An analytic model for the spatial clustering of dark matter haloes

Abstract

We develop a simple analytic model for the gravitational clustering of dark matter haloes to understand how their spatial distribution is biased relative to that of the mass. The statistical distribution of dark haloes within the initial density field (assumed Gaussian) is determined by an extension of the Press-Schechter formalism. Modifications of this distribution caused by gravitationally induced motions are treated using a spherical collapse approximation. We test this model against results from a variety of N-body simulations, and find that it gives an accurate description of a bias function. This bias function is sufficient to calculate the cross-correlation between dark haloes and mass, and again we find excellent agreement between simulation results and analytic predictions. Because haloes are spatially exclusive, the variance in the count of objects within spheres of fixed radius and overdensity is significantly smaller than the Poisson value. This seriously complicates any analytic calculation of the autocorrelation function of dark halos. Our simulation results show that this autocorrelation function is proportional to that of the mass over a wide range in $R$, even including scales where both functions are significantly greater than unity. The constant of proportionality is very close to that predicted on large scales by the analytic model. This result permits an entirely analytic estimate of the autocorrelation function of dark haloes. We use our model to study how the distribution of galaxies may be biased with respect to that of the mass. In conjunction with other data these techniques should make it possible to measure the amplitude of cosmic mass fluctuations and the density of the Universe.

arXiv comment34 pages including 7 figs, gziped ps file, submitted to MNRAS

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• The Spatial Clustering of Distant, z~1, Early-Type Galaxies
• Halo model and halo properties in Galileon gravity cosmologies
• Measuring Angular Diameter Distances through Halo Clustering
• A halo bias function measured deeply into voids without stochasticity
• Sunyaev-Zeldovich effect from hydrodynamical simulations: maps and low order statistics
• Stellar Populations of Elliptical Galaxies in the Local Universe
• A Lyman-α protocluster at redshift 6.9
• The SDSS-DR12 large-scale cross-correlation of Damped Lyman Alpha Systems with the Lyman Alpha Forest
• Observational evidence for a local underdensity in the Universe and its effect on the measurement of the Hubble Constant
• The Peaks Formalism and the Formation of Cold Dark Matter Haloes
• The Cosmic Large-Scale Structure in X-rays (CLASSIX) Cluster Survey I: Probing galaxy cluster magnetic fields with line of sight rotation measures
• Galaxy clustering from COMBO-17: The halo occupation distribution at <z>=0.6
• The 21cm Signature of the First Stars
• Clustering, Bias and the Accretion Mode of X-ray selected AGN
• The nebular emission of star-forming galaxies in a hierarchical universe
• Testing one-loop galaxy bias: joint analysis of power spectrum and bispectrum
• PRIMUS: Galaxy Clustering as a Function of Luminosity and Color at 0.2<z<1
• Halo model description of the non-linear dark matter power spectrum at $k\gg 1$ Mpc${}^{-1}$
• PRIMUS + DEEP2: Clustering of X-ray, Radio and IR-AGN at z~0.7
• Cosmology with the Large Synoptic Survey Telescope: an Overview
• Verifying the consistency relation for the scale-dependent bias from local primordial non-Gaussianity
• Do Distinct Cosmological Models Predict Degenerate Halo Populations?
• Dark matter halo abundances, clustering and assembly histories at high redshift
• The First Generation of Star-Forming Haloes
• Cosmological redshift-space distortion on clustering of high-redshift objects: correction for nonlinear effects in power spectrum and tests with N-body simulations
• Scale-dependent bias from primordial non-Gaussianity in general relativity
• Non-Linear gravitational growth of large scale structures inside and outside standard Cosmology
• Primordial Non-Gaussianity and the NRAO VLA Sky Survey
• Accurate Predictions for the Scale-Dependent Galaxy Bias from Primordial Non-Gaussianity
• N-body simulations with generic non-Gaussian initial conditions II: Halo bias
• Observational Signatures of the First Luminous Objects
• Constraining Primordial Non-Gaussianity with High-Redshift Probes
• The environmental dependence of galaxy clustering in the Sloan Digital Sky Survey
• Constraints on Primordial Non-Gaussianity from Large Scale Structure Probes
• Large-scale assembly bias of dark matter halos
• The clustering of SDSS galaxy groups: mass and color dependence
• The K20 survey. II. The Different Spatial Clustering of z~1 Old and Dusty Star-Forming EROs
• How unusual are the Shapley Supercluster and the Sloan Great Wall?
• The 2dF Galaxy Redshift Survey: The clustering of galaxy groups
• Correlation properties of the kinematic Sunyaev-Zel'dovich effect and implications for Dark Energy
• Einstein, Planck and Vera Rubin: relevant encounters between the Cosmological and the Quantum Worlds
• Halo bias in Lagrangian Space: Estimators and theoretical predictions
• The cross-correlation between galaxies of different luminosities and Colors
• The Three-point Correlation Function of Galaxies: Comparing Halo Occupation Models with Observations
• Combining clustering and abundances of galaxy clusters to test cosmology and primordial non-Gaussianity
• Damped Lyman alpha systems and disk galaxies: number density, column density distribution and gas density
• Biased Reionisation and Non-Gaussianity in Redshifted 21cm Intensity Maps of the Reionisation Epoch
• The VIMOS-VLT Deep Survey: Luminosity dependence of clustering at z~1
• On Combining Galaxy Clustering and Weak Lensing to Unveil Galaxy Biasing via the Halo Model
• Constraining halo occupation properties of X-ray AGNs using clustering of Chandra sources in the Bootes survey region
• The Cross-Correlation of High-Redshift 21 cm and Galaxy Surveys
• Constraining evolution in the Halo Model using galaxy redshift surveys
• Properties of Dark Matter Halos as a Function of Local Environment Density
• Bayesian inference of cosmic density fields from non-linear, scale-dependent, and stochastic biased tracers
• Primordial non-Gaussianity in the large scale structure of the Universe
• Weak Lensing by Large-Scale Structure: A Dark Matter Halo Approach
• Implications of Spikes in the Redshift Distribution of $z\sim 3$ Galaxies
• Sunyaev-Zeldovich Fluctuations from the First Stars?
