KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints

Abstract

We present a joint cosmological analysis of weak gravitational lensing observations from the Kilo-Degree Survey (KiDS-1000), with redshift-space galaxy clustering observations from the Baryon Oscillation Spectroscopic Survey (BOSS), and galaxy-galaxy lensing observations from the overlap between KiDS-1000, BOSS and the spectroscopic 2-degree Field Lensing Survey (2dFLenS). This combination of large-scale structure probes breaks the degeneracies between cosmological parameters for individual observables, resulting in a constraint on the structure growth parameter $S_8={\sigma }_8\sqrt{{\Omega }_{\mathrm{m}}/0.3}=0.766_{-0.014}^{+0.020}$, that has the same overall precision as that reported by the full-sky cosmic microwave background observations from Planck. The recovered $S_8$ amplitude is low, however, by $8.3\pm 2.6$ % relative to Planck. This result builds from a series of KiDS-1000 analyses where we validate our methodology with variable depth mock galaxy surveys, our lensing calibration with image simulations and null-tests, and our optical-to-near-infrared redshift calibration with multi-band mock catalogues and a spectroscopic-photometric clustering analysis. The systematic uncertainties identified by these analyses are folded through as nuisance parameters in our cosmological analysis. Inspecting the offset between the marginalised posterior distributions, we find that the $S_8$-difference with Planck is driven by a tension in the matter fluctuation amplitude parameter, ${\sigma }_8$. We quantify the level of agreement between the CMB and our large-scale structure constraints using a series of different metrics, finding differences with a significance ranging between $\sim 3\sigma$, when considering the offset in $S_8$, and $\sim 2\sigma$, when considering the full multi-dimensional parameter space.

arXiv comment25 pages, 11 figures, 5 tables, A&A accepted, including a new appendix on Intrinsic Alignments. The KiDS-1000 data products are available for download at http://kids.strw.leidenuniv.nl/DR4/lensing.php. This data release includes open source software, the shear-photo-z catalogue, the cosmic shear and 3x2pt data vectors and covariances, and posteriors in the form of Multinest chains

References in corpus (109)

• The Sloan Digital Sky Survey: Technical Summary
• Efficient Computation of CMB anisotropies in closed FRW models
• Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
• Cosmological parameters from CMB and other data: a Monte-Carlo approach
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
• MultiNest: an efficient and robust Bayesian inference tool for cosmology and particle physics
• The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample
• The Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III
• Weak Gravitational Lensing
• A 2.4% Determination of the Local Value of the Hubble Constant
• Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
• Multimodal nested sampling: an efficient and robust alternative to MCMC methods for astronomical data analysis
• Dark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
• Importance Nested Sampling and the MultiNest Algorithm
• Large-Scale Galaxy Bias
• KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics
• Dark Energy Survey Year 1 Results: Cosmological Constraints from Cosmic Shear
• CFHTLenS tomographic weak lensing cosmological parameter constraints: Mitigating the impact of intrinsic galaxy alignments
• The Atacama Cosmology Telescope: DR4 Maps and Cosmological Parameters
• Galaxy And Mass Assembly (GAMA): end of survey report and data release 2
• Intrinsic alignment-lensing interference as a contaminant of cosmic shear
• Renormalized Cosmological Perturbation Theory
• Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data
• Second Data Release of the Hyper Suprime-Cam Subaru Strategic Program
• Dark energy constraints from cosmic shear power spectra: impact of intrinsic alignments on photometric redshift requirements
• The effects of galaxy formation on the matter power spectrum: A challenge for precision cosmology
• Bayesian Galaxy Shape Measurement for Weak Lensing Surveys - III. Application to the Canada-France-Hawaii Telescope Lensing Survey
• Non-minimal dark sector physics and cosmological tensions
• Gravitational Lensing Analysis of the Kilo Degree Survey
• An accurate halo model for fitting non-linear cosmological power spectra and baryonic feedback models
• CFHTLenS: The Canada-France-Hawaii Telescope Lensing Survey - Imaging Data and Catalogue Products
• Weak lensing for precision cosmology
• Cluster Cosmology Constraints from the 2500 deg${}^2$ SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope
• KiDS+VIKING-450: Cosmic shear tomography with optical+infrared data
• HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
• Quantifying the effect of baryon physics on weak lensing tomography
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: mock galaxy catalogues for the BOSS Final Data Release
• The fourth data release of the Kilo-Degree Survey: ugri imaging and nine-band optical-IR photometry over 1000 square degrees
• Cosmological Model Predictions for Weak Lensing: Linear and Nonlinear Regimes
• CosmoSIS: modular cosmological parameter estimation
• Gravity and Large-Scale Non-local Bias
• KiDS-450 + 2dFLenS: Cosmological parameter constraints from weak gravitational lensing tomography and overlapping redshift-space galaxy clustering
• Core Cosmology Library: Precision Cosmological Predictions for LSST
• Power Spectrum Super-Sample Covariance
• Calibrating Redshift Distributions Beyond Spectroscopic Limits with Cross-Correlations
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Analysis of potential systematics
• Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances and Weak Lensing
• Cosmological constraints from cosmic shear two-point correlation functions with HSC survey first-year data
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Observational systematics and baryon acoustic oscillations in the correlation function
• CFHTLenS revisited: assessing concordance with Planck including astrophysical systematics
• Accurate halo-model matter power spectra with dark energy, massive neutrinos and modified gravitational forces
• Joint Galaxy-Lensing Observables and the Dark Energy
• KiDS+GAMA: Cosmology constraints from a joint analysis of cosmic shear, galaxy-galaxy lensing and angular clustering
• Constraints on intrinsic alignment contamination of weak lensing surveys using the MegaZ-LRG sample
• The Coyote Universe Extended: Precision Emulation of the Matter Power Spectrum
• Analysis of two-point statistics of cosmic shear: I. Estimators and covariances
• Concordance and Discordance in Cosmology
• The MICE Grand Challenge Lightcone Simulation I: Dark matter clustering
• Beyond linear galaxy alignments
• Lensing is Low: Cosmology, Galaxy Formation, or New Physics?
