The Luminosity and Color Dependence of the Galaxy Correlation Function

Abstract

We study the luminosity and color dependence of the galaxy 2-point correlation function in the Sloan Digital Sky Survey, starting from a sample of 200,000 galaxies over 2500 deg^2. We concentrate on the projected correlation function w(r_p), which is directly related to the real space ξ(r). The amplitude of w(r_p) grows continuously with luminosity, rising more steeply above the characteristic luminosity L_*. Redder galaxies exhibit a higher amplitude and steeper correlation function at all luminosities. The correlation amplitude of blue galaxies increases continuously with luminosity, but the luminosity dependence for red galaxies is less regular, with bright red galaxies more strongly clustered at large scales and faint red galaxies more strongly clustered at small scales. We interpret these results using halo occupation distribution (HOD) models assuming concordance cosmological parameters. For most samples, an HOD model with two adjustable parameters fits the w(r_p) data better than a power-law, explaining inflections at r_p ~ 1-3 Mpc/h as the transition between the 1-halo and 2-halo regimes of ξ(r). The implied minimum mass for a halo hosting a central galaxy above a luminosity threshold L grows as M_min ~ L at low luminosities and more steeply above L_*. The mass at which an average halo has one satellite galaxy brighter than L is M_1 ~ 23 M_min(L). These results imply a conditional luminosity function (at fixed halo mass) in which central galaxies lie far above a Schechter function extrapolation of the satellite population. HOD models nicely explain the joint luminosity-color dependence of w(r_p) in terms of the color fractions of central and satellite populations as a function of halo mass. The inferred HOD properties are in good qualitative agreement with theoretical predictions.

64 pages, 24 figures. Minor changes to match accepted ApJ version

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• Luminosity function of galaxies in groups in the SDSS DR7: the dependence on mass, environment and galaxy type
• A New Halo Finding Method for N-Body Simulations
• A Cosmic Coincidence: The Power-Law Galaxy Correlation Function
• The halo-model description of marked statistics
• TheHaloMod: An online calculator for the halo model
• Clustering of quasars in a wide luminosity range at redshift 4 with Subaru Hyper Suprime-Cam wide field imaging
• PRIMUS+DEEP2: The Dependence of Galaxy Clustering on Stellar Mass and Specific Star Formation Rate at 0.2 < z < 1.2
• The dependence of halo bias on age, concentration and spin
• Galaxy filaments as pearl necklaces
• Effects of Gravitational Evolution, Biasing, and Redshift Space Distortion on Topology
• Systematic effects in the sound horizon scale measurements
• Dark Energy Survey Year 1 Results: Methodology and Projections for Joint Analysis of Galaxy Clustering, Galaxy Lensing, and CMB Lensing Two-point Functions
• A Brighter Past: Galaxy Luminosity Function At High Redshifts
• Properties of Dark Matter Haloes and their Correlations: the Lesson from Principal Component Analysis
• The DEEP2 Galaxy Redshift Survey: The Evolution of Void Statistics from z~1 to z~0
• Clustering properties of a type-selected volume-limited sample of galaxies in the CFHTLS
• The evolution of galaxy clustering since z = 3 using the UKIDSS Ultra Deep Survey: the divergence of passive and star-forming galaxies
• The spatial clustering of ROSAT All-Sky Survey Active Galactic Nuclei IV. More massive black holes reside in more massive dark matter halos
• Exploring the squeezed three-point galaxy correlation function with generalized halo occupation distribution models
• The Stellar Mass Components of Galaxies: Comparing Semi-Analytical Models with Observation
• Towards understanding the structure of voids in the cosmic web
• Complete Treatment of Galaxy Two-Point Statistics: Gravitational Lensing Effects and Redshift-Space Distortions
• Absence of anti-correlations and of baryon acoustic oscillations in the galaxy correlation function from the Sloan Digital Sky Survey DR7
• The manifestation of secondary halo bias on the galaxy population from IllustrisTNG300
• Constraints on the merging timescale of luminous red galaxies, or, where do all the halos go?
