Galaxy Clustering in Early SDSS Redshift Data

Abstract

We present the first measurements of clustering in the Sloan Digital Sky Survey (SDSS) galaxy redshift survey. Our sample consists of 29,300 galaxies with redshifts 5,700 km/s < cz < 39,000 km/s, distributed in several long but narrow (2.5-5 degree) segments, covering 690 square degrees. For the full, flux-limited sample, the redshift-space correlation length is approximately 8 Mpc/h. The two-dimensional correlation function ξ(r_p,π) shows clear signatures of both the small-scale, ``fingers-of-God'' distortion caused by velocity dispersions in collapsed objects and the large-scale compression caused by coherent flows, though the latter cannot be measured with high precision in the present sample. The inferred real-space correlation function is well described by a power law, ξ(r)=(r/6.1+/-0.2 Mpc/h)^{-1.75+/-0.03}, for 0.1 Mpc/h < r < 16 Mpc/h. The galaxy pairwise velocity dispersion is σ_{12} ~ 600+/-100 km/s for projected separations 0.15 Mpc/h < r_p < 5 Mpc/h. When we divide the sample by color, the red galaxies exhibit a stronger and steeper real-space correlation function and a higher pairwise velocity dispersion than do the blue galaxies. The relative behavior of subsamples defined by high/low profile concentration or high/low surface brightness is qualitatively similar to that of the red/blue subsamples. Our most striking result is a clear measurement of scale-independent luminosity bias at r < 10 Mpc/h: subsamples with absolute magnitude ranges centered on M_*-1.5, M_*, and M_*+1.5 have real-space correlation functions that are parallel power laws of slope ~ -1.8 with correlation lengths of approximately 7.4 Mpc/h, 6.3 Mpc/h, and 4.7 Mpc/h, respectively.