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the configuration-space clustering wedges
• The implications of an extended dark energy cosmology with massive neutrinos for cosmological tensions
• Intrinsic alignments of SDSS-III BOSS LOWZ sample galaxies
• Simultaneous measurement of cosmology and intrinsic alignments using joint cosmic shear and galaxy number density correlations
• Systematic Bias in Cosmic Shear: Beyond the Fisher Matrix
• Cosmology from large-scale structure: Constraining $\Lambda$CDM with BOSS
• KiDS+VIKING-450 and DES-Y1 combined: Cosmology with cosmic shear
• KiDS-1000 catalogue: Redshift distributions and their calibration
• The WiggleZ Dark Energy Survey: Direct constraints on blue galaxy intrinsic alignments at intermediate redshifts
• A halo model for intrinsic alignments of galaxy ellipticities
• KiDS-1000 catalogue: Weak gravitational lensing shear measurements
• Weak lensing with COMBO-17: estimation and removal of intrinsic alignments
• Dark Energy Constraints from Weak Lensing Cross-Correlation Cosmography
• KiDS+VIKING-450 and DES-Y1 combined: Mitigating baryon feedback uncertainty with COSEBIs
• KiDS-1000 Methodology: Modelling and inference for joint weak gravitational lensing and spectroscopic galaxy clustering analysis
• Comprehensive Two-Point Analyses of Weak Gravitational Lensing Surveys
• Photometric Redshift Calibration with Self Organising Maps
• Quantifying tensions in cosmological parameters: Interpreting the DES evidence ratio
• The halo model as a versatile tool to predict intrinsic alignments
• anesthetic: nested sampling visualisation
• Towards emulating cosmic shear data: Revisiting the calibration of the shear measurements for the Kilo-Degree Survey
• Dark Energy Survey Year 1 Results: Constraints on Intrinsic Alignments and their Colour Dependence from Galaxy Clustering and Weak Lensing
• KiDS+GAMA: Intrinsic alignment model constraints for current and future weak lensing cosmology
• An EFT description of galaxy intrinsic alignments
• A hydrodynamical halo model for weak-lensing cross correlations
• The 2-degree Field Lensing Survey: design and clustering measurements
• Arguments against using $h^{-1}\mathrm{Mpc}$ units in observational cosmology
• Cross-Correlation of spectroscopic and photometric galaxy surveys: cosmology from lensing and redshift distortions
• On the road to percent accuracy IV: ReACT -- computing the non-linear power spectrum beyond $\Lambda$CDM
• On the non-linear scale of cosmological perturbation theory
• KiDS+VIKING-450: Improved cosmological parameter constraints from redshift calibration with self-organising maps
• Cosmological constraints from galaxy-lensing cross correlations using BOSS galaxies with SDSS and CMB lensing
• Statistical Inconsistencies in the KiDS-450 Dataset
• Testing KiDS cross-correlation redshifts with simulations
• Quantifying concordance of correlated cosmological data sets
• A Unified Analysis of Four Cosmic Shear Surveys
• 2dFLenS and KiDS: Determining source redshift distributions with cross-correlations
• Blinding multi-probe cosmological experiments
• New perspectives on the BOSS small-scale lensing discrepancy for the Planck $\Lambda$CDM Cosmology
• Consistent cosmic shear in the face of systematics: a B-mode analysis of KiDS-450, DES-SV and CFHTLenS
• Testing gravity using galaxy-galaxy lensing and clustering amplitudes in KiDS-1000, BOSS and 2dFLenS
• Quantifying Suspiciousness Within Correlated Data Sets
• KiDS-i-800: Comparing weak gravitational lensing measurements in same-sky surveys
• GAMA+KiDS: Alignment of galaxies in galaxy groups and its dependence on galaxy scale
• Luminous red galaxies in the Kilo Degree Survey: selection with broad-band photometry and weak lensing measurements
• The Subaru FMOS galaxy redshift survey (FastSound). V. Intrinsic alignments of emission line galaxies at $z\sim 1.4$
• The effects of varying depth in cosmic shear surveys
• Minimising the impact of scale-dependent galaxy bias on the joint cosmological analysis of large scale structures
• A blinding solution for inference from astronomical data

Cited by in corpus (480)

• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory
• Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
• DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
• Challenges for $\Lambda$CDM: An update
• Teleparallel Gravity: From Theory to Cosmology
• The $H_0$ Olympics: A fair ranking of proposed models
• Cosmology Intertwined III: $f{\sigma }_8$ and $S_8$
• Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Data Calibration
• Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Modeling Uncertainty
• Cosmology with the Laser Interferometer Space Antenna
• The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters
• New Horizons for Fundamental Physics with LISA
• The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
• The Atacama Cosmology Telescope: A Measurement of the DR6 CMB Lensing Power Spectrum and its Implications for Structure Growth
• DESI Bright Galaxy Survey: Final Target Selection, Design, and Validation
• The FLAMINGO project: cosmological hydrodynamical simulations for large-scale structure and galaxy cluster surveys
• Is the Observable Universe Consistent with the Cosmological Principle?
• Hyper Suprime-Cam Year 3 Results: Cosmology from Cosmic Shear Power Spectra
• Dark Energy Survey Year 3 Results: Photometric Data Set for Cosmology
• Arbitrating the $S_8$ discrepancy with growth rate measurements from Redshift-Space Distortions
• DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements
• COSMOPOWER: emulating cosmological power spectra for accelerated Bayesian inference from next-generation surveys
• A non-linear solution to the $S_8$ tension?
• A new analysis of galaxy 2-point functions in the BOSS survey, including full-shape information and post-reconstruction BAO
• KiDS-1000 catalogue: Redshift distributions and their calibration
• KiDS-1000 catalogue: Weak gravitational lensing shear measurements
• DESI 2024: Reconstructing Dark Energy using Crossing Statistics with DESI DR1 BAO data
• From galactic bars to the Hubble tension: weighing up the astrophysical evidence for Milgromian gravity
• Relaxing cosmological tensions with a sign switching cosmological constant
• KiDS-1000 Cosmology: constraints beyond flat $\Lambda$CDM
• KiDS-1000 Methodology: Modelling and inference for joint weak gravitational lensing and spectroscopic galaxy clustering analysis
• The Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) Survey Design, Reductions, and Detections
• Cosmological constraints from unWISE and Planck CMB lensing tomography
• Dark Energy at early times and ACT: a larger Hubble constant without late-time priors
• The SRG/eROSITA all-sky survey: Cosmology constraints from cluster abundances in the western Galactic hemisphere
• Running vacuum against the $H_0$ and ${\sigma }_8$ tensions
• Cosmological constraints from the tomographic cross-correlation of DESI Luminous Red Galaxies and Planck CMB lensing
• The Cosmological Constant Problem and Running Vacuum in the Expanding Universe
• Full-shape cosmology analysis of SDSS-III BOSS galaxy power spectrum using emulator-based halo model: a $5\%$ determination of ${\sigma }_8$
• Relaxing cosmological tensions with a sign switching cosmological constant: Improved results with Planck, BAO, and Pantheon data
• Hints of Early Dark Energy in Planck, SPT, and ACT data: new physics or systematics?
