Properties of Galaxy Groups in the SDSS: I.-- The Dependence of Colour, Star Formation, and Morphology on Halo Mass

Abstract

Using a large galaxy group catalogue constructed from the SDSS, we investigate the correlation between various galaxy properties and halo mass. We split the population of galaxies in early types, late types, and intermediate types, based on their colour and specific star formation rate. At fixed luminosity, the early type fraction increases with increasing halo mass. Most importantly, this mass dependence is smooth and persists over the entire mass range probed, without any break or feature at any mass scale. We argue that the previous claim of a characteristic feature on galaxy group scales is an artefact of the environment estimators used. At fixed halo mass, the luminosity dependence of the type fractions is surprisingly weak: galaxy type depends more strongly on halo mass than on luminosity. We also find that the early type fraction decreases with increasing halo-centric radius. Contrary to previous studies, we find that this radial dependence is also present in low mass haloes. The properties of satellite galaxies are strongly correlated with those of their central galaxy. In particular, the early type fraction of satellites is significantly higher in a halo with an early type central galaxy than in a halo of the same mass but with a late type central galaxy. This phenomenon, which we call `galactic conformity', is present in haloes of all masses and for satellites of all luminosities. Finally, the fraction of intermediate type galaxies is always ~20 percent, independent of luminosity, independent of halo mass, independent of halo-centric radius, and independent of whether the galaxy is a central galaxy or a satellite galaxy. We discuss the implications of all these findings for galaxy formation and evolution.

arXiv comment28 pages, 15 figures. Submitted for publication in MNRAS

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• Major Cluster Mergers and the Location of the Brightest Cluster Galaxy
• 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
• Multiple Mechanisms Quench Passive Spiral Galaxies
• Red star-forming and blue passive galaxies in clusters
• Nature versus nurture: what regulates star formation in satellite galaxies?
• The quiescent fraction of isolated low surface brightness galaxies: Observational constraints
• The galaxy-halo connection in the VIDEO Survey at 0.5<z<1.7
• PRIMUS: One- and Two-Halo Galactic Conformity at $0.2<z<1$
• The Dearth of Difference between Central and Satellite Galaxies I. Perspectives on star formation quenching and AGN activities
• A MeerKAT view of pre-processing in the Fornax A group
• Effects on Galaxy Evolution: Pair Interactions versus Environment
• Updated Results on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• The VIMOS VLT Deep Survey: the group catalogue
• The Color Bimodality in Galaxy Clusters since z = 0.9
• The impact of feedback and the hot halo on the rates of gas accretion onto galaxies
• Mass and Redshift Dependence of Star Formation in Relaxed Galaxy Clusters
• A journey from the outskirts to the cores of groups I: Color- and mass-segregation in 20K-zCOSMOS groups
• Offset between X-ray and optical centers in clusters of galaxies: connecting eROSITA data and simulations
• Isolated elliptical galaxies in the local Universe
• Central galaxies in different environments: Do they have similar properties?
• RASS-SDSS Galaxy Cluster Survey. VI. The dependence of the cluster SFR on the cluster global properties
• Semi-Analytic Model Predictions of the Galaxy Population in Proto-clusters
• The spatial distribution of cold gas in hierarchical galaxy formation models
• CFHT Legacy Ultraviolet Extension (CLUE): Witnessing Galaxy Transformations up to 7 Mpc from Rich Cluster Cores
• Groups of galaxies: relationship between environment and galaxy properties
• Comparing galaxy populations in compact and loose groups of galaxies
• The Zurich Environmental Study (ZENS) of Galaxies in Groups along the Cosmic Web. II. Galaxy Structural Measurements and the Concentration of Morphologically Classified Satellites in Diverse Environments
• Distribution of satellite galaxies in high redshift groups
• A comparative study of satellite galaxies in Milky Way-like galaxies from HSC, DECaLS and SDSS
• High-order 3D Voronoi tessellation for identifying Isolated galaxies, Pairs and Triplets
• The MillenniumTNG Project: Refining the one-halo model of red and blue galaxies at different redshifts
• A Huge Filamentary Structure at z=0.55 and Star Formation Histories of Galaxies at z<1
• The bright end of the colour-magnitude relation of cluster galaxies
• Discovery and analysis of low-surface-brightness galaxies in the environment of NGC 1052
• Connecting Compact Star-forming and Extended Star-forming Galaxies at Low-redshift: Implications for Galaxy Compaction and Quenching
• The Effect of Environment on Discs and Bulges
• The Centaurus Group and the Outer Halo of NGC 5128: Are they Dynamically Connected?
