The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant

Abstract

We analyse the large-scale correlation function of the 6dF Galaxy Survey (6dFGS) and detect a Baryon Acoustic Oscillation (BAO) signal. The 6dFGS BAO detection allows us to constrain the distance-redshift relation at z_{\rm eff} = 0.106. We achieve a distance measure of D_V(z_{\rm eff}) = 456\pm27 Mpc and a measurement of the distance ratio, r_s(z_d)/D_V(z_{\rm eff}) = 0.336\pm0.015 (4.5% precision), where r_s(z_d) is the sound horizon at the drag epoch z_d. The low effective redshift of 6dFGS makes it a competitive and independent alternative to Cepheids and low-z supernovae in constraining the Hubble constant. We find a Hubble constant of H_0 = 67\pm3.2 km s^{-1} Mpc^{-1} (4.8% precision) that depends only on the WMAP-7 calibration of the sound horizon and on the galaxy clustering in 6dFGS. Compared to earlier BAO studies at higher redshift, our analysis is less dependent on other cosmological parameters. The sensitivity to H_0 can be used to break the degeneracy between the dark energy equation of state parameter w and H_0 in the CMB data. We determine that w = -0.97\pm0.13, using only WMAP-7 and BAO data from both 6dFGS and \citet{Percival:2009xn}. We also discuss predictions for the large scale correlation function of two future wide-angle surveys: the WALLABY blind H{\sc I} survey (with the Australian SKA Pathfinder, ASKAP), and the proposed TAIPAN all-southern-sky optical galaxy survey with the UK Schmidt Telescope (UKST). We find that both surveys are very likely to yield detections of the BAO peak, making WALLABY the first radio galaxy survey to do so. We also predict that TAIPAN has the potential to constrain the Hubble constant with 3% precision.

18 pages, 17 figures, 3 tables

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• Implication of the Hubble tension for the primordial Universe in light of recent cosmological data
• Hubble parameter measurement constraints on dark energy
• How the Dark Energy Can Reconcile \textit{Planck} with Local Determination of the Hubble Constant
• $Om$ diagnostic applied to scalar field models and slowing down of cosmic acceleration
• Constraints on primordial gravitational waves from the Cosmic Microwave Background
• Angular Baryon Acoustic Oscillation measure at z=2.225 from the SDSS quasar survey
• Baryon Acoustic Oscillations from the SDSS DR10 galaxies angular correlation function
• Is exponential gravity a viable description for the whole cosmological history?
• The Taipan Galaxy Survey: Scientific Goals and Observing Strategy
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: weighing the neutrino mass using the galaxy power spectrum of the CMASS sample
• Cosmology Intertwined IV: The Age of the Universe and its Curvature
• Dark sectors with dynamical coupling
• Planck 2015 constraints on the non-flat $\Lambda$CDM inflation model
• Cosmology with the EFTofLSS and BOSS: dark energy constraints and a note on priors
• New Early Dark Energy is compatible with current LSS data
• Unified galaxy power spectrum measurements from 6dFGS, BOSS, and eBOSS
• The Weak Lensing Signal and the Clustering of BOSS Galaxies I: Measurements
• Exploring the full parameter space for an interacting dark energy model with recent observations including redshift-space distortions: Application of the parametrized post-Friedmann approach
• Testing coupled dark energy with large scale structure observation
• Evidence for Emergent Dark Energy
• Determining the Hubble Constant without the Sound Horizon: Measurements from Galaxy Surveys
• Dark sector interaction and the supernova absolute magnitude tension
• The Void Size Function in Dynamical Dark Energy Cosmologies
• Unraveling the effective fluid approach for $f(R)$ models in the subhorizon approximation
• The impact of the cosmic variance on $H_0$ on cosmological analyses
• The parameter space in Galileon gravity models
• A model with interaction of dark components and recent observational data
• Dark Sky Simulations: Early Data Release
• Wide Angle Effects in Future Galaxy Surveys
• nIFTy Cosmology: Galaxy/halo mock catalogue comparison project on clustering statistics
• The 2-degree Field Lensing Survey: design and clustering measurements
• 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
• A General Analysis of Direct Dark Matter Detection: From Microphysics to Observational Signatures
• Effects of neutrino mass hierarchies on dynamical dark energy models
• Searching for dark matter - dark energy interactions: going beyond the conformal case
• $H_0$ tension as a hint for a transition in gravitational theory
• Testing models of vacuum energy interacting with cold dark matter
• Homogeneity and isotropy in the 2MASS Photometric Redshift catalogue
• Observational constraints on generalized Proca theories
• Late time approaches to the Hubble tension deforming $H(z)$, worsen the growth tension
• Can dark energy be dynamical?
• Late-transition vs smooth $H(z)$ deformation models for the resolution of the Hubble crisis
• Reconciling $H_0$ tension in a six parameter space?
• Ultra-light axions and the $S_8$ tension: joint constraints from the cosmic microwave background and galaxy clustering
• Constraining interacting dark energy models with latest cosmological observations
• Neutrino Mass Bounds in the era of Tension Cosmology
• Testing coupled dark energy models with their cosmological background evolution
• Non-local gravity and comparison with observational datasets
• Can Conformally Coupled Modified Gravity Solve The Hubble Tension?
• Recombination-independent determination of the sound horizon and the Hubble constant from BAO
• Cosmological Constraints on Invisible Neutrino Decays Revisited
• Dynamical dark energy: scalar fields and running vacuum
• Realistic cosmological scenario with non-minimal kinetic coupling
• Cosmological constraints on neutrino self-interactions with a light mediator
• Quantifying dimensionality: Bayesian cosmological model complexities
• On the Validity of Cosmological Fisher Matrix Forecasts
• Super-renormalizable or finite completion of the Starobinsky theory
• The Sigma-8 Tension is a Drag
• Chasing the phantom: A closer look at Type Ia supernovae and the dark energy equation of state
• Effects of Anisotropic Stress in Interacting Dark Matter - Dark Energy Scenarios
• Ginzburg-Landau Theory of Dark Energy: A Framework to Study Both Temporal and Spatial Cosmological Tensions Simultaneously
• Phenomenology of Modified Gravity at Recombination
• 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
• Clustering and Halo Abundances in Early Dark Energy Cosmological Models
• Cosmological discordances II: Hubble constant, Planck and large-scale-structure data sets
• Dark Sector to Restore Cosmological Concordance
• MultiDark-Galaxies: data release and first results
• Is cosmic acceleration proven by local cosmological probes?
• Cosmological constraints on post-Newtonian parameters in effectively massless scalar-tensor theories of gravity
• A new null diagnostic customized for reconstructing the properties of dark energy from BAO data
• Constraining the time evolution of dark energy, curvature and neutrino properties with cosmic chronometers
• Cosmological Constraints on Interacting Light Particles
• Strong evidence for an accelerating universe
• Constraining cosmic deceleration-acceleration transition with type Ia supernova, BAO/CMB and H(z) data
• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: geometry and growth from the anisotropic void-galaxy correlation function in the luminous red galaxy sample
• Brans-Dicke cosmology with a $\Lambda$- term: a possible solution to $\Lambda$CDM tensions
• A Detection of the Baryon Acoustic Oscillation Features in the SDSS BOSS DR12 Galaxy Bispectrum
• The power spectrum and bispectrum of SDSS DR11 BOSS galaxies II: cosmological interpretation
• No new cosmological concordance with massive sterile neutrinos
• Comparison of dark energy models after Planck 2015
• Constraining a dark matter and dark energy interaction scenario with a dynamical equation of state
• Constraining models of $f(R)$ gravity with Planck and WiggleZ power spectrum data
• Euclid: Forecast constraints on the cosmic distance duality relation with complementary external probes
• Fast simulations for intensity mapping experiments
• Cosmological constraints on parametrized interacting dark energy
• Cosmological constraints from baryon acoustic oscillations and clustering of large-scale structure
• Analysis with observational constraints in $\Lambda$-cosmology in $f(R,T)$ gravity
• Early mass varying neutrino dark energy: Nugget formation and Hubble anomaly
• Cosmic slowing down of acceleration for several dark energy parametrizations
• Early-Universe-Physics Insensitive and Uncalibrated Cosmic Standards: Constraints on ${\Omega }_{\mathrm{m}}$ and Implications for the Hubble Tension
• Is there concordance within the concordance $\Lambda$CDM model?
• The Dark Matter equation of state through cosmic history
• Cosmology From CMB Lensing and Delensed EE Power Spectra Using 2019-2020 SPT-3G Polarization Data
• Towards early dark energy and $n_s$=1 with Planck, ACT and SPT
• The $H_0$ tension: $\Delta G_N$ vs. $\Delta N_{\mathrm{eff}}$
• The clustering of ALFALFA galaxies: dependence on HI mass, relationship to optical samples & clues on host halo properties
• Nonlinear structure formation in Nonlocal Gravity
• The BOSS-WiggleZ overlap region I: Baryon Acoustic Oscillations
• Cosmic expansion histories in massive bigravity with symmetric matter coupling
• Measuring the Hubble constant and spatial curvature from supernova apparent magnitude, baryon acoustic oscillation, and Hubble parameter data
• An Updated Tomographic Analysis of the Integrated Sachs-Wolfe Effect and implications for Dark Energy
• A new parametrization of Hubble parameter in $f(Q)$ gravity
• Updated constraints from the effective field theory analysis of BOSS power spectrum on Early Dark Energy
• Testing the Copernican principle by constraining spatial homogeneity
• Swampland Conjectures and Late-Time Cosmology
• Bounds on light sterile neutrino mass and mixing from cosmology and laboratory searches
• Observational constraints on interacting Tsallis holographic dark energy models
• Hubble flow variance and the cosmic rest frame
• Cosmological Bound on the QCD Axion Mass, Redux
• Cosmological constraints from the power spectrum of eBOSS emission line galaxies
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space
• The trouble beyond $H_0$ and the new cosmic triangles
• Forecast for cosmological parameter estimation with gravitational-wave standard siren observation from the Cosmic Explorer
• CMB and BAO constraints for an induced gravity dark energy model with a quartic potential
• Constraining the Dark Energy Equation of State with HII Galaxies
• Consistency of the growth rate in different environments with the 6dF Galaxy Survey: measurement of the void-galaxy and galaxy-galaxy correlation functions
• Hubble Frontier Fields: systematic errors in strong lensing models of galaxy clusters - Implications for cosmography
• No-go guide for the Hubble tension : Late-time solutions
• Halo model and halo properties in Galileon gravity cosmologies
• Constraints on cosmological parameters in power-law cosmology
• MGCAMB with massive neutrinos and dynamical dark energy
• The Hubble Tension as a Hint of Leptogenesis and Neutrino Mass Generation
• Revisit of the interacting holographic dark energy model after Planck 2015
• Symmetry of Cosmological Observables, and a High Hubble Constant as an Indicator of a Mirror World Dark Sector
• Ups and Downs in Dark Energy: phase transition in dark sector as a proposal to lessen cosmological tensions
• Cosmological discordances: a new measure, marginalization effects, and application to geometry vs growth current data sets
• We do not live in the R_h = c t universe
• The evidence of cosmic acceleration and observational constraints
• Addressing $H_0$ tension by means of VCDM
• Cosmological parameter estimation with future gravitational wave standard siren observation from the Einstein Telescope
• Constraints on non-flat cosmologies with massive neutrinos after Planck 2015
• Constraints on reconstructed dark energy model from SN Ia and BAO/CMB observations
• Soundness of Dark Energy properties
• Impacts of dark energy on weighing neutrinos: mass hierarchies considered
• Late time transitions in the quintessence field and the $H_0$ tension
• Determining the Hubble constant using Giant extragalactic HII regions and HII galaxies
• $\Lambda$CDM or self-interacting neutrinos? - how CMB data can tell the two models apart
• Updated Constraints and Forecasts on Primordial Tensor Modes
• Cosmology from large scale galaxy clustering and galaxy-galaxy lensing with Dark Energy Survey Science Verification data
• Phenomenology of the generalized cubic covariant Galileon model and cosmological bounds
• Signatures of the Primordial Universe from Its Emptiness: Measurement of Baryon Acoustic Oscillations from Minima of the Density Field
• Cosmological limits on neutrino unknowns versus low redshift priors
• Flavor-specific Interaction Favors Strong Neutrino Self-coupling in the Early Universe
• Cosmology with the Large Synoptic Survey Telescope: an Overview
• Results from the Wilkinson Microwave Anisotropy Probe
• A comprehensive comparison of cosmological models from latest observational data
• Can dark energy be expressed as a power series of the Hubble parameter?