• The Kurtosis of the Cosmic Shear Field
• Modeling the nonlinear clustering in modified gravity models I: A fitting formula for matter power spectrum of f(R) gravity
• The observational signature of the first H II regions
• Optimal capture of non-Gaussianity in weak lensing surveys: power spectrum, bispectrum and halo counts
• Accurate determination of the Lagrangian bias for the dark matter halos
• The Canada-France deep fields survey-II: Lyman-break galaxies and galaxy clustering at z~3
• The potential of X-ray cluster surveys to constrain primordial non-Gaussianity
• The galaxy-halo connection of emission-line galaxies in IllustrisTNG
• Joint Measurement of Lensing-Galaxy Correlations Using SPT and DES SV Data
• Cosmological Measurements with Forthcoming Radio Continuum Surveys
• The clustering of Ly-alpha emitters in a LambdaCDM Universe
• Large scale structure around a z=2.1 cluster
• Two Ways of Biasing Galaxy Formation
• The correlation structure of dark matter halo properties
• Euclid: Cosmological forecasts from the void size function
• The history of star formation from the cosmic infrared background anisotropies
• Nonlinear density evolution from an improved spherical collapse model
• Calibration of bias and scatter involved in cluster mass measurements using optical weak gravitational lensing
• Numerical and Analytical Predictions for the Large-Scale Sunyaev-Zel'dovich Effect
• PINOCCHIO and the hierarchical build-up of dark matter haloes
• Empirical constraints on the formation of early-type galaxies
• The multidimensional dependence of halo bias in the eye of a machine: a tale of halo structure, assembly and environment
• Strong clustering of underdense regions and the environmental dependence of clustering from Gaussian initial conditions
• Separate Universe Consistency Relation and Calibration of Halo Bias
• Measurement of the halo bias from stacked shear profiles of galaxy clusters
• Joint analysis of cluster number counts and weak lensing power spectrum to correct for the super-sample covariance
• Bias, redshift space distortions and primordial nongaussianity of nonlinear transformations: application to Lyman alpha forest
• Cosmological Parameters Degeneracies and Non-Gaussian Halo Bias
• How to Grow a Healthy Merger Tree
• A Strategy to Measure the Dark Energy Equation of State using the HII galaxy Hubble Relation & X-ray AGN Clustering: Preliminary Results
• The VIMOS-VLT Deep Survey. The dependence of clustering on galaxy stellar mass at z~1
• Extensions to models of the galaxy-halo connection
• Extragalactic gamma-ray background radiation from dark matter annihilation
• The Cosmic Reionization History as Revealed by the CMB Doppler--21-cm Correlation
• Constraining primordial non-Gaussianity using two galaxy surveys and CMB lensing
• Linear response to long wavelength fluctuations using curvature simulations
• Halo-model Analysis of the Clustering of Photometrically Selected Galaxies from SDSS
• Cosmological Constraints from the Clustering Properties of the X-Ray Brightest Abell-type Cluster Sample
• Deriving an Accurate Formula of Scale-dependent Bias with Primordial Non-Gaussianity: An Application of the Integrated Perturbation Theory
• The LBT Bootes Field Survey: I. The Rest-frame UV and Luminosity Functions and Clustering of Bright Lyman Break Galaxies at z~3
• Spatial Correlation Function of the Chandra Selected Active Galactic Nuclei
• The clustering and bias of radio-selected AGN and star-forming galaxies in the COSMOS field
• Mapping dark matter with cosmic magnification
• The Two-Point Correlation of Galaxy Groups: Probing the Clustering of Dark Matter Haloes
• An Analytical Approach to Inhomogeneous Structure Formation
• The Halo Bispectrum in N-body Simulations with non-Gaussian Initial Conditions
• Nonlinear clustering in models with primordial non-Gaussianity: the halo model approach
• Cosmic Mass Functions from Gaussian Stochastic Diffusion Processes
• Environment and Galaxy Evolution at Intermediate Redshift in the CNOC2 Survey
• Cosmological constraints from the BOSS DR12 void size function
• Nonlinear Biasing and Redshift-Space Distortions in Lagrangian Resummation Theory and N-body Simulations
• An analytical model for the non-linear redshift-space power spectrum
• Biases from neutrino bias: to worry or not to worry?
• Mapping stellar content to dark matter halos - III.Environmental dependence and conformity of galaxy colours
• Evidence of pre-processing and a dependence on dynamical state for low-mass satellite galaxies
• TheHaloMod: An online calculator for the halo model
• Modelling the post-reionization neutral Hydrogen (\HI) bias
• The XMM-Newton wide-field survey in the COSMOS field: V. Angular Clustering of the X-ray Point Sources
• LoCuSS: The infall of X-ray groups onto massive clusters
• Fluctuations in the High-Redshift Lyman-Werner and Lyman-alpha Radiation Backgrounds
• The spatial and velocity bias of linear density peaks and proto-haloes in the Lambda cold dark matter cosmology
• Scale dependent halo bias in the excursion set approach
• Approximate Bayesian Computation in Large Scale Structure: constraining the galaxy-halo connection
• Photon number conservation and the large-scale 21 cm power spectrum in semi-numerical models of reionization
• The clustering and abundance of star-forming and passive galaxies at $z\sim 2$
• Interpreting the Clustering of Distant Red Galaxies
• The DEEP2 Galaxy Redshift Survey: The Evolution of Void Statistics from z~1 to z~0
• Triaxial haloes, intrinsic alignments and the dark matter power spectrum
• Statistics of Weak Lensing at Small Angular Scales: Analytical Predictions for Lower Order Moments
• The nature of assembly bias - I. Clues from a LCDM cosmology
• The Evolution of Bias - Generalized
• The dependence of the galaxy stellar-to-halo mass relation on galaxy morphology
• Probing the IGM-Galaxy Connection Toward PKS0405-123 II : A Cross-Correlation Study of Lya Absorbers and Galaxies at z<0.5
• The evolution of galaxy clustering since z = 3 using the UKIDSS Ultra Deep Survey: the divergence of passive and star-forming galaxies
• The Mass Function of Void Galaxies in the SDSS Data Release 2
• Measuring our universe from galaxy redshift surveys
• Asymmetric Sky from the Long Mode Modulations
• Matter bispectrum of large-scale structure: Three-dimensional comparison between theoretical models and numerical simulations
• The VLT LBG Redshift Survey I: Clustering and Dynamics of ~1000 Galaxies at z~3
• The Asiago-ESO/RASS QSO Survey. III. Clustering analysis and its theoretical interpretation
• The effect of baryons on the variance and the skewness of the mass distribution in the universe at small scales
• The XXL Survey: XVI. The clustering of X-ray selected galaxy clusters at z~0.3
• The Atacama Cosmology Telescope: measuring radio galaxy bias through cross-correlation with lensing
• Angular correlation function of 1.5 million LRGs: clustering evolution and a search for BAO
• Quasar-Galaxy and Galaxy-Galaxy Cross-Correlations: Model Predictions with Realistic Galaxies
• Scale-dependent halo bias from scale-dependent growth
• Correlations in the Far Infrared Background
• Origin of Two Distinct Populations in Dwarf Spheroidal Galaxies
• The evolution of clustering length, large-scale bias and host halo mass at 2<z<5 in the VIMOS Ultra Deep Survey (VUDS)
• Reconstruction of cosmological initial conditions from galaxy redshift catalogues
• Elucidating Galaxy Assembly Bias in SDSS
• Voids in Modified Gravity Reloaded: Eulerian Void Assignment
• QSO-LRG 2-Point Cross-Correlation Function and Redshift-Space Distorions
• Environmental Effects on Real-Space and Redshift-Space Galaxy Clustering
• Spectroscopic observations of PHz G237.01+42.50: A galaxy protocluster at z=2.16 in the Cosmos field
• Clustering, host halos and environment of z$\sim$2 galaxies as a function of their physical properties
• Dark Matter Halo Models of Stellar Mass-Dependent Galaxy Clustering in PRIMUS+DEEP2 at 0.2<z<1.2
• The correlation between the distribution of galaxies and 21cm emission at high redshifts
• Gravitational redshifts from large-scale structure
• Effects of Sampling on Statistics of Large Scale Structure
• The Observed Evolution of Galaxy Clustering Vs. Epoch-Dependent Biasing Models
• Inhomogeneous Helium Reionization and the Equation of State of the Intergalactic Medium
• The clustering and evolution of H-alpha emitters at z~1 from HiZELS
• What is the best way to measure baryonic acoustic oscillations?
• The clustering properties of radio-selected AGN and star-forming galaxies up to redshifts z~3
• Measuring the Dark Matter Halo Mass of X-ray AGN at z~1 using photometric redshifts
• Spatially Resolved Galaxy Star Formation and its Environmental Dependence I
• Optimal linear reconstruction of dark matter from halo catalogs
• Non-Gaussianity from Large-Scale Structure Surveys
• Stochastic Biasing and Galaxy-Mass Density Relation in the Weakly Non-linear Regime
• Galaxy and Mass Assembly (GAMA): The evolution of bias in the radio source population to z ~ 1.5
• The Bias and Mass Function of Dark Matter Halos in Non-Markovian Extension of the Excursion Set Theory
• Large scale structure in the HI Parkes All-Sky Survey: Filling the Voids with HI galaxies?
