The Halo Occupation Distribution: Towards an Empirical Determination of the Relation Between Galaxies and Mass

Abstract

We investigate galaxy bias in the framework of the ``Halo Occupation Distribution'' (HOD), which defines the bias of a population of galaxies by the conditional probability P(N|M) that a dark matter halo of virial mass M contains N galaxies, together with prescriptions that specify the relative spatial and velocity distributions of galaxies and dark matter within halos. By populating the halos of a cosmological N-body simulation using a variety of HOD models, we examine the sensitivity of different galaxy clustering statistics to properties of the HOD. The galaxy correlation function responds to different aspects of P(N|M) on different scales. Obtaining the observed power-law form of xi(r) requires rather specific combinations of HOD parameters, implying a strong constraint on the physics of galaxy formation; the success of numerical and semi-analytic models in reproducing this form is entirely non-trivial. Other clustering statistics such as the galaxy-mass correlation function, the bispectrum, the void probability function, the pairwise velocity dispersion, and the group multiplicity function are sensitive to different combinations of HOD parameters and thus provide complementary information about galaxy bias. We outline a strategy for determining the HOD empirically from redshift survey data. This method starts from an assumed cosmological model, but we argue that cosmological and HOD parameters will have non-degenerate effects on galaxy clustering, so that a substantially incorrect cosmological model will not reproduce the observations for any choice of HOD. Empirical determinations of the HOD as a function of galaxy type from the 2dF and SDSS redshift surveys will provide a detailed target for theories of galaxy formation, insight into the origin of galaxy properties, and sharper tests of cosmological models.

60 pages + 21 eps figures. Replaced with accepted ApJ version. Minor changes + added references

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• Weighing obscured and unobscured quasar hosts with the CMB
• Dark Matter Halo Models of Stellar Mass-Dependent Galaxy Clustering in PRIMUS+DEEP2 at 0.2<z<1.2
• Mapping the allowed parameter space for decaying dark matter models
• Fourier analysis of multi-tracer cosmological surveys
• The Small-scale Clustering of Luminous Red Galaxies via Cross-Correlation Techniques
• Clustering of quasars in the First Year of the SDSS-IV eBOSS survey: Interpretation and halo occupation distribution
• Clustering on very small scales from a large sample of confirmed quasar pairs: Does quasar clustering track from Mpc to kpc scales?
• Galaxy properties and the cosmic web in simulations
• Euclid. V. The Flagship galaxy mock catalogue: a comprehensive simulation for the Euclid mission
• The dark matter of galaxy voids
• The RESOLVE Survey Atomic Gas Census and Environmental Influences on Galaxy Gas Reservoirs
• Stellar Property Statistics of Massive Halos from Cosmological Hydrodynamics Simulations: Common Kernel Shapes
• What Do Dark Matter Properties Tell Us About Their Mass Assembly Histories?
• The Halo Occupation Distribution of Active Galactic Nuclei
• Beyond halo mass: quenching galaxy mass assembly at the edge of filaments
• Near-Infrared Properties of Moderate-Redshift Galaxy Clusters: Halo Occupation Number, Mass-to-Light Ratios and Omega_m
• The Luminosity, Colour and Morphology dependence of galaxy filaments in the Sloan Digital Sky Survey Data Release Four
• The evolution of the stellar mass versus halo mass relationship
• 3\%-accurate predictions for the clustering of dark matter, haloes and subhaloes, over a wide range of cosmologies and scales
• A Hybrid Deep Learning Approach to Cosmological Constraints From Galaxy Redshift Surveys
• A tale of two populations: the stellar mass of central and satellite galaxies
• The effects of assembly bias on cosmological inference from galaxy-galaxy lensing and galaxy clusters
• A highly obscured and strongly clustered galaxy population discovered with the Spitzer Space Telescope
• Flybys, orbits, splashback: subhalos and the importance of the halo boundary
• The MillenniumTNG Project: An improved two-halo model for the galaxy-halo connection of red and blue galaxies
• Illustrating galaxy-halo connection in the DESI era with IllustrisTNG
• The X-ray Properties of Optically-Selected Galaxy Clusters
• Dark Energy Survey Year 1 Results: galaxy mock catalogues for BAO
• Learning effective physical laws for generating cosmological hydrodynamics with Lagrangian Deep Learning
• GaBoDS: The Garching-Bonn Deep Survey: VII. Probing galaxy bias using weak gravitational lensing
• Regarding the Line-of-Sight Baryonic Acoustic Feature in the Sloan Digital Sky Survey and Baryon Oscillation Spectroscopic Survey Luminous Red Galaxy Samples
• ADDGALS: Simulated Sky Catalogs for Wide Field Galaxy Surveys
• New perspectives on the BOSS small-scale lensing discrepancy for the Planck $\Lambda$CDM Cosmology
• Aemulus $\nu$: Precise Predictions for Matter and Biased Tracer Power Spectra in the Presence of Neutrinos
