The Stromlo-APM Redshift Survey II. Variation of Galaxy Clustering with Morphology and Luminosity

Abstract

We present clustering measurements for samples of galaxies selected by morphological type and luminosity from the recently completed Stromlo-APM Redshift Survey. Early type galaxies are clustered more strongly by a factor 3.5--5.5, than late type galaxies. Low-luminosity galaxies are clustered more weakly by a factor of $\sim 2$ than $L^{\ast }$ and brighter galaxies on scales $\simgt 1\hMpc$. Also the slope of the correlation function is steeper for low-luminosity galaxies, so that the amplitude is a factor 4 lower at $ 10 \hMpc$. No difference, however, is seen between the clustering of $L^{\ast }$ and more luminous galaxies, an observation which may be hard to reconcile with some theories of biased galaxy formation. Both redshift-space and real-space clustering estimates show a similar dependence on luminosity.

arXiv commentaccepted by The Astrophysical Journal, 26 September 1994; 30 pages, uuencoded compressed postscript, includes 9 figures; update of FERMILAB-PUB-94-147

Cited by in corpus (176)

• The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
• The Environmental Dependence of the Relations between Stellar Mass, Structure, Star Formation and Nuclear Activity in Galaxies
• Halo occupation numbers and galaxy bias
• Measuring and Modelling the Redshift Evolution of Clustering: the Hubble Deep Field North
• 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
• Galaxy Clustering in the Completed SDSS Redshift Survey: The Dependence on Color and Luminosity
• A measurement of the cosmological mass density from clustering in the 2dF Galaxy Redshift Survey
• Constraining Galaxy Formation and Cosmology with the Conditional Luminosity Function of Galaxies
• Galaxy Clustering in Early SDSS Redshift Data
• The density and peculiar velocity fields of nearby galaxies
• The 2dF Galaxy Redshift Survey: The dependence of galaxy clustering on luminosity and spectral type
• Subaru Deep Survey V. A Census of Lyman Break Galaxies at z=4 and 5 in the Subaru Deep Fields: Photometric Properties
• The 2dF Galaxy Redshift Survey: Luminosity dependence of galaxy clustering
• Galaxy and Mass Assembly (GAMA): The GAMA Galaxy Group Catalogue (G3Cv1)
• Stochastic Nonlinear Galaxy Biasing
• Linear Redshift Distortions: A Review
• Measuring the Redshift Evolution of Clustering: the Hubble Deep Field South
• New Techniques for Relating Dynamically Close Galaxy Pairs to Merger and Accretion Rates : Application to the SSRS2 Redshift Survey
• The Angular Clustering of Lyman-Break Galaxies at Redshift z=3
• The DEEP2 Galaxy Redshift Survey: Color and Luminosity Dependence of Galaxy Clustering at z~1
• The 2dF Galaxy Redshift Survey: galaxy clustering per spectral type
• Halo Occupation Distribution Modeling of Clustering of Luminous Red Galaxies
• Redshift-Space Distortions and the Real-Space Clustering of Different Galaxy Types
• The Intermediate-Scale Clustering of Luminous Red Galaxies
• Subaru Deep Survey VI. A Census of Lyman Break Galaxies at z=4 and 5 in the Subaru Deep Fields: Clustering Properties
• The DEEP2 Galaxy Redshift Survey: Clustering of Galaxies in Early Data
• Clustering Segregation With UV Luminosity in Lyman-Break Galaxies at z~3 and Its Implications
• Non-linear Stochastic Galaxy Biasing in Cosmological Simulations
• Evolution of bias in different cosmological models
