The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory

Abstract

We present the cosmological implications from final measurements of clustering using galaxies, quasars, and Ly$\alpha$ forests from the completed Sloan Digital Sky Survey (SDSS) lineage of experiments in large-scale structure. These experiments, composed of data from SDSS, SDSS-II, BOSS, and eBOSS, offer independent measurements of baryon acoustic oscillation (BAO) measurements of angular-diameter distances and Hubble distances relative to the sound horizon, $r_d$, from eight different samples and six measurements of the growth rate parameter, $f{\sigma }_8$, from redshift-space distortions (RSD). This composite sample is the most constraining of its kind and allows us to perform a comprehensive assessment of the cosmological model after two decades of dedicated spectroscopic observation. We show that the BAO data alone are able to rule out dark-energy-free models at more than eight standard deviations in an extension to the flat, $\Lambda$CDM model that allows for curvature. When combined with Planck Cosmic Microwave Background (CMB) measurements of temperature and polarization the BAO data provide nearly an order of magnitude improvement on curvature constraints. The RSD measurements indicate a growth rate that is consistent with predictions from Planck primary data and with General Relativity. When combining the results of SDSS BAO and RSD with external data, all multiple-parameter extensions remain consistent with a $\Lambda$CDM model. Regardless of cosmological model, the precision on ${\Omega }_{\Lambda }$, $H_0$, and ${\sigma }_8$, remains at roughly 1\%, showing changes of less than 0.6\% in the central values between models. The inverse distance ladder measurement under a o$w_0{w}_a$CDM yields $H_0=68.20\pm 0.81\mathrm{km}{\mathrm{s}}^{-1}\mathrm{Mp}{\mathrm{c}}^{-1}$, remaining in tension with several direct determination methods. (abridged)

A summary of all SDSS BAO and RSD measurements with accompanying legacy figures can be found here: https://www.sdss.org/science/final-bao-and-rsd-measurements/ . The full cosmological interpretation of these measurements can be found here: https://www.sdss.org/science/cosmology-results-from-eboss/

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• Massive neutrinos and cosmic composition
• The observed galaxy power spectrum in General Relativity
• Euclid: Forecasts from redshift-space distortions and the Alcock-Paczynski test with cosmic voids
• A Measurement of Gravitational Lensing of the Cosmic Microwave Background Using SPT-3G 2018 Data
• Late time interacting cosmologies and the Hubble constant tension
• Modeling Galaxies in Redshift Space at the Field Level
• Remedy of some cosmological tensions via effective phantom-like behavior of interacting vacuum energy
• BAO+BBN revisited -- Growing the Hubble tension with a 0.7km/s/Mpc constraint
• Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies
• Model-agnostic assessment of dark energy after DESI DR1 BAO
• Full-Shape Galaxy Power Spectra and the Curvature Tension
• Dynamical Dark Energy Beyond Planck? Constraints from multiple CMB probes, DESI BAO and Type-Ia Supernovae
• BAO angular scale at z_eff = 0.11 with the SDSS blue galaxies
• Do quasar X-ray and UV flux measurements provide a useful test of cosmological models?
• Einstein, Planck and Vera Rubin: relevant encounters between the Cosmological and the Quantum Worlds
• Dynamical Dark Energy in light of the DESI DR2 Baryonic Acoustic Oscillations Measurements
• Cosmological Constraints from Gas Mass Fractions of Massive, Relaxed Galaxy Clusters
• SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field
• Testing spatial curvature and anisotropic expansion on top of the $\Lambda$CDM model
• Gamma-Ray Bursts, Quasars, Baryonic Acoustic Oscillations, and Supernovae Ia: new statistical insights and cosmological constraints
• Minimal decoherence from inflation
• Testing AdS early dark energy with Planck, SPTpol and LSS data
• Quantifying the $S_8$ tension and evidence for interacting dark energy from redshift-space distortion measurements
• Quantifying Scalar Field Dynamics with DESI 2024 Y1 BAO measurements
• A tale of two (or more) $h$'s
• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from multi-tracer BAO analysis with galaxies and voids
• Health checkup test of the standard cosmological model in view of recent Cosmic Microwave Background Anisotropies experiments
• Bright galaxy sample in the Kilo-Degree Survey Data Release 4: selection, photometric redshifts, and physical properties
• Model-independent cosmological inference post DESI DR1 BAO measurements
• $H_0=69.8\pm 1.3$ $\mathrm{km}{\mathrm{s}}^{-1}\mathrm{Mp}{\mathrm{c}}^{-1}$, ${\Omega }_{m0}=0.288\pm 0.017$, and other constraints from lower-redshift, non-CMB, expansion-rate data
• Novel null tests for the spatial curvature and homogeneity of the Universe and their machine learning reconstructions
• Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter
• The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
• Combining pre- and post-recombination new physics to address cosmological tensions: case study with varying electron mass and sign-switching cosmological constant
• Simple-graduated dark energy and spatial curvature
• Detecting clusters of galaxies and active galactic nuclei in an eROSITA all-sky survey digital twin
• New constraint on the tensor-to-scalar ratio from the $Planck$ and BICEP/Keck Array data using the profile likelihood
• $\Lambda$CDM Tensions: Localising Missing Physics through Consistency Checks
• KiDS-1000: Combined halo-model cosmology constraints from galaxy abundance, galaxy clustering and galaxy-galaxy lensing
• Testing the consistency between cosmological data: the impact of spatial curvature and the dark energy EoS
• Observational constraints on Myrzakulov gravity
• The Atacama Cosmology Telescope: Cosmology from cross-correlations of unWISE galaxies and ACT DR6 CMB lensing
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: a multi-tracer analysis in Fourier space for measuring the cosmic structure growth and expansion rate
• The Persistence of Large Scale Structures I: Primordial non-Gaussianity
• Gamma-ray burst data strongly favor the three-parameter fundamental plane (Dainotti) correlation relation over the two-parameter one
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for the eBOSS Emission Line Galaxy Sample
• Uncertain Times: The Redshift-Time Relation from Cosmology and Stars
• Reducing the uncertainty on the Hubble constant up to 35\% with an improved statistical analysis: different best-fit likelihoods for Supernovae Ia, Baryon Acoustic Oscillations, Quasars, and Gamma-Ray Bursts
• $S_8$ increases with effective redshift in $\Lambda$CDM cosmology
• Cosmography with Supernova Refsdal through time-delay cluster lensing: independent measurements of the Hubble constant and geometry of the Universe
• Strong detection of the CMB lensingxgalaxy weak lensingcross-correlation from ACT-DR4,PlanckLegacy and KiDS-1000
• Baryon Acoustic Oscillation Theory and Modelling Systematics for the DESI 2024 results
• Field Level Neural Network Emulator for Cosmological N-body Simulations
• Consistency of Planck, ACT and SPT constraints on magnetically assisted recombination and forecasts for future experiments
• ENCORE: An $\mathcal{O}(N_{\mathrm{g}}^2)$ Estimator for Galaxy $N$-Point Correlation Functions
• One spectrum to cure them all: Signature from early Universe solves major anomalies and tensions in cosmology
• Pressure Parametrization of Dark Energy: First and Second-Order Constraints with Latest Cosmological Data
• FORGE -- the f(R) gravity cosmic emulator project I: Introduction and matter power spectrum emulator
• Growth of Cosmic Structure
• What it takes to solve the Hubble tension through modifications of cosmological recombination
• TangoSIDM: Tantalizing models of Self-Interacting Dark Matter
• Tightening the reins on non-minimal dark sector physics: Interacting Dark Energy with dynamical and non-dynamical equation of state
• Inflation, the Hubble Tension and Early Dark Energy: an alternative overview
• Strengthening the bound on the mass of the lightest neutrino with terrestrial and cosmological experiments
• Testing Gravity on Cosmic Scales: A Case Study of Jordan-Brans-Dicke Theory
• Metastable dark energy models in light of Planck 2018: Alleviating the $H_0$ tension
• Dark Energy Survey: A 2.1% measurement of the angular Baryonic Acoustic Oscillation scale at redshift $z_{\mathrm{eff}}$=0.85 from the final dataset
• Cosmological Constraint Precision of the Photometric and Spectroscopic Multi-probe Surveys of China Space Station Telescope (CSST)
• Is the dark energy equation of state parameter singular?