• A catalogue of structural and morphological measurements for DES Y1
• Group quenching and galactic conformity at low redshift
• Connections between galaxy mergers and Starburst: evidence from local Universe
• Evidence for Morphology and Luminosity Transformation of Galaxies at High Redshifts
• Extensions to the halo occupation distribution model for more accurate clustering predictions
• Probing the existence of a rich galaxy overdensity at z=5.2
• The morphological transformation and the quenching of galaxies
• Massive central galaxies of galaxy groups in the Romulus simulations: an overview of galaxy properties at z=0
• Small- and Large-Scale Galactic Conformity in SDSS DR7
• How to Optimally Constrain Galaxy Assembly Bias: Supplement Projected Correlation Functions with Count-in-cells Statistics
• The nature of the Sloan Digital Sky Survey galaxies in various classes based on morphology, colour and spectral features - III. Environments
• On the relationship between environment and galaxy properties in clusters of galaxies
• Brightest galaxies as halo centre tracers in SDSS DR7
• The Three Hundred Project: the stellar and gas profiles
• Simulating the evolution of disc galaxies in a group environment. II. The influence of close-encounters between galaxies
• The Mass Dependance of Satellite Quenching in Milky Way-like Halos
• The dependence of AGN activity on stellar and halo mass in Semi-Analytic Models
• A Parametrized Galaxy Catalog Simulator For Testing Cluster Finding, Mass Estimation and Photometric Redshift Estimation in Optical and Near Infrared Surveys
• The dependence of galaxy clustering on tidal environment in the Sloan Digital Sky Survey
• Gas depletion in cluster galaxies depends strongly on their internal structure
• Using Galaxy Pairs to Probe Star Formation During Major Halo Mergers
• Groups in the Millennium Simulation and in SDSS DR7
• The Physical Origin of Galactic Conformity: From Theory to Observation
• The SAGA Survey. IV. The Star Formation Properties of 101 Satellite Systems around Milky Way-mass Galaxies
• The Dwarf Galaxy Population in Nearby Groups. The data
• Environmental Quenching and Galactic Conformity in the Galaxy Cross-Correlation Signal
• The environmental dependence of the structure of galactic discs in STAGES S0 galaxies: implications for S0 formation
• Prevalence of neutral gas in centres of merging galaxies
• Local and global environmental effects on galaxies and active galactic nuclei
• Galaxy groups in the 2MASS Redshift Survey
• The evolution of galaxy groups and of galaxies therein
• The Role of Environment on the Formation of Early-Type Galaxies
• ELVES III: Environmental Quenching by Milky Way-Mass Hosts
• The GOGREEN survey: Dependence of galaxy properties on halo mass at z > 1 and implications for environmental quenching
• Probing the galaxy-halo connection with total satellite luminosity
• Galactic conformity measured in semi-analytic models
• ZOMG II: Does the halo assembly history influence central galaxies and gas accretion?
• Implications of the remarkable homogeneity of galaxy groups and clusters
• On the environmental influence of groups and clusters of galaxies beyond the virial radius: Galactic conformity at few Mpc scales
• What do simulations predict for the galaxy stellar mass function and its evolution in different environments?
• Do the stellar populations of the brightest two group galaxies depend on the magnitude gap?
