Theoretical Models of the Halo Occupation Distribution: Separating Central and Satellite Galaxies

Abstract

The halo occupation distribution (HOD) describes the relation between galaxies and dark matter at the level of individual dark matter halos. The properties of galaxies residing at the centers of halos differ from those of satellite galaxies because of differences in their formation histories. Using a smoothed particle hydrodynamics (SPH) simulation and a semi-analytic (SA) galaxy formation model, we examine the separate contributions of central and satellite galaxies to the HOD, more specifically to the probability P(N|M) that a halo of virial mass M contains N galaxies of a particular class. In agreement with earlier results for dark matter subhalos, we find that the mean occupation function <N> for galaxies above a baryonic mass threshold can be approximated by a step function for central galaxies plus a power law for satellites, and that the distribution of satellite numbers is close to Poisson at fixed halo mass. For galaxy samples defined by different baryonic mass thresholds, there is a nearly linear relation between the minimum halo mass Mmin required to host a central galaxy and the mass M1 at which an average halo hosts one satellite, with M1 ~ 14 Mmin (SPH) or M1 ~ 18 Mmin (SA). The mean occupation number of young galaxies exhibits a local minimum at M ~ 10 Mmin where halos are too massive to host a young central galaxy but not massive enough to host satellites. We show that the conditional galaxy mass function at fixed halo mass cannot be described by a Schechter function because central galaxies produce a "bump" at high masses. We suggest parameterizations for the HOD and the conditional luminosity function that can be used to model observed galaxy clustering. Many of our predictions are in good agreement with recent results inferred from clustering in the Sloan Digital Sky Survey.

38 pages, 13 figures. Figures are added to show model predictions on CLF and the conditional mass distribution of halos hosting galaxies at fixed luminosity. Accepted for publication in ApJ

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• The Dearth of Difference between Central and Satellite Galaxies I. Perspectives on star formation quenching and AGN activities
• The galaxy-halo connection in the VIDEO Survey at 0.5<z<1.7
• Tomographic Magnification of Lyman Break Galaxies in The Deep Lens Survey
• Hierarchical Galaxy Growth and Scatter in the Stellar Mass - Halo Mass Relation
• The Q Continuum Simulation: Harnessing the Power of GPU Accelerated Supercomputers
• The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for Galaxy Clustering Measurements
• Marked clustering statistics in $f(R)$ gravity cosmologies
• Exploring the halo occupation of AGN using dark-matter cosmological simulations
• Extrinsic Sources of Scatter in the Richness-Mass Relation of Galaxy Clusters
• Power spectrum tomography of dark matter annihilation with local galaxy distribution
• Optimal Weighting in Galaxy Surveys: Application to Redshift-Space Distortions
• The dependence of galaxy clustering on stellar mass, star-formation rate and redshift at z = 0.8-2.2, with HiZELS
• The Halo Occupation Distribution of X-ray-Bright Active Galactic Nuclei: A Comparison with Luminous Quasars
• Luminous Red Galaxy Halo Density Field Reconstruction and Application to Large Scale Structure Measurements
• Differential Neutrino Condensation onto Cosmic Structure
• The Incomplete Conditional Stellar Mass Function: Unveiling the Stellar Mass Functions of Galaxies at 0.1 < Z < 0.8 from BOSS Observations
• Combining FOF and halo-based algorithms for the identification of galaxy groups
• Perturbation theory for modeling galaxy bias: validation with simulations of the Dark Energy Survey
• Luminous Red Galaxies in hierarchical cosmologies
• Using galaxy-galaxy weak lensing measurements to correct the Finger-of-God
• Modeling the Very Small-Scale Clustering of Luminous Red Galaxies
• The clustering of typical Ly$\alpha$ emitters from $z\sim 2.5-6$: host halo masses depend on Ly$\alpha$ and UV luminosities
• Do model emission line galaxies live in filaments at z~1?
• The clustering of radio galaxies: biasing and evolution versus stellar mass
• Cosmic Voids and Galaxy Bias in the Halo Occupation Framework
• Priors on red galaxy stochasticity from hybrid effective field theory
• The Contribution of z<6 Sources to the Spatial Coherence in the Unresolved Cosmic near-Infrared and X-ray Backgrounds
• Testing modified gravity using a marked correlation function
• Clustering of X-Ray-Selected AGN
• Evolution of the Clustering of Photometrically Selected SDSS Galaxies
• Validating a minimal galaxy bias method for cosmological parameter inference using HSC-SDSS mock catalogs
• A new method to assign galaxy cluster membership using photometric redshifts
• Does the Galaxy-Halo Connection Vary with Environment?
