Relationship between environment and the broad-band optical properties of galaxies in the SDSS

Abstract

We examine the relationship between environment and the luminosities, surface brightnesses, colors, and profile shapes of luminous galaxies in the Sloan Digital Sky Survey (SDSS). For the SDSS sample, galaxy color is the galaxy property most predictive of the local environment. Galaxy color and luminosity jointly comprise the most predictive pair of properties. At fixed luminosity and color, density is not closely related to surface brightness or to Sersic index -- the parameter in this study that astronomers most often associate with morphology. In the text, we discuss what measureable residual relationships exist, generally finding that at red colors and fixed luminosity, the mean density decreases at the highest surface brightnesses and Sersic indices. In general, these results suggest that the morphological properties of galaxies are less closely related to galaxy environment than are their masses and star-formation histories.

submitted to ApJ, pedagogy and bitmapped figures for presentations available at http://cosmo.nyu.edu/blanton/full_density.html

References in corpus (26)

• Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
• The Sloan Digital Sky Survey: Technical Summary
• Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Main Galaxy Sample
• The Sloan Digital Sky Survey Photometric Camera
• The u'g'r'i'z' Standard Star Network
• The Galaxy Luminosity Function and Luminosity Density at Redshift z=0.1
• Spectroscopic Target Selection for the Sloan Digital Sky Survey: The Luminous Red Galaxy Sample
• Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Quasar Sample
• The First Data Release of the Sloan Digital Sky Survey
• Astrometric Calibration of the Sloan Digital Sky Survey
• The Broad-band Optical Properties of Galaxies with Redshifts 0.0 < z < 0.2
• A photometricity and extinction monitor at the Apache Point Observatory
• Galaxy Clustering in Early SDSS Redshift Data
• An Efficient Algorithm for Positioning Tiles in the Sloan Digital Sky Survey
• Estimating Fixed Frame Galaxy Magnitudes in the SDSS
• The 2dF Galaxy Redshift Survey: The dependence of galaxy clustering on luminosity and spectral type
• The dependence on environment of the color-magnitude relation of galaxies
• The overdensities of galaxy environments as a function of luminosity and color
• Redshift-Space Distortions and the Real-Space Clustering of Different Galaxy Types
• Angular Clustering with Photometric Redshifts in the Sloan Digital Sky Survey: Bimodality in the Clustering Properties of Galaxies
• The two-point correlation function and morphological segregation in the Optical Redshift Survey
• A Photometric and Spectroscopic Study of Dwarf and Giant Galaxies in the Coma Cluster - IV. The Luminosity Function
• Evidence for Steep Luminosity Functions in Clusters of Galaxies
• The Concentration-Density Relation of Galaxies in Las Campanas Redshift Survey
• The redshift-space two-point correlation functions of galaxies and groups in the Nearby Optical Galaxy sample
• Deprojecting Densities from Angular Cross-Correlations