• Constraints on the redshift evolution of astrophysical feedback with Sunyaev-Zeldovich effect cross-correlations
• The Strikingly Similar Relation between Satellite and Central Galaxies and Their Dark Matter Halos Since z=2
• Elucidating Galaxy Assembly Bias in SDSS
• Environmental Effects on Real-Space and Redshift-Space Galaxy Clustering
• The evolution of clustering length, large-scale bias and host halo mass at 2<z<5 in the VIMOS Ultra Deep Survey (VUDS)
• Angular correlation function of 1.5 million LRGs: clustering evolution and a search for BAO
• Precision Measurements of the Cluster Red Sequence using an Error Corrected Gaussian Mixture Model
• Cosmic voids: a novel probe to shed light on our Universe
• Modelling The Redshift-Space Three-Point Correlation Function in SDSS-III
• Dark Energy Survey Year 3 Results: Exploiting small-scale information with lensing shear ratios
• Mapping the allowed parameter space for decaying dark matter models
• The clustering and evolution of H-alpha emitters at z~1 from HiZELS
• Optimal linear reconstruction of dark matter from halo catalogs
• Revealing components of the galaxy population through nonparametric techniques
• Near-Infrared Properties of Moderate-Redshift Galaxy Clusters: Halo Occupation Number, Mass-to-Light Ratios and Omega_m
• The spectral-type/luminosity and the spectral type/satellite-density relations in the 2dFGRS
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): An unbiased estimate of the growth rate of structure at $⟨\mathbf{z}⟩=0.85$ using the clustering of luminous blue galaxies
• The Halo Occupation Distribution of Active Galactic Nuclei
• Satellite Galaxy Number Density Profiles in the Sloan Digital Sky Survey
• Testing one-loop galaxy bias: Power spectrum
• The Luminosity, Colour and Morphology dependence of galaxy filaments in the Sloan Digital Sky Survey Data Release Four
• Neutrino mass without cosmic variance
• A tale of two populations: the stellar mass of central and satellite galaxies
• The H-alpha luminosity-dependent clustering of star-forming galaxies from z~0.8 to z~2.2 with HiZELS
• Measuring Redshift-Space Distortions using Photometric Surveys
• Cosmology with Equivalence Principle Breaking in the Dark Sector
• The effects of assembly bias on cosmological inference from galaxy-galaxy lensing and galaxy clusters
• The Immitigable Nature of Assembly Bias: The Impact of Halo Definition on Assembly Bias
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Pairwise-Inverse-Probability and Angular Correction for Fibre Collisions in Clustering Measurements
• Satellite Luminosities in Galaxy Groups
• Major Cluster Mergers and the Location of the Brightest Cluster Galaxy
• Exploring galaxy colour in different environments of the cosmic web with SDSS
• Differences in the AGN Populations of Groups and Clusters: Clues to AGN Evolution
• On the evolution of clustering of 24um-selected galaxies
• The Large-Scale Environments of Type Ia Supernovae: Evidence for a Metallicity Bias in the Rate or Luminosity of Prompt Ia Events
• Large Scale Structure of the Universe
• The VIPERS Multi-Lambda Survey. I. UV and NIR Observations, multi-color catalogues and photometric redshifts
• Environment and the cosmic evolution of star formation
• Exploring the halo occupation of AGN using dark-matter cosmological simulations
• Updated Results on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• The dependence of galaxy clustering on stellar mass, star-formation rate and redshift at z = 0.8-2.2, with HiZELS
• The Environment of Galaxies at Low Redshift
• Internal kinematics of groups of galaxies in the Sloan Digital Sky Survey data release 7
• Probing the Radio Loud/Quiet AGN dichotomy with quasar clustering
• 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
• BAM: Bias Assignment Method to generate mock catalogs
• The dependence of the pairwise velocity dispersion on galaxy properties
• DES Y1 Results: Validating cosmological parameter estimation using simulated Dark Energy Surveys
• The spatial distribution of cold gas in hierarchical galaxy formation models
• Cosmic Voids and Galaxy Bias in the Halo Occupation Framework
• The progenitors of present-day massive red galaxies up to z ~ 0.7 - finding passive galaxies using SDSS-I/II and SDSS-III
• The clustering of X-ray selected AGN at z=0.1
• Breaking the self-averaging properties of spatial galaxy fluctuations in the Sloan Digital Sky Survey - Data Release Six
• Mid-Infrared Galaxy Luminosity Functions from the AGN and Galaxy Evolution Survey
• How much a galaxy knows about its large-scale environment?: An information theoretic perspective
• X-ray selected AGN in groups at redshifts z~1
• Correcting for Fibre Assignment Incompleteness in the DESI Bright Galaxy Survey
• The Low-Redshift Lyman Alpha Forest toward PKS 0405-123
• Spatial clustering and halo occupation distribution modeling of local AGN via cross-correlation measurements with 2MASS galaxies
• Evolution of the Clustering of Photometrically Selected SDSS Galaxies
• Does the Galaxy-Halo Connection Vary with Environment?
