Revising the Halofit Model for the Nonlinear Matter Power Spectrum

Abstract

Based on a suite of state-of-the-art high-resolution $N$-body simulations, we revisit the so-called halofit model (Smith et al. 2003) as an accurate fitting formula for the nonlinear matter power spectrum. While the halofit model has been frequently used as a standard cosmological tool to predict the nonlinear matter power spectrum in a universe dominated by cold dark matter, its precision has been limited by the low-resolution of $N$-body simulations used to determine the fitting parameters, suggesting the necessity of improved fitting formula at small scales for future cosmological studies. We run high-resolution $N$-body simulations for 16 cosmological models around the Wilkinson Microwave Anisotropy Probe (WMAP) best-fit cosmological parameters (1, 3, 5, and 7 year results), including dark energy models with a constant equation of state. The simulation results are used to re-calibrate the fitting parameters of the halofit model so as to reproduce small-scale power spectra of the $N$-body simulations, while keeping the precision at large scales. The revised fitting formula provides an accurate prediction of the nonlinear matter power spectrum in a wide range of wavenumber ($k\le 30h$\,Mpc${}^{-1}$) at redshifts $0\le z\le 10$, with 5% precision for $k\le 1h$ Mpc${}^{-1}$ at $0\le z\le 10$ and 10% for $1\le k\le 10h$ Mpc${}^{-1}$ at $0\le z\le 3$. We discuss the impact of the improved halofit model on weak lensing power spectra and correlation functions, and show that the improved model better reproduces ray-tracing simulation results.

11 pages, 7 figures, minor changes, references added, accepted for publication in ApJ

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• Statistical modelling of the cosmological dispersion measure
• KiDS-1000: Constraints on the intrinsic alignment of luminous red galaxies
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• Controlling and leveraging small-scale information in tomographic galaxy-galaxy lensing
• Effects of baryons on weak lensing peak statistics
• Observational constraints on early dark energy
• Fast and accurate predictions of the nonlinear matter power spectrum for general models of Dark Energy and Modified Gravity
• Equation of State of Dark Matter after Planck Data
• Preparing for the Cosmic Shear Data Flood: Optimal Data Extraction and Simulation Requirements for Stage IV Dark Energy Experiments
• Constraints on warm dark matter from weak lensing in anomalous quadruple lenses
• Joint analysis of DES Year 3 data and CMB lensing from SPT and Planck II: Cross-correlation measurements and cosmological constraints
• Beyond the traditional Line-of-Sight approach of cosmological angular statistics
• Validating a minimal galaxy bias method for cosmological parameter inference using HSC-SDSS mock catalogs
• Testing the Cosmic Shear Spatially-Flat Universe Approximation with Generalized Lensing and Shear Spectra
• Dark Energy Survey Year 1 Results: Measurement of the Galaxy Angular Power Spectrum
• CosmoGridV1: a simulated $w$CDM theory prediction for map-level cosmological inference
• Kernel-Based Emulator for the 3D Matter Power Spectrum from CLASS
• Constraining the spatial curvature with cosmic expansion history in a cosmological model with a non-standard sound horizon
• Systematic errors in the measurement of neutrino masses due to baryonic feedback processes: Prospects for stage IV lensing surveys
• Measurements of the Hubble Constant with a Two Rung Distance Ladder: Two Out of Three Ain't Bad
• Constraints on inflation with LSS surveys: features in the primordial power spectrum
• The importance of magnification effects in galaxy-galaxy lensing
• Does Concentration Drive the Scatter in the Stellar-to-Halo Mass Relation of Galaxy Clusters?
• Euclid: Forecasts from the void-lensing cross-correlation
• Non-linear damping of superimposed primordial oscillations on the matter power spectrum in galaxy surveys
• Euclid preparation. Sensitivity to neutrino parameters
• Dark energy imprints on the kinematic Sunyaev-Zel'dovich signal
• Fractional Dark Matter decay: cosmological imprints and observational constraints
• Machine Learning for Observational Cosmology
• MultiDarkLens Simulations: weak lensing light-cones and data base presentation
• Observing AGN feedback with CO intensity mapping
• On the road to percent accuracy III: non-linear reaction of the matter power spectrum to massive neutrinos
• Extracting cosmological information from the angular power spectrum of the 2MASS Photometric Redshift catalogue
• Persistent homology in cosmic shear II: A tomographic analysis of DES-Y1
• Cosmological Constraint on the Light Gravitino Mass from CMB Lensing and Cosmic Shear
• Moving around the cosmological parameter space: a nonlinear power spectrum reconstruction based on high-resolution cosmic responses
• ICE-COLA: fast simulations for weak lensing observables
• Effect of lensing non-Gaussianity on the CMB power spectra
• The imprint of $f(R)$ gravity on weak gravitational lensing II : Information content in cosmic shear statistics
• Testing Modified Gravity with Cosmic Shear
• Baryonic feedback biases on fundamental physics from lensed CMB power spectra
• Scale dependence of galaxy biasing investigated by weak gravitational lensing: An assessment using semi-analytic galaxies and simulated lensing data
• Self-calibration of weak lensing systematic effects using combined two- and three-point statistics
• The Effective Halo Model: Creating a Physical and Accurate Model of the Matter Power Spectrum and Cluster Counts
• Cross-correlating radio continuum surveys and CMB lensing: constraining redshift distributions, galaxy bias and cosmology
• On estimating cosmology-dependent covariance matrices
• Cosmological searches for a non-cold dark matter component
• Projected-Field Kinetic Sunyaev-Zel'dovich Cross-Correlations: Halo Model and Forecasts
• Euclid: The reduced shear approximation and magnification bias for Stage IV cosmic shear experiments
• Cosmology from weak lensing peaks and minima with Subaru Hyper Suprime-Cam survey first-year data
• Cosmological constraints from HSC survey first-year data using deep learning
• Information Gains from Cosmological Probes
• DES Y1 results: Splitting growth and geometry to test $\Lambda$CDM
• Minkowski Functionals of Convergence Maps and the Lensing Figure of Merit
• Is there evidence for anomalous dipole anisotropy in the large-scale structure?