• Constraining Satellite Galaxy Stellar Mass Loss and Predicting Intrahalo Light I: Framework and Results at Low Redshift
• The nature of assembly bias - III. Observational properties
• PRIMUS: One- and Two-Halo Galactic Conformity at $0.2<z<1$
• Marked clustering statistics in $f(R)$ gravity cosmologies
• The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for Galaxy Clustering Measurements
• Updated measurements of the dark matter halo masses of obscured quasars with improved WISE and Planck data
• Subhalo statistics of galactic halos: beyond the resolution limit
• The Q Continuum Simulation: Harnessing the Power of GPU Accelerated Supercomputers
• Large Scale Structure of the Universe
• The Halo Occupation Distribution of X-ray-Bright Active Galactic Nuclei: A Comparison with Luminous Quasars
• Exploring the halo occupation of AGN using dark-matter cosmological simulations
• The dependence of galaxy clustering on stellar mass, star-formation rate and redshift at z = 0.8-2.2, with HiZELS
• The dependence of the pairwise velocity dispersion on galaxy properties
• Perturbation theory for modeling galaxy bias: validation with simulations of the Dark Energy Survey
• Combining FOF and halo-based algorithms for the identification of galaxy groups
• The Incomplete Conditional Stellar Mass Function: Unveiling the Stellar Mass Functions of Galaxies at 0.1 < Z < 0.8 from BOSS Observations
• Differential Neutrino Condensation onto Cosmic Structure
• Measuring subhalo mass in redMaPPer clusters with CFHT Stripe 82 Survey
• Modeling the Very Small-Scale Clustering of Luminous Red Galaxies
• Halo abundances within the cosmic web
• The insignificant evolution of the richness-mass relation of galaxy clusters
• Cosmic Voids and Galaxy Bias in the Halo Occupation Framework
• The spatial distribution of cold gas in hierarchical galaxy formation models
• Non-linear Galaxy Power Spectrum and Cosmological Parameters
• The Secondary Spin Bias of Dark Matter Haloes
• Relating the structure of dark matter halos to their assembly and environment
• Priors on red galaxy stochasticity from hybrid effective field theory
• Controlling and leveraging small-scale information in tomographic galaxy-galaxy lensing
• Galaxy-galaxy-galaxy lensing: Third-order correlations between the galaxy and mass distributions in the Universe
• Constraints on $S_8$ from a full-scale and full-shape analysis of redshift-space clustering and galaxy-galaxy lensing in BOSS
• How much a galaxy knows about its large-scale environment?: An information theoretic perspective
• A Statistical Semi-Empirical Model: Satellite galaxies in Groups and Clusters
• Clustering of X-Ray-Selected AGN
• The High-Mass End of the Red Sequence at z~0.55 from SDSS-III/BOSS: completeness, bimodality and luminosity function
• Scaling relations of the colour-detected cluster RzCS 052 at z=1.016 and of some other high redshift clusters
• Deep Realistic Extragalactic Model (DREaM) Galaxy Catalogs: Predictions for a Roman Ultra-Deep Field
• The impact of halo shapes on the bispectrum in cosmology
• Does the Galaxy-Halo Connection Vary with Environment?
• The scaling relations of galaxy clusters and their dark matter halos
• How are galaxies assigned to halos? Searching for assembly bias in the SDSS galaxy clustering
• The MillenniumTNG Project: Refining the one-halo model of red and blue galaxies at different redshifts
• Testing the Accuracy of Halo Occupation Distribution Modelling using Hydrodynamic Simulations
• The pairwise velocity dispersion of galaxies: luminosity dependence and a new test of galaxy formation models
• The 6dF Galaxy Survey: Dependence of halo occupation on stellar mass
• Cosmology with Stacked Cluster Weak Lensing and Cluster-Galaxy Cross-Correlations
• Properties and Origin of Galaxy Velocity Bias in the Illustris Simulation
• The Conditional Colour-Magnitude Distribution: I. A Comprehensive Model of the Colour-Magnitude-Halo Mass Distribution of Present-Day Galaxies
• nIFTy Cosmology: the clustering consistency of galaxy formation models
• Probing Galaxy Assembly Bias in BOSS Galaxies Using Void Probabilities
• The VIMOS-VLT Deep Survey: Evolution in the Halo Occupation Number since z $\sim$ 1
• On Recovering the Nonlinear Bias Function from Counts in Cells Measurements
• Constraining thermal dust emission in distant galaxies with number counts and angular power spectra
• The Most Bound Halo Particle-Galaxy Correspondence Model: Comparison between Models with Different Merger Timescales
• Galaxy assembly bias of central galaxies in the Illustris simulation
• Towards Accurate Modelling of Galaxy Clustering on Small Scales: Testing the Standard $\Lambda \mathrm{CDM}$ + Halo Model
• 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
• Extensions to the halo occupation distribution model for more accurate clustering predictions
• $\mathrm{S}\mathrm{IM}\mathrm{BIG}$: Mock Challenge for a Forward Modeling Approach to Galaxy Clustering
• Massive central galaxies of galaxy groups in the Romulus simulations: an overview of galaxy properties at z=0
• Cosmological Three-Point Function: Testing The Halo Model Against Simulations
