Galaxy Evolution from Halo Occupation Distribution Modeling of DEEP2 and SDSS Galaxy Clustering

Abstract

We model the luminosity-dependent projected two-point correlation function of DEEP2 (z~1) and SDSS (z~0) galaxies within the Halo Occupation Distribution (HOD) framework. At both epochs, there is a tight correlation between central galaxy luminosity and halo mass, with the slope and scatter decreasing for larger halo masses, and the fraction of satellite galaxies decreasing at higher luminosity. Central L* galaxies reside in halos a few times more massive at z~1 than at z~0. We find little evolution in the relation between mass scales of host halos for central galaxies and satellite galaxies above the same luminosity threshold. Combining these HOD results with theoretical predictions of the typical growth of halos, we establish an evolutionary connection between the galaxy populations at the two redshifts by linking z~0 central galaxies to z~1 central galaxies that reside in their progenitor halos, which enables us to study the evolution of galaxies as a function of halo mass. We find that the stellar mass growth of galaxies depends on halo mass. On average, the majority of the stellar mass in central galaxies residing in z~0 low mass halos (~5x10^11 Msun/h) and only a small fraction of the stellar mass in central galaxies of high mass halos (~10^13 Msun/h) result from star formation between z~1 and z~0. In addition, the mass scale of halos where the star formation efficiency reaches a maximum is found to shift toward lower mass with time. Future work can combine HOD modeling of the clustering of galaxies at different redshifts with the assembly history and dynamical evolution of dark matter halos. This can lead to an understanding of the stellar mass growth due to both mergers and star formation as a function of host halo mass and provide powerful tests of galaxy formation theories. (Abridged).

22 pages, 11 figures, minor changes to match the published version

References in corpus (122)

• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
• Stellar population synthesis at the resolution of 2003
• The Sloan Digital Sky Survey: Technical Summary
• A Universal Density Profile from Hierarchical Clustering
• Galactic Stellar and Substellar Initial Mass Function
• The Structure of Cold Dark Matter Halos
• On the variation of the Initial Mass Function
• Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
• Simulating the joint evolution of quasars, galaxies and their large-scale distribution
• Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
• Cosmological parameters from SDSS and WMAP
• The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies
• Large scale bias and the peak background split
• The 2.5 m Telescope of the Sloan Digital Sky Survey
• The 2dF Galaxy Redshift Survey: Spectra and redshifts
• Profiles of dark haloes: evolution, scatter, and environment
• The Optical and Near-Infrared Properties of Galaxies: I. Luminosity and Stellar Mass Functions
• Baryonic Features in the Matter Transfer Function
• High Redshift Galaxies in the Hubble Deep Field. Color Selection and Star Formation History to z=4
• Halo Models of Large Scale Structure
• Star Formation in AEGIS Field Galaxies since z=1.1 : The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-Forming Galaxies
• Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Main Galaxy Sample
• Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes
• Stellar mass-to-light ratios and the Tully-Fisher relation
• The Sloan Digital Sky Survey Photometric Camera
• Mass function of dark matter halos
• New Insight on Galaxy Formation and Evolution from Keck Spectroscopy of the Hawaii Deep Fields
• An analytic model for the spatial clustering of dark matter haloes
• NYU-VAGC: a galaxy catalog based on new public surveys
• Analytic model for galaxy and dark matter clustering
• The Galaxy Luminosity Function and Luminosity Density at Redshift z=0.1
• Simulations of X-ray Clusters
• Spectroscopic Target Selection for the Sloan Digital Sky Survey: The Luminous Red Galaxy Sample
• Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Quasar Sample
• Halo occupation numbers and galaxy bias