• The DEEP Groth Strip Survey X: Number Density and Luminosity Function of Field E/S0 Galaxies at z < 1
• Cosmic Ray Protons and Magnetic Fields in Clusters of Galaxies and their Cosmological Consequences
• The Large-Scale Smoothness of the Universe
• Close Pairs of Field Galaxies in the CNOC1 Redshift Survey
• Southern Sky Redshift Survey: Clustering of Local Galaxies
• Galaxy Clustering and Galaxy Bias in a Lambda-CDM Universe
• The evolution of the galaxy distribution
• Spatial and Dynamical Properties of Voids in a LCDM Universe
• The Sloan Digital Sky Survey
• The Angular Correlation Function and Hierarchical Moments of 70000 Faint Galaxies to R=23.5
• Clustering at High Redshift: Precise Constraints from a Deep, Wide Area Survey
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Luminosity and stellar mass dependence of galaxy clustering at 0.5<z<1.1
• SDSS Galaxy Clustering: Luminosity & Colour Dependence and Stochasticity
• Nonlinear Stochastic Biasing of Galaxies and Dark Halos in Cosmological Hydrodynamic Simulations
• The Las Campanas IR Survey. II. Photometric redshifts, comparison with models and clustering evolution
• The Halo Distribution of 2dF Galaxies
• Scaling Laws in the Distribution of Galaxies
• Characterizing the Warm-Hot IGM at High Redshift: A High Resolution Survey for O VI at z = 2.5
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: modeling of the luminosity and colour dependence in the Data Release 10
• Evolution of Cluster Red-Sequence Galaxies from redshift 0.8 to 0.4: ages, metallicities and morphologies
• Physical Bias of Galaxies From Large-Scale Hydrodynamic Simulations
• The 2dF QSO Redshift Survey - II. Structure and evolution at high redshift
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Luminosity and Color Dependence and Redshift Evolution
• The Dependence of Velocity and Clustering Statistics on Galaxy Properties
• Modelling and interpreting the dependence of clustering on the spectral energy distributions of galaxies
• Time Evolution of Galaxy Formation and Bias in Cosmological Simulations
• Clustering Properties of Galaxies at z~4 in the Subaru/XMM Deep Survey Field
• The K-band luminosity function of nearby field galaxies
• The Real Space Power Spectrum of the PSCz Survey from 0.01 to 300 h/Mpc
• Clustering of Lyman alpha emitters at z ~ 4.5
• The Masses, Ancestors and Descendents of Extremely Red Objects: Constraints from Spatial Clustering
• The 2dF Galaxy Redshift Survey: voids and hierarchical scaling models
• The Clustering of High Redshift Galaxies in the Cold Dark Matter Scenario
• Luminosity dependence of the spatial and velocity distributions of galaxies: Semi-analytic models versus the Sloan Digital Sky Survey
• Clustering of galaxies around radio quasars at 0.5 < z < 0.8
• The Three-point Correlation Function of Galaxies Determined from the 2dF Galaxy Redshift Survey
• Quantifying angular clustering in wide-area radio surveys
• The Nearby Optical Galaxy Sample: The Local Galaxy Luminosity Function
• The Spatial Clustering of Distant, z~1, Early-Type Galaxies
• Is the Universe Homogeneous? (On Large Scales)
• Faint K Selected Galaxy Correlations and Clustering Evolution
• The local space density of dwarf galaxies
• On the least action principle in cosmology
• The cross-correlation between galaxies of different luminosities and Colors
• The Luminosity Distribution in Galaxy Clusters: A Dwarf Population - Density Relation?