• Measures of galaxy environment -- II. Rank-ordered mark correlations
• The definition of environment and its relation to the quenching of galaxies at z=1-2 in a hierarchical Universe
• Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
• Quantifying the role of ram pressure stripping of galaxies within galaxy groups
• GOGREEN: a critical assessment of environmental trends in cosmological hydrodynamical simulations at z ~ 1
• A revisit to agglomerates of early-type Hipparcos stars
• DustPedia - the relationships between stars, gas and dust for galaxies residing in different environments
• The dark side of galaxy stellar populations I: The stellar-to-halo mass relation and the velocity dispersion - halo mass relation
• The miniJPAS survey: The role of group environment in quenching the star formation
• Evolution in the Disks and Bulges of Group Galaxies since z=0.4
• The First Mid-IR View of the Star-forming Properties of Nearby Galaxy Groups
• On the Origin of the Dichotomy of Early-Type Galaxies: The Role of Dry Mergers and AGN Feedback
• Color Magnitude Relation and Morphology of Low-Redshift ULIRGs in SDSS
• Identifying galaxy groups at high redshift from incomplete spectroscopic data: I. The group finder and application to zCOSMOS
• Prevalence of neutral gas in centres of merging galaxies-II: nuclear HI and multi-wavelength properties
• Inclination-Independent Galaxy Classification
• Evolution of Group Galaxies from the First Red-Sequence Cluster Survey
• Determining the Halo Mass Scale where Galaxies Lose Their Gas
• Hosts and triggers of AGNs in the Local Universe
• The XXL Survey VIII: MUSE characterisation of intracluster light in a z$\sim$0.53 cluster of galaxies
• The Influence of Galaxy Environment on the Stellar Initial Mass Function of Early-Type Galaxies
• Alignment between satellite and central galaxies in the SDSS DR7: dependence on large-scale environment
• Properties of brightest group galaxies in cosmic web filaments
• Testing Galaxy Quenching Theories with Scatter in the Stellar to Halo Mass Relation
• A study on the statistical significance of mutual information between morphology of a galaxy and its large-scale environment
• Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model - I. Magnitude counts, redshift distribution, colour bimodality, and galaxy clustering
• Galaxy and Mass Assembly: luminosity and stellar mass functions in GAMA groups
• The Isophotal Structure of Early-Type Galaxies in the SDSS: Dependence on AGN Activity and Environment
• The dynamical state of galaxy groups and their luminosity content
• An HI View of Galaxy Conformity: HI-rich Environment around HI-excess Galaxies
• The evolution of the bi-modal colour distribution of galaxies in SDSS groups
• Testing redMaPPer centring probabilities using galaxy clustering and galaxy-galaxy lensing
• HOD-Dependent Systematics in Emission Line Galaxies for the DESI 2024 BAO analysis
• MUSE sneaks a peek at extreme ram-pressure stripping events -- V. Towards a complete view of the galaxy cluster A1367
• Multi-wavelength mock galaxy catalogs of the low-redshift Universe
• Subhaloes gone Notts: Subhaloes as tracers of the dark matter halo shape
• Red Misfits in the Sloan Digital Sky Survey: Properties of Star-forming Red Galaxies
• AGN-driven quenching of satellite galaxies
• On the mass assembly of low-mass galaxies in hydrodynamical simulations of structure formation
• Clustercentric distance or local density? It depends on galaxy morphology
• The Three Hundred project: connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
• Galaxy Formation with Local Photoionization Feedback -II. Effect of X-Ray Emission from Binaries and Hot Gas
• HI scaling relations of galaxies in the environment of HI-rich and control galaxies observed by the Bluedisk project
• Does jackknife scale really matter for accurate large-scale structure covariances?
• Ram pressure stripping of HI-rich galaxies infalling into massive clusters
• Halo models of HI selected galaxies
• PRIMUS: Obscured Star Formation on the Red Sequence
• Compact Groups of Galaxies in Sloan Digital Sky Survey and LAMOST Spectral Survey. II. Dynamical Properties of Isolated and Embedded Groups
• Star-formation quenching of cluster galaxies as traced by metallicity, presence of active galactic nuclei, and galactic conformity
• Galaxies in X-ray Groups. III. Satellite Color and Morphology Transformations
• Analysis of Sunyaev-Zel'dovich Effect Mass-Observable Relations using South Pole Telescope Observations of an X-ray Selected Sample of Low Mass Galaxy Clusters and Groups
• The anatomy of the NGC 5044 group - I. Group membership and dynamics
• Maturing Satellite Kinematics into a Competitive Probe of the Galaxy-Halo Connection
• The dearth of difference between central and satellite galaxies II. Comparison of observations with L-GALAXIES and EAGLE in star formation quenching
• Counts-in-Cylinders in the Sloan Digital Sky Survey with Comparisons to N-body Simulations
• The diversity of assembly histories leading to disc galaxy formation in a LambdaCDM model
• AKARI Observation of the North Ecliptic Pole (NEP) Supercluster at z = 0.087: mid-infrared view of transition galaxies
