gains from Cosmological Probes
• KiDS-Legacy: Consistency of cosmic shear measurements and joint cosmological constraints with external probes
• Dark Energy as a Critical Phenomenon: a Resolution for Hubble Tension
• Constraining spatial curvature with large-scale structure
• Exploring interacting holographic dark energy in a perturbed universe with parameterized post-Friedmann approach
• The extended Baryon Oscillation Spectroscopic Survey: measuring the cross-correlation between the MgII flux transmission field and quasars and galaxies at $z=0.59$
• Cosmological constraints to dark matter with two- and many-body decays
• Constraining the Expansion History and Early Dark Energy with Line Intensity Mapping
• sCOLA: The N-body COLA Method Extended to the Spatial Domain
• Baryon acoustic oscillations reconstruction using convolutional neural networks
• The $H_0$ Tension in Non-flat QCDM Cosmology
• Profiling Cold New Early Dark Energy
• Probing Early Modification of Gravity with Planck, ACT and SPT
• Constraining the $\Lambda$CDM and Galileon models with recent cosmological data
• J-PAS: Forecasts for dark matter - dark energy elastic couplings
• The QCD phase transition behind a PBH origin of LIGO/Virgo events?
• 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 ($w(z)\ge -1$)
• Narrowing down the possible explanations of cosmic acceleration with geometric probes
• Observational constraints on bimetric gravity
• Scale-invariant alternatives to general relativity. III. The inflation--dark-energy connection
• Dark energy and Dark matter interaction in light of the second law of thermodynamics
• The weak, the strong and the ugly -- A comparative analysis of interacting stepped dark radiation
• New MGCAMB tests of gravity with CosmoMC and Cobaya
• Evaporating primordial black holes as varying dark energy
• Prospects for constraining interacting dark energy models from gravitational wave and gamma ray burst joint observation
• Can varying the gravitational constant alleviate the tensions ?
• $f(Q)$-gravity and neutrino physics
• Constraints on massive vector dark energy models from integrated Sachs-Wolfe-galaxy cross-correlations
• Galaxy Bias and ${\sigma }_8$ from Counts in Cells from the SDSS Main Sample
• Limits on Clustering and Smooth Quintessence from the EFTofLSS
• Thermal Friction as a Solution to the Hubble and Large-Scale Structure Tensions
• Parameter splitting in dark energy: is dark energy the same in the background and in the cosmic structures?
• Data Analysis of three parameter models of deceleration parameter in FRW Universe
• $\alpha$ attractors in Quintessential Inflation motivated by Supergravity
• Dark energy and matter interacting scenario to relieve $H_0$ and $S_8$ tensions
• First study of reionization in the Planck 2015 normalized closed $\Lambda$CDM inflation model
• Perturbation Theory for BAO reconstructed fields: one-loop results in real-space matter density field
• Phantom scalar-tensor models and cosmological tensions
• Cosmological parameter estimation with Genetic Algorithms
• Optimal Reconstruction of Baryon Acoustic Oscillations for DESI 2024
• Including massive neutrinos in thermal Sunyaev Zeldovich power spectrum and cluster counts analyses
• Constraints on inflation revisited: An analysis including the latest local measurement of the Hubble constant
• Complementing the ground-based CMB Stage-4 experiment on large scales with the PIXIE satellite
• A forecast of using fast radio burst observations to constrain holographic dark energy
• A Cosmological Underdensity Does Not Solve the Hubble Tension
• Implications of an extended dark energy model with massive neutrinos
• Massive neutrino self-interactions with a light mediator in cosmology
• Cosmology-marginalized approaches in Bayesian model comparison: the neutrino mass as a case study
• Non-parametric dark energy reconstruction using the tomographic Alcock-Paczynski test
• Observational effects of a running Planck mass
• Constraining power of cosmological observables: blind redshift spots and optimal ranges
• Low-redshift estimates of the absolute scale of baryon acoustic oscillations
• Scaling Transformations and the Origins of Light Relics Constraints from Cosmic Microwave Background Observations
• IWDM: The fate of an interacting non-cold dark matter $-$ vacuum scenario
• Reaffirming the Cosmic Acceleration without Supernova and CMB
• Isotropic vs. Anisotropic components of BAO data: a tool for model selection
• Type Ia supernova Hubble diagram with near-infrared and optical observations
• Tracing the cosmic history by Gauss-Bonnet gravity
• Cosmological constraints on early dark energy from the full shape analysis of eBOSS DR16
• Constraining the dark energy statefinder hierarchy in a kinematic approach
• Constraints on decaying dark matter from weak lensing and cluster counts
• Super-CMB fluctuations and the Hubble tension
• Impact of the Hubble tension on the $r$-$n_s$ contour
• Probing the interaction between dark energy and dark matter with future fast radio burst observations
• A cosmographic analysis of the transition to acceleration using SN-Ia and BAO
• Improving sampling and calibration of GRBs as distance indicators
• Improved constraint on primordial gravitational waves in light of the Hubble tension and BICEP/Keck
• Nonlinear reconstruction of redshift space distortions
• Positivity bounds from multiple vacua and their cosmological consequences
• Observational Constraints on Dynamical Dark Energy Models
• Global view of neutrino interactions in cosmology: The freestreaming window as seen by Planck
• Observational constraints on conformal time symmetry, missing matter and double dark energy
• Hill crossing during preheating after hilltop inflation
• Cosmological Constraints on Non-flat Exponential $f(R)$ Gravity
• Constraining extended teleparallel gravity via cosmography: A model-independent approach
• Newest measurements of Hubble constant from DESI 2024 BAO observations
• Profile Likelihoods in Cosmology: When, Why and How illustrated with $\Lambda$CDM, Massive Neutrinos and Dark Energy
• Constraints on primordial lepton asymmetries with full neutrino transport
• Unveiling dark forces with measurements of the Large Scale Structure of the Universe
• A comprehensive forecast for cosmological parameter estimation using joint observations of gravitational waves and short $\gamma$-ray bursts
• Investigating the accelerated expansion of the Universe through updated constraints on viable $f(R)$ models within the metric formalism
• Prospects for measuring dark energy with 21 cm intensity mapping experiments: A joint survey strategy
• The Integrated Sachs Wolfe effect: unWISE and Planck constraints on Dynamical Dark Energy
• Comparing the scalar-field dark energy models with recent observations
• Toward a concordance teleparallel Cosmology II: Linear perturbation
• Quintessential inflation and cosmological seesaw Mechanism: reheating and observational constraints
• Cosmological constraints on non-adiabatic dark energy perturbations
• Impacts of dark energy on constraining neutrino mass after Planck 2018
• Hubble constant difference between CMB lensing and BAO measurements
• The Hubble-Lemaître constant and sound horizon from low-redshift probes
• Concordance Cosmology?
