Galaxy Clustering in the Completed SDSS Redshift Survey: The Dependence on Color and Luminosity

Abstract

We measure the luminosity and color dependence of galaxy clustering in the SDSS DR7 main galaxy sample, focusing on the projected correlation function w_p(r_p) of volume-limited samples. We interpret our measurements using halo occupation distribution (HOD) modeling assuming a Lambda-CDM cosmology. The amplitude of w_p(r_p) grows slowly with luminosity for L < L_* and increases sharply at higher luminosities, with bias factor b(>L)=1.06+0.23(L/L_*)^{1.12}. At fixed luminosity, redder galaxies have a stronger and steeper w_p(r_p), a trend that runs steadily from the bluest galaxies to the reddest galaxies. The individual luminosity trends for the red and blue galaxy populations are strikingly different. Blue galaxies show a slow but steady increase of w_p(r_p) with luminosity, at all scales. The large-scale clustering of red galaxies shows little luminosity dependence until a sharp increase at L > 4L_*, but the lowest luminosity red galaxies (0.04-0.25 L_*) show very strong clustering on scales r_p < 2 Mpc/h. Most of the observed trends can be naturally understood within the LCDM+HOD framework. The growth of w_p(r_p) with luminosity reflects an overall shift in the halo mass scale, in particular an increase in the minimum host halo mass Mmin. The mass at which a halo has, on average, one satellite galaxy brighter than L is M_1 ~ 17 Mmin(L) over most of the luminosity range. The growth and steepening of w_p(r_p) for redder galaxies reflects the increasing fraction of galaxies that are satellite systems in high mass halos instead of central systems in low mass halos, a trend that is especially marked at low luminosities. Our extensive measurements, provided in tabular form, will allow detailed tests of theoretical models of galaxy formation, a firm grounding of semi-empirical models of the galaxy population, and new cosmological tests.

35 pages, 22 figures, updated to match accepted version to ApJ. A version with Figures 1-4 in full resolution is available at http://astronomy.case.edu/izehavi/dr7v2_clustering.pdf

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• Dependence of Halo Bias and Kinematics on Assembly Variables
• Linear bias forecasts for emission line cosmological surveys
• Mapping the Universe: The 2010 Russell Lecture
• How to Optimally Constrain Galaxy Assembly Bias: Supplement Projected Correlation Functions with Count-in-cells Statistics
• 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
• The dependence of galaxy clustering on tidal environment in the Sloan Digital Sky Survey
• The evolution of the galaxy content of dark matter haloes
• The fraction of early-type galaxies in low redshift groups and clusters of galaxies
• Are the halo occupation predictions consistent with large scale galaxy clustering?
• The NIRSpec Wide GTO Survey
• Hierarchical probabilistic inference of cosmic shear
• Halo assembly bias from Separate Universe simulations
• On the prospect of using the maximum circular velocity of halos to encapsulate assembly bias in the galaxy-halo connection
• The cosmic web of X-ray active galactic nuclei seen through the eROSITA Final Equatorial Depth Survey (eFEDS)
• Galaxy clustering dependence on the $\left[\mathrm{O}\mathrm{II}\right]$ emission line luminosity in the local Universe
• An ALMA survey of the SCUBA-2 Cosmology Legacy SurveyUKIDSS/UDS Field: Halo Masses for Submillimetre Galaxies
• The impact of baryonic physics on the abundance, clustering, and concentration of halos
• The COS Absorption Survey of Baryon Harbors: The Galaxy Database and Cross-Correlation Analysis of OVI Systems
• Increasing the Lensing Figure of Merit through Higher Order Convergence Moments
• H-ATLAS/GAMA: Magnification Bias Tomography. Astrophysical constraints above $\sim 1$ arcmin
• Differences in Halo-Scale Environments between Type 1 and Type 2 AGNs at Low Redshift
• Effects of superstructure environment on galaxy groups
• Halo Occupation Distribution Modeling of Green Valley Galaxies
• Galaxy and Mass Assembly (GAMA): Colour and luminosity dependent clustering from calibrated photometric redshifts
• Structure in the 3D Galaxy Distribution: I. Methods and Example Results
• Probing galaxy assembly bias with LRG weak lensing observations