• The High-Mass End of the Red Sequence at z~0.55 from SDSS-III/BOSS: completeness, bimodality and luminosity function
• Deep Realistic Extragalactic Model (DREaM) Galaxy Catalogs: Predictions for a Roman Ultra-Deep Field
• Testing the Accuracy of Halo Occupation Distribution Modelling using Hydrodynamic Simulations
• Cosmological Constraints from Galaxy Clustering and the Mass-to-Number Ratio of Galaxy Clusters: Marginalizing over the Physics of Galaxy Formation
• A Prescription for Galaxy Biasing Evolution as a Nuisance Parameter
• The 6dF Galaxy Survey: Dependence of halo occupation on stellar mass
• Intensity mapping cross-correlations II: HI halo models including shot noise
• The VIMOS-VLT Deep Survey: Evolution in the Halo Occupation Number since z $\sim$ 1
• Power law correlations in galaxy distribution and finite volume effects from the Sloan Digital Sky Survey Data Release Four
• Constraining thermal dust emission in distant galaxies with number counts and angular power spectra
• 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
• Galaxy assembly bias of central galaxies in the Illustris simulation
• ELUCID. VI: Cosmic variance of galaxy distribution in the local Universe
• Towards Accurate Modelling of Galaxy Clustering on Small Scales: Testing the Standard $\Lambda \mathrm{CDM}$ + Halo Model
• MOIRCS Deep Survey. II. Clustering Properties of K-band Selected Galaxies in GOODS-North Region
• Statistical analysis of galaxy surveys - III: The non-linear clustering of red and blue galaxies in the 2dFGRS
• Galaxy clustering and projected density profiles as traced by satellites in photometric surveys: Methodology and luminosity dependence
• Small-scale galaxy clustering in the EAGLE simulation
• The stellar mass - halo mass relation from galaxy clustering in VUDS: a high star formation efficiency at z~3
• The origin of dispersion in DLA metallicities
• Small- and Large-Scale Galactic Conformity in SDSS DR7
• Dependence of Halo Bias and Kinematics on Assembly Variables
• The BOSS-WiggleZ overlap region II: dependence of cosmic growth on galaxy type
• Relative clustering and the joint halo occupation distribution of red-sequence and blue-cloud galaxies in COMBO-17
• How to Optimally Constrain Galaxy Assembly Bias: Supplement Projected Correlation Functions with Count-in-cells Statistics
• The dependence of galaxy clustering on tidal environment in the Sloan Digital Sky Survey
• Fourier Phase Analysis of SDSS Galaxies
• Testing homogeneity in the Sloan Digital Sky Survey Data Release Twelve with Shannon entropy
• Linking haloes to galaxies: how many halo properties are needed?
• Clustering Properties of restframe UV selected galaxies II: Migration of Star Formation sites with cosmic time from GALEX and CFHTLS
• The PEP survey: clustering of infrared-selected galaxies and structure formation at z~2 in the GOODS South
• What determines large scale galaxy clustering: halo mass or local density?
• The evolution of the galaxy content of dark matter haloes
• BSG alignment of SDSS galaxy groups
• The Physical Origin of Galactic Conformity: From Theory to Observation
• 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?