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• COWS: A filament finder for Hessian cosmic web identifiers
• The GOGREEN Survey: Constraining the Satellite Quenching Timescale in Massive Clusters at $\mathbf{z}\gtrsim 1$
• Euclid: Early Release Observations -- Overview of the Perseus cluster and analysis of its luminosity and stellar mass functions
• Red Misfits in the Sloan Digital Sky Survey: Properties of Star-forming Red Galaxies
• Comparing cosmic web classifiers using information theory
• X-ray Groups of Galaxies at 0.5<z<1 in zCOSMOS: Increased AGN Activities in High Redshift Groups
• The anatomy of the NGC 5044 group - I. Group membership and dynamics
• Halo models of HI selected galaxies
• Galaxies in X-ray Groups. III. Satellite Color and Morphology Transformations
• Anisotropic infall in the outskirts of OmegaWINGS galaxy clusters
• The Fornax3D project: Environmental effects on the assembly of dynamically cold disks in Fornax cluster galaxies
• The effect of environment on star formation activity and morphology at 0.5 < z < 2.5 in CANDELS
• Disc cloaking: Establishing a lower limit to the number density of local compact massive spheroids/bulges and the potential fate of some high-z red nuggets
• Local and large-scale effects on the astrophysics of void-galaxies
• OMEGA -- OSIRIS Mapping of Emission-line Galaxies in A901/2: II. -- Environmental influence on integrated star formation properties and AGN activity
• The CAVITY project. The spatially resolved stellar population properties of galaxies in voids
• The Stellar Mass Fundamental Plane and Compact Quiescent Galaxies at z < 0.6
• The cosmic web connection to the dark matter halo distribution through gravity
• The trajectories of galaxies in groups: mass loss and preprocessing
• On the Clustering of Faint Red Galaxies
• The stellar mass function of quiescent galaxies in 2 < z < 2.5 protoclusters
• Effects of galaxy environment on merger fraction
• Counts-in-Cylinders in the Sloan Digital Sky Survey with Comparisons to N-body Simulations
• On the relation between Seyfert 2 accretion rate and environment at z < 0.1
• AKARI Observation of the North Ecliptic Pole (NEP) Supercluster at z = 0.087: mid-infrared view of transition galaxies
• On the initial shear field of the cosmic web
• Substructure lensing in galaxy clusters as a constraint on low-mass sterile neutrinos in tensor-vector-scalar theory: The straight arc of Abell 2390
• The H$\alpha$ star formation main sequence in cluster and field galaxies at $z\sim 1.6$
• The anatomy of the NGC 5044 group -- II. Stellar populations and star-formation histories
• The stellar mass function and evolution of the density profile of galaxy clusters from the Hydrangea simulations at $0<z<1.5$
• Color, Structure, and Star Formation History of Dwarf Galaxies over the last ~3 Gyr with GEMS and SDSS
• HI gas content of SDSS galaxies revealed by ALFALFA: implications for the mass-metallicity relation and the environmental dependence of HI in the local Universe
• The strong environmental dependence of black hole scaling relations
• Relating bars with the environment in the nearby Universe
• Abundance ratios in dwarf elliptical galaxies
• Looking at quasars through galaxies
• Reconstructing the galaxy density field with photometric redshifts: II. Environment-dependent galaxy evolution since $z\simeq 3$
• Early-Type Galaxy Star Formation Histories in Different Environments
• The Properties of Massive Star-forming galaxies with Outside-in Assembly Mode
• Galaxy Properties in Clusters: Dependence on the Environment and the Cluster Identification Techniques
• Impact of cosmic filaments on the gas accretion rate of dark matter halos
• The impact of stellar bars on star-formation quenching: Insights from a spatially resolved analysis in the local Universe
• The Coevolution of Massive Quiescent Galaxies and Their Dark Matter Halos over the Last 6 Billion Years
• HI Galaxy Signatures in the SARAO MeerKAT Galactic Plane Survey -- II. The Local Void and its substructure
• The Effect of Halo Mass on the HI Content of Galaxies in Groups and Clusters
• The Neutral Hydrogen Properties of Galaxies in Gas-rich Groups
• How the Galaxy-Halo Connection Depends on Large-Scale Environment
• Estimating Sky Level
• OMEGA - OSIRIS Mapping of Emission-line Galaxies in A901/2: III. - Galaxy Properties Across Projected Phase Space in A901/2
• The Ursa Major cluster redefined as a `supergroup'
• The Voronoi tessellation method in astronomy
• The role of major gas-rich mergers on the evolution of galaxies from the blue cloud to the red sequence
• Uncovering Mass Segregation with Galaxy Analogues in Dark Matter Simulations
• Quenching or Bursting: Star Formation Acceleration--A New Methodology for Tracing Galaxy Evolution
• The dynamic stage of clusters and its influence on the stellar populations of galaxies
• Quiescent luminous red galaxies (LRGs) as cosmic chronometers: on the significance of mass and environmental dependence
• The XXL Survey: XXX. Characterisation of the XLSSsC N01 supercluster and analysis of the galaxy stellar populations
• Semi-Analytic Model Predictions of Mass Segregation from Groups to Clusters
• The Beyond-Halo Mass Effects of the Cosmic Web Environment on Galaxies
• Occurrence of LINER galaxies within the galaxy group environment
• Reconstructing Orbits of Galaxies in Extreme Regions (ROGER) II: reliability of projected phase-space in our understanding of galaxy populations
• Galaxy and Mass Assembly (GAMA): Tracing galaxy environment using the marked correlation function
• Groups of two galaxies in SDSS: implications of colours on star formation quenching time-scales