• How galaxies populate haloes in very low-density environments? An analysis of the Halo Occupation Distribution in cosmic voids
• Large-scale clustering as a probe of the origin and the host environment of fast radio bursts
• Green galaxies in the COSMOS field
• The spatial distribution of neutral hydrogen as traced by low HI mass galaxies
• Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias
• Galaxy bias from the Dark Energy Survey Science Verification data: combining galaxy density maps and weak lensing maps
• The Galaxy-Halo Connection for $1.5\lesssim z\lesssim 5$ as revealed by the \emph{Spitzer} Matching survey of the UltraVISTA ultra-deep Stripes
• The MillenniumTNG Project: The large-scale clustering of galaxies
• Clustering with JWST: Constraining Galaxy Host Halo Masses, Satellite Quenching Efficiencies, and Merger Rates at z=4-10
• Probing the galaxy-halo connection with total satellite luminosity
• Combination of cluster number counts and two-point correlations: Validation on Mock Dark Energy Survey
• Precision Redshift-Space Galaxy Power Spectra using Zel'dovich Control Variates
• Dissecting the roles of mass and environment quenching in galaxy evolution with EAGLE
• 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
• C${}^3$-Cluster Clustering Cosmology I. New constraints on the cosmic growth rate at z~0.3 from redshift-space clustering anisotropies
• The clustering amplitude of X-ray selected AGN at z=0.8: Evidence for a negative dependence on accretion luminosity
• Euclid preparation: XII. Optimizing the photometric sample of the Euclid survey for galaxy clustering and galaxy-galaxy lensing analyses
• Measures of galaxy environment -- II. Rank-ordered mark correlations
• Tracing the gravitational potential using cosmic voids
• Understanding the non-linear clustering of high redshift galaxies
• Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
• Evidence of Galaxy Assembly Bias in SDSS DR7 Galaxy Samples from Count Statistics
• The PAU Survey: Spectral features and galaxy clustering using simulated narrow band photometry
• From starburst to quiescence: post-starburst galaxies and their large-scale clustering over cosmic time
• Constraining the properties of gaseous halos via cross-correlations of upcoming galaxy surveys and thermal Sunyaev-Zel'dovich maps
• Testing the accuracy of clustering redshift with simulations
• Intergalactic filaments spin
• The clustering of submillimeter galaxies detected with ALMA
• Simulating the infrared sky with a Spritz
• Real- and redshift-space halo clustering in $f(R)$ cosmologies
• SDSS-IV MaNGA: Signatures of halo assembly in kinematically misaligned galaxies
• Spatial Clustering of High Redshift Lyman Break Galaxies
• Missing Giants: Predictions on Dust-Obscured Galaxy Stellar Mass Assembly Throughout Cosmic Time
• Galaxy And Mass Assembly (GAMA): Bivariate functions of H$\alpha$ star forming galaxies
• Cosmological dependence of the measurements of luminosity function, projected clustering and galaxy-galaxy lensing signal
• Modeling Intrinsic Galaxy Alignment in the MICE Simulation
• Linear bias and halo occupation distribution of emission line galaxies from Nancy Grace Roman Space Telescope
• Magnitude Gap Statistics and the Conditional Luminosity Function
• The clustering of H$\beta$+[OIII] and [OII] emitters since $z\sim 5$: dependencies with line luminosity and stellar mass
• 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
• The ALHAMBRA survey: an empirical estimation of the cosmic variance for merger fraction studies based on close pairs
• Extending the halo mass resolution of $N$-body simulations
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Measuring nonlinear galaxy bias at z~0.8
• The formation of supermassive black holes from Population III.1 seeds. II. Evolution to the local universe
• Detection of spatial correlations of fundamental plane residuals, and cosmological implications
• Galaxy And Mass Assembly (GAMA): The Bright Void Galaxy Population in the Optical and Mid-IR
• A study on the statistical significance of mutual information between morphology of a galaxy and its large-scale environment
• A Halo Model Approach to the $21\mathrm{cm}$ and $\mathrm{Ly}\alpha$ Cross-correlation
• Euclid: The selection of quiescent and star-forming galaxies using observed colours
• Evolution of hierarchical clustering in the CFHTLS-Wide since z~1