• Ruling Out New Physics at Low Redshift as a solution to the $H_0$ Tension
• Massive neutrino self-interactions and inflation
• Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions
• Determining the Hubble Constant without the Sound Horizon: Perspectives with Future Galaxy Surveys
• Reconstruction of the neutrino mass as a function of redshift
• Cosmology beyond BAO from the 3D distribution of the Lyman-$\alpha$ forest
• Scalar field dark energy models: Current and forecast constraints
• Peculiar-velocity cosmology with Types Ia and II supernovae
• Cosmological inference from the EFTofLSS: the eBOSS QSO full-shape analysis
• Aemulus $\nu$: Precise Predictions for Matter and Biased Tracer Power Spectra in the Presence of Neutrinos
• First Detection of the BAO Signal from Early DESI Data
• The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for Galaxy Clustering Measurements
• The Bacco Simulation Project: Bacco Hybrid Lagrangian Bias Expansion Model in Redshift Space
• Cosmology with varying fundamental constants from hyperlight, coupled scalars
• Gamma ray burst constraints on cosmological models from the improved Amati correlation
• Cosmological constraints from the power spectrum of eBOSS quasars
• Clustering in Massive Neutrino Cosmologies via Eulerian Perturbation Theory
• Self-Interacting Neutrinos in Light of Large-Scale Structure Data
• Constraining the dark energy models using Baryon Acoustic Oscillations: An approach independent of $H_0\cdot r_d$
• Dynamical dark energy in the light of DESI 2024 data
• Phenomenological emergent dark energy in the light of DESI Data Release 1
• Principal reconstructed modes of dark energy and gravity
• Axi-Higgs Cosmology
• Beyond $\Lambda$CDM constraints from the full shape clustering measurements from BOSS and eBOSS
• Towards deconstructing the simplest seesaw mechanism
• Cross-Correlation of Planck CMB Lensing with DESI-Like LRGs
• Full-shape BOSS constraints on dark matter interacting with dark radiation and lifting the $S_8$ tension
• Cosmological constraints on ${\Lambda }_{\mathrm{s}}$CDM scenario in a type II minimally modified gravity
• The Atacama Cosmology Telescope DR6 and DESI: Structure formation over cosmic time with a measurement of the cross-correlation of CMB Lensing and Luminous Red Galaxies
• Cosmic expansion parametrization: Implication for curvature and ${\text{H}}_0$ tension
• 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
• Information Content of Higher-Order Galaxy Correlation Functions
• Updating non-standard neutrinos properties with Planck-CMB data and full-shape analysis of BOSS and eBOSS galaxies
• Evidence for a high-z ISW signal from supervoids in the distribution of eBOSS quasars
• The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset
• Fast full N-body simulations of generic modified gravity: conformal coupling models
• Towards a reliable calculation of relic radiation from primordial gravitational waves
• Dynamical dark energy confronted with multiple CMB missions
• Consistency tests of field level inference with the EFT likelihood
• Fast and accurate predictions of the nonlinear matter power spectrum for general models of Dark Energy and Modified Gravity
• Creating Jackknife and Bootstrap estimates of the covariance matrix for the two-point correlation function
• Constraints on the cosmic expansion rate at redshift 2.3 from the Lyman-$\alpha$ forest
• Model-independent versus model-dependent interpretation of the SDSS-III BOSS power spectrum: Bridging the divide
• Model-independent constraints on ${\Omega }_m$ and $H(z)$ from the link between geometry and growth
• Second Data Release of the COSMOS Lyman-alpha Mapping and Tomographic Observation: The First 3D Maps of the Detailed Cosmic Web at 2.05<z<2.55
• Modified gravity and massive neutrinos: constraints from the full shape analysis of BOSS galaxies and forecasts for Stage IV surveys
• 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
• Redshift-space effects in voids and their impact on cosmological tests. Part II: the void-galaxy cross-correlation function
• Cosmological Constraints on sub-horizon scales modified gravity theories with MGCLASS II
• Impacts of dark energy on weighing neutrinos after DESI BAO
• Model marginalized constraints on neutrino properties from cosmology
• Machine Learning for Observational Cosmology
• MOG cosmology without dark matter and the cosmological constant
• Tightening geometric and dynamical constraints on dark energy and gravity: galaxy clustering, intrinsic alignment and kinetic Sunyaev-Zel'dovich effect
• Do you smell something decaying? Updated linear constraints on decaying dark matter scenarios
• Euclid preparation. Sensitivity to neutrino parameters
• Standardizing reverberation-measured C IV time-lag quasars, and using them with standardized Mg II quasars to constrain cosmological parameters
• The foreground transfer function for HI intensity mapping signal reconstruction: MeerKLASS and precision cosmology applications
• Neutrino Masses and Mass Hierarchy: Evidence for the Normal Hierarchy
• Cosmographic view on the $H_0$ and ${\sigma }_8$ tensions
• A local measurement of the growth rate from peculiar velocities and galaxy clustering correlations in the 6dF Galaxy Survey
• An effective description of Laniakea: impact on cosmology and the local determination of the Hubble constant
• Measuring the reionization optical depth without large-scale CMB polarization
• Cosmological constraints from HII starburst galaxy, quasar angular size, and other measurements
• KiDS-Legacy: Consistency of cosmic shear measurements and joint cosmological constraints with external probes
• Constraining spatial curvature with large-scale structure
• Model independent bounds on Type Ia supernova absolute peak magnitude
• An exploration of an early gravity transition in light of cosmological tensions
• The BINGO Project II: Instrument Description
• Fast full $N$-body simulations of generic modified gravity: derivative coupling models
• Tomographic Alcock-Paczynski Test with Redshift-Space Correlation Function: Evidence for the Dark Energy Equation of State Parameter w>-1
• A model-independent reconstruction of dark sector interactions
• A Parameter-Masked Mock Data Challenge for Beyond-Two-Point Galaxy Clustering Statistics
• Transition dynamics in the ${\Lambda }_{\mathrm{s}}$CDM model: Implications for bound cosmic structures
• $H_0$ Tension in Torsion-based Modified Gravity
• Inevitable manifestation of wiggles in the expansion of the late Universe
• Observational Constraints on Dark Energy Models with $\Lambda$ as an Equilibrium Point
• The weak, the strong and the ugly -- A comparative analysis of interacting stepped dark radiation
• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the growth rate of structure from the small-scale clustering of the luminous red galaxy sample
• Constraints on dark matter-neutrino scattering from the Milky-Way satellites and subhalo modeling for dark acoustic oscillations
• Analytic Gaussian Covariance Matrices for Galaxy $N$-Point Correlation Functions
• Exploring the Hubble tension with a late time Modified Gravity scenario
• Dark energy by natural evolution: Constraining dark energy using Approximate Bayesian Computation
• The homogeneity scale and the growth rate of cosmic structures
• Quasar UV/X-ray relation luminosity distances are shorter than reverberation-measured radius-luminosity relation luminosity distances
• Current data are consistent with flat spatial hypersurfaces in the $\Lambda$CDM cosmological model but favor more lensing than the model predicts
• General cosmological perturbations in teleparallel gravity
• Euclid: Forecast constraints on consistency tests of the $\Lambda$CDM model
• A comparison of template vs. direct model fitting for redshift-space distortions in BOSS
• Wide-angle and relativistic effects in Fourier-space clustering statistics
• Observational constraints on Starobinsky $f(R)$ cosmology from cosmic expansion and structure growth data
• Modeling Nearest Neighbor distributions of biased tracers using Hybrid Effective Field Theory
• Cosmology inference at the field level from biased tracers in redshift-space
• Forecast of Neutrino Cosmology from the CSST Photometric Galaxy Clustering and Cosmic Shear Surveys
• ${\Lambda }_{\mathrm{s}}$CDM cosmology: Alleviating major cosmological tensions by predicting standard neutrino properties
• Optimal Reconstruction of Baryon Acoustic Oscillations for DESI 2024
• Do reverberation-measured H$\beta$ quasars provide a useful test of cosmology?
