The Environmental Dependence of the Relations between Stellar Mass, Structure, Star Formation and Nuclear Activity in Galaxies

Abstract

We use a complete sample of galaxies drawn from the SDSS to study how structure, star formation and nuclear activity depend on local density and on stellar mass. Local density is estimated by counting galaxies above a fixed absolute magnitude limit within cylinders 2 Mpc in projected radius and +-500 km/s in depth. The stellar mass distribution of galaxies shifts by nearly a factor of two towards higher masses between low and high density regions. At fixed stellar mass, both star formation and nuclear activity depend strongly on local density, while structural parameters such as size and concentration are almost independent of it. The galaxy property most sensitive to environment is specific star formation rate. For galaxies with stellar masses less than 3 x 10^10 M_sun, the median SFR/M* decreases by more than a factor of 10 from low to high densities. This decrease is less marked for massive galaxies. At fixed stellar mass, twice as many galaxies host AGN with strong [OIII] emission in low density regions as in high. Massive galaxies in low-density environments also contain more dust. We have analyzed correlations between spectroscopic indicators that probe SFH on different timescales (D4000, Hdelta_A and SFR/M*). The correlations do not depend on environment, suggesting that the decrease in star formation has ocurred over long (>1 Gyr) timescales. Since structure does not depend on environment for more massive galaxies, trends in recent SFH, dust and AGN for these systems cannot be driven by processes that alter structure, e.g. mergers. The SFH-density correlation is strongest for small scale (< 1 Mpc) estimates of local density. Finally, we highlight a striking similarity between changes in the galaxy population as a function of density and as a function of redshift and we interpret this using N-body simulations.

submitted to MNRAS, 35 pages

References in corpus (3)

• The physical properties of star forming galaxies in the low redshift universe
• Galaxy ecology: groups and low-density environments in the SDSS and 2dFGRS
• The Morphology-Density Relation in the Sloan Digital Sky Survey

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• LATIS: The Ly$\alpha$ Tomography IMACS Survey
• BayeSED: A General Approach to Fitting the Spectral Energy Distribution of Galaxies
• The stellar mass function of galaxies in Planck-selected clusters at 0.5 < z < 0.7: new constraints on the timescale and location of satellite quenching
• Active Galactic Nuclei in Groups and Clusters of Galaxies: Detection and Host Morphology
• The ACS Fornax Cluster Survey. IX. The Color-Magnitude Relation of Globular Cluster Systems
• Nearly all Massive Quiescent Disk Galaxies have a Surprisingly Large Atomic Gas Reservoir
• Triggering of merger-induced starbursts by the tidal field of galaxy groups and clusters
• Large-scale radio continuum properties of 19 Virgo cluster galaxies The influence of tidal interactions, ram pressure stripping, and accreting gas envelopes
• The Colors of Central and Satellite Galaxies in zCOSMOS out to z ~ 0.8 and Implications for Quenching
• The effect of environment on star forming galaxies at redshift 1 - First insight from PACS
• VLT and ACS observations of RDCS J1252.9-2927: dynamical structure and galaxy populations in a massive cluster at z=1.237
• The Spatial Clustering of Low Luminosity AGN
• What Are the Progenitors of Compact, Massive, Quiescent Galaxies at z=2.3? The Population of Massive Galaxies at z>3 from NMBS and CANDELS
• The Lifetime of FRIIs in Groups and Clusters: Implications for Radio-Mode Feedback
• Disentangling Morphology, Star Formation, Stellar Mass, and Environment in Galaxy Evolution
• Environmentally Driven Global Evolution of Galaxies
• Connecting Dark Matter Halos with the Galaxy Center and the Supermassive Black Hole
• The Void Galaxy Survey: Star Formation Properties
• GASP. XVI. Does cosmic web enhancement turn on star formation in galaxies?
• Galaxy interactions II: High density environments
• A homogeneous measurement of the delay between the onsets of gas stripping and star formation quenching in satellite galaxies of groups and clusters
• OmegaWINGS: The first complete census of post starburst galaxies in clusters in the local universe
• What triggers galaxy transformations? The environments of post-starburst galaxies
• A multiscale approach to environment and its influence on the colour distribution of galaxies
• A Kinematic Approach To Assessing Environmental Effects: Star-Forming Galaxies in a z~0.9 SpARCS cluster using Spitzer 24um Observations
• Chandra and XMM Observations of Type II Quasars from the SDSS
• Enhancement of AGN in a protocluster at z=1.6
• X-ray Bright Active Galactic Nuclei in Massive Galaxy Clusters II: The Fraction of Galaxies Hosting Active Nuclei
• Galaxy And Mass Assembly (GAMA): Testing galaxy formation models through the most massive galaxies in the Universe
• Tracing the Quenching History in Galaxy Clusters in the EAGLE Simulation
• Star formation in galaxies along the Pisces-Cetus Supercluster filaments
• The properties of the stellar populations in ULIRGs II: the star formation histories and evolution
• Star formation in galaxies falling into clusters along supercluster-scale filaments
• Metal-enriched halo gas across galaxy overdensities over the last 10 billion years
• Dust-Obscured Star-Formation in Intermediate Redshift Galaxy Clusters
• The distribution of galaxy morphological types and the morphology-mass relation in different environments at low redshift
• On the origin of gas-poor galaxies in galaxy clusters using cosmological hydrodynamic simulations
• The GOGREEN survey: Post-infall environmental quenching fails to predict the observed age difference between quiescent field and cluster galaxies at z>1
• SDSS IV MaNGA: Visual Morphological and Statistical Characterization of the DR15 sample
• The Evolution of Galaxies in X-ray Luminous Groups
• Photometric classification of emission line galaxies with Machine Learning methods
• Multiscale probability mapping: groups, clusters and an algorithmic search for filaments in SDSS
• YZiCS: Unveiling Quenching History of Cluster Galaxies Using Phase-space Analysis
• TheHaloMod: An online calculator for the halo model
• Caught in the cosmic web: Environmental effect on halo concentrations, shape, and spin
• On the fast quenching of young low-mass galaxies up to z $\sim$ 0.6: new spotlight on the lead role of environment
• SPLASH-SXDF Multi-wavelength Photometric Catalog
• Resolution-independent modeling of environmental effects in semi-analytic models of galaxy formation that include ram-pressure stripping of both hot and cold gas
• Galaxy properties in different environments up to z ~ 3 in the GOODS NICMOS Survey
• A Serendipitous XMM Survey of the SDSS: the evolution of the colour-magnitude diagram of X-ray AGN from z=0.8 to z=0.1
• Superclusters of galaxies in the 2dF redshift survey. III. The properties of galaxies in superclusters
• Activity in galactic nuclei of cluster and field galaxies in the local universe
• The Carnegie-Spitzer-IMACS Redshift Survey of Galaxy Evolution since z=1.5: I. Description and Methodology and More!
• The Roles of Mass and Environment in the Quenching of Galaxies. II
• The migration of nearby spirals from the blue to red sequence: AGN feedback or environmental effects?