• Cosmic Infrared Background anisotropies as a window into primordial non-Gaussianity
• Extracting HI Astrophysics from Interferometric Intensity Mapping
• 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 Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: GLAM-QPM mock galaxy catalogs for the Emission Line Galaxy Sample
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Exploring the dependence of the three-point correlation function on stellar mass and luminosity at 0.5<z<1.1
• Euclid preparation. XLI. Galaxy power spectrum modelling in real space
• Cosmic Near-infrared Background Tomography with SPHEREx Using Galaxy Cross-correlations
• The assembly bias of emission line galaxies
• Joint Analysis of Galaxy-Galaxy Lensing and Galaxy Clustering: Methodology and Forecasts for DES
• 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
• Luminosity bias: from haloes to galaxies
• The distribution of faint satellites around central galaxies in the CFHT Legacy Survey
• Multi-wavelength mock galaxy catalogs of the low-redshift Universe
• The ALHAMBRA survey : $B-$band luminosity function of quiescent and star-forming galaxies at $0.2\le z<1$ by PDF analysis
• Subhaloes gone Notts: the clustering properties of subhaloes
• Halo models of HI selected galaxies
• Does jackknife scale really matter for accurate large-scale structure covariances?
• A gravitational lensing detection of filamentary structures connecting luminous red galaxies
• A new method to measure galaxy bias by combining the density and weak lensing fields
• The hot circumgalactic medium in the eROSITA All-Sky Survey III. Star-forming and quiescent galaxies
• The Herschel-PEP survey: evidence for downsizing in the hosts of dusty star-forming systems
• The very wide-field $gzK$ galaxy survey -- I. Details of the clustering properties of star-forming galaxies at $z\sim 2$
• Clustering Constraints on the Relative Sizes of Central and Satellite Galaxies
• Maturing Satellite Kinematics into a Competitive Probe of the Galaxy-Halo Connection
• Using angular two-point correlations to self-calibrate the photometric redshift distributions of DECaLS DR9
• Herschel-ATLAS/GAMA: spatial clustering of low-redshift sub-mm galaxies
• The Clustering Of Galaxies Around Radio-Loud AGNs
• Cosmological Constraints from applying SHAM to rescaled cosmological simulations
• On the Clustering of Faint Red Galaxies
• The ASAS-SN Bright Supernova Catalog -- V. 2018-2020
• The Cross-correlation of MgII Absorption and Galaxies in BOSS
• Analytical halo model of galactic conformity
• Modeling Redshift-Space Clustering with Abundance 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
• Separating the blue cloud and the red sequence using Otsu's method for image segmentation
• Halo Histories vs. Galaxy Properties at z=0, III: The Properties of Star-Forming Galaxies
• The Clustering and Halo Masses of Star Forming Galaxies at z<1
• Alcock-Paczynski Test with the Evolution of Redshift-Space Galaxy Clustering Anisotropy
• Building a Better Understanding of the High Redshift BOSS Galaxies as Tools for Cosmology
• Generating mock galaxy catalogues for flux-limited samples like the DESI Bright Galaxy Survey
• Autocorrelations of stellar light and mass at z~0 and ~1: From SDSS to DEEP2
• Minimising the impact of scale-dependent galaxy bias on the joint cosmological analysis of large scale structures
• Forward Modeling of Spectroscopic Galaxy Surveys: Application to SDSS
• Rosella: A mock catalogue from the P-Millennium simulation
• Towards optimal estimation of the galaxy power spectrum
• Angular clustering and host halo properties of [OII] emitters at $z>1$ in the Subaru HSC survey
• Colour matters: the effects of lensing on the positional offsets between optical and submillimetre galaxies in Herschel-ATLAS
• Cosmic Web Dissection in Fuzzy Dark Matter Cosmologies
• Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of H$\alpha$ and [O III] emitters
• The impact of systematic uncertainties in N-body simulations on the precision cosmology from galaxy clustering: a halo model approach
• Clustering of red-sequence galaxies in the fourth data release ofthe Kilo-Degree Survey
• Massive, red galaxies in a hierarchical universe-II Clustering of Extremely Red Objects
• Galaxy Three-Point Correlation Functions and Halo/Subhalo Models
• Do galaxy mergers prefer under-dense environments?