• Cosmology with Stacked Cluster Weak Lensing and Cluster-Galaxy Cross-Correlations
• How are galaxies assigned to halos? Searching for assembly bias in the SDSS galaxy clustering
• The 6dF Galaxy Survey: Dependence of halo occupation on stellar mass
• Intensity mapping cross-correlations II: HI halo models including shot noise
• Cosmological Constraints from Galaxy Clustering and the Mass-to-Number Ratio of Galaxy Clusters: Marginalizing over the Physics of Galaxy Formation
• 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
• A New Statistic for Analyzing Baryon Acoustic Oscillations
• Precise Cosmological Constraints from BOSS Galaxy Clustering with a Simulation-Based Emulator of the Wavelet Scattering Transform
• The Conditional Colour-Magnitude Distribution: I. A Comprehensive Model of the Colour-Magnitude-Halo Mass Distribution of Present-Day Galaxies
• On the statistics of proto-cluster candidates detected in the Planck all-sky survey
• The Most Bound Halo Particle-Galaxy Correspondence Model: Comparison between Models with Different Merger Timescales
• Extracting cosmological information from the angular power spectrum of the 2MASS Photometric Redshift catalogue
• 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
• The VIMOS Ultra Deep Survey. Luminosity and stellar mass dependence of galaxy clustering at z~3
• The stellar mass - halo mass relation from galaxy clustering in VUDS: a high star formation efficiency at z~3
• Intrinsic alignment statistics of density and velocity fields at large scales: Formulation, modeling, and baryon acoustic oscillation features
• Extensions to the halo occupation distribution model for more accurate clustering predictions
• Neutrino mass and dark energy constraints from redshift-space distortions
• 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
• Galaxy clustering and projected density profiles as traced by satellites in photometric surveys: Methodology and luminosity dependence
• Non-Gaussianity of the Cosmic Infrared Background anisotropies I : Diagrammatic formalism and application to the angular bispectrum
• How to Optimally Constrain Galaxy Assembly Bias: Supplement Projected Correlation Functions with Count-in-cells Statistics
• Relative clustering and the joint halo occupation distribution of red-sequence and blue-cloud galaxies in COMBO-17
• Dependence of Halo Bias and Kinematics on Assembly Variables
• A Parameter-Masked Mock Data Challenge for Beyond-Two-Point Galaxy Clustering Statistics
• Discriminating Topology in Galaxy Distributions using Network Analysis
• The MillenniumTNG Project: Inferring cosmology from galaxy clustering with accelerated N-body scaling and subhalo abundance matching
• Modeling Galaxy-Galaxy Weak Lensing with SDSS Groups
• Luminous Red Galaxy Population in Clusters at $0.2\le z\le 0.6$
• The evolution of the galaxy content of dark matter haloes
• The influence of halo assembly on galaxies and galaxy groups
• Where are the z=4 Lyman Break Galaxies? Results from Conditional Luminosity Function Models of Luminosity-dependent Correlation Functions
• Remapping dark matter halo catalogues between cosmological simulations
• On the prospect of using the maximum circular velocity of halos to encapsulate assembly bias in the galaxy-halo connection
• Cosmological inference from emulator based halo model I: Validation tests with HSC and SDSS mock catalogs
• The cosmic web of X-ray active galactic nuclei seen through the eROSITA Final Equatorial Depth Survey (eFEDS)
• Local gravitational redshifts can bias cosmological measurements
• Candidate Clusters of Galaxies at $z>1.3$ Identified in the Spitzer SPT Deep Field Survey
• Early Black Holes in Cosmological Simulations: Luminosity Functions and Clustering Behaviour
• The galaxy size - halo mass scaling relations and clustering properties of central and satellite galaxies
• Halo Occupation Distribution Modeling of Green Valley Galaxies
• One- and Two-point Source Statistics from the LOFAR Two-metre Sky Survey First Data Release
• Galaxy groups in the 2MASS Redshift Survey
• Galaxy and Mass Assembly (GAMA): Colour and luminosity dependent clustering from calibrated photometric redshifts
• Local and global environmental effects on galaxies and active galactic nuclei
• $\text{matryoshka}$: Halo Model Emulator for the Galaxy Power Spectrum
• SDSS-IV MaNGA: Internal mass distributions and orbital structures of early-type galaxies and their dependence on environment