• Can late-time extensions solve the $H_0$ and ${\sigma }_8$ tensions?
• Line-Intensity Mapping: Theory Review
• Consistent lensing and clustering in a low-$S_8$ Universe with BOSS, DES Year 3, HSC Year 1 and KiDS-1000
• Hubble tension or a transition of the Cepheid SnIa calibrator parameters?
• Evidence for suppression of structure growth in the concordance cosmological model
• Relieving the $H_0$ tension with a new interacting dark energy model
• Constraints on $\Lambda$CDM Extensions from the SPT-3G 2018 $EE$ and $TE$ Power Spectra
• The growth of density perturbations in the last $\sim$10 billion years from tomographic large-scale structure data
• Cosmology with the EFTofLSS and BOSS: dark energy constraints and a note on priors
• Joint constraints on cosmology and the impact of baryon feedback: combining KiDS-1000 lensing with the thermal Sunyaev-Zeldovich effect from Planck and ACT
• Hyper Suprime-Cam Year 3 Results: Cosmology from Galaxy Clustering and Weak Lensing with HSC and SDSS using the Minimal Bias Model
• The three-year shear catalog of the Subaru Hyper Suprime-Cam SSP Survey
• Ultra-light axions and the $S_8$ tension: joint constraints from the cosmic microwave background and galaxy clustering
• Quantifying the global parameter tensions between ACT, SPT and Planck
• Cosmic Shear Cosmology Beyond 2-Point Statistics: A Combined Peak Count and Correlation Function Analysis of DES-Y1
• The Sigma-8 Tension is a Drag
• Dark Sector to Restore Cosmological Concordance
• Dark Energy Survey Year 3 Results: Galaxy clustering and systematics treatment for lens galaxy samples
• Cosmology From CMB Lensing and Delensed EE Power Spectra Using 2019-2020 SPT-3G Polarization Data
• Consistency of effective field theory analyses of the BOSS power spectrum
• DES Y3 cosmic shear down to small scales: constraints on cosmology and baryons
• Updated constraints from the effective field theory analysis of BOSS power spectrum on Early Dark Energy
• Observational constraints on the deceleration parameter in a tilted universe
• Nuw CDM cosmology from the weak lensing convergence PDF
• Flavor-specific Interaction Favors Strong Neutrino Self-coupling in the Early Universe
• Revealing the effects of curvature on the cosmological models
• The Weak Lensing Radial Acceleration Relation: Constraining Modified Gravity and Cold Dark Matter theories with KiDS-1000
• Linear cosmological constraints on 2-body decaying dark matter scenarios and the $S_8$ tension
• KiDS-1000: cosmic shear with enhanced redshift calibration
• SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field
• Quantifying the $S_8$ tension and evidence for interacting dark energy from redshift-space distortion measurements
• Euclid Preparation. XXVIII. Forecasts for ten different higher-order weak lensing statistics
• Testing AdS early dark energy with Planck, SPTpol and LSS data
• A double take on early and interacting dark energy from JWST
• Unveiling dark fifth forces with linear cosmology
• Dark Energy Survey Year 3 Results: High-precision measurement and modeling of galaxy-galaxy lensing
• Model-independent cosmological inference post DESI DR1 BAO measurements
• Galaxy bias from forward models: linear and second-order bias of IllustrisTNG galaxies
• Health checkup test of the standard cosmological model in view of recent Cosmic Microwave Background Anisotropies experiments
• New Roads to the Small-Scale Universe: Measurements of the Clustering of Matter with the High-Redshift UV Galaxy Luminosity Function
• Bright galaxy sample in the Kilo-Degree Survey Data Release 4: selection, photometric redshifts, and physical properties
• Euclid preparation: XIX. Impact of magnification on photometric galaxy clustering
• Multidimensionality of the Hubble tension: the roles of ${\Omega }_m$ and ${\omega }_c$
• SP(k) -- A hydrodynamical simulation-based model for the impact of baryon physics on the non-linear matter power spectrum
• A Step in Understanding the $S_8$ Tension
• Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter
• How much information can be extracted from galaxy clustering at the field level?