• The Galaxy--Halo Connection in High-Redshift Universe: Details and Evolution of Stellar-to-Halo Mass Ratios of Lyman Break Galaxies on CFHTLS Deep Fields
• The scatter in the galaxy-halo connection: a machine learning analysis
• The BOSS-WiggleZ overlap region II: dependence of cosmic growth on galaxy type
• A Parameter-Masked Mock Data Challenge for Beyond-Two-Point Galaxy Clustering Statistics
• Linear bias forecasts for emission line cosmological surveys
• Small- and Large-Scale Galactic Conformity in SDSS DR7
• Relative clustering and the joint halo occupation distribution of red-sequence and blue-cloud galaxies in COMBO-17
• The ALHAMBRA survey: evolution of galaxy clustering since $z\sim 1$
• Intrinsic/Extrinsic Density-Ellipticity Correlations and Galaxy-Galaxy Lensing
• How to Optimally Constrain Galaxy Assembly Bias: Supplement Projected Correlation Functions with Count-in-cells Statistics
• The evolution of the galaxy content of dark matter haloes
• Revealing the cosmic web dependent halo bias
• Modeling Galaxy-Galaxy Weak Lensing with SDSS Groups
• Luminous Red Galaxy Population in Clusters at $0.2\le z\le 0.6$
• Spatial and Dynamical Biases in Velocity Statistics of Galaxies
• Discriminating Topology in Galaxy Distributions using Network Analysis
• What determines large scale galaxy clustering: halo mass or local density?
• How gas flows shape the stellar-halo mass relation in the EAGLE simulation
• Precise and Accurate Cosmology with CMBxLSS Power Spectra and Bispectra
• An observational proxy of halo assembly time and its correlation with galaxy properties
• Linking haloes to galaxies: how many halo properties are needed?
• A Parametrized Galaxy Catalog Simulator For Testing Cluster Finding, Mass Estimation and Photometric Redshift Estimation in Optical and Near Infrared Surveys
• Prediction of H$\alpha$ and [OIII] Emission Line Galaxy Number Counts for Future Galaxy Redshift Surveys
• The cosmic web of X-ray active galactic nuclei seen through the eROSITA Final Equatorial Depth Survey (eFEDS)
• GAMA+KiDS: Empirical correlations between halo mass and other galaxy properties near the knee of the stellar-to-halo mass relation
• On the prospect of using the maximum circular velocity of halos to encapsulate assembly bias in the galaxy-halo connection
• Where are the z=4 Lyman Break Galaxies? Results from Conditional Luminosity Function Models of Luminosity-dependent Correlation Functions
• Are the halo occupation predictions consistent with large scale galaxy clustering?
• Halo assembly bias from Separate Universe simulations
• Candidate Clusters of Galaxies at $z>1.3$ Identified in the Spitzer SPT Deep Field Survey
• ELUCID V. Lighting dark matter halos with galaxies
• Composition of Low Redshift Halo Gas
• On the observability of coupled dark energy with cosmic voids
• Galaxy groups in the 2MASS Redshift Survey
• The galaxy size - halo mass scaling relations and clustering properties of central and satellite galaxies
• One- and Two-point Source Statistics from the LOFAR Two-metre Sky Survey First Data Release
• Understanding the nature of luminous red galaxies (LRGs): Connecting LRGs to central and satellite subhalos
• Halo Occupation Distribution Modeling of Green Valley Galaxies
• Precision Measurements of Higher-Order Angular Galaxy Correlations Using 11 Million SDSS Galaxies
• The Luminosity Function of the NoSOCS Galaxy Cluster Sample
• Masses of high-z galaxy hosting haloes from angular clustering and their evolution in the CDM model
• 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
• The spatial distribution of neutral hydrogen as traced by low HI mass galaxies
• Forecasting the Dark Energy Measurement with Baryon Acoustic Oscillations: Prospects for the LAMOST surveys
• First detection of galaxy-galaxy-galaxy lensing in RCS. A new tool for studying the matter environment of galaxy pairs
• Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias
• A Subhalo-Galaxy Correspondence Model of Galaxy Formation
• The MillenniumTNG Project: The large-scale clustering of galaxies
• The extended ROSAT-ESO Flux-Limited X-ray Galaxy Cluster Survey (REFLEX II) VII The Mass Function of Galaxy Clusters
• How galaxies populate haloes in very low-density environments? An analysis of the Halo Occupation Distribution in cosmic voids
• Intergalactic Dust Extinction in Hydrodynamic Cosmological Simulations
• A unified model for the clustering of quasars and galaxies at $z\approx 6$
• Revisiting the Size-Luminosity Relation in the Era of Ultra Diffuse Galaxies
• Spin Flips - II. Evolution of dark matter halo spin orientation, and its correlation with major mergers
• The Halo Void (Dust) Model of Large Scale Structure
• Imprints of Supermassive Black Hole Evolution on the Spectral and Spatial Anisotropy of Nano-Hertz Stochastic Gravitational-Wave Background
• Clustering analysis of high-redshift Luminous Red Galaxies in Stripe 82
• An accurate method to determine the systematics due to the peculiar velocities of galaxies in measuring the Hubble constant from gravitational wave standard sirens
• Understanding the PSCz Galaxy Power Spectrum with N-body Simulations