• Impact of next-to-leading order contributions to CMB lensing
• Extending the Coyote emulator to dark energy models with standard $w_0$-$w_a$ parametrization of the equation of state
• Non-linear contributions to angular power spectra
• The squeezed matter bispectrum covariance with responses
• Dark Energy Survey Year 1 Results: Cross-correlation between DES Y1 galaxy weak lensing and SPT+Planck CMB weak lensing
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): Reconstruction of the redshift-space galaxy density field
• Stellar-to-halo mass relation of cluster galaxies
• Propagating sample variance uncertainties in redshift calibration: simulations, theory and application to the COSMOS2015 data
• Disentangling dark sector models using weak lensing statistics
• The weak, the strong and the ugly -- A comparative analysis of interacting stepped dark radiation
• Extragalactic gamma-ray signal from dark matter annihilation: an appraisal
• Full-sky ray-tracing simulation of weak lensing using ELUCID simulations: exploring galaxy intrinsic alignment and cosmic shear correlations
• DEMNUni: comparing nonlinear power spectra prescriptions in the presence of massive neutrinos and dynamical dark energy
• Constraint on $f(R)$ Gravity through the Redshift Space Distortion
• The cosmological dependence of halo and galaxy assembly bias
• Hundreds of weak lensing shear-selected clusters from the Hyper Suprime-Cam Subaru Strategic Program S19A data
• Kinetic Sunyaev-Zeldovich effect in modified gravity
• Cosmological inference from emulator based halo model I: Validation tests with HSC and SDSS mock catalogs
• Fast Weak Lensing Simulations with Halo Model
• On the information content of the matter power spectrum
• The SDSS-IV eBOSS: emission line galaxy catalogues at z=0.8 and study of systematic errors in the angular clustering
• First Constraints on Growth Rate from Redshift-Space Ellipticity Correlations of SDSS Galaxies at $0.16<z<0.70$
• Testing gravity with galaxy-galaxy lensing and redshift-space distortions using CFHT-Stripe 82, CFHTLenS and BOSS CMASS datasets
• Weak lensing by galaxy troughs with modified gravity
• Multi-wavelength properties of radio and machine-learning identified counterparts to submillimeter sources in S2COSMOS
• Power spectrum modelling of galaxy and radio intensity maps including observational effects
• One- and Two-point Source Statistics from the LOFAR Two-metre Sky Survey First Data Release
• Mask Effects on Cosmological Studies with Weak Lensing Peak Statistics
• An ALMA survey of the SCUBA-2 Cosmology Legacy SurveyUKIDSS/UDS Field: Halo Masses for Submillimetre Galaxies
• Probing primordial black holes with anisotropies in stochastic gravitational-wave background
• Investigating scalar-tensor-gravity with statistics of the cosmic large-scale structure
• Cross-correlation between Subaru Hyper Suprime-Cam Galaxy Weak Lensing and Planck Cosmic Microwave Background Lensing
• Probing galaxy bias and intergalactic gas pressure with KiDS Galaxies-tSZ-CMB lensing cross-correlations
• $\text{matryoshka}$: Halo Model Emulator for the Galaxy Power Spectrum
• Cosmological constraints on dark matter annihilation and decay: Cross-correlation analysis of the extragalactic $\gamma$-ray background and cosmic shear
• GLASS: Generator for Large Scale Structure
• Combination of cluster number counts and two-point correlations: Validation on Mock Dark Energy Survey
• Enhancement of gravitational waves at Q-ball decay including non-linear density perturbations
• Non-Gaussianity in the Weak Lensing Correlation Function Likelihood -- Implications for Cosmological Parameter Biases
• Multipole expansion for HI intensity mapping experiments: simulations and modelling
• Detecting Black-Hole Binary Clustering via the Second-Generation Gravitational-Wave Detectors
• Fast Generation of Covariance Matrices for Weak Lensing
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Never mind the gaps: comparing techniques to restore homogeneous sky coverage
• Cosmological gravity on all scales II: Model independent modified gravity $N$-body simulations
• Searching for Sterile Neutrino with X-ray Intensity Mapping
• KiDS-450: Enhancing cosmic shear with clipping transformations
• Multiple Lensing of the Cosmic Microwave Background anisotropies
• A direct detection of neutral hydrogen intensity mapping on Mpc scales at $z\approx 0.32$ and $z\approx 0.44$
• The Effect of Large-Scale Structure on the Magnification of High-Redshift Sources by Cluster-Lenses
• The Halo Void (Dust) Model of Large Scale Structure
• Euclid: Modelling massive neutrinos in cosmology -- a code comparison
• Monte Carlo Control Loops for cosmic shear cosmology with DES Year 1
• An optimal survey geometry of weak lensing survey: minimizing super-sample covariance
• Three-point phase correlations: A new measure of non-linear large-scale structure
• Evidence for the Cross-correlation between Cosmic Microwave Background Polarization Lensing from POLARBEAR and Cosmic Shear from Subaru Hyper Suprime-Cam
• Baryon Pasting Algorithm: Halo-based and Particle-based Pasting Methods
• Probability distribution function of the aperture mass field with large deviation theory
• A roadmap to cosmological parameter analysis with third-order shear statistics I: Modelling and validation
• x-cut Cosmic Shear: Optimally Removing Sensitivity to Baryonic and Nonlinear Physics with an Application to the Dark Energy Survey Year 1 Shear Data
• Precision growth index using the clustering of cosmic structures and growth data
• Parametrising non-linear dark energy perturbations
• Measurement of a Cosmographic Distance Ratio with Galaxy and CMB Lensing
• Tomographic imaging of the Fermi-LAT gamma-ray sky through cross-correlations: A wider and deeper look
• Detection of universality of dark matter profile from Subaru weak lensing measurements of 50 massive clusters
• Cosmic Shear as a Probe of Galaxy Formation Physics
• The Integrated Sachs-Wolfe Signal from BOSS Super-Structures
• Cosmological constraints on non-adiabatic dark energy perturbations