• Minimal theory of massive gravity in the light of CMB data and the $S_8$ tension
• Phantom scalar-tensor models and cosmological tensions
• $\text{matryoshka}$: Halo Model Emulator for the Galaxy Power Spectrum
• New cosmological constraints on $f(T)$ gravity in light of full Planck-CMB and type Ia supernovae data
• A New Probe of Relic Neutrino Clustering using Cosmogenic Neutrinos
• New constraints on cosmological modified gravity theories from anisotropic three-point correlation functions of BOSS DR12 galaxies
• Consistency study of high- and low-accreting Mg ii quasars: No significant effect of the Fe ii to Mg ii flux ratio on the radius-luminosity relation dispersion
• Cosmological constraints on early dark energy from the full shape analysis of eBOSS DR16
• Euclid: Modelling massive neutrinos in cosmology -- a code comparison
• C${}^3$-Cluster Clustering Cosmology I. New constraints on the cosmic growth rate at z~0.3 from redshift-space clustering anisotropies
• New late-time constraints on $f(R)$ gravity
• High $H_0$ Values from CMB E-mode Data: A Clue for Resolving the Hubble Tension?
• Quasars: standard candles up to z=7.5 with the precision of Supernovae Ia
• Testing General Relativity on cosmological scales at redshift z ~ 1.5 with quasar and CMB lensing
• Cosmological constraints on dark energy models using DESI BAO 2024
• Dynamical Dark Energy in the Crosshairs: A Joint Analysis with DESI, Pantheon plus, and TDCOSMO Constraints
• Minimal theory of massive gravity and constraints on the graviton mass
• Impact of the Hubble tension on the $r$-$n_s$ contour
• Testing an oscillatory behavior of dark energy
• The HETDEX Survey: Emission Line Exploration and Source Classification
• The Integrated Sachs Wolfe effect: unWISE and Planck constraints on Dynamical Dark Energy
• Quintessential Cosmological Tensions
• Gravitational Redshift Constraints on the Effective Theory of Interacting Dark Energy
• Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension
• Modeling HI at the field level
• PT challenge: Validation of ShapeFit on large-volume, high-resolution mocks
• Comparing the scalar-field dark energy models with recent observations
• Probing heavy Majorana neutrinos and the Weinberg operator through vector boson fusion processes in proton-proton collisions at $\sqrt{s}$ = 13 TeV
• Constraints on primordial lepton asymmetries with full neutrino transport
• Model-independent test for the cosmic distance duality relation with Pantheon and eBOSS DR16 quasar sample
• Profile Likelihoods in Cosmology: When, Why and How illustrated with $\Lambda$CDM, Massive Neutrinos and Dark Energy
• Detecting the power spectrum turnover with HI intensity mapping
• Phantom braneworld and the Hubble tension
• Dynamical systems analysis of tachyon dark energy model from a new perspective
• No-go guide for the Hubble tension: late-time or local-scale new physics
• Compressing the cosmological information in one-dimensional correlations of the Lyman-$\alpha$ forest
• Euclid: Cosmology forecasts from the void-galaxy cross-correlation function with reconstruction
• Analysis of Unified Galaxy Power Spectrum Multipole Measurements
• The 3D Lyman-$\alpha$ Forest Power Spectrum from eBOSS DR16
• Molecular Chemistry for Dark Matter II: Recombination, Molecule Formation, and Halo Mass Function in Atomic Dark Matter
• Constraining interacting dark energy models with the halo concentration-mass relation
• Is Dynamical Dark Energy Necessary? DESI BAO and Modified Recombination
• Cosmological constraints from the cross-correlation of DESI Luminous Red Galaxies with CMB lensing from Planck PR4 and ACT DR6
• Exploring new physics in the late Universe's expansion through non-parametric inference
• Analytical and EZmock covariance validation for the DESI 2024 results
• Coupled Multi Scalar Field Dark Energy
• Probing Modified Gravity with Integrated Sachs-Wolfe CMB and Galaxy Cross-correlations
• Consistency tests between SDSS and DESI BAO measurements
• Cosmological forecasts for future galaxy surveys with the linear point standard ruler: Toward consistent BAO analyses far from a fiducial cosmology
• Measuring Hubble constant in an anisotropic extension of $\Lambda$CDM model
• Rescuing constraints on modified gravity using gravitational redshift in large-scale structure
• Probing massive neutrinos with the Minkowski functionals of large-scale structure
• KiDS-1000 Cosmology: machine learning -- accelerated constraints on Interacting Dark Energy with COSMOPOWER
• $\Lambda$CDM is alive and well
• Extracting HI Astrophysics from Interferometric Intensity Mapping
• The Aemulus Project VI: Emulation of beyond-standard galaxy clustering statistics to improve cosmological constraints
• Fiducial-Cosmology-dependent systematics for the DESI 2024 BAO Analysis
• Key drivers of the preference for dynamic dark energy
• Reconciling $S_8$: Insights from Interacting Dark Sectors
• Does DESI DR2 challenge $\Lambda$CDM paradigm ?
• The assembly bias of emission line galaxies
• Planck-PR4 anisotropy spectra show (better) consistency with General Relativity
• Probing massive neutrinos with the Minkowski functionals of the galaxy distribution
• HOD-Dependent Systematics in Emission Line Galaxies for the DESI 2024 BAO analysis
• Joint reconstructions of growth and expansion histories from stage-IV surveys with minimal assumptions. II. Modified gravity and massive neutrinos
• Unified and consistent structure growth measurements from joint ACT, SPT and \textit{Planck} CMB lensing
• A critical discussion on the $H_0$ tension
• Improved null tests of $\Lambda$CDM and FLRW in light of DESI DR2
• Redshift Evolution and Non-Universal Dispersion of Quasar Luminosity Correlation
• Pseudoscalar sterile neutrino self-interactions in light of Planck, SPT and ACT data
• Measuring ${\sigma }_8$ using DESI Legacy Imaging Surveys Emission-Line Galaxies and Planck CMB Lensing and the Impact of Dust on Parameter Inference
• Sweeping Horndeski Canvas: New Growth-Rate Parameterization for Modified-Gravity Theories
• The matter density PDF for modified gravity and dark energy with Large Deviations Theory
• The Alcock-Paczyński effect from Lyman-$\alpha$ forest correlations: Analysis validation with synthetic data
• The $S_8$ Tension in Light of Updated Redshift-Space Distortion Data and PAge Approximation
• Validation of semi-analytical, semi-empirical covariance matrices for two-point correlation function for Early DESI data
• Growth-rate measurement with type-Ia supernovae using ZTF survey simulations
• A case study for measuring the relativistic dipole of a galaxy cross-correlation with the Dark Energy Spectroscopic Instrument
• Cosmological measurements from void-galaxy and galaxy-galaxy clustering in the Sloan Digital Sky Survey
• Cosmology from weak lensing alone and implications for the Hubble tension
• Scalar-Tensor Gravity and DESI 2024 BAO data
• Real-space quantum-to-classical transition of time dependent background fluctuations
• 21cmFirstCLASS I. Cosmological tool for $\Lambda$CDM and beyond
• Dark Energy Survey Year 3 Results: Measurement of the Baryon Acoustic Oscillations with Three-dimensional Clustering
• Modified Einstein versus Modified Euler for Dark Matter
• Evolution mapping: a new approach to describe matter clustering in the non-linear regime
• Theoretical and numerical perspectives on cosmic distance averages
• Effect of extinction on quasar luminosity distances determined from UV and X-ray flux measurements
• Current constraints on cosmological scenarios with very low reheating temperatures
• Compressed baryon acoustic oscillation analysis is robust to modified-gravity models
• Model-independent cosmological inference after the DESI DR2 data with improved inverse distance ladder
• To curve, or not to curve: Is curvature-assisted quintessence observationally viable?