• The clustering amplitude of X-ray selected AGN at z=0.8: Evidence for a negative dependence on accretion luminosity
• Understanding the non-linear clustering of high redshift galaxies
• Precision Redshift-Space Galaxy Power Spectra using Zel'dovich Control Variates
• Lyman-Break Galaxies at $z\sim 3$ in the Subaru Deep Field: Luminosity Function, Clustering and [OIII] Emission
• The Galaxy Cross-Correlation Function as a Probe of the Spatial Distribution of Galactic Satellites
• Tidal alignments as a contaminant of the galaxy bispectrum
• The detection of the imprint of filaments on cosmic microwave background lensing
• HInet: Generating neutral hydrogen from dark matter with neural networks
• ECO and RESOLVE: Galaxy Disk Growth in Environmental Context
• The halo light cone catalogues of \Abacus{AbacusSummit}
• A question of separation: disentangling tracer bias and gravitational nonlinearity with counts-in-cells statistics
• GalICS V : Low and high order clustering in mock SDSS's
• Measuring the Halo Mass of z=3 Damped Ly-alpha Absorbers from the Absorber-Galaxy Cross-correlation
• The MillenniumTNG Project: Semi-analytic galaxy formation models on the past lightcone
• On the scatter in the relation between stellar mass and halo mass: random or halo formation time dependent?
• The age dependence of galaxy clustering
• Spatial Clustering of High Redshift Lyman Break Galaxies
• Cosmological implications from the full shape of the large-scale power spectrum of the SDSS DR7 luminous red galaxies
• Quasar-Galaxy Clustering through Projected Galaxy Counts at z=0.6-1.2
• Convolution Lagrangian perturbation theory for biased tracers beyond general relativity
• The Clustering Evolution of Dusty Star-Forming Galaxies
• Constructing high-fidelity halo merger trees in AbacusSummit
• Taking advantage of photometric galaxy catalogues to determine the halo occupation distribution
• The connection between the host halo and the satellite galaxies of the Milky Way
• SHAM through the lens of a hydrodynamical simulation
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• Reconstructing the baryon acoustic oscillations using biased tracers
• Don't Forget the Forest for the Trees: The Stellar-Mass Halo-Mass Relation in Different Environments
• Construct the emission line galaxy-host halo connection through auto and cross correlations
• Clustering at high redshift: The connection between Lyman Alpha emitters and Lyman break galaxies
• Cosmic Infrared Background anisotropies as a window into primordial non-Gaussianity
• Pairwise velocities in the Halo Model: Luminosity and Scale Dependence
• Cosmic CARNage II: the evolution of the galaxy stellar mass function in observations and galaxy formation models
• Characterizing the local gamma-ray Universe via angular cross-correlations
• Crawling the Cosmic Network: Exploring the Morphology of Structure in the Galaxy Distribution
• Optimal filters for the moving lens effect
• A study on the statistical significance of mutual information between morphology of a galaxy and its large-scale environment
• The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: GLAM-QPM mock galaxy catalogs for the Emission Line Galaxy Sample
• [OII] emitters in MultiDark-Galaxies and DEEP2
• A Direct Measurement of the Mean Occupation Function of Quasars: Breaking Degeneracies between Halo Occupation Distribution Models
• DESCQA: An Automated Validation Framework for Synthetic Sky Catalogs
• The clustering of $z>7$ galaxies: Predictions from the BLUETIDES simulation
• Primordial trispectrum from kSZ tomography
• Dark matter halo occupation: environment and clustering
• The Formation History of Subhalos and the Evolution of Satellite Galaxies
• Host Dark Matter Halos of WISE-selected Obscured & Unobscured Quasars: Evidence for Evolution
• The Aemulus Project VI: Emulation of beyond-standard galaxy clustering statistics to improve cosmological constraints
• Photometric Objects around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. I. Methods
• The peculiar velocities of satellites of external disk galaxies
• Testing redMaPPer centring probabilities using galaxy clustering and galaxy-galaxy lensing
• Galaxy and Mass Assembly: luminosity and stellar mass functions in GAMA groups
• The environment and host haloes of the brightest z~6 Lyman-break galaxies
• An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies
• The Evolution of K* and the Halo Occupation Distribution since z=1.5: Observations vs. Simulations
• Determine the galaxy bias factors on large scales using bispectrum method
• Giant disk galaxies : Where environment trumps mass in galaxy evolution
• Passive Evolution of Galaxy Clustering
• Subhaloes gone Notts: the clustering properties of subhaloes
• On the role of feedback in shaping the cosmic abundance and clustering of neutral atomic hydrogen in galaxies
• Joint Analysis of Galaxy-Galaxy Lensing and Galaxy Clustering: Methodology and Forecasts for DES
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• The assembly bias of emission line galaxies
• A determination of dark matter bispectrum with a large set of N-body simulations
• Does jackknife scale really matter for accurate large-scale structure covariances?