• Modeling Nearest Neighbor distributions of biased tracers using Hybrid Effective Field Theory
• ELUCID V. Lighting dark matter halos with galaxies
• H-ATLAS/GAMA: Magnification Bias Tomography. Astrophysical constraints above $\sim 1$ arcmin
• Probing galaxy bias and intergalactic gas pressure with KiDS Galaxies-tSZ-CMB lensing cross-correlations
• How galaxies populate haloes in very low-density environments? An analysis of the Halo Occupation Distribution in cosmic voids
• Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias
• Forecasting the Dark Energy Measurement with Baryon Acoustic Oscillations: Prospects for the LAMOST surveys
• The MillenniumTNG Project: The large-scale clustering of galaxies
• An improved limit on the neutrino mass with CMB and redshift-dependent halo bias-mass relations from SDSS, DEEP2, and Lyman-Break Galaxies
• Cosmological information content in redshift-space power spectrum of SDSS-like galaxies in the quasi-nonlinear regime up to $k=0.3h$Mpc${}^{-1}$
• Impacts of satellite galaxies on the redshift-space distortions
• Searching for Sterile Neutrino with X-ray Intensity Mapping
• A Subhalo-Galaxy Correspondence Model of Galaxy Formation
• 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
• An accurate method to determine the systematics due to the peculiar velocities of galaxies in measuring the Hubble constant from gravitational wave standard sirens
• Splashback radius of nonspherical dark matter halos from cosmic density and velocity fields
• Dissecting the roles of mass and environment quenching in galaxy evolution with EAGLE
• Intrinsic Alignments and Splashback Radius of Dark Matter Halos from Cosmic Density and Velocity Fields
• Understanding the non-linear clustering of high redshift galaxies
• A Conditional Luminosity Function Model of the Cosmic Far-Infrared Background Anisotropy Power Spectrum
• RESOLVE and ECO: The Halo Mass-Dependent Shape of Galaxy Stellar and Baryonic Mass Functions
• 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
• The effects of halo alignment and shape on the clustering of galaxies
• The halo light cone catalogues of \Abacus{AbacusSummit}
• Constraining the properties of gaseous halos via cross-correlations of upcoming galaxy surveys and thermal Sunyaev-Zel'dovich maps
• Convolution Lagrangian perturbation theory for biased tracers beyond general relativity
• Quasar-Galaxy Clustering through Projected Galaxy Counts at z=0.6-1.2
• Taking advantage of photometric galaxy catalogues to determine the halo occupation distribution
• CSST Cosmological Emulator I: Matter Power Spectrum Emulation with one percent accuracy to k = 10 h/Mpc
• Spatial Clustering of High Redshift Lyman Break Galaxies
• Constructing high-fidelity halo merger trees in AbacusSummit
• Spatial Clustering from GALEX-SDSS samples: Star Formation History and large-scale clustering
• Linear bias and halo occupation distribution of emission line galaxies from Nancy Grace Roman Space Telescope
• Clustering at high redshift: The connection between Lyman Alpha emitters and Lyman break galaxies
• A Search for Satellite Galaxies of Nearby Star-Forming Galaxies with Resolved Stars in LBT-SONG
• Construct the emission line galaxy-host halo connection through auto and cross correlations
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• Galaxy-galaxy weak gravitational lensing in $f(R)$ gravity
• The clustering of H$\beta$+[OIII] and [OII] emitters since $z\sim 5$: dependencies with line luminosity and stellar mass
• Don't Forget the Forest for the Trees: The Stellar-Mass Halo-Mass Relation in Different Environments
• Generating Synthetic Cosmological Data with GalSampler
• Illuminating Dark Matter Halo Density Profiles Without Subhaloes
• Reconstructing the baryon acoustic oscillations using biased tracers
• The WIRCam Deep Survey II: Mass Selected Clustering
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Measuring nonlinear galaxy bias at z~0.8
• Pairwise velocities in the Halo Model: Luminosity and Scale Dependence
• Neutrino effects on the morphology of cosmic large-scale structure
• Cosmic Infrared Background anisotropies as a window into primordial non-Gaussianity
• 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
• The Aemulus Project VI: Emulation of beyond-standard galaxy clustering statistics to improve cosmological constraints