• Mirror Twin Higgs Cosmology: Constraints and a Possible Resolution to the $H_0$ and $S_8$ Tensions
• Neural Network Reconstruction of Late-Time Cosmology and Null Tests
• KiDS-1000: Combined halo-model cosmology constraints from galaxy abundance, galaxy clustering and galaxy-galaxy lensing
• The Atacama Cosmology Telescope: Cosmology from cross-correlations of unWISE galaxies and ACT DR6 CMB lensing
• Model-independent measurement of cosmic curvature with the latest $H(z)$ and SNe Ia data: A comprehensive investigation
• Hefty enhancement of cosmological constraints from the DES Y1 data using a Hybrid Effective Field Theory approach to galaxy bias
• Is the Harrison-Zel'dovich spectrum coming back? ACT preference for $n_s\sim 1$ and its discordance with Planck
• Cosmological cross-correlations and nearest neighbor distributions
• Strong detection of the CMB lensingxgalaxy weak lensingcross-correlation from ACT-DR4,PlanckLegacy and KiDS-1000
• KiDS & Euclid: Cosmological implications of a pseudo angular power spectrum analysis of KiDS-1000 cosmic shear tomography
• Return of Harrison-Zeldovich spectrum in light of recent cosmological tensions
• Bayesian evidence for the tensor-to-scalar ratio $r$ and neutrino masses $m_{\nu }$: Effects of uniform vs logarithmic priors
• Evaluating bulk flow estimators for CosmicFlows-4 measurements
• Consistency of Planck, ACT and SPT constraints on magnetically assisted recombination and forecasts for future experiments
• Growth of Cosmic Structure
• Euclid. V. The Flagship galaxy mock catalogue: a comprehensive simulation for the Euclid mission
• Investigating Deep Learning Methods for Obtaining Photometric Redshift Estimations from Images
• What it takes to solve the Hubble tension through modifications of cosmological recombination
• Cosmic shear with small scales: DES-Y3, KiDS-1000 and HSC-DR1
• Testing Gravity on Cosmic Scales: A Case Study of Jordan-Brans-Dicke Theory
• On the road to percent accuracy V: the non-linear power spectrum beyond $\Lambda$CDM with massive neutrinos and baryonic feedback
• KiDS-1000: Cosmology with improved cosmic shear measurements
• Cosmological Constraint Precision of the Photometric and Spectroscopic Multi-probe Surveys of China Space Station Telescope (CSST)
• A Bayesian interpretation of inconsistency measures in cosmology
• Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions
• On the dynamics of a dark sector coupling
• Aemulus $\nu$: Precise Predictions for Matter and Biased Tracer Power Spectra in the Presence of Neutrinos
• Dark Energy Survey Year 3 results: cosmology from combined galaxy clustering and lensing -- validation on cosmological simulations
• $\kappa$TNG: Effect of Baryonic Processes on Weak Lensing with IllustrisTNG Simulations
• Photometric selection and redshifts for quasars in the Kilo-Degree Survey Data Release 4
• Quantifying the global "CMB tension" between the Atacama Cosmology Telescope and the Planck satellite in extended models of cosmology
• Cross-correlating dark sirens and galaxies: constraints on $H_0$ from GWTC-3 of LIGO-Virgo-KAGRA
• Weak Lensing Tomographic Redshift Distribution Inference for the Hyper Suprime-Cam Subaru Strategic Program three-year shape catalogue
• Phenomenological emergent dark energy in the light of DESI Data Release 1
• Axi-Higgs Cosmology
• KiDS-Legacy calibration: unifying shear and redshift calibration with the SKiLLS multi-band image simulations
• Beyond $\Lambda$CDM constraints from the full shape clustering measurements from BOSS and eBOSS
• 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
• Priors on red galaxy stochasticity from hybrid effective field theory
• The DES view of the Eridanus supervoid and the CMB Cold Spot
• Full-shape BOSS constraints on dark matter interacting with dark radiation and lifting the $S_8$ tension
• Probing dark energy with tomographic weak-lensing aperture mass statistics
• Evidence for a high-z ISW signal from supervoids in the distribution of eBOSS quasars
• Constraints on $S_8$ from a full-scale and full-shape analysis of redshift-space clustering and galaxy-galaxy lensing in BOSS
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• Small-scale clumping at recombination and the Hubble tension
• The MillenniumTNG Project: The impact of baryons and massive neutrinos on high-resolution weak gravitational lensing convergence maps
• Magnification bias in galaxy surveys with complex sample selection functions
• Dark Energy Survey internal consistency tests of the joint cosmological probes analysis with posterior predictive distributions
• Model-independent constraints on ${\Omega }_m$ and $H(z)$ from the link between geometry and growth
• Stepped Partially Acoustic Dark Matter, Large Scale Structure, and the Hubble Tension
• Testing dark energy after pre-recombination early dark energy
• CosmoGridV1: a simulated $w$CDM theory prediction for map-level cosmological inference
• Confronting interacting dark radiation scenarios with cosmological data
• Mixed dark matter: matter power spectrum and halo mass function
• Modified gravity and massive neutrinos: constraints from the full shape analysis of BOSS galaxies and forecasts for Stage IV surveys
• Do you smell something decaying? Updated linear constraints on decaying dark matter scenarios
• Dark Energy Survey Year 3 results: Marginalisation over redshift distribution uncertainties using ranking of discrete realisations
• Constraining primordial non-Gaussianity from DESI quasar targets and Planck CMB lensing
• The foreground transfer function for HI intensity mapping signal reconstruction: MeerKLASS and precision cosmology applications
• Constraining cosmology with a new all-sky Compton parameter map from the Planck PR4 data
• Self-calibration of weak lensing systematic effects using combined two- and three-point statistics
• Persistent homology in cosmic shear II: A tomographic analysis of DES-Y1
• $5\sigma$ tension between Planck cosmic microwave background and eBOSS Lyman-alpha forest and constraints on physics beyond $\Lambda$CDM
• Observational constraints and predictions of the interacting dark sector with field-fluid mapping
• Cosmological constraints from HSC survey first-year data using deep learning
• Dark Energy as a Critical Phenomenon: a Resolution for Hubble Tension
• KiDS-Legacy: Consistency of cosmic shear measurements and joint cosmological constraints with external probes
• An exploration of an early gravity transition in light of cosmological tensions
• Constraining spatial curvature with large-scale structure
• Sources of $H_0$-tensions in dark energy scenarios
• KiDS-1000 cosmology: Combined second- and third-order shear statistics
• From infinite to infinitesimal: Using the Universe as a dataset to probe Casimir corrections to the vacuum energy from fields inhabiting the dark dimension
• Backreaction in Cosmology
• The weak, the strong and the ugly -- A comparative analysis of interacting stepped dark radiation
• Probing Early Modification of Gravity with Planck, ACT and SPT
• Cosmological inference from emulator based halo model I: Validation tests with HSC and SDSS mock catalogs
• KiDS-SBI: Simulation-based inference analysis of KiDS-1000 cosmic shear
• On the consistency of $\Lambda$CDM with CMB measurements in light of the latest Planck, ACT, and SPT data
