The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Abstract

We measure the clustering of dark matter halos in a large set of collisionless cosmological simulations of the flat LCDM cosmology. Halos are identified using the spherical overdensity algorithm, which finds the mass around isolated peaks in the density field such that the mean density is Delta times the background. We calibrate fitting functions for the large scale bias that are adaptable to any value of Delta we examine. We find a ~6% scatter about our best fit bias relation. Our fitting functions couple to the halo mass functions of Tinker et. al. (2008) such that bias of all dark matter is normalized to unity. We demonstrate that the bias of massive, rare halos is higher than that predicted in the modified ellipsoidal collapse model of Sheth, Mo, & Tormen (2001), and approaches the predictions of the spherical collapse model for the rarest halos. Halo bias results based on friends-of-friends halos identified with linking length 0.2 are systematically lower than for halos with the canonical Delta=200 overdensity by ~10%. In contrast to our previous results on the mass function, we find that the universal bias function evolves very weakly with redshift, if at all. We use our numerical results, both for the mass function and the bias relation, to test the peak-background split model for halo bias. We find that the peak-background split achieves a reasonable agreement with the numerical results, but ~20% residuals remain, both at high and low masses.

11 pages, submitted to ApJ, revised to include referee's coments

References in corpus (12)

• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data
• The universal galaxy cluster pressure profile from a representative sample of nearby systems (REXCESS) and the Y_SZ-M_500 relation
• Transients from Initial Conditions in Cosmological Simulations
• The Excursion Set Theory of Halo Mass Functions, Halo Clustering, and Halo Growth
• Calibration of the galaxy cluster M_500-Y_X relation with XMM-Newton
• LoCuSS: Comparison of Observed X-ray and Lensing Galaxy Cluster Scaling Relations with Simulations
• Environmental Dependence of Cold Dark Matter Halo Formation
• Asymmetries in the inner regions of LCDM haloes
• The assembly bias of dark matter haloes to higher orders
• The Structure of Halos: Implications for Group and Cluster Cosmology
• Dark matter halo abundances, clustering and assembly histories at high redshift
• The clustering of the first galaxy halos

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• Signatures of primordial black holes in gravitational wave clustering
• Halo assembly bias from Separate Universe simulations
• Are the halo occupation predictions consistent with large scale galaxy clustering?
• Cosmological inference from emulator based halo model I: Validation tests with HSC and SDSS mock catalogs
• GAMA+KiDS: Empirical correlations between halo mass and other galaxy properties near the knee of the stellar-to-halo mass relation
• Linear and non-linear bias: predictions vs. measurements
• Early Black Holes in Cosmological Simulations: Luminosity Functions and Clustering Behaviour
• Probing galaxy bias and intergalactic gas pressure with KiDS Galaxies-tSZ-CMB lensing cross-correlations
• An ALMA survey of the SCUBA-2 Cosmology Legacy SurveyUKIDSS/UDS Field: Halo Masses for Submillimetre Galaxies
• Cross-Correlation of the Extragalactic Gamma-ray Background with Luminous Red Galaxies
• The Gigaparsec WiggleZ Simulations: Characterising scale dependant bias and associated systematics in growth of structure measurements
• Constraining neutrino properties with a Euclid-like galaxy cluster survey
• Cosmology dependence of galaxy cluster scaling relations
• Constraining Primordial Non-Gaussianity with Post-reconstructed Galaxy Bispectrum in Redshift Space
• Weak-lensing-inferred scaling relations of galaxy clusters in the RCS2: mass-richness, mass-concentration, mass-bias, and more
• Cosmological constraints on dark matter annihilation and decay: Cross-correlation analysis of the extragalactic $\gamma$-ray background and cosmic shear
• Galaxy clustering dependence on the $\left[\mathrm{O}\mathrm{II}\right]$ emission line luminosity in the local Universe
• $\text{matryoshka}$: Halo Model Emulator for the Galaxy Power Spectrum
• An Intensity Mapping Constraint on the CO-Galaxy Cross Power Spectrum at Redshift ~ 3
• The importance of galaxy formation histories in models of reionization
• Halo Occupation Distribution Modeling of Green Valley Galaxies
• Clustering with JWST: Constraining Galaxy Host Halo Masses, Satellite Quenching Efficiencies, and Merger Rates at z=4-10
• Cross-correlation of DES Y3 lensing and ACT/$Planck$ thermal Sunyaev Zel'dovich Effect I: Measurements, systematics tests, and feedback model constraints
• Impacts of satellite galaxies on the redshift-space distortions
• The imprint of $f(R)$ gravity on weak gravitational lensing I: Connection between observables and large scale structure
• Probing galaxy assembly bias with LRG weak lensing observations
• Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias
• The Galaxy-Halo Connection for $1.5\lesssim z\lesssim 5$ as revealed by the \emph{Spitzer} Matching survey of the UltraVISTA ultra-deep Stripes