• The environments of high redshift radio galaxies and quasars: probes of protoclusters
• GASP. XII. The variety of physical processes occurring in a single galaxy group in formation
• YZiCS: Preprocessing of dark halos in the hydrodynamic zoom-in simulation of clusters
• NoSOCS in SDSS. VI. The Environmental Dependence of AGN in Clusters and Field in the Local Universe
• The Gravitational Lens -- Galaxy Group Connection. II. Groups Associated with B2319+051 and B1600+434
• Star formation in high-redshift quasars: excess [O II] emission in the radio-loud population
• The Evolution of Dusty Star formation in Galaxy Clusters to z = 1: Spitzer IR Observations of the First Red-Sequence Cluster Survey
• The fundamental plane of isolated early-type galaxies
• Backsplash galaxies in isolated clusters
• A radio-to-mm census of star-forming galaxies in protocluster 4C23.56 at z=2.5 : Gas mass and its fraction revealed with ALMA
• The impact of galaxy formation on satellite kinematics and redshift-space distortions
• WALLABY Early Science - III. An HI Study of the Spiral Galaxy NGC 1566
• The MAGPI Survey -- science goals, design, observing strategy, early results and theoretical framework
• Two Growing Modes and the Morphology-Quiescence Relation in Galaxies
• Environmental dependence of AGN activity. I.: the effects of host galaxy
• The cosmic web of the Local Universe: cosmic variance, matter content and its relation to galaxy morphology
• A large scale structure traced by [OII] emitters hosting a distant cluster at z=1.62
• CLASH-VLT: Abell~S1063. Cluster assembly history and spectroscopic catalogue
• COLD GASS, an IRAM Legacy Survey of Molecular Gas in Massive Galaxies: III. Comparison with semi-analytic models of galaxy formation
• Local Benchmarks for the Evolution of Major-Merger Galaxies -- Spitzer Observations of a K-Band Selected Sample
• The Phase Space of z~1.2 SpARCS Clusters: Using Herschel to probe Dust Temperature as a Function of Environment and Accretion History
• The origin of the enhanced metallicity of satellite galaxies
• The Pisces-Cetus Supercluster: a remarkable filament of galaxies in the 2dF Galaxy Redshift Survey and Sloan Digital Sky surveys
• Galaxy evolution in protoclusters
• The complete census of optically selected AGNs in the Coma Supercluster: the dependence of AGN activity on the local environment
• Galaxy Zoo: The interplay of quenching mechanisms in the group environment
• PRIMUS: Enhanced Specific Star Formation Rates In Close Galaxy Pairs
• Measuring galaxy environments in large scale photometric surveys
• Star formation and nuclear activity in close pairs of early-type galaxies
• The Void Galaxy Survey: Photometry, structure and identity of void galaxies
• The spectral-type/luminosity and the spectral type/satellite-density relations in the 2dFGRS
• Galaxy mass, cluster-centric distance and secular evolution: their role in the evolution of galaxies in clusters in the last 10 Gyr
• The dependence of galaxy group star formation rates and metallicities on large scale environment
• Does black-hole growth depend on the cosmic environment?
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). The decline of cosmic star formation: quenching, mass, and environment connections
• Triggering Active Galactic Nuclei in galaxy clusters
• Revealing the Dark Threads of the Cosmic Web
• The Accelerated Build-up of the Red Sequence in High Redshift Galaxy Clusters
• Extracting Star Formation Histories from Medium-resolution Galaxy Spectra
• TARDIS Paper I: A Constrained Reconstruction Approach to Modeling the z~2.5 Cosmic Web Probed by Lyman-alpha Forest Tomography
• The enhancement of rapidly quenched galaxies in distant clusters at 0.5<z<1.0
• A New Method to Quantify Environment and Model Ram-Pressure Stripping in N-Body Simulations
• Reversal or no reversal: the evolution of the star formation rate-density relation up to z~1.6
• X-ray Bright Active Galactic Nuclei in Massive Galaxy Clusters I: Number Counts and Spatial Distribution
• The Cosmic Evolution of Faint Satellite Galaxies as a Test of Galaxy Formation and the Nature of Dark Matter
• Exploring galaxy colour in different environments of the cosmic web with SDSS
• Galaxy And Mass Assembly (GAMA): Gas Fuelling of Spiral Galaxies in the Local Universe I. - The Effect of the Group Environment on Star Formation in Spiral Galaxies
• The clustering of barred galaxies in the local Universe
• The origin of the red sequence galaxy population in the EAGLE simulation
• The Fraction of Active Galactic Nuclei in the USS 1558-003 Protocluster at z = 2.53
• Nature versus nurture: what regulates star formation in satellite galaxies?
• The fate of the gaseous disks of galaxies that fall into clusters
• The AMIGA sample of isolated galaxies. XI. Optical characterisation of nuclear activity
• Halo Histories vs. Galaxy Properties at z=0, I: The Quenching of Star Formation
• Morphologies of Galaxies in and around a Protocluster at z=2.300
• The host galaxies of long-duration GRBs in a cosmological hierarchical scenario
• The Chemical and Ionization Conditions in Weak Mg II Absorbers
• Conditional Quenching: A detailed look at the SFR-Density Relation at z ~ 0.9 from ORELSE
• Hidden Starbursts and Active Galactic Nuclei at 0<z<4 from the Herschel-VVDS-CFHTLS-D1 Field: Inferences on Coevolution and Feedback
• Isolated galaxies in hierarchical galaxy formation models - present-day properties and environmental histories
• Multiscale cosmic web detachments, connectivity, and preprocessing in the supercluster SClA2142 cocoon
• Is there enough star formation in simulated protoclusters?
• Effects on Galaxy Evolution: Pair Interactions versus Environment
• The Dependence of AGN Activity on Environment in SDSS
• The Environment of Galaxies at Low Redshift
• The VIMOS VLT Deep Survey: the group catalogue
• Satellite Quenching, Galaxy Inner Density and the Halo Environment
• Exploring the halo occupation of AGN using dark-matter cosmological simulations
• The Fornax3D project: Assembly histories of lenticular galaxies from a combined dynamical and population orbital analysis
• Comparisons of the environmental dependence of galaxy properties between galaxies above and below M
• Do star formation rates of galaxy clusters depend on mass?: blue/late-type fractions, total star formation rates of 115 galaxy clusters as a function of cluster virial mass
• Evolution of Star-formation Properties of High-redshift Cluster Galaxies since $z=2$
• A journey from the outskirts to the cores of groups I: Color- and mass-segregation in 20K-zCOSMOS groups
• Black Hole Mass, Host galaxy classification and AGN activity
• Supermassive Black Holes and Their Environments
• Mass and Redshift Dependence of Star Formation in Relaxed Galaxy Clusters
• Stellar mass-gap as a probe of halo assembly history and concentration: youth hidden among old fossils
• Galaxy Environments in the UKIDSS Ultra Deep Survey (UDS)
• The Fornax Deep Survey with VST. X. The assembly history of the bright galaxies and intra-group light in the Fornax A subgroup
• The Three Hundred Project: The influence of environment on simulated galaxy properties
• Spitzer Planck Herschel Infrared Cluster (SPHerIC) survey: Candidate galaxy clusters at 1.3 < z < 3 selected by high star-formation rate
• The ($NUV-r$) vs. $M_r$ as a tracer of early-type galaxies evolution in USGC U376 and LGG 225 groups
• KAT-7 Science Verification: Cold Gas, Star Formation, and Substructure in the Nearby Antlia Cluster
• Quantitative Morphology of Galaxies from the SDSS I: Luminosity in Bulges and Disks
• The environmental dependence of clustering in hierarchical models
• The Tully-Fisher Relation for 25,000 SDSS Galaxies as Function of Environment
• X-ray selected AGN in groups at redshifts z~1
• How much a galaxy knows about its large-scale environment?: An information theoretic perspective
• Galaxy Merger Candidates in High-Redshift Cluster Environments