• The perspective of voids on rising cosmology tensions
• Modeling Nearest Neighbor distributions of biased tracers using Hybrid Effective Field Theory
• Constraints on anisotropic primordial non-Gaussianity from intrinsic alignments of SDSS-III BOSS galaxies
• Dark energy and matter interacting scenario to relieve $H_0$ and $S_8$ tensions
• Minimal theory of massive gravity in the light of CMB data and the $S_8$ tension
• Forecast of Neutrino Cosmology from the CSST Photometric Galaxy Clustering and Cosmic Shear Surveys
• Probing galaxy bias and intergalactic gas pressure with KiDS Galaxies-tSZ-CMB lensing cross-correlations
• Implications of an extended dark energy model with massive neutrinos
• The Cosmic Baryon Partition between the IGM and CGM in the SIMBA Simulations
• Cosmological constraints on early dark energy from the full shape analysis of eBOSS DR16
• KiDS-1000 Cosmology: Constraints from density split statistics
• New late-time constraints on $f(R)$ gravity
• The Corona Borealis supercluster: connectivity, collapse, and evolution
• Minimal theory of massive gravity and constraints on the graviton mass
• Quintessential Cosmological Tensions
• Evidence of Galaxy Assembly Bias in SDSS DR7 Galaxy Samples from Count Statistics
• A roadmap to cosmological parameter analysis with third-order shear statistics I: Modelling and validation
• Starlet l1-norm for weak lensing cosmology
• Organised Randoms: Learning and correcting for systematic galaxy clustering patterns in KiDS using self-organising maps
• Modeling Intrinsic Galaxy Alignment in the MICE Simulation
• First Identification of a CMB Lensing Signal Produced by $1.5$ Million Galaxies at $z\sim$4: Constraints on Matter Density Fluctuations at High Redshift
• KaRMMa -- Kappa Reconstruction for Mass Mapping
• Redshift requirements for cosmic shear with intrinsic alignment
• The FLAMINGO project: Baryon effects on the matter power spectrum
• Consistency of cosmic shear analyses in harmonic and real space
• Cosmological constraints from the cross-correlation of DESI Luminous Red Galaxies with CMB lensing from Planck PR4 and ACT DR6
• Dark matter solution to the $H_0$ and $S_8$ tensions, and the integrated Sachs-Wolfe void anomaly
• Consistent and simultaneous modelling of galaxy clustering and galaxy-galaxy lensing with Subhalo Abundance Matching
• Field-level inference of galaxy intrinsic alignment from the SDSS-III BOSS survey
• Probing Modified Gravity with Integrated Sachs-Wolfe CMB and Galaxy Cross-correlations
• Consistency tests between SDSS and DESI BAO measurements
• Measuring the Hubble Constant with cosmic chronometers: a machine learning approach
• Testing one-loop galaxy bias: cosmological constraints from the power spectrum
• KiDS-1000 Cosmology: machine learning -- accelerated constraints on Interacting Dark Energy with COSMOPOWER
• Constraining Self-Interacting Dark Matter with Dwarf Spheroidal Galaxies and High-resolution Cosmological $N$-body Simulations
• Cross-correlation of Planck CMB lensing with DESI galaxy groups
• On cosmological bias due to the magnification of shear and position samples in modern weak lensing analyses
• Dark Sectors with Mass Thresholds Face Cosmological Datasets
• Cosmological Studies from HSC-SSP Tomographic Weak Lensing Peak Abundances
• Unified and consistent structure growth measurements from joint ACT, SPT and \textit{Planck} CMB lensing
• HYMALAIA: A Hybrid Lagrangian Model for Intrinsic Alignments
• Reconciling $S_8$: Insights from Interacting Dark Sectors
• IDECAMB: an implementation of interacting dark energy cosmology in CAMB
• Pseudoscalar sterile neutrino self-interactions in light of Planck, SPT and ACT data
• The $S_8$ Tension in Light of Updated Redshift-Space Distortion Data and PAge Approximation
• Constraining constant and tomographic coupled dark energy with low-redshift and high-redshift probes
• The matter density PDF for modified gravity and dark energy with Large Deviations Theory
• Cosmology from weak lensing alone and implications for the Hubble tension
• Revisiting the dynamics of interacting vector-like dark energy
• The thermalisation of massive galaxy clusters
• Galaxy morphoto-Z with neural Networks (GaZNets). I. Optimized accuracy and outlier fraction from Imaging and Photometry
• A Composite Likelihood Approach for Inference under Photometric Redshift Uncertainty
• A simulation-based inference pipeline for cosmic shear with the Kilo-Degree Survey
• Towards a full $w$CDM map-based analysis for weak lensing surveys
• Static, spherically symmetric objects in Type-II minimally modified gravity
• Evolution mapping: a new approach to describe matter clustering in the non-linear regime
• When tension is just a fluctuation: How noisy data affect model comparison
• Phenomenological Gravitational Phase Transition: Reconciliation between the Late and Early Universe
• An exponential equation of state of dark energy in the light of 2018 CMB Planck data
• Analytical marginalisation over photometric redshift uncertainties in cosmic shear analyses
• Impact of survey geometry and super-sample covariance on future photometric galaxy surveys
• Towards alleviating the $H_0$ and $S_8$ tensions with Early Dark Energy - Dark Matter drag
• Cosmology from weak lensing, galaxy clustering, CMB lensing and tSZ: I. 10x2pt Modelling Methodology
• A null test of the Cosmological Principle with BAO measurements
• Addressing Cosmological Tensions by Non-Local Gravity
• Observational constraints on soft dark energy and soft dark matter: challenging $\Lambda$CDM
• BeyondPlanck XII. Cosmological parameter constraints with end-to-end error propagation
• Magnification Bias Estimators for Realistic Surveys: an Application to the BOSS Survey
• KiDS-1000: cross-correlation with Planck cosmic microwave background lensing and intrinsic alignment removal with self-calibration
• DESI Legacy Imaging Surveys Data Release 9: Cosmological Constraints from Galaxy Clustering and Weak Lensing using the Minimal Bias Model
• Neutrino mass tension or suppressed growth rate of matter perturbations?
• Cosmological Probes of Structure Growth and Tests of Gravity
• Cosmology in Minkowski space
• Cosmic Growth in $f(T)$ Teleparallel Gravity
• Altered Axion Abundance from a Dynamical Peccei-Quinn Scale
• New cosmological constraints on the evolution of dark matter energy density
• Exploring Mirror Twin Higgs Cosmology with Present and Future Weak Lensing Surveys
• Phase-space analysis of dark energy models in non-minimally coupled theories of gravity
• Testing the Cosmic Distance Duality Relation Using Strong Gravitational Lensing Time Delays and Type Ia Supernovae
• Observational constraints on interacting vacuum energy with linear interactions
• Exploring the Growth Index ${\gamma }_L$: Insights from Different CMB Dataset Combinations and Approaches
• Constraining the galaxy-halo connection of infrared-selected unWISE galaxies with galaxy clustering and galaxy-CMB lensing power spectra
• Clustering of red-sequence galaxies in the fourth data release ofthe Kilo-Degree Survey
• Transitioning from Stage-III to Stage-IV: Cosmology from galaxy$\times$CMB lensing and shear$\times$CMB lensing
• Euclid preparation. The Cosmic Dawn Survey (DAWN) of the Euclid Deep and Auxiliary Fields
• Closing up the cluster tension?