• Herschel-ATLAS : The spatial clustering of low and high redshift submillimetre galaxies
• Measuring the luminosity and virial black hole mass dependence of quasar-galaxy clustering at z ~ 0.8
• Clustering of Extremely Red Objects in Elais-N1 from the UKIDSS DXS with optical photometry from Pan-STARRS1 and Subaru
• Constraining the galaxy-halo connection of infrared-selected unWISE galaxies with galaxy clustering and galaxy-CMB lensing power spectra
• The Stellar-to-Halo Mass Ratios of Passive and Star-Forming Galaxies at z~2-3 from the SMUVS survey
• 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 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 Extended Local Supercluster
• The Clustering of Extremely Red Objects
• Retrieving the three-dimensional matter power spectrum and galaxy biasing parameters from lensing tomography
• Correlation function: biasing and fractal properties of the cosmic web
• The redshift dependence of Alcock-Paczynski effect: cosmological constraints from the current and next generation observations
• Constraining the scatter in the galaxy-halo connection at Milky Way masses
• Synergies across the spectrum for particle dark matter indirect detection: how HI intensity mapping meets gamma rays
• Constraining Dark Energy With Stacked Concave Lenses
• The clustering and halo occupation distribution of Lyman-break galaxies at $z\sim 4$
• How accurate is our knowledge of galaxy bias?
• Testing galaxy formation models with galaxy stellar mass functions
• Generalized Brans-Dicke theories in light of evolving dark energy
• A Halo Occupation Interpretation Of Quasars At $z\sim 1.5$ Using Very Small Scale Clustering Information
• A method for classification of red, blue and green galaxies using fuzzy set theory
• The relation between galaxy density and radio jet power for 1.4 GHz VLA selected AGN in Stripe 82
• The MUSE-Wide survey: Three-dimensional clustering analysis of Lyman-$\alpha$ emitters at $3.3<z<6$
• 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
• Analyzing Baryon Acoustic Oscillations in Sparse Spectroscopic Samples via Cross-Correlation with Dense Photometry
• Halo Occupation Distribution of Emission Line Galaxies: fitting method with Gaussian Processes
• Galaxy growth by merging in the nearby universe
• Close galaxy pairs with accurate photometric redshifts
• Bayesian framework to infer the Hubble constant from the cross-correlation of individual gravitational wave events with galaxies
• Using GAMA to probe the impact of small-scale galaxy physics on nonlinear redshift-space distortions
• Improving three-dimensional mass mapping with weak gravitational lensing using galaxy clustering
• Single parameter galaxy classification: The Principal Curve through the multi-dimensional space of galaxy properties
• The Beyond-Halo Mass Effects of the Cosmic Web Environment on Galaxies
• The Infrared Medium-Deep Survey II: How to Trigger Radio-AGN? Hints from Their Environments
• Dark-ages reionization and galaxy formation simulation XI: Clustering and halo masses of high redshift galaxies
• The ALHAMBRA survey: evolution of galaxy spectral segregation
• Properties of Galaxies around AGNs with Most Massive Supermassive Black Hole Revealed by the Clustering Analysis
• Galaxy and Mass Assembly (GAMA): Tracing galaxy environment using the marked correlation function
• New Statistical Perspective to The Cosmic Void Distribution
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Constraining the Galaxy-Halo Connection with Optimal Statistics
• Measuring the BAO peak position with different galaxy selections
• Using the Modified Nearest Neighbor Method to Correct Fiber-collision Effects on Galaxy Clustering
• The DESI One-Percent Survey: Modelling the clustering and halo occupation of all four DESI tracers with Uchuu
• Linking galaxies to dark matter haloes at $z\sim 1$ : dependence of galaxy clustering on stellar mass and specific star formation rate
• The impact of braiding covariance and in-survey covariance on next-generation galaxy surveys
• Revisiting the clustering of narrow-line AGN in the local Universe: Joint dependence on stellar mass and color
• The biasing phenomenon
• $\text{PineTree}$: 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
• An Introduction into the Theory of Cosmological Structure Formation
• On the origin of red spirals: Does assembly bias play a role?