• Large-scale clustering as a probe of the origin and the host environment of fast radio bursts
• Conditional Probabilities in the Excursion Set Theory. Generic Barriers and non-Gaussian Initial Conditions
• Combination of cluster number counts and two-point correlations: Validation on Mock Dark Energy Survey
• The role of the eROSITA all-sky survey in searches for sterile neutrino dark matter
• The locations of halo formation and the peaks formalism
• A unified model for the clustering of quasars and galaxies at $z\approx 6$
• Simulating galaxy formation in f(R) modified gravity: Matter, halo, and galaxy-statistics
• C${}^3$-Cluster Clustering Cosmology I. New constraints on the cosmic growth rate at z~0.3 from redshift-space clustering anisotropies
• EFTofLSS meets simulation-based inference: ${\sigma }_8$ from biased tracers
• The Halo Void (Dust) Model of Large Scale Structure
• Non-local bias contribution to third-order galaxy correlations
• Understanding the non-linear clustering of high redshift galaxies
• A direct detection of neutral hydrogen intensity mapping on Mpc scales at $z\approx 0.32$ and $z\approx 0.44$
• Statistics of Dark Matter Halos from the Excursion Set Approach
• Euclid: Modelling massive neutrinos in cosmology -- a code comparison
• First measurement of the characteristic depletion radius of dark matter haloes from weak lensing
• Effect of halo bias and Lyman Limit Systems on the history of cosmic reionization
• Prospects for distinguishing galaxy evolution models with surveys at redshifts $z\gtrsim 4$
• Baryon Pasting Algorithm: Halo-based and Particle-based Pasting Methods
• Feeding cosmic star formation: Exploring high-redshift molecular gas with CO intensity mapping
• Magnification of Photometric LRGs by Foreground LRGs and Clusters in SDSS
• Covariance matrices for halo number counts and correlation functions
• Constraining the properties of gaseous halos via cross-correlations of upcoming galaxy surveys and thermal Sunyaev-Zel'dovich maps
• Primordial non-Gaussianity with $\mu$-type and $y$-type spectral distortions: exploiting Cosmic Microwave Background polarization and dealing with secondary sources
• A Deep Ly$\alpha$ Survey in ECDF-S and COSMOS: I. General Properties of Lyman-alpha Emitters at $z\sim 2$
• Lyman-Break Galaxies at $z\sim 3$ in the Subaru Deep Field: Luminosity Function, Clustering and [OIII] Emission
• The Chandra COSMOS Legacy Survey: Clustering of X-ray selected AGN at 2.9<z<5.5 using photometric redshift Probability Distribution Functions
• Cosmological constraints from the power spectrum and bispectrum of 21cm intensity maps
• Coupling parsec and gigaparsec scales: primordial non-Gaussianity with multi-tracer intensity mapping
• 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
• Weak Lensing Analysis of CODEX Clusters using Dark Energy Camera Legacy Survey : Mass-Richness Relation
• Removing the giants and learning from the crowd: a new SZ power spectrum method and revised Compton $y$-map analysis
• The Atacama Cosmology Telescope: Weighing distant clusters with the most ancient light
• K-mouflage effects on clusters of galaxies
• Covariance matrices for galaxy cluster weak lensing: from virial regime to uncorrelated large-scale structure
• Disentangling interacting dark energy cosmologies with the three-point correlation function
• Cosmology with the largest galaxy cluster surveys: Going beyond Fisher matrix forecasts
• Probing Cosmology and Cluster Astrophysics with Multi-Wavelength Surveys I. Correlation Statistics
• Halo Properties and Mass Functions of Groups/Clusters from the DESI Legacy Imaging Surveys DR9
• Detectability of the gravitational redshift effect from the asymmetric galaxy clustering
• The BINGO Project VI: HI Halo Occupation Distribution and Mock Building
• Hosts and triggers of AGNs in the Local Universe
• Probing primordial non-Gaussianity with the power spectrum and bispectrum of future 21cm intensity maps
• A Systematic Search for Galaxy Proto-Cluster Cores at $z\sim 2$
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• The clustering of H$\beta$+[OIII] and [OII] emitters since $z\sim 5$: dependencies with line luminosity and stellar mass
• Describing galaxy weak lensing measurements from tenths to tens of Mpc and up to z~0.6 with a single model
• The Clustering of X-ray Luminous Quasars
• Kinetic Sunyaev-Zel'dovich tomography with line-intensity mapping
• Comparing Simple Quasar Demographics Models
• Cosmic Infrared Background anisotropies as a window into primordial non-Gaussianity
• CMB lensing reconstruction biases from masking extragalactic sources
• Velocity and mass bias in the distribution of dark matter halos
• Velocity reconstruction with the cosmic microwave background and galaxy surveys
• The halo mass of optically-luminous quasars at z=1-2 measured via gravitational deflection of the cosmic microwave background
• X-ray Cluster Constraints on Non-Gaussianity
• Euclid: Effect of sample covariance on the number counts of galaxy clusters
• Relation between the Turnaround radius and virial mass in $f(R)$ model
• Stacked lensing estimators and their covariance matrices: Excess surface mass density vs. Lensing shear
• How rare is the Bullet Cluster (in a $\Lambda$CDM universe)?