• Quantifying resolution in cosmological N-body simulations using self-similarity
• A Unified Catalog-level Reanalysis of Stage-III Cosmic Shear Surveys
• Cosmological constraints from the power spectrum and bispectrum of 21cm intensity maps
• Inference from the small scales of cosmic shear with current and future Dark Energy Survey data
• CSST Cosmological Emulator I: Matter Power Spectrum Emulation with one percent accuracy to k = 10 h/Mpc
• Constraints on the dark matter and dark energy interactions from weak lensing bispectrum tomography
• A Bayesian quantification of consistency in correlated datasets
• Organised Randoms: Learning and correcting for systematic galaxy clustering patterns in KiDS using self-organising maps
• Weak Lensing Analysis of CODEX Clusters using Dark Energy Camera Legacy Survey : Mass-Richness Relation
• The Subaru FMOS galaxy redshift survey (FastSound). V. Intrinsic alignments of emission line galaxies at $z\sim 1.4$
• Debiasing inference with approximate covariance matrices and other unidentified biases
• The first constraint from SDSS galaxy-galaxy weak lensing measurements on interacting dark energy models
• Constraints on Cosmology and Baryonic Feedback with the Deep Lens Survey Using Galaxy-Galaxy and Galaxy-Mass Power Spectra
• Probing primordial non-Gaussianity with the power spectrum and bispectrum of future 21cm intensity maps
• Consistency of cosmic shear analyses in harmonic and real space
• Power spectrum multipole expansion for HI intensity mapping experiments: unbiased parameter estimation
• Redshift requirements for cosmic shear with intrinsic alignment
• Testing for New Physics: Neutrinos and the Primordial Power Spectrum
• Cosmological constraints from the cross-correlation of DESI Luminous Red Galaxies with CMB lensing from Planck PR4 and ACT DR6
• Galaxy-galaxy weak gravitational lensing in $f(R)$ gravity
• Revisiting the impact of neutrino mass hierarchies on neutrino mass constraints in light of recent DESI data
• The FLAMINGO project: Baryon effects on the matter power spectrum
• syren-halofit: A fast, interpretable, high-precision formula for the $\Lambda$CDM nonlinear matter power spectrum
• The BINGO Project VI: HI Halo Occupation Distribution and Mock Building
• Enabling matter power spectrum emulation in beyond-$\Lambda$CDM cosmologies with COLA
• Probing Cosmology and Cluster Astrophysics with Multi-Wavelength Surveys I. Correlation Statistics
• Detecting Dark Matter Substructures on Small Scales with Fast Radio Bursts
• Joint analysis of DES Year 3 data and CMB lensing from SPT and Planck I: Construction of CMB Lensing Maps and Modeling Choices
• Efficient calculation of cosmological neutrino clustering with both linear and non-linear gravity
• Barry and the BAO Model Comparison
• Precision Prediction of the Log Power Spectrum
• Stacked lensing estimators and their covariance matrices: Excess surface mass density vs. Lensing shear
• Detection of spatial correlations of fundamental plane residuals, and cosmological implications
• Cosmological lensing ratios with DES Y1, SPT and Planck
• The e-MANTIS emulator: fast predictions of the non-linear matter power spectrum in $f(R)$CDM cosmology
• Impact of bias and redshift-space modelling for the halo power spectrum: Testing the effective field theory of large-scale structure
• The Clustering of X-ray Luminous Quasars
• Fitting and forecasting non-linear coupled dark energy
• RAY-RAMSES: a code for ray tracing on the fly in N-body simulations
• Weak lensing of large scale structure in the presence of screening
• The cosmic neutrino background as a collection of fluids in large-scale structure simulations
• A clustering-based self-calibration of the richness-to-mass relation of CAMIRA galaxy clusters out to $z\approx 1.1$ in the Hyper Suprime-Cam survey
• Cosmic variance of $H_0$ in light of forthcoming high-redshift surveys
• On the degeneracy between baryon feedback and massive neutrinos as probed by matter clustering and weak lensing
• Clustering dark energy imprints on cosmological observables of the gravitational field
• The LSST DESC Data Challenge 1: Generation and Analysis of Synthetic Images for Next Generation Surveys
• The PDF perspective on the tracer-matter connection: Lagrangian bias and non-Poissonian shot noise
• CFHTLenS: A Gaussian likelihood is a sufficient approximation for a cosmological analysis of third-order cosmic shear statistics
• Testing a quintessence model with Yukawa interaction from cosmological observations and N-body simulations
• Localizing Transformations of the Galaxy-Galaxy Lensing Observable
• Post-inflationary axion isocurvature perturbations facing CMB and large-scale structure
• HYMALAIA: A Hybrid Lagrangian Model for Intrinsic Alignments
• Fundamental Plane of BOSS galaxies: Correlations with galaxy properties, density field and impact on RSD measurements
• Cross-correlating 2D and 3D galaxy surveys
• Measuring the Hubble function with standard candle clustering
• Amending the halo model to satisfy cosmological conservation laws
• An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies
• Testing extended Jordan-Brans-Dicke theories with future cosmological observations
• Modelling the matter bispectrum at small scales in modified gravity
• Non-Linear Matter Power Spectrum Modeling in Interacting Dark Energy Cosmologies
• Cross-correlation of Planck CMB lensing with DESI galaxy groups
• Enhancing cosmic shear with the multi-scale lensing PDF
• Growth index of matter perturbations in the light of Dark Energy Survey
• On cosmological bias due to the magnification of shear and position samples in modern weak lensing analyses
• Cosmological Studies from HSC-SSP Tomographic Weak Lensing Peak Abundances
• AMICO galaxy clusters in KiDS-DR3: Measurement of the halo bias and power spectrum normalization from a stacked weak lensing analysis
• Photometric Redshift Uncertainties in Weak Gravitational Lensing Shear Analysis: Models and Marginalization
• Late time sky as a probe of steps and oscillations in primordial Universe
• Does jackknife scale really matter for accurate large-scale structure covariances?