• The Dark Side of the Halo Occupation Distribution
• The Halo Occupation Distribution: Towards an Empirical Determination of the Relation Between Galaxies and Mass
• Theoretical Models of the Halo Occupation Distribution: Separating Central and Satellite Galaxies
• The Luminosity and Color Dependence of the Galaxy Correlation Function
• The 2dF Galaxy Redshift Survey: correlation functions, peculiar velocities and the matter density of the Universe
• Modeling Luminosity-Dependent Galaxy Clustering Through Cosmic Time
• Galaxy halo masses and satellite fractions from galaxy-galaxy lensing in the SDSS: stellar mass, luminosity, morphology, and environment dependencies
• Properties of Galaxy Groups in the SDSS: I.-- The Dependence of Colour, Star Formation, and Morphology on Halo Mass
• The age dependence of halo clustering
• How Many Galaxies Fit in a Halo? Constraints on Galaxy Formation Efficiency from Spatial Clustering
• Constraining Galaxy Formation and Cosmology with the Conditional Luminosity Function of Galaxies
• The Mass Assembly History of Field Galaxies: Detection of an Evolving Mass Limit for Star Forming Galaxies
• Linking halo mass to galaxy luminosity
• The Dependence of Halo Clustering on Halo Formation History, Concentration, and Occupation
• Estimating Fixed Frame Galaxy Magnitudes in the SDSS
• The Stellar, Gas and Dynamical Masses of Star-Forming Galaxies at z~2
• Science Objectives and Early Results of the DEEP2 Redshift Survey
• K-band Properties of Galaxy Clusters and Groups: Brightest Cluster Galaxies and Intracluster Light
• The Complete Star Formation History of the Universe
• The Effects of Photoionization on Galaxy Formation - I: Model and Results at z=0
• Star formation in AEGIS field galaxies since z=1.1 . Staged galaxy formation, and a model of mass-dependent gas exhaustion
• Spatial correlation function and pairwise velocity dispersion of galaxies: CDM models versus the Las Campanas Survey
• A catalogue of the Chandra Deep Field South with multi-colour classification and photometric redshifts from COMBO-17
• H-alpha Observations of a Large Sample of Galaxies at z~2: Implications for Star Formation in High Redshift Galaxies
• On the Mass-to-Light Ratio of Large Scale Structure
• The DEEP2 Galaxy Redshift Survey: The Galaxy Luminosity Function to z ~ 1
• Assembly bias in the clustering of dark matter haloes
• Percolation Galaxy Groups and Clusters in the SDSS Redshift Survey: Identification, Catalogs, and the Multiplicity Function
• The Physics of Galaxy Clustering I: A Model for Subhalo Populations
• Cosmic Star Formation History and its Dependence on Galaxy Stellar Mass
• Deriving the Nonlinear Cosmological Power Spectrum and Bispectrum from Analytic Dark Matter Halo Profiles and Mass Functions
• The Spatial Clustering of Star-forming Galaxies at Redshifts 1.4<z<3.5
• Halo assembly bias and its effects on galaxy clustering
• New Relationships between Galaxy Properties and Host Halo Mass, and the Role of Feedbacks in Galaxy Formation
• On Departures From a Power Law in the Galaxy Correlation Function
• The star formation histories of galaxies in the Sloan Digital Sky Survey
• The stellar masses of 25000 galaxies at 0.2<z<1.0 estimated by the COMBO-17 survey
• Mass downsizing and "top-down" assembly of early-type galaxies
• The Non-Parametric Model for Linking Galaxy Luminosity with Halo/Subhalo Mass
• The Radial Distribution of Galaxies in LCDM clusters
• Linking Early and Late Type Galaxies to their Dark Matter Haloes
• A marked correlation function analysis of halo formation times in the Millennium Simulation
• PINOCCHIO: pinpointing orbit-crossing collapsed hierarchical objects in a linear density field
• The Dynamics of Sinking Satellites Around Disk Galaxies: A Poor Man's Alternative to High-Resolution Numerical Simulations
• The I-Band Tully-Fisher Relation for Cluster Galaxies: a Template Relation, its Scatter and Bias Corrections
• Subaru Deep Survey VI. A Census of Lyman Break Galaxies at z=4 and 5 in the Subaru Deep Fields: Clustering Properties
• Potential sources of contamination to weak lensing measurements: constraints from N-body simulations
• Redshift evolution of clustering