• Star Formation and AGN Activity in Interacting Galaxies: A Near-UV Perspective
• Distribution of satellite galaxies in high redshift groups
• Galaxy And Mass Assembly (GAMA): The environments of high- and low- excitation radio galaxies
• NoSOCS in SDSS III - The interplay between galaxy evolution and the dynamical state of galaxy clusters
• Deep Realistic Extragalactic Model (DREaM) Galaxy Catalogs: Predictions for a Roman Ultra-Deep Field
• High-order 3D Voronoi tessellation for identifying Isolated galaxies, Pairs and Triplets
• A Wide-Field Study of the z~0.8 Cluster RX J0152.7-1357: the Role of Environment in the Formation of the Red-Sequence
• Investigating the Relation between Galaxy Properties and the Gaussianity of the Velocity Distribution of Groups and Clusters
• Hot and Cold Galactic Gas in the NGC 2563 Galaxy Group
• Modelling narrow-line regions of active galaxies in the Sloan Digital Sky Survey - I.Sample selection and physical conditions
• Evidence of Environmental Quenching at Redshift z ~ 2
• Early-type galaxies at z~1.3. II. Masses and ages of early-type galaxies in different environments and their dependence on stellar population model assumptions
• Accelerated galaxy growth and environmental quenching in a protocluster at z=3.24
• Galaxy pre-processing in substructures around z$\sim$0.4 galaxy clusters
• Semi-empirical analysis of Sloan Digital Sky Survey galaxies: IV. A nature via nurture scenario for galaxy evolution
• Deep Synoptic Array science: A massive elliptical host among two galaxy-cluster fast radio bursts
• Mergers as triggers for nuclear activity: A near-IR study of the close environment of AGN in the VISTA-VIDEO survey
• Non-parametric Morphologies of Galaxies in the EAGLE Simulation
• The Grism lens-amplified survey from space (GLASS). VII. The diversity of the distribution of star formation in cluster and field galaxies at 0.3<z<0.7
• GAMA/H-ATLAS: Linking the Properties of Sub-mm Detected and Undetected Early-Type Galaxies: I. z$\le$0.06 Sample
• Specific Frequencies and Luminosity Profiles of Cluster Galaxies and Intracluster Light in Abell 1689
• The Effect of Environment on Discs and Bulges
• Similar Scaling Relations for the Gas Content of Galaxies across Environments to z ~ 3.5
• The SAMI Galaxy Survey: Mass and Environment as Independent Drivers of Galaxy Dynamics
• Crowded Field Galaxy Photometry: Precision Colors in the CLASH Clusters
• The Dependence of the Mass-Metallicity Relation on Large Scale Environment
• An orbital perspective on the starvation, stripping, and quenching of satellite galaxies in the EAGLE simulations
• The effect of cosmic web filaments on galaxy evolution
• Galaxy environments over cosmic time: the non-evolving radial galaxy distributions around massive galaxies since z=1.6
• Strong lensing statistics in large, z~<0.2 surveys: bias in the lens galaxy population
• A catalogue of structural and morphological measurements for DES Y1
• Revealing the z~2.5 Cosmic Web With 3D Lyman-Alpha Forest Tomography: A Deformation Tensor Approach
• HI-deficient galaxies in intermediate density environments
• The nature of red dwarf galaxies
• The morphological transformation and the quenching of galaxies
• Gravitational Potential and Surface Density Drive Stellar Populations -- II. Star-Forming Galaxies
• Probing the existence of a rich galaxy overdensity at z=5.2
• Evolution of the brightest cluster galaxies: the influence of morphology, stellar mass and environment
• Effects of large-scale environment on the assembly history of central galaxies
• Local primordial non-Gaussianity from the large-scale clustering of photometric DESI luminous red galaxies
• Compact groups in theory and practice -- IV. The connection to large-scale structure
• How to Optimally Constrain Galaxy Assembly Bias: Supplement Projected Correlation Functions with Count-in-cells Statistics
• CO Emission, Molecular Gas, and Metallicity in Main-Sequence Star-Forming Galaxies at $z\sim 2.3$
• Too dense to go through: The importance of low-mass clusters for satellite quenching
• The XXL survey XXXV. The role of cluster mass in AGN activity
• IQ Collaboratory II: The Quiescent Fraction of Isolated, Low Mass Galaxies Across Simulations and Observations
• Effect of local and large-scale environments on nuclear activity and star formation
• Dependence of Star Formation Activity On Stellar Mass and Environment From the Redshift One LDSS-3 Emission Line Survey (ROLES)
• BIRTH of the COSMOS Field: Primordial and Evolved Density Reconstructions During Cosmic High Noon
• Properties and environment of Radio Emitting Galaxies in the VLA-zCOSMOS survey
• Stellar masses, sizes, and radial profiles for 465 nearby early-type galaxies: an extension to the Spitzer Survey of Stellar Structure in Galaxies (S${}^4$G)
• Linking haloes to galaxies: how many halo properties are needed?
• Deep Investigation of Neutral Gas Origins (DINGO): HI stacking experiments with early science data
• Star formation, starbursts and quenching across the Coma supercluster
• The Metallicity of Diffuse Intrahalo Light
• The Gentle Growth of Galaxies at High Redshifts in Overdense Environments
• Spectral Properties of Galaxies in Void Regions
• Flows around galaxies. I. The dependency of galaxy connectivity on cosmic environments and effects on the star-formation rate
• An high definition view of the COSMOS Wall at z~0.73
• Gas Loss in Simulated Galaxies as They Fall into Clusters
• Gas depletion in cluster galaxies depends strongly on their internal structure
• Ages and Metallicities of Early-Type Void Galaxies from Line Strength Measurements
• Modeling Galaxy-Galaxy Weak Lensing with SDSS Groups
• The effects of LMC-mass environments on their dwarf satellite galaxies in the FIRE simulations
• The SPLASH survey: Quiescent galaxies are more strongly clustered but are not necessarily located in high-density environments
• The DEEP2 Galaxy Redshift Survey: The Red Sequence AGN Fraction and its Environment and Redshift Dependence
• VIS3COS: II. Nature and nurture in galaxy structure and morphology
• In and out star formation in z~1.5 quiescent galaxies from rest-frame UV spectroscopy and the far-infrared
• Study of galaxies on large-scale filaments in simulations
• AGN environments at z<1.5 in the UKIDSS Ultra-Deep Survey
• On the orbital and internal evolution of cluster galaxies
• WALLABY Pilot Survey: HI gas disc truncation and star formation of galaxies falling into the Hydra I cluster
• Evidence for Two Distinct Stellar Initial Mass Functions
• The galaxy size - halo mass scaling relations and clustering properties of central and satellite galaxies
• Local and global environmental effects on galaxies and active galactic nuclei
• Ultracompact Blue Dwarf Galaxies: Hubble Space Telescope Imaging and Stellar Population Analysis
• Structure in the 3D Galaxy Distribution: I. Methods and Example Results
• A few StePS forward in unveiling the complexity of galaxy evolution: light-weighted stellar ages of intermediate redshift galaxies with WEAVE
• Changing Ionization Conditions in SDSS Galaxies with AGN as a Function of Environment from Pairs to Clusters
• The GOGREEN survey: Dependence of galaxy properties on halo mass at z > 1 and implications for environmental quenching
• Brightest group galaxies and the large-scale environment
• X-ray AGN in the XMM-LSS galaxy clusters: no evidence of AGN suppression
• The Role of Environment on the Formation of Early-Type Galaxies
• Lower AGN Abundance in Galaxy Clusters at z < 0.5
• Morphology rather than environment drives the SFR-Mass relation in the local universe
• HST/WFC3 grism observations of $z\sim 1$ clusters: Evidence for rapid outside-in environmental quenching from spatially resolved H$\alpha$ maps
• The weak imprint of environment on the stellar populations of galaxies
• What do simulations predict for the galaxy stellar mass function and its evolution in different environments?