• Forecast for weighing neutrinos in cosmology with SKA
• Testing the warmness of dark matter
• Constraining light sterile neutrino mass with the BICEP2/Keck Array 2014 B-mode polarization data
• Cosmic constraint on massive neutrinos in viable f(R) gravity with producing LCDM background expansion
• Isolating the Lyman Alpha Forest BAO Anomaly
• Bayesian comparison of nonstandard cosmologies using type Ia supernovae and BAO data
• Phenomenological Reconstruction of $f(T)$ Teleparallel 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
• Linear bias and halo occupation distribution of emission line galaxies from Nancy Grace Roman Space Telescope
• Constraining Bianchi type V universe with recent H(z) and BAO observations in Brans-Dicke theory of gravitation
• 4D Gauss-Bonnet gravity: cosmological constraints, $H_0$ tension and large scale structure
• Probing a Steep EoS for Dark Energy with latest observations
• Model-independent study for a quintessence model of dark energy: Analysis and Observational constraints
• Current constraints on deviations from General Relativity using binning in redshift and scale
• Primordial magnetic field as a common solution of nanohertz gravitational waves and the Hubble tension
• First cosmological constraints combining Planck with the recent gravitational-wave standard siren measurement of the Hubble constant
• New cosmological constraints with extended-Baryon Oscillation Spectroscopic Survey DR14 quasar sample
• Cosmological Tests of Everpresent $\Lambda$
• The phenomenology of beyond Horndeski gravity
• A thorough investigation of the prospects of eLISA in addressing the Hubble tension: Fisher Forecast, MCMC and Machine Learning
• Testing f(R) gravity models with quasar X-ray and UV fluxes
• Cosmological constraints on the Multi Scalar Field Dark Matter model
• Revisiting the impact of neutrino mass hierarchies on neutrino mass constraints in light of recent DESI data
• Parametric resonance after hilltop inflation caused by an inhomogeneous inflaton field
• Hubble constant and sound horizon from the late-time Universe
• Strong constraints on a simple self-interacting neutrino cosmology
• Testing for New Physics: Neutrinos and the Primordial Power Spectrum
• The Clustering of Galaxies in the Completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmic Flows and Cosmic Web from Luminous Red Galaxies
• Do cosmological data rule out $f(\mathcal{R})$ with $w\ne -1$?
• Cosmological constraints from the cross-correlation of DESI Luminous Red Galaxies with CMB lensing from Planck PR4 and ACT DR6
• Constraints on $f(Q)$ logarithmic model using gravitational wave standard sirens
• Prospects for measuring dark energy with 21 cm intensity mapping experiments
• Constraining holographic cosmology using Planck data
• K-mouflage Imprints on Cosmological Observables and Data Constraints
• Alleviating Cosmological Tensions with a Coupled Scalar Fields Model
• Observational constraints on $\alpha$-attractor inflationary models with a Higgs-like potential
• Constraining f(R) Gravity with Planck Sunyaev-Zel'dovich Clusters
• Non-Canonical Volume-Form Formulation of Modified Gravity Theories and Cosmology
• Dark matter solution to the $H_0$ and $S_8$ tensions, and the integrated Sachs-Wolfe void anomaly
• Barry and the BAO Model Comparison
• Constraints on neutrino mass in the scenario of vacuum energy interacting with cold dark matter after Planck 2018
• Reexploration of interacting holographic dark energy model: Cases of interaction term excluding the Hubble parameter
• Nested sampling with any prior you like
• The role of CMB spectral distortions in the Hubble tension: a proof of principle
• Cosmological Constraints from Galaxy Cluster Sparsity, Cluster Gas Mass Fraction and Baryon Acoustic Oscillations Data
• Constraining Sterile Neutrino Cosmology with Terrestrial Oscillation Experiments
• Probing Modified Gravity with Integrated Sachs-Wolfe CMB and Galaxy Cross-correlations
• Constraints on Newton's Constant from Cosmological Observations
• Cascading Dark Energy
• Testing cosmic acceleration for $w(z)$ parameterizations using $f_{gas}$ measurements in galaxy clusters
• Cosmological constraints and phenomenology of a beyond-Horndeski model
• Constraints on Steep Equation of State for the Dark Energy using BAO
• Probing dynamics of dark energy with latest observations
• Theoretical priors in scalar-tensor cosmologies: Thawing quintessence
• Extended $\Lambda$CDM model
• Update constraints on neutrino mass and mass hierarchy in light of dark energy models
• Time-dependent $G$ in Einstein's equations as an alternative to the cosmological constant
• The Linear Point Standard Ruler for galaxy survey data: validation with mock catalogues
• Spatial Curvature in $f(R)$ Gravity
• Constraining the interaction between dark sectors with future HI intensity mapping observations
• Probing the primordial universe with gravitational waves detectors
• Vacuum Energy Density Measured from Cosmological Data
• Cosmological discordances III: more on measure properties, Large-Scale-Structure constraints, the Hubble constant and Planck
• Cosmological search for sterile neutrinos after Planck 2018
• Planck-PR4 anisotropy spectra show (better) consistency with General Relativity
• Analytical approximations for curved primordial power spectra
• Reconciling $S_8$: Insights from Interacting Dark Sectors
• Constraining cosmology with the cosmic microwave and infrared backgrounds correlation
• C${}^3$-Cluster Clustering Cosmology II. First detection of the BAO peak in the three-point correlation function of galaxy clusters
• Testing extended Jordan-Brans-Dicke theories with future cosmological observations
• Post-inflationary axion isocurvature perturbations facing CMB and large-scale structure
• Decay of multiple dark matter particles to dark radiation in different epochs does not alleviate the Hubble tension
• A note on the relations between thermodynamics, energy definitions and Friedmann equations
• Big Bang Nucleosynthesis constraints on varying electron mass solution to the Hubble tension
• Dark Sectors with Mass Thresholds Face Cosmological Datasets
• IDECAMB: an implementation of interacting dark energy cosmology in CAMB
• Unified and consistent structure growth measurements from joint ACT, SPT and \textit{Planck} CMB lensing