• DESCQA: An Automated Validation Framework for Synthetic Sky Catalogs
• The peculiar velocities of satellites of external disk galaxies
• Cosmic Near-infrared Background Tomography with SPHEREx Using Galaxy Cross-correlations
• The Effects of Galaxy Assembly Bias on the Inference of Growth Rate from Redshift-Space Distortions
• Photometric Objects around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. I. Methods
• Testing redMaPPer centring probabilities using galaxy clustering and galaxy-galaxy lensing
• [OII] emitters in MultiDark-Galaxies and DEEP2
• A Direct Measurement of the Mean Occupation Function of Quasars: Breaking Degeneracies between Halo Occupation Distribution Models
• The clustering of $z>7$ galaxies: Predictions from the BLUETIDES simulation
• Non-Gaussianity of secondary anisotropies from ACTPol and Planck
• Determine the galaxy bias factors on large scales using bispectrum method
• A determination of dark matter bispectrum with a large set of N-body simulations
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• The galaxy correlation function as a constraint on galaxy formation physics
• Cosmology with the sub-millimetre galaxies magnification bias: Tomographic Analysis
• HOD-Dependent Systematics in Emission Line Galaxies for the DESI 2024 BAO analysis
• The environment and host haloes of the brightest z~6 Lyman-break galaxies
• Luminosity bias: from haloes to galaxies
• Passive Evolution of Galaxy Clustering
• The dependence of subhalo abundance matching on galaxy photometry and selection criteria
• The assembly bias of emission line galaxies
• Joint Analysis of Galaxy-Galaxy Lensing and Galaxy Clustering: Methodology and Forecasts for DES
• Group-galaxy correlations in redshift space as a probe of the growth of structure
• Searching for axion-like particle decay in the near-infrared background: an updated analysis
• (DarkAI) Mapping the large-scale density field of dark matter using artificial intelligence
• Extending Recovery of the Primordial Matter Power Spectrum
• Galaxy and Mass Assembly (GAMA): Small-scale anisotropic galaxy clustering and the pairwise velocity dispersion of galaxies
• Halo models of HI selected galaxies
• Does jackknife scale really matter for accurate large-scale structure covariances?
• The Halo Occupation Distribution of Obscured Quasars: Revisiting the Unification Model
• Cosmological constraints with the sub-millimetre galaxies Magnification Bias after large scale bias corrections
• On the Clustering of Faint Red Galaxies
• Disentangling redshift-space distortions and nonlinear bias using the 2D power spectrum
• A direct and robust method to observationally constrain the halo mass function via the submillimeter magnification bias: Proof of concept
• Halo Occupation Distribution of Massive Galaxies since z = 1
• Environmental dependence of the mass-metallicity relation in cosmological hydrodynamical simulations
• Improved Mock Galaxy Catalogs for the DEEP2 Galaxy Redshift Survey from Subhalo Abundance and Environment Matching
• 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
• How do galaxies populate halos in extreme density environments? An analysis of the Halo Occupation Distribution in SDSS
• Analytic marginalization of $N(z)$ uncertainties in tomographic galaxy surveys
• Generating mock galaxy catalogues for flux-limited samples like the DESI Bright Galaxy Survey
• The Clustering and Halo Masses of Star Forming Galaxies at z<1
• Building a Better Understanding of the High Redshift BOSS Galaxies as Tools for Cosmology
• Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-$y$-maps from SPT and Planck
• The Cross-correlation of MgII Absorption and Galaxies in BOSS
• Cosmology with the submillimetre galaxies magnification bias: Proof of concept
• Full forward model of galaxy clustering statistics with AbacusSummit lightcones
• HOD-Dependent Systematics for Luminous Red Galaxies in the DESI 2024 BAO Analysis
• Angular clustering and host halo properties of [OII] emitters at $z>1$ in the Subaru HSC survey
• Observational constraints of an anisotropic boost due to the projection effects using redMaPPer clusters
• Non-Gaussianity of the Cosmic Infrared Background anisotropies II : Predictions of the bispectrum and constraints forecast
• Extragalactic sources in Cosmic Microwave Background maps
• Normalization of the Matter Power Spectrum via Higher-Order Angular Correlations of Luminous Red Galaxies