• The dependence of dark halo clustering on the formation epoch and the concentration parameter
• The Large-scale and Small-scale Clustering of Lyman-Break Galaxies at 3.5 < z< 5.5 from the GOODS survey
• The dependence of Star Formation on Galaxy Stellar Mass
• Halo Model at Its Best: Constraints on Conditional Luminosity Functions from Measured Galaxy Statistics
• The Evolution of Substructure in Galaxy, Group and Cluster Haloes I: Basic Dynamics
• Galaxy Halo Occupation at High Redshift
• Galaxy Occupation Statistics of Dark Matter Haloes: Observational Results
• The DEEP2 Galaxy Redshift Survey: First results on galaxy groups
• Definitive Identification of the Transition between Small- to Large-Scale Clustering for Lyman Break Galaxies
• The DEEP2 Galaxy Redshift Survey: Clustering of Galaxies as a Function of Luminosity at z=1
• Modelling galaxy clustering at high redshift
• The DEEP2 Galaxy Redshift Survey: Clustering of Quasars and Galaxies at z=1
• Radial distribution and strong lensing statistics of satellite galaxies and substructure using high resolution LCDM hydrodynamical simulations
• Detection of strong clustering of red K-selected galaxies at 2<z_phot<4 in the Hubble Deep Field South
• The Clustering of Massive Halos
• Interpreting the Observed Clustering of Red Galaxies at z~3
• The Halo Distribution of 2dF Galaxies
• Cosmology and the Halo Occupation Distribution from Small-Scale Galaxy Clustering in the Sloan Digital Sky Survey
• The Dependence of the Occupation of Galaxies on the Halo Formation Time
• On The Assembly History of Dark Matter Haloes
• Predicting the number, spatial distribution and merging history of dark matter haloes
• The Three-point Correlation Function of Galaxies Determined from the Las Campanas Redshift Survey
• Preheating by Previrialization and its Impact on Galaxy Formation
• The Masses, Ancestors and Descendents of Extremely Red Objects: Constraints from Spatial Clustering
• Cluster Merger Variance and the Luminosity Gap Statistic
• Baryonic Conversion Tree: The global assembly of stars and dark matter in galaxies from the SDSS
• Constraining evolution in the Halo Model using galaxy redshift surveys
• Spatial correlation functions and the pairwise peculiar velocity dispersion of galaxies in the PSCz survey: implications for the galaxy biasing in cold dark matter models
• The DEEP2 Galaxy Redshift Survey: Clustering of Groups and Group Galaxies at z~1
• PINOCCHIO and the hierarchical build-up of dark matter haloes
• Dissipationless Merging and the Assembly of Central Galaxies
• A Realistic Model for Spatial and Mass Distributions of Dark Halo Substructures: An Analytic Approach
• A Brighter Past: Galaxy Luminosity Function At High Redshifts
• Mock Catalogs for the DEEP2 redshift survey
• Strong Spatial Clustering of UV-selected Galaxies with Magnitude Ks<20.5 and Redshift Z~2
• The Oxford-Dartmouth Thirty Degree Survey II: Clustering of Bright Lyman Break Galaxies - Strong Luminosity Dependent Bias at z=4
• Where are the z=4 Lyman Break Galaxies? Results from Conditional Luminosity Function Models of Luminosity-dependent Correlation Functions
• Masses of high-z galaxy hosting haloes from angular clustering and their evolution in the CDM model
• GaBoDS: The Garching-Bonn Deep Survey - III. Lyman-Break Galaxies in the Chandra Deep Field South

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• Illustrating galaxy-halo connection in the DESI era with IllustrisTNG
• The Unchanging Circumgalactic Medium Over the Past 11 Billion Years
• ADDGALS: Simulated Sky Catalogs for Wide Field Galaxy Surveys
• Shot noise and biased tracers: a new look at the halo model
• Tomographic Magnification of Lyman Break Galaxies in The Deep Lens Survey
• The central dark matter content of early-type galaxies: scaling relations and connections with star formation histories
• Hierarchical Galaxy Growth and Scatter in the Stellar Mass - Halo Mass Relation
• Large Scale Structure of the Universe
• Constraining Satellite Galaxy Stellar Mass Loss and Predicting Intrahalo Light I: Framework and Results at Low Redshift
• 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
• 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
