Dark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing

Abstract

We present cosmological results from a combined analysis of galaxy clustering and weak gravitational lensing, using 1321 deg${}^2$ of $griz$ imaging data from the first year of the Dark Energy Survey (DES Y1). We combine three two-point functions: (i) the cosmic shear correlation function of 26 million source galaxies in four redshift bins, (ii) the galaxy angular autocorrelation function of 650,000 luminous red galaxies in five redshift bins, and (iii) the galaxy-shear cross-correlation of luminous red galaxy positions and source galaxy shears. To demonstrate the robustness of these results, we use independent pairs of galaxy shape, photometric redshift estimation and validation, and likelihood analysis pipelines. To prevent confirmation bias, the bulk of the analysis was carried out while blind to the true results; we describe an extensive suite of systematics checks performed and passed during this blinded phase. The data are modeled in flat $\Lambda$CDM and $w$CDM cosmologies, marginalizing over 20 nuisance parameters, varying 6 (for $\Lambda$CDM) or 7 (for $w$CDM) cosmological parameters including the neutrino mass density and including the 457 $\times$ 457 element analytic covariance matrix. We find consistent cosmological results from these three two-point functions, and from their combination obtain $S_8\equiv {\sigma }_8({\Omega }_m/0.3{)}^{0.5}=0.783_{-0.025}^{+0.021}$ and ${\Omega }_m=0.264_{-0.019}^{+0.032}$ for $\Lambda$CDM for $w$CDM, we find $S_8=0.794_{-0.027}^{+0.029}$, ${\Omega }_m=0.279_{-0.022}^{+0.043}$, and $w=-0.80_{-0.22}^{+0.20}$ at 68% CL. The precision of these DES Y1 results rivals that from the Planck cosmic microwave background measurements, allowing a comparison of structure in the very early and late Universe on equal terms. Although the DES Y1 best-fit values for $S_8$ and ${\Omega }_m$ are lower than the central values from Planck ...

arXiv commentMatches published version. Results essentially unchanged, except updated covariance matrix leads to improved chi^2 (colored text removed)

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• Simple-graduated dark energy and spatial curvature
• Detecting clusters of galaxies and active galactic nuclei in an eROSITA all-sky survey digital twin
• Dark Energy Survey Year 1 Results: tomographic cross-correlations between DES galaxies and CMB lensing from SPT+Planck
• The road ahead of Horndeski: cosmology of surviving scalar-tensor theories
• Search for RR Lyrae stars in DES ultra-faint systems: Grus I, Kim 2, Phoenix II, and Grus II
• Solving the curvature and Hubble parameter inconsistencies through structure formation-induced curvature
• Cosmological Constraint on ${\Omega }_m$ and ${\sigma }_8$ from Cluster Abundances using the $GalWCat19$ Optical-Spectroscopic SDSS Catalog
• KiDS-1000: Combined halo-model cosmology constraints from galaxy abundance, galaxy clustering and galaxy-galaxy lensing
• Improving Weak Lensing Mass Map Reconstructions using Gaussian and Sparsity Priors: Application to DES SV
• Optical selection bias and projection effects in stacked galaxy cluster weak lensing
• Baryonic effects on the matter bispectrum
• Cosmology with the Wide-Field Infrared Survey Telescope -- Synergies with the Rubin Observatory Legacy Survey of Space and Time
• Dark Energy Survey Year 1 Results: Methodology and Projections for Joint Analysis of Galaxy Clustering, Galaxy Lensing, and CMB Lensing Two-point Functions
• Advances in Constraining Intrinsic Alignment Models with Hydrodynamic Simulations
• A volumetric deep Convolutional Neural Network for simulation of mock dark matter halo catalogues
• Reconstructing teleparallel gravity with cosmic structure growth and expansion rate data
• Dark Energy Survey Year 1 Results: Constraining Baryonic Physics in the Universe
• Hints of Modified Gravity in Cosmos and in the Lab?
• Mitigating contamination in LSS surveys: a comparison of methods
• Probing gravity with a joint analysis of galaxy and CMB lensing and SDSS spectroscopy
• Hefty enhancement of cosmological constraints from the DES Y1 data using a Hybrid Effective Field Theory approach to galaxy bias
• On the relative bias of void tracers in the Dark Energy Survey
• Updated constraints on decaying cold dark matter
• Is the Harrison-Zel'dovich spectrum coming back? ACT preference for $n_s\sim 1$ and its discordance with Planck
• nestcheck: diagnostic tests for nested sampling calculations
• Multi-interacting dark energy and its cosmological implications
• Cosmological cross-correlations and nearest neighbor distributions
• Cosmology with dropout selection: Straw-man surveys and CMB lensing
• Power spectrum of halo intrinsic alignments in simulations
• Field Level Neural Network Emulator for Cosmological N-body Simulations
• Exploring Early Dark Energy solution to the Hubble tension with Planck and SPTPol data
• KiDS & Euclid: Cosmological implications of a pseudo angular power spectrum analysis of KiDS-1000 cosmic shear tomography
• The full Boltzmann hierarchy for dark matter-massive neutrino interactions
• Wide-area tomography of CMB lensing and the growth of cosmological density fluctuations
• Blinding multi-probe cosmological experiments
• Detecting Galaxy-Filament Alignments in the Sloan Digital Sky Survey III
• Modified gravity realizations of quintom dark energy after DESI DR2
• Dark Energy Survey Year 1 Results: Calibration of redMaGiC Redshift Distributions in DES and SDSS from Cross-Correlations
• Consistency of Planck, ACT and SPT constraints on magnetically assisted recombination and forecasts for future experiments
• Weak Lensing Minima and Peaks: Cosmological Constraints and the Impact of Baryons
• Separate Universe Simulations with IllustrisTNG: baryonic effects on power spectrum responses and higher-order statistics
• What it takes to solve the Hubble tension through modifications of cosmological recombination
• Reconstruction of the Dark Energy equation of state from latest data: the impact of theoretical priors
• One spectrum to cure them all: Signature from early Universe solves major anomalies and tensions in cosmology
• Hints of dark energy anisotropic stress using Machine Learning
• The growth rate of cosmic structures in the local Universe with the ALFALFA survey
• Dynamical Dark sectors and Neutrino masses and abundances
• Consistency tests in cosmology using relative entropy
• Weak lensing constraints on splashback around massive clusters
• Redshift inference from the combination of galaxy colors and clustering in a hierarchical Bayesian model $-$ Application to realistic $N$-body simulations
• $H_0$ tension and the String Swampland
• A Hybrid Deep Learning Approach to Cosmological Constraints From Galaxy Redshift Surveys
• The Accuracy of Weak Lensing Simulations