• Comparing galaxy disk and star-formation properties in X-ray bright and faint groups and clusters
• A Tale of Two Clusters: An Analysis of Gas-Phase Metallicity and Nebular Gas Conditions in Proto-cluster Galaxies at z~2
• The environmental dependence of the red galaxy sequence
• More connected, more active: galaxy clusters and groups at z~1 and the connection between their quiescent galaxy fractions and large-scale environments
• BANG-MaNGA: A census of kinematic discs and bulges across mass and star formation in the local Universe
• Revealing ringed galaxies in group environments
• Backsplash galaxies and their impact on galaxy evolution: a three-stage, four-type perspective
• Dissecting the morphological and spectroscopic properties of galaxies in the local Universe: I. Elliptical galaxies
• A New Perspective on the Large-Scale Tidal Effect on the Galaxy Luminosity and Morphology
• Colours of isolated galaxies selected from the Two-Micron All-Sky Survey
• The Properties of Type Ia Supernova Host Galaxies from the Sloan Digital Sky Survey
• Direct geometrical measurement of the Hubble constant from galaxy parallax: predictions for the Vera C. Rubin Observatory and Nancy Grace Roman Space Telescope
• Reconstructing Orbits of Galaxies in Extreme Regions (ROGER) III: galaxy evolution patterns in projected phase space around massive X-ray clusters
• Comparing galaxy populations in compact and loose groups of galaxies II: brightest group galaxies
• Lagrangian Methods Of Cosmic Web Classification
• Galaxy assembly bias in the stellar-to-halo mass relation for red central galaxies from SDSS
• The low mass end of the neutral gas mass and velocity width functions of galaxies in $\Lambda$CDM
• Kinematics of disk galaxies in (proto-)clusters at z=1.5
• Age and Metallicity of galaxies in different environments of the Coma supercluster
• The stellar mass function and efficiency of galaxy formation with a varying initial mass function
• The influence of galaxy surface brightness on the mass-metallicity relation
• The Occurrence of Compact Groups of Galaxies Through Cosmic Time
• The survival of stellar discs in Fornax-like environments, from TNG50 to real galaxies
• The dependence of cluster galaxy properties on the central entropy of their host cluster
• The XXL Survey XLV. Linking the ages of optically selected groups to their X-ray emission
• Galaxy-galaxy and galaxy-cluster lensing with the SDSS and FIRST surveys
• SED-inferred properties and morphology of Lyman-break galaxies at $z\sim 1$ in the CDF-S
• The impact of environment on the lives of disk galaxies as revealed by SDSS-IV MaNGA
• Stellar Population Properties of ETGs in Compact Groups of Galaxies
• Bimodal Formation Time Distribution for Infall Dark Matter Halos
• The Relative Role of Bars and Environments in AGN Triggering
• Continuous Filament Network of the Local Universe
• The effects of environment on galaxies' dynamical structures: From simulations to observations
• Satellites and central galaxies in SDSS: the influence of interactions on their properties
• Environmental effects on associations of dwarf galaxies
• Comparing IMF-sensitive indices of intermediate-mass quiescent galaxies in various environments
• Energetic constraints to chemo-photometric evolution of spiral galaxies
• Clustering properties and halo masses for central galaxies in the local Universe
• Ram pressure stripping in the z~0.5 galaxy cluster MS 0451.6-0305
• Evidence of Increased UV FeII Emission in Quasars in Candidate Overdense Regions
• Post-processing of galaxies due to major cluster mergers I. hints from galaxy colours and morphologies
• The roles of environment and interactions on the evolution of red and blue galaxies in the EAGLE simulation
• Environmental dependence of different colors in the CMASS sample of the SDSS DR9
• The Large Scale Structure in the Universe: From Power-Laws to Acoustic Peaks
• More than just halo mass: Modelling how the red galaxy fraction depends on multiscale density in a HOD framework
• The influence of superstructures on bright galaxy environments: clustering properties
• SOMBI: Bayesian identification of parameter relations in unstructured cosmological data
• Spatial clustering in the ESO-Sculptor Survey: two-point correlation functions by galaxy type at redshifts 0.1 - 0.5
• Particle Physics in the Sky and Astrophysics Underground: Connecting the Universe's Largest and Smallest Scales
• Insights into the dependence of galaxy properties on the environment with explainable machine learning models
• Impact of the large-scale cosmic web on the X-ray emitting circumgalactic medium
• On the relation of host properties and environment of AGN galaxies across the standard optical diagnostic diagram
• The impact of cosmic filaments on the abundance of satellite galaxies
• A group finder algorithm optimised for the study of local galaxy environment
• Mechanisms Affecting Galaxies Nearby and Environmental Trends (MAGNET)
• The Homogeneous Properties of Halpha-Selected Galaxies at (0.05<z<0.15)
• Exploring the evolution of red and blue galaxies in different cosmic web environments using IllustrisTNG simulation
• Lack of influence of the environment in the earliest stages of massive galaxy formation
• Exploring supermassive black hole physics and galaxy quenching across halo mass in FIRE cosmological zoom simulations
• Mapping Nearby Galaxies with Apache Point Observatory: Group and field galaxies' morphologies in the colour-magnitude plane
• Environmental Sculpting of Galaxy Structure at Fixed Stellar Mass: A Multi-Scale Analysis Across Cosmic Time using 3 Million HSC Galaxies
• Galaxy And Mass Assembly (GAMA): Deconstructing the galaxy stellar mass function by star formation and environment