• The BAHAMAS project: Effects of dynamical dark energy on large-scale structure
• SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES) IV: Spatial clustering and halo masses of 450-$\mu$m-selected sub-millimeter galaxies
• Detection and estimation of the cosmic dipole with the Einstein Telescope and Cosmic Explorer
• The CMB lensing bi-spectrum as a probe of modified gravity theories
• Cosmology from Clustering, Cosmic Shear, CMB Lensing, and Cross Correlations: Combining Rubin Observatory and Simons Observatory
• Integrated Cosmological Probes: Extended Analysis
• Constraints on features in the inflationary potential from future Euclid data
• First Evidence of Intrinsic Alignments of Red Galaxies at $z>1$: Cross-correlation between CFHTLenS and FastSound Samples
• Robust Evidence for Dynamical Dark Energy from DESI Galaxy-CMB Lensing Cross-Correlation and Geometric Probes
• The Impact of Non-Gaussianity upon Cosmological Forecasts
• Measuring ${\sigma }_8$ using DESI Legacy Imaging Surveys Emission-Line Galaxies and Planck CMB Lensing and the Impact of Dust on Parameter Inference
• The effects of varying depth in cosmic shear surveys
• The matter density PDF for modified gravity and dark energy with Large Deviations Theory
• Measuring weak lensing correlations of Type Ia Supernovae
• Simulating the Large-Scale Structure of HI Intensity Maps
• Theoretical and numerical perspectives on cosmic distance averages
• Constraining the primordial power spectrum from SNIa lensing dispersion
• Neutrinos and dark energy constraints from future galaxy surveys and CMB lensing information
• Weak Lensing by Intergalactic Mini-Structures in Quadruple Lens Systems: Simulation and Detection
• Sufficiency of a Gaussian power spectrum likelihood for accurate cosmology from upcoming weak lensing surveys
• Squeezing $f_{\mathrm{NL}}$ out of the matter bispectrum with consistency relations
• Cosmological Angular Trispectra and Non-Gaussian Covariance
• Observable Predictions for Massive-Neutrino Cosmologies with Model-Independent Dark Energy
• Cosmological parameter forecasts by a joint 2D tomographic approach to CMB and galaxy clustering
• Constraining dark matter decays with cosmic microwave background and weak lensing shear observations
• Evolution mapping: a new approach to describe matter clustering in the non-linear regime
• Statistical connection of peak counts to power spectrum and moments in weak lensing field
• The 6x2pt method: supernova velocities meet multiple tracers
• Time of flight of ultra-relativistic particles in a realistic Universe: a viable tool for fundamental physics?
• Analytical halo model of galactic conformity
• Euclid: Constraining linearly scale-independent modifications of gravity with the spectroscopic and photometric primary probes
• Galaxy clustering with photometric surveys using PDF redshift information
• Covariances for cosmic shear and galaxy-galaxy lensing in the response approach
• A simple parametrisation for coupled dark energy
• High mass and halo resolution from fast low resolution simulations
• Redshift Space Distortion of 21cm line at 1<z<5 with Cosmological Hydrodynamic Simulations
• Velocity reconstruction in the era of DESI and Rubin (part I): Exploring spectroscopic, photometric & hybrid samples
• DESI Legacy Imaging Surveys Data Release 9: Cosmological Constraints from Galaxy Clustering and Weak Lensing using the Minimal Bias Model
• Analytical marginalisation over photometric redshift uncertainties in cosmic shear analyses
• Evolution of skewness and kurtosis of cosmic density fields
• Exploring the Redshift-Space Peculiar Velocity Field and its Power Spectrum
• Baryon Acoustic Oscillations in the projected cross-correlation function between the eBOSS DR16 quasars and photometric galaxies from the DESI Legacy Imaging Surveys
• Analytic marginalization of $N(z)$ uncertainties in tomographic galaxy surveys
• The dipole anisotropy of WISE x SuperCOSMOS number counts
• Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-$y$-maps from SPT and Planck
• Fast estimation of aperture mass statistics II: Detectability of higher order statistics in current and future surveys
• The BAHAMAS project: Effects of a running scalar spectral index on large-scale structure
• Intensity mapping of the 21cm emission: lensing
• Effects of neutrino mass and asymmetry on cosmological structure formation
• Simultaneous Constraints on Cosmology and Photometric Redshift Bias from Weak Lensing and Galaxy Clustering
• General Relativistic corrections in density-shear correlations
• Angular clustering and host halo properties of [OII] emitters at $z>1$ in the Subaru HSC survey
• Galaxy bias from galaxy-galaxy lensing in the DES Science Verification Data
• Cosmologically probing ultra-light particle dark matter using 21 cm signals
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). The matter density and baryon fraction from the galaxy power spectrum at redshift $0.6<z<1.1$
• Combining gravitational lensing and gravitational redshift to measure the anisotropic stress with future galaxy surveys
• Measuring our velocity from fluctuations in number counts
• A General Framework for Removing Point Spread Function Additive Systematics in Cosmological Weak Lensing Analysis
• Optimizing simulation parameters for weak lensing analyses involving non-Gaussian observables
• Measuring the scale dependence of intrinsic alignments using multiple shear estimates
• syren-new: Precise formulae for the linear and nonlinear matter power spectra with massive neutrinos and dynamical dark energy
• Probing the two-body decaying dark matter scenario with weak lensing and the cosmic microwave background
• Cosmology before noon with multiple galaxy populations
• Linear and non-linear perturbations in dark energy models
• Clustering of red-sequence galaxies in the fourth data release ofthe Kilo-Degree Survey