• Spatially Offset Active Galactic Nuclei. II: Triggering in Galaxy Mergers
• The interstellar medium and feedback in the progenitors of the compact passive galaxies at z~2
• VIS3COS: I. survey overview and the role of environment and stellar mass on star formation
• The definition of environment and its relation to the quenching of galaxies at z=1-2 in a hierarchical Universe
• Observational constraints on the physics behind the evolution of AGN since z ~ 1
• Stellar Mass Growth of Brightest Cluster Galaxy Progenitors in COSMOS Since z ~ 3
• Passive galaxies as tracers of cluster environments at z~2
• Implications of the Environments of Radio-detected AGN in a Complex Protostructure at z$\sim$3.3
• WALLABY Pre-Pilot Survey: The effects of tidal interaction on radial distribution of color in galaxies of the Eridanus supergroup
• A detailed study of massive galaxies in a protocluster at z=3.13
• VIS3COS: III. environmental effects on the star formation histories of galaxies at z~0.8 seen in [OII], H$\delta$, and Dn4000
• Tracing high redshift cosmic web with quasar systems
• The time delay between star formation quenching and morphological transformation of galaxies in clusters: a phase-space view of EDisCS
• Galaxy Luminosities in 2PIGG groups
• The Nuclear Outflows and Feedback in the Seyfert 2 Galaxy Markarian 573
• XMM-Newton Surveys of the Canada-France Redshift Survey Fields - III: The Environments of X-ray Selected AGN at 0.4<z<0.6
• ECO and RESOLVE: Galaxy Disk Growth in Environmental Context
• NoSOCS in SDSS. V. Red Disc and Blue Bulge Galaxies Across Different Environments
• An IFU View of the Active Galactic Nuclei in MaNGA Galaxy Pairs
• Star formation and environment in clusters up to z~2.2
• The miniJPAS survey: The role of group environment in quenching the star formation
• The environment of AGN dwarf galaxies at z$\sim$0.7 from the VIPERS survey
• GOGREEN: a critical assessment of environmental trends in cosmological hydrodynamical simulations at z ~ 1
• An AGN with an ionized gas outflow in a massive quiescent galaxy in a protocluster at $\mathbf{z}=3.09$
• Environments of Nearby Quasars in Sloan Digital Sky Survey
• Is the cluster environment quenching the Seyfert activity in elliptical and spiral galaxies?
• DustPedia - the relationships between stars, gas and dust for galaxies residing in different environments
• MAMMOTH: Confirmation of Two Massive Galaxy Overdensities at $z=2.24$ with H$\alpha$ Emitters
• Evidence of Galaxy Assembly Bias in SDSS DR7 Galaxy Samples from Count Statistics
• Measures of Galaxy Environment - III. Difficulties in identifying proto-clusters at z ~ 2
• Obscured star-formation and environment in the COSMOS field
• Classification and environmental properties of X-ray selected point-like sources in the XMM-LSS field
• Do group dynamics play a role in the evolution of member galaxies?
• Living with Neighbors. I. Observational Clues to Hydrodynamic Impact of Neighboring Galaxies on Star Formation
• NoSOCS in SDSS. IV. The Role of Environment Beyond the Extent of Galaxy Clusters
• High-resolution ALMA study of CO (2-1) line and dust continuum emissions in cluster galaxies at z = 1.46
• Chandra reveals a luminous Compton-thick QSO powering a $Ly\alpha$ blob in a $z=4$ starbursting protocluster
• Revealing HI gas in emission and absorption on pc to kpc scales in a galaxy at z ~ 0.017
• Preprocessing, mass loss and mass segregation of galaxies in DM simulations
• CO($J$=1-0) mapping survey of 64 galaxies in the Fornax cluster with the ALMA Morita array
• Low and High Surface Brightness Galaxies at Void Walls
• The First Mid-IR View of the Star-forming Properties of Nearby Galaxy Groups
• Properties of Long Gamma-Ray Burst Host Galaxies in Cosmological Simulation
• Role of environment on nuclear activity
• Spatial Clustering from GALEX-SDSS samples: Star Formation History and large-scale clustering
• Discovery of Protoclusters at z~3.7 & 4.9: Embedded in Primordial Superclusters
• A deep Parkes HI survey of the Sculptor group and filament: HI mass function and environment
• Determining the Halo Mass Scale where Galaxies Lose Their Gas
• Multi-frequency studies of galaxies and groups: I. Environmental effect on galaxy stellar mass and morphology
• The effect of environment on AGN activity: the properties of radio and optical AGN in void, isolated and group galaxies
• Large Scale Structures in COSMOS2020: Evolution of Star Formation Activity in Different Environments at 0.4 < z < 4
• Molecular gas in two companion cluster galaxies at z=1.2
• Characterizing Protoclusters and Protogroups at z $\sim$ 2.5 Using Ly$\alpha$ Tomography
• Caught in the act: Cluster `k+a' galaxies as a link between spirals and S0s
• Environmental Enhancement of DM Haloes
• The mass and environmental dependence on the secular processes of AGN in terms of morphology, colour, and specific star-formation rate
• Euclid: The selection of quiescent and star-forming galaxies using observed colours
• Alignment between satellite and central galaxies in the SDSS DR7: dependence on large-scale environment
• The Evolution and Environments of X-ray Emitting Active Galactic Nuclei in High-Redshift Large-Scale Structures
• Emission Line Galaxies and Active Galactic Nuclei in WINGS clusters
• The Grism lens-amplified survey from space (GLASS). VIII. The influence of the cluster properties on Halpha emitter galaxies at 0.3<z<0.7
• Galaxy Rotation Coherent with the Motions of Neighbors: Discovery of Observational Evidence
• Galaxy And Mass Assembly (GAMA): The Bright Void Galaxy Population in the Optical and Mid-IR
• HI Selected Galaxies in the Sloan Digital Sky Survey II: The Colors of Gas-Rich Galaxies
• Properties of brightest group galaxies in cosmic web filaments
• Seyfert galaxies that are undergoing merging but appear non-interacting
• A study on the statistical significance of mutual information between morphology of a galaxy and its large-scale environment
• The Variation of the Galaxy Luminosity Function with Group Properties
• The relation between morphology, star formation history, and environment in local universe galaxies
• The Evolution of [OII] Emission from Cluster Galaxies
• A survey of weak MgII absorbers at redshift <z>=1.78
• Morphological Segregation in the Surroundings of Cosmic Voids
• A complete spectroscopic catalogue of local galaxies in the Northern spring sky -- Gas properties and nuclear activity in different environments
• The stellar populations of early-type galaxies -- II. The effects of environment and mass
• The evolution of the bi-modal colour distribution of galaxies in SDSS groups
• Multiband galaxy morphologies for CLASH: a convolutional neural network transferred from CANDELS
• X-ray Groups of Galaxies at 0.5<z<1 in zCOSMOS: Increased AGN Activities in High Redshift Groups
• Red Misfits in the Sloan Digital Sky Survey: Properties of Star-forming Red Galaxies
• Hidden activity in high-redshift spheroidal galaxies from mid-infrared and X-ray observations in the GOODS-North field
• Environmental processing in cluster core galaxies at z=1.7
• ALMA/ACA CO Survey of the IC 1459 and NGC 4636 Groups: Environmental Effects on the Molecular Gas of Group Galaxies
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• Robust automatic photometry of local galaxies from SDSS Dissecting the color magnitude relation with color profiles
• WEAVE-StePS. A stellar population survey using WEAVE at WHT
• Uncovering the formation of ultra-compact dwarf galaxies by multivariate statistical analysis
• Differences in the structural properties and star-formation rates of field and cluster galaxies at z~1
• Galaxies in X-ray Groups. III. Satellite Color and Morphology Transformations
• The submillimetre view of massive clusters at z~0.8-1.6
• Clustercentric distance or local density? It depends on galaxy morphology
• The effect of environment on star formation activity and morphology at 0.5 < z < 2.5 in CANDELS
• The Three Hundred project: connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
• Local and large-scale effects on the astrophysics of void-galaxies
• Shaping physical properties of galaxy subtypes in the VIPERS survey: environment matters
• PRIMUS: Obscured Star Formation on the Red Sequence