• Thin-wall vacuum decay in the presence of a compact dimension meets the $H_0$ and $S_8$ tensions
• Effects of galaxy intrinsic alignment on weak lensing peak statistics
• BAO cosmology in non-spatially flat background geometry from BOSS+eBOSS and lessons for future surveys
• Photometric redshifts and intrinsic alignments: degeneracies and biases in 3$\times$2pt analysis
• Cosmology from Cross-Correlation of ACT-DR4 CMB Lensing and DES-Y3 Cosmic Shear
• A multitracer analysis for the eBOSS galaxy sample based on the effective field theory of large-scale structure
• Early dark energy constraints with late-time expansion marginalization
• Non-thermal neutrino-like hot dark matter in light of the $S_8$ tension
• A revised density split statistic model for general filters
• Holographic energy density, dark energy sound speed, and tensions in cosmological parameters: $H_0$ and $S_8$
• Simulation-based inference of deep fields: galaxy population model and redshift distributions
• Impact of stellar population synthesis choices on forward modelling-based redshift distribution estimates
• Linear matter density perturbations in the ${\Lambda }_{\mathrm{s}}$CDM model: Examining growth dynamics and addressing the $S_8$ tension
• Testing the growth rate in homogeneous and inhomogeneous interacting vacuum models
• CMB lensing in a modified $\Lambda$CDM model in light of the $H_0$ tension
• Euclid preparation. LIII. LensMC, weak lensing cosmic shear measurement with forward modelling and Markov Chain Monte Carlo sampling
• A fully data-driven algorithm for accurate shear estimation
• Conformally and Disformally Coupled Vector field Models of Dark Energy
• Dark Degeneracy in DESI DR2: Interacting or Evolving Dark Energy?
• A visual tool for assessing tension-resolving models in the $H_0$-${\sigma }_8$ plane
• Dissecting kinetically coupled quintessence: phenomenology and observational tests
• One-parameter dynamical dark-energy from the generalized Chaplygin gas
• Galaxy Clustering in the Mira-Titan Universe I: Emulators for the redshift space galaxy correlation function and galaxy-galaxy lensing
• Early-time thermalization of cosmic components? A hint for solving cosmic tensions
• Signatures of Light Massive Relics on nonlinear structure formation
• Do we need wavelets in the late Universe?
• Galaxy blending effects in deep imaging cosmic shear probes of cosmology
• Improving Photometric Redshift Estimates with Training Sample Augmentation
• Impact of tidal environment on galaxy clustering in GAMA
• Imprint of baryons and massive neutrinos on velocity statistics
• Comprehensive Constraints on Dark Radiation Injection After BBN
• Cosmology from LOFAR Two-metre Sky Survey Data Release 2: Cross-correlation with the cosmic microwave background
• Shan--Chen interacting vacuum cosmology
• Cosmological feedback from a halo assembly perspective
• A representation learning approach to probe for dynamical dark energy in matter power spectra
• Self-interacting neutrinos, the Hubble parameter tension, and the Cosmic Microwave Background
• Late Time Modification of Structure Growth and the S8 Tension
• Gravitino Cosmology Helped by a Right Handed (S)Neutrino
• Constraining the physics of star formation from CIB-cosmic shear cross-correlations
• Cosmological implications of tracker scalar fields: Testing the evidence for dynamical dark energy with recent data
• ${\Lambda }_{\mathrm{s}}$CDM cosmology from a type-II minimally modified gravity
• The interacting vacuum and tensions: a comparison of theoretical models
• Constraints on dark matter and astrophysics from tomographic $\gamma$-ray cross-correlations
• KiDS-Legacy: Covariance validation and the unified OneCovariance framework for projected large-scale structure observables
• Interacting dark energy constraints from the full-shape analyses of BOSS DR12 and DES Year 3 measurements
• Cosmology with Galaxy Cluster Properties using Machine Learning
• A roadmap to cosmological parameter analysis with third-order shear statistics II: Analytic covariance estimate
• Forecast of cross-correlation of CSST cosmic shear tomography with AliCPT-1 CMB lensing
• Probing Dark Relativistic Species and Their Interactions with Dark Matter through CMB and 21cm surveys
• Probing interacting dark sector models with future weak lensing-informed galaxy cluster abundance constraints from SPT-3G and CMB-S4
• Mitigating baryonic effects with a theoretical error covariance
• I. Linear Interacting Dark Energy: Analytical Solutions and Theoretical Pathologies
• Coupled Quintessence scalar field model in light of observational datasets
• Quintessential Implications of the presence of AdS in the Dark Energy sector
• Euclid preparation. LIX. Angular power spectra from discrete observations
• Tensions in cosmology: a discussion of statistical tools to determine inconsistencies
• Tracking the validity of the quasi-static and sub-horizon approximations in modified gravity
• Dark Energy Survey Year 3 Results: Constraints on cosmological parameters and galaxy bias models from galaxy clustering and galaxy-galaxy lensing using the redMaGiC sample
• Modern Cosmology, an Amuse-Gueule
• Measuring the matter fluctuations in the Local Universe with the ALFALFA catalog
• Can acoustic and axion-like early dark energy still resolve the Hubble tension?
• On constraining Cosmology and the Halo Mass Function with Weak Gravitational Lensing
• The CIDER simulations: Nonlinear structure formation in the Constrained Interacting Dark Energy Scenario
• The impact of 2D and 3D BAO measurements on the Cosmic Distance Duality Relation with HII galaxies
• Axi-Higgs cosmology: Cosmic Microwave Background and cosmological tensions
• Halo Growth and Merger Rates as a Cosmological Test
• Improved Tomographic Binning of 3x2pt Lens Samples: Neural Network Classifiers and Optimal Bin Assignments
• A Systematic Study of Projection Biases in Weak Lensing Analysis
• KiDS-Legacy: Angular galaxy clustering from deep surveys with complex selection effects
• The CMB lensing imprint of cosmic voids detected in the WISE-Pan-STARRS luminous red galaxy catalog
• Examining the validity of the minimal varying speed of light model through cosmological observations: relaxing the null curvature constraint
• Unveiling the Universe with Emerging Cosmological Probes
• Growth and Geometry Split in Light of the DES-Y3 Survey
• Dynamics of dark energy in a scalar-vector-torsion theory
• Non-parametric reconstructions of cosmic curvature: current constraints and forecasts
• Difficulties in reconciling non-negligible differences between the local and cosmological values of the gravitational coupling in extended Brans-Dicke theories
• The DAMIC-M Low Background Chamber
• Reconstructing the parameter space of non-analytical cosmological fixed points
• Can Baby Universe Absorption Explain Dark Energy?