• Updated Results on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• The Redshift-Space Momentum Power Spectrum I: Optimal Estimation From Peculiar Velocity Surveys
• The Incomplete Conditional Stellar Mass Function: Unveiling the Stellar Mass Functions of Galaxies at 0.1 < Z < 0.8 from BOSS Observations
• Modeling the Very Small-Scale Clustering of Luminous Red Galaxies
• The progenitors of present-day massive red galaxies up to z ~ 0.7 - finding passive galaxies using SDSS-I/II and SDSS-III
• The Atacama Cosmology Telescope DR6 and DESI: Structure formation over cosmic time with a measurement of the cross-correlation of CMB Lensing and Luminous Red Galaxies
• LOFAR observations of the XMM-LSS field
• The clustering of X-ray selected AGN at z=0.1
• Priors on red galaxy stochasticity from hybrid effective field theory
• Clustering of X-Ray-Selected AGN
• Spatial clustering and halo occupation distribution modeling of local AGN via cross-correlation measurements with 2MASS galaxies
• HectoMAP and Horizon Run 4: Dense Structures and Voids in the Real and Simulated Universe
• Galaxy downsizing evidenced by hybrid evolutionary tracks
• Constraints on $S_8$ from a full-scale and full-shape analysis of redshift-space clustering and galaxy-galaxy lensing in BOSS
• Does the Galaxy-Halo Connection Vary with Environment?
• Evolution of the Clustering of Photometrically Selected SDSS Galaxies
• A scaling relation between merger rate of galaxies and their close pair count
• How are galaxies assigned to halos? Searching for assembly bias in the SDSS galaxy clustering
• Testing the Accuracy of Halo Occupation Distribution Modelling using Hydrodynamic Simulations
• The 6dF Galaxy Survey: Dependence of halo occupation on stellar mass
• A Zeldovich reconstruction method for measuring redshift space distortions using cosmic voids
• Modeling the JWST high-redshift galaxies with a general formation scenario and the consistency with the $\Lambda$CDM model
• Dark matter halos and scaling relations of extremely massive spiral galaxies from extended HI rotation curves
• The Conditional Colour-Magnitude Distribution: I. A Comprehensive Model of the Colour-Magnitude-Halo Mass Distribution of Present-Day Galaxies
• The Most Bound Halo Particle-Galaxy Correspondence Model: Comparison between Models with Different Merger Timescales
• The VIMOS-VLT Deep Survey: Evolution in the Halo Occupation Number since z $\sim$ 1
• Probing Galaxy Assembly Bias in BOSS Galaxies Using Void Probabilities
• Precise Cosmological Constraints from BOSS Galaxy Clustering with a Simulation-Based Emulator of the Wavelet Scattering Transform
• 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
• Projected-Field Kinetic Sunyaev-Zel'dovich Cross-Correlations: Halo Model and Forecasts
• Galaxy clustering and projected density profiles as traced by satellites in photometric surveys: Methodology and luminosity dependence
• $\mathrm{S}\mathrm{IM}\mathrm{BIG}$: Mock Challenge for a Forward Modeling Approach to Galaxy Clustering
• Unbound Particles in Dark Matter Halos
• The VIMOS Ultra Deep Survey. Luminosity and stellar mass dependence of galaxy clustering at z~3
• Small-scale galaxy clustering in the EAGLE simulation
• The Gravitational Lensing Signatures of BOSS Voids in the Cosmic Microwave Background
• How to Optimally Constrain Galaxy Assembly Bias: Supplement Projected Correlation Functions with Count-in-cells Statistics
• A Parameter-Masked Mock Data Challenge for Beyond-Two-Point Galaxy Clustering Statistics
• Brightest galaxies as halo centre tracers in SDSS DR7
• Cosmological Evidence Modelling: a new simulation-based approach to constrain cosmology on non-linear scales
• Relative clustering and the joint halo occupation distribution of red-sequence and blue-cloud galaxies in COMBO-17
• An observational proxy of halo assembly time and its correlation with galaxy properties
• The dependence of galaxy clustering on tidal environment in the Sloan Digital Sky Survey
• The evolution of the galaxy content of dark matter haloes
• A Kennicutt-Schmidt Law for Intervening Absorption Line Systems
• What determines large scale galaxy clustering: halo mass or local density?