• Extending Recovery of the Primordial Matter Power Spectrum
• Second Moment of Halo Occupation Number
• A Hybrid Fast Multipole Method for Cosmological N-body Simulations
• On the Clustering of Faint Red Galaxies
• A Steep Slope and Small Scatter for the High-Mass End of the L-$\sigma$ Relation at $z\sim 0.55$
• ELUCID -- Exploring the Local Universe with the reConstructed Initial Density field. II: Reconstruction diagnostics, applied to numerical halo catalogs
• Disentangling redshift-space distortions and nonlinear bias using the 2D power spectrum
• The Halo Occupation Distribution of Obscured Quasars: Revisiting the Unification Model
• Clustering Properties of restframe UV selected galaxies I: the correlation length derived from GALEX data in the local Universe
• Counts-in-Cylinders in the Sloan Digital Sky Survey with Comparisons to N-body Simulations
• Tracing the Nature of Dark Energy with Galaxy Distribution
• Tracing the cosmic velocity field at z ~ 0.1 from galaxy luminosities in the SDSS DR7
• Generating mock galaxy catalogues for flux-limited samples like the DESI Bright Galaxy Survey
• Analytical halo model of galactic conformity
• Building a Better Understanding of the High Redshift BOSS Galaxies as Tools for Cosmology
• CSST large-scale structure analysis pipeline: I. constructing reference mock galaxy redshift surveys
• Analytic marginalization of $N(z)$ uncertainties in tomographic galaxy surveys
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• 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
• Modeling Redshift-Space Clustering with Abundance Matching
• Effect of model-dependent covariance matrix for studying Baryon Acoustic Oscillations
• How do galaxies populate halos in extreme density environments? An analysis of the Halo Occupation Distribution in SDSS
• Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-$y$-maps from SPT and Planck
• HOD-Dependent Systematics for Luminous Red Galaxies in the DESI 2024 BAO Analysis
• The Baryonic Collapse Efficiency of Galaxy Groups in the RESOLVE and ECO Surveys
• Brightest group galaxies-II: the relative contribution of BGGs to the total baryon content of groups at z<1.3
• Angular clustering and host halo properties of [OII] emitters at $z>1$ in the Subaru HSC survey
• Hybrid analytic and machine-learned baryonic property insertion into galactic dark matter haloes
• Robustness of the covariance matrix for galaxy clustering measurements
• Cosmological Probes of Structure Growth and Tests of Gravity
• Testing the consistency of three-point halo clustering in Fourier and configuration space
• Predictions of Quasar Clustering: Redshift, Luminosity and Selection Dependence
• Rosella: A mock catalogue from the P-Millennium simulation
• On the Redshift Evolution of MgII Absorption Systems
• Non-Gaussianity of the Cosmic Infrared Background anisotropies II : Predictions of the bispectrum and constraints forecast
• Galaxy Three-Point Correlation Functions and Halo/Subhalo Models
• Clustering of Extremely Red Objects in Elais-N1 from the UKIDSS DXS with optical photometry from Pan-STARRS1 and Subaru
• A Halo Model with Environment Dependence: Theoretical Considerations
• Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. IV. High Precision Constraints on the Evolution of Stellar-Halo Mass Relation at Redshift $z<0.7$
• The impact of systematic uncertainties in N-body simulations on the precision cosmology from galaxy clustering: a halo model approach
• A Direct Measurement of the High-Mass End of the Velocity Dispersion Function at $z\sim 0.55$ from SDSS-III/BOSS
• How feedback shapes galaxies: an analytic model
• Revisiting the Extreme Clustering of $z\approx 4$ Quasars with Large Volume Cosmological Simulations
• HOD modelling of high redshift galaxies using the BLUETIDES simulation
• Constraining Primordial Non-Gaussianity with Moments of the Large Scale Density Field
• Constraints on sigma_8 from galaxy clustering in N-body simulations and semi-analytic models
• Massive, red galaxies in a hierarchical universe-II Clustering of Extremely Red Objects
• 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
• Clustering of red-sequence galaxies in the fourth data release ofthe Kilo-Degree Survey
• The Halo Occupation Distribution of HI from 21cm Intensity Mapping at Moderate Redshifts
• Simulating the Anisotropic Clustering of Luminous Red Galaxies with Subhalos: A Direct Confrontation with Observation and Cosmological Implications
• The clustering and halo occupation distribution of Lyman-break galaxies at $z\sim 4$
• Correlation function: biasing and fractal properties of the cosmic web
• Galaxy And Mass Assembly (GAMA): The absence of stellar mass segregation in galaxy groups and consistent predictions from GALFORM and EAGLE simulations
• Testing galaxy formation models with galaxy stellar mass functions
• Galaxy Clusters in the Line of Sight to Background Quasars: II. Environmental effects on the sizes of baryonic halo sizes
• A Halo Occupation Interpretation Of Quasars At $z\sim 1.5$ Using Very Small Scale Clustering Information