• Enhancing Photometric Redshift Catalogs Through Color-Space Analysis: Application to KiDS-Bright Galaxies
• What is the super-sample covariance? A fresh perspective for second-order shear statistics
• Starlet higher order statistics for galaxy clustering and weak lensing
• What does a cosmological experiment really measure? Covariant posterior decomposition with normalizing flows
• Field-level multiprobe analysis of the CMB, integrated Sachs-Wolfe effect, and the galaxy density maps
• Combining cosmic shear data with correlated photo-$z$ uncertainties: constraints from DESY1 and HSC-DR1
• Cosmological parameters from Planck data in SU(2)${}_{\mathrm{CMB}}$, their local $\Lambda$CDM values, and the modified photon Boltzmann equation
• Cluster Assembly Times as a Cosmological Test
• Current and Future constraints on single-field $\alpha$-Attractor model
• Lensing amplitude anomaly and varying electron mass alleviate the Hubble and $S_8$ tensions
• Prospects for disentangling dark matter with weak lensing
• The X-ray Angular Power Spectrum of Extended Sources in the eROSITA Final Equatorial Depth Survey
• Cosmic star formation history with tomographic cosmic infrared background-galaxy cross-correlation
• Constraining cosmological parameters using void statistics from the SDSS survey
• Accurate method for ultralight axion CMB and matter power spectra
• Measuring the speed of light with cosmological observations: current constraints and forecasts
• Mitigating baryon feedback bias in cosmic shear through a theoretical error covariance in the matter power spectrum
• CFHTLenS: Galaxy bias as function of scale, stellar mass, and colour. Conflicts with predictions by semi-analytic models
• Non-local contribution from small scales in galaxy-galaxy lensing: Comparison of mitigation schemes
• Impact of the primordial fluctuation power spectrum on the reionization history
• Constraining Hot Dark Matter Sub-Species with Weak Lensing and the Cosmic Microwave Background Radiation
• Fluctuating Dark Energy and the Luminosity Distance
• Dynamics of Inspiraling Dark Energy
• Tomographic cross correlations between galaxy surveys and the CMB gravitational lensing potential. Effect of the redshift bin mismatch
• Testing Quadratic Maximum Likelihood estimators for forthcoming Stage-IV weak lensing surveys
• Impact of weak lensing on bright standard siren analyses
• Kinematic Lensing with the Roman Space Telescope
• Cosmology and Astrophysics with the Diffuse eRASS1 X-ray Angular Power Spectrum
• Pure-mode correlation functions for cosmic shear and application to KiDS-1000
• Inflation in non-local hybrid metric-Palatini gravity
• Cosmological constraints from galaxy clustering and galaxy-galaxy lensing with extended SubHalo Abundance Matching
• Exponential quintessence with momentum coupling to dark matter
• Convergent Bayesian Global Fits of 4D Composite Higgs Models
• Dynamical Dark Energy and the Unresolved Hubble Tension: Multi-model Constraints from DESI 2025 and Other Probes
• Covariances of density probability distribution functions. Lessons from hierarchical models
• Early dark energy in the pre- and post-recombination epochs
• The COSMOS-Web Lens Survey (COWLS) III: forecasts versus data
• Cool dark sector, concordance, and a low ${\sigma }_8$
• Informed total-error-minimizing priors: Interpretable cosmological parameter constraints despite complex nuisance effects
• The Velocity Field Olympics: Assessing velocity field reconstructions with direct distance tracers
• $\Lambda$CDM and early dark energy in latent space: a data-driven parametrization of the CMB temperature power spectrum
• Star-Crossed Labours: Checking Consistency Between Current Supernovae Compilations
• Weak Lensing Constraints on Dark Matter-Baryon Interactions with $N$-Body Simulations and Machine Learning
• Numerical implementation of the Cubic Galileon model in PINOCCHIO
• Dark Matter-Radiation Scattering Enhances CMB Phase Shift through Dark Matter-loading
• AMICO galaxy clusters in KiDS-DR3: constraints on $\Lambda$CDM from extreme value statistics
• Intrinsic alignments of the extended radio continuum emission of galaxies in the EAGLE simulations
• Optimizing Redshift Distribution Inference through Joint Self-Calibration and Clustering-Redshift Synergy
• Testing the coupling of dark radiations in light of the Hubble tension
• Constraints on Tsallis cosmology using recent low and high redshift measurements
• Model independent variance cancellation in CMB lensing cross-correlations
• Photometric calibration in u-band using blue halo stars
• KiDS-Legacy: Constraints on Horndeski gravity from weak lensing combined with galaxy clustering and cosmic microwave background anisotropies
• Non-linear Eulerian Hydrodynamics of Dark Energy: Riemann problem and Finite Volume Schemes
• Weak Gravitational Lensing
• Screening fifth forces in scalar-vector-tensor theories
• Improving Galaxy Cluster Selection with the Outskirt Stellar Mass of Galaxies
• Model-Agnostic Cosmological Inference with SDSS-IV eBOSS: Simultaneous Probing for Background and Perturbed Universe
• Weak lensing peak statistics -- steepness versus height
• KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing
• Mapping Variations of Redshift Distributions with Probability Integral Transforms
• Cosmological Constraints with Void Lensing I: the Simulation-Based Inference Framework
• A frequentist view on the two-body decaying dark matter model
• The RSD Sorting Hat: Unmixing Radial Scales in Projection
• Euclid preparation. Improving cosmological constraints using a new multi-tracer method with the spectroscopic and photometric samples
• Disentangling the Halo: Joint Model for Measurements of the Kinetic Sunyaev-Zeldovich Effect and Galaxy-Galaxy Lensing
• Interacting dark sector with quadratic coupling: theoretical and observational viability
• The Gravitational Lensing Imprints of DES Y3 Superstructures on the CMB: A Matched Filtering Approach
• Intrinsic alignment from multiple shear estimates: A first application to data and forecasts for Stage IV
• Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: ${\Lambda }_{\mathrm{s}}$CDM versus $\Lambda$CDM
• Assembly bias in quadratic bias parameters of dark matter halos from forward modeling
• The frozen vanilla model: Exploring dark sector interactions with delta effective theories
• The AIDA-TNG project: 3D halo shapes
• Role of Spatial Curvature in a Dark Energy Interacting Model
• Results and forecasts on cosmic inflation from weak lensing
• On the Outskirts of Dark Matter Haloes
• Impact of Large-Scale Structure Systematics on Cosmological Parameter Estimation
• Bounds on galaxy stochasticity from halo occupation distribution modeling
• Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints
• Parameter inference with non-linear galaxy clustering: accounting for theoretical uncertainties
• Stirring the cosmic pot: how black hole feedback shapes the matter power spectrum in the Fable simulations
• Data-driven Cosmology from Three-dimensional Light Cones
• 6x2pt: Forecasting gains from joint weak lensing and galaxy clustering analyses with spectroscopic-photometric galaxy cross-correlations
• Line-of-sight effects on double source plane lenses
• Dark Energy Survey Year 3 results: Galaxy-halo connection from galaxy-galaxy lensing
• Mapping luminous and dark matter in the Universe
• Do JWST reionization (optical depth) puzzle, cosmological tensions, and CMB anomalies imply Harrison-Zel'dovich spectrum?