• The Group Evolution Multiwavelength Study (GEMS): bimodal luminosity functions in galaxy groups
• Comparing estimators of the galaxy correlation function
• The Canada-France deep fields survey-II: Lyman-break galaxies and galaxy clustering at z~3
• The Clustering of Colour Selected Galaxies
• The Weak Clustering of Gas-Rich Galaxies
• Evolution of the Angular Correlation Function
• ISW measurements with photometric redshift surveys: 2MASS results and future prospects
• Quasar clustering: evidence for an increase with redshift and implications for the nature of AGNs
• The 2dF QSO Redshift Survey - IX. A measurement of the luminosity dependence of QSO clustering
• Luminosity function of galaxies in groups in the SDSS DR7: the dependence on mass, environment and galaxy type
• The Canada-France deep fields survey-I: 100,000 galaxies, 1 deg^2: a precise measurement of ω(θ) to IAB~25
• Spectral Analysis of the Stromlo-APM Survey II. Galaxy luminosity function and clustering by spectral type
• PRIMUS+DEEP2: The Dependence of Galaxy Clustering on Stellar Mass and Specific Star Formation Rate at 0.2 < z < 1.2
• Red Galaxy Clustering in the NOAO Deep Wide-Field Survey
• The DEEP2 Galaxy Redshift Survey: The Evolution of Void Statistics from z~1 to z~0
• The Angular Correlation Function of K=19.5 Galaxies and the Detection of a Cluster at z=0.775
• Properties of QSO Metal Line Absorption Systems at High Redshifts: Nature and Evolution of the Absorbers and New Evidence on Escape of Ionizing Radiation from Galaxies
• Probing the IGM-Galaxy Connection Toward PKS0405-123 II : A Cross-Correlation Study of Lya Absorbers and Galaxies at z<0.5
• Radio-quiet quasar environments at 0.5 < z < 0.8
• Evidence for anisotropy in the distribution of short-lived gamma-ray bursts
• The Small-scale Clustering of Luminous Red Galaxies via Cross-Correlation Techniques
• The Luminosity, Colour and Morphology dependence of galaxy filaments in the Sloan Digital Sky Survey Data Release Four
• Measuring the Nonlinear Biasing Function from a Galaxy Redshift Survey
• Bias and Hierarchical Clustering
• GaBoDS: The Garching-Bonn Deep Survey: VII. Probing galaxy bias using weak gravitational lensing
• Galaxy Clustering Evolution in the CNOC2 High-Luminosity Sample
• Critical analysis of the luminosity functions per galaxy type measured from redshift surveys
• The Galaxy Correlation Function in the CNOC2 Redshift Survey: Dependence on Color, Luminosity and Redshift
• The redshift-space two-point correlation functions of galaxies and groups in the Nearby Optical Galaxy sample
• HI Properties of Low Luminosity Star-Forming Galaxies in the KPNO International Spectroscopic Survey
• Galaxy Clustering and Large-Scale Structure from z = 0.2 to z = 0.5 in Two Norris Redshift Surveys
• Constraints on the Clustering, Biasing and Redshift Distribution of Radio Sources
• The Durham/UKST Galaxy Redshift Survey - VI. Power spectrum analysis of clustering
• The Local Environment of HII Galaxies
• Confusion noise at far-IR to millimeter wavelengths
• Spatial and Dynamical Biases in Velocity Statistics of Galaxies
• Galaxy Clustering and Dark Energy
• Galaxy and Mass Assembly (GAMA): Colour and luminosity dependent clustering from calibrated photometric redshifts
• The Gigaparsec WiggleZ Simulations: Characterising scale dependant bias and associated systematics in growth of structure measurements
• Exploring star formation using the filaments in the Sloan Digital Sky Survey Data Release Five (SDSS DR5)
• Measuring the Angular Correlation Function for Faint Galaxies in High Galactic Latitude Fields
• Steps toward the power spectrum of matter. I.The mean spectrum of galaxies
• The Omega Dependence of the Evolution of xi(r)
• The WiggleZ Dark Energy Survey: small-scale clustering of Lyman Break Galaxies at z < 1
• Galaxy Clustering Evolution in the UH8K Weak Lensing Fields
• The Sloan Digital Sky Survey
• The zCOSMOS-Bright survey: the clustering of early and late galaxy morphological types since z~1
• Emission-Line Galaxy Surveys as Probes of the Spatial Distribution of Dwarf Galaxies. I. The University of Michigan Survey