• Testing Dark Matter Halo Models of Quasars With Thermal Sunyaev-Zeldovich Effect
• Building a digital twin of a luminous red galaxy spectroscopic survey: galaxy properties and clustering covariance
• Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of H$\alpha$ and [O III] emitters
• Massive, red galaxies in a hierarchical universe-II Clustering of Extremely Red Objects
• HOD modelling of high redshift galaxies using the BLUETIDES simulation
• The FMOS-COSMOS survey of star-forming galaxies at $z\sim 1.6$. V: Properties of dark matter halos containing H$\alpha$ emitting galaxies
• Reconstruction of halo power spectrum from redshift-space galaxy distribution: cylinder-grouping method and halo exclusion effect
• The Stellar-to-Halo Mass Ratios of Passive and Star-Forming Galaxies at z~2-3 from the SMUVS survey
• 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 $z<0.7$
• Constraints on sigma_8 from galaxy clustering in N-body simulations and semi-analytic models
• Galaxy Three-Point Correlation Functions and Halo/Subhalo Models
• Semi-analytic modelling of AGNs: auto-correlation function and halo occupation
• Modeling assembly bias with machine learning and symbolic regression
• The impact of systematic uncertainties in N-body simulations on the precision cosmology from galaxy clustering: a halo model approach
• Clustering of Extremely Red Objects in Elais-N1 from the UKIDSS DXS with optical photometry from Pan-STARRS1 and Subaru
• The clustering and halo occupation distribution of Lyman-break galaxies at $z\sim 4$
• Differentiable Predictions for Large Scale Structure with SHAMNet
• Good and Proper: Self-similarity of N-body Simulations with Proper Force Softening
• The Halo Occupation Distribution of Black Holes: Dependence on Mass
• The Dark Matter Haloes and Host Galaxies of MgII Absorbers at z~1
• Tracing the galaxy-halo connection with galaxy clustering in COSMOS-Web from z = 0.1 to z ~ 12
• Using galaxy pairs to investigate the three-point correlation function in the squeezed limit
• Constraining Dark Energy With Stacked Concave Lenses
• Biased tracer reconstruction with halo mass information
• The halo model with beyond-linear halo bias: unbiasing cosmological constraints from galaxy-galaxy lensing and clustering
• A Halo Occupation Interpretation Of Quasars At $z\sim 1.5$ Using Very Small Scale Clustering Information
• Effect of primordial non-Gaussianities on the far-UV luminosity function of high-redshift galaxies: implications for cosmic reionization
• Galaxy And Mass Assembly (GAMA): The absence of stellar mass segregation in galaxy groups and consistent predictions from GALFORM and EAGLE simulations
• Weak lensing power spectrum reconstruction by counting galaxies.-- I: the ABS method
• A physical model for the origin of the diffuse cosmic infrared background
• Galaxy clustering from the bottom up: A Streaming Model emulator I
• Efficient Construction of Mock Catalogs for Baryon Acoustic Oscillation Surveys
• How the Galaxy-Halo Connection Depends on Large-Scale Environment
• Cosmology with the thermal-kinetic Sunyaev-Zel'dovich effect
• Fingers-of-God effect of infalling satellite galaxies
• Probing gravity with redshift-space distortions: effects of tracer bias and sample selection
• 2D k-th nearest neighbor statistics: a highly informative probe of galaxy clustering
• Quasars at intermediate redshift are not special; but they are often satellites
• Galaxy growth by merging in the nearby universe
• Halo Occupation Distribution of Emission Line Galaxies: fitting method with Gaussian Processes
• Using GAMA to probe the impact of small-scale galaxy physics on nonlinear redshift-space distortions
• HI intensity mapping correlation function from UNIT simulations: BAO and observationally induced anisotropy
• An analytic halo approach to the bispectrum of galaxies in redshift space
• SHAMe-SF: Predicting the clustering of star-forming galaxies with an enhanced abundance matching model
• 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
• How do galaxy properties affect void statistics?
• Higher multipoles of the galaxy bispectrum in redshift space
• Constraining Halo Occupation Distribution and Cosmic Growth Rate using Multipole Power Spectrum
• Sunyaev-Zel'dovich Signal from Quasar Hosts: Implications for Detection of Quasar Feedback
• Evolution of CIV Absorbers. II. Where does CIV live?