• Excursion Set Halo Mass Function and Bias in a Stochastic Barrier Model of Ellipsoidal Collapse
• Testing one-loop galaxy bias: Power spectrum
• Exploring galaxies-gravitational waves cross-correlations as an astrophysical probe
• Local stochastic non-Gaussianity and N-body simulations
• Scale-dependent bias and the halo model
• Why Do Stars Form In Clusters? An Analytic Model for Stellar Correlation Functions
• The VLT LBG Redshift Survey - V. Characterising the z = 3.1 Lyman Alpha Emitter Population
• Measuring the Nonlinear Biasing Function from a Galaxy Redshift Survey
• Cosmology Inference from Biased Tracers using the EFT-based Likelihood
• Cluster Formation Rate in Models with Dark Energy
• Two-point correlation function of high-redshift objects: an explicit formulation on a light-cone hypersurface
• Spherical Collapse and Cluster Counts in Modified Gravity Models
• Angular power spectrum of gamma-ray sources for GLAST: blazars and clusters of galaxies
• Bias and Hierarchical Clustering
• The Imprint of f(R) Gravity on Non-Linear Structure Formation
• Modelling large-scale halo bias using the bispectrum
• Combined analysis of galaxy cluster number count, thermal Sunyaev-Zel'dovich power spectrum, and bispectrum
• Nonlinear stochastic biasing from the formation epoch distribution of dark halos
• On the measurements of assembly bias and splashback radius using optically selected galaxy clusters
• The Morphology-Density relationship in 1<z<2 clusters
• GaBoDS: The Garching-Bonn Deep Survey: VII. Probing galaxy bias using weak gravitational lensing
• Constraining large scale HI bias using redshifted 21-cm signal from the post-reionization epoch
• Galaxy Clustering Evolution in the CNOC2 High-Luminosity Sample
• Redshifted 21 Centimeter Emission from Minihalos Before Reionization
• Probing primordial non-Gaussianity via iSW measurements with SKA continuum surveys
• Joint Analysis of Gravitational Lensing, Clustering and Abundance: Toward the Unification of Large-Scale Structure Analysis
• Testing standard perturbation theory and the Eulerian local biasing scheme against N-body simulations
• Large Scale Structure of the Universe
• Observational constraints on particle production during inflation
• From Images to Dark Matter: End-To-End Inference of Substructure From Hundreds of Strong Gravitational Lenses
• The evolution of host mass and black hole mass in QSOs from the 2dF QSO Redshift Survey
• Cluster abundances and S-Z power spectra: effects of non-Gaussianity and early dark energy
• On the evolution of clustering of 24um-selected galaxies
• The Impact of Theoretical Uncertainties in the Halo Mass Function and Halo Bias on Precision Cosmology
• Scale-dependent Galaxy Bias
• Formation time distribution of dark matter haloes: theories versus N-body simulations
• The XMM-{\em Newton}/2dF Survey - VI: Clustering and Bias of the Soft X-ray Point Sources
• The Difference PDF of 21-cm Fluctuations: A Powerful Statistical Tool for Probing Cosmic Reionization
• Halo stochasticity in global clustering analysis
• Is there enough star formation in simulated protoclusters?
• Estimating Luminosity Function Constraints from High-Redshift Galaxy Surveys
• Fractal Dimensions of a Weakly Clustered Distribution and the Scale of Homogeneity
• Bias deconstructed: Unravelling the scale dependence of halo bias using real space measurements
• The clustering of galaxy clusters in cosmological models with non-Gaussian initial conditions: Predictions for future surveys
• The formation of CDM haloes I: Collapse thresholds and the ellipsoidal collapse model
• The Halo Occupation Distribution of X-ray-Bright Active Galactic Nuclei: A Comparison with Luminous Quasars
• Bispectrum Supersample Covariance
• The Galaxy Correlation Function in the CNOC2 Redshift Survey: Dependence on Color, Luminosity and Redshift
• Mass function and bias of dark matter halos for non-Gaussian initial conditions
• Spectroscopic Confirmation of a Coma Cluster Progenitor at z ~ 2.2
• How smooth are particle trajectories in a $\Lambda$CDM Universe?
• The Effects of Halo Assembly Bias on Self-Calibration in Galaxy Cluster Surveys
• Halo abundances within the cosmic web
• Cross correlation of Lyman-alpha absorbers with gas-rich galaxies
• BAM: Bias Assignment Method to generate mock catalogs
• Nonlinear Bias of Cosmological Halo Formation in the Early Universe
• Edgeworth streaming model for redshift space distortions
• The massive end of the luminosity and stellar mass functions and clustering from CMASS to SDSS: Evidence for and against passive evolution
• Detection of anisotropic galaxy assembly bias in BOSS DR12
• The Three Hundred Project: The influence of environment on simulated galaxy properties
• Relating the structure of dark matter halos to their assembly and environment
• Angular correlations in the cosmic gamma-ray background from dark matter annihilation around intermediate-mass black holes
• The environmental dependence of clustering in hierarchical models
• Substructure in dark matter halos: Towards a model of the abundance and spatial distribution of subclumps
• The clustering of X-ray selected AGN at z=0.1
• Reliability of the dark matter clustering in cosmological N-body simulation on scales below the mean separation length of particles
• Population III Star Formation In Large Cosmological Simulations I. Halo Temporal and Physical Environment
• On the spatial distribution of dark matter halos
• A new method of measuring the cluster peculiar velocity power spectrum
• The Secondary Spin Bias of Dark Matter Haloes
• Non-linear Galaxy Power Spectrum and Cosmological Parameters
• Position-dependent correlation function from the SDSS-III Baryon Oscillation Spectroscopic Survey Data Release 10 CMASS Sample
• Constraint of Void Bias on Primordial non-Gaussianity
• A Search for the Most Massive Galaxies. II. Structure, Environment and Formation
• Most massive halos with Gumbel Statistics
• Integrated Perturbation Theory and One-loop Power Spectra of Biased Tracers
• Cosmological Evolution of Linear Bias
• Cosmological constraints from galaxy clustering in the presence of massive neutrinos
• How much a galaxy knows about its large-scale environment?: An information theoretic perspective
• Clustering of X-Ray-Selected AGN
• The Environmental Dependence of the Luminosity-Size Relation for Galaxies
• Why does the clustering of haloes depend on their formation history
• Measurement of the thermal Sunyaev-Zel'dovich effect around cosmic voids
• The impact of halo shapes on the bispectrum in cosmology
• The Selection Function of SZ Cluster Surveys
• Deep Realistic Extragalactic Model (DREaM) Galaxy Catalogs: Predictions for a Roman Ultra-Deep Field
• Massive Star-Forming Galaxies Have Converted Most of Their Halo Gas into Stars
• PLCK G165.7+67.0: Analysis of a Massive Lensing Cluster in a Hubble Space Telescope Census of Submillimeter Giant Arcs Selected Using Planck/Herschel
• A Prescription for Galaxy Biasing Evolution as a Nuisance Parameter
• A Redefinition of the Halo Boundary Leads to a Simple yet Accurate Halo Model of Large Scale Structure
• A local bias approach to the clustering of discrete density peaks
• Constraints on the Clustering, Biasing and Redshift Distribution of Radio Sources
• Sub-Megaparsec Individual Photometric Redshift Estimation from Cosmic Web Constraints
• On the CGM Fundamental Plane: The Halo Mass Dependency of Circumgalactic HI
• From Snakes to Stars, the Statistics of Collapsed Objects - II. Testing a Generic Scaling Ansatz for Hierarchical Clustering
• On the Spatial Correlations of Lyman Break Galaxies
• Mapping the real space distributions of galaxies in SDSS DR7: I. Two Point Correlation Functions
• The Conditional Colour-Magnitude Distribution: I. A Comprehensive Model of the Colour-Magnitude-Halo Mass Distribution of Present-Day Galaxies
• Dependence of halo bias on mass and environment
• CFHTLenS: A Weak Lensing Shear Analysis of the 3D-Matched-Filter Galaxy Clusters
• A Study of High-Order Non-Gaussianity with Applications to Massive Clusters and Large Voids
• Does Concentration Drive the Scatter in the Stellar-to-Halo Mass Relation of Galaxy Clusters?