• Ultra-compact structure in radio quasars as a cosmological probe: a revised study of the interaction between cosmic dark sectors
• Dynamical Dark Matter from Thermal Freeze-Out
• Cosmological measurements from void-galaxy and galaxy-galaxy clustering in the Sloan Digital Sky Survey
• A New Test of Dynamical Dark Energy Models and Cosmic Tensions in Hořava Gravity
• Combining cosmological and local bounds on bimetric theory
• New Early Dark Energy as a solution to the $H_0$ and $S_8$ tensions
• Perturbation theory for the redshift-space matter power spectra after reconstruction
• The Alcock-Paczyński effect from Lyman-$\alpha$ forest correlations: Analysis validation with synthetic data
• Primordial power spectrum and cosmology from black-box galaxy surveys
• Constraints on decaying early modified gravity from cosmological observations
• Pseudoscalar sterile neutrino self-interactions in light of Planck, SPT and ACT data
• Testing the local void hypothesis using baryon acoustic oscillation measurements over the last twenty years
• The BAHAMAS project: Effects of dynamical dark energy on large-scale structure
• Resonant neutrino self-interactions and the $H_0$ tension
• Testing the $n_s-H_0$ scaling relation with Planck-independent CMB data
• Thermal axions with multi-eV masses are possible in low-reheating scenarios
• Cosmology from weak lensing alone and implications for the Hubble tension
• Extended $\Lambda$CDM model and viscous dark energy: A Bayesian analysis
• A critical discussion on the $H_0$ tension
• Redshift remapping and cosmic acceleration in dark-matter-dominated cosmological models
• Probing $\Lambda$CDM cosmology with the Evolutionary Map of the Universe survey
• Sweeping Horndeski Canvas: New Growth-Rate Parameterization for Modified-Gravity Theories
• Unitarity at the Late time Boundary of de Sitter
• Probing the Neutrino Mass Hierarchy beyond $\Lambda$CDM Model
• Phenomenological Gravitational Phase Transition: Early and Late Modifications
• Cosmology-informed neural networks to solve the background dynamics of the Universe
• Model-independent cosmological inference after the DESI DR2 data with improved inverse distance ladder
• A brief review on cosmological analysis of galaxy surveys with multiple tracers
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: Anisotropic Baryon Acoustic Oscillations measurements in Fourier-space with optimal redshift weights
• Current constraints on cosmological scenarios with very low reheating temperatures
• Scalar-Tensor Gravity and DESI 2024 BAO data
• Phenomenological Gravitational Phase Transition: Reconciliation between the Late and Early Universe
• Modeling the large-scale power deficit with smooth and discontinuous primordial spectra
• A novel CMB polarization likelihood package for large angular scales built from combined WMAP and Planck LFI legacy maps
• Dark Energy Survey Year 3 Results: Measurement of the Baryon Acoustic Oscillations with Three-dimensional Clustering
• Dark energy versus modified gravity: Impacts on measuring neutrino mass
• Reconstructing Quintessence
• An exponential equation of state of dark energy in the light of 2018 CMB Planck data
• Observable Predictions for Massive-Neutrino Cosmologies with Model-Independent Dark Energy
• Observational constraints on the interacting dark energy - dark matter (IDM) cosmological models
• Improving cosmological parameter estimation with the future 21 cm observation from SKA
• Latest data constraint of some parameterized dark energy models
• Towards alleviating the $H_0$ and $S_8$ tensions with Early Dark Energy - Dark Matter drag
• Parameter estimation of eccentric gravitational waves with a decihertz observatory and its cosmological implications
• Updating constraints on phantom crossing $f(T)$ gravity
• Differentiating dark interactions with perturbation
• The Swampland Conjectures and Slow-Roll Thawing Quintessence
• Covariance of the redshift-space matter power spectrum after reconstruction
• Probing the Seesaw Mechanism with Cosmological Data
• Forbidden Scalar Dark Matter and Dark Higgses
• Roles of Modified Chaplygin-Jacobi and Chaplygin-Abel Gases in FRW Universe
• Observational constraints on soft dark energy and soft dark matter: challenging $\Lambda$CDM
• Dark Energy Constraints in light of Pantheon SNe Ia, BAO, Cosmic Chronometers and CMB Polarization and Lensing Data
• Tight $H_0$ constraint from galaxy redshfit surveys: combining baryon acoustic osillation measurements and Alcock-Paczynski test
• Hubble tension as a window on the gravitation of the dark matter sector
• A cosmic glitch in gravity
• Electron mass variation from dark sector interactions and compatibility with cosmological observations
• Redshift Space Distortion of 21cm line at 1<z<5 with Cosmological Hydrodynamic Simulations
• Diagnostic and Comparative Analysis of Dark Energy Models with $q(z)$ Parametrizations
• A novel model-marginalized cosmological bound on the QCD axion mass
• Cosmological bound on neutrino masses in the light of $H_0$ tension
• Testing averaged cosmology with type Ia supernovae and BAO data
• Cosmic Growth in $f(T)$ Teleparallel Gravity
• Constraining quantum collapse inflationary models with current data: The semiclassical approach
• Forecast constraints on Anisotropic Stress in Dark Energy using gravitational-waves
• Clustering with general photo-$z$ uncertainties: Application to Baryon Acoustic Oscillations
• Radiative stability and observational constraints on dark energy and modified gravity
• Baryon Physics and Tight Coupling Approximation in Boltzmann Codes
• Exploring Mirror Twin Higgs Cosmology with Present and Future Weak Lensing Surveys
• Forecasts on interacting dark energy with standard sirens
• A Test of the Standard Cosmological Model with Geometry and Growth
• Analytic Solutions and Observational support: A study of $f(R,T)$ gravity with $f(R,T)=R+h(T)$
• Testing distance duality with CMB anisotropies
• Cosmological constraint on Brans-Dicke Model
• Volume Statistics as a Probe of Large-Scale Structure
• Tachyon inflation in the Large-$N$ formalism
• Growth of structures using redshift space distortion in $f(T)$ Cosmology
• The QCD Axion: Some Like It Hot
• A comparison between axion-like and power law potentials in cosmological background
• Type Ia supernovae data with scalar-tensor gravity
• Phase Space description of Nonlocal Teleparallel Gravity