• On the tomographic cluster clustering as a cosmological probe
• Lensing Without Borders. I. A Blind Comparison of the Amplitude of Galaxy-Galaxy Lensing Between Independent Imaging Surveys
• Weighing Cosmic Structures with Clusters of Galaxies and the Intergalactic Medium
• Galaxy clustering in modified gravity from full-physics simulations. I: two-point correlation functions
• One Galaxy Sample to Rule Them All: Halo Occupation Distribution Modeling of DES Year 3 Source Galaxies
• Cosmological constraints on mass-varying dark matter
• Constraining decaying dark matter with BOSS data and the effective field theory of large-scale structures
• Momentum transfer models of interacting dark energy
• Apparent $w<-1$ and a Lower $S_8$ from Dark Axion and Dark Baryons Interactions
• A New Wavelet Scattering Transform-Based Statistic for Cosmological Analysis of Large-Scale Structure
• Probing Time-Varying Dark Energy with DESI: The Crucial Role of Precision Matter Density (Ω_{m0}) Measurements
• Denoising weak lensing mass maps with diffusion model: systematic comparison with generative adversarial network
• Power Spectrum Emulators from Neural Networks and Tree-Based Methods
• Cosmological measurements from the CMB and BAO are insensitive to the tail probability in the assumed likelihood
• Galaxy Clustering in Harmonic Space from the Dark Energy Survey Year 1 Data: Compatibility with Real-Space Results
• STRAWBERRY: Finding haloes in the gravitational potential
• A step in the right direction? Analyzing the Wess Zumino Dark Radiation solution to the Hubble tension
• First measurement of the Hubble constant from a combined weak lensing and gravitational-wave standard siren analysis
• From Nonparametric Distance Reconstruction to Testing the Etherington Relation and Cosmic Curvature Using 2D and 3D BAO Measurements
• Exploring Late-Time Cosmic Acceleration in VCDM Cosmology
• Layered dark structure with a Structuring Field: A $Z_4$-symmetric Inert Doublet-Singlet realization and implications for the $S_8$ tension
• Dusty Clump Survival in Supernova Ejecta: Dust-Mediated Growth vs. Crushing by the Reverse Shock
• Revisiting Galaxy Cluster Scaling Relations through Dark Matter-Gas Coherence: Scatter Dependence on Dynamical State
• Cosmic backgrounds from the radio to the far-infrared: recent results and perspectives from cosmological and astrophysical surveys
• Effective $\Lambda$CDM model emerging from $f(Q,T)$ under a special EOS limit in symmetric cosmology with Bayesian and ANN observational constraints
• The Covariance of Photometric and Spectroscopic Two-Point Statistics: Implications for Cosmological Parameter Inference
• Replicating weak-lensing summary-statistic covariances with normalizing flows
• Non-Gaussian likelihood of weak lensing power spectra
• Interacting dark energy from redshift-space galaxy clustering
• Response approach to the integrated shear 3-point correlation function: the impact of baryonic effects on small scales
• 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
• Redshift Duality with Pantheon+SH0ES in a Planck-anchored Flat $\Lambda$CDM Framework: Implications for Hubble Tension and Observational Inference
• Geometric Matching of Local Static Regions in Cosmological Spacetimes with an Evolving Lapse
• Revisiting the equation of state of dark energy from DESI BAO with SNe Ia and CMB
• Signatures of Extended Dark Energy Parametrisations in Structure Formation under Background Constraints
• Advancing weak lensing mass mapping with a mask-aware HEALPix transformer
• Emulating redshift mixing due to blending in weak gravitational lensing
• Improving Photometric Galaxy Clustering Constraints With Cross-Bin Correlations
• A model-independent test of speed of light variability with cosmological observations
• Dark Energy Survey Year 3 results: Cosmology with peaks using an emulator approach
• Cosmological implications of the full shape of anisotropic clustering measurements in BOSS and eBOSS
• FuGa3D: Fast full-sky analysis of Galaxy catalogs in 3D
• On the road to percent accuracy VI: the nonlinear power spectrum for interacting dark energy with baryonic feedback and massive neutrinos
• Current constraints on the minimally extended varying speed of light model through the cosmic distance duality relation
• Superhorizon isocurvature fluctuations relax tensions
• Matching Bayesian and frequentist coverage probabilities when using an approximate data covariance matrix
• Testing the growth of cosmic structures during the Dark Ages
• Interpretability of deep-learning methods applied to large-scale structure surveys
• Halo spin and orientation in Interacting Dark Matter Dark Energy Cosmology
• Void spin distribution as a powerful probe of ${\sigma }_8$
• Complete Classification of Analytical Models in Einstein-Aether Cosmology
• Cosmology with the Roman Space Telescope -- Synergies with CMB lensing
• Cross-correlations between mm-wave line-intensity mapping and weak lensing surveys: preliminary consideration of long-term prospects
• Non-linear infusion of intrinsic alignment and source clustering: impact on non-Gaussian cosmic shear statistics
• An effective fluid description of scalar-vector-tensor theories under the sub-horizon and quasi-static approximations
• Bayesian and Machine-Learning Analyses of Nonminimal $f(Q)$ Gravity and $H_0$ Tension
• Spectral distortions in the decaying QCD dark matter scenario
• Systematics mitigation for catalogue-based angular power spectra
• Intrinsic alignments of galaxies in multiple projections
• Detecting Local and Integrated Relativistic Effects by Multi-Tracing a Single Galaxy Population in Harmonic Space