• Star-formation quenching of cluster galaxies as traced by metallicity, presence of active galactic nuclei, and galactic conformity
• The XXL Survey: XII. Optical spectroscopy of X-ray-selected clusters and the frequency of AGN in superclusters
• MaNGA galaxy properties -- I. An extensive optical, mid-infrared photometric, and environmental catalogue
• The density of dark matter haloes of early-type galaxies in low-density environments
• The anatomy of the NGC 5044 group - I. Group membership and dynamics
• The Role of Galaxy Interaction in Environmental Dependence of the Star Formation Activity at z~1.2
• The Case for Strangulation in Low-Mass Hosts: DDO 113
• Clustering Properties of restframe UV selected galaxies I: the correlation length derived from GALEX data in the local Universe
• Physical Properties of Weak MgII Absorbers at z~2
• The Effect of Environment on Galaxy Spiral Arms, Bars, Concentration, and Quenching
• AKARI Observation of the North Ecliptic Pole (NEP) Supercluster at z = 0.087: mid-infrared view of transition galaxies
• The impact of protocluster environments at z = 1.6
• A tool for the morphological classification of galaxies: the concentration index
• The trajectories of galaxies in groups: mass loss and preprocessing
• The cosmic web connection to the dark matter halo distribution through gravity
• Counts-in-Cylinders in the Sloan Digital Sky Survey with Comparisons to N-body Simulations
• Effects of galaxy environment on merger fraction
• Nature vs. nurture in the low-density environment: structure and evolution of early-type dwarf galaxies in poor groups
• One-Two Quench: A Double Minor Merger Scenario
• Analytical halo model of galactic conformity
• The Clustering and Halo Masses of Star Forming Galaxies at z<1
• Environmental Effect on the Interstellar Medium in Galaxies across the Cosmic Web at z=0.73
• Dichotomy in host environments and signs of recycled AGN
• NUV signatures of environment driven galaxy quenching in SDSS groups
• The role of stellar mass and environment for cluster blue fraction, AGN fraction and star-formation indicators from a targeted analysis of Abell 1691
• A Multi-wavelength Survey of AGN in Massive Clusters: AGN Detection and Cluster AGN Fraction
• The clustering of X-ray AGN at 0.5 < z < 4.5: host galaxies dictate dark matter halo mass
• On the accretion of a new group of galaxies onto Virgo: II. The effect of pre-processing on the stellar population content of dEs
• Forensic reconstruction of galaxy colour evolution and population characterisation
• The XXL Survey: XXXVII. The role of the environment in shaping the stellar population properties of galaxies at 0.1<z<0.5
• Effect of richness on AGN and star formation activities in SDSS galaxy groups
• The Kinematics of Cluster Galaxies via Velocity Dispersion Profiles
• Observational evidence for AGN fueling. I. The merging of NGC6104 with a companion
• ZFIRE: Measuring Electron Density with [OII] as a function of environment at z = 1.62
• Morphological Dependence of Star Formation Properties for the Galaxies in the Merging Galaxy Cluster A2255
• {\em Herschel}-ATLAS/GAMA: The Environmental Density of Far-Infrared Bright Galaxies at $z\le 0.5$
• On the Reversal of SFR-Density Relation at z=1: Insights from Simulations
• Deep Extragalactic VIsible Legacy Survey (DEVILS): Evolution of the ${\sigma }_{\mathrm{SFR}}$-M${}_{\star }$ relation and implications for self-regulated star formation
• The Differing Relationships Between Size, Mass, Metallicity and Core Velocity Dispersion of Central and Satellite Galaxies
• Tidal Interactions and Mergers in Intermediate Redshift EDisCS Clusters
• The anatomy of the NGC 5044 group -- II. Stellar populations and star-formation histories
• VERTICO V: The environmentally driven evolution of the inner cold gas discs of Virgo cluster galaxies
• The H$\alpha$ star formation main sequence in cluster and field galaxies at $z\sim 1.6$
• The stellar mass function and evolution of the density profile of galaxy clusters from the Hydrangea simulations at $0<z<1.5$
• The effect of the environment on the Faber Jackson relation
• Evolution of galaxies in groups in the Coma Supercluster
• Galaxy quenching timescales from a forensic reconstruction of their colour evolution
• Evidence for gas-phase metal deficiency in massive protocluster galaxies at z~2.2
• The Phoenix Deep Survey: The star-formation rates and the stellar masses of EROs
• The formation of bulges and black holes: lessons from a census of active galaxies in the SDSS
• The Environment of Local Ultraluminous Infrared Galaxies
• Measuring the total infrared light from galaxy clusters at z=0.5-1.6: connecting stellar populations to dusty star formation
• Quasars as a tracer of large-scale structures in the distant universe
• HectoMAP: The Complete Redshift Survey (Data Release 2)
• Morphology-dependent trends of galaxy age with environment in Abell 901/902 seen with COMBO-17
• Imprints of Environment on Cluster and Field Late-type Galaxies at z~1
• What Regulates Galaxy Evolution? Open Questions in Our Understanding of Galaxy Formation and Evolution
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs -- II. The catalogue
• Reconstructing the galaxy density field with photometric redshifts: II. Environment-dependent galaxy evolution since $z\simeq 3$
• Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model. II. The colour-density relation up to z=1.5
• The Global Environment of Small Galaxy Systems
• The environmental dependence of X-ray AGN activity at $z\sim 0.4$
• The large-scale structure around the Fornax-Eridanus Complex
• Spectroscopic Identifications of SWIRE sources in ELAIS-N1
• The evolution of the density of galaxy clusters and groups: denser environments at higher redshifts
• On The Effect of Environment on Line Emission from the Circumgalactic Medium
• The SDSS Discovery of a Strongly Lensed Post-Starburst Galaxy at z=0.766
• A Multi-Wavelength Study of Low Redshift Clusters of Galaxies I. Comparison of X-ray and Mid-Infrared Selected AGNs
• SSGSS: The Spitzer-SDSS-GALEX Spectroscopic Survey
• Star-formation rates of cluster galaxies: nature vs nurture
• The Properties of Massive Star-forming galaxies with Outside-in Assembly Mode
• K-CLASH: Strangulation and Ram Pressure Stripping in Galaxy Cluster Members at 0.3 < z < 0.6
• Impact of cosmic filaments on the gas accretion rate of dark matter halos
• Using galaxy pairs to investigate the three-point correlation function in the squeezed limit
• Galaxy interactions in filaments and sheets: effects of the large-scale structures versus the local density
• A Novel Method to Identify AGNs Based on Emission Line Excess and the Nature of Low-luminosity AGNs in the Sloan Digital Sky Survey: II - Nature of Low-luminosity AGNs
• The Neutral Hydrogen Properties of Galaxies in Gas-rich Groups
• GLACE survey: OSIRIS/GTC Tuneable Filter H$\alpha$ imaging of the rich galaxy cluster ZwCl 0024.0+1652 at z = 0.395. Part I -- Survey presentation, TF data reduction techniques and catalogue
• The Coevolution of Massive Quiescent Galaxies and Their Dark Matter Halos over the Last 6 Billion Years
• How the Galaxy-Halo Connection Depends on Large-Scale Environment
• Host galaxies of long gamma-ray bursts in the Millennium Simulation
• Evolution of Galaxy Types and HI Gas Contents in Galaxy Groups
• Subaru Hyper Suprime-Cam revisits the large-scale environmental dependence on galaxy morphology over 360 deg${}^2$ at z=0.3-0.6
• Green valley galaxies in the cosmic web: internal versus environmental quenching
• A z=1.85 galaxy group in CEERS: evolved, dustless, massive intra-halo light and a brightest group galaxy in the making
• SITELLE Hα Imaging Spectroscopy of z~0.25 Clusters: Emission Line Galaxy Detection and Ionized Gas Offset in Abell 2390 & Abell 2465
• A possible signature of the influence of tidal perturbations in dwarf galaxy scaling relations
• Morphological Parameters and Associated Uncertainties for 8 Million Galaxies in the Hyper Suprime-Cam Wide Survey
• The miniJPAS survey: The galaxy populations in the most massive cluster in miniJPAS, mJPC2470-1771
• The relation between galaxy density and radio jet power for 1.4 GHz VLA selected AGN in Stripe 82
• Timescales for Hi consumption and SFR depletion of satellite galaxies in groups
• AGN pairs: chance superpositions or black hole binaries?