• A preference for dynamical phantom dark energy using one-parameter model with Planck, DESI DR1 BAO and SN data
• Hints of Neutrino Dark Matter scattering in the CMB? Constraints from the Marginalized and Profile Distributions
• Constraints from High-Precision Measurements of the Cosmic Microwave Background: The Case of Disintegrating Dark Matter with $\Lambda$ or Dynamical Dark Energy
• From 100 kpc to 10 Gpc: Dark Matter self-interactions before and after DESI
• Cluster counts III. $\Lambda$CDM extensions and the cluster tension
• Modified Gravity Away from a $\Lambda$CDM Background
• Theoretical and observational constraints on Tachyon Inflation
• Eliminating polarization leakage effect for neutral hydrogen intensity mapping with deep learning
• Asymmetric dark matter with a spontaneously broken $U(1{)}^{\prime }$: self-interaction and gravitational waves
• Pantheon+ constraints on dark energy and modified gravity: An evidence of dynamical dark energy
• Forecasting the Cross-Correlation of the CSST galaxy survey with the FAST HI Intensity Map
• Momentum transfer in the dark sector and lensing convergence in upcoming galaxy surveys
• Primordial power spectrum features in phenomenological descriptions of inflation
• Building a digital twin of a luminous red galaxy spectroscopic survey: galaxy properties and clustering covariance
• Recovering $\Lambda$CDM Model From a Cosmographic Study
• Investigating dark energy by electromagnetic frequency shifts
• Brane inflation and the robustness of the Starobinsky inflationary model
• A low Hubble Constant from galaxy distribution observations
• Biased tracer reconstruction with halo mass information
• Reducing the $H_0$ Tension with Exponential Acoustic Dark Energy
• A single parameterization for dark energy and modified gravity models
• Discrepancy between cosmological and electroweak observables in Higgs Inflation
• Cosmology of an Axion-Like Majoron
• The impact and mitigation of broad absorption line quasars in Lyman$-\alpha$ forest correlations
• Generalized Brans-Dicke theories in light of evolving dark energy
• A model independent parametrization of the late time cosmic acceleration: constraints on the parameters from recent observations
• Kinetically Coupled Scalar Fields Model and Cosmological Tensions
• Constraints on interacting dark energy revisited: implications for the Hubble tension
• Testing f(R)-gravity models with DESI DR2 2025-BAO and other cosmological data
• Probing cosmic acceleration by strong gravitational lensing systems
• The redshift dependence of Alcock-Paczynski effect: cosmological constraints from the current and next generation observations
• Multipole expansion for 21cm Intensity Mapping power spectrum: forecasted cosmological parameters estimation for the SKA Observatory
• Observational status of the Galileon model general solution from cosmological data and gravitational waves
• Revisiting signatures of thermal axions in nonstandard cosmologies
• Probing a panoply of curvaton-decay scenarios using CMB data
• Clustering in the Simulated H$\alpha$ Galaxy Redshift Survey from Nancy Grace Roman Space Telescope
• Measuring the spectral running from cosmic microwave background and primordial black holes
• Non-thermal neutrino-like hot dark matter in light of the $S_8$ tension
• Reconstructing a non-linear interaction in the dark sector with cosmological observations
• Does the fraction of dark matter diminish with early dark energy?
• Holographic energy density, dark energy sound speed, and tensions in cosmological parameters: $H_0$ and $S_8$
• No evidence for the evolution of mass density power-law index $\gamma$ from strong gravitational lensing observation
• Dynamics and statefinder analysis of a class of sign-changeable interacting dark energy scenarios
• Cosmological constraints of Palatini $f(\mathcal{R})$ gravity
• ISiTGR: Testing deviations from GR at cosmological scales including dynamical dark energy, massive neutrinos, functional or binned parametrizations, and spatial curvature
• The cosmic transparency measured with Type Ia supernovae: implications for intergalactic dust
• $f(T)$ cosmology in the regime of quasar observations
• Constraining power of open likelihoods, made prior-independent
• Space-borne atom interferometric gravitational wave detections. Part I. The forecast of bright sirens on cosmology
• Finding structure in the dark: coupled dark energy, weak lensing, and the mildly nonlinear regime
• Early dark energy constraints with late-time expansion marginalization
• A More Accurate Parameterization based on cosmic Age (MAPAge)
• Harmonic Hybrid Inflation
• A visual tool for assessing tension-resolving models in the $H_0$-${\sigma }_8$ plane
• First constraints on non-minimally coupled Natural and Coleman-Weinberg inflation and massive neutrino self-interactions with Planck+BICEP/Keck
• Spatial curvature sensitivity to local $H_0$ from the Cepheid distance ladder
• Reconstructing the Hubble parameter with future Gravitational Wave missions using Machine Learning
• Imprint of a Steep Equation of State in the growth of structure
• Quantifying effects of inhomogeneities and curvature on gravitational wave standard siren measurements of $H(z)$
• Joint Constraints on the Hubble Constant, Spatial Curvature, and Sound Horizon from the Late-time Universe with Cosmography
• Constraints on brane inflation after Planck 2015: Impacts of the latest local measurement of the Hubble constant
• Probing alternative cosmologies through the inverse distance ladder
• $f(T,B)$ Gravity in the late Universe in the context of local measurements
• Constraining the emergent dark energy models with observational data at intermediate redshift
• Cosmological Parameter Estimation from the Two-Dimensional Genus Topology -- Measuring the Expansion History using the Genus Amplitude as a Standard Ruler
• Dark Energy Survey: Galaxy Sample for the Baryonic Acoustic Oscillation Measurement from the Final Dataset
• Testing the nature of Dark Energy with Precision Cosmological constraints
• The interaction of neutrinos with Phantom, Quintessence, and Quintum scalar fields and its effect on the formation of structures in the early Universe
• Evidence of dark energy in different cosmological observations
• Explanation of high redshift luminous galaxies from JWST by early dark energy model