• On the prospect of using the maximum circular velocity of halos to encapsulate assembly bias in the galaxy-halo connection
• The galaxy size - halo mass scaling relations and clustering properties of central and satellite galaxies
• The Gigaparsec WiggleZ Simulations: Characterising scale dependant bias and associated systematics in growth of structure measurements
• ELUCID V. Lighting dark matter halos with galaxies
• Galaxy and Mass Assembly (GAMA): Colour and luminosity dependent clustering from calibrated photometric redshifts
• An ALMA survey of the SCUBA-2 Cosmology Legacy SurveyUKIDSS/UDS Field: Halo Masses for Submillimetre Galaxies
• Exploring star formation using the filaments in the Sloan Digital Sky Survey Data Release Five (SDSS DR5)
• Halo Occupation Distribution Modeling of Green Valley Galaxies
• A systematic reclassification of type IIn supernovae
• Effects of superstructure environment on galaxy groups
• Higher-Order Angular Galaxy Correlations in the SDSS: Redshift and Color Dependence of non-Linear Bias
• Forecasting the Dark Energy Measurement with Baryon Acoustic Oscillations: Prospects for the LAMOST surveys
• Further spectroscopic observations of the CSL-1 object
• An improved limit on the neutrino mass with CMB and redshift-dependent halo bias-mass relations from SDSS, DEEP2, and Lyman-Break Galaxies
• Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias
• Precision Measurements of Higher-Order Angular Galaxy Correlations Using 11 Million SDSS Galaxies
• The UV-Optical Color Dependence of Galaxy Clustering in the Local Universe
• The MillenniumTNG Project: The large-scale clustering of galaxies
• Cosmological constraints on early dark energy from the full shape analysis of eBOSS DR16
• Probing the galaxy-halo connection with total satellite luminosity
• Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
• WALLABY Pre-Pilot Survey: The effects of tidal interaction on radial distribution of color in galaxies of the Eridanus supergroup
• Understanding the non-linear clustering of high redshift galaxies
• Dissecting the roles of mass and environment quenching in galaxy evolution with EAGLE
• Nurturing Lyman Break Galaxies: Observed link between environment and spectroscopic features
• Clustering of the IR Background Light with Spitzer: Contribution from Resolved Sources
• Clustering analysis of high-redshift Luminous Red Galaxies in Stripe 82
• VVDS-SWIRE: Clustering evolution from a spectroscopic sample of galaxies with redshift 0.2<z<2.1 selected from Spitzer IRAC 3.6 micron and 4.5 micron photometry
• The luminosities of the brightest cluster galaxies and brightest satellites in SDSS groups
• Statistical Analysis of Galaxy Surveys-IV: An objective way to quantify the impact of superstructures on galaxy clustering statistics
• Halos and voids in a multifractal model of cosmic structure
• Measures of galaxy environment -- II. Rank-ordered mark correlations
• An IFU View of the Active Galactic Nuclei in MaNGA Galaxy Pairs
• Radiation-induced large-scale structure during the reionization epoch: the autocorrelation function
• The Galaxy Cross-Correlation Function as a Probe of the Spatial Distribution of Galactic Satellites
• Classification and environmental properties of X-ray selected point-like sources in the XMM-LSS field
• The zCOSMOS-Bright survey: the clustering of early and late galaxy morphological types since z~1
• Exploring Galaxy Formation Models and Cosmologies with Galaxy Clustering
• Spatial Clustering from GALEX-SDSS samples: Star Formation History and large-scale clustering
• A census of radio-selected AGN on the COSMOS field and of their FIR properties
• Spatial Clustering of High Redshift Lyman Break Galaxies
• Quasar-Galaxy Clustering through Projected Galaxy Counts at z=0.6-1.2
• On the scatter in the relation between stellar mass and halo mass: random or halo formation time dependent?