• Taming assembly bias for primordial non-Gaussianity
• The PDF perspective on the tracer-matter connection: Lagrangian bias and non-Poissonian shot noise
• pop-cosmos: A comprehensive picture of the galaxy population from COSMOS data
• Guess the cheese flavour by the size of its holes: A cosmological test using the abundance of Popcorn voids
• Primordial trispectrum from kSZ tomography
• Extracting HI Astrophysics from Interferometric Intensity Mapping
• 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
• Host Dark Matter Halos of WISE-selected Obscured & Unobscured Quasars: Evidence for Evolution
• The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: GLAM-QPM mock galaxy catalogs for the Emission Line Galaxy Sample
• PNG-UNITsims: Halo clustering response to primordial non-Gaussianities as a function of mass
• Synergies between radio, optical and microwave observations at high redshift
• The clustering of $z>7$ galaxies: Predictions from the BLUETIDES simulation
• Evolution of the luminosity-to-halo mass relation of LRGs from a combined SDSS-DR10+RCS2 analysis
• The clustering of baryonic matter. I: a halo-model approach
• The environment and host haloes of the brightest z~6 Lyman-break galaxies
• The galaxy correlation function as a constraint on galaxy formation physics
• Connecting cosmological accretion to strong Lyman-alpha absorbers
• Inferring host-galaxy properties of LIGO-Virgo-KAGRA's black holes
• Dust in galaxy clusters: Modeling at millimeter wavelengths and impact on Planck cluster cosmology
• AMICO galaxy clusters in KiDS-DR3: Measurement of the halo bias and power spectrum normalization from a stacked weak lensing analysis
• Joint Analysis of Galaxy-Galaxy Lensing and Galaxy Clustering: Methodology and Forecasts for DES
• Dense Regions in Supersonic Isothermal Turbulence
• Multi-wavelength scaling relations in galaxy groups: a detailed comparison of GAMA and KiDS observations to BAHAMAS simulations
• Amending the halo model to satisfy cosmological conservation laws
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• Subhaloes gone Notts: the clustering properties of subhaloes
• Imprints of gravitational lensing in the Planck CMB data at the location of WISExSCOS galaxies
• C${}^3$-Cluster Clustering Cosmology II. First detection of the BAO peak in the three-point correlation function of galaxy clusters
• Prospects for 21cm-Galaxy Cross-Correlations with HERA and the Roman High-Latitude Survey
• Modelling the matter bispectrum at small scales in modified gravity
• Cross-correlation of Planck CMB lensing with DESI galaxy groups
• Modelling Baryonic Effects on Galaxy Cluster Mass Profiles
• MultiDark-Clusters: Galaxy Cluster Mock Light-Cones, eROSITA and the Cluster Power Spectrum
• Inadequacy of internal covariance estimation for super-sample covariance
• Improving models of the cosmic infrared background using CMB lensing mass maps
• Systematic uncertainties in models of the cosmic dawn
• Compatibility of JWST results with exotic halos
• Effect of asphericity in caustic mass estimates of galaxy clusters
• Probing cosmology and gastrophysics with fast radio bursts: Cross-correlations of dark matter haloes and cosmic dispersion measures
• The large-scale 21-cm power spectrum from reionization
• The clustering of dark matter halos: scale-dependent bias on quasi-linear scales
• The local PNG bias of neutral Hydrogen, ${\mathrm{H}}_{\mathrm{I}}$
• Constraints on Modified Gravity from Sunyaev-Zeldovich Cluster Surveys
• The dominant origin of diffuse Ly$\alpha$ halos around LAEs explored by SED fitting and clustering analysis
• Searching for High-Energy Neutrino Emission from Galaxy Clusters with IceCube
• Cosmology with galaxy cluster weak lensing: statistical limits and experimental design
• Cold dark energy constraints from the abundance of galaxy clusters
• A new method to measure galaxy bias by combining the density and weak lensing fields
• Halo models of HI selected galaxies
• Effects of Completeness and Purity on Cluster Dark Energy Constraints
• BASS. XXXVI. Constraining the Local Supermassive Black Hole - Halo Connection with BASS DR2 AGN
• A galaxy group candidate at z~3.7 in the COSMOS field
• Renormalisation of linear halo bias in N-body simulations
• The cosmic web connection to the dark matter halo distribution through gravity
• An Accurate Analytic Model for the Thermal Sunyaev-Zel'dovich One-Point PDF
• BE-HaPPY: Bias Emulator for Halo Power Spectrum including massive neutrinos
• Velocity reconstruction in the era of DESI and Rubin (part I): Exploring spectroscopic, photometric & hybrid samples
• Covariances for cosmic shear and galaxy-galaxy lensing in the response approach
• NOEMA formIng Cluster survEy (NICE): Characterizing eight massive galaxy groups at $1.5<z<4$ in the COSMOS field
• 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
• Virial halo mass function in the $Planck$ cosmology
• Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-$y$-maps from SPT and Planck
• Cosmic Reionization On Computers: The Galaxy-Halo Connection between $5\le z\le 10$
• Analytic marginalization of $N(z)$ uncertainties in tomographic galaxy surveys
• New Local Volume Dwarf Galaxy Candidates from the DESI Legacy Imaging Surveys
• Cosmology from weak lensing, galaxy clustering, CMB lensing and tSZ: I. 10x2pt Modelling Methodology
• Analytical halo model of galactic conformity
• Effects of self-consistent rest-ultraviolet colours in semi-empirical galaxy formation models
• Patchy Screening of the CMB from Dark Photons
• Angular clustering and host halo properties of [OII] emitters at $z>1$ in the Subaru HSC survey
• Neutrino Mass Inference from SZ Surveys
• Galaxy clustering at cosmic dawn from JWST/NIRCam observations to redshift z$\sim$11
• Interrelation of the environment of Ly$\alpha$ emitters and massive galaxies at $2<z<4.5$
• Redshift-space correlation functions in large galaxy cluster surveys
• AMICO galaxy clusters in KiDS-DR3: measuring the splashback radius from weak gravitational lensing
• Dependence of galaxy clustering on UV-luminosity and stellar mass at $z\sim 4-7$
• Measurement of redshift dependent cross correlation of HSC clusters and Fermi $\gamma$ rays
• The Breakdown Scale of HI Bias Linearity
• Large-scale bias of dark matter halos
• Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. III. Accurate Measurement of Galaxy Stellar Mass Function with the Aid of Cosmological Redshift Surveys
• Clustering of Extremely Red Objects in Elais-N1 from the UKIDSS DXS with optical photometry from Pan-STARRS1 and Subaru
• Herschel-ATLAS : The spatial clustering of low and high redshift submillimetre galaxies
• The Stellar-to-Halo Mass Ratios of Passive and Star-Forming Galaxies at z~2-3 from the SMUVS survey
• Constraining the galaxy-halo connection of infrared-selected unWISE galaxies with galaxy clustering and galaxy-CMB lensing power spectra
• Lonely Little Red Dots: Challenges to the AGN-nature of little red dots through their clustering and spectral energy distributions
• A Consistent Comparison of Bias Models using Observational Data
• Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of H$\alpha$ and [O III] emitters
• The FMOS-COSMOS survey of star-forming galaxies at $z\sim 1.6$. V: Properties of dark matter halos containing H$\alpha$ emitting galaxies
• Revisiting the Extreme Clustering of $z\approx 4$ Quasars with Large Volume Cosmological Simulations
• The impact of systematic uncertainties in N-body simulations on the precision cosmology from galaxy clustering: a halo model approach
• Percent-level constraints on baryonic feedback with spectral distortion measurements
• Quijote-PNG: The Information Content of the Halo Mass Function
• Cross Correlation between the Thermal Sunyaev-Zel'dovich Effect and Projected Galaxy Density Field
• Halo assembly bias from a deep learning model of halo formation
• Forecasting the Cross-Correlation of the CSST galaxy survey with the FAST HI Intensity Map
• Semi-analytic modelling of AGNs: auto-correlation function and halo occupation
• A minimal empirical model for the cosmic far-infrared background anisotropies
• Towards 1% accurate galaxy cluster masses: Including baryons in weak-lensing mass inference
• A unifying evolutionary framework for infrared-selected obscured and unobscured quasar host haloes
• How accurate is our knowledge of galaxy bias?
• The Cosmic Large-Scale Structure in X-rays (CLASSIX) cluster survey IV: Superclusters in the local Universe at z <= 0.03
• Observing relativistic features in large-scale structure surveys -- I: Multipoles of the power spectrum
• The Dark Matter Haloes and Host Galaxies of MgII Absorbers at z~1
• On the small scale clustering of quasars: constraints from the MassiveBlack II simulation
• Downsizing of Star Formation Measured from the Clustered Infrared Background Correlated with Quasars
• Super-sample covariance of the thermal Sunyaev-Zel'dovich effect
• The halo model with beyond-linear halo bias: unbiasing cosmological constraints from galaxy-galaxy lensing and clustering
• A group-galaxy cross-correlation function analysis in zCOSMOS
• Tracing the galaxy-halo connection with galaxy clustering in COSMOS-Web from z = 0.1 to z ~ 12
• Separate Universe calibration of the dependence of halo bias on cosmic web anisotropy
• Compensated Isocurvature Perturbations in the Galaxy Power Spectrum
• Constraining Scatter in the Stellar Mass--Halo Mass Relation for Haloes Less Massive than the Milky Way
• Multiwavelength study of X-ray Luminous Clusters in the Hyper Suprime-Cam Subaru Strategic Program S16A field
• Differentiable Predictions for Large Scale Structure with SHAMNet
• Indra: a Public Computationally Accessible Suite of Cosmological $N$-body Simulations
• The star formation history in the last 10 billion years from CIB cross-correlations