• Cosmological constraints from the redshift dependence of the volume effect using the galaxy 2-point correlation function across the line-of-sight
• A semi-analytic model of pairwise velocity distribution between dark matter halos
• 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
• Global analysis of luminosity- and colour-dependent galaxy clustering in the Sloan Digital Sky Survey
• Angular clustering of z~2 star-forming and passive galaxies in 2.5 square degrees of deep CFHT imaging
• The Impact of the Dusty Torus on Obscured Quasar Halo Mass Measurements
• The XMM Cluster Survey: The Halo Occupation Number of BOSS galaxies in X-ray clusters
• The Color and Stellar Mass Dependence of Small-scale Galaxy Clustering in SDSS-III BOSS
• 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
• Correlation functions in 2D and 3D as descriptors of the cosmic web
• Recovering dark-matter clustering from galaxies with Gaussianization
• The phenomenology of the external field effect in cold dark matter models
• Color dependence of clustering of massive galaxies at 0.5$\le z\le$2.5: similar spatial distributions between green valley galaxies and AGNs
• PRIMUS: Clustering of Star-forming and Quiescent Central Galaxies at $0.2<z<0.9$
• Relating information entropy and mass variance to measure bias and non-Gaussianity
• A power spectrum approach to the search for Axion-like Particles from resolved galaxy clusters using CMB as a backlight
• Exploring the links between star formation and minor companions around isolated galaxies
• Angular Correlation Function Estimators Accounting for Contamination from Probabilistic Distance Measurements
• A New Stellar Mass Proxy for Subhalo Abundance Matching
• 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
• Accurate Modeling of the Projected Galaxy Clustering in Photometric Surveys: I. Tests with Mock Catalogs
• Two-point statistics without bins: A continuous-function generalization of the correlation function estimator for large-scale structure
• Observational determination of the galaxy bias from cosmic variance with a random pointing survey: Clustering of z~2 galaxies from Hubble's BoRG survey
• Three- and two-point spatial correlations of IGM at $z\sim 2$: Cloud based analysis using simulations
• Fast Forward Modelling of Galaxy Spatial and Statistical Distributions
• Peculiar Radio Structures in the Central Regions of Galaxy Cluster Abell 585
• PRIMUS: The Effect of Physical Scale on the Luminosity-Dependence of Galaxy Clustering via Cross-Correlations
• Scatter in the satellite galaxy SHMR: fitting functions, scaling relations & physical processes from the IllustrisTNG simulation
• Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
• Self-calibrating optical galaxy cluster selection bias using cluster, galaxy, and shear cross-correlations
• Galaxy And Mass Assembly (GAMA): the signatures of galaxy interactions as viewed from small scale galaxy clustering
• Cosmology in the non-linear regime : the small scale miracle
• Growth and Geometry Split in Light of the DES-Y3 Survey
• Multi-wavelength consensus of large-scale linear bias
• Semi-empirical catalog of early-type galaxy-halo systems: dark matter density profiles, halo contraction and dark matter annihilation strength
• Clustering, Cosmology and a New Era of Black Hole Demographics -- I. The Conditional Luminosity Function of Active Galactic Nuclei
• LARgE Survey -- II. The Dark Matter Halos and the Progenitors and Descendants of Ultra-Massive Passive Galaxies at Cosmic Noon
• Third-order intrinsic alignment of SDSS BOSS LOWZ galaxies
• Multi-Component Decomposition of Cosmic Infrared Background Fluctuations
• Towards a Model-Independent Measurement of the Halo Mass Function with Observables
• Measuring galaxy-galaxy-galaxy-lensing with higher precision and accuracy
• Euclid preparation: VI. Verifying the Performance of Cosmic Shear Experiments
• Clustering of galaxies around AGN in the HSC Wide survey
• The dark matter halo masses of elliptical galaxies as a function of observationally robust quantities
• Galaxy clustering using photometric redshifts
• Star-Forming Compact Groups (SFCGs): An ultraviolet search for a local sample
• Small scale clustering of BOSS galaxies: dependence on luminosity, color, age, stellar mass, specific star formation rate and other properties
• Star-forming and Quiescent Central Galaxies Cluster Similarly: Implications for the Galaxy-Halo Connection
• Euclid: Relativistic effects in the dipole of the 2-point correlation function
• Cosmological model dependence of the galaxy luminosity function: far-infrared results in the Lemaitre-Tolman-Bondi model