• A 2% Distance to z = 0.35 by Reconstructing Baryon Acoustic Oscillations - III : Cosmological Measurements and Interpretation
• The Impact of the Fiducial Cosmology Assumption on BAO Cosmological Parameter Inference
• Testing Low-Redshift Cosmic Acceleration with Large-Scale Structure
• 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
• Revealing the effects of curvature on the cosmological models
• A Measurement of Gravitational Lensing of the Cosmic Microwave Background Using SPT-3G 2018 Data
• Cosmological constraints on late-universe decaying dark matter as a solution to the $H_0$ tension
• Late time interacting cosmologies and the Hubble constant tension
• An Efficient and Accurate Hybrid Method for Simulating Non-Linear Neutrino Structure
• Cosmology and the neutrino mass ordering
• $T_0$ censorship of early dark energy and AdS vacua
• Constraints on the Brans-Dicke gravity theory with the Planck data
• Full-Shape Galaxy Power Spectra and the Curvature Tension
• 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
• Impacts of dark energy on weighing neutrinos after Planck 2015
• Constraints on the neutrino mass and mass hierarchy from cosmological observations
• Probing Cosmological Isotropy With Type IA Supernovae
• Observational signatures of anisotropic inflationary models
• Robustness of baryon acoustic oscillation constraints for early-Universe modifications to $\Lambda$CDM
• Einstein, Planck and Vera Rubin: relevant encounters between the Cosmological and the Quantum Worlds
• Observational Constraints on Oscillating Dark-Energy Parametrizations
• Long Range Interactions in Cosmology: Implications for Neutrinos
• BAO angular scale at z_eff = 0.11 with the SDSS blue galaxies
• Cosmological constraints on induced gravity dark energy models
• Dark Energy Constraints after Planck
• Coupled and uncoupled early dark energy, massive neutrinos and the cosmological tensions
• 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
• Testing H0 in Acoustic Dark Energy Models with Planck and ACT Polarization
• In search of the dark matter dark energy interaction: a kinematic approach
• Cosmological parameter inference with Bayesian statistics
• Post-$Planck$ constraints on interacting vacuum energy
• Dark Neutrino interactions phase out the Hubble tension
• Revisit of the Interaction between Holographic Dark Energy and Dark Matter
• Independent Cosmological Constraints from high-z HII Galaxies
• Prospects for improving cosmological parameter estimation with gravitational-wave standard sirens from Taiji
• Generalized Emergent Dark Energy Model and the Hubble Constant Tension
• Planck 2015 constraints on the non-flat $\varphi$CDM inflation model
• 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
• Cosmological Constraints from Gas Mass Fractions of Massive, Relaxed Galaxy Clusters
• The Clustering of Galaxies in the Completed SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from DR12 galaxy clustering -- towards an accurate model
• Coupled dark energy with perturbed Hubble expansion rate
• Efficient Reconstruction of Linear Baryon Acoustic Oscillations in Galaxy Surveys
• New observational constraints on $f(T)$ cosmology from radio quasars
• Rastall gravity extension of the standard $\Lambda$CDM model: theoretical features and observational constraints
• Linear growth of structure in massive bigravity
• Large Scale Structure Constraints for a Class of f(R) Theories of Gravity
• The BINGO Project I: Baryon Acoustic Oscillations from Integrated Neutral Gas Observations
• Gamma-Ray Bursts, Quasars, Baryonic Acoustic Oscillations, and Supernovae Ia: new statistical insights and cosmological constraints
• Data-driven Reconstruction of the Late-time Cosmic Acceleration with f(T) Gravity
• Prospects for Constraining Interacting Dark Energy Models with 21 cm Intensity Mapping Experiments
• Weighing neutrinos in the scenario of vacuum energy interacting with cold dark matter: application of the parameterized post-Friedmann approach
• Banana Split: Testing the Dark Energy Consistency with Geometry and Growth
• The Price of Shifting the Hubble Constant
• Model independent calibrations of gamma ray bursts using machine learning
• The Carnegie Hubble Program
• Connecting early and late epochs by f(z)CDM cosmography
• Cosmological constraints on an exponential interaction in the dark sector
• Testing AdS early dark energy with Planck, SPTpol and LSS data
• 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
• Changing the prior: absolute neutrino mass constraints in nonlocal gravity
• An evaluation of cosmological models from expansion and growth of structure measurements
• Forecasts for CMB μ- and i-type spectral distortion constraints on the primordial power spectrum on scales 8 < k < 10^4 Mpc^-1 with the future Pixie-like experiments
• Combining Planck with Large Scale Structure gives strong neutrino mass constraint
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: constraining modified gravity
• Hot New Early Dark Energy
• Measuring the transverse baryonic acoustic scale from the SDSS DR11 galaxies
• Robust and model-independent cosmological constraints from distance measurements
• Barrow Entropy Cosmology: an observational approach with a hint of stability analysis
• How clustering dark energy affects matter perturbations
• Unveiling dark fifth forces with linear cosmology
• Dark degeneracy I: Dynamical or interacting dark energy?
• A Critique of Holographic Dark Energy
• Cosmological implications of scale-independent energy-momentum squared gravity: Pseudo nonminimal interactions in dark matter and relativistic relics
• A search for sterile neutrinos with the latest cosmological observations
• A parametric reconstruction of the cosmological jerk from diverse observational data sets
• Robust model comparison disfavors power law cosmology
• AIC and BIC for cosmological interacting scenarios
• Acceleration of the universe: a reconstruction of the effective equation of state
• Constraints on neutrino masses from Planck and Galaxy Clustering data
• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from multi-tracer BAO analysis with galaxies and voids
• How closely do baryons follow dark matter on large scales?
• The $H_0$ and ${\sigma }_8$ tensions and the scale invariant spectrum
• Cosmological constraints on coupled dark energy
• Neutrinos in the holographic dark energy model: constraints from latest measurements of expansion history and growth of structure
• Model-independent limits and constraints on extended theories of gravity from cosmic reconstruction techniques
• Health checkup test of the standard cosmological model in view of recent Cosmic Microwave Background Anisotropies experiments
• Partially Acoustic Dark Matter Cosmology and Cosmological Constraints
• Ultra-light Axions: Degeneracies with Massive Neutrinos and Forecasts for Future Cosmological Observations
• Novel null tests for the spatial curvature and homogeneity of the Universe and their machine learning reconstructions
• Metastable Dark Energy with Radioactive-like Decay
• Galaxy Populations in Massive Galaxy Clusters to z=1.1: Color Distribution, Concentration, Halo Occupation Number and Red Sequence Fraction
• Primordial power spectra for curved inflating universes
• Dark Energy and Dark Matter from an additional adiabatic fluid
• Probing elastic interactions in the dark sector and the role of $S_8$
• Cosmological constraints on slow-roll inflation: an update
• Observational constraints on dark matter-dark energy scattering cross section
• New cosmological bounds on hot relics: Axions $\&$ Neutrinos
• 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
• CMB tensions with low-redshift $H_0$ and $S_8$ measurements: impact of a redshift-dependent type-Ia supernovae intrinsic luminosity
• Constraints on interacting dark energy models from time-delay cosmography with seven lensed quasars
• A Step in Understanding the $S_8$ Tension
• Fast and Credible Likelihood-Free Cosmology with Truncated Marginal Neural Ratio Estimation
• The foreground wedge and 21 cm BAO surveys
• Warm Decaying Dark Matter and the Hubble Tension
• Novel cosmological bounds on thermally-produced axion-like particles
• Planck 2015 constraints on the non-flat XCDM inflation model
• Improving constraints on the growth rate of structure by modelling the density-velocity cross-correlation in the 6dF Galaxy Survey
• Cosmological parameter estimation for dynamical dark energy models with future fast radio burst observations
• Effective field description of the Anton-Schmidt cosmic fluid
• Kinematic constraints beyond $z\simeq 0$ using calibrated GRB correlations
• Future Constraints on Dynamical Dark-Energy using Gravitational-Wave Standard Sirens
• Constraints on dark-matter properties from large-scale structure
• Gaussian processes reconstruction of modified gravitational wave propagation
• Primordial gravitational waves and the H0-tension problem
• From a Bounce to the Dark Energy Era with $F(R)$ Gravity
• Dark Radiation and interacting scenarios
• Theoretical Systematics of Future Baryon Acoustic Oscillation Surveys
• Cosmological bounds on dark matter-photon coupling
• Reheating in quintessential inflation via gravitational production of heavy massive particles: A detailed analysis
• Emergent Dark Energy, neutrinos and cosmological tensions
• Large-scale (in-) stability Analysis of an Exactly Solved Coupled Dark-Energy Model
• Speeding up $N$-body simulations of modified gravity: Chameleon screening models
• Designing Horndeski and the effective fluid approach
• Distinguishing interacting dark energy from wCDM with CMB, lensing, and baryon acoustic oscillation data
• Cosmic microwave background constraints on secret interactions among sterile neutrinos
• Combining pre- and post-recombination new physics to address cosmological tensions: case study with varying electron mass and sign-switching cosmological constant
• Sterile neutrino self-interactions: $H_0$ tension and short-baseline anomalies
• Planck intermediate results. XXIV. Constraints on variation of fundamental constants
• Testing the equation of state for viscous dark energy
• Non-local gravity and comparison with observational datasets. II. Updated results and Bayesian model comparison with $\Lambda$CDM
• Hints, neutrino bounds and WDM constraints from SDSS DR14 Lyman-$\alpha$ and Planck full-survey data
• Cosmology with nonminimal kinetic coupling and a power-law potential
• Constraints on active and sterile neutrinos in an interacting dark energy cosmology
• The Clustering of Galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Measuring H(z) and D_A(z) at z = 0.57 with Clustering Wedges
• Simple-graduated dark energy and spatial curvature
• Observational constraints on non-flat dynamical dark energy cosmological models
• Is there a concordance value for $H_0$?
• Mirror Twin Higgs Cosmology: Constraints and a Possible Resolution to the $H_0$ and $S_8$ Tensions
• Probing cosmology with weak lensing selected clusters I: Halo approach and all-sky simulations
• Comparison between different methods of model selection in cosmology
• Probing the neutrino mass hierarchy with CMB weak lensing
• Cosmological Constraint on ${\Omega }_m$ and ${\sigma }_8$ from Cluster Abundances using the $GalWCat19$ Optical-Spectroscopic SDSS Catalog
• Higgs-Dilaton Cosmology: An inflation - dark energy connection and forecasts for future galaxy surveys
• Testing Hu-Sawicki f(R) gravity with the Effective Field Theory approach
• Chain Early Dark Energy: Solving the Hubble Tension and Explaining Today's Dark Energy
• Testing the consistency between cosmological data: the impact of spatial curvature and the dark energy EoS
• Time-varying neutrino mass from a supercooled phase transition: current cosmological constraints and impact on the ${\Omega }_m$-${\sigma }_8$ plane
• On structure formation from a small-scales-interacting dark sector
• Horava Gravity in the Effective Field Theory formalism: from cosmology to observational constraints
• Constraining Supersymmetry using the relic density and the Higgs boson
• Ultralight Scalar Decay and the Hubble Tension
• Constraining dark matter properties with Cosmic Microwave Background observations
• Searching for Modified Gravity: Scale and Redshift Dependent Constraints from Galaxy Peculiar Velocities
• Planck 2015 constraints on spatially-flat dynamical 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
• A novel approach to quantifying the sensitivity of current and future cosmological datasets to the neutrino mass ordering through Bayesian hierarchical modeling
• Cosmological constraints of phantom dark energy models
• Starobinsky cosmological model in Palatini formalism
• Planck confronts large scale structure: methods to quantify discordance
• LyaCoLoRe: Synthetic Datasets for Current and Future Lyman-$\alpha$ Forest BAO Surveys
• Accelerating Universe in Hybrid and Logarithmic Teleparallel Gravity
• Phantom cosmological model with observational constraints in $f(Q)$ gravity
• Constraints on hybrid metric-Palatini models from background evolution
• Testing Dark energy models in the light of ${\sigma }_8$ tension
• Dark Energy Survey Year 1 Results: Constraining Baryonic Physics in the Universe
• EFTCAMB/EFTCosmoMC: massive neutrinos in dark cosmologies
• Accelerating expansion of the universe in modified symmetric teleparallel gravity
• The Atacama Cosmology Telescope: Cosmology from cross-correlations of unWISE galaxies and ACT DR6 CMB lensing
• An improved measurement of baryon acoustic oscillations from the correlation function of galaxy clusters at $z\sim 0.3$
• Screened fifth forces lower the TRGB-calibrated Hubble constant too
• A preliminary forecast for cosmological parameter estimation with gravitational-wave standard sirens from TianQin
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: application to the SDSS-III BOSS DR12 galaxies
• Quasi-dilaton non-linear massive gravity: Investigations of background cosmological dynamics
• Cosmological constraints with self-interacting sterile neutrinos
• Bayesian 3d velocity field reconstruction with VIRBIuS
• Modelling and testing the equation of state for (Early) dark energy
• Experimental constraints on the uncoupled Galileon model from SNLS3 data and other cosmological probes
• Cosmological parameter forecasts for HI intensity mapping experiments using the angular power spectrum
• Latest astronomical constraints on some nonlinear parametric dark energy models
• Phantom dark energy as an effect of bulk viscosity
• Cosmological Constraints on First-Order Phase Transitions
• Forecast for FAST: from Galaxies Survey to Intensity Mapping
• Search for sterile neutrinos in a universe of vacuum energy interacting with cold dark matter
• Modified gravity for surveys
• 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
• Constraints on quintessence scalar field models using cosmological observations
• Cosmological aspects of a hyperbolic solution in $f(R,T)$ gravity
• Multi-interacting dark energy and its cosmological implications
• Neutrinos and dark energy after Planck and BICEP2: data consistency tests and cosmological parameter constraints
• Assessment of the cosmic distance duality relation using Gaussian Process
• The SAMI Galaxy Survey: stellar population and structural trends across the Fundamental Plane
• Interaction between dark energy and dark matter: observational constraints from OHD, BAO, CMB and SNe Ia
• Field Level Neural Network Emulator for Cosmological N-body Simulations
• The DFSZ axion in the CMB
• Quantifying Tensions between CMB and Distance Datasets in Models with Free Curvature or Lensing Amplitude
• Standard-siren cosmology using gravitational waves from binary black holes
• Massive Photon and Dark Energy
• 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
• Gravity in the infrared and effective nonlocal models
• The Jubilee ISW Project II: observed and simulated imprints of voids and superclusters on the cosmic microwave background
• Dark Catalysis
• Testing interacting dark matter and dark energy model with cosmological data
• Return of Harrison-Zeldovich spectrum in light of recent cosmological tensions
• Baryon Acoustic Oscillation Theory and Modelling Systematics for the DESI 2024 results
• Consistency of Planck, ACT and SPT constraints on magnetically assisted recombination and forecasts for future experiments
• Distinguishing between Neutrinos and time-varying Dark Energy through Cosmic Time
• A Bayesian comparison between $\Lambda$CDM and phenomenologically emergent dark energy models
• Cosmology with matter diffusion
• Redshift Measurement and Spectral Classification for eBOSS Galaxies with the Redmonster Software
• Self-interacting dark matter from late decays and the $H_0$ tension
• Tension in the Void: Cosmic Rulers Strain Inhomogeneous Cosmologies
• Viscous cosmology in the Weyl-type $f(Q,T)$ gravity
• The full Boltzmann hierarchy for dark matter-massive neutrino interactions
• Dark Matter properties through cosmic history
• Joint growth rate measurements from redshift-space distortions and peculiar velocities in the 6dF Galaxy Survey
• A new test of $f(R)$ gravity with the cosmological standard rulers in radio quasars
• Reconstruction of the Dark Energy equation of state from latest data: the impact of theoretical priors
• Early Cosmology Constrained
• Hints of dark matter-neutrino interactions in Lyman-$\alpha$ data
• Cosmological investigations of (extended) nonlinear massive gravity schemes with non-minimal coupling
• Building a Predictive Model of Galaxy Formation - I: Phenomenological Model Constrained to the $z=0$ Stellar Mass Function
• Cosmological surveys with the Australian Square Kilometre Array Pathfinder
• Running the running
• Priors on the effective Dark Energy equation of state in scalar-tensor theories
• Dynamical Dark sectors and Neutrino masses and abundances
• Neutron star merger GW170817 strongly constrains doubly coupled bigravity
• Constraints and tensions in testing general relativity from Planck and CFHTLenS including intrinsic alignment systematics
• FORGE -- the f(R) gravity cosmic emulator project I: Introduction and matter power spectrum emulator
• Hints of dark energy anisotropic stress using Machine Learning
• Unified Dark Energy and Dark Matter from Dynamical Space Time
• Constraints on Pre-Recombination Early Dark Energy from SPT-3G Public Data
• One spectrum to cure them all: Signature from early Universe solves major anomalies and tensions in cosmology
• Strengthening the bound on the mass of the lightest neutrino with terrestrial and cosmological experiments
• Light Sterile Neutrinos in Cosmology and Short-Baseline Oscillation Experiments
• Testing the Etherington's distance duality relation at higher redshifts: the combination of radio quasars and gravitational waves
• Gravitational-Wave Detector Networks: Standard Sirens on Cosmology and Modified Gravity Theory
• How to relax the cosmological neutrino mass bound
• Generalized tracker quintessence models for dark energy
• Updated observational constraints on quintessence dark energy models
• Dark matter component decaying after recombination: Sensitivity to BAO and RSD probes
• The Cosmic Expansion History from Line-Intensity Mapping
• Sterile neutrinos with pseudoscalar self-interactions and cosmology
• 2MTF V. Cosmography, Beta, and the residual bulk flow
• Inflation model constraints from data released in 2015
• Cold dark matter plus not-so-clumpy dark relics
• Bayesian Evidences for Dark Energy models in light of current obsevational data
• Testing Gravity on Cosmic Scales: A Case Study of Jordan-Brans-Dicke Theory
• Using dark energy to suppress power at small scales
• Dark Energy Survey Year 1 Results: galaxy mock catalogues for BAO
• 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
• Cosmic equation of state from combined angular diameter distances: Does the tension with luminosity distances exist?