• A PAge-like Unified Dark Fluid Model
• Abundance and properties of dark radiation from the cosmic microwave background
• Shan--Chen interacting vacuum cosmology
• Constraints on small-scale primordial density fluctuation from cosmic microwave background through dark matter annihilation
• Investigating dark energy by electromagnetic frequency shifts II: the Pantheon+ sample
• Decaying dark energy in light of the latest cosmological dataset
• The H0 trouble: Confronting Non-thermal Dark Matter and Phantom Cosmology with the CMB, BAO, and Type Ia Supernovae data
• Prospects for weighing neutrinos in interacting dark energy models using joint observations of gravitational waves and $\gamma$-ray bursts
• Cosmological effects of the Galileon term in Scalar-Tensor Theories
• Running cosmological constant with observational tests
• Observational Constraints on the Dark Energy with a Quadratic Equation of State
• The tension in the absolute magnitude of Type Ia supernovae
• Signatures of Light Massive Relics on nonlinear structure formation
• Comprehensive Constraints on Dark Radiation Injection After BBN
• Interacting dark energy in the dark $SU(2{)}_R$ model
• Cosmological N-body simulations with generic hot dark matter
• Terrestrial Probes of Electromagnetically Interacting Dark Radiation
• Testing the consistency between cosmological measurements of distance and age
• Mitigating the binary viewing angle bias for standard sirens
• Quintessential early dark energy
• Dissecting kinetically coupled quintessence: phenomenology and observational tests
• Cornering (quasi) degenerate neutrinos with cosmology
• On The Distribution of Bayesian Evidences
• Constraining Holographic Dark Energy and Analyzing Cosmological Tensions
• Cosmological constraints on $\gamma$-gravity models
• One-parameter dynamical dark-energy from the generalized Chaplygin gas
• Minihalos as probes of the inflationary spectrum: accurate boost factor calculation and new CMB constraints
• Measuring the BAO peak position with different galaxy selections
• Cosmological implications of tracker scalar fields: Testing the evidence for dynamical dark energy with recent data
• Exploring cosmological imprints of phantom crossing with dynamical dark energy in Horndeski gravity
• Cosmological constraints with the Effective Fluid approach for Modified Gravity
• Constraining non-minimally coupled $\beta$-exponential inflation with CMB data
• On the concordance of cosmological data in the case of the generalized Chaplygin gas
• Constraints on Dark Matter-Photon Coupling in the Presence of Time-Varying Dark Energy
• Self-interacting neutrinos, the Hubble parameter tension, and the Cosmic Microwave Background
• Revisit of constraints on dark energy with Hubble parameter measurements including future redshift drift observations
• The DESI One-Percent Survey: Modelling the clustering and halo occupation of all four DESI tracers with Uchuu
• Real-time cosmology with SKA
• Late Time Modification of Structure Growth and the S8 Tension
• Roles of sterile neutrinos in particle physics and cosmology
• No evidence for EDE from Planck data in extended scenarios
• Scaling solutions as Early Dark Energy resolutions to the Hubble tension
• Breaking the baryon-dark matter degeneracy in a model-independent way through the Sunyaev-Zeldovich effect
• Cosmological tests of gravity with latest observations
• Hubble tension as a window on the gravitation of the dark matter sector: Exploration of a family of models
• Coupled Dark Sector Models and Cosmological Tensions
• The interacting vacuum and tensions: a comparison of theoretical models
• Constraints on sterile neutrinos and the cosmological tensions
• Testing Modified Gravity theory (MOG) with Type Ia Supernovae, Cosmic Chronometers and Baryon Acoustic Oscillations
• Using the Mark Weighted Correlation Functions to Improve the Constraints on Cosmological Parameters
• Distance-duality in theories with a nonminimal coupling to gravity
• Late-time acceleration with steep exponential potentials
• Coupled dark energy model inspired from general conformal transformation
• Reconstruction with velocities
• Optimal prior for Bayesian inference in a constrained parameter space
• Potentialities of Hubble parameter and expansion rate function data to alleviate Hubble tension
• Sound-Horizon-Agnostic Inference of the Hubble Constant and Neutrino Mass from BAO, CMB Lensing, and Galaxy Weak Lensing and Clustering
• Cosmological surveys with multi-object spectrographs
• Cosmological constraints on ultra-light axion fields
• Probing the Weak Gravity Conjecture in the Cosmic Microwave Background
• Bound Dark Energy: towards understanding the nature of the Dark Energy
• Exploring evidence of interaction between dark energy and dark matter
• Reconstructions of $f(\mathcal{P})$ and $f(\mathcal{Q})$ gravity models from $(m,n)$-type Barrow Holographic Dark Energy: Analysis and Observational Constraints
• Cosmological constraints from the redshift dependence of the volume effect using the galaxy 2-point correlation function across the line-of-sight
• Is there another coincidence problem at the reionization epoch?
• Domain Wall Network: A Dual Solution for Gravitational Waves and Hubble Tension?
• Large-Distance Lens Uncertainties and Time-Delay Measurements of $H_0$
• External priors for the next generation of CMB experiments
• Gravitational waves, CMB polarization, and the Hubble tension
• Low-Redshift Constraints on Covariant Canonical Gauge Theory of Gravity
• Cosmology and CPT violating neutrinos
• Reheating constraints to WIMPflation
• Model Selection with Baryonic Acoustic Oscillations in the Lyman-alpha Forest
• Bayesian Comparison of Interacting Modified Holographic Ricci Dark Energy Scenarios
• Dynamical dark energy in light of cosmic distance measurements II: a study using current observations
• Interacting dark energy constraints from the full-shape analyses of BOSS DR12 and DES Year 3 measurements
• Cosmological Constraints on Thermal Friction of Axion Dark Matter
• Coupled Quintessence scalar field model in light of observational datasets
• Euclid: Testing the Copernican principle with next-generation surveys
• The viable f(G) gravity models via reconstruction from the observations
• Can acoustic and axion-like early dark energy still resolve the Hubble tension?