• Exploring compensated isocurvature perturbations with CMB spectral distortion anisotropies
• Unveiling the largest structures in the nearby Universe: Discovery of the Quipu superstructure
• AMICO galaxy clusters in KiDS-DR3: Cosmological constraints from angular power spectrum and correlation function
• Host Dark Matter Halos of SDSS Red and Blue Quasars: No Significant Difference in Large-scale Environment
• Probing Gravitational Lensing of the CMB with SDSS-IV Quasars
• Incorporating galaxy cluster triaxiality in stacked cluster weak lensing analyses
• Probing gravity with redshift-space distortions: effects of tracer bias and sample selection
• Bayesian framework to infer the Hubble constant from the cross-correlation of individual gravitational wave events with galaxies
• Formation of the large-scale structure of the Universe
• Clustering of CODEX clusters
• Searching for eV-mass Axion-like Particles with Cross Correlations between Line Intensity and Weak Lensing Maps
• An analytic halo approach to the bispectrum of galaxies in redshift space
• Impact of radio sources and cosmic infrared background on thermal Sunyaev-Zel'dovich - gravitational lensing cross correlation
• An Optical Observational Cluster Mass Function at $z\sim 1$ with the ORELSE Survey
• Unveiling cosmological information on small scales with line intensity mapping
• Testing the accuracy of likelihoods for cluster abundance cosmology
• The Cosmic Large-Scale Structure in X-rays (CLASSIX) Cluster Survey III: The Perseus-Pisces supercluster and the Southern Great Wall as traced by X-ray luminous galaxy clusters
• The Cosmic Large-Scale Structure in X-rays (CLASSIX) Cluster Survey II: Unveiling a pancake structure with a 100 Mpc radius in the local Universe
• Improved analytical modeling of the non-linear power spectrum in modified gravity cosmologies
• Higher multipoles of the galaxy bispectrum in redshift space
• A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). VI. Distant Filamentary Structures Pointed by High-z Radio Galaxies at z~4
• The generalized evolution of linear bias: a tool to test gravity
• Optimizing future experiments of cosmic far-infrared background: a principal component approach
• Interpreting the cosmic far-infrared background anisotropies using a gas regulator model
• Signatures of Rapidly Rotating Stars with Chemically Homogeneous Evolution in the First Galaxies
• ODIN: Clustering Analysis of 14,000 Lyα Emitting Galaxies at z=2.4, 3.1, and 4.5
• KiDS+VIKING-450: An internal-consistency test for cosmic shear tomography with a colour-based split of source galaxies
• Dark-ages reionization and galaxy formation simulation XI: Clustering and halo masses of high redshift galaxies
• Validating the methodology for constraining the linear growth rate from clustering anisotropies
• The weak dependence of velocity dispersion on disk fractions, mass-to-light ratio and redshift: Implications for galaxy and black hole evolution
• Intensity Mapping without Cosmic Variance
• CGM${}^2$ $+$ CASBaH: The Mass Dependence of H~I Ly$\alpha$-Galaxy Clustering and the Extent of the CGM
• Exploration of 3D wavelet scattering transform coefficients for line-intensity mapping measurements
• Quasar -- CIV forest cross-correlation with SDSS DR12
• The BAHAMAS project: Evaluating the accuracy of the halo model in predicting the non-linear matter power spectrum
• A systematic search for galaxy protocluster cores at the transition epoch of their star formation activity
• Testing General Relativity Using the Evolution of Linear Bias
• KiDS-1000: Weak lensing and intrinsic alignment around luminous red galaxies
• Reconstruction of Baryon Fraction in Intergalactic Medium through Dispersion Measurements of Fast Radio Bursts
• MaNGA DynPop -- IV. Stacked total density profile of galaxy groups and clusters from combining dynamical models of integral-field stellar kinematics and galaxy-galaxy lensing
• Thermal and Reionisation History within a Large-Volume Semi-Analytic Galaxy Formation Simulation
• Constraints on Neutrino Mass from Sunyaev--Zeldovich Cluster Surveys
• Constraining the physics of star formation from CIB-cosmic shear cross-correlations
• Constraining the Halo Mass of Damped Ly$\alpha$ Absorption Systems (DLAs) at $z=2-3.5$ using the Quasar-CMB Lensing Cross-correlation
• Extracting galaxy merger timescales I: Tracking haloes with WhereWolf and spinning orbits with OrbWeaver
• Dynamical friction in the primordial neutrino sea
• Cosmological feedback from a halo assembly perspective
• The thermal and gravitational energy densities in the large-scale structure of the Universe
• Statistics of Dark Matter Halos in the Excursion Set Peak Framework
• Linking galaxies to dark matter haloes at $z\sim 1$ : dependence of galaxy clustering on stellar mass and specific star formation rate
• What can the spatial distribution of galaxy clusters tell about their scaling relations?