• Herschel-ATLAS : The spatial clustering of low and high redshift submillimetre galaxies
• The RayGalGroupSims cosmological simulation suite for the study of relativistic effects: an application to lensing-matter clustering statistics
• Transitioning from Stage-III to Stage-IV: Cosmology from galaxy$\times$CMB lensing and shear$\times$CMB lensing
• Testing the tensor-vector-scalar Theory with the latest cosmological observations
• Accelerating cosmological inference with Gaussian processes and neural networks -- an application to LSST Y1 weak lensing and galaxy clustering
• Matter bispectrum of large-scale structure with Gaussian and non-Gaussian initial conditions: Halo models, perturbation theory, and a three-shape model
• The Merian Survey: Design, Construction, and Characterization of a Filter Set Optimized to Find Dwarf Galaxies and Measure their Dark Matter Halo Properties with Weak Lensing
• Spherical collapse in Generalized Dark Matter models
• The clustering of baryonic matter. II: halo model and hydrodynamic simulations
• An empirical approach to model selection: weak lensing and intrinsic alignments
• Constraining dark sector perturbations I: cosmic shear and CMB lensing
• Cosmology from Cross-Correlation of ACT-DR4 CMB Lensing and DES-Y3 Cosmic Shear
• Nonlinear effects of dark energy clustering beyond the acoustic scales
• CMB lensing bi-spectrum: assessing analytical predictions against full-sky lensing simulations
• The Sejong Suite: Cosmological Hydrodynamical Simulations with Massive Neutrinos, Dark Radiation, and Warm Dark Matter
• Parameter constraints from weak lensing tomography of galaxy shapes and cosmic microwave background fluctuations
• A physical and concise halo model based on the depletion radius
• The halo model with beyond-linear halo bias: unbiasing cosmological constraints from galaxy-galaxy lensing and clustering
• Post-Born corrections to the one-point statistics of (CMB) lensing convergence obtained via large deviation theory
• Constraints on small-scale cosmological fluctuations from SNe lensing dispersion
• Constraining f(R) gravity with cross-correlation of galaxies and cosmic microwave background lensing
• Post-Limber Weak Lensing Bispectrum, Reduced Shear Correction, and Magnification Bias Correction
• Rotation of the CMB polarisation by foreground lensing
• Deep+Wide Lensing Surveys will Provide Exquisite Measurements of the Dark Matter Halos of Dwarf Galaxies
• Linear Systematics Mitigation in Galaxy Clustering in the Dark Energy Survey Year 1 Data
• Towards determining the neutrino mass hierarchy: weak lensing and galaxy clustering forecasts with baryons and intrinsic alignments
• A revised density split statistic model for general filters
• A joint 2- and 3-point clustering analysis of the VIPERS PDR2 catalogue at z~1: breaking the degeneracy of cosmological parameters
• Model-Independent Predictions for Smooth Cosmic Acceleration Scenarios
• Probing Gravitational Lensing of the CMB with SDSS-IV Quasars
• Early dark energy constraints with late-time expansion marginalization
• Cornering Extended Starobinsky Inflation with CMB and SKA
• The star formation history in the last 10 billion years from CIB cross-correlations
• Impact of Massive Neutrinos and Dark Radiation on the High-redshift Cosmic Web. I. Lyman-Alpha Forest Observables
• Euclid: Covariance of weak lensing pseudo-$C_{\ell }$ estimates. Calculation, comparison to simulations, and dependence on survey geometry
• Bayesian framework to infer the Hubble constant from the cross-correlation of individual gravitational wave events with galaxies
• Accuracy requirements on intrinsic alignments for Stage-IV cosmic shear
• Forecasting the power of Higher Order Weak Lensing Statistics with automatically differentiable simulations
• Improved analytical modeling of the non-linear power spectrum in modified gravity cosmologies
• Weak lensing of gravitational waves in wave optics: Beyond the Born approximation
• Constraining the neutrino mass using a multi-tracer combination of two galaxy surveys and CMB lensing
• Searching for eV-mass Axion-like Particles with Cross Correlations between Line Intensity and Weak Lensing Maps
• Lensing smoothing of BAO wiggles
• Combining spectroscopic and photometric surveys using angular cross-correlations I: Algorithm and modelling
• Testing the Impact of Satellite Anisotropy on Large and Small Scale Intrinsic Alignments using Hydrodynamical Simulations
• Revisiting Vainshtein Screening for fast N-body simulations
• Validating the methodology for constraining the linear growth rate from clustering anisotropies
• Projection effects of large-scale structures on weak-lensing peak abundances
• Cosmological Tests of Gravity: A Future Perspective
• Using large scale structure data and a halo model to constrain Generalised Dark Matter
• Constraints on neutrino masses from the lensing dispersion of Type Ia supernovae
• Joint cosmology and mass calibration from tSZ cluster counts and cosmic shear
• Imitating intrinsic alignments: A bias to the CMB lensing-galaxy shape cross-correlation power spectrum induced by the large-scale structure bispectrum
• Cosmology from LOFAR Two-metre Sky Survey Data Release 2: Cross-correlation with the cosmic microwave background
• Galaxy blending effects in deep imaging cosmic shear probes of cosmology
• KiDS+VIKING-450: An internal-consistency test for cosmic shear tomography with a colour-based split of source galaxies
• Three-point intrinsic alignments of dark matter halos in the IllustrisTNG simulation
• Probing cosmology with weak lensing selected clusters II: Dark energy and f(R) gravity models
• The BAHAMAS project: Evaluating the accuracy of the halo model in predicting the non-linear matter power spectrum
• LimberJack.jl: auto-differentiable methods for angular power spectra analyses
• The statistics of peaks of weakly non-Gaussian random fields: Effects of bispectrum in two- and three-dimensions