• Semi-Analytic Model Predictions of Mass Segregation from Groups to Clusters
• KiDS-1000: Weak lensing and intrinsic alignment around luminous red galaxies
• Combining spectroscopic and photometric surveys using angular cross-correlations III: Galaxy bias and stochastisity
• Shedding Light on Low Surface Brightness Galaxies in Dark Energy Survey with Transformers
• Late-formed halos prefer to host quiescent central galaxies. I. Observational results
• Weak Lensing Measurement of Filamentary Structure with the SDSS BOSS and Subaru Hyper Suprime-Cam Data
• Galaxy Clustering in the Mira-Titan Universe I: Emulators for the redshift space galaxy correlation function and galaxy-galaxy lensing
• Measuring the BAO peak position with different galaxy selections
• Galaxy and Mass Assembly (GAMA): Tracing galaxy environment using the marked correlation function
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Constraining the Galaxy-Halo Connection with Optimal Statistics
• Rapid Simulations of Halo and Subhalo Clustering
• Got plenty of nothing: cosmic voids as a probe of particle dark matter
• Biases to primordial non-Gaussianity measurements from CMB secondary anisotropies
• Subtracting the kinetic Sunyaev-Zeldovich effect from the cosmic microwave background with surveys of large-scale structure
• The DESI One-Percent Survey: Modelling the clustering and halo occupation of all four DESI tracers with Uchuu
• $\text{PineTree}$: A generative, fast, and differentiable halo model for wide-field galaxy surveys
• Investigating the galaxy-halo connection of DESI Emission-Line Galaxies with SHAMe-SF
• Constraints on primordial non-Gaussianity from WMAP7 and Luminous Red Galaxies power spectrum and forecast for future surveys
• A semi-analytical perspective on massive galaxies at $z\sim 0.55$
• Remapping simulated halo catalogues in redshift space
• Linking galaxies to dark matter haloes at $z\sim 1$ : dependence of galaxy clustering on stellar mass and specific star formation rate
• Challenges in Constraining Gravity with Cosmic Voids
• Weak lensing measurement of the mass-richness relation using the SDSS database
• Resolving the problem of galaxy clustering on small scales: any new physics needed?
• Constraints on dark matter and astrophysics from tomographic $\gamma$-ray cross-correlations
• Validating the clustering predictions of empirical models with the FLAMINGO 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
• The Impact of the Dusty Torus on Obscured Quasar Halo Mass Measurements
• Clustering and descendants of MUSYC galaxies at z<1.5
• Towards an accurate model of small-scale redshift-space distortions in modified gravity
• Cell Count Moments in the Halo Model
• Statistics of Two-point Correlation and Network Topology for Lyman Alpha Emitters at $z\approx 2.67$
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions and Lingering Tension
• Probing bursty star formation by cross-correlating extragalactic background light and galaxy surveys
• The XMM Cluster Survey: The Halo Occupation Number of BOSS galaxies in X-ray clusters
• Dark against luminous matter around isolated central galaxies: a comparative study between modern surveys and Illustris-TNG
• Fast generation of mock galaxy catalogues with COLA
• Angular clustering of z~2 star-forming and passive galaxies in 2.5 square degrees of deep CFHT imaging
• Nonlinear redshift space distortion in halo ellipticity correlations: Analytical model and N-body simulations
• The CIB-lensing bispectrum: impact on primordial non-Gaussianity and detectability for the Planck mission
• Dark Energy Survey Year 3 Results: Constraints on cosmological parameters and galaxy bias models from galaxy clustering and galaxy-galaxy lensing using the redMaGiC sample
• Galaxy populations in haloes in high-density environments
• Comparing Galaxy Clustering in Horizon-AGN Simulated Lightcone Mocks and VIDEO Observations
• Constraining galaxy-halo connection with high-order statistics
• Multi-wavelength consensus of large-scale linear bias
• Perturbation theory models for LSST-era galaxy clustering: tests with sub-percent mock catalog measurements in Fourier and configuration space
• What can we learn from higher multipole power spectra of galaxy distribution in redshift space?