• The Galaxy Halo Connection in Modified Gravity Cosmologies: Environment Dependence of Galaxy Luminosity function
• Joint constraints on galaxy bias and ${\sigma }_8$ through the N-pdf of the galaxy number density
• The H$\alpha$ luminosity and stellar mass dependent clustering of star-forming galaxies at $0.7<z<1.5$ with 3D-HST
• Testing the Reliability of Fast Methods for Weak Lensing Simulations: WL-MOKA on PINOCCHIO
• Unexpected clustering pattern in dwarf galaxies challenges formation models
• On the Constraints of Galaxy Assembly Bias in Velocity Space
• Unraveling emission line galaxy conformity at z~1 with DESI early data
• Optical Spectroscopy of Dual Quasar Candidates from the Subaru HSC-SSP program
• A test of invariance of dark matter halo surface density using multiwavelength mock galaxy catalogues
• Evolution of matter and galaxy clustering in cosmological hydrodynamical simulations
• Quantifying the Colour-Dependent Stochasticity of Large-Scale Structure
• The Circular Velocity Function of Group Galaxies
• Cross-correlation between soft X-rays and galaxies A new benchmark for galaxy evolution models
• The Spatial Range of Conformity
• What is the optimal way to measure the galaxy power spectrum?
• Modeling spatially-resolved galactic H$\alpha$ emission for galaxy clustering
• Galaxy and halo angular clustering in LCDM and Modified Gravity cosmologies
• An Empirical Mass Function Distribution
• Can anisotropy in the galaxy distribution tell the bias?
• Cluster-counterpart Voids: Void Identification from Galaxy Density Field
• The Low Redshift survey at Calar Alto (LoRCA)
• The size and shape dependence of the SDSS galaxy bispectrum
• The impact of AGN X-ray selection on the AGN halo occupation distribution
• Estimating lifetimes of uv-selected massive galaxies at $0.5\le z\le 2.5$ in the cosmos/ultravista field through clustering analyses
• Galaxy and Mass Assembly (GAMA): Mid-infrared properties as tracers of galaxy environment
• A Large Massive Quiescent Galaxy Sample at z~1.2
• A Statistical Study of H I Gas in Nearby Narrow-Line AGN-Hosting Galaxies
• 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
• The assembly of the most rotationally supported disc galaxies in the TNG100 simulations
• Clustering properties and halo masses for central galaxies in the local Universe
• The influence of superstructures on bright galaxy environments: clustering properties
• BASILISK II. Improved Constraints on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• Quasar Pairs as Large--Scale Structure tracers
• The time evolution of bias
• Pulsar B1237+25 Aberration/Retardation Analysis from Decimeter to Decameter Wavelength: Challenge to "Radius-to-Frequency Mapping"
• Galaxy Correlation Function and Local Density from Photometric Redshifts Using the Stochastic Order Redshift Technique (SORT)
• SpectrAx: Spectral Search of Axion-Like Particles Using Multi-Band Observations of Galaxy Clusters from SKA, SO, CMB-S4 and eROSITA
• More than just halo mass: Modelling how the red galaxy fraction depends on multiscale density in a HOD framework
• Cosmic Census: Relative Distributions of Dark Matter, Galaxies and Diffuse Gas
• Properties beyond mass for unresolved haloes across redshift and cosmology using correlations with local halo environment
• Impact of Cosmic Variance on the Galaxy-Halo Connection for Lyman-$\alpha$ Emitters
• The mass and galaxy distribution around SZ-selected clusters
• Lognormal Distribution of Cosmic Voids in Simulations and Mocks
• On the Clustering of Compact Galaxy Pairs in Dark Matter Haloes
• Approximate methods for the generation of dark matter halo catalogs in the age of precision cosmology
• Inferring Host Dark Matter Halo Masses of Individual Galaxies from Neighboring Galaxy Counts
• Measuring galaxy abundance and clustering at high redshift from incomplete spectroscopic data: Tests on mock catalogs
• Impact of projection-induced optical selection bias on the weak lensing mass calibration of galaxy clusters
• DESI Emission-line Galaxies: Clustering Dependence on Stellar Mass and [OII] Luminosity
• Dark Energy Survey Year 3 results: Galaxy-halo connection from galaxy-galaxy lensing
• An Order Statistics Approach to the Halo Model for Galaxies
• The galaxy luminosity function in the LAMOST Complete Spectroscopic Survey of Pointing Area at the Southern Galactic Cap
• Improving the Accuracy of Halo Mass Based Statistics For Fast Approximate N-body Simulations
• Can we constrain the evolution of HI bias using configuration entropy?