• Testing non-local gravity by clusters of galaxies
• Addressing Cosmological Tensions by Non-Local Gravity
• Observational bounds on extended minimal theories of massive gravity: New limits on the graviton mass
• A null test of the Cosmological Principle with BAO measurements
• The 6x2pt method: supernova velocities meet multiple tracers
• Validating the Galaxy and Quasar Catalog-Level Blinding Scheme for the DESI 2024 analysis
• Hubble tension as a window on the gravitation of the dark matter sector
• Two-loop power spectrum with full time- and scale-dependence and EFT corrections: impact of massive neutrinos and going beyond EdS
• CSST large-scale structure analysis pipeline: I. constructing reference mock galaxy redshift surveys
• ELG Spectroscopic Systematics Analysis of the DESI Data Release 1
• Unexplored regions in teleparallel $f(T)$ gravity: Sign-changing dark energy density
• Towards alleviating the $H_0$ and $S_8$ tensions with Early Dark Energy - Dark Matter drag
• Differentiating dark interactions with perturbation
• Dark energy reconstructions combining BAO data with galaxy clusters and intermediate redshift catalogs
• HOD-Dependent Systematics for Luminous Red Galaxies in the DESI 2024 BAO Analysis
• Velocity profiles of matter and biased tracers around voids
• Nonparametric reconstructions of dynamical dark energy via flexknots
• A preference for dynamical phantom dark energy using one-parameter model with Planck, DESI DR1 BAO and SN data
• A Test of the Standard Cosmological Model with Geometry and Growth
• Non-parametric reconstruction of cosmological observables using Gaussian Processes Regression
• Growth of structures using redshift space distortion in $f(T)$ Cosmology
• Combining gravitational lensing and gravitational redshift to measure the anisotropic stress with future galaxy surveys
• Observational constraints on interacting vacuum energy with linear interactions
• Hybrid-basis inference for large-scale galaxy clustering: combining spherical and Cartesian Fourier analyses
• Positive neutrino masses with DESI DR2 via matter conversion to dark energy
• Revisiting progenitor-age dependence of type Ia supernova luminosity standardization process
• Reducing the Variance of Redshift Space Distortion Measurements from Mock Galaxy Catalogues with Different Lines of Sight
• Exploring the Growth Index ${\gamma }_L$: Insights from Different CMB Dataset Combinations and Approaches
• Constraining extended cosmologies with GW$\times$LSS cross-correlations
• The QCD Axion: Some Like It Hot
• Cosmological Probes of Structure Growth and Tests of Gravity
• Constraints on Cosmological Models from Quasars Calibrated with Type Ia Supernova by a Gaussian Process
• Beyond Yamamoto: Anisotropic Power Spectra and Correlation Functions with Pairwise Lines-of-Sight
• Closing up the cluster tension?
• Determination of cosmic curvature independent of the sound horizon and $H_0$ using BOSS/eBOSS and DESI DR1 BAO observations
• Investigating dark energy by electromagnetic frequency shifts
• Hints of Neutrino Dark Matter scattering in the CMB? Constraints from the Marginalized and Profile Distributions
• Cosmological Constraints on 4-Dimensional Einstein-Gauss-Bonnet Gravity
• Impact of the damping tail on neutrino mass constraints
• Detecting the HI Power Spectrum in the Post-Reionization Universe with SKA-Low
• Forecast Analysis on Interacting Dark Energy Models from Future Generation PICO and DESI Missions
• Superhorizon perturbations: A possible explanation of the Hubble--Lemaître Tension and the Large Scale Anisotropy of the Universe
• BAO cosmology in non-spatially flat background geometry from BOSS+eBOSS and lessons for future surveys
• $H_0$ tension without CMB data: beyond the $\Lambda$CDM
• Chasing cosmic inflation: constraints for inflationary models and reheating insights
• The impact and mitigation of broad absorption line quasars in Lyman$-\alpha$ forest correlations
• Cosmology of an Axion-Like Majoron
• Measurement of the matter-radiation equality scale using the extended Baryon Oscillation Spectroscopic Survey Quasar Sample
• Multi-component DHOST analysis in galaxy clusters
• Constraints on interacting dark energy revisited: implications for the Hubble tension
• Extracting high-order cosmological information in galaxy surveys with power spectra
• Measuring the distortion of time with relativistic effects in large-scale structure
• Swiss-cheese cosmologies with variable $G$ and $\Lambda$ from the renormalization group
• The halo model with beyond-linear halo bias: unbiasing cosmological constraints from galaxy-galaxy lensing and clustering
• Fast Radio Bursts and Artificial Neural Networks: a cosmological-model-independent estimation of the Hubble Constant
• A multitracer analysis for the eBOSS galaxy sample based on the effective field theory of large-scale structure
• A GREAT model comparison against the cosmological constant
• Lensing impact on cosmic relics and tensions
• Inferring dark energy properties from the scale factor parametrisation
• Searching for Chameleon Dark Energy with Mechanical Systems
• f(R) Gravity in an Ellipsoidal Universe
• The impact of the Universe's expansion rate on constraints on modified growth of structure
• Search for heavy Majorana neutrinos in $e^{\pm }{e}^{\pm }$ and $e^{\pm }{\mu }^{\pm }$ final states via WW scattering in $pp$ collisions at $\sqrt{s}=13$ TeV with the ATLAS detector
• The cross-correlation of galaxies in absorption with the Lyman $\alpha$ forest
• Third-order corrections to the slow-roll expansion: calculation and constraints with Planck, ACT, SPT, and BICEP/Keck
• A joint 2- and 3-point clustering analysis of the VIPERS PDR2 catalogue at z~1: breaking the degeneracy of cosmological parameters
• Unveiling the Hubble Constant through Galaxy Cluster Gas Mass Fractions
• Deep Forest: Neural Network reconstruction of the Lyman-alpha forest
• Towards a Solution to the H0 Tension: the Price to Pay
• Fresh Look at Neutrino Self-Interactions With the Lyman-$\alpha$ Forest: Constraints from EFT and PRIYA Simulations
• Nested solitons in two-field fuzzy dark matter
• Rényi Holographic Dark Energy
• A More Accurate Parameterization based on cosmic Age (MAPAge)
• New dwarf galaxy candidates in the sphere of influence of the Local Volume spiral galaxy NGC2683
• The miniJPAS survey quasar selection II: Machine learning classification with photometric measurements and uncertainties
• A novel approach to cosmological non-linearities as an effective fluid
• Minimal model dependent constraints on cosmological nuisance parameters and cosmic curvature from combinations of cosmological data
• HI intensity mapping correlation function from UNIT simulations: BAO and observationally induced anisotropy
• Dark Energy Survey: Galaxy Sample for the Baryonic Acoustic Oscillation Measurement from the Final Dataset
• Detecting neutrino-boosted axion dark matter in the MeV gap
• Joint Constraints on the Hubble Constant, Spatial Curvature, and Sound Horizon from the Late-time Universe with Cosmography
• Improved analytical modeling of the non-linear power spectrum in modified gravity cosmologies
• How robust are the parameter constraints extending the $\Lambda$CDM model?