• Clustering, Cosmology and a New Era of Black Hole Demographics -- II. The Conditional Luminosity Functions of Type 2 and Type 1 Active Galactic Nuclei
• The impact of braiding covariance and in-survey covariance on next-generation galaxy surveys
• Neutrino winds on the sky
• Forecasts on neutrino mass constraints from the redshift-space two-point correlation function
• Dark Stars and Boosted Dark Matter Annihilation Rates
• Nonlinearities in modified gravity cosmology. II. Impacts of modified gravity on the halo properties
• A Universal Profile for Stacked Filaments from Cold Dark Matter Simulations
• A measurement of the Integrated Sachs-Wolfe Effect with the Rapid ASKAP Continuum Survey
• Lensing dispersion of supernova flux: a probe of nonlinear structure growth
• Cross Correlation of the Extragalactic Gamma-ray Background with Thermal Sunyaev-Zel'dovich Effect in the Cosmic Microwave Background
• The XXL Survey XXXII. Spatial clustering of the XXL-S AGN
• The Subaru HSC weak lensing mass-observable scaling relations of spectroscopic galaxy groups from the GAMA survey
• Cosmological constraints from multiple tracers in spectroscopic surveys
• The Impact of the Dusty Torus on Obscured Quasar Halo Mass Measurements
• A semi-analytic model of pairwise velocity distribution between dark matter halos
• Testing the SZ-based tomographic approach to the thermal history of the universe with pressure-density cross-correlations: Insights from the Magneticum simulation
• Inverse-Compton Scattering of the Cosmic Infrared Background
• Constraints on dark matter and astrophysics from tomographic $\gamma$-ray cross-correlations
• PAC in DESI. I. Galaxy Stellar Mass Function into the $10^6{\mathrm{M}}_{\odot }$ Frontier
• Modified initial power spectrum and too big to fail problem
• 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
• 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
• The halo bispectrum as a sensitive probe of massive neutrinos and baryon physics
• Constraints on galaxy formation from the cosmic-far-infrared-background\,$-$\,optical-imaging cross-correlation using \textit{Herschel} and UNIONS
• The CIDER simulations: Nonlinear structure formation in the Constrained Interacting Dark Energy Scenario
• The deconvolved distribution estimator: enhancing reionisation-era CO line-intensity mapping analyses with a cross-correlation analogue for one-point statistics
• On the ISW-cluster cross-correlation in future surveys
• Euclid preparation. LII. Forecast impact of super-sample covariance on 3x2pt analysis with Euclid
• Modeling Lyman-α Forest Cross-Correlations with LyMAS
• Exploring the mass and redshift dependence of the cluster pressure profile with stacks on thermal SZ maps
• The integrated angular bispectrum
• A forecast for the detection of the power asymmetry from galaxy surveys
• A Stochastic Theory of the Hierarchical Clustering II. Halo progenitor mass function and large-scale bias
• A pseudo-spectrum analysis of galaxy-galaxy lensing
• Constraints on Non-Gaussianity from Sunyaev--Zeldovich Cluster Surveys
• Improving Constraints on Fundamental Physics Parameters with the Clustering of Sunyaev-Zeldovich Selected Galaxy Clusters
• Clustering, Cosmology and a New Era of Black Hole Demographics -- I. The Conditional Luminosity Function of Active Galactic Nuclei
• Multi-wavelength consensus of large-scale linear bias
• Cosmology in the non-linear regime : the small scale miracle
• Modeling Post-Reionization HI Distributions in Fuzzy Dark Matter Cosmologies Using Conditional Normalizing Flows
• Primordial Black-Hole-Based Pathways to Little Red Dots
• An efficient hybrid method to produce high resolution large volume dark matter simulations for semi-analytic models of reionisation
• Quantifying the statistics of CMB-lensing-derived galaxy cluster mass measurements with simulations
• X-ray cluster cosmology
• Probing Reionization-Era Galaxies with JWST UV Luminosity Functions and Large-Scale Clustering
• The feasibility of constraining DM interactions with high-redshift observations by JWST
• Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
• Removing Interlopers From Intensity Mapping Probes Of Primordial Non-Gaussianity
• Euclid preparation: Determining the weak lensing mass accuracy and precision for galaxy clusters
• Exploring the physical origins of halo assembly bias from early times
• Galaxy clusters as intrinsic alignment tracers: present and future
• The X-ray Angular Power Spectrum of Extended Sources in the eROSITA Final Equatorial Depth Survey
• Cosmic star formation history with tomographic cosmic infrared background-galaxy cross-correlation
• Towards Optimal Foreground Mitigation Strategies for Interferometric HI Intensity Mapping in the Low-Redshift Universe
• Tidal shear and the consistency of microscopic Lagrangian halo approaches
• New insight into the variability of the Be star $\pi$ Aquarii: Determination of stellar and disk parameters
• A Pair of Early- and Late-Forming Galaxy Cluster Samples: a Novel Way of Studying Halo Assembly Bias Assisted by a Constrained Simulation
• Towards Accurate Modeling of Line-Intensity Mapping One-Point Statistics: Including Extended Profiles
• Probing the Cosmological Principle with the CSST Photometric Survey
• The PAU Survey: Close galaxy pairs identification and analysis
• Deep learning insights into non-universality in the halo mass function
• The shape of dark matter halos: a new fundamental cosmological invariance
• AMICO galaxy clusters in KiDS-1000: cosmological constraints and mass calibration from counts and weak lensing
• Signatures of reionization feedback in the near-infrared background
• The galaxy power spectrum on the lightcone: deep, wide-angle redshift surveys and the turnover scale
• Redshifted 21-cm emission signal from the halos in Dark Ages
• The galaxy bias profile of cosmic voids
• The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
• Cosmology and Astrophysics with the Diffuse eRASS1 X-ray Angular Power Spectrum
• Unexpected clustering pattern in dwarf galaxies challenges formation models
• Cross-correlation between soft X-rays and galaxies A new benchmark for galaxy evolution models
• Secondary halo bias through cosmic time II: Reconstructing halo properties using clustering information
• Physical Models for the Clustering of Obscured and Unobscured Quasars
• Mass bias and cosmological constraints from Planck cluster clustering
• Evolution of matter and galaxy clustering in cosmological hydrodynamical simulations
• Accurate dark matter halo elongation from weak-lensing stacking analysis
• Weak gravitational lensing as a probe of physical properties of substructures in dark matter halos
• B-modes from galaxy cluster alignments in future surveys
• Fast Simulation of Cosmological Neutral Hydrogen based on the Halo Model
• Non-Gaussian assembly bias from a semi-analytic galaxy formation model
• Cosmic Variance and the Inhomogeneous UV Luminosity Function of Galaxies During Reionization
• Correlation Analysis of Decaying Sterile Neutrino Dark Matter in the Context of the SRG Mission
• Forecasts for Warm Dark Matter from Photometric Galaxy Surveys
• Dependence on the environment of the abundance function of light-cone simulation dark matter haloes
• Bias-Limited Extraction of Cosmological Parameters
• How do uncertainties in galaxy formation physics impact field-level galaxy bias?