• Cosmic shear with small scales: DES-Y3, KiDS-1000 and HSC-DR1
• Unified Superfluid Dark Sector
• On the dissection of degenerate cosmologies with machine learning
• Reconstructing Horndeski theories from phenomenological modified gravity and dark energy models on cosmological scales
• Cosmology Inference from Biased Tracers using the EFT-based Likelihood
• Robust sampling for weak lensing and clustering analyses with the Dark Energy Survey
• A Dark Matter Interpretation of the ANITA Anomalous Events
• Cross-correlation of DES Y3 lensing and ACT/$Planck$ thermal Sunyaev Zel'dovich Effect II: Modeling and constraints on halo pressure profiles
• Metastable dark energy models in light of Planck 2018: Alleviating the $H_0$ tension
• Cosmological Constraint Precision of the Photometric and Spectroscopic Multi-probe Surveys of China Space Station Telescope (CSST)
• Dark Energy Survey Year 1 results: Validation of weak lensing cluster member contamination estimates from P(z) decomposition
• Peculiar-velocity cosmology with Types Ia and II supernovae
• New perspectives on the BOSS small-scale lensing discrepancy for the Planck $\Lambda$CDM Cosmology
• ADDGALS: Simulated Sky Catalogs for Wide Field Galaxy Surveys
• The one-loop matter bispectrum as a probe of gravity and dark energy
• Dark Energy Survey Year 1 Results: Cross-Correlation Redshifts in the DES -- Calibration of the Weak Lensing Source Redshift Distributions
• Testing gravity using galaxy-galaxy lensing and clustering amplitudes in KiDS-1000, BOSS and 2dFLenS
• Dark Energy Survey Year 3 results: cosmology from combined galaxy clustering and lensing -- validation on cosmological simulations
• A fast particle-mesh simulation of non-linear cosmological structure formation with massive neutrinos
• $\kappa$TNG: Effect of Baryonic Processes on Weak Lensing with IllustrisTNG Simulations
• Cosmological constraints from the power spectrum of eBOSS quasars
• Galaxy cluster strong lensing cosmography: cosmological constraints from a sample of regular galaxy clusters
• Weak gravitational lensing by two-power-law densities using the Gauss-Bonnet theorem
• Ponderings on the Possible Preponderance of Perpendicular Planets
• On the halo-mass and radial scale dependence of the lensing is low effect
• Beware of commonly used approximations II: estimating systematic biases in the best-fit parameters
• Principal reconstructed modes of dark energy and gravity
• Unified early and late Universe cosmology through dissipative effects in steep quintessential inflation potential models
• Perturbation theory for modeling galaxy bias: validation with simulations of the Dark Energy Survey
• Quantifying Suspiciousness Within Correlated Data Sets
• Screening anisotropy via energy-momentum squared gravity: $\Lambda$CDM model with hidden anisotropy
• RascalC: A Jackknife Approach to Estimating Single and Multi-Tracer Galaxy Covariance Matrices
• Cosmology with 6 parameters in the Stage-IV era: efficient marginalisation over nuisance parameters
• Constraints on dark matter to dark radiation conversion in the late universe with DES-Y1 and external data
• Dynamical dark energy in the light of DESI 2024 data
• Relativistic numerical cosmology with Silent Universes
• Cosmological constraints on the gravitational constant
• Beyond $\Lambda$CDM constraints from the full shape clustering measurements from BOSS and eBOSS
• $N$-body simulations for parametrised modified gravity
• Strong orientation dependence of surface mass density profiles of dark haloes at large scales
• Lensing-like tensions in the Planck legacy release
• Investigating the Hubble Constant Tension -- Two Numbers in the Standard Cosmological Model
• Revisiting CMB constraints on dark matter annihilation
• Star-galaxy classification in the Dark Energy Survey Y1 dataset
• Non-minimal geometry-matter couplings in Weyl-Cartan space-times: $f(R,T,Q,T_m)$ gravity
• Observational constraints on early dark energy
• Cosmological parameter estimation via iterative emulation of likelihoods
• The Hubble Tension, The $M$ Crisis of Late Time $H(z)$ Deformation Models and the Reconstruction of Quintessence Lagrangians
• Controlling and leveraging small-scale information in tomographic galaxy-galaxy lensing
• Small-scale clumping at recombination and the Hubble tension
• Spectroscopic Quantification of Projection Effects in the SDSS redMaPPer Galaxy Cluster Catalogue
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• Machine learning constraints on deviations from general relativity from the large scale structure of the Universe
• Information Content of Higher-Order Galaxy Correlation Functions
• Dark Energy Survey Year 1 Results: the lensing imprint of cosmic voids on the Cosmic Microwave Background
• Validating a minimal galaxy bias method for cosmological parameter inference using HSC-SDSS mock catalogs
• Dark Energy Survey internal consistency tests of the joint cosmological probes analysis with posterior predictive distributions
• Magnification bias in galaxy surveys with complex sample selection functions
• An X-ray selected catalog of extended galaxy clusters from the ROSAT All-Sky Survey (RXGCC)
• Dark Energy Survey Year 1 Results: Measurement of the Galaxy Angular Power Spectrum
• Impact of $H_0$ priors on $f(T)$ late time cosmology
• Smoothing the $H_0$ tension with a dynamical dark energy model
• Super-sample covariance approximations and partial sky coverage
• The MillenniumTNG Project: Intrinsic alignments of galaxies and halos
• Low redshift constraints on energy-momentum-powered gravity models
• Joint cosmological inference of standard sirens and gravitational wave weak lensing
• Exploration of interacting dynamical dark energy model with interaction term including the equation-of-state parameter: alleviation of the $H_0$ tension
• BAO from angular clustering: optimization and mitigation of theoretical systematics
• Exploring the contamination of the DES-Y1 Cluster Sample with SPT-SZ selected clusters
• Phantom singularities and their quantum fate: general relativity and beyond
• Inferring high redshift large-scale structure dynamics from the Lyman-alpha forest
• Using X-Ray Morphological Parameters to Strengthen Galaxy Cluster Mass Estimates via Machine Learning
• Fitting string inflation to real cosmological data: the Fibre Inflation case
• Proca in the sky
• Capse.jl: efficient and auto-differentiable CMB power spectra emulation
• Cross-correlating radio continuum surveys and CMB lensing: constraining redshift distributions, galaxy bias and cosmology
• Stochastic dark energy from inflationary quantum fluctuations
• 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
• Testing Shear Recovery with Field Distortion
• Sources of $H_0$-tensions in dark energy scenarios
• Cosmological implications of an interacting model of dark matter \& dark energy