• A Physical Model of Lyman Alpha Emitters
• Clustering of Intermediate Luminosity X-ray selected AGN at z~3
• The age dependence of galaxy clustering
• The clustering of H$\beta$+[OIII] and [OII] emitters since $z\sim 5$: dependencies with line luminosity and stellar mass
• Magnitude Gap Statistics and the Conditional Luminosity Function
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• Describing galaxy weak lensing measurements from tenths to tens of Mpc and up to z~0.6 with a single model
• Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model - I. Magnitude counts, redshift distribution, colour bimodality, and galaxy 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
• Improving Correlation Function Fitting with Ridge Regression: Application to Cross-Correlation Reconstruction
• The bias of dark matter tracers: assessing the accuracy of mapping techniques
• The clustering of $z>7$ galaxies: Predictions from the BLUETIDES simulation
• Helium Reionization Simulations. I. Modeling Quasars as Radiation Sources
• The Nuclear Activities of Nearby S0 Galaxies
• Understanding the faint red galaxy population using large-scale clustering measurements from SDSS DR7
• 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
• Testing one-loop galaxy bias: cosmological constraints from the power spectrum
• Extracting HI Astrophysics from Interferometric Intensity Mapping
• Calibrating photometric redshift distributions with cross-correlations
• The distribution of faint satellites around central galaxies in the CFHT Legacy Survey
• HOD-Dependent Systematics in Emission Line Galaxies for the DESI 2024 BAO analysis
• The dependence of subhalo abundance matching on galaxy photometry and selection criteria
• Passive Evolution of Galaxy Clustering
• The galaxy correlation function as a constraint on galaxy formation physics
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• Maturing Satellite Kinematics into a Competitive Probe of the Galaxy-Halo Connection
• Decomposition of Spectra from Redshift Distortion Maps
• Extending Recovery of the Primordial Matter Power Spectrum
• Probing the large scale structure using gravitational-wave observations of binary black holes
• Does jackknife scale really matter for accurate large-scale structure covariances?
• Halo models of HI selected galaxies
• The very wide-field $gzK$ galaxy survey -- I. Details of the clustering properties of star-forming galaxies at $z\sim 2$
• SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES) IV: Spatial clustering and halo masses of 450-$\mu$m-selected sub-millimeter galaxies
• The Galactic Environment of the NeVIII Absorber toward HE0226-4110
• The Imperial IRAS-FSC Redshift Catalogue: luminosity functions, evolution and galaxy bias
• Counts-in-Cylinders in the Sloan Digital Sky Survey with Comparisons to N-body Simulations
• The Halo Occupation Distribution of Obscured Quasars: Revisiting the Unification Model
• A Steep Slope and Small Scatter for the High-Mass End of the L-$\sigma$ Relation at $z\sim 0.55$
• Halo Occupation Distribution of Massive Galaxies since z = 1
• Clustering Properties of restframe UV selected galaxies I: the correlation length derived from GALEX data in the local Universe
• The Complementarity of Redshift-space Distortions and the Integrated Sachs-Wolfe Effect: A 3D Spherical Analysis
• A direct and robust method to observationally constrain the halo mass function via the submillimeter magnification bias: Proof of concept
• The clustering of X-ray AGN at 0.5 < z < 4.5: host galaxies dictate dark matter halo mass
• Constraints on a scale-dependent bias from galaxy clustering
• Building a Better Understanding of the High Redshift BOSS Galaxies as Tools for Cosmology
• Maximum Likelihood Random Galaxy Catalogues and Luminosity Function Estimation
• MOIRCS Deep Survey. X. Evolution of Quiescent Galaxies as a Function of Stellar Mass at 0.5<z<2.5
• Analytical halo model of galactic conformity
• Modeling Redshift-Space Clustering with Abundance Matching
• Broadband Alcock-Paczynski test exploiting redshift distortions
• The Nature of Low Surface Brightness Galaxies in the Hyper Suprime-Cam Survey
• Towards optimal estimation of the galaxy power spectrum
• Autocorrelations of stellar light and mass at z~0 and ~1: From SDSS to DEEP2
• Rosella: A mock catalogue from the P-Millennium simulation
• A Halo Model with Environment Dependence: Theoretical Considerations
• Transitioning from Stage-III to Stage-IV: Cosmology from galaxy$\times$CMB lensing and shear$\times$CMB lensing
• Constraining the galaxy-halo connection of infrared-selected unWISE galaxies with galaxy clustering and galaxy-CMB lensing power spectra
• Clustering of Extremely Red Objects in Elais-N1 from the UKIDSS DXS with optical photometry from Pan-STARRS1 and Subaru
• The FMOS-COSMOS survey of star-forming galaxies at $z\sim 1.6$. V: Properties of dark matter halos containing H$\alpha$ emitting galaxies
• Constraints on sigma_8 from galaxy clustering in N-body simulations and semi-analytic models
• The strong environmental dependence of black hole scaling relations
• A Direct Measurement of the High-Mass End of the Velocity Dispersion Function at $z\sim 0.55$ from SDSS-III/BOSS
• Downsizing of Star Formation Measured from the Clustered Infrared Background Correlated with Quasars
• Correlation function: biasing and fractal properties of the cosmic web
• Tracing the galaxy-halo connection with galaxy clustering in COSMOS-Web from z = 0.1 to z ~ 12
• How accurate is our knowledge of galaxy bias?