• Origin of Metals around Galaxies I: Catalogs of Metal-line Absorption Doublets from High-Resolution Quasar Spectra
• Galaxy and Mass Assembly (GAMA): Probing galaxy-group correlations in redshift space with the halo streaming model
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• Doppler boosted dust emission and CIB-galaxy cross-correlations: a new probe of cosmology and astrophysics
• Constraining cosmology with thermal Sunyaev-Zel'dovich maps: Minkowski functionals, peaks, minima, and moments
• Stacked phase-space density of galaxies around massive clusters: Comparison of dynamical and lensing masses
• Euclid preparation. Exploring the properties of proto-clusters in the Simulated Euclid Wide Survey
• An Improved Treatment of Cosmological Intergalactic Medium Evolution
• The SRG/eROSITA All-Sky Survey: Exploring halo assembly bias with X-ray selected superclusters
• Scaling of the 1-halo terms with bias
• Leveraging cross-correlations and linear covariance-based filtering for line-intensity map reconstructions at linear scales
• The Dependence of Dark Matter Halo Properties on the Morphology of Their Central Galaxies from Weak Lensing
• The mass and galaxy distribution around SZ-selected clusters
• Disentangling the Halo: Joint Model for Measurements of the Kinetic Sunyaev-Zeldovich Effect and Galaxy-Galaxy Lensing
• Intrinsic alignment from multiple shear estimates: A first application to data and forecasts for Stage IV
• Astrophysical systematics in Kinematic Lensing: quantifying an Intrinsic Alignment analog
• Measuring the scatter of the mass-richness relation in galaxy clusters in photometric imaging surveys by means of their correlation function
• Inferring Host Dark Matter Halo Masses of Individual Galaxies from Neighboring Galaxy Counts
• Cosmic Census: Relative Distributions of Dark Matter, Galaxies and Diffuse Gas
• Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
• Constraining the Star Formation Rate using Joint CIB Continuum and [CII] Intensity Mapping
• Fisher matrix forecasts on the astrophysics of galaxies during the epoch of reionisation from the 21-cm power spectra
• The impact of halo concentration on the Sunyaev Zel'dovich effect signal from massive galaxy clusters
• The influence of superstructures on bright galaxy environments: clustering properties
• LATIS: Comparing Galaxy and IGM Tomography Maps as Tracers of Large-scale Structure and Protoclusters at $z\sim 2.5$
• An empirical method for mitigating an excess up-scattering mass bias on the weak lensing mass estimates for shear-selected cluster samples
• On the Dark Matter Halos of Optical and IR-selected AGN in the Local Universe
• Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
• Deciphering Baryonic Feedback from ACT tSZ Galaxy Clusters
• Relatively Fast and Reasonably Furious: Evidence for Increased Burstiness in Smaller Halos at Cosmic Dawn
• The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes
• Towards a multi-tracer neutrino mass measurement with line-intensity mapping
• Aemulus $\nu$: Precision halo mass functions in w$\nu$CDM cosmologies
• The linear bias of radio galaxies at z~0.3 via cosmic microwave background lensing
• An Order Statistics Approach to the Halo Model for Galaxies
• Comparison of the linear bias models in the light of the Dark Energy Survey
• A halo model approach to describe clustering and emission of the two main star forming galaxy populations for Cosmic Infrared Background studies
• Removal of interloper contamination to line-intensity maps using correlations with ancillary tracers of the large-scale structure
• Probabilistic Lagrangian bias estimators and the cumulant bias expansion
• Direct correlation of line intensity mapping and CMB lensing from evolution along the lightcone
• Bounds on galaxy stochasticity from halo occupation distribution modeling
• Dark Energy Survey Year 3 results: Galaxy-halo connection from galaxy-galaxy lensing
• Assembly bias in quadratic bias parameters of dark matter halos from forward modeling
• oLIMpus: An Effective Model for Line Intensity Mapping Auto- and Cross- Power Spectra in Cosmic Dawn and Reionization
• Constraining the halo-ISM connection through multi-transition carbon monoxide line-intensity mapping
• Forecasts for cosmological measurements based on the angular power spectra of AGN and clusters of galaxies in the SRG/eROSITA all-sky survey
• Impact of projection-induced optical selection bias on the weak lensing mass calibration of galaxy clusters