• Fast and easy super-sample covariance of large scale structure observables
• The Signatures of Self-Interacting Dark Matter and Subhalo Disruption on Cluster Substructure
• DES Y1 results: Splitting growth and geometry to test $\Lambda$CDM
• Constraining spatial curvature with large-scale structure
• Photo-z outlier self-calibration in weak lensing surveys
• Projected-Field Kinetic Sunyaev-Zel'dovich Cross-Correlations: Halo Model and Forecasts
• Latest evidence for a late time vacuum -- geodesic CDM interaction
• Gravitational wave as probe of superfluid dark matter
• Cosmological Evidence Modelling: a new simulation-based approach to constrain cosmology on non-linear scales
• Gravitationally induced particle production in scalar-tensor $f(R,T)$ gravity
• Cosmology with the Einstein Telescope: No Slip Gravity Model and Redshift Specifications
• Dark Energy Survey Year 1 Results: Cross-correlation between DES Y1 galaxy weak lensing and SPT+Planck CMB weak lensing
• Beyond two-point statistics: using the minimum spanning tree as a tool for cosmology
• $H_0$ Tension in Torsion-based Modified Gravity
• 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
• New MGCAMB tests of gravity with CosmoMC and Cobaya
• Cosmological constraints from abundance, weak-lensing and clustering of galaxy clusters: application to the SDSS
• GAMA+KiDS: Alignment of galaxies in galaxy groups and its dependence on galaxy scale
• Parameter discordance in Planck CMB and low-redshift measurements: projection in the primordial power spectrum
• Measuring the Small-Scale Matter Power Spectrum with High-Resolution CMB Lensing
• Cosmological inference from emulator based halo model I: Validation tests with HSC and SDSS mock catalogs
• $f(Q)$-gravity and neutrino physics
• Testing gravity with galaxy-galaxy lensing and redshift-space distortions using CFHT-Stripe 82, CFHTLenS and BOSS CMASS datasets
• Galaxy-Galaxy Lensing in HSC: Validation Tests and the Impact of Heterogeneous Spectroscopic Training Sets
• The PAU Survey: star-galaxy classification with multi narrow-band data
• Is Dark Energy Dynamical in the DESI Era? A Critical Review
• Can varying the gravitational constant alleviate the tensions ?
• CMB Anomalies and the Hubble Tension
• Velocity-dependent interacting dark energy and dark matter with a Lagrangian description of perfect fluids
• The perspective of voids on rising cosmology tensions
• Thermal Friction as a Solution to the Hubble and Large-Scale Structure Tensions
• Including massive neutrinos in thermal Sunyaev Zeldovich power spectrum and cluster counts analyses
• Developing a unified pipeline for large-scale structure data analysis with angular power spectra -- I. The importance of redshift-space distortions for galaxy number counts
• Forecast of Neutrino Cosmology from the CSST Photometric Galaxy Clustering and Cosmic Shear Surveys
• Constraints on anisotropic primordial non-Gaussianity from intrinsic alignments of SDSS-III BOSS galaxies
• Implications of an extended dark energy model with massive neutrinos
• Combination of cluster number counts and two-point correlations: Validation on Mock Dark Energy Survey
• Cosmological gravity on all scales II: Model independent modified gravity $N$-body simulations
• KiDS-450: Enhancing cosmic shear with clipping transformations
• Fast Generation of Covariance Matrices for Weak Lensing
• A new measure of tension between experiments
• Cosmological constraints on Hořava gravity revised in light of GW170817 and GRB170817A and the degeneracy with massive neutrinos
• Constraining power of cosmological observables: blind redshift spots and optimal ranges
• Cross-correlation of DES Y3 lensing and ACT/$Planck$ thermal Sunyaev Zel'dovich Effect I: Measurements, systematics tests, and feedback model constraints
• Non-Gaussianity in the Weak Lensing Correlation Function Likelihood -- Implications for Cosmological Parameter Biases
• Clustering dark energy and halo abundances
• Producing a BOSS-CMASS sample with DES imaging
• Multipole expansion for HI intensity mapping experiments: simulations and modelling
• Constraints on decaying dark matter from weak lensing and cluster counts
• Disentangling magnification in combined shear-clustering analyses
• WFIRST: The Essential Cosmology Space Observatory for the Coming Decade
• KiDS-1000 Cosmology: Constraints from density split statistics
• Next generation design and prospects for CANNEX
• Comparison of different approaches to the quasi-static approximation in Horndeski models
• Monte Carlo Control Loops for cosmic shear cosmology with DES Year 1
• Anisotropic massive Brans-Dicke gravity extension of the standard $\Lambda$CDM model
• Cosmological constraints on nonphantom dynamical dark energy with DESI Data Release 2 Baryon Acoustic Oscillations: A 3$\sigma$+ lensing anomaly
• Euclid preparation: XII. Optimizing the photometric sample of the Euclid survey for galaxy clustering and galaxy-galaxy lensing analyses
• Redshift space power spectrum beyond Einstein-de Sitter kernels
• Luminous red galaxies in the Kilo Degree Survey: selection with broad-band photometry and weak lensing measurements
• x-cut Cosmic Shear: Optimally Removing Sensitivity to Baryonic and Nonlinear Physics with an Application to the Dark Energy Survey Year 1 Shear Data
• ETHOS -- An Effective Theory of Structure Formation: Impact of Dark Acoustic Oscillations on Cosmic Dawn
• Viable Gauge Choices in Cosmologies with Non-Linear Structures
• Hints for possible low redshift oscillation around the best fit $\Lambda$CDM model in the expansion history of the Universe
• Organised Randoms: Learning and correcting for systematic galaxy clustering patterns in KiDS using self-organising maps
• A short review on clustering dark energy
• CSST Cosmological Emulator I: Matter Power Spectrum Emulation with one percent accuracy to k = 10 h/Mpc
• The LSST-DESC 3x2pt Tomography Optimization Challenge
• A Bayesian quantification of consistency in correlated datasets
• Impact of Weak Lensing Mass Calibration on eROSITA Galaxy Cluster Cosmological Studies -- a Forecast
• New constraints on the mass bias of galaxy clusters from the power spectra of the thermal Sunyaev-Zeldovich effect and cosmic shear
• Easing cosmic tensions with an open and hotter universe
• Cosmic convergence and shear with extended sources
• Can phantom transition at $z\sim 1$ restore the Cosmic concordance?
• Current constraints on deviations from General Relativity using binning in redshift and scale
• Dynamical systems analysis of tachyon dark energy model from a new perspective
• Constraints on nature of ultra light dark matter particles with 21cm forest
• 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
• Clustering and redshift-space distortions in modified gravity models with massive neutrinos
• Cluster counts: calibration issue or new physics?