• Cosmological Constraint Precision of the Photometric and Spectroscopic Multi-probe Surveys of China Space Station Telescope (CSST)
• Metastable dark energy models in light of Planck 2018: Alleviating the $H_0$ tension
• Model-Independent Constraints on Lorentz Invariance Violation via the Cosmographic Approach
• Strong Planck constraints on braneworld and non-commutative inflation
• Unbiased methods for removing systematics from galaxy clustering measurements
• Prospect for constraining holographic dark energy with gravitational wave standard sirens from the Einstein Telescope
• Unbiased pseudo-Cl power spectrum estimation with mode projection
• Massive neutrino self-interactions and inflation
• Model-independent cosmic acceleration and type Ia supernovae intrinsic luminosity redshift dependence
• Impacts of gravitational-wave standard siren observations from Einstein Telescope and Cosmic Explorer on weighing neutrinos in interacting dark energy models
• Nonlocal Teleparallel Cosmology
• Early Dark Energy with Power-law F(R) Gravity
• Cosmological inference from the EFTofLSS: the eBOSS QSO full-shape analysis
• 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
• On the dynamics of a dark sector coupling
• Reconstruction of the neutrino mass as a function of redshift
• Cannibalism hinders growth: Cannibal Dark Matter and the $S_8$ tension
• Thermodynamical aspects of Bianchi type-I Universe in quadratic form of $f\left(Q\right)$ gravity and observational constraints
• Measuring the 2D Baryon Acoustic Oscillation signal of galaxies in WiggleZ: Cosmological constraints
• AGN and their host galaxies in the local Universe: two mass independent Eddington ratio distribution functions characterize black hole growth
• An Axially Symmetric Transitioning models with Observational Constraints
• Forecasting the Interaction in Dark Matter-Dark Energy Models with Standard Sirens From the Einstein Telescope
• New constraints on the distance duality relation from the local data
• Constraints on the sum of neutrino masses using cosmological data including the latest extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample
• Growth of matter perturbations in clustered holographic dark energy cosmologies
• Measuring Baryon Acoustic Oscillations from the clustering of voids
• The galaxy-halo connection in the VIDEO Survey at 0.5<z<1.7
• Observational constraints on cosmological models with Chaplygin gas and quadratic equation of state
• Non-linear evolution of the BAO scale in alternative theories of gravity
• (Lack of) Cosmological evidence for dark radiation after Planck
• Quintessence with Yukawa Interaction
• Cosmology with varying fundamental constants from hyperlight, coupled scalars
• Reconstruction of the dark matter-vacuum energy interaction
• Observational constraints of the modified cosmology through Barrow entropy
• Planck intermediate results. XVI. Profile likelihoods for cosmological parameters
• Power spectrum multipoles on the curved sky: an application to the 6-degree Field Galaxy Survey
• Implications of the B-mode Polarization Measurement for Direct Detection of Inflationary Gravitational Waves
• Searching for sterile neutrinos in dynamical dark energy cosmologies
• Cosmology with Gravitational Wave/Fast Radio Burst Associations
• Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy
• Redshift drift exploration for interacting dark energy
• Revisiting a non-parametric reconstruction of the deceleration parameter from combined background and the growth rate data
• 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
• Exploring neutrino mass and mass hierarchy in interacting dark energy models
• Parametrized modified gravity constraints after Planck
• Measurement of Hubble constant with stellar-mass binary black holes
• Model selection applied to reconstructions of the Dark Energy
• Principal reconstructed modes of dark energy and gravity
• Limits on the cosmic neutrino background
• 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
• Power law cosmology model comparison with CMB scale information
• Interacting viscous dark fluids
• Cosmic distance duality and cosmic transparency
• Simultaneous constraints on the number and mass of relativistic species
• $\nu$Galileon: modified gravity with massive neutrinos as a testable alternative to $\Lambda$CDM
• Galaxy formation on the largest scales: The impact of astrophysics on the BAO peak
• Axi-Higgs Cosmology
• Neutrino and Dark Radiation properties in light of latest CMB observations
• The BINGO telescope: a new instrument exploring the new 21-cm cosmology window
• Dynamical dark energy in the light of DESI 2024 data
• Full-shape BOSS constraints on dark matter interacting with dark radiation and lifting the $S_8$ tension
• Touch of Neutrinos on the Vacuum Metamorphosis: is the $H_0$ Solution Back?
• Can Holographic dark energy models fit the observational data?
• Forecasting Interacting Vacuum-Energy Models using Gravitational Waves
• Revisiting Metastable Dark Energy and Tensions in the Estimation of Cosmological Parameters
• Cosmology with fast radio bursts in the era of SKA
• Testing logarithmic corrections on $R^2$-exponential gravity by observational data
• Free-streaming and Coupled Dark Radiation Isocurvature Perturbations: Constraints and Application to the Hubble Tension
• Minimal dark energy: key to sterile neutrino and Hubble constant tensions?
• Investigating the Hubble Constant Tension -- Two Numbers in the Standard Cosmological Model
• Testing the distance duality relation using type Ia supernovae and ultracompact radio sources
• Lensing-like tensions in the Planck legacy release
• High Redshift Standard Candles: Predicted Cosmological Constraints
• Revisiting CMB constraints on dark matter annihilation
• What can CMB observations tell us about the neutrino distribution function?
• Cosmological constraints on the gravitational constant
• Improved constraint on the primordial gravitational-wave density using recent cosmological data and its impact on cosmic string models
• A measurement of the CMB E-mode angular power spectrum at subdegree scales from 670 square degrees of POLARBEAR data
• Reducing the $H_0$ tension with generalized Proca theory
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: Measuring the anisotropic Baryon Acoustic Oscillations with redshift weights
• Power-law cosmology, SN Ia, and BAO
• Information Content of Higher-Order Galaxy Correlation Functions
• Model selection and constraints from Holographic dark energy scenarios
• Can small-scale baryon inhomogeneities resolve the Hubble tension? An investigation with ACT DR4
• Fast full N-body simulations of generic modified gravity: conformal coupling models
• Machine learning constraints on deviations from general relativity from the large scale structure of the Universe
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• Testing Einstein's gravity and dark energy with growth of matter perturbations: Indications for new Physics?
• Exploring the properties of milliarcsecond radio sources
• New Limits on Coupled Dark Energy from Planck
• Probing the properties of relic neutrinos using the cosmic microwave background, the Hubble Space Telescope and galaxy clusters
• Stochastic bias of colour-selected BAO tracers by joint clustering-weak lensing analysis
• Asymmetric Dark Matter Models in SO(10)
• CMB Constraint on Dark Matter Annihilation after Planck 2015
• Tensions with the flat $\mathbf{\Lambda }$CDM model from high-redshift cosmography
• $H_0$ Tension and the Phantom Regime: A Case Study In Terms of an Infrared $f(T)$ Gravity
• Measuring the distance-redshift relation with the baryon acoustic oscillations of galaxy clusters
• Dark Energy Survey Year 1 Results: Galaxy Sample for BAO Measurement
• Machine Learning improved fits of the sound horizon at the baryon drag epoch
• CosmicNet II: Emulating extended cosmologies with efficient and accurate neural networks
• Theoretical and observational bounds on some interacting vacuum energy scenarios
• Distance Priors from \emph{Planck} 2015 data
• The XXL survey: XLVI. Forward cosmological analysis of the C1 cluster sample
• Stepped Partially Acoustic Dark Matter, Large Scale Structure, and the Hubble Tension
• Estimating the galaxy two-point correlation function using a split random catalog
• Towards a self-consistent analysis of the anisotropic galaxy two- and three-point correlation functions on large scales: application to mock galaxy catalogues
• Brane with variable tension as a possible solution to the problem of the late cosmic acceleration
• A New $Om(z)$ Diagnostic of Dark Energy in General Relativity Theory
• Toward a concordance teleparallel Cosmology I: Background Dynamics
• Constraining the spatial curvature with cosmic expansion history in a cosmological model with a non-standard sound horizon
• No-go guide for late-time solutions to the Hubble tension: Matter perturbations
• The 6dF Galaxy Survey: Dependence of halo occupation on stellar mass
• Smoothing the $H_0$ tension with a dynamical dark energy model
• Strongly Lensed Gravitational Waves and Electromagnetic Signals as Powerful Cosmic Rulers
• The Dark Side of the Universe after Planck
• 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
• Exploration of interacting dynamical dark energy model with interaction term including the equation-of-state parameter: alleviation of the $H_0$ tension
• Late-time cosmology in $f(Q,L_m)$ gravity: Analytical solutions and observational fits
• Cosmology With Low-Redshift Observations: No Signal For New Physics
• Bulk viscous matter and the cosmic acceleration of the universe in $f(Q,T)$ gravity
• No H_0 Assistance from Assisted Quintessence
• Measuring the sound horizon and absolute magnitude of SNIa by maximizing the consistency between low-redshift data sets
• Minimally Modified Gravity fitting Planck data better than $\Lambda$CDM
• Testing dark energy after pre-recombination early dark energy
• Gravitational wave propagation in $f(R)$ models: New parametrizations and observational constraints
• Confronting interacting dark radiation scenarios with cosmological data
• Impact of $H_0$ priors on $f(T)$ late time cosmology
• Modified gravity and massive neutrinos: constraints from the full shape analysis of BOSS galaxies and forecasts for Stage IV surveys
• Imprints of an extended Chevallier-Polarski-Linder parametrization on the large scale of our universe
• Dynamics and cosmological constraints on Brans-Dicke cosmology
• Testing Predictions of the Quantum Landscape Multiverse 2: The Exponential Inflationary Potential
• Neutrinos secretly converting to lighter particles to please both KATRIN and the cosmos
• Cosmological Constraints on sub-horizon scales modified gravity theories with MGCLASS II
• Hubble tension in lepton asymmetric cosmology with an extra radiation
• Luminosity distance and anisotropic sky-sampling at low redshifts: a numerical relativity study
• Microphysics of Early Dark Energy
• Constraints on Lorentz Invariance Violation with gamma-ray bursts via a Markov Chain Monte Carlo approach
• Holographic Dark Energy with Cosmological Constant
• Revisiting the holographic dark energy in a non-flat universe: alternative model and cosmological parameter constraints
• Do you smell something decaying? Updated linear constraints on decaying dark matter scenarios
• CosmoBit: A GAMBIT module for computing cosmological observables and likelihoods
• $H_0$ Ex Machina: Vacuum Metamorphosis and Beyond $H_0$
• Observational Constraints on Axion(s) Dark Energy with a Cosmological Constant
• Fitting string inflation to real cosmological data: the Fibre Inflation case
• BAO from angular clustering: optimization and mitigation of theoretical systematics
• A Dark Matter Trigger for Early Dark Energy Coincidence
• Conservative cosmology: combining data with allowance for unknown systematics
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: Dynamical dark energy
• Bayesian Comparison of Interacting Scenarios
• Dark energy imprints on the kinematic Sunyaev-Zel'dovich signal
• Tsallis holographic dark energy in Fractal Universe
• Fractional Dark Matter decay: cosmological imprints and observational constraints
• Weighing Neutrinos in $f(R)$ gravity
• Wandering in the Lyman-alpha Forest: A Study of Dark Matter-Dark Radiation Interactions
• Testing Predictions of the Quantum Landscape Multiverse 1: The Starobinsky Inflationary Potential
• Exploring accelerated expansion in the universe: A study of $f(Q,T)$ gravity with parameterized EoS and cosmological constraints
• Observational constraints and predictions of the interacting dark sector with field-fluid mapping
• Constraints on $f(T)$ Cosmology with Pantheon+
• Using the topology of large-scale structure in the WiggleZ Dark Energy Survey as a cosmological standard ruler
• The Copernican principle in light of the latest cosmological data
• Robustness of cosmic neutrino background detection in the cosmic microwave background
• The correlation function of galaxy clusters and detection of baryon acoustic oscillations
• A local measurement of the growth rate from peculiar velocities and galaxy clustering correlations in the 6dF Galaxy Survey
• Hydrodynamical simulations of coupled and uncoupled quintessence models I: Halo properties and the cosmic web
• A void in the Hubble tension? The end of the line for the Hubble bubble
• CoLoRe: fast cosmological realisations over large volumes with multiple tracers
• $5\sigma$ tension between Planck cosmic microwave background and eBOSS Lyman-alpha forest and constraints on physics beyond $\Lambda$CDM
• Cosmological Constraints on Higgs-Dilaton Inflation
• Estimating the power spectrum covariance matrix with fewer mock samples
• Precision CMB constraints on eV-scale bosons coupled to neutrinos
• On cosmological signatures of baryons-dark energy elastic couplings
• FLRW cosmology with EDSFD parametrization
• Searching for scalar gravitational interactions in current and future cosmological data
• Exploring the Dark Universe: constraints on dynamical Dark Energy models from CMB, BAO and growth rate measurements
• Interacting two-component fluid models with varying EoS parameter
• Models of vacuum energy interacting with cold dark matter: Constraints and comparison
• Dark Energy as a Critical Phenomenon: a Resolution for Hubble Tension
• Cosmology in massive gravity
• Dark Radiation and Inflationary Freedom after Planck 2015
• Powerbox: A Python package for creating structured fields with isotropic power spectra
• Observational constraints on Tsallis modified gravity
• Constraining spatial curvature with large-scale structure
• An exploration of an early gravity transition in light of cosmological tensions
• Two Fluid Scenario in Bianchi Type-I Universe
• Information Gains from Cosmological Probes
• 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 $z=0.59$
• Multiple transitions in vacuum dark energy and $H_0$ tension
• Is there evidence for anomalous dipole anisotropy in the large-scale structure?