• CLASH-VLT: Enhancement of (O/H) in z=0.35 RXJ 2248-4431 cluster galaxies
• The Ursa Major cluster redefined as a `supergroup'
• The Structural Evolution of Isolated Galaxies at Low Redshift in the IllustrisTNG Simulation
• The mass dependence of structure, star formation rate, and mass assembly mode at 0.5<z< 2.5
• Resolved Stellar Mass Maps of Galaxies in the Hubble Frontier Fields: Evidence for Mass Dependency in Environmental Quenching
• Hubble Space Telescope Imaging of the Ultracompact Blue Dwarf Galaxy HS 0822+3542: An Assembling Galaxy in a Local Void?
• The Velocity Dispersion Function for Quiescent Galaxies in Nine Strong-Lensing Clusters
• The Roles of Mass and Environment in the Quenching of Galaxies
• Uncovering Mass Segregation with Galaxy Analogues in Dark Matter Simulations
• OMEGA -- OSIRIS Mapping of Emission-line Galaxies in A901/2: I.-- Survey description, data analysis, and star formation and AGN activity in the highest density regions
• A catalogue of faint local radio AGN and the properties of their host galaxies
• Bulgeless galaxies in the COSMOS field: environment and star formation evolution at $z<1$
• Environments of dwarf galaxies with optical AGN characteristics
• YZiCS: On the Mass Segregation of Galaxies in Clusters
• The role of major gas-rich mergers on the evolution of galaxies from the blue cloud to the red sequence
• Do cluster properties affect the quenching rate?
• On the nature of Small Galaxy Systems
• Semi-Analytic Model Predictions of Mass Segregation from Groups to Clusters
• On radio-bright Active Galactic Nuclei in a complete Spectroscopic Redshift Survey
• Revealing the quiescent galaxy population in the Spiderweb protocluster at z=2.16 with deep HST/WFC3 slitless spectroscopy
• The VIMOS Public Extragalactic Redshift Survey (VIPERS) -- Environment-size relation of massive passive galaxies at 0.5 < z < 0.8
• The Infrared Medium-Deep Survey II: How to Trigger Radio-AGN? Hints from Their Environments
• Questioning Planck-selected star-forming high-redshift galaxy protoclusters and their fate
• Evolution of the Population of Very Strong MgII Absorbers
• The dynamic stage of clusters and its influence on the stellar populations of galaxies
• The Local Cluster Survey II: Disk-Dominated Cluster Galaxies with Suppressed Star Formation
• The effect of the environment on the structure, morphology and star-formation history of intermediate-redshift galaxies
• The XXL Survey: XXX. Characterisation of the XLSSsC N01 supercluster and analysis of the galaxy stellar populations
• Classification and Evolution of Galaxies According to the Dynamical State of Host Clusters and Galaxy Luminosities
• A morphological study of galaxies in ZwCl0024+1652, a galaxy cluster at redshift z $\sim$ 0.4
• Studying Large and Small Scale Environments of Ultraviolet Luminous Galaxies
• AGN and Star-Formation Properties of Inside-out Assembled Galaxy Candidates at z<0.1
• Galaxy and Mass Assembly (GAMA): Tracing galaxy environment using the marked correlation function
• More connected, more active: galaxy clusters and groups at z~1 and the connection between their quiescent galaxy fractions and large-scale environments
• Star Formation In The Cluster Merger DLSCL J0916.2+2953
• The bimodality of the 10k zCOSMOS-bright galaxies up to z ~ 1: a new statistical and portable classification based on the optical galaxy properties
• SEEDisCS I. Molecular gas in galaxy clusters and their large scale structure: the case of CL1411.1$-$1148 at $z\sim 0.5$
• The CluMPR Galaxy Cluster-Finding Algorithm and DESI Legacy Survey Galaxy Cluster Catalogue
• A Catalog of Emission-Line Galaxies from the Faint Infrared Grism Survey: Studying Environmental Influence on Star Formation
• Cosmic dance in the Shapley Concentration Core - I. A study of the radio emission of the BCGs and tailed radio galaxies
• The physical properties of massive green valley galaxies as a function of environments at $0.5<z<2.5$ in 3D-\textit{HST}/CANDELS fields
• Quenching in the Right Place at the Right Time: Tracing the Shared History of Starbursts, AGNs, and Post-starburst Galaxies Using Their Structures and Multiscale Environments
• Gravitational Potential Environment of Galaxies: I. Simulation
• The causal effect of environment on halo mass and concentration
• Revealing the Galaxy-Halo Connection Through Machine Learning
• The Munich Near-Infrared Cluster Survey (MUNICS) - IX. Galaxy Evolution to z ~ 2 From Optically Selected Catalogues
• The nature of H$\alpha$-selected galaxies along the large-scale structure at z=0.4 revealed by Subaru Hyper Suprime-Cam survey
• The effect of the morphological quenching mechanism on star formation activity at 0.5 < z < 1.5 in 3D-HST/CANDELS
• On the weak lensing masses of a new sample of galaxy groups
• Environments of red nuggets at z~0.7 from the VIPERS survey
• Revisiting the clustering of narrow-line AGN in the local Universe: Joint dependence on stellar mass and color
• The effects of environment on the intrinsic shape of galaxies
• Ram pressure profiles in galaxy groups and clusters
• Census of Gaseous Satellites around Local Spiral Galaxies
• Environment from cross-correlations: connecting hot gas and the quenching of galaxies
• The Atomic Hydrogen Content of Galaxies as a function of Group-Centric Radius
• A New Perspective on the Large-Scale Tidal Effect on the Galaxy Luminosity and Morphology
• The Environments of Local Luminous Infrared Galaxies: Star Formation Rates increase with Density
• Revealing ringed galaxies in group environments
• On the origin of red spirals: Does assembly bias play a role?
• Segregation effects in DEEP2 galaxy groups
• Can a conditioning on stellar mass explain the mutual information between morphology and environment?