• Constraining the emergent dark energy models with observational data at intermediate redshift
• Do we need wavelets in the late Universe?
• Constraining Holographic Dark Energy and Analyzing Cosmological Tensions
• Investigating dark energy by electromagnetic frequency shifts II: the Pantheon+ sample
• Cosmological effects of the Galileon term in Scalar-Tensor Theories
• One-parameter dynamical dark-energy from the generalized Chaplygin gas
• Impact of tidal environment on galaxy clustering in GAMA
• Testing $\alpha$-attractor quintessential inflation against CMB and low-redshift data
• High redshift LBGs from deep broadband imaging for future spectroscopic surveys
• New dwarf galaxy candidates in the sphere of influence of the Sombrero galaxy
• The Uchuu-GLAM BOSS and eBOSS LRG lightcones: Exploring clustering and covariance errors
• Axion star condensation around primordial black holes and microlensing limits
• A PAge-like Unified Dark Fluid Model
• Abundance and properties of dark radiation from the cosmic microwave background
• Explanation of high redshift luminous galaxies from JWST by early dark energy model
• Testing tree level TeV scale seesaw scenarios in $\mu$TRISTAN
• Narrowing down the Hubble tension to the first two rungs of distance ladders
• Joint analyses of 2D CMB lensing and 3D galaxy clustering in the spherical Fourier-Bessel basis
• Interferometric HI intensity mapping: perturbation theory predictions and foreground removal effects
• Comprehensive Constraints on Dark Radiation Injection After BBN
• LimberJack.jl: auto-differentiable methods for angular power spectra analyses
• Cosmology from LOFAR Two-metre Sky Survey Data Release 2: Cross-correlation with the cosmic microwave background
• Weak field and slow motion limits in energy-momentum powered gravity
• Cosmological Fisher forecasts for next-generation spectroscopic surveys
• Dark Matter Cosmology with Varying Viscosity: a Possible Resolution to the $S_8$ Tension
• Using peculiar velocity surveys to constrain neutrino masses
• Cosmology with the kinetic Sunyaev-Zeldovich effect: Independent of the optical depth and ${\sigma }_8$
• The impact of large-scale galaxy clustering on the variance of the Hellings-Downs correlation: theoretical framework
• Torsion cosmology in the light of DESI, supernovae and CMB observational constraints
• Neutrino winds on the sky
• Morphology of Weak Lensing Convergence Maps
• Hubble tension as a window on the gravitation of the dark matter sector: Exploration of a family of models
• Testing the equivalence principle across the Universe: a model-independent approach with galaxy multi-tracing
• Theoretical and Experimental Challenges in the Measurement of Neutrino Mass
• The DESI One-Percent Survey: Modelling the clustering and halo occupation of all four DESI tracers with Uchuu
• Optical Design of the EXperiment for Cryogenic Large-Aperture Intensity Mapping (EXCLAIM)
• $A_4$-based model with linear seesaw scheme for lepton mass and mixing
• Cosmology from Planck CMB Lensing and DESI DR1 Quasar Tomography
• Towards an accurate model of small-scale redshift-space distortions in modified gravity
• Bounds on Velocity-Dependent Dark Matter-Baryon Scattering from Large-Scale Structure
• Constraints on the Optical Depth to Reionization from Balloon-Borne CMB Measurements
• Detecting Baryon Acoustic Oscillations with third generation gravitational wave observatories
• A study on the Clustering Properties of Radio-Selected sources in the Lockman Hole Region at 325 MHz
• Probing interacting dark sector models with future weak lensing-informed galaxy cluster abundance constraints from SPT-3G and CMB-S4
• Disentangling modified gravity from a dark force with gravitational redshift
• The Hubble Rate Trouble: An Effective Field Theory of Dark Matter
• Reconstructions of $f(\mathcal{P})$ and $f(\mathcal{Q})$ gravity models from $(m,n)$-type Barrow Holographic Dark Energy: Analysis and Observational Constraints
• Biasing relation, environmental dependencies and estimation of the growth rate from star forming galaxies
• Non-parametric modeling of the cosmological data, base on the ${\chi }^2$ distribution
• Sound-Horizon-Agnostic Inference of the Hubble Constant and Neutrino Mass from BAO, CMB Lensing, and Galaxy Weak Lensing and Clustering
• Is there a dynamical tendency in H0 with late time measurements?
• Forecast for growth-rate measurement using peculiar velocities from LSST supernovae
• Alcock-Paczyński effect on void-finding: Implications for void-galaxy cross-correlation modelling
• Imprint of massive neutrinos on Persistent Homology of large-scale structure
• Effects of anisotropy in an anisotropic extension of $w$CDM model
• Modern Cosmology, an Amuse-Gueule
• An unbiased method of measuring the ratio of two data sets
• Testing the consistency of early and late cosmological parameters with BAO and CMB data
• Fundamental Physics and Cosmology with TianQin
• Predictions of $m_{ee}$ and neutrino mass from a consistent Froggatt-Nielsen model
• Low- and high-redshift H II starburst galaxies obey different luminosity-velocity dispersion relations
• Evolution mapping II: describing statistics of the non-linear cosmic velocity field
• Quintessential Implications of the presence of AdS in the Dark Energy sector
• A convenient approach to characterizing model uncertainty with application to early dark energy solutions of the Hubble tension
• Improving initialization and evolution accuracy of cosmological neutrino simulations
• Mitigating baryonic effects with a theoretical error covariance
• Can acoustic and axion-like early dark energy still resolve the Hubble tension?