• A grounded perspective on New Early Dark Energy using ACT, SPT, and BICEP/Keck
• The degeneracy between primordial non-Gaussianity and foregrounds in 21cm intensity mapping experiments
• Constraining the dark matter-vacuum energy interaction using the EDGES 21-cm absorption signal
• Constraints on the Early and Late Integrated Sachs-Wolfe effects from Planck 2015 Cosmic Microwave Background Anisotropies angular power spectra
• Latest evidence for a late time vacuum -- geodesic CDM interaction
• Status on bidimensional dark energy parameterizations using SNe Ia JLA and BAO datasets
• Redshift-space streaming velocity effects on the Lyman-$\alpha$ forest baryon acoustic oscillation scale
• Constraining the Expansion History and Early Dark Energy with Line Intensity Mapping
• Testing standard and non-standard neutrino physics with cosmological data
• Fast full $N$-body simulations of generic modified gravity: derivative coupling models
• The $H_0$ Tension in Non-flat QCDM Cosmology
• Disconnected Covariance of 2-point Functions in Large-Scale Structure
• Inflationary cosmology with Chaplygin gas in Palatini formalism
• Post-Planck Dark Energy Constraints
• Cosmological constraints to dark matter with two- and many-body decays
• Perturbation theory challenge for cosmological parameters estimation: Matter power spectrum in real space
• Profiling Cold New Early Dark Energy
• Bayesian evidence for $\alpha$-attractor dark energy models
• Constraining the dynamical dark energy parameters: Planck-2013 vs WMAP9
• The weak, the strong and the ugly -- A comparative analysis of interacting stepped dark radiation
• A comprehensive investigation on the slowing down of cosmic acceleration
• Scale-invariant alternatives to general relativity. III. The inflation--dark-energy connection
• New MGCAMB tests of gravity with CosmoMC and Cobaya
• Exploring late-time cosmic acceleration: A study of a linear $f(T)$ cosmological model using observational data
• Observational constraints on bimetric gravity
• On the current status of Modified Gravity
• Dark energy and Dark matter interaction in light of the second law of thermodynamics
• Dark energy by natural evolution: Constraining dark energy using Approximate Bayesian Computation
• The QCD phase transition behind a PBH origin of LIGO/Virgo events?
• Probing Early Modification of Gravity with Planck, ACT and SPT
• J-PAS: Forecasts for dark matter - dark energy elastic couplings
• How does non-linear dynamics affect the baryon acoustic oscillation?
• Cross-correlation of galaxies and galaxy clusters in the Sloan Digital Sky Survey and the importance of non-Poissonian shot noise
• Gravitational quantum effects on power spectra and spectral indices with higher-order corrections
• Strong Bounds on Sum of Neutrino Masses in a 12 Parameter Extended Scenario with Non-Phantom Dynamical Dark Energy ($w(z)\ge -1$)
• Constraining the $\Lambda$CDM and Galileon models with recent cosmological data
• Euclid: Forecast constraints on consistency tests of the $\Lambda$CDM model
• Statistical tests of sterile neutrinos using cosmology and short-baseline data
• Constraint on $f(R)$ Gravity through the Redshift Space Distortion
• Detecting quantum gravitational effects of loop quantum cosmology in the early universe?
• Environmental Quenching and Galactic Conformity in the Galaxy Cross-Correlation Signal
• Observational Tests of Gauss-Bonnet Like Dark Energy Model
• Parameter splitting in dark energy: is dark energy the same in the background and in the cosmic structures?
• Evaporating primordial black holes as varying dark energy
• Can varying the gravitational constant alleviate the tensions ?
• The distinctions between $\Lambda$CDM and $f(T)$ gravity according Noether symmetry
• Mitigating the Impact of the DESI Fiber Assignment on Galaxy Clustering
• Tickling the CMB damping tail: scrutinizing the tension between the ACT and SPT experiments
• Thermal Friction as a Solution to the Hubble and Large-Scale Structure Tensions
• Cosmological perturbations for two cold fluids in $\Lambda$CDM
• Localizing modes of massive fermions and a U(1) gauge field in the inflating baby-skyrmion branes
• Limits on Clustering and Smooth Quintessence from the EFTofLSS
• Is Dark Energy Dynamical in the DESI Era? A Critical Review
• Constraints on massive vector dark energy models from integrated Sachs-Wolfe-galaxy cross-correlations
• First experimental constraints on the disformally coupled Galileon model
• $f(Q)$-gravity and neutrino physics
• Data Analysis of three parameter models of deceleration parameter in FRW Universe
• Modified Cosmology Models from Thermodynamical Approach
• Prospects for constraining interacting dark energy models from gravitational wave and gamma ray burst joint observation
• N-body simulations with a cosmic vector for dark energy
• Constraining massive gravity with recent cosmological data
• $\alpha$ attractors in Quintessential Inflation motivated by Supergravity
• Constraints on inflation revisited: An analysis including the latest local measurement of the Hubble constant
• Implications of an extended dark energy model with massive neutrinos
• Cosmology-marginalized approaches in Bayesian model comparison: the neutrino mass as a case study
• Massive neutrino self-interactions with a light mediator in cosmology
• Non-parametric dark energy reconstruction using the tomographic Alcock-Paczynski test
• First study of reionization in the Planck 2015 normalized closed $\Lambda$CDM inflation model
• Cosmological model with decaying vacuum energy law from principles of quantum mechanics
• BAO cosmography
• Phantom scalar-tensor models and cosmological tensions
• Dark energy and matter interacting scenario to relieve $H_0$ and $S_8$ tensions
• Increasing the Lensing Figure of Merit through Higher Order Convergence Moments
• Dynamics of the diffusive DM-DE interaction--dynamical system approach
• A Cosmological Underdensity Does Not Solve the Hubble Tension
• Complementing the ground-based CMB Stage-4 experiment on large scales with the PIXIE satellite
• Cosmological parameter estimation with Genetic Algorithms
• Including massive neutrinos in thermal Sunyaev Zeldovich power spectrum and cluster counts analyses
• Analysis of accretion disk around a black hole in dRGT massive gravity
• A forecast of using fast radio burst observations to constrain holographic dark energy
• Non-minimal Derivative Coupling Scalar Field and Bulk Viscous Dark Energy
• Forecast of Neutrino Cosmology from the CSST Photometric Galaxy Clustering and Cosmic Shear Surveys
• IWDM: The fate of an interacting non-cold dark matter $-$ vacuum scenario
• Cosmological model of the interaction between dark matter and dark energy
• Constraining power of cosmological observables: blind redshift spots and optimal ranges
• Low-redshift estimates of the absolute scale of baryon acoustic oscillations
• Gravitino LSP and leptogenesis after the first LHC results
• Constraints on decaying dark matter from weak lensing and cluster counts
• Axion cold dark matter: status after Planck and BICEP2
• Reaffirming the Cosmic Acceleration without Supernova and CMB
• A magnified glance into the dark sector: probing cosmological models with strong lensing in A1689
• Cosmological constraints on early dark energy from the full shape analysis of eBOSS DR16
• Type Ia supernova Hubble diagram with near-infrared and optical observations
• Scaling Transformations and the Origins of Light Relics Constraints from Cosmic Microwave Background Observations
• SDSS-III Baryon Oscillation Spectroscopic Survey: Analysis of Potential Systematics in Fitting of Baryon Acoustic Feature
• Constraining the dark energy statefinder hierarchy in a kinematic approach
• Connecting inflation with late cosmic acceleration by particle production
• Observational effects of a running Planck mass
• Tracing the cosmic history by Gauss-Bonnet gravity
• Isotropic vs. Anisotropic components of BAO data: a tool for model selection
• Separate Constraints on Early and Late Cosmology
• MeV dark matter in the 3+1+1 model
• Impact of the Hubble tension on the $r$-$n_s$ contour
• Positivity bounds from multiple vacua and their cosmological consequences
• Super-CMB fluctuations and the Hubble tension
• Updated constraints from the PLANCK experiment on modified gravity
• Measuring growth index in a universe with sterile neutrinos
• Cosmological evidence for leptonic asymmetry after Planck
• Probing $f(R)$ cosmology with sterile neutrinos via measurements of scale-dependent growth rate of structure
• Cosmological constraints on dark energy models using DESI BAO 2024
• Bayesian model selection on Scalar $\epsilon$-Field Dark Energy
• Broadband distortion modeling in Lyman-$\alpha$ forest BAO fitting
• Improved constraint on primordial gravitational waves in light of the Hubble tension and BICEP/Keck
• Global view of neutrino interactions in cosmology: The freestreaming window as seen by Planck
• A cosmographic analysis of the transition to acceleration using SN-Ia and BAO
• Constraint on noncommutative spacetime from PLANCK data
• Probing the interaction between dark energy and dark matter with future fast radio burst observations
• Observational Constraints on Dynamical Dark Energy Models
• Improving sampling and calibration of GRBs as distance indicators
• Observational constraints on conformal time symmetry, missing matter and double dark energy
• Constraining light sterile neutrino mass with the BICEP2/Keck Array 2014 B-mode polarization data
• Investigating the accelerated expansion of the Universe through updated constraints on viable $f(R)$ models within the metric formalism
• The Hubble-Lemaître constant and sound horizon from low-redshift probes
• Constraints on primordial lepton asymmetries with full neutrino transport
• Concordance Cosmology?
• Hubble constant difference between CMB lensing and BAO measurements
• Testing the warmness of dark matter
• Hill crossing during preheating after hilltop inflation
• Reconstruction of interaction rate in Holographic dark energy model with Hubble horizon as the infrared cut-off
• Cosmology with nonminimal kinetic coupling and a Higgs-like potential
• Cosmological constraints on non-adiabatic dark energy perturbations
• Quintessential inflation and cosmological seesaw Mechanism: reheating and observational constraints
• Impacts of dark energy on constraining neutrino mass after Planck 2018
• Cosmological Constraints on Non-flat Exponential $f(R)$ Gravity
• Profile Likelihoods in Cosmology: When, Why and How illustrated with $\Lambda$CDM, Massive Neutrinos and Dark Energy
• Prospects for measuring dark energy with 21 cm intensity mapping experiments: A joint survey strategy
• Toward a concordance teleparallel Cosmology II: Linear perturbation
• Isolating the Lyman Alpha Forest BAO Anomaly
• 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
• Phantom braneworld and the Hubble tension
• Sound speed of scalar field dark energy: weak effects and large uncertainties
• Cosmic constraint on massive neutrinos in viable f(R) gravity with producing LCDM background expansion
• Comparing the scalar-field dark energy models with recent observations
• First Results from the La Silla-QUEST Supernova Survey and the Carnegie Supernova Project
• The Integrated Sachs Wolfe effect: unWISE and Planck constraints on Dynamical Dark Energy
• Strong gravitational lensing constraints on holographic dark energy
• Forecast for weighing neutrinos in cosmology with SKA
• Newest measurements of Hubble constant from DESI 2024 BAO observations
• Bayesian comparison of nonstandard cosmologies using type Ia supernovae and BAO data
• Linear bias and halo occupation distribution of emission line galaxies from Nancy Grace Roman Space Telescope
• Current constraints on deviations from General Relativity using binning in redshift and scale
• Probing a Steep EoS for Dark Energy with latest observations
• TDCOSMO VI: Distance Measurements in Time-delay Cosmography under the Mass-sheet transformation
• First cosmological constraints combining Planck with the recent gravitational-wave standard siren measurement of the Hubble constant
• Primordial magnetic field as a common solution of nanohertz gravitational waves and the Hubble tension
• Can phantom transition at $z\sim 1$ restore the Cosmic concordance?