• The Halo Occupation Distribution of Black Holes: Dependence on Mass
• The luminosity bias relation from filaments in the Sloan Digital Sky Survey Data Release Four
• Using galaxy pairs to investigate the three-point correlation function in the squeezed limit
• Early Science Result from the Japanese Virtual Observatory: AGN and Galaxy Clustering at z = 0.3 to 3.0
• The Global Environment of Small Galaxy Systems
• A Halo Occupation Interpretation Of Quasars At $z\sim 1.5$ Using Very Small Scale Clustering Information
• Fingers-of-God effect of infalling satellite galaxies
• Fractal Approach to Large-Scale Galaxy Distribution
• A Coarse-Grained Field Theory for Density Fluctuations and Correlation Functions of Galactic Objects
• Extremely Massive Quasars are not Good Proxies for Dense Environments Compared to Massive Galaxies: Environments of Extremely Massive Quasars and Galaxies
• Quasars at intermediate redshift are not special; but they are often satellites
• Field Theory of the Correlation Function of Mass Density Fluctuations for Self-Gravitating Systems
• EMPRESS. XI. SDSS and JWST Search for Local and z~4-5 Extremely Metal-Poor Galaxies (EMPGs): Clustering and Chemical Properties of Local EMPGs
• Constraining Halo Occupation Distribution and Cosmic Growth Rate using Multipole Power Spectrum
• Recovering the real-space correlation function from photometric redshift surveys
• A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). VI. Distant Filamentary Structures Pointed by High-z Radio Galaxies at z~4
• 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
• Single parameter galaxy classification: The Principal Curve through the multi-dimensional space of galaxy properties
• Quantifying the coherent outflows of galaxies around voids in the SDSS DR7
• Shedding Light on Low Surface Brightness Galaxies in Dark Energy Survey with Transformers
• Dark-ages reionization and galaxy formation simulation XI: Clustering and halo masses of high redshift galaxies
• Nonlinear Density Fluctuation Field Theory for Large Scale Structure
• Uncertainty in 2-point correlation function estimators and BAO detection in SDSS DR7
• An empirical model to form and evolve galaxies in dark matter halos
• Linking galaxies to dark matter haloes at $z\sim 1$ : dependence of galaxy clustering on stellar mass and specific star formation rate
• Got plenty of nothing: cosmic voids as a probe of particle dark matter
• Tomography-based observational measurements of the halo mass function via the submillimeter magnification bias
• QSO Lensing Magnification: A Comparison of 2QZ and SDSS Results
• Galaxy and Mass Assembly (GAMA): Tracing galaxy environment using the marked correlation function
• Using the Modified Nearest Neighbor Method to Correct Fiber-collision Effects on Galaxy Clustering
• Field Equation of Correlation Function of Mass Density Fluctuation for Self-Gravitating Systems
• Field Equation of Correlation Function of Mass Density Fluctuation for Self-Gravitating Systems
• Massive Neutrinos in Cosmology
• BASILISK: Bayesian Hierarchical Inference of the Galaxy-Halo Connection using Satellite Kinematics--I. Method and Validation
• A weak lensing view of the downsizing of star-forming galaxies
• Mitigating the impact of fiber assignment on clustering measurements from deep galaxy redshift surveys
• Spatial density fluctuations and selection effects in galaxy redshift surveys
• Gravitational Lensing Effects on the Baryonic Acoustic Oscillation Signature in the Redshift-Space Correlation Function
• 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 Color and Stellar Mass Dependence of Small-scale Galaxy Clustering in SDSS-III BOSS
• A New Perspective on the Large-Scale Tidal Effect on the Galaxy Luminosity and Morphology
• Can a conditioning on stellar mass explain the mutual information between morphology and environment?