• Determining Absolute Neutrino Mass using Quantum Technologies
• Exploring Alternative Cosmologies with the LSST: Simulated Forecasts and Current Observational Constraints
• Revisiting CPL with sign-switching density: To cross or not to cross the NECB
• Tensions in cosmology: a discussion of statistical tools to determine inconsistencies
• Exploring Modified Gravity: Constraints on the $\mu$ and $\Sigma$ Parametrization with WMAP, ACT, and SPT
• KiDS-Legacy: Angular galaxy clustering from deep surveys with complex selection effects
• Impact of intrinsic alignments on clustering constraints of the growth rate
• Cosmology at high redshift -- a probe of fundamental physics
• Beyond $\Lambda$CDM: Exploring a Dynamical Cosmological Constant Framework Consistent with Late-Time Observations
• Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
• Deviations from Tribimaximal and Golden Ratio mixings under radiative corrections of neutrino masses and mixings
• Thawing k-essence dark energy in the PAge space
• Inferring Cosmological Parameters with Evidential Physics-Informed Neural Networks
• The DAMIC-M Low Background Chamber
• The impact of 2D and 3D BAO measurements on the Cosmic Distance Duality Relation with HII galaxies
• CombineHarvesterFlow: Joint Probe Analysis Made Easy with Normalizing Flows
• Investigating the $w$CDM Model with Latest DESI BAO Observations
• Growth and Geometry Split in Light of the DES-Y3 Survey
• Magrathea-Pathfinder: A 3D adaptive-mesh code for geodesic ray tracing in $N$-body simulations
• Relativistic binary systems in scale-independent energy-momentum squared gravity
• Characteristic Functions for Cosmological Cross-Correlations
• Litmus tests of the flat $\Lambda$CDM model and model-independent measurement of $H_0{r}_{\mathrm{d}}$ with LSST and DESI
• Modeling the Spectral Diversity of Quasars in the Sixteenth Data Release from the Sloan Digital Sky Survey
• Perturbation theory models for LSST-era galaxy clustering: tests with sub-percent mock catalog measurements in Fourier and configuration space
• Examining the validity of the minimal varying speed of light model through cosmological observations: relaxing the null curvature constraint
• Constraining modified gravity scenarios with the 6dFGS and SDSS galaxy peculiar velocity datasets
• Isolating the linear signal when making redshift space distortion measurements
• Lower tensor-to-scalar ratio as possible signature of modified gravity
• Incompatibility of fine-structure constant variations at recombination with local observations
• Unveiling the Universe with Emerging Cosmological Probes
• Triumvirate: A Python/C++ package for three-point clustering measurements
• Improved two-point correlation function estimates using glass-like distributions as a reference sample
• Cosmic inflation from broken conformal symmetry
• The BINGO project VIII: On the recoverability of the BAO signal on HI intensity mapping simulations
• New simple and accurate quintessence approximations
• Atomic corrections for the unique first forbidden $\beta$ transition of ${}^{187}$Re
• Possible Impact of non-Gaussianities on cosmological constraints in neutrino physics
• H-band light curves of Milky Way Cepheids via Difference Imaging
• Fisher forecast for the BAO measurements from the CSST spectroscopic and photometric galaxy clustering
• A proposal to improve the accuracy of cosmological observables and address the Hubble tension problem
• Small scale clustering of BOSS galaxies: dependence on luminosity, color, age, stellar mass, specific star formation rate and other properties
• Baryon acoustic scale at $z_{\eff} = 0.166$ with the SDSS blue galaxies
• Enhancing Cosmological Model Selection with Interpretable Machine Learning
• Cosmic void exclusion models and their impact on the distance scale measurements from large scale structure
• Axions in Andromeda: Searching for Minicluster -- Neutron Star Encounters with the Green Bank Telescope
• A Machine Learning Approach to Correct for Mass Resolution Effects in Simulated Halo Clustering Statistics
• Impact of Low ell's on Large Scale Structure Anomalies
• On Evidence for Elastic Interactions in the Dark Sector
• Euclid: Relativistic effects in the dipole of the 2-point correlation function
• Measuring the speed of light with cosmological observations: current constraints and forecasts
• A solution to the S8 tension through neutrino-dark matter interactions
• SHARP -- IX. The dense, low-mass perturbers in B1938+666 and J0946+1006: implications for cold and self-interacting dark matter
• Towards Optimal Foreground Mitigation Strategies for Interferometric HI Intensity Mapping in the Low-Redshift Universe
• Prospects for disentangling dark matter with weak lensing
• Modelling self-interacting dark matter substructures I: Calibration with N-body simulations of a Milky-Way-sized halo and its satellite
• Model Selection using Baryon Acoustic Oscillations in the Final SDSS-IV Release
• Is ${\omega }_0{\omega }_a$CDM a good model for the clumpy Universe?
• Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-$\Lambda$CDM Interpretations, and Tensions
• Constraints on Spatial Curvature and Dark Energy Dynamics in the $w$CDM Model from DESI DR1 and DR2
• One Extension to Explain Them All, One Scale-Invariant Spectrum to Test Them All, and in One Model Bind Them
• Statistics of Thawing K-essence Dark Energy Models
• Cosmic Tidal Reconstruction with Halo Fields
• Tilted non-spatially-flat inflation
• Signatures of Very Early Dark Energy in the Matter Power Spectrum
• A Hubble Constant Determination Through Quasar Time Delays and Type Ia Supernovae
• The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar and APOGEE-2 Data
• An Analytically Tractable Marked Power Spectrum
• Investigating the Origin of CMB Large-Scale Features Using LiteBIRD and CMB-S4
• Impact of lensing magnification on the analysis of galaxy clustering in redshift space
• Using relativistic effects in large-scale structure to constrain astrophysical properties of galaxy populations
• Cosmological signatures of a Rapid Diluted Energy Density
• Covariance matrices for variance-suppressed simulations
• Faster cosmological analysis with power spectrum without simulations
• Dark Energy: is it `just' Einstein's Cosmological Constant Lambda?
• Impact of dark matter-baryon relative velocity on the 21cm forest
• Probing cosmology via the clustering of critical points
• Relaxing cosmological constraints on current neutrino masses
• Cosmic curvature on large-scale structures with homogeneous dark energy
• Measurement of the Weyl potential evolution from the first three years of Dark Energy Survey data
• Impact of the primordial fluctuation power spectrum on the reionization history
• Anisotropic effective redshift and evolving clustering amplitude
• The first direct measurement of gravitational potential decay rate at cosmological scales and improved dark energy constraint
• A Model for the Redshift-Space Galaxy 4-Point Correlation Function
• Constructing Viable Interacting Dark Matter and Dark Energy Models: A Dynamical Systems Approach
• Redshift-space distortion constraints on the neutrino mass and models to alleviate the Hubble tension
• Special Issue on Modified Gravity Approaches to the Tensions of $\Lambda$CDM: Goals and Highlights
• Predictive uncertainty on improved astrophysics recovery from multifield cosmology
• Quintessence scalar field and cosmological constant: Dynamics of a multi-component dark energy model
• Fast Simulation of Cosmological Neutral Hydrogen based on the Halo Model
• Addressing the DESI DR2 Phantom-Crossing Anomaly and Enhanced $H_0$ Tension with Reconstructed Scalar-Tensor Gravity
• Cosmology and Astrophysics with the Diffuse eRASS1 X-ray Angular Power Spectrum
• Cosmological Evolution in Bimetric Gravity: Observational Constraints and LSS Signatures
• Hint of dark matter-dark energy interaction in DESI DR2 and current cosmological dataset?
• Dynamical Dark Energy and the Unresolved Hubble Tension: Multi-model Constraints from DESI 2025 and Other Probes
• DESI Mock Challenge: Constructing DESI galaxy catalogues based on FastPM simulations
• Photometric IGM tomography with Subaru/HSC: the large-scale structure of Ly$\alpha$ emitters and IGM transmission in the COSMOS field at $z\sim 5$
• Star-Crossed Labours: Checking Consistency Between Current Supernovae Compilations
• HI Intensity Mapping with the MIGHTEE Survey: First Results of the HI Power Spectrum
• Standardizing reverberation-measured Mg II time-lag quasars, by using the radius-luminosity relation, and constraining cosmological model parameters
• When Dark Matter Heats Up: A Model-Independent Search for Non-Cold Behavior
• Spin-Flavor Oscillations of Relic Neutrinos in Primordial Magnetic Field
• Cosmic Strings as Dynamical Dark Energy: Novel Constraints
• Galaxy and halo angular clustering in LCDM and Modified Gravity cosmologies
• Cosmology on a Gravitational Wave Background
• Constraints on the varying electron mass and early dark energy in light of ACT DR6 and DESI DR2 and the implications for inflation
• The 4MOST-Cosmology Redshift Survey: Target Selection of Bright Galaxies and Luminous Red Galaxies
• Stochastic dark matter: Covariant Brownian motion from Planckian discreteness
• Euclid: performance on main cosmological parameter science
• On the origin of the BAOtr-DESI tension
• Dynamical Oscillations in Dark Energy: Joint Constraints on the $w_{sin}$CDM Model from DESI, OHD, and Supernova Samples
• Hints of the $H_0-r_d$ tension in uncorrelated Baryon Acoustic Oscillations dataset
• Misinterpreting Modified Gravity as Dark Energy: a Quantitative Study
• Testing General Relativity through the $E_G$ Statistic Using the Weyl Potential and Galaxy Velocities
• Signature of Massive Neutrinos from the Clustering of Critical Points. I. Density-threshold-based Analysis in Configuration Space
• Measuring neutrino mass and asymmetry with matter pairwise velocities
• Novel Cosmological Joint Constraints in Multidimensional Observables Space with Redshift-free Inferences
• Comparing the motion of dark matter and standard model particles on cosmological scales
• Galaxy and Mass Assembly (GAMA): Probing galaxy-group correlations in redshift space with the halo streaming model
• Lognormal semi-numerical simulations of the Lyman-$\alpha$ forest: comparison with full hydrodynamic simulations
• Effective field theory of coupled dark energy and dark matter
• Model-Agnostic Cosmological Inference with SDSS-IV eBOSS: Simultaneous Probing for Background and Perturbed Universe
• Cross-correlating radial peculiar velocities and CMB lensing convergence
• Constraints on Tsallis cosmology using recent low and high redshift measurements
• Quintom Dark Energy: Future Attractor and Phantom Crossing in Light of DESI DR2 Observation
• The Hydrogen Intensity and Real-time Analysis eXperiment: 256-Element Array Status and Overview
• Primary gravitational waves at high frequencies I: Origin of suppression in the power spectrum
• Cosmological Signatures of Neutrino Seesaw Mechanism
• KiDS-Legacy: Constraints on Horndeski gravity from weak lensing combined with galaxy clustering and cosmic microwave background anisotropies
• Cosmic expansion beyond $\Lambda$CDM: Investigating power-law and logarithmic corrections
• The RSD Sorting Hat: Unmixing Radial Scales in Projection
• Is the large-scale structure traced by the BOSS LOWZ galaxies consistent with $\text{Planck}$?