• The MillenniumTNG Project: Inferring cosmology from galaxy clustering with accelerated N-body scaling and subhalo abundance matching
• Cosmological Information in Skew Spectra of Biased Tracers in Redshift Space
• The cosmic web of X-ray active galactic nuclei seen through the eROSITA Final Equatorial Depth Survey (eFEDS)
• Are the halo occupation predictions consistent with large scale galaxy clustering?
• Composition of Low Redshift Halo Gas
• $\text{matryoshka}$: Halo Model Emulator for the Galaxy Power Spectrum
• Understanding the nature of luminous red galaxies (LRGs): Connecting LRGs to central and satellite subhalos
• 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
• Probing the galaxy-halo connection with total satellite luminosity
• Void profile from Planck lensing potential map
• A Subhalo-Galaxy Correspondence Model of Galaxy Formation
• An improved limit on the neutrino mass with CMB and redshift-dependent halo bias-mass relations from SDSS, DEEP2, and Lyman-Break Galaxies
• Tracing the gravitational potential using cosmic voids
• Dissecting the roles of mass and environment quenching in galaxy evolution with EAGLE
• Why are AGN found in High Mass Galaxies?
• The Halo Void (Dust) Model of Large Scale Structure
• Precision Redshift-Space Galaxy Power Spectra using Zel'dovich Control Variates
• The Effective Field Theory of Large-Scale Structure and Multi-tracer
• The dark side of galaxy stellar populations I: The stellar-to-halo mass relation and the velocity dispersion - halo mass relation
• From starburst to quiescence: post-starburst galaxies and their large-scale clustering over cosmic time
• The Galaxy Cross-Correlation Function as a Probe of the Spatial Distribution of Galactic Satellites
• Evidence of Galaxy Assembly Bias in SDSS DR7 Galaxy Samples from Count Statistics
• Massive Dark Matter Halos at High Redshift: Implications for Observations in the JWST Era
• Linear bias and halo occupation distribution of emission line galaxies from Nancy Grace Roman Space Telescope
• An empirical prediction for stellar metallicity distributions in nearby galaxies
• Magnitude Gap Statistics and the Conditional Luminosity Function
• Reconstructing the baryon acoustic oscillations using biased tracers
• Detection of thermal Sunyaev-Zel'dovich Effect in the circumgalactic medium of low-mass galaxies -- a surprising pattern in self-similarity and baryon sufficiency
• Construct the emission line galaxy-host halo connection through auto and cross correlations
• TARDIS Paper II: Synergistic Density Reconstruction from Lyman-alpha Forest and Spectroscopic Galaxy Surveys with Applications to Protoclusters and the Cosmic Web
• Crawling the Cosmic Network: Exploring the Morphology of Structure in the Galaxy Distribution
• Host Dark Matter Halos of WISE-selected Obscured & Unobscured Quasars: Evidence for Evolution
• Stellar Mass and color dependence of the three-point correlation function of galaxies in the local universe
• The nonlinear biasing of the 10k zCOSMOS galaxies up to z~1
• The Formation History of Subhalos and the Evolution of Satellite Galaxies
• The clustering of $z>7$ galaxies: Predictions from the BLUETIDES simulation
• [OII] emitters in MultiDark-Galaxies and DEEP2
• Probing massive neutrinos with the Minkowski functionals of the galaxy distribution
• An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies
• HOD-Dependent Systematics in Emission Line Galaxies for the DESI 2024 BAO analysis
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• The Evolution of K* and the Halo Occupation Distribution since z=1.5: Observations vs. Simulations
• Subhaloes gone Notts: the clustering properties of subhaloes
• On the mass assembly of low-mass galaxies in hydrodynamical simulations of structure formation
• Passive Evolution of Galaxy Clustering
• The distribution of faint satellites around central galaxies in the CFHT Legacy Survey
• The very wide-field $gzK$ galaxy survey -- I. Details of the clustering properties of star-forming galaxies at $z\sim 2$