• Pair Counting without Binning -- A New Approach to Correlation Functions in Clustering Statistics
• Constraining $z\lesssim 2$ ultraviolet emission with the upcoming ULTRASAT satellite
• Properties of environment around AGN and luminous galaxy pairs through HSC wide survey
• Toward accurate measurement of property-dependent galaxy clustering I. Comparison of the Vmax method and the "shuffled" method
• Atomic Hydrogen Shows its True Colours: Correlations between HI and Galaxy Colour in Simulations
• Impact of cosmic web on galaxy properties and their correlations: Insights from Principal Component Analysis
• Galaxies in X-ray Selected Clusters and Groups in Dark Energy Survey Data II: Hierarchical Bayesian Modeling of the Red-Sequence Galaxy Luminosity Function
• Blueberry and Green Pea galaxies live in low density environments
• Predicting halo occupation and galaxy assembly bias with machine learning
• The evolution of Balmer jump selected galaxies in the ALHAMBRA survey
• Morpho-statistical characterisation of the spatial galaxy distribution through Gibbs point processes
• Toward accurate measurement of property-dependent galaxy clustering: II. Tests of the smoothed density-corrected $V_{\max }$ method
• The multi-dimensional halo assembly bias can be preserved when enhancing halo properties with HALOSCOPE
• The invariance of group occupation across the cosmic web
• The Spitzer Extragalactic Representative Volume Survey and DeepDrill extension: clustering of near-infrared galaxies
• Exploiting Non-linear Scales in Galaxy-Galaxy Lensing and Galaxy Clustering: A Forecast for the Dark Energy Survey
• Void probability function in the Quijote simulations
• Quantifying the Poor Purity and Completeness of Morphological Samples Selected by Galaxy Colour
• Solving small-scale clustering problems in approximate lightcone mocks
• The effect of spiral arms on the Sérsic photometry of galaxies
• Uncertainties in measuring the dark matter signal from Milky Way satellites using Cherenkov telescopes
• DarkMix: Mixture Models for the Detection and Characterization of Dark Matter Halos
• Euclid preparation. 3D reconstruction of the cosmic web with simulated Euclid Deep spectroscopic samples
• A lightcone catalogue from the Millennium-XXL simulation: improved spatial interpolation and colour distributions for the DESI BGS
• ELUCID-DESI I: A Parallel MPI Implementation of the Initial Condition Solver for Large-Scale Reconstruction Simulations
• Finding and characterising WHIM structures using the luminosity density method
• Compact star forming galaxies as the progenitors of compact quiescent galaxies: clustering result
• An Optimal In-Situ Multipole Algorithm for the Isotropic Three-Point Correlation Functions
• Probing cosmic velocity-density correlations with galaxy luminosity modulations
• New leaves of the tree: percolation analysis for cosmic web with discrete points
• Tracing correlations between galaxy properties across the Cosmic Web: An IllustrisTNG-based study
• Biasing phenomenon
• Discovery of a supercluster candidate at $z\sim 1.1$
• Investigating the Circumgalactic Medium through Mg II absorption coincidence
• Cosmology with the 6-degree Field Galaxy Survey