• Topological Echoes of Primordial Physics in the Universe at Large Scales
• kSZ Pairwise Velocity Reconstruction with Machine Learning
• Probing Cosmology with Baryon Acoustic Oscillations using Gravitational Waves
• Constraints on cosmological parameters and CMB first acoustic peak in conformal Killing gravity
• Cosmological Non-Gaussianity from Neutrino Seesaw Mechanism
• The Correlation Function and Detection of Baryon Acoustic Oscillation Peak from the Spectroscopic SDSS GalWCat Galaxy Cluster Catalogue
• Euclid: Fast two-point correlation function covariance through linear construction
• Euclid preparation. 3-dimensional galaxy clustering in configuration space. Part I. 2-point correlation function estimation
• Potential reconstruction from general power spectrum in single-field inflation
• Enhanced Small-Scale Structure in the Cosmic Dark Ages
• Thermo-Coupled Early Dark Energy
• Dark matter for Majorana neutrinos in a ${\mathbb{Z}}_4$ symmetry
• A high-resolution view of the source-plane magnification near cluster caustics in wave dark matter models
• A model-independent measurement of the expansion and growth rates from BOSS using the FreePower method
• Remarks on overestimating the effects of inhomogeneities on the Hubble constant
• Can the angular scale of cosmic homogeneity be used as a cosmological test?
• Baryon Acoustic Oscillations analyses with Density-Split Statistics
• From Large Telescopes to the MUltiplexed Survey Telescope (MUST)
• Statistical Nuances in BAO Analysis: Likelihood Formulations and Non-Gaussianities
• Non-Affine Extensions of the Raychaudhuri Equation in the K-essence Framework
• Densified pupil spectrograph as high-precision radial velocimetry: From direct measurement of the Universe's expansion history to characterization of nearby habitable planet candidates
• Cosmological gravity on all scales IV: 3x2pt Fisher forecasts for pixelised phenomenological modified gravity
• Probabilistic Lagrangian bias estimators and the cumulant bias expansion
• Combined $13\times 2$-point analysis of the Cosmic Microwave Background and Large-Scale Structure: implications for the $S_8$-tension and neutrino mass constraints
• The Quasar Candidates Catalogs of DESI Legacy Imaging Survey Data Release 9
• The miniJPAS survey quasar selection IV: Classification and redshift estimation with SQUEzE
• 3D Correlations in the Lyman-$\alpha$ Forest from Early DESI Data
• Superfluid-tight cryogenic receiver with continuous sub-Kelvin cooling for EXCLAIM
• The Atacama Cosmology Telescope: A Test of the Gravitational Force Law on Cosmological Scales Using the Kinematic Sunyaev-Zeldovich Effect
• A Review on Resolving the Hubble Tension via Late-Universe Physics
• Dark Energy Survey: DESI-Independent Angular BAO Measurement
• KiDS-Legacy: Constraining dark energy, neutrino mass, and curvature
• Non-linear structure formation with elastic interactions in the dark sector
• The frozen vanilla model: Exploring dark sector interactions with delta effective theories
• Constraining Axially Symmetric Bianchi Type I Model with Self-Consistent Recombination History and Observables
• Primary Beam Chromaticity in HIRAX: I. Characterization from Simulations and Power Spectrum Implications
• Cosmology with Persistent Homology: Parameter Inference via Machine Learning
• PySCo: A fast Particle-Mesh $N$-body code for modified gravity simulations in Python
• Modelling the covariance matrix for the power spectra before and after the BAO reconstruction
• Pair Counting without Binning -- A New Approach to Correlation Functions in Clustering Statistics
• Bending the web: exploring the impact of modified gravity on the density field and halo properties within the cosmic web
• Model independent calibration for sound horizon combining observations of supernovae and transversal BAO measurements
• The virial mode $k_v$ approach to Structure Formation with Warm Dark Matter
• Role of Spatial Curvature in a Dark Energy Interacting Model
• Particle Production Scenario in an Algebraically Coupled Quintessence Field with a Dark Matter Fluid
• Predictive linear seesaw model with $\Delta \left(27\right)$ family symmetry
• Observational constraints on the second-order primordial power spectrum: Exploring a Continuous Spontaneous Localization inspired inflationary model
• Results and forecasts on cosmic inflation from weak lensing
• Biases in velocity reconstruction: investigating the effects on growth rate and expansion measurements in the local universe
• Perturbation theory challenge for cosmological parameters estimation II.: Matter power spectrum in redshift space
• Glass-Like Random Catalogues for Two-Point Estimates on the Light Cone
• Forecasts for cosmological measurements based on the angular power spectra of AGN and clusters of galaxies in the SRG/eROSITA all-sky survey
• Data-driven Cosmology from Three-dimensional Light Cones
• Gaussian discriminators between $\Lambda$CDM and wCDM cosmologies using expansion data
• Mock catalogues of emission line galaxies based on the local mass density in dark-matter only simulations
• Mapping the cosmic expansion history from LIGO-Virgo-KAGRA in synergy with DESI and SPHEREx
• Dark Energy Survey Year 3 Results: Galaxy mock catalogs for BAO analysis
• UNITSIM-Galaxies: data release and clustering of emission-line galaxies
• Mitigating the impact of fiber assignment on the measurement of galaxy-lensing cross correlation
• Accelerating BAO Scale Fitting Using Taylor Series
• How to optimally combine pre-reconstruction full shape and post-reconstruction BAO signals
• Weighing Cosmic Structures with Clusters of Galaxies and the Intergalactic Medium
• New tests of dark sector interactions from the full-shape galaxy power spectrum
• Fermionic wave functions and Grassmann fields as possible sources of dark energy
• Testing $\Lambda$CDM with eBOSS data using a model independent diagnostic
• Toward accurate measurement of property-dependent galaxy clustering: II. Tests of the smoothed density-corrected $V_{\max }$ method
• Fermion masses and mixings and $g-2$ muon anomaly in a $Q_6$ flavored 2HDM
• Hubble Tension and Gravitational Self-Interaction
• Mock data sets for the Eboss and DESI Lyman-$\alpha$ forest surveys
• Cosmological measurements from the CMB and BAO are insensitive to the tail probability in the assumed likelihood
• Lepton-flavor changing decays and non-unitarity in the inverse seesaw mechanism
• Testing the robustness of the BAO determination in the presence of massive neutrinos
• Geometry vs growth: Internal consistency of the flat ΛCDM model with KiDS-1000
• Spatial anisotropies from long wavelength scalar and tensor modes
• Improving cosmological constraints via galaxy intrinsic alignment in full-shape analysis
• The cosmological Mass Varying Neutrino model in the late universe
• Cluster optical depth and pairwise velocity estimation using machine learning
• Galaxy Clustering in Harmonic Space from the Dark Energy Survey Year 1 Data: Compatibility with Real-Space Results