• An accurate perturbative approach to redshift space clustering of biased tracers in modified gravity
• Probing Galaxy Assembly Bias in BOSS Galaxies Using Void Probabilities
• On the reliability of merger-trees and the mass growth histories of dark matter haloes
• nIFTy Cosmology: the clustering consistency of galaxy formation models
• Imprint of anisotropic primordial non-Gaussianity on halo intrinsic alignments in simulations
• Lensing Studies with Diffuse Backgrounds
• Excursion set theory for modified gravity: correlated steps, mass functions and halo bias
• How the dark matter halos cluster in Lagrangian space
• Void Galaxies Follow a Distinct Evolutionary Path in the Environmental COntext Catalog
• Gravitational waves $\times$ HI intensity mapping: cosmological and astrophysical applications
• Optimal Weighting Scheme in Redshift-space Power Spectrum Analysis and a Prospect for Measuring the Cosmic Equation of State
• Self-calibration of weak lensing systematic effects using combined two- and three-point statistics
• Modeling peculiar velocities of dark matter halos
• High-precision multi-band measurements of the angular clustering of X-ray sources
• ELUCID. VI: Cosmic variance of galaxy distribution in the local Universe
• Zipf's Law from Scale-free Geometry
• Galaxy assembly bias of central galaxies in the Illustris simulation
• From Snakes to Stars, the Statistics of Collapsed Objects - I. Lower--order Clustering Properties
• Peak exclusion, stochasticity and convergence of perturbative bias expansions in 1+1 gravity
• The clustering of galaxies around three damped Ly-alpha absorbers at Redshift Three
• Predicting the Clustering of X-Ray Selected Galaxy Clusters in Flux-Limited Surveys
• Spatially Extended 21 cm Signal from Strongly Clustered UV and X-Ray Sources in the Early Universe
• What will anisotropies in the clustering pattern in redshifted 21 cm maps tell us?
• The VIMOS Ultra Deep Survey. Luminosity and stellar mass dependence of galaxy clustering at z~3
• Comparing halo bias from abundance and clustering
• Projected-Field Kinetic Sunyaev-Zel'dovich Cross-Correlations: Halo Model and Forecasts
• Cosmological Three-Point Function: Testing The Halo Model Against Simulations
• Clustering and Bias Measurements of SDSS Voids
• Probing the existence of a rich galaxy overdensity at z=5.2
• Confusion noise at far-IR to millimeter wavelengths
• Robust PCA and MIC statistics of baryons in early mini-haloes
• The DESI $N$-body Simulation Project I: Testing the Robustness of Simulations for the DESI Dark Time Survey
• Small-scale galaxy clustering in the EAGLE simulation
• Galaxy clustering and projected density profiles as traced by satellites in photometric surveys: Methodology and luminosity dependence
• Effects of large-scale environment on the assembly history of central galaxies
• The ROSAT-ESO Flux-Limited X-Ray (REFLEX) Galaxy Cluster Survey VI: Constraints on the cosmic matter density from the KL power spectrum
• Cosmology with Galaxy Clusters in the XMM Large-Scale Structure Survey
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): Reconstruction of the redshift-space galaxy density field
• Quasi Non-linear Evolution of Stochastic Bias
• How to Optimally Constrain Galaxy Assembly Bias: Supplement Projected Correlation Functions with Count-in-cells Statistics
• Luminosity Dependent X-ray AGN Clustering ?
• Calibrating the Galaxy Halo - Black Hole Relation Based on the Clustering of Quasars
• Non-local bias in the halo bispectrum with primordial non-Gaussianity
• Dependence of Halo Bias and Kinematics on Assembly Variables
• Cross-Correlation Studies between CMB Temperature Anisotropies and 21 cm Fluctuations
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): ${\Omega }_{{\mathrm{m}}_0}$ from the galaxy clustering ratio measured at $z\sim 1$
• Intrinsic/Extrinsic Density-Ellipticity Correlations and Galaxy-Galaxy Lensing
• The Halo Mass-Bias Redshift Evolution in the $\Lambda$CDM Cosmology
• Reionization and the large-scale 21 cm-cosmic microwave background cross correlation
• Cluster correlations in redshift space
• Galaxy Clustering and Dark Energy
• On the Average Comoving Number Density of Halos
• Feedback from Clustered Sources During Reionization
• Cosmological constraints from abundance, weak-lensing and clustering of galaxy clusters: application to the SDSS
• AMICO galaxy clusters in KiDS-DR3: cosmological constraints from large-scale stacked weak lensing profiles
• Revealing the cosmic web dependent halo bias
• What determines large scale galaxy clustering: halo mass or local density?
• The PEP survey: clustering of infrared-selected galaxies and structure formation at z~2 in the GOODS South
• The mass-concentration relationship of virialized halos and its impact on cosmological observables
• Reionization Bias in High Redshift Quasar Near-Zones
• Non-Gravitational Contributions to the Clustering of Ly-alpha Selected Galaxies: Implications for Cosmological Surveys
• The ISW-tSZ cross correlation: ISW extraction out of pure CMB data
• A Flexible Analytic Model of Cosmic Variance in the First Billion Years
• Mass functions and bias of dark matter halos
• Nonlinearity and stochasticity in the density--velocity relation
• The 2QDES Pilot : The luminosity and redshift dependence of quasar clustering
• Cosmological Structure Formation in Decaying Dark Matter Models
• Evolution in the bias of faint radio sources to z ~ 2.2
• Candidate Clusters of Galaxies at $z>1.3$ Identified in the Spitzer SPT Deep Field Survey
• Probing dark energy with future redshift surveys: A comparison of emission line and broad band selection in the near infrared
• Modeling the clustering of dark-matter haloes in resummed perturbation theories
• An improved model of HII bubbles during the epoch of reionization
• Halo assembly bias from Separate Universe simulations
• AGN environments at z<1.5 in the UKIDSS Ultra-Deep Survey
• The cosmological dependence of halo and galaxy assembly bias
• Remapping dark matter halo catalogues between cosmological simulations
• Clustering of dark matter halos on the light-cone: scale-, time- and mass-dependence of the halo biasing in the Hubble volume simulations
• The influence of halo assembly on galaxies and galaxy groups
• Scale Radii and Aggregation Histories of Dark Haloes
• The importance of galaxy formation histories in models of reionization
• Effects of superstructure environment on galaxy groups
• One- and Two-point Source Statistics from the LOFAR Two-metre Sky Survey First Data Release
• Clustering of Lyman-alpha Emitters Around Quasars at $z\sim 4$
• A Comparison of The PSCz and Stromlo-APM Redshift Surveys
• Local and global environmental effects on galaxies and active galactic nuclei
• The Angular Three-Point Correlation Function in the Quasilinear Regime
• Multi-wavelength properties of radio and machine-learning identified counterparts to submillimeter sources in S2COSMOS
• The Gigaparsec WiggleZ Simulations: Characterising scale dependant bias and associated systematics in growth of structure measurements
• Self-consistency of the Excursion Set Approach
• Constraining cosmological parameters with the clustering properties of galaxy clusters in optical and X-ray bands
• Halo Sampling, Local Bias and Loop Corrections
• Scale-Dependent Bias of Galaxies from Baryonic Acoustic Oscillations
• ALMA reveals large overdensity and strong clustering of galaxies in quasar environments at $z\sim 4$
• Exploring the cosmological synergy between galaxy cluster and cosmic void number counts
• Light-cone effect on higher-order clustering in redshift surveys
• The binary-host connection: astrophysics of gravitational wave binaries from their host galaxy properties
• Measuring the evolution of intergalactic gas from z=0 to 5 using the kinematic Sunyaev-Zel'dovich effect
• The halo bias inside cosmic voids
• What Can the Distribution of Intergalactic Metals Tell us About the History of Cosmological Enrichment?