• Testing f(R) gravity with the simulated data of gravitational waves from the Einstein Telescope
• Phenomenological Reconstruction of $f(T)$ Teleparallel Gravity
• CMB and matter power spectra with non-linear dark-sector interactions
• 4D Gauss-Bonnet gravity: cosmological constraints, $H_0$ tension and large scale structure
• Possible indication for non-zero neutrino mass and additional neutrino species from cosmological observations
• Constraining the relative velocity effect using the Baryon Oscillation Spectroscopic Survey
• Cosmic slowing down of acceleration using $f_{gas}$
• Cosmological Constraints on the Gravitational Interactions of Matter and Dark Matter
• Dynamical systems analysis of tachyon dark energy model from a new perspective
• On An Interacting New Holographic Dark Energy Model: observational constraints
• Model-independent study for a quintessence model of dark energy: Analysis and Observational constraints
• Constraining a late time transition of $G_{\mathrm{eff}}$ using low-z galaxy survey data
• Cosmological constraints on the Multi Scalar Field Dark Matter model
• Testing for New Physics: Neutrinos and the Primordial Power Spectrum
• New cosmological constraints with extended-Baryon Oscillation Spectroscopic Survey DR14 quasar sample
• A thorough investigation of the prospects of eLISA in addressing the Hubble tension: Fisher Forecast, MCMC and Machine Learning
• The phenomenology of beyond Horndeski gravity
• Hubble constant and sound horizon from the late-time Universe
• Constraints on $f(Q)$ logarithmic model using gravitational wave standard sirens
• Cosmological constraints from the cross-correlation of DESI Luminous Red Galaxies with CMB lensing from Planck PR4 and ACT DR6
• Friedmann cosmology with decaying vacuum density in Brans-Dicke theory
• Late-time acceleration with a scalar field source: Observational constraints and statefinder diagnostics
• New parametrization of the dark-energy equation of state with a single parameter
• Exploring hints for dark energy density evolution in light of recent data
• Prospects for measuring dark energy with 21 cm intensity mapping experiments
• Parametric resonance after hilltop inflation caused by an inhomogeneous inflaton field
• Strong constraints on a simple self-interacting neutrino cosmology
• Cosmological Tests of Everpresent $\Lambda$
• Analytical and EZmock covariance validation for the DESI 2024 results
• Revisiting the impact of neutrino mass hierarchies on neutrino mass constraints in light of recent DESI data
• Disentangling interacting dark energy cosmologies with the three-point correlation function
• Constraining f(R) Gravity with Planck Sunyaev-Zel'dovich Clusters
• Redshift drift constraints on holographic dark energy
• A detection of baryon acoustic oscillations from the distribution of galaxy clusters
• Constraining Sterile Neutrino Cosmology with Terrestrial Oscillation Experiments
• Cascading Dark Energy
• Observational constraints on $\alpha$-attractor inflationary models with a Higgs-like potential
• The role of CMB spectral distortions in the Hubble tension: a proof of principle
• Nested sampling with any prior you like
• Modeling cosmic acceleration with a generalized varying deceleration parameter
• The Impact of Line Misidentification on Cosmological Constraints from Euclid and other Spectroscopic Galaxy Surveys
• Cosmological constraints and phenomenology of a beyond-Horndeski model
• Constraints on Steep Equation of State for the Dark Energy using BAO
• Extending the halo mass resolution of $N$-body simulations
• Constraining holographic cosmology using Planck data
• Non-Canonical Volume-Form Formulation of Modified Gravity Theories and Cosmology
• Cosmological implications of the transition from the false vacuum to the true vacuum state
• The WiggleZ Dark Energy Survey: Probing the Epoch of Radiation Domination using Large Scale Structure
• Probing Modified Gravity with Integrated Sachs-Wolfe CMB and Galaxy Cross-correlations
• Constraints on Newton's Constant from Cosmological Observations
• Constraints on dark energy from the Lyα forest baryon acoustic oscillations measurement of the redshift 2.3 Hubble parameter
• Constraints on neutrino mass in the scenario of vacuum energy interacting with cold dark matter after Planck 2018
• Alleviating Cosmological Tensions with a Coupled Scalar Fields Model
• Cosmological Constraints from Galaxy Cluster Sparsity, Cluster Gas Mass Fraction and Baryon Acoustic Oscillations Data
• Anisotropic f(Q) gravity model with bulk viscosity
• Gaugessence: a dark energy model with early time radiation-like equation of state
• Reconstruction of interaction rate in Holographic dark energy
• Constraints on shear and rotation with massive galaxy clusters
• K-mouflage Imprints on Cosmological Observables and Data Constraints
• Reexploration of interacting holographic dark energy model: Cases of interaction term excluding the Hubble parameter
• Neutrino Anisotropies after Planck
• Testing cosmic acceleration for $w(z)$ parameterizations using $f_{gas}$ measurements in galaxy clusters
• Barry and the BAO Model Comparison
• Viscous cosmology in $f(T)$ gravity
• A new $f(Q)$ cosmological model with $H(z)$ quadratic expansion
• Probing dynamics of dark energy with latest observations
• Early dark energy and its interaction with dark matter
• Cosmological discordances III: more on measure properties, Large-Scale-Structure constraints, the Hubble constant and Planck
• Vacuum Energy Density Measured from Cosmological Data
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Exploring the dependence of the three-point correlation function on stellar mass and luminosity at 0.5<z<1.1
• Quantum mechanical look at the radioactive-like decay of metastable dark energy
• Update constraints on neutrino mass and mass hierarchy in light of dark energy models
• Exploring Universe acceleration through observational constraints via Hubble parameter reconstruction
• Extended $\Lambda$CDM model
• An accurate determination of the Hubble constant from Baryon Acoustic Oscillation datasets
• Constraining the interaction between dark sectors with future HI intensity mapping observations
• Cosmological search for sterile neutrinos after Planck 2018
• Spatial Curvature in $f(R)$ Gravity
• Probing the primordial universe with gravitational waves detectors
• Investigating early and late-time epochs in $f(Q)$ gravity
• Observational constraints on the oscillating dark energy cosmologies
• Corrected holographic dark energy with power-law entropy and Hubble Horizon cut-off in FRW Universe
• Is the Cosmic Transparency Spatially Homogeneous?
• Dark sectors of the Universe: A Euclid survey approach
• A comprehensive parametrization approach for the Hubble parameter in scalar field dark energy models
• Time-dependent $G$ in Einstein's equations as an alternative to the cosmological constant
• Theoretical priors in scalar-tensor cosmologies: Thawing quintessence
• On measuring the absolute scale of baryon acoustic oscillations
• Decay of multiple dark matter particles to dark radiation in different epochs does not alleviate the Hubble tension
• C${}^3$-Cluster Clustering Cosmology II. First detection of the BAO peak in the three-point correlation function of galaxy clusters
• Analytical approximations for curved primordial power spectra
• Big Bang Nucleosynthesis constraints on varying electron mass solution to the Hubble tension
• Post-inflationary axion isocurvature perturbations facing CMB and large-scale structure
• Dark Sectors with Mass Thresholds Face Cosmological Datasets
• IDECAMB: an implementation of interacting dark energy cosmology in CAMB
• Constraining cosmology with the cosmic microwave and infrared backgrounds correlation
• Reconciling $S_8$: Insights from Interacting Dark Sectors
• HOD-Dependent Systematics in Emission Line Galaxies for the DESI 2024 BAO analysis
• Reduced modified Chaplygin gas cosmology
• Dynamical Dark Matter from Thermal Freeze-Out
• Unified and consistent structure growth measurements from joint ACT, SPT and \textit{Planck} CMB lensing
• Testing extended Jordan-Brans-Dicke theories with future cosmological observations
• The traces of anisotropic dark energy in light of Planck
• Ultra-compact structure in radio quasars as a cosmological probe: a revised study of the interaction between cosmic dark sectors
• The environment and host haloes of the brightest z~6 Lyman-break galaxies
• Effective equation of state in modified gravity and observational constraints
• Observational constraints on the generalized $\alpha$ attractor model
• Cosmological acceleration
• A note on the relations between thermodynamics, energy definitions and Friedmann equations
• Testing the $n_s-H_0$ scaling relation with Planck-independent CMB data
• Probing $\Lambda$CDM cosmology with the Evolutionary Map of the Universe survey
• Extended $\Lambda$CDM model and viscous dark energy: A Bayesian analysis
• Ultra-large-scale approximations and galaxy clustering: debiasing constraints on cosmological parameters
• Measuring the Geometry of the Universe from Weak Gravitational Lensing behind Galaxy Groups in the HST COSMOS survey
• Does jackknife scale really matter for accurate large-scale structure covariances?
• Resonant neutrino self-interactions and the $H_0$ tension
• The Alcock-Paczyński effect from Lyman-$\alpha$ forest correlations: Analysis validation with synthetic data
• No evidence for dynamical dark energy in two models
• Constraints on the exponential $f(R)$ model from latest Hubble parameter measurements
• Sweeping Horndeski Canvas: New Growth-Rate Parameterization for Modified-Gravity Theories
• Confronting Tracker Field Quintessence with Data
• Cold dark energy constraints from the abundance of galaxy clusters
• The BAHAMAS project: Effects of dynamical dark energy on large-scale structure
• A New Test of Dynamical Dark Energy Models and Cosmic Tensions in Hořava Gravity
• Combining cosmological and local bounds on bimetric theory
• Redshift remapping and cosmic acceleration in dark-matter-dominated cosmological models
• A critical discussion on the $H_0$ tension
• Testing the local void hypothesis using baryon acoustic oscillation measurements over the last twenty years
• Principal components of dark energy with SNLS supernovae: the effects of systematic errors
• Cosmology from weak lensing alone and implications for the Hubble tension
• Constraints on decaying early modified gravity from cosmological observations
• The simplest parametrization of equation of state parameter in the scalar field Universe
• New Early Dark Energy as a solution to the $H_0$ and $S_8$ tensions
• Pseudoscalar sterile neutrino self-interactions in light of Planck, SPT and ACT data
• Thermal axions with multi-eV masses are possible in low-reheating scenarios
• A brief review on cosmological analysis of galaxy surveys with multiple tracers
• A novel CMB polarization likelihood package for large angular scales built from combined WMAP and Planck LFI legacy maps
• Scalar-Tensor Gravity and DESI 2024 BAO data
• Compressed baryon acoustic oscillation analysis is robust to modified-gravity models
• The clustering of critical points in the evolving cosmic web
• The effect of different observational data on the constraints of cosmological parameters
• Dark energy versus modified gravity: Impacts on measuring neutrino mass
• Phase space analysis of the bouncing universe with stringy effects
• Data Compression and Inference in Cosmology with Self-Supervised Machine Learning
• Improving cosmological parameter estimation with the future 21 cm observation from SKA
• Viscous universe with cosmological constant
• Observational constraints on the interacting dark energy - dark matter (IDM) cosmological models
• Study of parametrized dark energy models with a general non-canonical scalar field
• Modeling the large-scale power deficit with smooth and discontinuous primordial spectra
• Unitarity at the Late time Boundary of de Sitter
• Reconstructing Quintessence
• General dynamical properties of cosmological models with nonminimal kinetic coupling
• Probing the Neutrino Mass Hierarchy beyond $\Lambda$CDM Model
• Phenomenological Gravitational Phase Transition: Reconciliation between the Late and Early Universe
• Constraints on running vacuum model with $H(z)$ and $f{\sigma }_8$
• The Clustering Of Galaxies Around Radio-Loud AGNs
• Using Lagrangian perturbation theory for precision cosmology
• Model-independent cosmological inference after the DESI DR2 data with improved inverse distance ladder
• Cosmological parameter estimation from CMB and X-ray clusters after Planck
• An exponential equation of state of dark energy in the light of 2018 CMB Planck data
• Dark Energy Survey Year 3 Results: Measurement of the Baryon Acoustic Oscillations with Three-dimensional Clustering
• Current constraints on cosmological scenarios with very low reheating temperatures
• Observable Predictions for Massive-Neutrino Cosmologies with Model-Independent Dark Energy
• Latest data constraint of some parameterized dark energy models
• Phenomenological Gravitational Phase Transition: Early and Late Modifications
• Quintessence versus phantom dark energy: the arbitrating power of current and future observations
• Comparison of cosmological models using standard rulers and candles
• Diagnostic and Comparative Analysis of Dark Energy Models with $q(z)$ Parametrizations
• On general features of warm dark matter with reduced relativistic gas
• Dark Energy Constraints in light of Pantheon SNe Ia, BAO, Cosmic Chronometers and CMB Polarization and Lensing Data
• Parameter estimation of eccentric gravitational waves with a decihertz observatory and its cosmological implications
• Towards alleviating the $H_0$ and $S_8$ tensions with Early Dark Energy - Dark Matter drag
• Updating constraints on phantom crossing $f(T)$ gravity
• Quintessence-like features in the late-time cosmological evolution of $f(Q)$ symmetric teleparallel gravity
• To curve, or not to curve: Is curvature-assisted quintessence observationally viable?
• A novel model-marginalized cosmological bound on the QCD axion mass
• Probing the Seesaw Mechanism with Cosmological Data
• On the effect of the degeneracy between w_0 and w_a
• Observational constraints on soft dark energy and soft dark matter: challenging $\Lambda$CDM
• Cosmological constraints on the new holographic dark energy model with action principle
• The Swampland Conjectures and Slow-Roll Thawing Quintessence
• Current constraints on early and stressed dark energy models and future 21 cm perspectives
• Roles of Modified Chaplygin-Jacobi and Chaplygin-Abel Gases in FRW Universe
• Observational constraints on dark energy cosmological model parameters
• Effect of model-dependent covariance matrix for studying Baryon Acoustic Oscillations
• Redshift Space Distortion of 21cm line at 1<z<5 with Cosmological Hydrodynamic Simulations
• Differentiating dark interactions with perturbation
• Growth of perturbations in dark energy parametrization scenarios
• Electron mass variation from dark sector interactions and compatibility with cosmological observations
• Forbidden Scalar Dark Matter and Dark Higgses
• Phantom crossing dark energy in Horndeski's theory
• Hubble tension as a window on the gravitation of the dark matter sector
• Dark energy reconstructions combining BAO data with galaxy clusters and intermediate redshift catalogs
• Is the $W$-boson mass enhanced by the axion-like particle, dark photon, or chameleon dark energy?
• A cosmic glitch in gravity
• Tight $H_0$ constraint from galaxy redshfit surveys: combining baryon acoustic osillation measurements and Alcock-Paczynski test
• Which Fundamental Constants for CMB and BAO?
• Revisiting progenitor-age dependence of type Ia supernova luminosity standardization process
• Cosmological bound on neutrino masses in the light of $H_0$ tension
• The redshift-space galaxy two-point correlation function and baryon acoustic oscillations
• A preference for dynamical phantom dark energy using one-parameter model with Planck, DESI DR1 BAO and SN data
• Volume Statistics as a Probe of Large-Scale Structure
• Forecasts on interacting dark energy with standard sirens
• Baryon Physics and Tight Coupling Approximation in Boltzmann Codes
• Gravitational Waves: A Test for Modified Gravity
• Tachyon inflation in the Large-$N$ formalism
• Testing averaged cosmology with type Ia supernovae and BAO data
• Is the CMB telling us that dark matter is weaker than weakly interacting?