• Environment-based selection effects of Planck clusters
• A first look at quasar-galaxy clustering at $z\simeq 7.3$
• Lyα Intensity Mapping in HETDEX: Galaxy-Lyα Intensity Cross-Power Spectrum
• Breaking degeneracies with the Sunyaev-Zeldovich full bispectrum
• On the tomographic cluster clustering as a cosmological probe
• On the Assembly Bias of Cool Core Clusters Traced by H$\alpha$ Nebulae
• A semi-analytic estimate for the effective sound speed counterterm in the EFTofLSS
• A physically-motivated template set for high-z galaxy SED fitting
• Comparison of the spatial and the angular clustering of X-ray AGN
• Euclid preparation. L. Calibration of the linear halo bias in $\Lambda (\nu )$CDM cosmologies
• Individual halo bias in models of $f(R)$ gravity
• A New Wavelet Scattering Transform-Based Statistic for Cosmological Analysis of Large-Scale Structure
• Angular correlation functions of bright Lyman-break galaxies at $3\lesssim \mathbf{z}\lesssim 5$
• The SRG/eROSITA All-Sky Survey. Detection of shock-heated gas beyond the halo boundary into the accretion region
• KiDS-Legacy: WIMP dark matter constraints from the cross-correlation of weak lensing and Fermi-LAT gamma rays
• MIGHTEE: The dark matter haloes, duty cycle and mechanical feedback from radio-AGN up to $z\sim 2.5$
• Probing baryonic feedback with fast radio bursts: joint analyses with cosmic shear and galaxy clustering
• Stellar population modelling of neutron stars and black holes: spatially-resolved graveyards in MaNGA/SDSS-IV galaxies
• A CMB lensing analysis of the extended mass distribution of clusters
• The pairwise and cross-pairwise y-type polarised kinetic Sunyaev Zeldovich effect from transverse velocity of galaxy clusters
• Constraining AGN feedback model with SZ profile
• Dark matter halos of luminous AGNs from galaxy-galaxy lensing with the HSC Subaru Strategic Program
• The non-thermal secondary CMB anisotropies from a cosmic distribution of radio galaxy lobes
• Strong Conformity and Assembly Bias: Towards a Physical Understanding of the Galaxy-Halo Connection in SDSS Clusters
• Exploiting Non-linear Scales in Galaxy-Galaxy Lensing and Galaxy Clustering: A Forecast for the Dark Energy Survey
• AMICO galaxy clusters in KiDS-DR3: the impact of estimator statistics on the luminosity-mass scaling relation
• Cross-correlations between mm-wave line-intensity mapping and weak lensing surveys: preliminary consideration of long-term prospects
• Cosmic voids and BAO with relative baryon-CDM perturbations
• Measuring weak lensing masses on individual clusters
• Forecasting the potential of weak lensing magnification to enhance LSST large-scale structure analyses
• A dynamics-based density profile for dark haloes. I. Algorithm and basic results
• Uncertainty-Aware Neural Networks for Fuzzy Dark Matter Model Selection from \texorpdfstring{$x_{\mathrm{HI}}$}{x_HI} Measurements
• On Weak Lensing Response Functions
• Constraining cosmological parameters using density split lensing and the conditional stellar mass function
• Streaming Velocity Effects on the Post-reionization 21 cm Baryon Acoustic Oscillation Signal
• Towards including super-sample covariance in the unbinned likelihood for cluster abundance cosmology
• Lagrangian Perturbation Theory for Biased Tracers: Significance of the Number Conservation
• Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy
• A redshift distortion free correlation function at third order in the nonlinear regime
• A Non-parametric Method for the Inference of Halo Occupation Distributions
• Impact of the calibration of the Halo Mass Function on galaxy cluster number count cosmology
• The Hydrostatic Mass Bias and the ${\sigma }_8$ Tension: A Multi-Probe Forecast for Stage-IV/V Surveys
• Sahyadri: A simulation suite for the cosmology dependence of the Cosmic Web
• Catalogs of optically-selected clusters and photometric luminous red galaxies from the Hyper Suprime-Cam Subaru Strategic Program final year dataset
• Unveiling the evolution of the CO excitation ladder through cross-correlation of CONCERTO-like experiments and galaxy redshift surveys
• Built-in precision: Improving cluster cosmology through the self-calibration of a galaxy cluster sample
• Challenges of standard halo models in constraining galaxy properties from CIB anisotropies
• Improving cosmological covariance matrices with machine learning
• Revisiting secondary CMB distortions due to kinetic Sunyaev-Zel'dovich effect from quasar bubbles before reionization