• Clustering with JWST: Constraining Galaxy Host Halo Masses, Satellite Quenching Efficiencies, and Merger Rates at z=4-10
• Testing the Halo Model Against the SDSS Photometric Survey
• Large Scale Anisotropic Bias from Primordial non-Gaussianity
• Anisotropic halo assembly bias and redshift-space distortions
• A Fundamental Line for Elliptical Galaxies
• Reionization in the Warm Dark Matter Model
• "Little red dots" cannot reside in the same dark matter halos as comparably luminous unobscured quasars
• An improved limit on the neutrino mass with CMB and redshift-dependent halo bias-mass relations from SDSS, DEEP2, and Lyman-Break Galaxies
• Masses of high-z galaxy hosting haloes from angular clustering and their evolution in the CDM model
• How Density Environment Changes the Influence of the Dark Matter-Baryon Streaming Velocity on the Cosmological Structure Formation
• Conditional Probabilities in the Excursion Set Theory. Generic Barriers and non-Gaussian Initial Conditions
• Halos and voids in a multifractal model of cosmic structure
• The unusual smoothness of the extragalactic unresolved radio background
• Spectroscopic Confirmation of two Extremely Massive Protoclusters BOSS1244 and BOSS1542 at $z=2.24$
• A unified model for the clustering of quasars and galaxies at $z\approx 6$
• Statistics of Dark Matter Halos from the Excursion Set Approach
• The correlation function of X-ray galaxy clusters in the RASS1 Bright Sample
• Power Spectrum Normalisation and the Non-Gaussian Halo Model
• Non-local bias contribution to third-order galaxy correlations
• Neural physical engines for inferring the halo mass distribution function
• Probing the first galaxies with the SKA
• Galaxy Clustering Evolution in the UH8K Weak Lensing Fields
• Cosmological Constraints with Clustering-Based Redshifts
• The clustering of the first galaxy halos
• Understanding the non-linear clustering of high redshift galaxies
• The probability distribution function of the SZ power spectrum: an analytical approach
• The Optical Luminosity Function of Virialized Systems
• Lyman-Break Galaxies at $z\sim 3$ in the Subaru Deep Field: Luminosity Function, Clustering and [OIII] Emission
• Relativistic effects and primordial non-Gaussianity in the galaxy bias
• Pair Correlations and Merger Bias
• Primordial non-Gaussianity in the bispectra of large-scale structure
• The clustering of submillimeter galaxies detected with ALMA
• A question of separation: disentangling tracer bias and gravitational nonlinearity with counts-in-cells statistics
• DM haloes in the fifth-force cosmology
• The zCOSMOS-Bright survey: the clustering of early and late galaxy morphological types since z~1
• On Correlated Random Walks and 21-cm Fluctuations During Cosmic Reionization
• From starburst to quiescence: post-starburst galaxies and their large-scale clustering over cosmic time
• Convolution Lagrangian perturbation theory for biased tracers beyond general relativity
• Removing the giants and learning from the crowd: a new SZ power spectrum method and revised Compton $y$-map analysis
• K-mouflage effects on clusters of galaxies
• Gravitational wave astronomy with radio galaxy surveys
• Cosmological constraints from the observed angular cross-power spectrum between Sunyaev-Zel'dovich and X-ray surveys
• Galaxy Bias in Quintessence Cosmological Models
• Modeling the QSO luminosity and spatial clustering at low redshifts
• Exploring Galaxy Formation Models and Cosmologies with Galaxy Clustering
• The large scale clustering of radio sources
• Identifying galaxy groups at high redshift from incomplete spectroscopic data: I. The group finder and application to zCOSMOS
• Clustering and lifetime of Lyman Alpha Emitters in the Epoch of Reionization
• SDSS-IV MaNGA: Signatures of halo assembly in kinematically misaligned galaxies
• The Host Haloes of Lyman Break Galaxies and Sub-millimeter Sources
• Quasar-Galaxy Clustering through Projected Galaxy Counts at z=0.6-1.2
• Clustering of Intermediate Luminosity X-ray selected AGN at z~3
• The nature of the relative bias between galaxies of different spectral type in 2dFGRS
• Spatial Clustering of High Redshift Lyman Break Galaxies
• From linear to non-linear scales: analytical and numerical predictions for the weak lensing convergence
• The hybrid SZ power spectrum: Combining cluster counts and SZ fluctuations to probe gas physics
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• The Subaru/XMM-Newton Deep Survey (SXDS) -VII. Clustering Segregation with Ultraviolet and Optical Luminosities of Lyman-Break Galaxies at z~3
• The clustering of H$\beta$+[OIII] and [OII] emitters since $z\sim 5$: dependencies with line luminosity and stellar mass
• Hosts and triggers of AGNs in the Local Universe
• Error Estimates for Measurements of Cosmic Shear
• Clustering at high redshift: The connection between Lyman Alpha emitters and Lyman break galaxies
• Detecting Reionization in the Star Formation Histories of High-Redshift Galaxies
• Star-galaxy separation in the AKARI NEP Deep Field
• Evolution of the Cluster Mass and Correlation Functions in LCDM Cosmology
• The WIRCam Deep Survey II: Mass Selected Clustering
• The universal multiplicity function: counting halos and voids
• Halo based reconstruction of the cosmic mass density field
• A study on the statistical significance of mutual information between morphology of a galaxy and its large-scale environment
• The Effect of Local non-Gaussianity on the Matter Bispectrum at Small Scales
• The cosmological light-cone effect on the power spectrum of galaxies and quasars in wide-field redshift surveys
• Evolution of hierarchical clustering in the CFHTLS-Wide since z~1
• Evidence for Merger-Driven Activity in the Clustering of High Redshift Quasars
• It takes two to know one: Computing accurate one-point PDF covariances from effective two-point PDF models
• Nonlinear Stochastic Biasing of Peaks and Halos: Scale-Dependence, Time-Evolution, and Redshift-Space Distortion from Cosmological N-body Simulations
• A Direct Measurement of the Mean Occupation Function of Quasars: Breaking Degeneracies between Halo Occupation Distribution Models
• Euclid preparation. XLI. Galaxy power spectrum modelling in real space
• What do cluster counts really tell us about the Universe?
• Probing massive neutrinos with the Minkowski functionals of large-scale structure
• The clustering of $z>7$ galaxies: Predictions from the BLUETIDES simulation
• Dark matter halo occupation: environment and clustering
• Constraints on Primordial non-Gaussianity from Future HI Intensity Mapping Experiments
• The Thermal Sunyaev-Zel'dovich Effect from Massive, Quiescent 0.5 $\le$ z $\le$ 1.5 Galaxies
• On the peculiar momentum of baryons after Reionization
• Testing one-loop galaxy bias: cosmological constraints from the power spectrum
• The nonlinear biasing of the 10k zCOSMOS galaxies up to z~1
• Where can we really find the First Stars' Remnants today?
• 21 cm Angular Power Spectrum from Minihalos as a Probe of Primordial Spectral Runnings
• Subhaloes gone Notts: the clustering properties of subhaloes
• AMICO galaxy clusters in KiDS-DR3: Measurement of the halo bias and power spectrum normalization from a stacked weak lensing analysis
• Quintessential Scale Dependence from Separate Universe Simulations
• The ALHAMBRA survey : $B-$band luminosity function of quiescent and star-forming galaxies at $0.2\le z<1$ by PDF analysis
• Patchy blazar heating: diversifying the thermal history of the intergalactic medium
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• The importance of stochasticity in determining galaxy emissivities and UV LFs during cosmic dawn and reionization
• Non-Gaussianity and Excursion Set Theory: Halo Bias
• Multiwavelength cluster mass estimates and machine learning
• Imprint of Inhomogeneous Reionization on the Power Spectrum of Galaxy Surveys at High Redshifts
• Halo Assembly Bias in the Quasi-linear Regime
• Luminosity bias: from haloes to galaxies
• The Clustering of Hot and Cold IRAS Galaxies: The Redshift Space Correlation Function
• Stochastic bias in multi-dimensional excursion set approaches
• Fossil Ionized Bubbles Around Dead Quasars During Reionization
• The Density Contrast of the Shapley Supercluster
• Dense Regions in Supersonic Isothermal Turbulence
• The Effect of Radiative Cooling on the Sunyaev-Zel'dovich Cluster Counts and Angular Power Spectrum: Analytic Treatment
• Stochastic Biasing and Weakly Non-linear Evolution of Power Spectrum