• Cosmological Constraints using the newest VLT-KMOS HII Galaxies and the full Planck CMB spectrum
• Exploring Modified Gravity: Constraints on the $\mu$ and $\Sigma$ Parametrization with WMAP, ACT, and SPT
• Cosmological bounds on neutrino statistics
• Testing the consistency of early and late cosmological parameters with BAO and CMB data
• Implications for cosmology from Ground-based Cosmic Microwave Background observations
• Deep Learning and genetic algorithms for cosmological Bayesian inference speed-up
• Constraining Cosmological Parameters with Viscous Modified Chaplygin Gas and Generalized Cosmic Chaplygin Gas Models in Horava-Lifshitz Gravity: Utilizing Late-time Datasets
• A convenient approach to characterizing model uncertainty with application to early dark energy solutions of the Hubble tension
• cp3-bench: A tool for benchmarking symbolic regression algorithms tested with cosmology
• The measurements of matter density perturbations amplitude from cosmological data
• Constraining cosmological scaling solutions of a Galileon field
• Scalar Dark Energy Models and Scalar-Tensor Gravity: Theoretical Explanations for the Accelerated Expansion of Present Universe
• Combining strongly lensed and unlensed fast radio bursts: To be a more precise late-universe probe
• Non-linear Structure Formation for Dark Energy Models with a Steep Equation of State
• Axi-Higgs cosmology: Cosmic Microwave Background and cosmological tensions
• Lower tensor-to-scalar ratio as possible signature of modified gravity
• Degeneracy between nonadiabatic dark energy models and $\Lambda$CDM: ISW effect and the cross correlation of CMB with galaxy clustering data
• Growth and Geometry Split in Light of the DES-Y3 Survey
• Analysis cosmological tachyon and fermion model and observation data constraints
• Constraints on Late Time Violations of the Equivalence Principle in the Dark Sector
• Revisiting holographic dark energy from the perspective of multi-messenger gravitational wave astronomy: future joint observations with short gamma-ray bursts
• Singling out modified gravity parameters and datasets reveals a dichotomy between Planck and lensing
• Tachyonic vs Quintessence dark energy: linear perturbations and CMB data
• Investigating the dynamical models of cosmology with recent observations and upcoming gravitational-wave data
• Chameleon Early Dark Energy and the Hubble Tension
• Thermal WIMPs and the Scale of New Physics: Global Fits of Dirac Dark Matter Effective Field Theories
• Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos
• On tachyonic stability priors for dark energy
• Observational constraints on running vacuum model
• Late-Time Anisotropy Sourced by a 2-Form Field Non-Minimally Coupled to Cold Dark Matter
• Perturbation Theory Remixed: Improved Nonlinearity Modeling beyond Standard Perturbation Theory
• Constraints on dark energy from TDCOSMO & SLACS lenses
• Flatness without CMB - the Entanglement of Spatial Curvature and Dark Energy Equation of State
• Endowing $\mathbf{\Lambda }$ with a dynamic nature: constraints in a spatially curved Universe
• Possible Impact of non-Gaussianities on cosmological constraints in neutrino physics
• Nonlinear structure formation in Bound Dark Energy
• Higgs Inflation: constraining the top quark mass and breaking the $H_0$-${\sigma }_8$ correlation
• Can Baby Universe Absorption Explain Dark Energy?
• A New Probe of the High-z BAO scale: BAO tomography With CMB $\times$ LIM-Nulling Convergence
• Prospects for searching for sterile neutrinos with gravitational wave and $\gamma$-ray burst joint observations
• Impact of Low ell's on Large Scale Structure Anomalies
• Holographic Dark Energy from the Anti-de Sitter Black Hole
• Cosmological constant constraints from observation-derived energy condition bounds and their application to bimetric massive gravity
• Beyond dark energy Fisher forecasts: how DESI will constrain LCDM and quintessence models
• Brane inflation driven by an arctan potential: CMB constraints and Reheating
• One Extension to Explain Them All, One Scale-Invariant Spectrum to Test Them All, and in One Model Bind Them
• A solution to the S8 tension through neutrino-dark matter interactions
• Climbing out of the shadows: building the distance ladder with black hole images
• Addressing the $r_d$ Tension using Late-Time Observational Measurements in a Novel deceleration Parametrization
• Elucidating Dark Energy with Future 21 cm Observations at the Epoch of Reionization
• Constraining neutrino mass in dynamical dark energy cosmologies with the logarithm parametrization and the oscillating parametrization
• Scrutinizing coupled vector dark energy in light of data
• Cosmological test of an extended quintessence model
• Measuring the scalar induced gravitational waves from observations
• Improvement of cosmological constraints with the cross correlation between line-of-sight optical galaxy and FRB dispersion measure
• Effects of Dark Energy anisotropic stress on the matter power spectrum
• Observational Constraints on the Parameters of Hořava-Lifshitz Gravity
• Observational constraints on inflection point quintessence with a cubic potential
• Super-Eddington accreting massive black holes explore high-$z$ cosmology: Monte-Carlo simulations
• The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar and APOGEE-2 Data
• 2D BAO vs 3D BAO: Hints for new physics?
• Spatial variation of fundamental constants: testing models with thermonuclear supernovae
• Type Ia supernova constraints on compact object dark matter
• Dark Energy with a Triplet of Classical U(1) Fields
• Deep learning for cosmological parameter inference from a dark matter halo density field
• Redshift-space distortion constraints on the neutrino mass and models to alleviate the Hubble tension
• Equality scale-based and sound horizon-based analysis of the Hubble tension
• Hint of dark matter-dark energy interaction in DESI DR2 and current cosmological dataset?