• The QCD Axion: Some Like It Hot
• A comparison between axion-like and power law potentials in cosmological background
• Possible dark energy imprints in gravitational wave spectrum of mixed neutron-dark-energy stars
• Growth of structures using redshift space distortion in $f(T)$ Cosmology
• Phase Space description of Nonlocal Teleparallel Gravity
• Exploring Mirror Twin Higgs Cosmology with Present and Future Weak Lensing Surveys
• Cosmological constraint on Brans-Dicke Model
• Type Ia supernovae data with scalar-tensor gravity
• A critical assessment of some inhomogeneous pressure Stephani models
• Clustering with general photo-$z$ uncertainties: Application to Baryon Acoustic Oscillations
• Cosmic Growth in $f(T)$ Teleparallel Gravity
• Forecast constraints on Anisotropic Stress in Dark Energy using gravitational-waves
• Testing distance duality with CMB anisotropies
• Constraining quantum collapse inflationary models with current data: The semiclassical approach
• FLRW accelerating universe with interactive dark energy
• The tension on the cosmological parameters from different observational data
• Neutrino footprint in Large Scale Structure
• Primordial power spectrum features in phenomenological descriptions of inflation
• A first model-independent radial BAO constraint from the final BOSS sample
• Theoretical and observational constraints on Tachyon Inflation
• Constraints from High-Precision Measurements of the Cosmic Microwave Background: The Case of Disintegrating Dark Matter with $\Lambda$ or Dynamical Dark Energy
• Constraints on Modified Gravity from ACT and SPT
• Distance Probes of Dark Energy
• Estimating the uncorrelated dark energy evolution in the Planck era
• Building a digital twin of a luminous red galaxy spectroscopic survey: galaxy properties and clustering covariance
• A new parametrization for dark energy density and future deceleration
• From 100 kpc to 10 Gpc: Dark Matter self-interactions before and after DESI
• Observational constraints to a phenomenological $f\left(R,\nabla R\right)$-model
• Investigating dark energy by electromagnetic frequency shifts
• Momentum transfer in the dark sector and lensing convergence in upcoming galaxy surveys
• Determination of cosmic curvature independent of the sound horizon and $H_0$ using BOSS/eBOSS and DESI DR1 BAO observations
• Eliminating polarization leakage effect for neutral hydrogen intensity mapping with deep learning
• Isocurvature perturbations and tensor mode in light of Planck and BICEP2
• Linear and non-linear perturbations in dark energy models
• Pantheon+ constraints on dark energy and modified gravity: An evidence of dynamical dark energy
• Cluster counts III. $\Lambda$CDM extensions and the cluster tension
• Hints of Neutrino Dark Matter scattering in the CMB? Constraints from the Marginalized and Profile Distributions
• Brane inflation and the robustness of the Starobinsky inflationary model
• Kinetically Coupled Scalar Fields Model and Cosmological Tensions
• Is dark energy evolving?
• Reducing the $H_0$ Tension with Exponential Acoustic Dark Energy
• A low Hubble Constant from galaxy distribution observations
• Vainshtein Screening in Bimetric Cosmology
• Cosmology of an Axion-Like Majoron
• Barrow entropic Quintessence and Dilation dark energy Models with Generalized HDE cut-off
• Late time acceleration in a slow moving galileon field
• Towards realistic $f(T)$ models with nonminimal torsion-matter coupling extension
• Constraining dark sector perturbations I: cosmic shear and CMB lensing
• Improving Dark Energy Constraints with High Redshift Type Ia Supernovae from CANDELS and CLASH
• The redshift dependence of Alcock-Paczynski effect: cosmological constraints from the current and next generation observations
• A single parameterization for dark energy and modified gravity models
• A model independent parametrization of the late time cosmic acceleration: constraints on the parameters from recent observations
• A GREAT model comparison against the cosmological constant
• Constraints on interacting dark energy revisited: implications for the Hubble tension
• Redshift Weights for Baryon Acoustic Oscillations : Application to Mock Galaxy Catalogs
• Discrepancy between cosmological and electroweak observables in Higgs Inflation
• The impact and mitigation of broad absorption line quasars in Lyman$-\alpha$ forest correlations
• Bayesian evidence of non-standard inflation: isocurvature perturbations and running spectral index
• Generalized Brans-Dicke theories in light of evolving dark energy
• Measurement of the matter-radiation equality scale using the extended Baryon Oscillation Spectroscopic Survey Quasar Sample
• Growth of non-linear structures and spherical collapse in the Galileon Ghost Condensate model
• Exact Solutions and Accelerating Universe in Modified Brans-Dicke Theories
• An FLRW interacting dark energy model of the Universe
• Reconstructing Probability Distributions with Gaussian Processes
• Probing cosmic acceleration by strong gravitational lensing systems
• Observational status of the Galileon model general solution from cosmological data and gravitational waves
• Constraints on single-field inflation with WMAP, SPT and ACT data -- A last-minute stand before Planck
• $f(T)$ cosmology in the regime of quasar observations
• Revisiting signatures of thermal axions in nonstandard cosmologies
• FRW dark energy cosmological model with hybrid expansion law
• Confronting brane inflation with Planck and pre-Planck data
• ISiTGR: Testing deviations from GR at cosmological scales including dynamical dark energy, massive neutrinos, functional or binned parametrizations, and spatial curvature
• Constraining power of open likelihoods, made prior-independent
• Measuring the spectral running from cosmic microwave background and primordial black holes
• The cosmic transparency measured with Type Ia supernovae: implications for intergalactic dust
• Early dark energy constraints with late-time expansion marginalization
• No evidence for the evolution of mass density power-law index $\gamma$ from strong gravitational lensing observation
• Forecast and analysis of the cosmological redshift drift
• The ESO's VLT Type Ia supernova spectral set of the final two years of SNLS
• Local probes strongly favor $\Lambda$CDM against power-law and $R_h=ct$ universe
• Holographic energy density, dark energy sound speed, and tensions in cosmological parameters: $H_0$ and $S_8$
• Multipole expansion for 21cm Intensity Mapping power spectrum: forecasted cosmological parameters estimation for the SKA Observatory
• Does the fraction of dark matter diminish with early dark energy?
• Redshift drift constraints on f(T) gravity
• Constraining thawing and freezing models with cluster number counts
• Finding structure in the dark: coupled dark energy, weak lensing, and the mildly nonlinear regime
• Clustering in the Simulated H$\alpha$ Galaxy Redshift Survey from Nancy Grace Roman Space Telescope
• Screening Mechanism and Late-time Cosmology: Role of a Chameleon-Brans-Dicke Scalar Field
• Cosmic Voids in Evolving Dark Sector Cosmologies: the Low Redshift Universe
• Constraining dark sector perturbations II: ISW and CMB lensing tomography
• Reconstructing a non-linear interaction in the dark sector with cosmological observations
• Shell-like structures in our cosmic neighbourhood
• Dynamics and statefinder analysis of a class of sign-changeable interacting dark energy scenarios
• Non-thermal neutrino-like hot dark matter in light of the $S_8$ tension
• Optimal Weights For Measuring Redshift Space Distortions in Multi-tracer Galaxy Catalogues
• Cosmological fluids in the equivalence between Rastall and Einstein gravity
• Space-borne atom interferometric gravitational wave detections. Part I. The forecast of bright sirens on cosmology
• Cosmological constraints of Palatini $f(\mathcal{R})$ gravity
• Consistency of nonlinear interacting ghost dark energy with recent observations
• The interaction of neutrinos with Phantom, Quintessence, and Quintum scalar fields and its effect on the formation of structures in the early Universe
• How CMB and large-scale structure constrain chameleon interacting dark energy
• Observational constraints on the fractal cosmology
• Constraints on interacting dynamical dark energy and a new test for $\Lambda$CDM
• Impact of the latest measurement of Hubble constant on constraining inflation models
• Confronting Dark Energy Anisotropic Stress
• HI intensity mapping with MeerKAT: forecast for delay power spectrum measurement using interferometer mode
• Testing the nature of Dark Energy with Precision Cosmological constraints
• Forecasting cosmological parameter constraints from near-future space-based galaxy surveys
• Reconstructing the Hubble parameter with future Gravitational Wave missions using Machine Learning
• Spatial curvature sensitivity to local $H_0$ from the Cepheid distance ladder
• A visual tool for assessing tension-resolving models in the $H_0$-${\sigma }_8$ plane
• Harmonic Hybrid Inflation
• Weighing neutrinos in $f(R)$ gravity in light of BICEP2
• A Reconstruction of Quintessence Dark Energy
• Dark Energy Survey: Galaxy Sample for the Baryonic Acoustic Oscillation Measurement from the Final Dataset
• Imprint of a Steep Equation of State in the growth of structure
• Light mass galileon and late time acceleration of the Universe
• Dark Matter in Fractional Gravity I: Astrophysical Tests on Galactic Scales
• Observation constraints on scalar field cosmological model in Anisotropic universe
• Constraints on a special running vacuum model
• Constraints on brane inflation after Planck 2015: Impacts of the latest local measurement of the Hubble constant
• HI intensity mapping correlation function from UNIT simulations: BAO and observationally induced anisotropy
• Cosmic acceleration from coupling of baryonic and dark matter components: Analysis and diagnostics
• Cosmic Variation of Proton to Electron Mass Ratio with an interacting Higgs Scalar Field
• Constraining the emergent dark energy models with observational data at intermediate redshift
• Exploring the Cosmological Model in $f(R,T^{\varphi })$ Gravity with Observational Constraints
• Cosmic Voids in Evolving Dark Sector Cosmologies: the High Redshift Universe
• Probing alternative cosmologies through the inverse distance ladder
• Forecasts of cosmological constraints from HI intensity mapping with FAST, BINGO & SKA-I
• Quantifying effects of inhomogeneities and curvature on gravitational wave standard siren measurements of $H(z)$
• First constraints on non-minimally coupled Natural and Coleman-Weinberg inflation and massive neutrino self-interactions with Planck+BICEP/Keck
• $f(T,B)$ Gravity in the late Universe in the context of local measurements
• How accurately can we measure the baryon acoustic oscillation feature?
• A More Accurate Parameterization based on cosmic Age (MAPAge)
• The effect of inhomogeneities on dark energy constraints
• Cosmological N-body simulations with generic hot dark matter
• Cornering (quasi) degenerate neutrinos with cosmology
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: constraints on the time variation of fundamental constants from the large-scale two-point correlation function
• DBI Galileon and Late time acceleration of the universe
• Explanation of high redshift luminous galaxies from JWST by early dark energy model
• Observationally constrained accelerating cosmological model with higher power of non-metricity and squared trace
• A power-law coupled three-form dark energy model
• Do we need wavelets in the late Universe?
• Quintessential early dark energy
• Using large scale structure data and a halo model to constrain Generalised Dark Matter
• Cosmological constraints on $\gamma$-gravity models
• The failure of testing for cosmic opacity via the distance-duality relation
• Shan--Chen interacting vacuum cosmology
• Constraints On Dark Energy Models From Galaxy Clusters and Gravitational Lensing Data
• Bulk viscous matter in $f(T)$ gravity: A path to cosmic acceleration
• Constraints on Brane-World Inflation from the CMB Power Spectrum: Revisited
• Cosmology With Axionic-quintessence Coupled with Dark Matter
• Constraining Holographic Dark Energy and Analyzing Cosmological Tensions
• A PAge-like Unified Dark Fluid Model
• Cosmological effects of the Galileon term in Scalar-Tensor Theories
• Signatures of Light Massive Relics on nonlinear structure formation
• Running cosmological constant with observational tests
• Prospects for weighing neutrinos in interacting dark energy models using joint observations of gravitational waves and $\gamma$-ray bursts
• The H0 trouble: Confronting Non-thermal Dark Matter and Phantom Cosmology with the CMB, BAO, and Type Ia Supernovae data
• Decaying dark energy in light of the latest cosmological dataset
• Future evolution in a backreaction model and the analogous scalar field cosmology
• Observational Constraints on the Dark Energy with a Quadratic Equation of State
• Detecting baryon acoustic oscillations by 3d weak lensing
• Testing the consistency between cosmological measurements of distance and age
• Comprehensive Constraints on Dark Radiation Injection After BBN
• Dissecting kinetically coupled quintessence: phenomenology and observational tests
• 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
• Probing cosmology with weak lensing selected clusters II: Dark energy and f(R) gravity models
• Fast, large volume, GPU enabled simulations for the Ly-alpha forest: power spectrum forecasts for baryon acoustic oscillation experiments
• Evidence of dark energy in different cosmological observations
• Cosmological tests of gravity with latest observations
• Late-time acceleration with steep exponential potentials
• No stable dissipative phantom scenario in the framework of a complete cosmological dynamics
• Scaling solutions as Early Dark Energy resolutions to the Hubble tension
• Late Time Modification of Structure Growth and the S8 Tension
• Analytical growth functions for cosmic structures in a $\Lambda$CDM Universe
• Bulk viscous fluid in symmetric teleparallel cosmology: theory versus experiment
• 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
• Hubble tension as a window on the gravitation of the dark matter sector: Exploration of a family of models
• Constraints on Dark Matter-Photon Coupling in the Presence of Time-Varying Dark Energy
• Coupled dark energy model inspired from general conformal transformation
• Self-interacting neutrinos, the Hubble parameter tension, and the Cosmic Microwave Background
• The interacting vacuum and tensions: a comparison of theoretical models
• Cosmological constraints with the Effective Fluid approach for Modified Gravity
• Roles of sterile neutrinos in particle physics and cosmology
• No evidence for EDE from Planck data in extended scenarios
• Exploring cosmological imprints of phantom crossing with dynamical dark energy in Horndeski gravity
• Can a void mimic the $\Lambda$ in $\Lambda$CDM?
• The Tilt of Primordial Gravitational Waves Spectra from BICEP2
• Constraining non-minimally coupled $\beta$-exponential inflation with CMB data
• Dark-energy dependent test of general relativity at cosmological scales
• Testing Modified Gravity theory (MOG) with Type Ia Supernovae, Cosmic Chronometers and Baryon Acoustic Oscillations
• Revisit of constraints on dark energy with Hubble parameter measurements including future redshift drift observations
• Cosmological models with running cosmological term and decaying dark matter
• A thermodynamic point of view on dark energy models
• Cosmological Boundary Flux Parameter
• Optimal prior for Bayesian inference in a constrained parameter space
• Constraints on sterile neutrinos and the cosmological tensions
• Distance-duality in theories with a nonminimal coupling to gravity
• Coupled Dark Sector Models and Cosmological Tensions
• Real-time cosmology with SKA
• On the concordance of cosmological data in the case of the generalized Chaplygin gas
• How does pressure gravitate? Cosmological constant problem confronts observational cosmology
• Study in the noncanonical domain of Goldstone inflation
• Domain Wall Network: A Dual Solution for Gravitational Waves and Hubble Tension?