• Extending Recovery of the Primordial Matter Power Spectrum
• An Imaging and Spectroscopic Study of Four Strong MgII Absorbers Revealed By GRB060418
• Studying large-scale structure probes of modified gravity with COLA
• Fast generation of mock galaxy catalogues in modified gravity models with COLA
• Improved Mock Galaxy Catalogs for the DEEP2 Galaxy Redshift Survey from Subhalo Abundance and Environment Matching
• The Imperial IRAS-FSC Redshift Catalogue: luminosity functions, evolution and galaxy bias
• On the Clustering of Faint Red Galaxies
• Cosmological Constraints from applying SHAM to rescaled cosmological simulations
• The Halo Occupation Distribution of Obscured Quasars: Revisiting the Unification Model
• Velocity reconstruction in the era of DESI and Rubin (part I): Exploring spectroscopic, photometric & hybrid samples
• Building a Better Understanding of the High Redshift BOSS Galaxies as Tools for Cosmology
• Using member galaxy luminosities as halo mass proxies of galaxy groups
• Cosmic Reionization On Computers: The Galaxy-Halo Connection between $5\le z\le 10$
• Modeling Redshift-Space Clustering with Abundance Matching
• Angular clustering and host halo properties of [OII] emitters at $z>1$ in the Subaru HSC survey
• Testing Dark Matter Halo Models of Quasars With Thermal Sunyaev-Zeldovich Effect
• Full forward model of galaxy clustering statistics with AbacusSummit lightcones
• Cosmology with Persistent Homology: a Fisher Forecast
• HOD-Dependent Systematics for Luminous Red Galaxies in the DESI 2024 BAO Analysis
• Clustering dependence on Lyman-$\alpha$ luminosity from MUSE surveys at $3<z<6$
• The Chandra COSMOS Legacy Survey: clustering dependence of Type 2 AGN on host galaxy properties
• On the Redshift Evolution of MgII Absorption Systems
• Brightest group galaxies-II: the relative contribution of BGGs to the total baryon content of groups at z<1.3
• The Differing Relationships Between Size, Mass, Metallicity and Core Velocity Dispersion of Central and Satellite Galaxies
• Hubble Space Telescope Images of Red Mergers: How Dry are They?
• Do galaxy mergers prefer under-dense environments?
• Constraining the galaxy-halo connection of infrared-selected unWISE galaxies with galaxy clustering and galaxy-CMB lensing power spectra
• 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 $z<0.7$
• Galaxy Three-Point Correlation Functions and Halo/Subhalo Models
• 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
• The strong environmental dependence of black hole scaling relations
• A Halo Occupation Interpretation Of Quasars At $z\sim 1.5$ Using Very Small Scale Clustering Information
• Using galaxy pairs to investigate the three-point correlation function in the squeezed limit
• Tracing the galaxy-halo connection with galaxy clustering in COSMOS-Web from z = 0.1 to z ~ 12
• On the small scale clustering of quasars: constraints from the MassiveBlack II simulation
• The spatial clustering of ROSAT all-sky survey Active Galactic Nuclei: V. The evolution of broad-line AGN clustering properties in the last 6 Gyr
• The Clustering of Extremely Red Objects
• The Halo Occupation Distribution of Black Holes: Dependence on Mass
• Extracting high-order cosmological information in galaxy surveys with power spectra
• MEDUSA: Minkowski functionals estimated from Delaunay tessellations of the three-dimensional large-scale structure
• 2D k-th nearest neighbor statistics: a highly informative probe of galaxy clustering
• Probing gravity with redshift-space distortions: effects of tracer bias and sample selection
• The MUSE-Wide survey: Three-dimensional clustering analysis of Lyman-$\alpha$ emitters at $3.3<z<6$
• SHAMe-SF: Predicting the clustering of star-forming galaxies with an enhanced abundance matching model
• Robustness of the pairwise kinematic Sunyaev-Zeldovich power spectrum shape as a cosmological gravity probe