• Accurately Weighing Neutrinos with Cosmological Surveys
• Consistency of cosmic shear analyses in harmonic and real space
• A thorough investigation of the prospects of eLISA in addressing the Hubble tension: Fisher Forecast, MCMC and Machine Learning
• The effect of outflows on CMB bounds from Primordial Black Hole accretion
• Redshift requirements for cosmic shear with intrinsic alignment
• Hint of a truncated primordial spectrum from the CMB large-scale anomalies
• KaRMMa -- Kappa Reconstruction for Mass Mapping
• Galaxy-galaxy weak gravitational lensing in $f(R)$ gravity
• Stability analysis and constraints on interacting viscous cosmology
• Observational Constraints on Warm Inflation in Loop Quantum Cosmology
• Constraints on Cosmology and Baryonic Feedback with the Deep Lens Survey Using Galaxy-Galaxy and Galaxy-Mass Power Spectra
• Reconciling galaxy cluster shapes, measured by theorists vs observers
• A Bayesian method for combining theoretical and simulated covariance matrices for large-scale structure surveys
• A Deeper Look at DES Dwarf Galaxy Candidates: Grus I and Indus II
• Cascading Dark Energy
• Self-calibration and robust propagation of photometric redshift distribution uncertainties in weak gravitational lensing
• Stacked lensing estimators and their covariance matrices: Excess surface mass density vs. Lensing shear
• The Impact of Line Misidentification on Cosmological Constraints from Euclid and other Spectroscopic Galaxy Surveys
• Cosmological constrains on minimally and non-minimally coupled scalar field models
• Inherently stable effective field theory for dark energy and modified gravity
• Cosmological test on viscous bulk models using Hubble Parameter measurements and type Ia Supernovae data
• Cosmological constraints and phenomenology of a beyond-Horndeski model
• Observational Constraints in Nonlocal Gravity: the Deser-Woodard Case
• Revealing the Local Cosmic Web from Galaxies by Deep Learning
• The cosmic neutrino background as a collection of fluids in large-scale structure simulations
• Cosmological lensing ratios with DES Y1, SPT and Planck
• Cosmological discordances III: more on measure properties, Large-Scale-Structure constraints, the Hubble constant and Planck
• Quantum behavior of the "Little Sibling" of the Big Rip induced by a three-form field
• Testing one-loop galaxy bias: cosmological constraints from the power spectrum
• RedMaPPer: Evolution and Mass Dependence of the Conditional Luminosity Functions of Red Galaxies in Galaxy Clusters
• LINNA: Likelihood Inference Neural Network Accelerator
• Cosmological Inference from Galaxy-Clustering Power Spectrum: Gaussianization and Covariance Decomposition
• Power-counting during single-field slow-roll inflation
• Vacuum Energy Density Measured from Cosmological Data
• Massive neutrinos and degeneracies in Lyman-alpha forest simulations
• Localizing Transformations of the Galaxy-Galaxy Lensing Observable
• Analytical approximations for curved primordial power spectra
• Constraints on Cosmological Parameters with a Sample of Type Ia Supernovae from JWST
• Cosmology with the sub-millimetre galaxies magnification bias: Tomographic Analysis
• On cosmological bias due to the magnification of shear and position samples in modern weak lensing analyses
• Testing a quintessence model with Yukawa interaction from cosmological observations and N-body simulations
• HOD-Dependent Systematics in Emission Line Galaxies for the DESI 2024 BAO analysis
• Modelling the matter bispectrum at small scales in modified gravity
• From dwarf galaxies to galaxy clusters: Self-Interacting Dark Matter over 7 orders of magnitude in halo mass
• Growth of Matter Perturbations in the Bi-Galileons Field Model
• DELVE-ing into the Jet: a thin stellar stream on a retrograde orbit at 30 kpc
• Blind Observers of the Sky
• Alleviating the Hubble-constant tension and the growth tension via a transition of absolute magnitude favored by the Pantheon+ sample
• An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies
• Constraining constant and tomographic coupled dark energy with low-redshift and high-redshift probes
• Observational Constraints on Growth Index with Cosmography
• Galaxy morphoto-Z with neural Networks (GaZNets). I. Optimized accuracy and outlier fraction from Imaging and Photometry
• New scaling solutions in cubic Horndeski theories
• Bayesian photometric redshifts of blended sources
• Detecting Dark Energy Fluctuations with Gravitational Waves
• Cosmology with galaxy cluster weak lensing: statistical limits and experimental design
• Higher order statistics of shear field: a machine learning approach
• Cosmology from weak lensing alone and implications for the Hubble tension
• Sweeping Horndeski Canvas: New Growth-Rate Parameterization for Modified-Gravity Theories
• Weak lensing distortions beyond shear
• When tension is just a fluctuation: How noisy data affect model comparison
• The clustering of critical points in the evolving cosmic web
• $f\left(R,{\nabla }_{{\mu }_1}R,\dots ,{\nabla }_{{\mu }_1}\dots {\nabla }_{{\mu }_n}R\right)$ theories of gravity in Einstein frame: A higher order modified Starobinsky inflation model in the Palatini approach
• Observational constraints on the interacting dark energy - dark matter (IDM) cosmological models
• Constraining the cosmological evolution of scalar-tensor theories with local measurements of the time variation of G
• Observable Predictions for Massive-Neutrino Cosmologies with Model-Independent Dark Energy
• Phenomenological Gravitational Phase Transition: Reconciliation between the Late and Early Universe
• Breaking cosmic degeneracies: Disentangling neutrinos and modified gravity with kinematic information
• A Composite Likelihood Approach for Inference under Photometric Redshift Uncertainty
• Reconstructing Quintessence
• Analytic marginalization of $N(z)$ uncertainties in tomographic galaxy surveys
• Electron mass variation from dark sector interactions and compatibility with cosmological observations
• Constraining a causal dissipative cosmological model
• Analytical marginalisation over photometric redshift uncertainties in cosmic shear analyses
• Anisotropy in Pantheon+ supernovae