• Verifying the Identity of High-Redshift Massive Galaxies Through the Clustering of Lower Mass Galaxies Around Them
• Double Distribution of Dark Matter Halos with respect to Mass and Local Overdensity
• Optimal Transport Reconstruction of Baryon Acoustic Oscillations
• On the equivalence between the effective cosmology and excursion set treatments of environment
• The Herschel-PEP survey: evidence for downsizing in the hosts of dusty star-forming systems
• Clustering of Ly-alpha emitters around luminous quasars at z = 2-3: an alternative probe of reionization on galaxy formation
• Impacts of biasing schemes in the one-loop integrated perturbation theory
• The clustering of dark matter halos: scale-dependent bias on quasi-linear scales
• The 21cm radiation from minihalos as a probe of small primordial non-Gaussianity
• Detection and Fundamental Applications of Individual First Galaxies
• The scale-dependent signature of primordial non-Gaussianity in the large-scale structure of cosmic reionization
• A new method to measure galaxy bias by combining the density and weak lensing fields
• Perturbation theory for nonlinear halo power spectrum: the renormalized bias and halo bias
• Halo bias in the excursion set approach with correlated steps
• Probing cosmology and gastrophysics with fast radio bursts: Cross-correlations of dark matter haloes and cosmic dispersion measures
• First Structure Formation under the Influence of Gas-Dark Matter Streaming Velocity and Density: Impact of the Baryons-trace-dark matter Approximation
• The cosmic web connection to the dark matter halo distribution through gravity
• The Halo Occupation Distribution of Obscured Quasars: Revisiting the Unification Model
• Two-point correlation functions of X-ray selected clusters of galaxies: theoretical predictions for flux-limited surveys
• A Method to Measure the Mass of Damped Ly-alpha Absorber Host Galaxies Using Fluctuations in 21cm Emission
• Renormalisation of linear halo bias in N-body simulations
• Constraining isocurvature perturbations with the 21cm emission from minihaloes
• Gravitational Magnification of Pop III Supernovae in Hierarchical Cosmological Models: NGST Perspectives
• The halo mass function conditioned on density from the Millennium Simulation: insights into missing baryons and galaxy mass functions
• Modelling the dusty universe II: The clustering of submillimetre-selected galaxies
• The dearth of difference between central and satellite galaxies II. Comparison of observations with L-GALAXIES and EAGLE in star formation quenching
• Finding closure: approximating Vlasov-Poisson using finitely generated cumulants
• The COSMOS Density Field: A Reconstruction Using Both Weak Lensing and Galaxy Distributions
• Clustering of SZ clusters on a past light-cone: acoustic oscillations and constraints on dark energy
• Modification of the 21-cm power spectrum by X-rays during the epoch of reionisation
• Measuring Linear and Non-linear Galaxy Bias Using Counts-in-Cells in the Dark Energy Survey Science Verification Data
• Cross-correlation studies as a probe of reionization physics
• Generating mock galaxy catalogues for flux-limited samples like the DESI Bright Galaxy Survey
• Dissect two-halo galactic conformity effect for central galaxies: The dependence of star formation activities on the large-scale environment
• Mass Selection Bias in Galaxy Cluster Peculiar Velocities from the Kinetic Sunyaev-Zel'dovich Effect
• Keck Deep Fields. IV. Luminosity Dependent Clustering and Galaxy Downsizing in UV-Selected Galaxies at z=4, 3, and 2
• Genus statistics for galaxy clusters and nonlinear biasing of dark matter halos
• The abundance of dark matter haloes down to Earth mass
• Virialization of Galaxy Clusters and Beyond
• Cross-correlation of CFHTLenS galaxy catalogue and Planck CMB lensing using the halo model prescription
• The fractal distribution of haloes
• Statistical properties of the linear tidal shear
• Sunyaev-Zel'dovich Cluster Survey Simulations for Planck
• Galaxy clustering at cosmic dawn from JWST/NIRCam observations to redshift z$\sim$11
• Dependence of galaxy clustering on UV-luminosity and stellar mass at $z\sim 4-7$
• The contribution of the IGM and minihalos to the 21 cm signal of reionization
• Modelling the shapes of the largest gravitationally bound objects
• Predictions of Quasar Clustering: Redshift, Luminosity and Selection Dependence
• Halo concentrations from extended Press-Schechter merger histories
• Towards optimal estimation of the galaxy power spectrum
• Late Bloomer Galaxies: Growing Up in Cosmic Autumn
• Large-scale bias of dark matter halos
• Cosmological constrains from X-ray AGN clustering and SNIa data
• Constraints on $f(R)$ and nDGP Modified Gravity Model Parameters with Cluster Abundances and Galaxy Clustering
• Predicting the CIB-$\varphi$ contamination in the cross-correlation of the tSZ effect and $\varphi$
• A Consistent Comparison of Bias Models using Observational Data
• Testing gravity with gravitational waves $\times$ electromagnetic probes cross-correlations
• Cosmic dichotomy in the hosts of rapidly star-forming systems at low and high redshifts
• Measurement of Void Bias Using Separate Universe Simulations
• Clustering of Extremely Red Objects in Elais-N1 from the UKIDSS DXS with optical photometry from Pan-STARRS1 and Subaru
• Measuring the luminosity and virial black hole mass dependence of quasar-galaxy clustering at z ~ 0.8
• The Integrated Bispectrum in Modified Gravity Theories
• Do galaxy mergers prefer under-dense environments?
• Close Pairs as Proxies for Galaxy Cluster Mergers
• Modification of the 21-cm power spectrum by quasars during the epoch of reionisation
• Euclid preparation. The Cosmic Dawn Survey (DAWN) of the Euclid Deep and Auxiliary Fields
• Halo assembly bias from a deep learning model of halo formation
• Two-point correlation function of high-redshift objects on a light-cone: Effect of the linear redshift-space distortion
• 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
• Small-scale clustering of Primordial Black Holes: cloud-in-cloud and exclusion effects
• A Halo Model with Environment Dependence: Theoretical Considerations
• A group-galaxy cross-correlation function analysis in zCOSMOS
• Impact of early dark energy on the Planck SZ cluster sample
• High-redshift voids in the excursion set formalism
• Constraining the CDM spectrum normalization in flat dark energy cosmologies
• Proto-clusters in the Lambda CDM Universe
• Tomography of the Reionization Epoch with Multifrequency CMB Observations
• Separate Universe calibration of the dependence of halo bias on cosmic web anisotropy
• The Cosmic Large-Scale Structure in X-rays (CLASSIX) cluster survey IV: Superclusters in the local Universe at z <= 0.03
• Galaxy clustering measurements out to redshift z$\sim$8 from Hubble Legacy Fields
• Towards 1% accurate galaxy cluster masses: Including baryons in weak-lensing mass inference
• The clustering and halo occupation distribution of Lyman-break galaxies at $z\sim 4$
• An analytical model of the large neutral regions during the late stage of reionization
• Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model. II. The colour-density relation up to z=1.5
• Early Science Result from the Japanese Virtual Observatory: AGN and Galaxy Clustering at z = 0.3 to 3.0
• The effect of Galactic foreground subtraction on redshifted 21-cm observations of quasar HII regions
• The Imprint of Cosmic Reionization on Galaxy Clustering
• Time evolution of the stochastic linear bias of interacting galaxies on linear scales
• Evolution of the Cluster Correlation Function
• On the Angular Correlation Function of SZ Clusters : Extracting cosmological information from a 2D catalog
• Optical identifications of $\sim 4000$ radio sources at the 1 mJy level
• $\alpha$-attractor dark energy in view of next-generation cosmological surveys
• The Morphology of the Thermal Sunyaev-Zel'dovich Sky
• AMICO galaxy clusters in KiDS-DR3: Cosmological constraints from angular power spectrum and correlation function
• Toward an Improved Analytical Description of Lagrangian Bias
• Testing the conditional mass function of dark matter halos against numerical N-body simulations
• Redshift Evolution of the Nonlinear Two-Point Correlation Function
• PhotoWeb redshift: boosting photometric redshift accuracy with large spectroscopic surveys
• Cosmic Statistics through Weak Lenses
• A prescription for the conditional mass function of dark matter haloes
• How is the local-scale gravitational instability influenced by the surrounding large-scale structure formation?