51 pages, 18 figures. Replaced to match accepted ApJ version

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• The Tiling Algorithm for the 6dF Galaxy Survey
• Building a Better Understanding of the High Redshift BOSS Galaxies as Tools for Cosmology
• The MUSE-Wide survey: Detection of a clustering signal from Lyman-α-emitters at 3<z<6
• Modeling Redshift-Space Clustering with Abundance Matching
• Measuring Linear and Non-linear Galaxy Bias Using Counts-in-Cells in the Dark Energy Survey Science Verification Data
• Autocorrelations of stellar light and mass at z~0 and ~1: From SDSS to DEEP2
• Towards optimal estimation of the galaxy power spectrum
• The CIDA-UCM-Yale Shallow Survey for Emission Line Galaxies
• Cosmological Information from the Small-scale Redshift Space Distortions
• Scaling behavior in a stochastic self-gravitating system
• The Environment on few Mpc scales of Infrared Luminous Galaxies at Redshifts z~1
• Forecasting the Cross-Correlation of the CSST galaxy survey with the FAST HI Intensity Map
• Detection of spatial clustering in the 1000 richest SDSS DR8 redMaPPer clusters with Nearest Neighbor distributions
• 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
• Massive, red galaxies in a hierarchical universe-II Clustering of Extremely Red Objects
• Expected properties of the Two-Point Autocorrelation Function of the IGM
• The local environmental dependence of galaxy properties in the volume-limited sample of Main Galaxies from the SDSS Data Release 5
• Downsizing of Star Formation Measured from the Clustered Infrared Background Correlated with Quasars
• Using galaxy pairs to investigate the three-point correlation function in the squeezed limit
• The Global Environment of Small Galaxy Systems
• Pairwise velocity dispersion of galaxies at high redshift: theoretical predictions
• The clustering and halo occupation distribution of Lyman-break galaxies at $z\sim 4$
• Galaxy interactions in filaments and sheets: effects of the large-scale structures versus the local density
• The MUSE-Wide survey: Three-dimensional clustering analysis of Lyman-$\alpha$ emitters at $3.3<z<6$
• Clustering of galaxies at 3.6 microns in the Spitzer Wide-area Infrared Extragalactic legacy survey
• Galaxy-Galaxy Lensing in EAGLE: comparison with data from 180 square degrees of the KiDS and GAMA surveys
• Galaxy luminosity evolution: how much is due to a model choice?
• Fractal Approach to Large-Scale Galaxy Distribution
• Large Scale Structure in the ELAIS S1 Survey
• The Dynamics of Inhomogeneous Cosmologies
• A Coarse-Grained Field Theory for Density Fluctuations and Correlation Functions of Galactic Objects
• The Unusual Milky Way-Local Sheet System: Implications for Spin Strength and Alignment
• A galaxy-halo model of large-scale structure
• SHAMe-SF: Predicting the clustering of star-forming galaxies with an enhanced abundance matching model
• Quenching or Bursting: Star Formation Acceleration--A New Methodology for Tracing Galaxy Evolution
• Measuring galaxy segregation using the mark connection function
• Dark-ages reionization and galaxy formation simulation XI: Clustering and halo masses of high redshift galaxies
• The evolution of galaxy clustering since z=1 from the Calar Alto Deep Imaging Survey
• Halo Masses of MgII absorbers at z\sim 0.5 from SDSS DR7
• Large scale structures in the Early SDSS: Comparison of the North and South Galactic strips
• Cosmological constraints from the masses and abundances of L* galaxies
• Nonlinear Density Fluctuation Field Theory for Large Scale Structure
• Correlation function of quasars in real and redshift space from the Sloan Digital Sky Survey Data Release 7
• The ESO-Sculptor Survey: Evolution of late-type galaxies at redshifts 0.1-0.5
• A weak lensing view of the downsizing of star-forming galaxies
• Using the Modified Nearest Neighbor Method to Correct Fiber-collision Effects on Galaxy Clustering
• Halo Model Analysis of Cluster Statistics
• Investigating the galaxy-halo connection of DESI Emission-Line Galaxies with SHAMe-SF
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Constraining the Galaxy-Halo Connection with Optimal Statistics
• Linking galaxies to dark matter haloes at $z\sim 1$ : dependence of galaxy clustering on stellar mass and specific star formation rate
• Photometric and clustering properties of hydrodynamical galaxies in a cosmological volume: results at z=0
• Autocorrelations of stellar light and mass in the low-redshift Universe
• Statistical measurements of dispersion measure fluctuations of FRBs
• The 2dF Galaxy Redshift Survey as a Cosmological Laboratory
• Can a conditioning on stellar mass explain the mutual information between morphology and environment?
• Validating the clustering predictions of empirical models with the FLAMINGO simulations
• A potentially pure test of cosmic geometry: galaxy clusters and the real space Alcock-Paczynski test
• The Color and Stellar Mass Dependence of Small-scale Galaxy Clustering in SDSS-III BOSS
• Cosmological surveys with multi-object spectrographs
• Angular clustering of z~2 star-forming and passive galaxies in 2.5 square degrees of deep CFHT imaging
• 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
• Recovering dark-matter clustering from galaxies with Gaussianization
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions and Lingering Tension
• Large-Scale Structure of Short-Lived LymanαEmitters
• Angular Correlation Function Estimators Accounting for Contamination from Probabilistic Distance Measurements
• Modeling non-linear effects in the redshift space two-point correlation function and its implications for the pairwise velocity dispersion
• Field-level simulation-based inference with galaxy catalogs: the impact of systematic effects
• Luminous Matter Distribution, Bulk Flows and Baryon Contents in Cosmological Models with a Local Void
• Void Probability Function of Simulated Surveys of high-redshift Lyman-Alpha Emitters
• The correlations between galaxy properties in different environments of the cosmic web
• Emergent gravity fails to explain color-dependent galaxy-galaxy lensing signals from SDSS Dr7
• The Two-Point Correlation Function of Gamma-ray Bursts
• On the statistical theory of self-gravitating collisionless dark matter flow
• Local Supercluster Dynamics: External Tidal Impact of the PSCz sample traced by Optimized Numerical Least Action Method
• Clustering Properties of Low-Luminosity Star-Forming galaxies at z = 0.24 and 0.40 in the Subaru Deep Field
• The Circular Velocity Function of Group Galaxies
• Detecting unresolved moving sources in a diffuse background
• What is the optimal way to measure the galaxy power spectrum?
• KiDS+VIKING+GAMA: Testing semi-analytic models of galaxy evolution with galaxy-galaxy-galaxy lensing
• Measuring neutrino mass and asymmetry with matter pairwise velocities
• Angular Correlation Function from sample covariance with BOSS and eBOSS LRG
• Galaxy Assembly and Evolution in the P-Millennium simulation: galaxy clustering
• A Measurement of The Faint Source Correlation Function in the GOODS and UDF Survey
• Clustering of K-band selected local galaxies
• The Redshift-Space Two Point Correlation Function of ELAIS-S1 Galaxies
• Experimental evaluation of complete safe coordination of astrobots for Sloan Digital Sky Survey V
• Non-Gaussianity of one-point distribution functions in extended Lagrangian perturbation theory
• The Large Scale Structure in the Universe: From Power-Laws to Acoustic Peaks
• Environmental dependence of different colors in the CMASS sample of the SDSS DR9
• Spatial clustering in the ESO-Sculptor Survey: two-point correlation functions by galaxy type at redshifts 0.1 - 0.5
• Assessing the connection between galactic conformity and assembly-type bias
• Toward accurate measurement of property-dependent galaxy clustering I. Comparison of the Vmax method and the "shuffled" method
• Impact of cosmic web on galaxy properties and their correlations: Insights from Principal Component Analysis
• A hierarchical clustering method for quantifying satellite abundance
• Spectroscopic Confirmation of Two X-ray Diffuse and Massive Galaxy Clusters at Low Redshift
• Probing the Type 3 interacting dark-energy model using matter pairwise velocity
• On the fairness of the main galaxy sample of SDSS
• Toward accurate measurement of property-dependent galaxy clustering: II. Tests of the smoothed density-corrected $V_{\max }$ method
• The Neighborhood Function and Its Application to Identifying Large-Scale Structure in the Comoving Universe Frame
• The evolution of Balmer jump selected galaxies in the ALHAMBRA survey
• Luminosity segregation versus fractal scaling in the galaxy distribution
• The formation of blue cluster in local Universe
• Recent Advances in Large-Scale Structure and Galaxy Formation Studies