• Cosmology from weak lensing, galaxy clustering, CMB lensing and tSZ: I. 10x2pt Modelling Methodology
• Covariances for cosmic shear and galaxy-galaxy lensing in the response approach
• DESI Legacy Imaging Surveys Data Release 9: Cosmological Constraints from Galaxy Clustering and Weak Lensing using the Minimal Bias Model
• Magnification Bias Estimators for Realistic Surveys: an Application to the BOSS Survey
• Two-loop power spectrum with full time- and scale-dependence and EFT corrections: impact of massive neutrinos and going beyond EdS
• Observational constraints on soft dark energy and soft dark matter: challenging $\Lambda$CDM
• Extreme data compression while searching for new physics
• A cosmic glitch in gravity
• Halo-model analysis of the clustering of photometric luminous red galaxies at $0.10\le z\le 1.05$ from the Subaru Hyper Suprime-Cam Survey
• The Halo Spin Transition as a Probe of Dark Energy
• Addressing Cosmological Tensions by Non-Local Gravity
• Measuring anisotropic stress with relativistic effects
• Differentiating dark interactions with perturbation
• Hubble tension as a window on the gravitation of the dark matter sector
• Baryon Acoustic Oscillations in the projected cross-correlation function between the eBOSS DR16 quasars and photometric galaxies from the DESI Legacy Imaging Surveys
• Deconstructing the Planck TT Power Spectrum to Constrain Deviations from $\Lambda$CDM
• Toward a simultaneous resolution of the $H_0$ and $S_8$ tensions: early dark energy and an interacting dark sector model
• Mass Functions, Luminosity Functions, and Completeness Measurements from Clustering Redshifts
• The unequal-time matter power spectrum: impact on weak lensing observables
• Gaussian-process reconstructions and model building of quintom dark energy from latest cosmological observations
• Validating the Fisher approach for stage IV spectroscopic surveys
• Detection of Cosmic Magnification via Galaxy Shear -- Galaxy Number Density Correlation from HSC Survey Data
• Cosmological bound on neutrino masses in the light of $H_0$ tension
• A Test of the Standard Cosmological Model with Geometry and Growth
• Minimising the impact of scale-dependent galaxy bias on the joint cosmological analysis of large scale structures
• FLRW Cosmology in Metric-Affine $F(R,Q)$ Gravity
• fkPT: Constraining scale-dependent modified gravity with the full-shape galaxy power spectrum
• The orbital evolution of UFDs and GCs in an evolving Galactic potential
• General Relativistic corrections in density-shear correlations
• Altered Axion Abundance from a Dynamical Peccei-Quinn Scale
• Exploring Mirror Twin Higgs Cosmology with Present and Future Weak Lensing Surveys
• Measuring the scale dependence of intrinsic alignments using multiple shear estimates
• Forecast Analysis on Interacting Dark Energy Models from Future Generation PICO and DESI Missions
• Clustering of red-sequence galaxies in the fourth data release ofthe Kilo-Degree Survey
• Cluster counts III. $\Lambda$CDM extensions and the cluster tension
• Detection of spatial clustering in the 1000 richest SDSS DR8 redMaPPer clusters with Nearest Neighbor distributions
• Closing up the cluster tension?
• The Effect of Systematic Redshift Biases in BAO Cosmology
• Asymmetric dark matter with a spontaneously broken $U(1{)}^{\prime }$: self-interaction and gravitational waves
• Modified Gravity Away from a $\Lambda$CDM Background
• A DECam Search for Explosive Optical Transients Associated with IceCube Neutrinos
• Brighter-fatter effect in near-infrared detectors -- III. Fourier-domain treatment of flat field correlations and application to WFIRST
• Tomographic Constraints on Gravity from Angular Redshift Fluctuations in the Late Universe
• Reconstructing Probability Distributions with Gaussian Processes
• Cosmology from Cross-Correlation of ACT-DR4 CMB Lensing and DES-Y3 Cosmic Shear
• Intrinsic and extrinsic correlations of galaxy shapes and sizes in weak lensing data
• The Sejong Suite: Cosmological Hydrodynamical Simulations with Massive Neutrinos, Dark Radiation, and Warm Dark Matter
• The observable $E_g$ statistics
• Generalized Brans-Dicke theories in light of evolving dark energy
• The Integrated Sachs-Wolfe Effect in Interacting Dark Matter-Dark Energy Models
• Linear Systematics Mitigation in Galaxy Clustering in the Dark Energy Survey Year 1 Data
• Role of the Hubble Scale in the Weak Lensing vs. CMB Tension
• Bayesian methods for fitting Baryon Acoustic Oscillations in the Lyman-$\alpha$ forest
• BAO cosmology in non-spatially flat background geometry from BOSS+eBOSS and lessons for future surveys
• Planting a Lyman alpha forest on AbacusSummit
• Incorporating galaxy cluster triaxiality in stacked cluster weak lensing analyses
• Non-thermal neutrino-like hot dark matter in light of the $S_8$ tension
• deeplenstronomy: A dataset simulation package for strong gravitational lensing
• Non-thermal Hot Dark Matter from Inflaton/Moduli Decay: The Momentum Distribution and Relaxing the Cosmological Mass Bound
• Observing the dark sector
• ${\mu }_{\star }$ Masses: Weak Lensing Calibration of the Dark Energy Survey Year 1 redMaPPer Clusters using Stellar Masses
• Early dark energy constraints with late-time expansion marginalization
• Does the fraction of dark matter diminish with early dark energy?
• Model-independent way to determine the Hubble constant and the curvature from phase shift of gravitational waves with DECIGO
• ISiTGR: Testing deviations from GR at cosmological scales including dynamical dark energy, massive neutrinos, functional or binned parametrizations, and spatial curvature
• A revised density split statistic model for general filters
• An adapted filter function for density split statistics in weak lensing
• Dark sector evolution in Horndeski models
• Myrzakulov $F(T,Q)$ gravity: cosmological implications and constraints
• Lensing impact on cosmic relics and tensions
• A fully data-driven algorithm for accurate shear estimation
• Probing alternative cosmologies through the inverse distance ladder
• Dark Energy Survey Year 1 Results: Wide field mass maps via forward fitting in harmonic space
• Cosmological Constraints from Weak Lensing Peaks: Can Halo Models Accurately Predict Peak Counts?