• Integrated perturbation theory for cosmological tensor fields. I. Basic formulation
• Lyman-alpha Emitters in Ionized Bubbles: Constraining the Environment and Ionized Fraction
• The impact of environment on the dynamical structure of satellite systems
• The Power Spectrum, Bias Evolution, and the Spatial Three-Point Correlation Function
• Clustering of CODEX clusters
• KiDS+VIKING+GAMA: Halo occupation distributions and correlations of satellite numbers with a new halo model of the galaxy-matter bispectrum for galaxy-galaxy-galaxy lensing
• The generalized evolution of linear bias: a tool to test gravity
• Detecting ultra-high energy cosmic ray anisotropies through cross-correlations
• Lagrangian bias in the local bias model
• The bias of weighted dark matter halos from peak theory
• CMBR Weak Lensing and HI 21-cm Cross-correlation Angular Power Spectrum
• The redshift evolution of bias and baryonic matter distribution
• The ALHAMBRA survey : Estimation of the clustering signal encoded in the cosmic variance
• 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
• A galaxy-halo model of large-scale structure
• 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
• Modelling the stochasticity of high-redshift halo bias
• Dark Matter annihilation energy output and its effects on the high-z IGM
• The Tessellation-Level-Tree: characterising the nested hierarchy of density peaks and their spatial distribution in cosmological N-body simulations
• Dark-ages reionization and galaxy formation simulation XI: Clustering and halo masses of high redshift galaxies
• Late-formed halos prefer to host quiescent central galaxies. I. Observational results
• Evolution of the cosmological mass function in a moving barrier model
• Cosmology from LOFAR Two-metre Sky Survey Data Release 2: Cross-correlation with the cosmic microwave background
• Numerical Simulation of Non-Gaussian Random Fields with Prescribed Marginal Distributions and Cross-Correlation Structure II: Multivariate Random Fields
• Alternative High-z Cosmic Tracers and the Dark Energy Equation of State
• Cosmology with Galaxy Clusters: Systematic Effects in the Halo Mass Function
• Predicting the clustering properties of galaxy clusters detectable for the Planck satellite
• Probing Hot Gas in Galaxy Groups through the Sunyaev-Zeldovich Effect
• Light-Cone Distortion of the Clustering and Abundance of Massive Galaxies at High-Redshifts
• The effect of cluster magnetic field on the Sunyaev Zeldovich power spectrum
• Bias and Conditional Mass Function of Dark Halos Based on the Nonspherical Collapse Model
• A Stochastic Theory of the Hierarchical Clustering I. Halo Mass Function
• The mass and temperature functions in a moving barrier model
• Painting baryons onto N-body simulations of galaxy clusters with image-to-image deep learning
• Testing General Relativity Using the Evolution of Linear Bias
• Galaxy power spectrum and biasing results from the LOFAR Two-metre Sky Survey (first data release)
• The Power Spectrum of Clusters of Galaxies and the Press-Schechter Approximation
• $\text{PineTree}$: A generative, fast, and differentiable halo model for wide-field galaxy surveys
• Predicting the peculiar velocities of nearby PSC-z galaxies using the Least Action Principle
• The Ultramarine Simulation: properties of dark matter haloes before redshift 5.5
• Scale Dependence of the Halo Bias in General Local-Type Non-Gaussian Models I: Analytical Predictions and Consistency Relations
• The 21cm Power Spectrum and the Shapes of Non-Gaussianity
• What can the spatial distribution of galaxy clusters tell about their scaling relations?
• An Introduction into the Theory of Cosmological Structure Formation
• Statistics of Dark Matter Halos in the Excursion Set Peak Framework
• Fingerprints of Anomalous Primordial Universe on the Abundance of Large Scale Structures
• Clustering of the AKARI NEP Deep Field 24 $\mu$m selected galaxies
• Recovering the Tidal Field in the Projected Galaxy Distribution
• Modeling the cross power spectrum of Sunyaev-Zel'dovich and X-ray surveys
• BASILISK: Bayesian Hierarchical Inference of the Galaxy-Halo Connection using Satellite Kinematics--I. Method and Validation
• Shot noise in multi-tracer constraints on $f_{\text{NL}}$ and relativistic projections: Power Spectrum
• Measuring Feedback Using the Intergalactic Medium State and Evolution Inferred from the Soft X-ray Background
• How to empirically model star formation in dark matter halos: I. Inferences about central galaxies from numerical simulations
• Galaxy and Mass Assembly (GAMA): Tracing galaxy environment using the marked correlation function
• Power spectrum of density fluctuations, halo abundances and clustering with primordial black holes
• Angular clustering of z~2 star-forming and passive galaxies in 2.5 square degrees of deep CFHT imaging
• Simultaneous effect of Modified Gravity and Primordial Non-Gaussianity in Large Scale Structure Observations
• Nonlinearities in modified gravity cosmology. II. Impacts of modified gravity on the halo properties
• On the origin of red spirals: Does assembly bias play a role?
• A Possible Bias Model for Quasars
• Galaxy and Mass Assembly (GAMA): the clustering of galaxy groups
• Non-perturbative halo clustering from cosmological density peaks
• A Framework for Simultaneously Measuring Field Densities and the High-z Luminosity Function
• Numerical action reconstruction of the dynamical history of dark matter haloes in N-body simulations
• The very wide-field $gzK$ galaxy survey -- II. The relationship between star-forming galaxies at $z\sim 2$ and their host haloes based upon HOD modelling
• A potentially pure test of cosmic geometry: galaxy clusters and the real space Alcock-Paczynski test
• Choose to smooth: Gaussian streaming with the truncated Zel'dovich approximation
• Biasing and Genus Statistics of Dark Matter Halos in the Hubble Volume Simulation
• The Impact of HI in Galaxies on 21-cm Intensity Fluctuations During the Reionisation Epoch
• Small-scale clumping of dark matter and the mean free path of ionizing photons at $z=6$
• Modified initial power spectrum and too big to fail problem
• Probing axion dark matter with 21cm fluctuations from minihalos
• Anisotropies in Cosmological 21 cm Background by Oscillons/I-balls of Ultra-light Axion-like Particle
• Galaxy assembly bias in the stellar-to-halo mass relation for red central galaxies from SDSS
• Cosmic shear statistics in cosmologies with non-Gaussian initial conditions
• Merging History Trees for Dark Matter Halos: Tests of the Merging Cell Model in a CDM Cosmology
• Primordial density perturbations with running spectral index: impact on non-linear cosmic structures
• Consistency relations for the Lagrangian halo bias and their implications
• Evidence of Turbulence-like Universality on the Formation of Galaxy-sized Dark Matter Haloes
• Stochastic Model of the Spin Distribution of Dark Matter Halos
• The feasibility of constraining DM interactions with high-redshift observations by JWST
• Observational determination of the galaxy bias from cosmic variance with a random pointing survey: Clustering of z~2 galaxies from Hubble's BoRG survey
• Halo mass function in scale invariant models
• Galaxy Formation by Galactic Magnetic Fields
• A forecast for the detection of the power asymmetry from galaxy surveys
• Multi-wavelength consensus of large-scale linear bias
• The effects of anti-correlation on gravitational clustering
• Probing Reionization-Era Galaxies with JWST UV Luminosity Functions and Large-Scale Clustering
• LARgE Survey -- II. The Dark Matter Halos and the Progenitors and Descendants of Ultra-Massive Passive Galaxies at Cosmic Noon
• A Stochastic Theory of the Hierarchical Clustering II. Halo progenitor mass function and large-scale bias
• The fractional Brownian motion and the halo mass function
• X-ray cluster cosmology
• COMBO-17 measurements of the effect of environment on the type-dependent galaxy luminosity function
• Testing the Large-Scale Environments of Cool-core and Noncool-core Clusters with Clustering Bias
• The Correlation Between Star Formation and 21cm Emission During the Reionization Epoch
• Clustering Properties of Low-Luminosity Star-Forming galaxies at z = 0.24 and 0.40 in the Subaru Deep Field
• Statistically significant length scale of filaments as a robust measure of galaxy distribution
• Toward optimal cluster power spectrum analysis
• Smooth halos in the cosmic web
• Galaxy clustering using photometric redshifts
• Autocorrelation function of the soft X-ray background produced by warm-hot gas in dark halos
• Tidal shear and the consistency of microscopic Lagrangian halo approaches
• Velocity bias and the nonlinear perturbation theory of peaks
• ScamPy -- A sub-halo clustering & abundance matching based Python interface for painting galaxies on the dark matter halo/sub-halo hierarchy
• How are Lyman $\alpha$ absorbers in the cosmic web related to gas-rich galaxies?