• Investigating early-type galaxy evolution with a multi-wavelength approach. III. Insights from SPH simulations with chemo-photometric implementation
• BreakBRD Galaxies I: Global Properties of Spiral Galaxies with Central Star Formation in Red Disks
• Radial stellar populations of AGN-host dwarf galaxies in SDSS-IV MaNGA survey
• A Multi-wavelength Survey of AGN in Massive Clusters: AGN Distribution and Host Galaxy Properties
• Using large galaxy surveys to distinguish z~0.5 quiescent galaxy models
• Massive molecular gas reservoir around the central AGN in the CARLA J1103+3449 cluster at z=1.44
• NGC 474 as viewed with KCWI: diagnosing a shell galaxy
• On the influence of environment on star forming galaxies
• Autocorrelations of stellar light and mass in the low-redshift Universe
• HELP: star formation as function of galaxy environmentwith Herschel
• Pre-processing of Galaxies in the Early Stages of Cluster Formation in Abell 1882 at $z$=0.139
• Galaxy populations in the most distant SPT-SZ clusters -- II. Galaxy structural properties in massive clusters at 1.4<z<1.7
• Cosmic evolution of the incidence of Active Galactic Nuclei in massive clusters: Simulations versus observations
• Star formation history and transition epoch of cluster galaxies based on the Horizon-AGN simulation
• Overdensity of galaxies in the environment of quasar pairs
• Environmental cluster effects and galaxy evolution: The HI properties of the Abell clusters A85/A496/A2670
• The Differences of Star Formation History Between Merging Galaxies and Field Galaxies in the EDR of the SDSS
• PAC.V. The Roles of Mass and Environment in the Quenching of Galaxies
• XMM-Newton view of X-ray overdensities from nearby galaxy clusters: the environmental dependencies
• Probing the Mpc-scale environment of hyperluminous infrared galaxies at 2<z<4
• CALSAGOS: Clustering ALgorithmS Applied to Galaxies in Overdense Systems
• Environmental Effects on AGN activity via Extinction-free Mid-Infrared Census
• Linking the Supermassive Black Hole Growth with the Megamaser Emission
• Survival of Massive Star-forming Galaxies in Cluster Cores Drives Gas-Phase Metallicity Gradients : The Effects of Ram Pressure Stripping
• From haloes to galaxies. III. The gas cycle of local galaxy populations
• The Young, the Old, and the Dusty: Stellar Populations of AGN Hosts
• SEEDisCS II. Molecular gas in galaxy clusters and their large scale structure: low gas fraction galaxies, the case of CL1301.7$-$1139
• The LAMOST Complete Spectroscopic Survey of Pointing Area (LaCoSSPAr) in the Southern Galactic Cap I. The Spectroscopic Redshift Catalog
• On The Role of Supermassive Black Holes in Quenching Star Formation in Local Central Galaxies
• The survival of stellar discs in Fornax-like environments, from TNG50 to real galaxies
• Galaxy clusters and their outskirts: the "red sequence", star formation rate, stellar mass
• The variation of the gas content of galaxy groups and pairs compared to isolated galaxies
• Low Star Formation Rates for z=1 Early-Type Galaxies in the Very Deep GOODS-MIPS Imaging: Implications for their Optical/Near-Infrared Spectral Energy Distributions
• Forward modeling of galaxy kinematics in slitless spectroscopy
• The Ultraviolet Deep Imaging Survey of Galaxies in the Bootes Void I: catalog, color-magnitude relations and star formation
• A direct measurement of hierarchical growth in galaxy groups since z~1
• Cluster candidates with massive quiescent galaxies at $z\sim 2$
• The HI and stellar mass bivariate distribution of centrals and satellites for all, late- and early-type local galaxies
• Properties of Galaxies in the Disc Central Surface Brightness Gap
• Clustering, Cosmology and a New Era of Black Hole Demographics -- I. The Conditional Luminosity Function of Active Galactic Nuclei
• The correlations between galaxy properties in different environments of the cosmic web
• Small-Scale Conformity of the Virgo Cluster Galaxies
• Star Formation in CALIFA survey perturbed galaxies. I. Effects of Tidal Interactions
• A Multi-Wavelength Study of Low Redshift Cluster of Galaxies II. Environmental Impact on Galaxy Growth
• Galaxy interactions in filaments and sheets: insights from EAGLE simulations
• Star formation at different stages of ram-pressure stripping as observed through far-ultraviolet imaging of 13 GASP galaxies
• The XXL Survey XLV. Linking the ages of optically selected groups to their X-ray emission
• COSMOS2020: Disentangling the Role of Mass and Environment in Star Formation Activity of Galaxies at $0.4<z<4$
• On the Effects of Local Environment on Active Galactic Nucleus (AGN) in the Horizon Run 5 Simulation
• Herschel and ALMA Observations of Massive SZE-selected Clusters
• The quantity of dark matter in early-type galaxies and its relation to the environment
• On the Structure of the AGN Torus through the Fraction of Optically-Selected Type 1 AGNs
• Understanding Galaxy Formation and Evolution
• MaNGA AGN dwarf galaxies (MAD). III. The role of mergers and environment in active galactic nucleus activity in dwarf galaxies
• The abundance of massive compact galaxies at $1.0<z<3.0$ in 3D-HST/CANDELS
• The Spitzer-IRAC/MIPS Extragalactic Survey (SIMES): II enhanced nuclear accretion rate in galaxy groups at z$\sim$0.2
• The Impact of Disturbed Galaxy Clusters on the Kinematics of Active Galactic Nuclei
• The impact of environment on the lives of disk galaxies as revealed by SDSS-IV MaNGA
• Central star formation in an early-type galaxy I~Zw~81 in the Bootes void
• XXL-HSC: Host properties of X-ray detected AGNs in XXL clusters
• Structure and large scale environment of galaxy pairs in the S-PLUS DR4
• H$\alpha$-based Star Formation Rates in and around z $\sim$ 0.5 EDisCS clusters
• Quantifying galactic morphological transformations in the cluster environment
• Red riding on hood: Exploring how galaxy colour depends on environment
• The Co-Evolution of Galaxies and Black Holes: Current Status and Future Prospects
• Estimation of the Galaxy Quenching Rate in the Illustris Simulation
• The luminosity of cluster galaxies in the Cluster-EAGLE simulations
• Unravelling the orbits of cluster galaxy populations according to their dominant gas ionization source
• The galaxy environment in GAMA G3C groups using the Kilo Degree Survey Data Release 3
• LeMMINGs. VI. Connecting nuclear activity to bulge properties of active and inactive galaxies: radio scaling relations and galaxy environment
• The Compactness of Galaxy Groups in the Sloan Digital Sky Survey
• Jellyfish galaxies with the IllustrisTNG simulations -- Supermassive black hole activity in dense environments with ram-pressure stripped satellites
• Clustering properties and halo masses for central galaxies in the local Universe
• Environmental effects on associations of dwarf galaxies
• Interactions of galaxies outside clusters and massive groups
• The Environment of Lyman Break Analogues (ELBA) survey: Star-forming galaxies in small groups
• ZFIRE: The Beginning of the End for Massive Galaxies at z ~ 2 and Why Environment Matters
• Differences in the Physical Properties of Satellite Galaxies within Relaxed and Disturbed Galaxy Groups and Clusters
• Comparing IMF-sensitive indices of intermediate-mass quiescent galaxies in various environments
• Self-Similar Buildup and Inside-Out Growth: Tracing the Evolution of Intermediate to High-Mass Star-Forming Galaxies Since $z=2$
• Quantifying the Impact of Incompleteness on Identifying and Interpreting Galaxy Protocluster Populations with the TNG-Cluster Simulation
• Spectroscopic characterization of the protocluster of galaxies around 7C 1756+6520 at z ~ 1.4
• Ram pressure stripping in the z~0.5 galaxy cluster MS 0451.6-0305
• What size halos do local LIRGs live in?