• Galaxy Clustering in the Mira-Titan Universe I: Emulators for the redshift space galaxy correlation function and galaxy-galaxy lensing
• Constraining the Halo Mass of Damped Ly$\alpha$ Absorption Systems (DLAs) at $z=2-3.5$ using the Quasar-CMB Lensing Cross-correlation
• Exploring neutrino interactions in light of present and upcoming galaxy surveys
• Constraints on primordial non-Gaussianity from the cross-correlation of DESI Luminous Red Galaxies and $Planck$ CMB lensing
• Cosmology with extragalactic proper motions: harmonic formalism, estimators, and forecasts
• Late Time Modification of Structure Growth and the S8 Tension
• The skewness of the distance-redshift relation in $\Lambda$CDM
• On the degeneracies between baryons, massive neutrinos and f(R) gravity in Stage IV cosmic shear analyses
• Constraining $f(R)$ Gravity with a $k$-cut Cosmic Shear Analysis of the Hyper Suprime-Cam First-Year Data
• Constraining the physics of star formation from CIB-cosmic shear cross-correlations
• A cross-correlation analysis of CMB lensing and radio galaxy maps
• Accuracy of power spectra in dissipationless cosmological simulations
• Halo Mass-Concentration Relation at High-Mass End
• The thermal and gravitational energy densities in the large-scale structure of the Universe
• A semi-analytic model of pairwise velocity distribution between dark matter halos
• Probing the Cosmological Principle with weak lensing shear
• Constraints on dark matter and astrophysics from tomographic $\gamma$-ray cross-correlations
• A roadmap to cosmological parameter analysis with third-order shear statistics II: Analytic covariance estimate
• Statistics of Two-point Correlation and Network Topology for Lyman Alpha Emitters at $z\approx 2.67$
• Neutrino Masses, Scale-Dependent Growth, and Redshift-Space Distortions
• Forecast of cross-correlation of CSST cosmic shear tomography with AliCPT-1 CMB lensing
• Forecasts of cosmological constraints from Type Ia supernovae including the weak-lensing convergence
• Emission-line Stacking of 21cm Intensity Maps with MeerKLASS: Inference Pipeline and Application to the L-band Deep-field Data
• KiDS-Legacy: Covariance validation and the unified OneCovariance framework for projected large-scale structure observables
• Lensing dispersion of supernova flux: a probe of nonlinear structure growth
• Improved Modeling of the Kinematic Sunyaev-Zel'dovich Projected-Fields signal and its Cosmological Dependence
• Constraining neutrino mass and dark energy with peculiar velocities and lensing dispersions of Type Ia supernovae
• Bounds on Velocity-Dependent Dark Matter-Baryon Scattering from Large-Scale Structure
• Interpreting Internal Consistency of DES Measurements
• Dark Energy Survey Year 1: An independent E/B-mode cosmic shear analysis
• The density distributions of cosmic structures: impact of the local environment on weak-lensing convergence
• Mitigating baryonic effects with a theoretical error covariance
• The flat-sky approximation to galaxy number counts -- redshift space correlation function
• Forecasting Super-Sample Covariance in Future Weak Lensing Surveys with SuperSCRAM
• Cross-correlation of POLARBEAR CMB Polarization Lensing with High-$z$ Sub-mm Herschel-ATLAS galaxies
• On constraining Cosmology and the Halo Mass Function with Weak Gravitational Lensing
• GEO-FPT: a model of the galaxy bispectrum at mildly non-linear scales
• Euclid preparation. LII. Forecast impact of super-sample covariance on 3x2pt analysis with Euclid
• Cosmological evolution of the gravitational entropy of the large-scale structure
• Ray tracing the integrated Sachs-Wolfe effect through the light cones of the Dark Energy Universe Simulation -- Full Universe Runs
• 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
• The CIDER simulations: Nonlinear structure formation in the Constrained Interacting Dark Energy Scenario
• Small scale effects in the observable power spectrum at large angular scales
• Nonlinear redshift space distortion in halo ellipticity correlations: Analytical model and N-body simulations
• Intrinsic galaxy alignments in the KiDS-1000 bright sample: dependence on colour, luminosity, morphology, and galaxy scale
• A tomographic spherical mass map emulator of the KiDS-1000 survey using conditional generative adversarial networks
• Exploring the distance-redshift relation with gravitational wave standard sirens and tomographic weak lensing
• The Quest for the Inflationary Spectral Runnings in the Presence of Systematic Errors
• Optimizing galaxy samples for clustering measurements in photometric surveys
• Beyond the Lognormal Approximation: a General Simulation Scheme
• Dark Energy Survey Year 3 Results: Cosmological constraints from second and third-order shear statistics
• Detectable Data-driven Features in the Primordial Scalar Power Spectrum
• Power Spectrum Precision for Redshift Space Distortions
• Stable clustering and the resolution of dissipationless cosmological N-body simulations
• Cosmology at high redshift -- a probe of fundamental physics
• A Systematic Study of Projection Biases in Weak Lensing Analysis
• Perturbation theory models for LSST-era galaxy clustering: tests with sub-percent mock catalog measurements in Fourier and configuration space
• Axi-Higgs cosmology: Cosmic Microwave Background and cosmological tensions
• Thawing k-essence dark energy in the PAge space
• Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
• Efficient computation of the super-sample covariance for stage IV galaxy surveys
• The catalog-to-cosmology framework for weak lensing and galaxy clustering for LSST
• Intrinsic size correlations in weak lensing
• DEMNUni: cross-correlating the nonlinear ISWRS effect with CMB-lensing and galaxies in the presence of massive neutrinos
• Cosmological Leverage from the Matter Power Spectrum in the Presence of Baryon and Nonlinear Effects
• Weighing the Light Gravitino Mass with Weak Lensing Surveys