• Clustering tomography: measuring cosmological distances through angular clustering in thin redshift shells
• The Halo Occupation Distribution of Black Holes: Dependence on Mass
• Downsizing of Star Formation Measured from the Clustered Infrared Background Correlated with Quasars
• Effect of primordial non-Gaussianities on the far-UV luminosity function of high-redshift galaxies: implications for cosmic reionization
• The structure of the merging RCS 231953+00 Supercluster at z ~ 0.9
• Using galaxy pairs to investigate the three-point correlation function in the squeezed limit
• Constraining Dark Energy With Stacked Concave Lenses
• ISW-Galaxy Cross Correlation:A probe of Dark Energy clustering and distribution of Dark Matter tracers
• Cosmology with the thermal-kinetic Sunyaev-Zel'dovich effect
• Quasars at intermediate redshift are not special; but they are often satellites
• How the Galaxy-Halo Connection Depends on Large-Scale Environment
• The star formation history in the last 10 billion years from CIB cross-correlations
• Properties of Voids in the 2dFGRS Galaxy Survey
• A physical model for the origin of the diffuse cosmic infrared background
• Clustering of galaxies at 3.6 microns in the Spitzer Wide-area Infrared Extragalactic legacy survey
• Baryon oscillations in galaxy and matter power-spectrum covariance matrices
• Using GAMA to probe the impact of small-scale galaxy physics on nonlinear redshift-space distortions
• Galaxy growth by merging in the nearby universe
• A galaxy-halo model of large-scale structure
• Constraining Halo Occupation Distribution and Cosmic Growth Rate using Multipole Power Spectrum
• High-fidelity reproduction of central galaxy joint distributions with Neural Networks
• Galaxy Clustering in the Mira-Titan Universe I: Emulators for the redshift space galaxy correlation function and galaxy-galaxy lensing
• MAHGIC: A Model Adapter for the Halo-Galaxy Inter-Connection
• The Uchuu-GLAM BOSS and eBOSS LRG lightcones: Exploring clustering and covariance errors
• Halo Masses of MgII absorbers at z\sim 0.5 from SDSS DR7
• Tracking the orbit of unresolved subhalos for semi-analytic models
• Cosmology from LOFAR Two-metre Sky Survey Data Release 2: Cross-correlation with the cosmic microwave background
• Impact of tidal environment on galaxy clustering in GAMA
• KiDS-1000: Weak lensing and intrinsic alignment around luminous red galaxies
• The Beyond-Halo Mass Effects of the Cosmic Web Environment on Galaxies
• An empirical model to form and evolve galaxies in dark matter halos
• Sunyaev-Zel'dovich Signal from Quasar Hosts: Implications for Detection of Quasar Feedback
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Constraining the Galaxy-Halo Connection with Optimal Statistics
• How to empirically model star formation in dark matter halos: I. Inferences about central galaxies from numerical simulations
• Subtracting the kinetic Sunyaev-Zeldovich effect from the cosmic microwave background with surveys of large-scale structure
• Recovering the Tidal Field in the Projected Galaxy Distribution
• The contribution of star-forming galaxies to fluctuations in the cosmic background light
• Got plenty of nothing: cosmic voids as a probe of particle dark matter
• Constraints on primordial non-Gaussianity from WMAP7 and Luminous Red Galaxies power spectrum and forecast for future surveys
• Rapid Simulations of Halo and Subhalo Clustering
• Halo Model Analysis of Cluster Statistics
• The abundance and colours of galaxies in high redshift clusters in the cold dark matter cosmology
• Linking galaxies to dark matter haloes at $z\sim 1$ : dependence of galaxy clustering on stellar mass and specific star formation rate
• The Impact of the Dusty Torus on Obscured Quasar Halo Mass Measurements
• Damped Lyman-$\alpha$ absorbers and atomic hydrogen in galaxies: the view of the GAEA model
• Weak lensing measurement of the mass-richness relation using the SDSS database
• Global analysis of luminosity- and colour-dependent galaxy clustering in the Sloan Digital Sky Survey
• Can a conditioning on stellar mass explain the mutual information between morphology and environment?
• Dark against luminous matter around isolated central galaxies: a comparative study between modern surveys and Illustris-TNG
• The XMM Cluster Survey: The Halo Occupation Number of BOSS galaxies in X-ray clusters
• Validating the clustering predictions of empirical models with the FLAMINGO simulations
• Angular clustering of z~2 star-forming and passive galaxies in 2.5 square degrees of deep CFHT imaging
• Skewing the CMB$\times$LSS: a Fast Method for Bispectrum Analysis
• Cell Count Moments in the Halo Model
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions and Lingering Tension
• 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
• Constraints on dark matter and astrophysics from tomographic $\gamma$-ray cross-correlations
• Herschel-ATLAS/GAMA:How does the far-IR luminosity function depend on galaxy group properties?