• Self-calibrating optical galaxy cluster selection bias using cluster, galaxy, and shear cross-correlations
• KiDS-Legacy: Angular galaxy clustering from deep surveys with complex selection effects
• Accurate Modeling of the Projected Galaxy Clustering in Photometric Surveys: I. Tests with Mock Catalogs
• Growth and Geometry Split in Light of the DES-Y3 Survey
• Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
• Fast Forward Modelling of Galaxy Spatial and Statistical Distributions
• A pseudo-spectrum analysis of galaxy-galaxy lensing
• Gravitational Redshifts in Clusters and Voids
• Optical galaxy cluster mock catalogs with realistic projection effects: Validations with the SDSS clusters
• Observations of Ly$\alpha$ Emitters at High Redshift
• ScamPy -- A sub-halo clustering & abundance matching based Python interface for painting galaxies on the dark matter halo/sub-halo hierarchy
• The PAU Survey: Close galaxy pairs identification and analysis
• Towards Optimal Foreground Mitigation Strategies for Interferometric HI Intensity Mapping in the Low-Redshift Universe
• Methodological refinement of the submillimeter galaxy magnification bias. II. Cosmological analysis with tomography
• New insight into the variability of the Be star $\pi$ Aquarii: Determination of stellar and disk parameters
• Towards a Model-Independent Measurement of the Halo Mass Function with Observables
• Exploring the physical origins of halo assembly bias from early times
• Small scale clustering of BOSS galaxies: dependence on luminosity, color, age, stellar mass, specific star formation rate and other properties
• Cosmic star formation history with tomographic cosmic infrared background-galaxy cross-correlation
• Intrinsic mass-richness relation of clusters from THE THREE HUNDRED hydrodynamic simulations
• Improvement of cosmological constraints with the cross correlation between line-of-sight optical galaxy and FRB dispersion measure
• The miniJPAS survey. Evolution of the luminosity and stellar mass functions of galaxies up to $z\sim 0.7$
• Total and dark mass from observations of galaxy centers with Machine Learning
• Clustering environment of BL Lac object RGB 1745+398
• On the Constraints of Galaxy Assembly Bias in Velocity Space
• Clusters and Groups of Galaxies in the Simulated Local Universe
• The global energetics of radio AGN kinetic feedback in the local universe
• Cross-correlation between soft X-rays and galaxies A new benchmark for galaxy evolution models
• DESI Mock Challenge: Constructing DESI galaxy catalogues based on FastPM simulations
• Unraveling emission line galaxy conformity at z~1 with DESI early data
• Galaxy-galaxy lensing in the VOICE deep survey
• Non-Gaussian assembly bias from a semi-analytic galaxy formation model
• Correlation Analysis of Decaying Sterile Neutrino Dark Matter in the Context of the SRG Mission
• Peaks in the cosmological density field: parameter constraints from 2dF Galaxy Redshift Survey data
• Probabilistic Estimators of Lagrangian Shape Biases: Universal Relations and Physical Insights
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• Effect of Massive Neutrinos on the Position of Cold Dark Matter Halo: Revealed via Delaunay Triangulation Void
• Scaling of the 1-halo terms with bias
• Physical Processes Behind the Co-Evolution of Halos, Galaxies and Supermassive Black Holes in the IllustrisTNG Simulation
• Modeling spatially-resolved galactic H$\alpha$ emission for galaxy clustering
• How do uncertainties in galaxy formation physics impact field-level galaxy bias?
• Estimating lifetimes of uv-selected massive galaxies at $0.5\le z\le 2.5$ in the cosmos/ultravista field through clustering analyses
• On the accuracy of the high redshift cluster luminosity function
• Exploring HOD-dependent systematics for the DESI 2024 Full-Shape galaxy clustering analysis
• The Compactness of Galaxy Groups in the Sloan Digital Sky Survey
• Making use of sub-resolution halos in N-body simulations
• Evolution of the real-space correlation function from next generation cluster surveys
• Conditional Colour-Magnitude Distribution of Central Galaxies in Galaxy Formation Models
• Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• Detecting Relativistic Doppler in Galaxy Clustering with Tailored Galaxy Samples
• On the Clustering of Compact Galaxy Pairs in Dark Matter Haloes
• Inferring Host Dark Matter Halo Masses of Individual Galaxies from Neighboring Galaxy Counts
• More than just halo mass: Modelling how the red galaxy fraction depends on multiscale density in a HOD framework
• ELG$\times$LRG distribution through dark matter halo dynamics
• The Herschel-SPIRE Legacy Survey (HSLS): the scientific goals of a shallow and wide submillimeter imaging survey with SPIRE
• Cosmological gravity on all scales IV: 3x2pt Fisher forecasts for pixelised phenomenological modified gravity
• Testing Models of Quasar Hosts With Strong Gravitational Lensing by Quasar Hosts