• Correlation functions in 2D and 3D as descriptors of the cosmic web
• A semi-analytic model of pairwise velocity distribution between dark matter halos
• Effects of proper motion of neutron stars on continuous gravitational-wave searches
• Detecting Baryon Acoustic Oscillations with third generation gravitational wave observatories
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions and Lingering Tension
• Clustering and descendants of MUSYC galaxies at z<1.5
• Validating the clustering predictions of empirical models with the FLAMINGO simulations
• Autocorrelations of stellar light and mass in the low-redshift Universe
• Global analysis of luminosity- and colour-dependent galaxy clustering in the Sloan Digital Sky Survey
• Global structure of the Local Universe according to 2MRS survey
• Angular clustering of z~2 star-forming and passive galaxies in 2.5 square degrees of deep CFHT imaging
• The Host Galaxies and Narrow Line Regions of Four Double-Peaked [OIII] AGN
• A potentially pure test of cosmic geometry: galaxy clusters and the real space Alcock-Paczynski test
• On the Apparent Power Law in CDM Halo Pseudo Phase Space Density Profiles
• PRIMUS: Clustering of Star-forming and Quiescent Central Galaxies at $0.2<z<0.9$
• Galaxy And Mass Assembly (GAMA): the signatures of galaxy interactions as viewed from small scale galaxy clustering
• Observational determination of the galaxy bias from cosmic variance with a random pointing survey: Clustering of z~2 galaxies from Hubble's BoRG survey
• Connection Between Galaxies and HI in the Circumgalactic and Intergalactic Media: Variation According to Galaxy Stellar Mass and Star-formation Activity
• COMBO-17 measurements of the effect of environment on the type-dependent galaxy luminosity function
• Accurate Modeling of the Projected Galaxy Clustering in Photometric Surveys: I. Tests with Mock Catalogs
• PRIMUS: The Effect of Physical Scale on the Luminosity-Dependence of Galaxy Clustering via Cross-Correlations
• Improved Tomographic Binning of 3x2pt Lens Samples: Neural Network Classifiers and Optimal Bin Assignments
• Three- and two-point spatial correlations of IGM at $z\sim 2$: Cloud based analysis using simulations
• LARgE Survey -- II. The Dark Matter Halos and the Progenitors and Descendants of Ultra-Massive Passive Galaxies at Cosmic Noon
• The correlations between galaxy properties in different environments of the cosmic web
• Baryon acoustic scale at $z_{\eff} = 0.166$ with the SDSS blue galaxies
• Dwarf Galaxy Clustering and Missing Satellites
• Clustering Properties of Low-Luminosity Star-Forming galaxies at z = 0.24 and 0.40 in the Subaru Deep Field
• Methodological refinement of the submillimeter galaxy magnification bias. II. Cosmological analysis with tomography
• Galaxy interactions in filaments and sheets: insights from EAGLE simulations
• The Degeneracy of Galaxy Formation Models
• Cross-correlation between soft X-rays and galaxies A new benchmark for galaxy evolution models
• CFHTLenS: Galaxy bias as function of scale, stellar mass, and colour. Conflicts with predictions by semi-analytic models
• The 2.4 $\mu$m Galaxy Luminosity Function as Measured Using WISE. I. Measurement Techniques
• Clusters and Groups of Galaxies in the Simulated Local Universe
• On the Constraints of Galaxy Assembly Bias in Velocity Space
• Anomalous anisotropic cross-correlations between WMAP CMB maps and SDSS galaxy distribution and implications on the dark flow scenario
• Measuring the growth of structure by matching dark matter haloes to galaxies with VIPERS and SDSS
• A Maximum Likelihood Approach to Estimating Correlation Functions
• Joint constraints on galaxy bias and ${\sigma }_8$ through the N-pdf of the galaxy number density
• What is the optimal way to measure the galaxy power spectrum?