• Cosmology and CPT violating neutrinos
• Gravitational waves, CMB polarization, and the Hubble tension
• Bound Dark Energy: towards understanding the nature of the Dark Energy
• The CMB neutrino mass / vacuum energy degeneracy: a simple derivation of the degeneracy slopes
• Bayesian Comparison of Interacting Modified Holographic Ricci Dark Energy Scenarios
• On fast Generation of Cosmological Random Fields
• Dynamical dark energy in light of cosmic distance measurements II: a study using current observations
• Sound-Horizon-Agnostic Inference of the Hubble Constant and Neutrino Mass from BAO, CMB Lensing, and Galaxy Weak Lensing and Clustering
• WALLABY Pilot Survey: HI gas kinematics of galaxy pairs in cluster environment
• Model Selection with Baryonic Acoustic Oscillations in the Lyman-alpha Forest
• Cosmological constraints from the redshift dependence of the volume effect using the galaxy 2-point correlation function across the line-of-sight
• Decaying Vacuum Inflationary Cosmologies: A Complete Scenario Including Curvature Effects
• Detecting Baryon Acoustic Oscillations with third generation gravitational wave observatories
• Reheating constraints to WIMPflation
• Distinguish the $f(T)$ model from $\Lambda$CDM model with Gravitational Wave observations
• Viable dark energy models using pseudo-Nambu-Goldstone bosons
• Is there another coincidence problem at the reionization epoch?
• Cosmological Constraints on Thermal Friction of Axion Dark Matter
• Cosmological surveys with multi-object spectrographs
• Low-Redshift Constraints on Covariant Canonical Gauge Theory of Gravity
• Interacting dark energy constraints from the full-shape analyses of BOSS DR12 and DES Year 3 measurements
• Aether-quasi-dilaton massive gravity
• Running vacuum model in non-flat universe
• Cosmology with a Continuous Tower of Scalar Fields
• Constraints on Cosmological Models from Hubble Parameters Measurements
• Emission-line Stacking of 21cm Intensity Maps with MeerKLASS: Inference Pipeline and Application to the L-band Deep-field Data
• Large-Distance Lens Uncertainties and Time-Delay Measurements of $H_0$
• Constraints on the Spacetime Dynamics of an Early Dark Energy Component
• Exploring evidence of interaction between dark energy and dark matter
• External priors for the next generation of CMB experiments
• Cosmological constraints on ultra-light axion fields
• Probing the Weak Gravity Conjecture in the Cosmic Microwave Background
• Reconstructions of $f(\mathcal{P})$ and $f(\mathcal{Q})$ gravity models from $(m,n)$-type Barrow Holographic Dark Energy: Analysis and Observational Constraints
• Potentialities of Hubble parameter and expansion rate function data to alleviate Hubble tension
• Determining $H_0$ using a model-independent method
• Cosmology of Dirac-Born-Infeld dRGT massive gravity
• Can we distinguish early dark energy from a cosmological constant?
• Testing the consistency of early and late cosmological parameters with BAO and CMB data
• Hidden from view: Coupled Dark Sector Physics and Small Scales
• Direct geometrical measurement of the Hubble constant from galaxy parallax: predictions for the Vera C. Rubin Observatory and Nancy Grace Roman Space Telescope
• Coupled Quintessence scalar field model in light of observational datasets
• Deep Learning and genetic algorithms for cosmological Bayesian inference speed-up
• Cosmological implications of different baryon acoustic oscillation data
• Can acoustic and axion-like early dark energy still resolve the Hubble tension?
• Computing 3 point correlation function randoms counts without the randoms catalogue
• Cosmological Constraints using the newest VLT-KMOS HII Galaxies and the full Planck CMB spectrum
• BullFrog: Multi-step perturbation theory as a time integrator for cosmological simulations
• Implications for cosmology from Ground-based Cosmic Microwave Background observations
• What have we learned from observational cosmology ?
• Interacting parametrized post-Friedmann method
• The viable f(G) gravity models via reconstruction from the observations
• Euclid: Testing the Copernican principle with next-generation surveys
• Constraining Cosmological Parameters with Viscous Modified Chaplygin Gas and Generalized Cosmic Chaplygin Gas Models in Horava-Lifshitz Gravity: Utilizing Late-time Datasets
• Cosmological bounds on neutrino statistics
• Forecasting cosmological constraints from age of high-z galaxies
• Axi-Higgs cosmology: Cosmic Microwave Background and cosmological tensions
• Constraining cosmological scaling solutions of a Galileon field
• Thermal WIMPs and the Scale of New Physics: Global Fits of Dirac Dark Matter Effective Field Theories
• Investigating the dynamical models of cosmology with recent observations and upcoming gravitational-wave data
• Tachyonic vs Quintessence dark energy: linear perturbations and CMB data
• Late-Time Anisotropy Sourced by a 2-Form Field Non-Minimally Coupled to Cold Dark Matter
• Thawing k-essence dark energy in the PAge space
• Singling out modified gravity parameters and datasets reveals a dichotomy between Planck and lensing
• Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
• A coupled generalized three-form dark energy model
• Perturbation Theory Remixed: Improved Nonlinearity Modeling beyond Standard Perturbation Theory
• Renormalization group and UV completion of cosmological perturbations: Gravitational collapse as a critical phenomenon
• Constraints on Late Time Violations of the Equivalence Principle in the Dark Sector
• Growth and Geometry Split in Light of the DES-Y3 Survey
• Non-linear Structure Formation for Dark Energy Models with a Steep Equation of State
• A new method to test the cosmic distance duality relation using the strongly lensed gravitational waves
• Constraints on dark energy from TDCOSMO & SLACS lenses
• Lower tensor-to-scalar ratio as possible signature of modified gravity
• The measurements of matter density perturbations amplitude from cosmological data
• cp3-bench: A tool for benchmarking symbolic regression algorithms tested with cosmology
• 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
• Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos
• Beyond $\Lambda$CDM: Exploring a Dynamical Cosmological Constant Framework Consistent with Late-Time Observations
• Investigating the $w$CDM Model with Latest DESI BAO Observations
• Smoothing the redshift distributions of random samples for the baryon acoustic oscillations : applications to the SDSS-III BOSS DR12 and QPM mock samples
• Scalar Dark Energy Models and Scalar-Tensor Gravity: Theoretical Explanations for the Accelerated Expansion of Present Universe
• Constraining modified gravity scenarios with the 6dFGS and SDSS galaxy peculiar velocity datasets
• On Dark Gravitational Wave Standard Sirens as Cosmological Inference and Forecasting the Constraint on Hubble Constant using Binary Black Holes Detected by Deci-hertz Observatory
• Analysis cosmological tachyon and fermion model and observation data constraints
• Surface Tension: Accelerated Expansion, Coincidence Problem & Hubble Tension
• Observational constraints on running vacuum model
• Flatness without CMB - the Entanglement of Spatial Curvature and Dark Energy Equation of State
• Constraints on the $\Lambda$CDM model with redshift tomography
• Reconciling BICEP2 and Planck results with right-handed Dirac neutrinos in the fundamental representation of grand unified E_6
• Re-examining the role of curvature in the slowing down acceleration scenario
• Evolution of linear perturbations in Lemaître-Tolman-Bondi void models
• Constraining the Lattice Fluid Dark Energy from SNe Ia, BAO and OHD
• 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
• Cosmological constant constraints from observation-derived energy condition bounds and their application to bimetric massive gravity
• A solution to the S8 tension through neutrino-dark matter interactions
• Investigating the Possibility of a Turning Point in the Dark Energy Equation of State
• Beyond dark energy Fisher forecasts: how DESI will constrain LCDM and quintessence models
• Constraining dark energy using observational growth rate data
• Dark energy-dark matter interactions as a solution to the $S_8$ tension
• Cosmic Acceleration in an Extended Brans-Dicke-Higgs Theory
• Measuring H0 from the 6dF Galaxy Survey and future low-redshift surveys
• Baryon acoustic oscillations from HI intensity mapping: the importance of cross-correlations in the monopole and quadrupole
• Modern Cosmology: Interactive Computer Simulations that use Recent Observational Surveys
• Scalar field dark energy: Insights into cosmological evolution and black hole accretion
• Constraining neutrino mass in dynamical dark energy cosmologies with the logarithm parametrization and the oscillating parametrization
• Holographic Dark Energy from the Anti-de Sitter Black Hole
• The Two-Point Correlation Function of Gamma-ray Bursts
• Higgs Inflation: constraining the top quark mass and breaking the $H_0$-${\sigma }_8$ correlation
• Fisher forecast for the BAO measurements from the CSST spectroscopic and photometric galaxy clustering
• Baryon acoustic oscillations with the cross-correlation of spectroscopic and photometric samples
• Dynamics of dark energy in the gravitational fields of matter inhomogeneities
• Addressing the $r_d$ Tension using Late-Time Observational Measurements in a Novel deceleration Parametrization
• Nonlinear structure formation in Bound Dark Energy
• Holographic dark information energy: Predicted dark energy measurement
• A New Probe of the High-z BAO scale: BAO tomography With CMB $\times$ LIM-Nulling Convergence
• Scrutinizing coupled vector dark energy in light of data
• Possible Impact of non-Gaussianities on cosmological constraints in neutrino physics
• Novel aspects of C-theories in Cosmology
• Endowing $\mathbf{\Lambda }$ with a dynamic nature: constraints in a spatially curved Universe
• Elucidating Dark Energy with Future 21 cm Observations at the Epoch of Reionization
• Cosmological constraints on $\Lambda (\alpha )$CDM models with time-varying fine structure constant
• Baryon acoustic scale at $z_{\eff} = 0.166$ with the SDSS blue galaxies
• A new parametrization of Hubble function and Hubble tension
• Observational constraints to a unified cosmological model
• Scalar-tensor extension of the $\Lambda$CDM model
• Automated reliability assessment for spectroscopic redshift measurements
• Measuring the scalar induced gravitational waves from observations
• Cosmological test of an extended quintessence model
• Brane inflation driven by an arctan potential: CMB constraints and Reheating
• Thermodynamics of Modified Chaplygin-Jacobi Gas and Modified Chaplygin-Abel Gas: Stability Analysis and Observational Constraints
• Phenomenological models of Universe with varying $G$ and $\Lambda$
• Quintessence scalar field and cosmological constant: Dynamics of a multi-component dark energy model
• Redshift-space distortion constraints on the neutrino mass and models to alleviate the Hubble tension
• Super-Eddington accreting massive black holes explore high-$z$ cosmology: Monte-Carlo simulations
• Towards a sound massive cosmology
• Gravitational wave probes of Barrow cosmology with LISA standard sirens
• Constraining hybrid potential scalar field cosmological model in Lyra's geometry with recent observational data
• A Study of Selection Methods for H alpha Emitting Galaxies at z~1.3 for the Subaru/FMOS Galaxy Redshift Survey for Cosmology (FastSound)
• A new way to test the WIMP dark matter models
• Relaxing cosmological constraints on current neutrino masses
• Signatures of Very Early Dark Energy in the Matter Power Spectrum
• Dark Energy with a Triplet of Classical U(1) Fields
• Growth of cosmic perturbations in the modified $f(R,T)$ gravity
• Probing cosmology via the clustering of critical points
• Equality scale-based and sound horizon-based analysis of the Hubble tension
• Testing Dvali-Gabadadze-Porrati Gravity with Planck
• Reconstructing the dark matter and dark energy interaction scenarios from observations
• Redshift evolution of the Hubble constant: Constraints and new insights from an interacting dark energy model
• Observational Constraints on Extended Starobinsky and Weyl Gravity Model of Inflation
• Bayesian deep learning for dark energy
• Impact of dark energy on the equation of state in light of the latest cosmological data
• Observational constraints on dynamical dark energy with pivoting redshift
• Observational Constraints on the Parameters of Hořava-Lifshitz Gravity
• Effects of Dark Energy anisotropic stress on the matter power spectrum
• Type Ia supernova constraints on compact object dark matter
• 2D BAO vs 3D BAO: Hints for new physics?
• Dynamical Dark Energy and the Unresolved Hubble Tension: Multi-model Constraints from DESI 2025 and Other Probes
• The environmental dependence of the baryon acoustic peak in the Baryon Oscillation Spectroscopic Survey CMASS sample
• Constraints on Metastable Dark Energy Decaying into Dark Matter
• Constraints on Dark Energy from New Observations including Pan-STARRS
• Hint of dark matter-dark energy interaction in DESI DR2 and current cosmological dataset?