• Galaxy clustering in the Herschel deep field
• The nature of the relative bias between galaxies of different spectral type in 2dFGRS
• The Morphology Dependence of Luminosity Segregation in the Coma Cluster
• The WIRCam Deep Survey II: Mass Selected Clustering
• The Caltech Faint Galaxy Redshift Survey XII: Clustering of Galaxies
• Stellar Mass and color dependence of the three-point correlation function of galaxies in the local universe
• 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
• A simple tool for assessing the completeness in apparent magnitude of magnitude-redshift samples
• K-band luminosity (mass) segregation in AC118 at z=0.31
• The Clustering of Hot and Cold IRAS Galaxies: The Redshift Space Correlation Function
• The Group Evolution Multiwavelength Study (GEMS): The near-infrared luminosity function of nearby galaxy groups
• The CNOC2 Field Galaxy Redshift Survey
• Higher Order Clustering in the Durham/UKST and Stromlo-APM Galaxy Redshift Surveys
• The environments of hyperluminous infrared galaxies at 0.44<z<1.55
• Halo Occupation Distribution of Massive Galaxies since z = 1
• The Form and Evolution of the Clustering of QSO Heavy-Element Absorption-Line Systems
• Autocorrelations of stellar light and mass at z~0 and ~1: From SDSS to DEEP2
• Late Bloomer Galaxies: Growing Up in Cosmic Autumn
• The Clustering of AGN and Galaxies at Intermediate Redshift
• Nonlinear redshift distortions: The two-point correlation function
• Star-Forming Galaxies at z=0.24 in the Subaru Deep Field and the Sloan Digital Sky Survey
• A Constant Clustering Amplitude for Faint Galaxies?
• Scale Invariance of Rich Cluster Abundance: A Possible Test for Models of Structure Formation
• Optical identifications of $\sim 4000$ radio sources at the 1 mJy level
• Clustering of loose groups and galaxies from the Perseus--Pisces Survey
• The local environmental dependence of galaxy properties in the volume-limited sample of Main Galaxies from the SDSS Data Release 5
• Does the galaxy correlation length increase with the sample depth?
• The luminosity bias relation from filaments in the Sloan Digital Sky Survey Data Release Four
• Time evolution of the stochastic linear bias of interacting galaxies on linear scales
• Approaching a homogeneous galaxy distribution: results from the Stromlo-APM redshift survey
• Clustering of galaxies at 3.6 microns in the Spitzer Wide-area Infrared Extragalactic legacy survey
• Measuring galaxy segregation using the mark connection function
• The redshift evolution of bias and baryonic matter distribution
• The evolution of galaxy clustering since z=1 from the Calar Alto Deep Imaging Survey
• The ALHAMBRA survey: evolution of galaxy spectral segregation
• Detecting Scale-Dependence of Bias from APM-BGC Galaxies
• Luminosity Functions of XMM-LSS C1 Galaxy Clusters
• Galaxy Clustering at z ~ 2 and Halo Radii
• The ESO-Sculptor Survey: Evolution of late-type galaxies at redshifts 0.1-0.5
• Autocorrelations of stellar light and mass in the low-redshift Universe
• A Possible Effect of the Period of Galaxy Formation on the Angular Correlation Function
• Color dependence of clustering of massive galaxies at 0.5$\le z\le$2.5: similar spatial distributions between green valley galaxies and AGNs
• Abundances and Correlations of Structures Beyond Galaxy Clusters
• Correlation Function of Superclusters of Galaxies
• Galaxy Formation by Galactic Magnetic Fields
• Local Supercluster Dynamics: External Tidal Impact of the PSCz sample traced by Optimized Numerical Least Action Method
• Reconstruction Analysis of the IRAS Point Source Catalog Redshift Survey
• Cluster-Galaxy Correlations in CDM Models
• On the Effective Spatial Separations in the Clustering of Faint Galaxies
• Spatial clustering in the ESO-Sculptor Survey: two-point correlation functions by galaxy type at redshifts 0.1 - 0.5
• Measuring the Cosmic Web
• Estimating the K-function of a point process with an application to cosmology
• The spatial clustering of radio sources in NVSS and FIRST; implications for galaxy clustering evolution