• Unraveling emission line galaxy conformity at z~1 with DESI early data
• Galaxy-galaxy lensing in the VOICE deep survey
• Origin of Metals around Galaxies I: Catalogs of Metal-line Absorption Doublets from High-Resolution Quasar Spectra
• The size and shape dependence of the SDSS galaxy bispectrum
• Evolution of the real-space correlation function from next generation cluster surveys
• Applying unsupervised learning to resolve evolutionary histories and explore the galaxy-halo connection in IllustrisTNG
• Conditional Colour-Magnitude Distribution of Central Galaxies in Galaxy Formation Models
• A Galaxy-Halo Model for Multiple Cosmological Tracers
• Scaling laws in the stellar mass distribution and the transition to homogeneity
• A Large Massive Quiescent Galaxy Sample at z~1.2
• An Empirical Mass Function Distribution
• The influence of superstructures on bright galaxy environments: clustering properties
• ELG$\times$LRG distribution through dark matter halo dynamics
• More than just halo mass: Modelling how the red galaxy fraction depends on multiscale density in a HOD framework
• Clustering of K-band selected local galaxies
• Clustering of 2PIGG galaxy groups with 2dFGRS galaxies
• CLIMBER: Galaxy-Halo Connection Constraints from Next-Generation Surveys
• The roles of environment and interactions on the evolution of red and blue galaxies in the EAGLE simulation
• Cosmology with Galaxy Correlations
• BASILISK II. Improved Constraints on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• Measuring galaxy abundance and clustering at high redshift from incomplete spectroscopic data: Tests on mock catalogs
• Pulsar B1237+25 Aberration/Retardation Analysis from Decimeter to Decameter Wavelength: Challenge to "Radius-to-Frequency Mapping"
• An Order Statistics Approach to the Halo Model for Galaxies
• Toward accurate measurement of property-dependent galaxy clustering I. Comparison of the Vmax method and the "shuffled" method
• A halo model approach to describe clustering and emission of the two main star forming galaxy populations for Cosmic Infrared Background studies
• Atomic Hydrogen Shows its True Colours: Correlations between HI and Galaxy Colour in Simulations
• Spatial clustering in the ESO-Sculptor Survey: two-point correlation functions by galaxy type at redshifts 0.1 - 0.5
• Tighter bounds on a hypothetical graviton screening mass from the gravitational wave observation GW150914 at LIGO
• Direct Determination of Expansion History Using Redshift Distortions
• DESI Emission-line Galaxies: Clustering Dependence on Stellar Mass and [OII] Luminosity
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• The galaxy luminosity function in the LAMOST Complete Spectroscopic Survey of Pointing Area at the Southern Galactic Cap
• Correlation Properties of Galaxies from the Main Galaxy Sample of the SDSS Survey
• Optical Confirmation of X-ray selected Galaxy clusters from the Swift AGN and Cluster survey with MDM and Pan-STARRS Data (Paper III)
• Using two point correlation functions to understand the assembly histories of Milky Way-like galaxies
• The mass and redshift dependence of halo star clustering
• Methodological refinement of the submillimeter galaxy cross-correlation function measurements and their uncertainty estimation
• 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
• Impact of a Rapid Diluted Energy Density on the halo mass function
• Toward accurate measurement of property-dependent galaxy clustering: II. Tests of the smoothed density-corrected $V_{\max }$ method
• Mitigating the impact of fiber assignment on the measurement of galaxy-lensing cross correlation
• Alignment of spiral and elliptical galaxies from Siena Galaxy Atlas with filaments
• Cosmic magnification on high-redshift submillimeter galaxies
• Clustering Property of Wolf-Rayet Galaxies in the SDSS
• Predicting halo occupation and galaxy assembly bias with machine learning
• Blueberry and Green Pea galaxies live in low density environments
• One Galaxy Sample to Rule Them All: Halo Occupation Distribution Modeling of DES Year 3 Source Galaxies
• Exploring the evolution of red and blue galaxies in different cosmic web environments using IllustrisTNG simulation
• A semi-analytical perspective on massive red galaxies: I. Assembly history, environment & redshift evolution
• Mapping Nearby Galaxies with Apache Point Observatory: Group and field galaxies' morphologies in the colour-magnitude plane
• Correlation between Outlying Halo Abundance and Host Halo Properties
• Using a Neural Network Classifier to Select Galaxies with the Most Accurate Photometric Redshifts
• Colour Dependence of the Distribution of IRAS Galaxies revealed by Multifractal Measures
• Comparison of clustering properties of observed objects and dark matter halos on different mass and spatial scales
• ELUCID-DESI I: A Parallel MPI Implementation of the Initial Condition Solver for Large-Scale Reconstruction Simulations
• A multiwavelength study of near- and mid-infrared selected galaxies at high redshift: ERGs, AGN-identification and the contribution from dust
• Testing cosmic homogeneity and isotropy using galaxy correlations