• Impact of cosmic web on the properties of galaxies in IllustrisTNG simulations
• A Morphological Study on AGN-host Dwarf Galaxies
• On the Clustering of Compact Galaxy Pairs in Dark Matter Haloes
• The SAMI Galaxy Survey: The relationship between galaxy rotation and the motion of neighbours
• Brighter and More Massive Galaxies in the Vicinity of Lyman-alpha Nebulae
• The distribution of local star formation activity as a function of galaxy stellar mass, environment and morphology
• Deep Extragalactic VIsible Legacy Survey (DEVILS): First Data Release Covering The D10 (COSMOS) Region
• Environmental Effects on the Star Formation Activity at z~0.9 in the COSMOS Field
• Measurable Relationship Between Bright Galaxies and Their Faint Companions in WHL J085910.0+294957, a Galaxy Cluster at z = 0.30: Vestiges of Infallen Groups?
• More than just halo mass: Modelling how the red galaxy fraction depends on multiscale density in a HOD framework
• The effect of environment on the properties of the most massive galaxies at $0.5<z<2.5$ in the cosmos-dash field
• Environmental Effects in the Evolution of Galactic Bulges
• What is the right way to quench star formation in semi-analytic model of galaxy formation?
• A far-infrared survey at the North Galactic Pole I: Nearby star-forming galaxies and the effect of confused sources on source counts
• Late growth of early-type galaxies in low-z massive clusters
• Galaxy Optical Variability of Virgo Cluster: New Tracer for Environmental Influences on Galaxies
• From Halos to Galaxies. X: Decoding Galaxy SEDs with Physical Priors and Accurate Star Formation History Reconstruction
• Impact of cosmic web on galaxy properties and their correlations: Insights from Principal Component Analysis
• Star formation activity in a young galaxy cluster at z=0.866
• The link between galaxy structure properties and star formation in local galaxies
• Enhanced AGN Activity in Overdense Galactic Environments at $2<z<4$
• Automatic morphological classification of galaxies: convolutional autoencoder and bagging-based multiclustering model
• Pre-heating of the intergalactic medium by gravitational collapse and ultraviolet background
• Evolution of star-forming dwarf galaxies in different environments
• The HST-Hyperion Survey: Companion Fraction and Overdensity in a z ~ 2.5 Proto-supercluster
• Euclid preparation: TBD. Cosmic Dawn Survey: evolution of the galaxy stellar mass function across 0.2<z<6.5 measured over 10 square degrees
• Estimating infall times of galaxies around clusters: how accurately can it be done with observational data?
• Star formation properties of galaxy cluster A1767
• The Way to Quench: Galaxy evolution in Abell 2142
• Constraints on the Minor Merging and Star Formation History of the Wolf-Rayet Galaxy NGC 5430 Through Observations
• Study of central intensity ratio of early-type galaxies from low density environment
• The Two-Point Correlation of 2QZ Quasars and 2SLAQ LRGs: From a Quasar Fueling Perspective
• ZTF SN Ia DR2: Exploring SN Ia properties in the vicinity of under-dense environments
• SOMBI: Bayesian identification of parameter relations in unstructured cosmological data
• Alignment of spiral and elliptical galaxies from Siena Galaxy Atlas with filaments
• Cluster environment quenches the star formation of low-mass satellite galaxies from the inside-out
• Can luminous Lyman alpha emitters at $z$ $\simeq$ 5.7 and $z$ $\simeq$ 6.6 suppress star formation?
• Galaxy And Mass Assembly (GAMA): From filaments to voids, how extreme environment affects gas metallicity and SFR in galaxies
• Environmental Invariance of the Galaxy Size-Mass Relation
• Photometric and Spectroscopic Study of Abell 0671
• Blueberry and Green Pea galaxies live in low density environments
• The VIMOS VLT Deep Survey. The different assembly history of passive and star-forming L_B >= L*_B galaxies in the group environment at z < 1
• Star formation quenching precedes morphological transformation in COSMOS-WEB's richest galaxy groups
• ODIN: Using multiplicity of Lyman-Alpha Emitters to assess star formation activity in dark matter halos
• GLACE survey: galaxy activity in ZwCl0024+1652 cluster from strong optical emission lines
• The Next Generation Virgo Cluster Survey (NGVS). XL. The Morphological Classification of Virgo Cluster Galaxies
• The impact of cosmic filaments on the abundance of satellite galaxies
• Dark matter halos of luminous AGNs from galaxy-galaxy lensing with the HSC Subaru Strategic Program
• Fraction of the X-ray selected AGNs with optical emission lines in galaxy groups
• Wide Field Multiband Imaging of Low Redshift Quasar Environments
• 3D intrinsic shapes of quiescent galaxies in observations and simulations
• Large Scale Distribution of Galaxies in The Field HS 47.5-22. I. Data Analysis Technique
• Main sequence of star formation and colour bimodality considering galaxy environment
• Isolated and group environment dependence of stellar mass and different star formation rates
• Emission line galaxies in clusters
• Free-floating molecular clumps and gas mixing: hydrodynamic aftermaths of the intracluster$-$interstellar medium interaction
• Star-formation Properties of z ~ 1 Galaxy Clusters and Groups from Horizon Run 5
• Spectral Energy Distribution Modeling of Broad Emission Line Quasars: From X-ray to Radio Wavelengths
• Ageing and Quenching: Influence of Galaxy Environment and Nuclear Activity in Transition Stage
• The origin of ionized gas in retired galaxies: dynamical clues
• Environmental Sculpting of Galaxy Structure at Fixed Stellar Mass: A Multi-Scale Analysis Across Cosmic Time using 3 Million HSC Galaxies
• Comparison of some properties of star forming galaxies and active galactic nuclei (AGNs) between two BOSS galaxy samples of SDSS DR9
• Galaxy And Mass Assembly (GAMA): Deconstructing the galaxy stellar mass function by star formation and environment
• The Kormendy relation of cluster galaxies in PPS regions
• Investigating the Impacts of AGN Activities on Dwarf Galaxies with FAST HI Observations
• Large Scale Distribution of Galaxies in The Field HS 47.5-22. II. Observational Data Analysis
• Multi-Object Spectroscopy of Galaxy Clusters at $z\sim 0.95$ in Ultra Deep Survey Field with Different Star-formation Properties and Large-scale Environments
• The miniJPAS survey: Dissecting galaxy properties across environments with spatially resolved photometry
• Clustering and physical properties of AGN and Star-Forming Galaxies at fixed stellar mass: does assembly bias have a role in AGN activity?
• The Evolution of the SFR-M_* relation at 0.1<z<4: Environmental and Morphological Dependencies
• SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass
• Morphological Transformation and Star Formation Quenching of Massive Galaxies at 0.5 < z < 2.5 in 3D-HST/CANDELS
• The cosmic environment overtakes the local density in shaping galaxy star formation
• Galaxy Evolution in the Local Universe: Group Richness Effects on Mergers and Non-Mergers
• From the Densest Clusters to the Emptiest Voids: No Evidence For Environmental Effects on the Galaxy Size-Mass Relation at Low Redshift
• Using the EAGLE simulations to elucidate the origin of disc surface brightness profile breaks as a function of mass and environment
• Analysis of spatially resolved stellar populations and emission line properties in nearby galaxies with J-PLUS data. II-Results for the M51 group and first comparison with the M101 group
• Tracing correlations between galaxy properties across the Cosmic Web: An IllustrisTNG-based study
• Variability Selected Active Galactic Nuclei from ASAS-SN Survey: Constraining the Low Luminosity AGN Population
• OMEGA: OSIRIS Mapping of Emission-Line Galaxies in A901/2