• Spatial variation of fundamental constants: testing models with thermonuclear supernovae
• On the $2^{\text{nd}}$ feature of the matter two-point function
• Dark matter component decaying after recombination: constraints from diffuse gamma-ray and neutrino flux measurements
• Deep learning for cosmological parameter inference from a dark matter halo density field
• Perturbation in an interacting dark universe
• Early dark energy in the pre- and post-recombination epochs
• Cosmic Reionization Study : Principle Component Analysis After Planck
• Averaged universe confronted with cosmological observations: A fully covariant approach
• A closer look at the cosmological implications of the $\Lambda$HDE model
• Exploring the Evolution of Nonlinear Electrodynamics in the Universe: A Dynamical Systems Approach
• New measures to test modified gravity cosmologies
• The consistency test on the cosmic evolution
• Cosmological Signatures of Dark Sector Physics: The Evolution of Haloes and Spin Alignment
• Constraints on the varying electron mass and early dark energy in light of ACT DR6 and DESI DR2 and the implications for inflation
• Hints of the $H_0-r_d$ tension in uncorrelated Baryon Acoustic Oscillations dataset
• Multi-messenger standard-siren cosmology for third-generation gravitational-wave detectors: forecasts considering observations of gamma-ray bursts and kilonovae
• A glitch in gravity: cosmic Lorentz-violation from fiery Big Bang to glacial heat death
• Reconstruction of energy conditions from observations and implications for extended theories of gravity
• Reconstructions of Einstein-Aether Gravity from Barrow Agegraphic and New Barrow Agegraphic Dark Energy models: Examinations and Observational Limits
• Detection significance of Baryon Acoustic Oscillations peaks in galaxy and quasar clustering
• Modified $f(R,T)$ theory in light of gravitational wave standard sirens
• Discerning Dark Energy Models with High-Redshift Standard Candles
• Analytic Study of Cosmological Perturbations in a Unified Model of Dark Matter and Dark Energy with a Sharp Transition
• Prospects for cosmological research with the FAST array: 21-cm intensity mapping survey observation strategies
• Testing and selecting cosmological models with ultra-compact radio quasars
• Cosmology and the Dark Matter Frontier
• Oscillating solutions of the matter density contrast in Horndeski's theory
• Dark Matter-Radiation Scattering Enhances CMB Phase Shift through Dark Matter-loading
• Data Analysis and Phenomenological Cosmology
• Sound Horizon Independent Constraints on Early Dark Energy: The Role of Supernova Data
• Improving SDSS cosmological constraints through $\beta$-skeleton weighted correlation functions
• Weak Lensing Constraints on Dark Matter-Baryon Interactions with $N$-Body Simulations and Machine Learning
• Cool dark sector, concordance, and a low ${\sigma }_8$
• Local Limit of Nonlocal Gravity: Cosmological Perturbations
• Cosmology on a Gravitational Wave Background
• Angular Correlation Function from sample covariance with BOSS and eBOSS LRG
• Constraining primordial vector mode from B-mode polarization
• Distance Duality Test: The Evolution of Radio Sources Mimics a Nonexpanding Universe
• Constraints on the non-minimally coupled Witten-O'Raifeartaigh inflation
• Role of Future SNIa Data from Rubin LSST in Reinvestigating Cosmological Models
• Mass-Dependent Baryon Acoustic Oscillation Signal and Halo Bias
• Local Limit of Nonlocal Gravity: A Teleparallel Extension of General Relativity
• Satellite Content and Halo Mass of Galaxy Clusters: Comparison between Red-Sequence and Halo-based Optical Cluster Finders
• Allan Sandage and the Distance Scale
• Improvements in cosmological constraints from breaking growth degeneracy
• Constraints on the phase transition of Early Dark Energy with the CMB anisotropies
• Mass assembly history of dark matter halos in the light of $H_0$ tension
• Voids and Halos in Voids statistics as a probe of the Expansion History of the Universe
• Updated reduced CMB data and constraints on cosmological parameters
• Cosmological Standard Timers from Unstable Primordial Relics
• The Low Redshift survey at Calar Alto (LoRCA)
• Implications of Dynamical Dark Energy in the expansion of the Universe and the Structure Formation
• Phenomenological power spectrum models for H$\alpha$ emission line galaxies from the Nancy Grace Roman Space Telescope
• Common Origin of Warm Dark Matter and Dark Radiation
• The dark Stodolsky effect: constraining effective dark matter operators with spin-dependent interactions
• Observational constraints in late time for an axially symmetric transitioning model with bulk viscous fluid
• Observational Constraints on the Cosmology with Holographic Dark Fluid
• Probing the independence within the dark sector in the fluid approximation
• Testing the coupling of dark radiations in light of the Hubble tension
• Lensing convergence and anisotropic dark energy in galaxy redshift surveys
• $g_{\mathrm{NL}}$ in the curvaton model constrained by PLANCK
• An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$
• Equivalence of Dark Energy Models: A Theoretical and Bayesian Perspective
• Influence of the correlation prior on reconstruction of the dark energy equation of state
• Anisotropic cosmology using observational datasets: exploring via machine learning approaches
• Action functional of the Cardassian universe
• Constraining Chaplygin models using diffuse supernova neutrino background
• Baryon acoustic oscillations from a joint analysis of the large-scale clustering in Fourier and configuration space
• Realising effective theories of tribrid inflation: Are there effects from messenger fields?
• Cosmological Perturbations in the 5D Holographic Big Bang Model
• A frequentist view on the two-body decaying dark matter model
• Late Time Phenomena in $f(T,\mathcal{T})$ Gravity Framework: Role of $H_0$ Priors
• Hubble Expansion as an Einstein Curvature
• Observational constraints and dynamical analysis of Kaniadakis horizon-entropy cosmology
• Anisotropic cosmology in Bumblebee gravity theory
• On the Field Theoretical Description of an Alternative Model to Generalized Chaplygin Gas and its Thermodynamic Behaviour
• Measuring the primordial gravitational waves from cosmic microwave background and stochastic gravitational wave background observations
• A Dynamic Dark Information Energy Consistent with Planck Data
• Quintessence and tachyon dark energy in interaction with dark matter: Observational constraints and model selection
• Cosmological perturbation theory for large scale structure in phase space
• A Semiblind Reconstruction of the History of Effective Number of Neutrinos Using CMB Data
• Non-Affine Extensions of the Raychaudhuri Equation in the K-essence Framework
• Observational constraints on inflationary potentials within the quantum collapse framework
• Reducing the Tension Between the BICEP2 and the Planck Measurements: A Complete Exploration of the Parameter Space
• Observational constraints on cosmological parameters in the Bianchi type III Universe with f(R,T) gravity theory
• A model of the anisotropic correlation function xi(rp, pi) in redshift space including redshift errors
• Constraints on Axions from Cosmic Distance Measurements
• Baryon Acoustic Oscillations analyses with Density-Split Statistics
• Pantheon+ tomography and Hubble tension
• Effects of high-order operators in non-relativistic Lifshitz holography
• Linear perturbations spectra for dynamical dark energy inspired by modified gravity
• Detecting Baryon Acoustic Oscillations in Dark Matter from Kinematic Weak Lensing Surveys
• Measuring the primordial curvature perturbations from the scalar induced gravitational waves
• Baryon Acoustic Oscillations from Integrated Neutral Gas Observations: an instrument to observe the 21cm hydrogen line in the redshift range 0.13 $<$ z $<$ 0.45 -- status update
• $\Lambda CDM$ periodic cosmology
• Reconciling cosmic dipolar tensions with a gigaparsec void
• Updated neutrino mass constraints from galaxy clustering and CMB lensing-galaxy cross-correlation measurements
• Gravitational Lensing of Dark Energy Models and $\Lambda$CDM Using Observational data in Loop Quantum Cosmology
• Cosmological Implications of a Neutrino Mass Detection
• Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints
• Pair Counting without Binning -- A New Approach to Correlation Functions in Clustering Statistics
• Theoretical priors in scalar-tensor cosmologies: Shift-symmetric Horndeski models
• Can cosmic rotation resolve the Hubble tension? Constraints from CMB and large-scale structure
• Improved source classification and performance analysis using Gaia DR3
• A pressure parametric dark energy model
• Role of Spatial Curvature in a Dark Energy Interacting Model
• Cosmological constraints from galaxy multi-tracers in the nearby Universe
• Subdominant Dark Matter sterile neutrino resonant production in the light of Planck
• Non-linear structure formation with elastic interactions in the dark sector
• Constraining Violations of the Weak Equivalence Principle in the Dark Sector
• Dark Energy Survey: DESI-Independent Angular BAO Measurement
• Gravitational Waves in a Closed Spacetime via Deviation Equation
• Constraining LTB models with JLA supernovae and BAO
• Dynamical Dark Energy Signatures from a New Transition $Om(z)$ Parametrization in Flat FLRW Cosmology
• Dark aspects of massive spinor electrodynamics
• A cosmic speed-trap: a gravity-independent test of cosmic acceleration using baryon acoustic oscillations
• Mimetic Tensor-Vector-Scalar Cosmology: Incorporating Dark Matter, Dark Energy and Stiff Matter
• Mimicking the $\Lambda$CDM Universe through inhomogeneous space-time
• Parameter space stability of multiple soft interactions
• Perturbation theory challenge for cosmological parameters estimation II.: Matter power spectrum in redshift space
• Observational constraints on thawing quintessence scalar field model
• A possible geometrical origin of the accelerated expansion of the universe
• Forecasts for cosmological measurements based on the angular power spectra of AGN and clusters of galaxies in the SRG/eROSITA all-sky survey
• Constraints on Multicomponent Dark Energy from Cosmological Observations
• Dark Energy Survey Year 3 Results: Galaxy mock catalogs for BAO analysis
• Observational effects of the early episodically dominating dark energy
• Toward Cosmological Standard Timers in Primordial Black Hole Binaries
• Neutrinos as a probe of curvature
• Can Dark Energy Emerge from a Varying $G$ and Spacetime Geometry?
• Cosmic acceleration sourced by modification of gravity without extra degrees of freedom
• Cuscuton-like contribution to dark energy evolution
• 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
• Cosmological parameter fittings with the BICEP2 data
• Estimating Cosmological Parameters and Reconstructing Hubble Constant with Artificial Neural Networks: A Test with covariance matrix and mock H(z)
• Reconstructing cosmic evolution with a density parametrization
• Toy models of Universe with an Effective varying $\Lambda$-Term in Lyra Manifold
• Modelling the covariance matrix for the power spectra before and after the BAO reconstruction
• Accelerating BAO Scale Fitting Using Taylor Series
• A gigaparsec-scale local void and the Hubble tension
• Some Classes of Interacting Two-Fluid Model of the Expanding Universe
• The equation and solution of 4-point correlation function of galaxies in Gaussian approximation and its parity-odd part
• Dark Energy Survey Year 3 Results: Galaxy Sample for BAO Measurement
• Cosmic Dark Energy Emerging from Gravitationally Effective Vacuum Fluctuations
• A semi-analytic estimate for the effective sound speed counterterm in the EFTofLSS
• On observational signatures of multi-fractional theory
• Observational constraints on massive gravity
• Confronting Einstein Yang Mills Higgs Dark Energy in light of observations
• Dissecting the $H_0$ and $S_8$ tensions with Planck + BAO + supernova type Ia in multi-parameter cosmologies
• Robustness of cosmological axion mass limits
• A step in the right direction? Analyzing the Wess Zumino Dark Radiation solution to the Hubble tension
• Assessing the potential of cluster edges as a standard ruler
• Refitting cosmological data with neutrino mass and degeneracy
• The magnitude of the dark ages 21-cm signal in the context of existing early and late time constraints on $\Lambda$CDM
• Cosmology of Quasi-Dilaton Massive Gravity with Non-minimal Kinetic Coupling
• On the baryon acoustic oscillation amplitude as a probe of radiation density
• Power Suppression and Lensing Anomaly -- A phenomenological investigation
• Faint galaxies in the Zone of Avoidance revealed by JWST/NIRCam
• Motion of the Local Group as a cosmological probe
• Generalized neutrino isocurvature
• A New Paradigm for Testing Gravity: Theory-Independent Constraints Using Data From All Astrophysical and Cosmological Scales
• Ricci-Cubic Holographic Dark Energy: Confronting Observations, Stability and the Cosmic Coincidence Problem
• Constraining decaying dark matter with BOSS data and the effective field theory of large-scale structures
• Dark energy with oscillatory tracking potential: Observational Constraints and Perturbative effects
• Solar System Tests of a New Class of $f(z)$ Theory
• The Cosmological Effect of CMB/BAO Measurements
• Implementing spectra response function approaches for fast calculation of power spectra and bispectra
• Geometry vs growth: Internal consistency of the flat ΛCDM model with KiDS-1000
• Exploring the Universe Expansion History with f(R,T) Gravity: Constraints on Cosmological Parameters
• Does History Repeat Itself? Periodic Time Cosmology
• Production and constraints for a massive dark photon at electron-positron colliders
• Model independent reconstruction of cosmological accelerated-decelerated phase
• Does the Reionization Model Influence the Constraints on Dark Matter Decay or Annihilation?
• Artificial Neural Networks for Galaxy Clustering. Learning from the two-point correlation function of BOSS galaxies
• Cosmological constraints on mass-varying dark matter
• Statistical consistency of sign-switching vacuum energy with cosmological observations
• Checking T and CPT violation with sterile neutrino
• Beyond thermal approximations: Precise cosmological bounds on Axion-Like Particles
• Coupling dark-baryonic matter density profile for vacuum decay scenarios
• The BINGO project X. Cosmological parameter constraints from HI Intensity Mapping lognormal simulations
• Probing the Hubble Tension with an Infinite-Future Condition on the Hubble Parameter
• Fluctuations in the Ginzburg-Landau Theory of Dark Energy: internal (in-)consistencies in PLANCK data set
• Perturbations In Some Dark Energy Models
• A Quantum Genetic Algorithm with application to Cosmological Parameters Estimation
• A Chi-Squared Analysis of the Measurements of Two Cosmological Parameters Over Time
• Exploring the constraints on cosmological models with CosmoEJS
• Enhancing Cosmological Constraints by Two-dimensional $\beta$-cosmic-web Weighted Angular Correlation Functions
• Combining Planck and SPT cluster catalogs: cosmological analysis and impact on Planck scaling relation calibration
• The dynamics of background evolution and structure formation in phase space: a semi-cosmographic reconstruction
• Bayesian evidence and model selection approach for time-dependent dark energy
• Measuring the speed of scalar induced gravitational waves from observations
• Freeze-in Dark Matter via Lepton Portal: Hubble Tension and Stellar Cooling
• Gravitational redshift from large-scale structure: nonlinearities, antisymmetries, and the dipole
• Investigating Graviton Mass Effects on Black Hole Lensing in dRGT Massive Gravity
• Baryon Acoustic Oscillations in tomographic Angular Density and Redshift Fluctuations
• Improved cosmological constraints on the neutrino mass and lifetime
• Running vacuum model versus $\Lambda$CDM -- a Bayesian analysis
• From Geometry to Observation: Gravitational Waves and the Raychaudhuri Equation
• The Lambert $W$ equation of state in light of DESI BAO
• On Generalized Theories of Varying Fine Structure Constant
• Testing the effects from dark radiation
• Probing dark energy with braneworld cosmology in the light of recent cosmological data
• Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension
• Redshift-space distortion from dynamical dark energy with time-dependent Lagrangian perturbation theory
• Gamma-Ray Bursts, Supernovae Ia and Baryon Acoustic Oscillations: a binned cosmological analysis
• Dark Radiation and Inflationary Freedom
• The impact of the locally measured Hubble parameter on the mass of Sterile neutrino
• Recent results and perspectives on cosmology and fundamental physics from microwave surveys
• Cosmological aspects of cubic Galileon massive gravity
• Effective $\Lambda$CDM model emerging from $f(Q,T)$ under a special EOS limit in symmetric cosmology with Bayesian and ANN observational constraints
• Cosmological constraints on sterile neutrino Dark Matter production mechanisms
• Cosmography via stellar archaeology of low-redshift early-type galaxies from SDSS
• Intermediate evolution using SNIa, and BAO
• Testing General Relativity on Galactic Scales via DESI-BAO and Strong Lensing: Circumventing Assumptions on the Hubble Constant, Sound Horizon, and Dark Energy
• Dark Radiation and Inflationary Freedom
• An Overview of CHIME, the Canadian Hydrogen Intensity Mapping Experiment
• The nonlinear equation of correlation function of galaxies in the expanding universe and the solution in linear approximation
• An Optimal In-Situ Multipole Algorithm for the Isotropic Three-Point Correlation Functions
• Skewness as a Probe of Gravity: Real and Redshift Space Counts-In-Cells
• Testing Large-Scale Structure Measurements Against Fisher Matrix Predictions
• A speed limit on tachyon fields from cosmological and fine-structure data