• Measuring the Galaxy-Galaxy-Mass Three-point Correlation Function with Weak Gravitational Lensing
• On the Apparent Power Law in CDM Halo Pseudo Phase Space Density Profiles
• Void Probability Function of Simulated Surveys of high-redshift Lyman-Alpha Emitters
• Non-linear power spectra of dark and luminous matter in halo model of structure formation
• Computing 3 point correlation function randoms counts without the randoms catalogue
• Constraining galaxy-halo connection with high-order statistics
• Galaxy populations in haloes in high-density environments
• PRIMUS: Clustering of Star-forming and Quiescent Central Galaxies at $0.2<z<0.9$
• A new test of gravity -- I: Introduction to the method
• Fast Forward Modelling of Galaxy Spatial and Statistical Distributions
• Perturbation theory models for LSST-era galaxy clustering: tests with sub-percent mock catalog measurements in Fourier and configuration space
• A direct measurement of hierarchical growth in galaxy groups since z~1
• Self-calibrating optical galaxy cluster selection bias using cluster, galaxy, and shear cross-correlations
• PRIMUS: The Effect of Physical Scale on the Luminosity-Dependence of Galaxy Clustering via Cross-Correlations
• Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
• Accurate Modeling of the Projected Galaxy Clustering in Photometric Surveys: I. Tests with Mock Catalogs
• LARgE Survey -- II. The Dark Matter Halos and the Progenitors and Descendants of Ultra-Massive Passive Galaxies at Cosmic Noon
• Optical galaxy cluster mock catalogs with realistic projection effects: Validations with the SDSS clusters
• HI HOD -- I. The Halo Occupation Distribution of HI Galaxies
• Multi-wavelength consensus of large-scale linear bias
• Quasi-periodical features in the distribution of Luminous Red Galaxies
• Geometrical tests of cosmological models. I. Probing dark energy using the kinematics of high-redshift galaxies
• Galaxy clustering using photometric redshifts
• Towards a Model-Independent Measurement of the Halo Mass Function with Observables
• Small scale clustering of BOSS galaxies: dependence on luminosity, color, age, stellar mass, specific star formation rate and other properties
• Star-forming and Quiescent Central Galaxies Cluster Similarly: Implications for the Galaxy-Halo Connection
• A two-phase model of galaxy formation: III. The formation of globular clusters
• ScamPy -- A sub-halo clustering & abundance matching based Python interface for painting galaxies on the dark matter halo/sub-halo hierarchy
• Galaxy-galaxy lensing in the VOICE deep survey
• DESI Mock Challenge: Constructing DESI galaxy catalogues based on FastPM simulations
• Secondary halo bias through cosmic time II: Reconstructing halo properties using clustering information
• Improving Constraint on ${\Omega }_m$ from SDSS Using Marked Correlation Functions
• Correlation Analysis of Decaying Sterile Neutrino Dark Matter in the Context of the SRG Mission
• CFHTLenS: Galaxy bias as function of scale, stellar mass, and colour. Conflicts with predictions by semi-analytic models
• Non-Gaussian assembly bias from a semi-analytic galaxy formation model
• The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
• Baryon effects on the dark matter halos constrained from strong gravitational lensing
• Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation
• Effect of Massive Neutrinos on the Position of Cold Dark Matter Halo: Revealed via Delaunay Triangulation Void
• Modeling spatially-resolved galactic H$\alpha$ emission for galaxy clustering
• Estimating lifetimes of uv-selected massive galaxies at $0.5\le z\le 2.5$ in the cosmos/ultravista field through clustering analyses
• Euclid: Photometric redshift calibration with self-organising maps
• Peaks in the cosmological density field: parameter constraints from 2dF Galaxy Redshift Survey data
• The impact of AGN X-ray selection on the AGN halo occupation distribution
• Scaling of the 1-halo terms with bias
• How do uncertainties in galaxy formation physics impact field-level galaxy bias?