• Constraints on Metastable Dark Energy Decaying into Dark Matter
• Dark matter component decaying after recombination: constraints from diffuse gamma-ray and neutrino flux measurements
• Observational Constraints on Extended Starobinsky and Weyl Gravity Model of Inflation
• Relaxing cosmological constraints on current neutrino masses
• The environmental dependence of the baryon acoustic peak in the Baryon Oscillation Spectroscopic Survey CMASS sample
• Improving Constraint on ${\Omega }_m$ from SDSS Using Marked Correlation Functions
• Thermodynamics of Modified Chaplygin-Jacobi Gas and Modified Chaplygin-Abel Gas: Stability Analysis and Observational Constraints
• A new way to test the WIMP dark matter models
• Constraints on the phase transition of Early Dark Energy with the CMB anisotropies
• Local Limit of Nonlocal Gravity: A Teleparallel Extension of General Relativity
• Voids and Halos in Voids statistics as a probe of the Expansion History of the Universe
• Role of Future SNIa Data from Rubin LSST in Reinvestigating Cosmological Models
• Constraints on the non-minimally coupled Witten-O'Raifeartaigh inflation
• Perturbation in an interacting dark universe
• Data Analysis and Phenomenological Cosmology
• Local Limit of Nonlocal Gravity: Cosmological Perturbations
• Cool dark sector, concordance, and a low ${\sigma }_8$
• Weak Lensing Constraints on Dark Matter-Baryon Interactions with $N$-Body Simulations and Machine Learning
• Improving SDSS cosmological constraints through $\beta$-skeleton weighted correlation functions
• Sound Horizon Independent Constraints on Early Dark Energy: The Role of Supernova Data
• Structure Formation in Dark Matter Particle Production Cosmology
• Detection significance of Baryon Acoustic Oscillations peaks in galaxy and quasar clustering
• Dark Matter-Radiation Scattering Enhances CMB Phase Shift through Dark Matter-loading
• Reconstruction of energy conditions from observations and implications for extended theories of gravity
• Cosmological Standard Timers from Unstable Primordial Relics
• Prospects for cosmological research with the FAST array: 21-cm intensity mapping survey observation strategies
• Reconstructions of Einstein-Aether Gravity from Barrow Agegraphic and New Barrow Agegraphic Dark Energy models: Examinations and Observational Limits
• Hints of the $H_0-r_d$ tension in uncorrelated Baryon Acoustic Oscillations dataset
• A glitch in gravity: cosmic Lorentz-violation from fiery Big Bang to glacial heat death
• Multi-messenger standard-siren cosmology for third-generation gravitational-wave detectors: forecasts considering observations of gamma-ray bursts and kilonovae
• The smearing scale in Laguerre reconstructions of the correlation function
• Constraints on the varying electron mass and early dark energy in light of ACT DR6 and DESI DR2 and the implications for inflation
• On the origin of the BAOtr-DESI tension
• Exploring the Evolution of Nonlinear Electrodynamics in the Universe: A Dynamical Systems Approach
• Averaged universe confronted with cosmological observations: A fully covariant approach
• Implications of Dynamical Dark Energy in the expansion of the Universe and the Structure Formation
• Cosmic Reionization Study : Principle Component Analysis After Planck
• Early dark energy in the pre- and post-recombination epochs
• Improvements in cosmological constraints from breaking growth degeneracy
• The Low Redshift survey at Calar Alto (LoRCA)
• Discerning Dark Energy Models with High-Redshift Standard Candles
• The consistency test on the cosmic evolution
• Mass assembly history of dark matter halos in the light of $H_0$ tension
• Dark Energy Constraints from Pantheon+ Ia Supernovae Data
• Quintessence and tachyon dark energy in interaction with dark matter: Observational constraints and model selection
• Testing the coupling of dark radiations in light of the Hubble tension
• On the Field Theoretical Description of an Alternative Model to Generalized Chaplygin Gas and its Thermodynamic Behaviour
• Common Origin of Warm Dark Matter and Dark Radiation
• Late Time Phenomena in $f(T,\mathcal{T})$ Gravity Framework: Role of $H_0$ Priors
• The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes
• Observational constraints on cosmological parameters in the Bianchi type III Universe with f(R,T) gravity theory
• Reconciling cosmic dipolar tensions with a gigaparsec void
• Mixing Bispectrum Multipoles Under Geometric Distortions
• Lensing convergence and anisotropic dark energy in galaxy redshift surveys
• Updated neutrino mass constraints from galaxy clustering and CMB lensing-galaxy cross-correlation measurements
• Hubble Tension and Dark Energy in Teleparallel Gauss-Bonnet Gravity: New Constraints from DESI BAO, Pantheon${}^{+}$ and Hubble Data
• Measuring the primordial curvature perturbations from the scalar induced gravitational waves
• Anisotropic cosmology in Bumblebee gravity theory
• Cosmological Perturbations in the 5D Holographic Big Bang Model
• Influence of the correlation prior on reconstruction of the dark energy equation of state
• Baryon acoustic oscillations from a joint analysis of the large-scale clustering in Fourier and configuration space
• A frequentist view on the two-body decaying dark matter model
• Baryon Acoustic Oscillations analyses with Density-Split Statistics
• An Introduction to the Planck Mission
• Observational constraints on inflationary potentials within the quantum collapse framework
• Measuring the primordial gravitational waves from cosmic microwave background and stochastic gravitational wave background observations
• Constraints on Axions from Cosmic Distance Measurements
• Pantheon+ tomography and Hubble tension
• KiDS-Legacy: Constraints on Horndeski gravity from weak lensing combined with galaxy clustering and cosmic microwave background anisotropies
• Non-linear coupling in the dark sector as a running vacuum model
• Equivalence of Dark Energy Models: A Theoretical and Bayesian Perspective
• Observational Constraints on the Cosmology with Holographic Dark Fluid
• Probing the independence within the dark sector in the fluid approximation
• Realising effective theories of tribrid inflation: Are there effects from messenger fields?