• Dark energy constraints in light of theoretical priors
• A New Paradigm for Testing Gravity: Theory-Independent Constraints Using Data From All Astrophysical and Cosmological Scales
• STRAWBERRY: Finding haloes in the gravitational potential
• Holographic dark energy in a coasting cosmology
• Faint galaxies in the Zone of Avoidance revealed by JWST/NIRCam
• Information content in mean pairwise velocity and mean relative velocity between pairs in a triplet
• Illuminating the Dark Sector: Understanding Modified Gravity Signatures with Cross-Correlations of Gravitational Waves and Large-Scale Structure
• Forecasting the Constraint on the Hu-Sawicki $f(R)$ Modified Gravity in the CSST $3\times 2$pt Photometric Survey
• From Nonparametric Distance Reconstruction to Testing the Etherington Relation and Cosmic Curvature Using 2D and 3D BAO Measurements
• Layered dark structure with a Structuring Field: A $Z_4$-symmetric Inert Doublet-Singlet realization and implications for the $S_8$ tension
• Cosmological Constraints on f(T,B) Gravity from Observations of Early and Late Universe
• Evolution of linear matter perturbations with error-bounded bundle physics-informed neural networks
• Dusty Clump Survival in Supernova Ejecta: Dust-Mediated Growth vs. Crushing by the Reverse Shock
• Sub-percentage measure of distances to redshift of 0.1 by a new cosmic ruler
• The Universe at the MeV era: neutrino evolution and cosmological observables
• An emulation-based model for the projected correlation function
• From Geometry to Observation: Gravitational Waves and the Raychaudhuri Equation
• Modified Cosmology from Mass-to-Horizon Relation: Background Evolution
• Hubble tension problem encompassed by phase-space quantum cosmology
• Effects of virtual Majorana neutrinos on charged Lepton Flavor Violation decays from a seesaw variant with radiatively induced light neutrino masses
• Current constraints on the minimally extended varying speed of light model through the cosmic distance duality relation
• The dynamics of background evolution and structure formation in phase space: a semi-cosmographic reconstruction
• Interacting dark energy from redshift-space galaxy clustering
• Revisiting the CMB homogeneity scale: low multipoles removal effect and extragalactic foreground masking
• Gravitational redshift from large-scale structure: nonlinearities, antisymmetries, and the dipole
• How to embed any likelihood into SBI: Application to Planck + Stage IV galaxy surveys and Dynamical Dark Energy
• Merging Galaxy Clusters and the Search for New Physics of Dark Matter: A Review
• An Optimal In-Situ Multipole Algorithm for the Isotropic Three-Point Correlation Functions
• Cosmological Constraints on the DGP Model in light of DESI DR2 2025 Data
• Sample Variance for Supernovae Distance Measurements and the Hubble tension
• Universality of the halo mass function in modified gravity cosmologies
• Cavendish experiment with fast radio bursts on cosmological scales
• Confirming the uniformity of the Hubble flow with Pantheon+ Supernovae
• Matching Bayesian and frequentist coverage probabilities when using an approximate data covariance matrix
• Cosmic voids and BAO with relative baryon-CDM perturbations
• Quantifying Weighted Morphological Content of Large-Scale Structures via Simulation-Based Inference
• Bayesian and Machine-Learning Analyses of Nonminimal $f(Q)$ Gravity and $H_0$ Tension
• Spectral distortions in the decaying QCD dark matter scenario
• Aletheia: Emulating the non-linear matter power spectrum in the context of evolution mapping
• Structural Limitations on Constraining the Time Evolution of Dark Energy
• Encyclopedia of Astrophysics: The Expanding Universe
• Growth rate measurements from a joint analysis of the large-scale galaxy clustering in Fourier and configuration space
• Gamma-Ray Bursts, Supernovae Ia and Baryon Acoustic Oscillations: a binned cosmological analysis
• On the road to percent accuracy VI: the nonlinear power spectrum for interacting dark energy with baryonic feedback and massive neutrinos
• A model-independent test of speed of light variability with cosmological observations
• Cosmic Collider Gravitational Waves sourced by Right-handed Neutrino production from Bubbles: Testing Seesaw, Leptogenesis and Dark Matter
• Clustering redshifts with the 21cm-galaxy cross-bispectrum
• Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension
• An Overview of CHIME, the Canadian Hydrogen Intensity Mapping Experiment
• The Lambert $W$ equation of state in light of DESI BAO
• Light rings, gravitational lensing, and ISCOs of exotic compact objects in Einstein-scalar-Maxwell theories
• Type Ia supernova Hubble diagrams with host galaxy photometric redshifts
• Model-agnostic interpretation of 10 billion years of cosmic evolution traced by BOSS and eBOSS data
• Measurements of cosmic expansion and growth rate of structure from voids in the Sloan Digital Sky Survey between redshift 0.07 and 1.0
• Cosmology in the presence of diffeomorphism-violating, nondynamical background fields
• The Covariance of Photometric and Spectroscopic Two-Point Statistics: Implications for Cosmological Parameter Inference
• Solving small-scale clustering problems in approximate lightcone mocks
• Cosmology with the Redshift-Space Galaxy Bispectrum Monopole at One-Loop Order
• A Quantum Genetic Algorithm with application to Cosmological Parameters Estimation
• A Non-parametric Method for the Inference of Halo Occupation Distributions
• Background dynamics and observational constraints of flat and non-flat $\Lambda (t)$CDM models from $H(z)$ and DESI DR2 BAO measurements
• Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy
• APES: Approximate Posterior Ensemble Sampler
• VarIabiLity seLection of AstrophysIcal sources iN PTF (VILLAIN) I. Structure function fits to 71 million objects
• Enhancing Bispectrum Estimators for Galaxy Redshift Surveys with Velocities
• Optimal data compression for Lyman-$\alpha$ forest cosmology
• Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families
• Statistical consistency of sign-switching vacuum energy with cosmological observations
• $G_3$ -- interacting scalar tensor dark energy
• Testing General Relativity on Galactic Scales via DESI-BAO and Strong Lensing: Circumventing Assumptions on the Hubble Constant, Sound Horizon, and Dark Energy
• Joint Curvature and Growth Rate measurements with Supernova Peculiar Velocities and the CMB
• Beyond the Cosmological Constant: Breaking the Geometric Degeneracy of $f(Q)$ cosmology via Redshift-Space Distortions
• Constraining Early Dark Energy cosmological models with Big Bang Nucleosynthesis
• Geometric Matching of Local Static Regions in Cosmological Spacetimes with an Evolving Lapse
• Void spin distribution as a powerful probe of ${\sigma }_8$
• Neutrino Oscillations in the Three Flavor Paradigm
• Late-time cosmological constraints on three holographic dark energy models with DESI DR2 BAO and Type Ia supernovae