• Measuring galaxy abundance and clustering at high redshift from incomplete spectroscopic data: Tests on mock catalogs
• The mass and galaxy distribution around SZ-selected clusters
• Cosmic Census: Relative Distributions of Dark Matter, Galaxies and Diffuse Gas
• Pulsar B1237+25 Aberration/Retardation Analysis from Decimeter to Decameter Wavelength: Challenge to "Radius-to-Frequency Mapping"
• Bounds on galaxy stochasticity from halo occupation distribution modeling
• Cosmic Insights from Galaxy Clusters: Exploring Magnification Bias on Sub-millimeter Galaxies
• 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
• The informativeness of [C II] line-intensity mapping as a probe of the H I content and metallicity of galaxies at the end of reionization
• A High-resolution Far-infrared Survey to Probe Black Hole-Galaxy Co-evolution
• The Influence of Subhaloes on Host Halo Properties
• Dark Energy Survey Year 3 results: Galaxy-halo connection from galaxy-galaxy lensing
• Toward accurate measurement of property-dependent galaxy clustering I. Comparison of the Vmax method and the "shuffled" method
• Detecting Relativistic Doppler by Multi-Tracing a Single Galaxy Population
• Probabilistic Lagrangian bias estimators and the cumulant bias expansion
• Preliminary clustering properties of the DESI BGS bright targets using DR9 Legacy Imaging Surveys
• Cosmic backgrounds from the radio to the far-infrared: recent results and perspectives from cosmological and astrophysical surveys
• Exploiting Non-linear Scales in Galaxy-Galaxy Lensing and Galaxy Clustering: A Forecast for the Dark Energy Survey
• Towards an optimal extraction of cosmological parameters from galaxy cluster surveys using convolutional neural networks
• Halo Merger Tree Comparison: Impact on Galaxy Formation Models
• Galaxy assembly bias in cosmological hydrodynamical simulations: a comparison between SIMBA and IllustrisTNG
• The VIMOS VLT Deep Survey. The different assembly history of passive and star-forming L_B >= L*_B galaxies in the group environment at z < 1
• One Galaxy Sample to Rule Them All: Halo Occupation Distribution Modeling of DES Year 3 Source Galaxies
• Cosmic magnification on high-redshift submillimeter galaxies
• The invariance of group occupation across the cosmic web
• Using two point correlation functions to understand the assembly histories of Milky Way-like galaxies
• Dark Matter and Galaxy Cross-Correlations with the Cherenkov Telescope Array Observatory
• HI Intensity Mapping cross-correlation with thermal SZ fluctuations: forecasted cosmological parameters estimation for FAST and Planck
• The multi-dimensional halo assembly bias can be preserved when enhancing halo properties with HALOSCOPE
• The mass and redshift dependence of halo star clustering
• Toward accurate measurement of property-dependent galaxy clustering: II. Tests of the smoothed density-corrected $V_{\max }$ method
• Predicting halo occupation and galaxy assembly bias with machine learning
• On the fairness of the main galaxy sample of SDSS
• Particle Physics in the Sky and Astrophysics Underground: Connecting the Universe's Largest and Smallest Scales
• Constraining Galaxy-Halo Connection Using Machine Learning
• Probing baryonic feedback with fast radio bursts: joint analyses with cosmic shear and galaxy clustering
• MIGHTEE: The dark matter haloes, duty cycle and mechanical feedback from radio-AGN up to $z\sim 2.5$
• Relativistic Angular Redshift Fluctuations embedded in Large Scale Varying Gravitational Potentials
• The impact of projection effects on cluster observables: stacked lensing and projected clustering
• A lightcone catalogue from the Millennium-XXL simulation: improved spatial interpolation and colour distributions for the DESI BGS
• NeutralUniverseMachine: Predictions of HI gas in Different Theoretical Models
• Cosmology from LOFAR Two-metre Sky Survey Data Release 2: Counts-in-Cells Statistics
• Skewness as a Probe of Gravity: Real and Redshift Space Counts-In-Cells
• Cosmology with the 6-degree Field Galaxy Survey
• An emulation-based model for the projected correlation function
• Axion-Like Particle Dark Matter Intensity Mapping: A New Probe via Cross-Correlation with Galaxy Surveys
• Cluster gravitational redshifts: uncertainties and survey requirements
• Correlation between Outlying Halo Abundance and Host Halo Properties
• A Non-parametric Method for the Inference of Halo Occupation Distributions
• Wiener filtering and multi-tracer techniques for dark matter cross-correlations between gamma-ray emission and galaxy catalogs
• Evidence for merging or disruption of red galaxies from the evolution of their clustering
• ELUCID-DESI I: A Parallel MPI Implementation of the Initial Condition Solver for Large-Scale Reconstruction Simulations
• The Hydrostatic Mass Bias and the ${\sigma }_8$ Tension: A Multi-Probe Forecast for Stage-IV/V Surveys
• Euclid: Improving redshift distribution reconstruction using a deep-to-wide transfer function