• Constraints on Cosmological and Biasing models using AGN clustering
• Constraining cosmological parameters using void statistics from the SDSS survey
• Exploring the physical origins of halo assembly bias from early times
• New insight into the variability of the Be star $\pi$ Aquarii: Determination of stellar and disk parameters
• Galaxy Clustering at z~3
• The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
• Fast Simulation of Cosmological Neutral Hydrogen based on the Halo Model
• Environmental effects on halo abundance and weak lensing peak statistics toward large underdense regions
• Non-Gaussian assembly bias from a semi-analytic galaxy formation model
• Characterizing the assembly of dark matter halos with protohalo size histories: I. Redshift evolution, relation to descendant halos, and halo assembly bias
• HD 42659: The only known roAp star in a spectroscopic binary observed with B photometry, TESS and SALT
• Covariances of density probability distribution functions. Lessons from hierarchical models
• Evolution of matter and galaxy clustering in cosmological hydrodynamical simulations
• Forecasts for Warm Dark Matter from Photometric Galaxy Surveys
• Probing cosmology via the clustering of critical points
• Evaluating the origins of the secondary bias based on the correlation of halo properties with the linear density field
• Unexpected clustering pattern in dwarf galaxies challenges formation models
• The galaxy bias profile of cosmic voids
• Weak lensing of the Sunyaev-Zel'dovich sky
• Incompatibility of Standard Galaxy Bias Models in General Relativity
• Accurate halo mass functions from the simplest excursion set theory
• The SRG/eROSITA All-Sky Survey: Exploring halo assembly bias with X-ray selected superclusters
• Galaxy and Mass Assembly (GAMA): Mid-infrared properties as tracers of galaxy environment
• How do uncertainties in galaxy formation physics impact field-level galaxy bias?
• Prospects for measuring neutrino mass with 21-cm forest
• A fully Lagrangian, non-parametric bias model for dark-matter halos
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• Massive Black Hole Mergers
• Testing Theoretical Models for the Higher-Order Moments of Dark Halo Distribution
• The Impact of Baryons on the Large-Scale Structure of the Universe
• Evolution of the real-space correlation function from next generation cluster surveys
• Ultraviolet background fluctuations with clustered sources
• Scaling of the 1-halo terms with bias
• Mass-Dependent Baryon Acoustic Oscillation Signal and Halo Bias
• Probing the bias of radio sources at high redshift
• Bayesian analysis of cosmic structures
• Evolution of Power Spectrum in Non-Gaussian Models
• The north-south asymmetry of the ALFALFA HI velocity width function
• Pulsar B1237+25 Aberration/Retardation Analysis from Decimeter to Decameter Wavelength: Challenge to "Radius-to-Frequency Mapping"
• BASILISK II. Improved Constraints on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• Spatial Correlation of Massive Black Hole Mergers: Probing the Formation Mechanism and Reionization
• On the Physical Nature of Ly$\alpha$ Transmission Spikes in High Redshift Quasar Spectra
• Simulating the epoch of Helium Reionization in photon-conserving semi-numerical code SCRIPT
• CLIMBER: Galaxy-Halo Connection Constraints from Next-Generation Surveys
• A Stochastic Theory of the Hierarchical Clustering III. The Non-universality and Non-stationarity of the Halo Mass Function
• Measuring the scatter of the mass-richness relation in galaxy clusters in photometric imaging surveys by means of their correlation function
• Approximate methods for the generation of dark matter halo catalogs in the age of precision cosmology
• Cosmological constraints from galaxy clustering
• Environmental history of filament galaxies: stellar mass assembly and star-formation of filament galaxies
• Improving photometric redshifts with Ly$\alpha$ tomography
• Evolution of Lyman Break Galaxies Beyond Redshift Four
• Symmetries, Invariants and Generating Functions: Higher-order Statistics of Biased Tracers
• The pair-wise velocity dispersion of galaxies: effects of non radial motions
• Cosmological parameters from Galaxy Clusters: an Introduction
• Isodensity Statistics on Clustering of High-z Objects in Cosmological Redshift-spaces
• Tracing the cosmological origin of gas that fuels in situ star formation in TNG50 galaxies
• The clustering properties of high-redshift passive galaxies
• The Reionization History in the Lognormal Model
• DESI Emission-line Galaxies: Clustering Dependence on Stellar Mass and [OII] Luminosity
• The imprints of massive neutrinos on the three-point correlation function of large-scale structures
• Breaking degeneracies with the Sunyaev-Zeldovich full bispectrum
• Toward accurate measurement of property-dependent galaxy clustering I. Comparison of the Vmax method and the "shuffled" method
• Comparison of the linear bias models in the light of the Dark Energy Survey
• Models for the Clustering of Far-Infrared and Sub-millimetre selected Galaxies
• On the spin distributions of $\Lambda$CDM haloes
• A halo model approach to describe clustering and emission of the two main star forming galaxy populations for Cosmic Infrared Background studies
• On the tomographic cluster clustering as a cosmological probe
• Luminosity Bias (II): The Cosmic Web of the First Stars
• Probabilistic Lagrangian bias estimators and the cumulant bias expansion
• Gaussian Lagrangian Galaxy Bias
• Accelerating HI density predictions during the Epoch of Reionization using a GPR-based emulator on N-body simulations
• Hosts and environments: a (large-scale) radio history of AGN and star-forming galaxies
• Predicting halo occupation and galaxy assembly bias with machine learning
• Non-parametric Lagrangian biasing from the insights of neural nets
• Cosmic magnification on high-redshift submillimeter galaxies
• The Mass Function of Dark Halos in Superclusters and Voids
• Towards an Observational Detection of Halo Spin Bias using Spin-Orbit Coherence
• Particle Physics in the Sky and Astrophysics Underground: Connecting the Universe's Largest and Smallest Scales
• A New Wavelet Scattering Transform-Based Statistic for Cosmological Analysis of Large-Scale Structure
• The same with less: The cosmic web of warm versus cold dark matter dwarf galaxies
• Individual halo bias in models of $f(R)$ gravity
• Analytical modeling of the one-dimensional power spectrum of 21-cm forest based on a halo model method
• Cross-correlating the EMU Pilot Survey 1 with CMB lensing: Constraints on cosmology and galaxy bias with harmonic-space power spectra
• Testing the thermal Sunyaev-Zel'dovich power spectrum of a halo model using hydrodynamical simulations
• The Origin of the Orbital Parameter Distribution of Merging Halos
• A data compression and optimal galaxy weights scheme for Dark Energy Spectroscopic Instrument and weak lensing datasets
• Layered dark structure with a Structuring Field: A $Z_4$-symmetric Inert Doublet-Singlet realization and implications for the $S_8$ tension
• Euclid preparation. L. Calibration of the linear halo bias in $\Lambda (\nu )$CDM cosmologies
• MIGHTEE: The dark matter haloes, duty cycle and mechanical feedback from radio-AGN up to $z\sim 2.5$
• Investigation of homogeneity and matter distribution on large scales using large quasar groups
• The spatial clustering of radio sources in NVSS and FIRST; implications for galaxy clustering evolution
• The eventful life journey of galaxy clusters. II. Impact of mass accretion on the thermodynamical structure of the ICM
• Kinematic effects of the velocity fluctuations for dark halos population in LCDM model
• A halo approach to the evaluation of the cross-correlation between the SZ sky and galaxy survey
• Recent Advances in Large-Scale Structure and Galaxy Formation Studies
• Hybrid $P_{\ell }(k)$: general, unified, non-linear matter power spectrum in redshift space
• Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy
• Cosmological free-free emission from dark matter halos in the $\Lambda$CDM model
• A Fast and Simple Algorithm for Detecting Large Scale Structures
• Lagrangian Perturbation Theory for Biased Tracers: Significance of the Number Conservation
• Cosmological parameters from the clustering of AGN
• Seeing Wiggles without Seeing Wiggles: BAO Recovery in 21 cm Intensity Mapping with Deep Learning
• Towards including super-sample covariance in the unbinned likelihood for cluster abundance cosmology
• Colour Dependence of the Distribution of IRAS Galaxies revealed by Multifractal Measures
• Cosmological constraints from clustering properties of galaxy clusters
• Analytical Approximations to Galaxy Clustering
• Non-Gaussianity in the Squeezed Three-Point Correlation from the Relativistic Effects
• Probing power spectrum enhancement at small scales with the SKA
• Luminosity Function of Galaxies in Voids: A Modification Inspired by Excursion Set Theory
• Contribution of Cross-Correlations to the 21cm Angular Power Spectrum in the Epoch of Reionization
• A redshift distortion free correlation function at third order in the nonlinear regime