• Einstein-Vlasov Calculations of Structure Formation
• Probing Oscillons of Ultra-Light Axion-like Particle by 21cm Forest
• Structure Formation in Various Dynamical Dark Energy Scenarios
• Conformally and Disformally Coupled Vector field Models of Dark Energy
• HI intensity mapping with MeerKAT: forecast for delay power spectrum measurement using interferometer mode
• Axial Anomaly in Galaxies and the Dark Universe
• Exploring bulk viscous unified scenarios with Gravitational Waves Standard Sirens
• New dwarf galaxy candidates in the sphere of influence of the Local Volume spiral galaxy NGC2683
• Joint Constraints on the Hubble Constant, Spatial Curvature, and Sound Horizon from the Late-time Universe with Cosmography
• Euclid preparation. LIII. LensMC, weak lensing cosmic shear measurement with forward modelling and Markov Chain Monte Carlo sampling
• The local dark sector. Probing gravitation's low-acceleration frontier and dark matter in the Solar System neighborhood
• Anisotropic Scalar Field Dark Energy with a Disformally Coupled Yang-Mills Field
• The Phase of the BAO on Observable Scales
• Improving Photometric Redshift Estimates with Training Sample Augmentation
• CSST Large-scale Structure Analysis Pipeline: II. the CSST Emulator for Slitless Spectroscopy (CESS)
• The Buzzard Flock: Dark Energy Survey Synthetic Sky Catalogs
• Early-time thermalization of cosmic components? A hint for solving cosmic tensions
• Cosmological Model Parameter Dependence of the Matter Power Spectrum Covariance from the DEUS-PUR $Cosmo$ Simulations
• Constraints on small-scale primordial density fluctuation from cosmic microwave background through dark matter annihilation
• The Tessellation-Level-Tree: characterising the nested hierarchy of density peaks and their spatial distribution in cosmological N-body simulations
• Devouring the Milky Way Satellites: Modeling Dwarf Galaxies with Galacticus
• Galaxy Clustering in the Mira-Titan Universe I: Emulators for the redshift space galaxy correlation function and galaxy-galaxy lensing
• Baryogenesis through Asymmetric Hawking Radiation from Primordial Black Holes as Dark Matter
• Post-reionization HI 21-cm signal: A probe of negative cosmological constant
• Observational constraints on interactions between dark energy and dark matter with momentum and energy transfers
• LimberJack.jl: auto-differentiable methods for angular power spectra analyses
• New dwarf galaxy candidates in the sphere of influence of the Sombrero galaxy
• Evidence of dark energy in different cosmological observations
• Testing the Impact of Satellite Anisotropy on Large and Small Scale Intrinsic Alignments using Hydrodynamical Simulations
• Fast Sampling from Wiener Posteriors for Image Data with Dataflow Engines
• Parameter inference and model comparison using theoretical predictions from noisy simulations
• Weak Lensing of Type Ia Supernovae from the Dark Energy Survey
• High resolution tomography for galaxy spectroscopic surveys with angular redshift fluctuations
• Hubble tension as a window on the gravitation of the dark matter sector: Exploration of a family of models
• Impact of baryonic feedback on HSC Y1 weak lensing non-Gaussian statistics
• The Effective Fluid approach for Modified Gravity and its applications
• Halo Mass-Concentration Relation at High-Mass End
• Complete classification of Friedmann-Lemaître-Robertson-Walker solutions with linear equation of state: parallelly propagated curvature singularities for general geodesics
• Cosmological constraints with the Effective Fluid approach for Modified Gravity
• Galaxy Deblending using Residual Dense Neural networks
• Constraints on sterile neutrinos and the cosmological tensions
• Relic Neutrino Degeneracies and Their Impact on Cosmological Parameters
• Gravitino Cosmology Helped by a Right Handed (S)Neutrino
• BASILISK: Bayesian Hierarchical Inference of the Galaxy-Halo Connection using Satellite Kinematics--I. Method and Validation
• Dynamical dark energy can amplify the expansion rate of the Universe
• First Star Formation in the Presence of Primordial Magnetic Fields
• Primordial non-Gaussianity with Angular correlation function: Integral constraint and validation for DES
• KiDS-Legacy: Covariance validation and the unified OneCovariance framework for projected large-scale structure observables
• Cosmology with Galaxy Cluster Properties using Machine Learning
• Marginal Bayesian Statistics Using Masked Autoregressive Flows and Kernel Density Estimators with Examples in Cosmology
• Interplay of CMB Temperature, Space Curvature, and Expansion Rate Parameters
• Disentangling modified gravity from a dark force with gravitational redshift
• Non-perturbative halo clustering from cosmological density peaks
• Interpreting Internal Consistency of DES Measurements
• Non-parametric modeling of the cosmological data, base on the ${\chi }^2$ distribution
• Improving initialization and evolution accuracy of cosmological neutrino simulations
• Angular Correlation Function Estimators Accounting for Contamination from Probabilistic Distance Measurements
• Mass-varying Dark Matter from a Phase Transition
• Anisotropies in Cosmological 21 cm Background by Oscillons/I-balls of Ultra-light Axion-like Particle
• Cosmological Constraints from Fourier Phase Statistics
• Cosmological bounds on neutrino statistics
• Stress testing the dark energy equation of state imprint on supernova data
• Forecasting Super-Sample Covariance in Future Weak Lensing Surveys with SuperSCRAM
• PhoSim-NIRCam: Photon-by-photon image simulations of the James Webb Space Telescope's Near-Infrared Camera
• Euclid preparation. LII. Forecast impact of super-sample covariance on 3x2pt analysis with Euclid
• Probing departures from $\Lambda$CDM by late-time datasets
• The halo bispectrum as a sensitive probe of massive neutrinos and baryon physics
• Mitigating baryonic effects with a theoretical error covariance
• Dark Energy Survey Year 1: An independent E/B-mode cosmic shear analysis
• Detecting Low-Mass Perturbers in Cluster Lenses using Curved Arc Bases
• 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
• Constraining viscous fluid models in $f(Q)$ gravity with data
• A Mystery in Chamaeleon: Serendipitous Discovery of a Galactic Symbiotic Nova
• Improved Tomographic Binning of 3x2pt Lens Samples: Neural Network Classifiers and Optimal Bin Assignments
• Growth and Geometry Split in Light of the DES-Y3 Survey
• Perturbation Theory Remixed: Improved Nonlinearity Modeling beyond Standard Perturbation Theory
• Magnification bias in the shear-ratio test: a viable mitigation strategy
• Cosmological gravity on all scales III: non-linear matter power spectrum in phenomenological modified gravity
• The Weak Lensing Peak Statistics in the Mocks by the inverse-Gaussianization Method
• Cosmic dipole tensions: confronting the cosmic microwave background with infrared and radio populations of cosmological sources
• Perturbation theory models for LSST-era galaxy clustering: tests with sub-percent mock catalog measurements in Fourier and configuration space
• Removing Interlopers From Intensity Mapping Probes Of Primordial Non-Gaussianity
• A Systematic Study of Projection Biases in Weak Lensing Analysis
• Full-sky weak lensing: a nonlinear post-Friedmann treatment
• Constraining the growth rate of structure with phase correlations
• Chameleon Early Dark Energy and the Hubble Tension
• Influence of the local Universe on weak gravitational lensing surveys
• Constrained transit cosmological models in $f(R,L_m,T)$-gravity
• Difficulties in reconciling non-negligible differences between the local and cosmological values of the gravitational coupling in extended Brans-Dicke theories