• Third-order intrinsic alignment of SDSS BOSS LOWZ galaxies
• Euclid preparation LXXI. Simulations and nonlinearities beyond $\mathsf{\Lambda }$CDM. 3. Constraints on $f(R)$ models from the photometric primary probes
• What is the super-sample covariance? A fresh perspective for second-order shear statistics
• Probing the Neutrino Mass through the Cross Correlation between the Rees-Sciama Effect and Weak Lensing
• Mitigating baryon feedback bias in cosmic shear through a theoretical error covariance in the matter power spectrum
• Euclid preparation. Sensitivity to non-standard particle dark matter model
• All-sky angular power spectra from cleaned WISE$\times$SuperCOSMOS galaxy number counts
• A solution to the S8 tension through neutrino-dark matter interactions
• Sensitivity of Cosmological Parameter Estimation to Nonlinear Prescription from Galaxy Clustering
• PhotoNs-GPU:A GPU accelerated cosmological simulation code
• E/B mode decomposition of HSC-Y1 cosmic shear using COSEBIs: cosmological constraints and comparison with other two-point statistics
• Observational Constraints on Early Coupled Quintessence
• Baryon acoustic oscillations from HI intensity mapping: the importance of cross-correlations in the monopole and quadrupole
• Accessing the high-$\ell$ frontier under the Reduced Shear Approximation with $k$-cut Cosmic Shear
• Non-parametric Cosmology with Cosmic Shear
• CFHTLenS: Galaxy bias as function of scale, stellar mass, and colour. Conflicts with predictions by semi-analytic models
• Subhalo abundance matching using progenitor mass at varying redshift: Two modes of stellar mass growth imprinted into the Subaru HSC galaxy clustering
• Void Lensing in Cubic Galileon Gravity
• Non-local contribution from small scales in galaxy-galaxy lensing: Comparison of mitigation schemes
• Cosmological inference including massive neutrinos from the matter power spectrum: biases induced by uncertainties in the covariance matrix
• Fitting functions on the cheap: the relative nonlinear matter power spectrum
• Euclid: Photometric redshift calibration with the clustering redshifts technique
• Impacts of pre-initial conditions on anisotropic separate universe simulations: a boosted tidal response in the epoch of reionization
• Comparison of results on $N_{\mathrm{eff}}$ from various Planck likelihoods
• Dynamics of pairwise motions in the fully non-linear regime in LCDM and Modified Gravity cosmologies
• Cosmological constraints from galaxy clustering and galaxy-galaxy lensing with extended SubHalo Abundance Matching
• Quasi-2D Weak Lensing Cosmological Constraints Using the PDF-SYM method
• Impact of cosmological signatures in two-point statistics beyond the linear regime
• Impact of our local environment on cosmological statistics
• Tele-Correlation: Calibrating Shear-Shear Correlation with Real Data
• The galaxy power spectrum on the lightcone: deep, wide-angle redshift surveys and the turnover scale
• Einasto profile as the halo model solution coupled to the depletion radius
• Constraining Hot Dark Matter Sub-Species with Weak Lensing and the Cosmic Microwave Background Radiation
• A Bayesian estimate of the CMB-large-scale structure cross-correlation
• Nonlinear power spectrum in clustering and smooth dark energy models beyond the BAO scale
• Assessing theoretical uncertainties for cosmological constraints from weak lensing surveys
• Testing the Reliability of Fast Methods for Weak Lensing Simulations: WL-MOKA on PINOCCHIO
• The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
• Forecasts for Warm Dark Matter from Photometric Galaxy Surveys
• The impact of super-survey modes on cosmological constraints from cosmic shear fields
• Data Compression and Covariance Matrix Inspection: Cosmic Shear
• Weak Lensing Constraints on Dark Matter-Baryon Interactions with $N$-Body Simulations and Machine Learning
• Modelling the impact of intrinsic size and luminosity correlations on magnification estimation
• Cross-correlating IceCube neutrinos with a large set of galaxy samples around redshift z ~ 1
• The Velocity Field Olympics: Assessing velocity field reconstructions with direct distance tracers
• Imprints of dark matter-massive neutrino interaction in upcoming post-reionization and galaxy surveys
• The bias from hydrodynamic simulations: mapping baryon physics onto dark matter fields
• Cosmological boost factor for dark matter annihilation at redshifts of $z=10$-$100$ using the power spectrum approach
• Calibrating baryonic effects in cosmic shear with external data in the LSST era
• Neutrino decays as a natural explanation of the neutrino mass tension
• Galaxy and Mass Assembly (GAMA): Probing galaxy-group correlations in redshift space with the halo streaming model
• Matter power spectrum reconstruction with KiDS-Legacy: Improved internal $\Lambda$CDM consistency and preference for strong baryonic feedback
• Fourier imaging of non-linear structure formation
• Prospects for cosmic magnification measurements using HI intensity mapping
• Intrinsic correlations of galaxy sizes in a hydrodynamical cosmological simulation
• A frequentist view on the two-body decaying dark matter model
• An Estimator for the lensing potential from galaxy number counts
• Detecting Baryon Acoustic Oscillations in Dark Matter from Kinematic Weak Lensing Surveys
• The RSD Sorting Hat: Unmixing Radial Scales in Projection
• Forecasting Cosmological Constraints from the Weak Lensing Magnification of Type Ia Supernovae Measured by the Nancy Grace Roman Space Telescope
• KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing
• Self-calibrating BAO measurements in the presence of Small Displacement Interlopers
• Lensing convergence and anisotropic dark energy in galaxy redshift surveys
• Weak Lensing Reconstruction by Counting DECaLS Galaxies
• Is the large-scale structure traced by the BOSS LOWZ galaxies consistent with $\text{Planck}$?