• The association between gas and galaxies III: The Cross-correlation of Galaxies and Ly-alpha Absorbers at z ~ 1
• Halo Occupation Distribution of Emission Line Galaxies: fitting method with Gaussian Processes
• 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 XMM-Newton Wide Field Survey in the COSMOS Field: Clustering Dependence of X-ray Selected AGN on Host Galaxy Properties
• The Beyond-Halo Mass Effects of the Cosmic Web Environment on Galaxies
• 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
• Relating galaxies across different redshift to study galaxy evolution
• New Statistical Perspective to The Cosmic Void Distribution
• Got plenty of nothing: cosmic voids as a probe of particle dark matter
• Linking galaxies to dark matter haloes at $z\sim 1$ : dependence of galaxy clustering on stellar mass and specific star formation rate
• Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic survey. II. Morphology, Color and Size Dependences of the Stellar-halo Mass Relation for Massive Galaxies
• Investigating the galaxy-halo connection of DESI Emission-Line Galaxies with SHAMe-SF
• Cold Gas in Massive Galaxies as A Critical Test of Black Hole Feedback Models
• The Circumgalactic Medium in Massive Halos
• Cell Count Moments in the Halo Model
• Global analysis of luminosity- and colour-dependent galaxy clustering in the Sloan Digital Sky Survey
• An Empirical Model For Intrinsic Alignments: Insights From Cosmological Simulations
• A semi-analytic model of pairwise velocity distribution between dark matter halos
• Challenges in Constraining Gravity with Cosmic Voids
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions and Lingering Tension
• Validating the clustering predictions of empirical models with the FLAMINGO simulations
• The XMM Cluster Survey: The Halo Occupation Number of BOSS galaxies in X-ray clusters
• 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
• Clustering and descendants of MUSYC galaxies at z<1.5
• Selecting samples of galaxies with fewer Fingers-of-God
• Constraining galaxy-halo connection with high-order statistics
• Cross-Correlation Forecast of CSST Spectroscopic Galaxy and MeerKAT Neutral Hydrogen Intensity Mapping Surveys
• Towards an optimal marked correlation function analysis for the detection of modified gravity
• The dependence of cluster galaxy properties on the central entropy of their host cluster
• The Evolution of Early-type Galaxies Selected by Their Spatial Clustering
• Investigating the Dark Matter Halo of NGC 5128 using a Discrete Dynamical Model
• Tests of Acoustic Scale Shifts in Halo-based Mock Galaxy Catalogues
• PRIMUS: The Effect of Physical Scale on the Luminosity-Dependence of Galaxy Clustering via Cross-Correlations
• HI HOD -- I. The Halo Occupation Distribution of HI Galaxies
• Generalized framework for likelihood-based field-level inference of growth rate from velocity and density fields
• A new test of gravity -- I: Introduction to the method
• Clustering, Cosmology and a New Era of Black Hole Demographics -- I. The Conditional Luminosity Function of Active Galactic Nuclei
• Accurate Modeling of the Projected Galaxy Clustering in Photometric Surveys: I. Tests with Mock Catalogs
• New insight into the variability of the Be star $\pi$ Aquarii: Determination of stellar and disk parameters
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• ScamPy -- A sub-halo clustering & abundance matching based Python interface for painting galaxies on the dark matter halo/sub-halo hierarchy
• Small scale clustering of BOSS galaxies: dependence on luminosity, color, age, stellar mass, specific star formation rate and other properties
• Towards a Model-Independent Measurement of the Halo Mass Function with Observables
• Exploring the physical origins of halo assembly bias from early times
• Fitting functions for a disk-galaxy model with different LCDM-halo profiles
• The environments of the radio galaxy population in SIMBA
• Cross-correlation between soft X-rays and galaxies A new benchmark for galaxy evolution models