• The XMM Cluster Survey: Exploring scaling relations and completeness of the Dark Energy Survey Year 3 redMaPPer cluster catalogue
• Singling out modified gravity parameters and datasets reveals a dichotomy between Planck and lensing
• Gravitation And the Universe from large Scale-Structures: The GAUSS mission concept
• Variational Inference for Deblending Crowded Starfields
• Analytic Calculation of Covariance between Cosmological Parameters from Correlated Data Sets, with an Application to SPTpol
• Optimizing galaxy samples for clustering measurements in photometric surveys
• Self-calibrating optical galaxy cluster selection bias using cluster, galaxy, and shear cross-correlations
• The catalog-to-cosmology framework for weak lensing and galaxy clustering for LSST
• Beyond dark energy Fisher forecasts: how DESI will constrain LCDM and quintessence models
• Neural Network Based Point Spread Function Deconvolution For Astronomical Applications
• Qualitative analysis for viscous cosmologies in a non linear regime of the Israel-Stewart formalism
• On Evidence for Elastic Interactions in the Dark Sector
• Comparing Dark Energy models with Hubble versus Growth Rate data
• All-sky angular power spectra from cleaned WISE$\times$SuperCOSMOS galaxy number counts
• Current and Future constraints on single-field $\alpha$-Attractor model
• Cluster Cosmology with the Velocity Distribution Function of the HeCS-SZ Sample
• The Impact of Photometric Redshift Errors on Lensing Statistics in Ray-Tracing Simulations
• Combining cosmic shear data with correlated photo-$z$ uncertainties: constraints from DESY1 and HSC-DR1
• Effects of Redshift Uncertainty on Cross-Correlations of CMB Lensing and Galaxy Surveys
• What does a cosmological experiment really measure? Covariant posterior decomposition with normalizing flows
• An SU(2) gauge principle for the Cosmic Microwave Background: Perspectives on the Dark Sector of the Cosmological Model
• Measuring the Matter Density of the Galactic Disk Using Stellar Streams
• Limit on the dark matter mass from its interaction with photons
• From Barthel Randers Kropina Geometries to the Accelerating Universe: A Brief Review of Recent Advances in Finslerian Cosmology
• Distinguishing freezing and thawing dark energy models through measurements of the fine-structure constant
• Phantom Dirac-Born-Infeld Dark Energy
• Can Baby Universe Absorption Explain Dark Energy?
• A solution to the S8 tension through neutrino-dark matter interactions
• Cosmological test of an extended quintessence model
• Dark energy-dark matter interactions as a solution to the $S_8$ tension
• Galaxy-galaxy lensing in the VOICE deep survey
• What Prevents Resolving the Hubble Tension through Late-Time Expansion Modifications?
• Fine-structure constant constraints on late-time dark energy transitions
• Covariances of density probability distribution functions. Lessons from hierarchical models
• Dark Energy: is it `just' Einstein's Cosmological Constant Lambda?
• Impact of cosmological signatures in two-point statistics beyond the linear regime
• Kinematic Lensing with the Roman Space Telescope
• Quintessence scalar field and cosmological constant: Dynamics of a multi-component dark energy model
• Does nonlocal gravity yield divergent gravitational energy-momentum fluxes?
• Equality scale-based and sound horizon-based analysis of the Hubble tension
• Radio-Optical Galaxy Shape and Shear Correlations in the COSMOS Field using 3 GHz VLA Observations
• Dark Matter Substructure or Source Model Systematics? A Case Study of Cluster Lens Abell S1063
• Non-local contribution from small scales in galaxy-galaxy lensing: Comparison of mitigation schemes
• Effects of Dark Energy anisotropic stress on the matter power spectrum
• Observational Constraints on Extended Starobinsky and Weyl Gravity Model of Inflation
• Tomographic cross correlations between galaxy surveys and the CMB gravitational lensing potential. Effect of the redshift bin mismatch
• Forecasts for Warm Dark Matter from Photometric Galaxy Surveys
• Prospects of probing dark energy with eLISA: Standard versus null diagnostics
• Scaling laws in the stellar mass distribution and the transition to homogeneity
• Satellite Content and Halo Mass of Galaxy Clusters: Comparison between Red-Sequence and Halo-based Optical Cluster Finders
• ${\text{SwiftC}}_{\ell }$: fast differentiable angular power spectra beyond Limber
• DELVE-DEEP Survey: The Faint Satellite System of NGC 55
• AMICO galaxy clusters in KiDS-1000: cosmological sample
• Scale and redshift dependent limits on cosmic neutrino properties
• Effective field theory of coupled dark energy and dark matter
• Does fractal Universe favour warm inflation: Observational support?
• Calibrating baryonic effects in cosmic shear with external data in the LSST era
• Euclid: Photometric redshift calibration with self-organising maps
• Implications of Dynamical Dark Energy in the expansion of the Universe and the Structure Formation
• Transient weak gravity in scalar-tensor theories
• Weak Lensing Constraints on Dark Matter-Baryon Interactions with $N$-Body Simulations and Machine Learning
• Blending and obscuration in weak lensing magnification
• Can the quasi-molecular mechanism of recombination decrease the Hubble tension?
• Position-dependent Voronoi probability distribution functions for matter and halos
• A Framework for Measuring Weak-Lensing Magnification Using the Fundamental Plane
• Star-Crossed Labours: Checking Consistency Between Current Supernovae Compilations
• A Pop III generated dust screen at z~16
• Can radial motions in the stellar halo constrain the rate of change of mass in the Galaxy?
• A glitch in gravity: cosmic Lorentz-violation from fiery Big Bang to glacial heat death
• Data Compression and Covariance Matrix Inspection: Cosmic Shear
• Devouring The Centaurus A Satellites: Modeling Dwarf Galaxies with Galacticus
• Observational Constraints on the Cosmology with Holographic Dark Fluid
• Unified Dark Energy and Dark Matter from Dynamical Spacetime Cosmology
• The RSD Sorting Hat: Unmixing Radial Scales in Projection
• The Hydrogen Intensity and Real-time Analysis eXperiment: 256-Element Array Status and Overview
• An Estimator for the lensing potential from galaxy number counts
• Measuring lensing ratios with future cosmological surveys
• Mapping Variations of Redshift Distributions with Probability Integral Transforms
• Lensing convergence and anisotropic dark energy in galaxy redshift surveys
• The chromatic Point Spread Function of weak lensing measurement in Chinese Space Station survey Telescope
• Intrinsic alignment from multiple shear estimates: A first application to data and forecasts for Stage IV
• Kinetic recoupling of dark matter
• Gaussbock: Fast parallel-iterative cosmological parameter estimation with Bayesian nonparametrics
• Catalog-level blinding on the bispectrum for DESI-like galaxy surveys
• Optimizing Redshift Distribution Inference through Joint Self-Calibration and Clustering-Redshift Synergy
• Improving Galaxy Cluster Selection with the Outskirt Stellar Mass of Galaxies
• KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing
• Deciphering Baryonic Feedback from ACT tSZ Galaxy Clusters
• DARKSKIES: A suite of super-sampled zoom-in simulations of galaxy clusters with self-interacting dark matter
• Quintessence and tachyon dark energy in interaction with dark matter: Observational constraints and model selection
• Quintom Dark Energy: Future Attractor and Phantom Crossing in Light of DESI DR2 Observation
• Is warm inflation quasi-stable?