• Predicting the Sufficient-Statistics Power Spectrum for Galaxy Surveys: A Recipe for $P_{A\ast }(k)$
• Detecting deviations from Gaussianity in high-redshift CMB lensing maps
• Neural style transfer of weak lensing mass maps
• Interpretable and physics-informed emulator for the linear matter power spectrum from machine learning
• Testing extensions to LCDM on small scales with forthcoming cosmic shear surveys
• Gaussbock: Fast parallel-iterative cosmological parameter estimation with Bayesian nonparametrics
• Fast and spurious: a robust determination of our peculiar velocity with future galaxy surveys
• Pulsar B1237+25 Aberration/Retardation Analysis from Decimeter to Decameter Wavelength: Challenge to "Radius-to-Frequency Mapping"
• DESI forecast for Dark Matter-Neutrino interactions using EFTofLSS
• Phenomenological power spectrum models for H$\alpha$ emission line galaxies from the Nancy Grace Roman Space Telescope
• A Novel Bispectrum Estimator of the Kinematic Sunyaev-Zel'dovich Effect using Projected Fields
• Measuring lensing ratios with future cosmological surveys
• Measuring the scatter of the mass-richness relation in galaxy clusters in photometric imaging surveys by means of their correlation function
• The mass and galaxy distribution around SZ-selected clusters
• An Optimally Weighted Estimator of the Linear Power Spectrum Disentangling the Growth of Density Perturbations Across Galaxy Surveys
• 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
• Lyα Intensity Mapping in HETDEX: Galaxy-Lyα Intensity Cross-Power Spectrum
• Implications for the missing low-mass galaxies (satellites) problem from cosmic shear
• Needlet estimation of cross-correlation between CMB lensing maps and LSS
• Dark Energy Survey Year 3 results: Galaxy-halo connection from galaxy-galaxy lensing
• The frozen vanilla model: Exploring dark sector interactions with delta effective theories
• Comparison of the linear bias models in the light of the Dark Energy Survey
• Mock catalogues of emission line galaxies based on the local mass density in dark-matter only simulations
• Impact of projection-induced optical selection bias on the weak lensing mass calibration of galaxy clusters
• Estimating power spectrum of discrete cosmic momentum field with fast Fourier transform
• Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics
• Parameter inference with non-linear galaxy clustering: accounting for theoretical uncertainties
• Improved cosmological constraints on axion-lepton interactions
• Dark Energy Survey: DESI-Independent Angular BAO Measurement
• On the Outskirts of Dark Matter Haloes
• Euclid: Constraints on f(R) cosmologies from the spectroscopic and photometric primary probes
• The Pseudo Evolution of Galaxy-Cluster Masses and Its Connection to Mass Density Profile
• Cosmology with shear ratios: a joint study of weak lensing and spectroscopic redshift datasets
• A systematic study of projection biases in the Weak Lensing analysis of cosmic shear and the combination of galaxy clustering and galaxy-galaxy lensing
• Cosmological Constraints on Neutrino Masses in a Second-Order CPL Dark Energy Model
• Baryonic effects in the Effective Field Theory of Large-Scale Structure and an analytic recipe for lensing in CMB-S4
• Impact of Large-Scale Structure along Line-of-Sight on Time-Delay Cosmography
• Refitting cosmological data with neutrino mass and degeneracy
• Cosmological Parameter Biases from Doppler-Shifted Weak Lensing in Stage IV Experiments
• KiDS-Legacy: WIMP dark matter constraints from the cross-correlation of weak lensing and Fermi-LAT gamma rays
• Cosmic magnification on high-redshift submillimeter galaxies
• Cosmology behind the mask: Constraining the parameters of $\Lambda$CDM with the unmasked galaxy density field from VIPERS
• Strong Conformity and Assembly Bias: Towards a Physical Understanding of the Galaxy-Halo Connection in SDSS Clusters
• The Impact of Tomographic Redshift Bin Width Errors on Cosmological Probes
• Angular correlation functions of bright Lyman-break galaxies at $3\lesssim \mathbf{z}\lesssim 5$
• Decaying Dark Matter: Simulations and Weak-Lensing Forecast
• Implementing spectra response function approaches for fast calculation of power spectra and bispectra
• A Hamiltonian, post-Born, three-dimensional, on-the-fly ray tracing algorithm for gravitational lensing
• Cosmic shear beyond 2-point statistics: Accounting for galaxy intrinsic alignment with projected tidal fields
• Galaxy Clustering in Harmonic Space from the Dark Energy Survey Year 1 Data: Compatibility with Real-Space Results
• A data compression and optimal galaxy weights scheme for Dark Energy Spectroscopic Instrument and weak lensing datasets
• Cross-correlating the EMU Pilot Survey 1 with CMB lensing: Constraints on cosmology and galaxy bias with harmonic-space power spectra
• AMICO-WL: an optimal filtering algorithm for galaxy cluster detections with weak lensing
• Power Spectrum Emulators from Neural Networks and Tree-Based Methods
• Influence of photometric galaxies redshift distribution in BAO estimation
• A semi-analytic estimate for the effective sound speed counterterm in the EFTofLSS
• Clustering of the extreme: A theoretical description of weak lensing critical points power spectra in the mildly nonlinear regime
• Non-linear infusion of intrinsic alignment and source clustering: impact on non-Gaussian cosmic shear statistics
• Clustering properties of TGSS radio sources
• Euclid: Early Release Observations. Weak gravitational lensing analysis of Abell 2390
• Variational autoencoder for generating realistic $N$-body simulations for dark matter halos
• Self-similarity of the mass distribution in rich galaxy clusters up z~1 tracked with weak lensing
• Euclid: Optimising tomographic redshift binning for 3$\times$2pt power spectrum constraints on dark energy
• Neural Network Acceleration of Large-scale Structure Theory Calculations
• Evidence for Intrinsic Galaxy Alignments in Ellipticity Autocorrelations out to $100h^{-1}\text{Mpc}$ from SDSS Galaxies with DESI Imaging
• CMB lensing tomography with clustering estimation of lens redshift distributions
• Indicator Power Spectra: Surgical Excision of Non-linearities and Covariance Matrices for Counts in Cells
• Probing power spectrum enhancement at small scales with the SKA
• Probing inflation with large-scale structure data: the contribution of information at small scales
• The BINGO project X. Cosmological parameter constraints from HI Intensity Mapping lognormal simulations
• The Covariance of Photometric and Spectroscopic Two-Point Statistics: Implications for Cosmological Parameter Inference
• Sahyadri: A simulation suite for the cosmology dependence of the Cosmic Web
• Reconstructing spatially-varying multiplicative bias for Stage IV weak lensing galaxy surveys with a quadratic estimator
• Cosmic Shear in Harmonic Space from the Dark Energy Survey Year 1 Data: Compatibility with Configuration Space Results
• Dark Energy Survey Year 3 results: Cosmology with peaks using an emulator approach
• Fast Sampling of Cosmological Initial Conditions with Gaussian Neural Posterior Estimation
• Forecasting the potential of weak lensing magnification to enhance LSST large-scale structure analyses
• About One-point Statistics of the Ratio of Two Fourier-transformed Cosmic Fields and an Application
• Toward testing gravity with LSST using $E_G$
• Sensitivity of Cosmological Parameter Estimation to Nonlinear Prescription from Cosmic Shear
• Probing gravity with non-linear clustering in redshift space
• A simple prediction of the nonlinear matter power spectrum in Brans-Dicke gravity from linear theory
• Constraining the lensing dispersion from the angular clustering of binary black hole mergers
• Web-Halo Model (WHM): Accurate non-linear matter power spectrum predictions without free parameters
• How to embed any likelihood into SBI: Application to Planck + Stage IV galaxy surveys and Dynamical Dark Energy