• Exploring HOD-dependent systematics for the DESI 2024 Full-Shape galaxy clustering analysis
• Clustering of galaxies around GRB sight-lines
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• Conditional Colour-Magnitude Distribution of Central Galaxies in Galaxy Formation Models
• A Galaxy-Halo Model for Multiple Cosmological Tracers
• Incompatibility of Standard Galaxy Bias Models in General Relativity
• ACACIA: a new method to produce on-the-fly merger trees in the RAMSES code
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• ELG$\times$LRG distribution through dark matter halo dynamics
• Relatively Fast and Reasonably Furious: Evidence for Increased Burstiness in Smaller Halos at Cosmic Dawn
• Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
• BASILISK II. Improved Constraints on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• Influence of baryons on spatial distribution of matter: higher order correlation functions
• Constraining galaxy properties with complete samples of lenses
• Galaxy Correlation Function and Local Density from Photometric Redshifts Using the Stochastic Order Redshift Technique (SORT)
• CLIMBER: Galaxy-Halo Connection Constraints from Next-Generation Surveys
• Measuring the scatter of the mass-richness relation in galaxy clusters in photometric imaging surveys by means of their correlation function
• Pulsar B1237+25 Aberration/Retardation Analysis from Decimeter to Decameter Wavelength: Challenge to "Radius-to-Frequency Mapping"
• Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
• Atomic Hydrogen Shows its True Colours: Correlations between HI and Galaxy Colour in Simulations
• Studying baryon acoustic oscillations using photometric redshifts from the DESI Legacy Imaging survey DR9
• Bounds on galaxy stochasticity from halo occupation distribution modeling
• The evolution of the halo occupation distribution in cosmic voids
• Impact of projection-induced optical selection bias on the weak lensing mass calibration of galaxy clusters
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• Toward accurate measurement of property-dependent galaxy clustering I. Comparison of the Vmax method and the "shuffled" method
• Improving the Accuracy of Halo Mass Based Statistics For Fast Approximate N-body Simulations
• DESI Emission-line Galaxies: Clustering Dependence on Stellar Mass and [OII] Luminosity
• Completeness III: identifying characteristic systematics and evolution in galaxy redshift surveys
• Spatial clustering in the ESO-Sculptor Survey: two-point correlation functions by galaxy type at redshifts 0.1 - 0.5
• Constraining galactic baryon cycle using the galaxy stellar-to-halo mass relations
• Probabilistic Lagrangian bias estimators and the cumulant bias expansion
• Dark Energy Survey Year 3 results: Galaxy-halo connection from galaxy-galaxy lensing
• Towards an optimal extraction of cosmological parameters from galaxy cluster surveys using convolutional neural networks
• Galaxy clustering in modified gravity from full-physics simulations. I: two-point correlation functions
• A semi-analytic estimate for the effective sound speed counterterm in the EFTofLSS
• Exploiting Non-linear Scales in Galaxy-Galaxy Lensing and Galaxy Clustering: A Forecast for the Dark Energy Survey
• Halo Merger Tree Comparison: Impact on Galaxy Formation Models
• Simultaneous Estimation of Large-Scale Structure and Milky Way Dust Extinction from Galaxy Surveys
• Morpho-statistical characterisation of the spatial galaxy distribution through Gibbs point processes
• Predicting halo occupation and galaxy assembly bias with machine learning
• The mass and redshift dependence of halo star clustering
• Constraining Galaxy-Halo Connection Using Machine Learning
• Using two point correlation functions to understand the assembly histories of Milky Way-like galaxies
• Answers from the void: VIDE and its applications
• JERALD: high-fidelity dark matter, stellar mass and neutral hydrogen maps from fast N-body simulations
• Galaxies in X-ray Selected Clusters and Groups in Dark Energy Survey Data II: Hierarchical Bayesian Modeling of the Red-Sequence Galaxy Luminosity Function
• MIGHTEE: The dark matter haloes, duty cycle and mechanical feedback from radio-AGN up to $z\sim 2.5$
• Galaxy assembly bias in cosmological hydrodynamical simulations: a comparison between SIMBA and IllustrisTNG
• The invariance of group occupation across the cosmic web
• On the fairness of the main galaxy sample of SDSS
• CosmoGLINT: Cosmological Generative Model for Line Intensity Mapping with Transformer
• Dark Matter and Galaxy Cross-Correlations with the Cherenkov Telescope Array Observatory
• Three-Dimensional Filamentation Analysis of SDSS DR5 Survey
• A hierarchical clustering method for quantifying satellite abundance
• One Galaxy Sample to Rule Them All: Halo Occupation Distribution Modeling of DES Year 3 Source Galaxies
• ODIN: Using multiplicity of Lyman-Alpha Emitters to assess star formation activity in dark matter halos
• HI Intensity Mapping cross-correlation with thermal SZ fluctuations: forecasted cosmological parameters estimation for FAST and Planck
• Sample Variance in Cosmological Observations with a Narrow Field-of-View
• Euclid: Improving redshift distribution reconstruction using a deep-to-wide transfer function
• A Non-parametric Method for the Inference of Halo Occupation Distributions
• NeutralUniverseMachine: Predictions of HI gas in Different Theoretical Models
• Fast Baryonic Field Painting for Sunyaev-Zel'dovich Analyses: Transfer Function vs. Hybrid Effective Field Theory
• A redshift distortion free correlation function at third order in the nonlinear regime
• Wiener filtering and multi-tracer techniques for dark matter cross-correlations between gamma-ray emission and galaxy catalogs
• Marked statistics across the cosmic web: Environmental dependent clustering in modified gravity simulations
• Mimicking the halo-galaxy connection using machine learning
• Dynamic Zoom Simulations of structure formation beyond standard cosmology
• Cosmology from LOFAR Two-metre Sky Survey Data Release 2: Counts-in-Cells Statistics
• A lightcone catalogue from the Millennium-XXL simulation: improved spatial interpolation and colour distributions for the DESI BGS
• An emulation-based model for the projected correlation function