• A Semiblind Reconstruction of the History of Effective Number of Neutrinos Using CMB Data
• The Hydrogen Intensity and Real-time Analysis eXperiment: 256-Element Array Status and Overview
• Hubble Expansion as an Einstein Curvature
• Gravitational Lensing of Dark Energy Models and $\Lambda$CDM Using Observational data in Loop Quantum Cosmology
• The Correlation Function and Detection of Baryon Acoustic Oscillation Peak from the Spectroscopic SDSS GalWCat Galaxy Cluster Catalogue
• Phenomenological power spectrum models for H$\alpha$ emission line galaxies from the Nancy Grace Roman Space Telescope
• Neutrinos as a probe of curvature
• Cosmological constraints from galaxy multi-tracers in the nearby Universe
• FAST drift scan survey for HI intensity mapping: simulation on hunting HI filament with pairwise stacking
• Mimetic Tensor-Vector-Scalar Cosmology: Incorporating Dark Matter, Dark Energy and Stiff Matter
• Probing gravity with the DES-CMASS sample and BOSS spectroscopy
• Cosmological Implications of a Neutrino Mass Detection
• Derivative hierarchy as the origin of kernel-dependent trends in Gaussian process reconstructions of the hubble parameter
• A new pressure-parametric cosmological model
• Constraining Axially Symmetric Bianchi Type I Model with Self-Consistent Recombination History and Observables
• Dark Energy Survey: DESI-Independent Angular BAO Measurement
• Role of Spatial Curvature in a Dark Energy Interacting Model
• Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints
• Constraints on Multicomponent Dark Energy from Cosmological Observations
• Unimodular Theory of Gravity in Light of the Latest Cosmological Data
• Results and forecasts on cosmic inflation from weak lensing
• Non-linear structure formation with elastic interactions in the dark sector
• Can cosmic rotation resolve the Hubble tension? Constraints from CMB and large-scale structure
• Studying baryon acoustic oscillations using photometric redshifts from the DESI Legacy Imaging survey DR9
• Cuscuton-like contribution to dark energy evolution
• Toward Cosmological Standard Timers in Primordial Black Hole Binaries
• Detecting the neutrino mass and mass hierarchy from global data
• The BINGO/ABDUS Project: Forecast for cosmological parameters from a mock Fast Radio Bursts survey
• Mimicking the $\Lambda$CDM Universe through inhomogeneous space-time
• Can Dark Energy Emerge from a Varying $G$ and Spacetime Geometry?
• Gravitational Waves in a Closed Spacetime via Deviation Equation
• KiDS-Legacy: Constraining dark energy, neutrino mass, and curvature
• Forecasts for cosmological measurements based on the angular power spectra of AGN and clusters of galaxies in the SRG/eROSITA all-sky survey
• Constraining decaying dark matter with BOSS data and the effective field theory of large-scale structures
• Dusty Clump Survival in Supernova Ejecta: Dust-Mediated Growth vs. Crushing by the Reverse Shock
• Dissecting the $H_0$ and $S_8$ tensions with Planck + BAO + supernova type Ia in multi-parameter cosmologies
• Dark Energy Survey Year 3 Results: Galaxy Sample for BAO Measurement
• Sub-percentage measure of distances to redshift of 0.1 by a new cosmic ruler
• Accelerating BAO Scale Fitting Using Taylor Series
• Reference frame dependence of the local measurement of the Hubble constant
• Does the Reionization Model Influence the Constraints on Dark Matter Decay or Annihilation?
• Model independent reconstruction of cosmological accelerated-decelerated phase
• Some Classes of Interacting Two-Fluid Model of the Expanding Universe
• Preliminary clustering properties of the DESI BGS bright targets using DR9 Legacy Imaging Surveys
• Low-redshift tests of Newtonian cosmologies with a time-varying gravitational constant
• Does History Repeat Itself? Periodic Time Cosmology
• Cosmological constraints on mass-varying dark matter
• Cosmological measurements from the CMB and BAO are insensitive to the tail probability in the assumed likelihood
• Refitting cosmological data with neutrino mass and degeneracy
• Toward accurate measurement of property-dependent galaxy clustering: II. Tests of the smoothed density-corrected $V_{\max }$ method
• Confronting Einstein Yang Mills Higgs Dark Energy in light of observations
• A step in the right direction? Analyzing the Wess Zumino Dark Radiation solution to the Hubble tension
• A New Paradigm for Testing Gravity: Theory-Independent Constraints Using Data From All Astrophysical and Cosmological Scales
• Generalized neutrino isocurvature
• Power Suppression and Lensing Anomaly -- A phenomenological investigation
• Dark energy with oscillatory tracking potential: Observational Constraints and Perturbative effects
• A gigaparsec-scale local void and the Hubble tension
• The magnitude of the dark ages 21-cm signal in the context of existing early and late time constraints on $\Lambda$CDM
• Cosmological constraints from the density gradient weighted correlation function
• Bayes' Theorem, Inflation, and the Ekpyrotic Universe
• Exploring the constraints on cosmological models with CosmoEJS
• A speed limit on tachyon fields from cosmological and fine-structure data
• Baryon Acoustic Oscillations in tomographic Angular Density and Redshift Fluctuations
• Recent results and perspectives on cosmology and fundamental physics from microwave surveys
• Combining Planck and SPT cluster catalogs: cosmological analysis and impact on Planck scaling relation calibration
• Improved cosmological constraints on the neutrino mass and lifetime
• Gamma-Ray Bursts, Supernovae Ia and Baryon Acoustic Oscillations: a binned cosmological analysis
• Measurements of cosmic expansion and growth rate of structure from voids in the Sloan Digital Sky Survey between redshift 0.07 and 1.0
• SHARP VIII: J0924+0219 lens mass distribution and time-delay prediction through adaptive-optics imaging
• Enhancing Cosmological Constraints by Two-dimensional $\beta$-cosmic-web Weighted Angular Correlation Functions
• Probing dark energy with braneworld cosmology in the light of recent cosmological data
• Bayesian evidence and model selection approach for time-dependent dark energy
• Model-independent reconstruction of cosmic thermodynamics and dark energy dynamics
• Cosmography via stellar archaeology of low-redshift early-type galaxies from SDSS
• A Quantum Genetic Algorithm with application to Cosmological Parameters Estimation
• Beyond thermal approximations: Precise cosmological bounds on Axion-Like Particles
• Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension
• Freeze-in Dark Matter via Lepton Portal: Hubble Tension and Stellar Cooling
• The impact of the locally measured Hubble parameter on the mass of Sterile neutrino
• Measuring the speed of scalar induced gravitational waves from observations
• The $H_0$ and $S_8$ tensions necessitate early and late time changes to $\Lambda$CDM
• An Overview of CHIME, the Canadian Hydrogen Intensity Mapping Experiment
• Perturbations In Some Dark Energy Models
• Inflation in a scalar-vector gravity theory
• Fluctuations in the Ginzburg-Landau Theory of Dark Energy: internal (in-)consistencies in PLANCK data set
• Testing Large-Scale Structure Measurements Against Fisher Matrix Predictions