• The Baryon Mapping Experiment (BMX), a 21cm intensity mapping pathfinder
• Mimetic Tensor-Vector-Scalar Cosmology: Incorporating Dark Matter, Dark Energy and Stiff Matter
• Phantom scalar field cosmologies constrained by early cosmic measurements
• A systematic study of projection biases in the Weak Lensing analysis of cosmic shear and the combination of galaxy clustering and galaxy-galaxy lensing
• Speeding up the detectability of the harmonic-space galaxy bispectrum
• Z-Sequence: Photometric redshift predictions for galaxy clusters with sequential random k-nearest neighbours
• Constraining disformal couplings with Redshift Space Distortion
• Analytic expressions for the background evolution of massive neutrinos and dark matter particles
• Analytic Derivation of the Halo Mass Function from the Non-Linear Cosmic Density Field
• 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
• Cosmology of Single Species Hidden Dark Matter
• Cosmological consequences of intrinsic alignments super-sample covariance
• Galaxy-galaxy lensing with the DES-CMASS catalogue: measurement and constraints on the galaxy-matter cross-correlation
• Probing gravity with the DES-CMASS sample and BOSS spectroscopy
• Cosmological Simulations of Number Counts
• Cosmological Constant from Boundary Condition and Its Implications beyond the Standard Model
• Testing Exponential $f(R)$ Gravity with CMB, DESI-DR2, and Supernova Data
• The relation of galaxies and dark matter haloes to the filamentary cosmic web
• UNITSIM-Galaxies: data release and clustering of emission-line galaxies
• The Lambda-CDM-NG cosmological model: A possible resolution of the Hubble tension
• 6x2pt: Forecasting gains from joint weak lensing and galaxy clustering analyses with spectroscopic-photometric galaxy cross-correlations
• Implications for the missing low-mass galaxies (satellites) problem from cosmic shear
• The Case for Nonlocal Modifications of Gravity
• Cosmological parameters from the joint analysis of Density Split and Second Order Statistics: an Emulator based on the Halo Occupation Distribution
• Dark Energy Survey Year 3 results: Galaxy-halo connection from galaxy-galaxy lensing
• Euclid Preparation: XIV. The Complete Calibration of the Color-Redshift Relation (C3R2) Survey: Data Release 3
• Quantum Statistical Effects on Warm Dark Matter and the Mass Constraint from the Cosmic Structure at Small Scales
• Comparison of the linear bias models in the light of the Dark Energy Survey
• Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenböck Spacetime with Observational Data
• Probing baryonic feedback with fast radio bursts: joint analyses with cosmic shear and galaxy clustering
• Constructing Merger Trees of Density Peaks Using Phase-Space Watershed Segmentation Algorithm
• Forecasting the Constraint on the Hu-Sawicki $f(R)$ Modified Gravity in the CSST $3\times 2$pt Photometric Survey
• The magnitude of the dark ages 21-cm signal in the context of existing early and late time constraints on $\Lambda$CDM
• STRAWBERRY: Finding haloes in the gravitational potential
• Power Suppression and Lensing Anomaly -- A phenomenological investigation
• Constraining cosmology with N-body simulations for future spectroscopic galaxy surveys at $2\le z\le 3$
• Dark sector interactions in light of weak lensing data
• One Galaxy Sample to Rule Them All: Halo Occupation Distribution Modeling of DES Year 3 Source Galaxies
• Cosmological constraints on mass-varying dark matter
• Refitting cosmological data with neutrino mass and degeneracy
• New Technologies for Discovery
• Assessing the potential of cluster edges as a standard ruler
• Lensing Without Borders. I. A Blind Comparison of the Amplitude of Galaxy-Galaxy Lensing Between Independent Imaging Surveys
• On the asymptotics of 3+1D cosmologies with bounded scalar potential and isometry group forming 2-dimensional orbits
• Cosmic backgrounds from the radio to the far-infrared: recent results and perspectives from cosmological and astrophysical surveys
• Momentum transfer models of interacting dark energy
• Geometry vs growth: Internal consistency of the flat ΛCDM model with KiDS-1000
• Galaxy Clustering in Harmonic Space from the Dark Energy Survey Year 1 Data: Compatibility with Real-Space Results
• Obtaining non-linear galaxy bias constraints from galaxy-lensing phase differences
• Milky Way Satellite Census. IV. Constraints on Decaying Dark Matter from Observations of Milky Way Satellite Galaxies
• Sensitivity of Cosmological Parameter Estimation to Nonlinear Prescription from Cosmic Shear
• Accidental deep field bias in CMB T and SNe $z$ correlation
• Prospects for radio weak lensing: studies using LOFAR observations in the ELAIS-N1 field
• Variational autoencoder for generating realistic $N$-body simulations for dark matter halos
• Cosmological constraints on sterile neutrino Dark Matter production mechanisms
• Cosmological implications of the full shape of anisotropic clustering measurements in BOSS and eBOSS
• Dark Energy Survey Year 3 results: Cosmology with peaks using an emulator approach
• Improving Photometric Galaxy Clustering Constraints With Cross-Bin Correlations
• Accretion of Generalized Chaplygin Gas onto Cosmologically Coupled Black Holes
• Structure of cosmic web in non-linear regime: the nearest neighbour and spherical contact distributions
• Scaling pair count to next galaxy surveys
• Origin & evolution of the Universe
• Cosmology with the Roman Space Telescope -- Synergies with CMB lensing
• Forecasting the potential of weak lensing magnification to enhance LSST large-scale structure analyses
• Calibrating Bayesian Tension Statistics using Neural Ratio Estimation
• Extragalactic Searches for Dark Matter Annihilation
• Cosmological tests of the gravastar hypothesis
• Constraining Dark Energy Perturbations: the Role of Early Dark Energy
• Halo structure and lensing signatures of a polytropic dark matter fluid
• Bayesian evidence and model selection approach for time-dependent dark energy
• Probing Dark Matter with Strong Gravitational Lensing through an Effective Density Slope
• An effective fluid description of scalar-vector-tensor theories under the sub-horizon and quasi-static approximations
• Non-Gaussian likelihood of weak lensing power spectra
• Cosmological constraints on viable $f(R)$ models using weak lensing
• Perturbations In Some Dark Energy Models