• The H$\alpha$ luminosity and stellar mass dependent clustering of star-forming galaxies at $0.7<z<1.5$ with 3D-HST
• Unraveling emission line galaxy conformity at z~1 with DESI early data
• A Large Massive Quiescent Galaxy Sample at z~1.2
• Exploring HOD-dependent systematics for the DESI 2024 Full-Shape galaxy clustering analysis
• Modeling spatially-resolved galactic H$\alpha$ emission for galaxy clustering
• Breaking the ${\tau }_{\mathrm{T}}-f$ degeneracy of the kinetic Sunyaev Zel'dovich cosmology in redshift space
• The contribution of faint Lyman-$\alpha$ emitters to extended Lyman-$\alpha$ halos constrained by MUSE clustering measurements
• Scaling of the 1-halo terms with bias
• Estimating lifetimes of uv-selected massive galaxies at $0.5\le z\le 2.5$ in the cosmos/ultravista field through clustering analyses
• Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation
• The smearing scale in Laguerre reconstructions of the correlation function
• The impact of AGN X-ray selection on the AGN halo occupation distribution
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• Decorrelating the errors of the galaxy correlation function with compact transformation matrices
• Lognormal Distribution of Cosmic Voids in Simulations and Mocks
• Pulsar B1237+25 Aberration/Retardation Analysis from Decimeter to Decameter Wavelength: Challenge to "Radius-to-Frequency Mapping"
• ELG$\times$LRG distribution through dark matter halo dynamics
• BASILISK II. Improved Constraints on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• On the Clustering of Compact Galaxy Pairs in Dark Matter Haloes
• CLIMBER: Galaxy-Halo Connection Constraints from Next-Generation Surveys
• Dark Energy Survey Year 3 results: Galaxy-halo connection from galaxy-galaxy lensing
• Studying baryon acoustic oscillations using photometric redshifts from the DESI Legacy Imaging survey DR9
• Bounds on galaxy stochasticity from halo occupation distribution modeling
• Atomic Hydrogen Shows its True Colours: Correlations between HI and Galaxy Colour in Simulations
• Cosmological parameters from the joint analysis of Density Split and Second Order Statistics: an Emulator based on the Halo Occupation Distribution
• Constraining galactic baryon cycle using the galaxy stellar-to-halo mass relations
• Improving the Accuracy of Halo Mass Based Statistics For Fast Approximate N-body Simulations
• Adaptive friends-of-friends algorithm for identifying gravitationally bound cosmological structures
• A novel analysis of contamination in Lyman-break galaxy samples at $\mathbf{z}\sim 6-8$: spatial correlation with intermediate-redshift galaxies at $\mathbf{z}\sim 1.3-2$
• Constraining Galaxy-Halo Connection Using Machine Learning
• Galaxies in X-ray Selected Clusters and Groups in Dark Energy Survey Data II: Hierarchical Bayesian Modeling of the Red-Sequence Galaxy Luminosity Function
• Dark matter in ALFALFA galaxies: Investigating galaxy-halo connection
• Dark matter halos of luminous AGNs from galaxy-galaxy lensing with the HSC Subaru Strategic Program
• Cosmological implications of the full shape of anisotropic clustering measurements in BOSS and eBOSS
• Probing the large-scale structure with 21cm-galaxy cross-bispectrum: Estimates from simulations and forecasts for upcoming cosmological surveys
• Cluster gravitational redshifts: uncertainties and survey requirements
• A Non-parametric Method for the Inference of Halo Occupation Distributions
• Emulating galaxy and peculiar velocity clustering on non-linear scales
• Spatially resolved stellar-to-total dynamical mass relation: Radial variations, gradients and profiles of galaxy stellar populations
• Marked statistics across the cosmic web: Environmental dependent clustering in modified gravity simulations
• Clustering analysis of medium-band selected high-redshift galaxies
• On the range of validity of perturbative models for galaxy clustering and its uncertainty
• Void probability function in the Quijote simulations