• The Zurich Environmental Study (ZENS) of Galaxies in Groups along the Cosmic Web. V. Properties and Frequency of Merging Satellites and Centrals in Different Environments
• The evolution of star formation activity in galaxy groups
• Groups and protocluster candidates in the CLAUDS and HSC-SSP joint deep surveys
• Interacting galaxies in the IllustrisTNG simulations -- V: Comparing the influence of star-forming vs. passive companions
• Star Formation and Supercluster Environment of 107 Nearby Galaxy Clusters
• Using member galaxy luminosities as halo mass proxies of galaxy groups
• Analytical halo model of galactic conformity
• Halo-model analysis of the clustering of photometric luminous red galaxies at $0.10\le z\le 1.05$ from the Subaru Hyper Suprime-Cam Survey
• The frequency of very young galaxies in the local Universe: I. A test for galaxy formation and cosmological models
• Mufasa:The strength and evolution of galaxy conformity in various tracers
• NUV signatures of environment driven galaxy quenching in SDSS groups
• Galactic Conformity in both Star-formation and Morphological Properties
• Dissect two-halo galactic conformity effect for central galaxies: The dependence of star formation activities on the large-scale environment
• Analysis of the Properties of Clusters of Galaxies in the Region of the Ursa Major Supercluster
• Modeling Redshift-Space Clustering with Abundance Matching
• The Clustering and Halo Masses of Star Forming Galaxies at z<1
• The active and passive populations of Extremely Red Objects
• The Dearth of Difference between Central and Satellite Galaxies III. Environmental Dependence of Mass-Size and Mass-Structure Relations
• The Baryonic Collapse Efficiency of Galaxy Groups in the RESOLVE and ECO Surveys
• Revisiting the low-luminosity galaxy population of the NGC 5846 group with SDSS
• Ram pressure stripping: An analytical approach
• The SAMI Galaxy Survey: galaxy spin is more strongly correlated with stellar population age than mass or environment
• Evolution of galaxies in groups in the Coma Supercluster
• The strong environmental dependence of black hole scaling relations
• Integrated specific star formation rates of galaxies, groups, and clusters: A continuous upper limit with stellar mass?
• Early-Type Galaxy Star Formation Histories in Different Environments
• What Regulates Galaxy Evolution? Open Questions in Our Understanding of Galaxy Formation and Evolution
• Characteristic mass in galaxy quenching: environmental versus internal effects
• AXES-SDSS: comparison of SDSS galaxy groups with all-sky X-ray extended sources
• Galaxy and Mass Assembly (GAMA): Probing the merger histories of massive galaxies via stellar populations
• Dust accretion and destruction in galaxy groups and clusters
• The Stellar Mass Assembly of Low Redshift, Massive, Central Galaxies in SDSS and the TNG300 simulation
• Morphological Parameters and Associated Uncertainties for 8 Million Galaxies in the Hyper Suprime-Cam Wide Survey
• Host galaxies of long gamma-ray bursts in the Millennium Simulation
• The transformation and quenching of simulated gas-rich dwarf satellites within a group environment
• Timescales for Hi consumption and SFR depletion of satellite galaxies in groups
• How the Galaxy-Halo Connection Depends on Large-Scale Environment
• Satellite Alignment: III. Satellite Galaxies Spatial Distribution and their Dependence on Redshift with A Novel Galaxy Finder
• Observing Correlations Between Dark Matter Accretion and Galaxy Growth: I. Recent Star Formation Activity in Isolated Milky Way-Mass Galaxies
• YZiCS: On the Mass Segregation of Galaxies in Clusters
• Gas Accretion and Angular Momentum
• MAGIC: Muse gAlaxy Groups In Cosmos -- A survey to probe the impact of environment on galaxy evolution over the last 8 Gyr
• The Roles of Mass and Environment in the Quenching of Galaxies
• Clustering of MgII absorption line systems around massive galaxies: an important constraint on feedback processes in galaxy formation
• Evidence for anisotropic quenching in massive galaxy clusters at $z\approx 0.5$
• A systematic search for galaxy protocluster cores at the transition epoch of their star formation activity
• Semi-Analytic Model Predictions of Mass Segregation from Groups to Clusters
• Galaxy populations in groups and clusters: evidence for a characteristic stellar mass scale at $M_{\ast }\sim 10^{9.5}{M}_{\odot }$
• Do cluster properties affect the quenching rate?
• Discovery of a Bimodal Environmental Distribution of Compact Ellipticals in the Local Universe
• The Large-scale Effect of Environment on Galactic Conformity
• Groups of two galaxies in SDSS: implications of colours on star formation quenching time-scales
• Ram pressure stripping in clusters: Gravity can bind the ISM but not the CGM
• The Fundamental Plane Relation of Early-Type Galaxies: Environmental Dependence
• The Munich Near-Infrared Cluster Survey (MUNICS) - IX. Galaxy Evolution to z ~ 2 From Optically Selected Catalogues
• Investigating the galaxy-halo connection of DESI Emission-Line Galaxies with SHAMe-SF
• BASILISK: Bayesian Hierarchical Inference of the Galaxy-Halo Connection using Satellite Kinematics--I. Method and Validation
• Clustering of the AKARI NEP Deep Field 24 $\mu$m selected galaxies
• Quantifying the effect of black hole feedback from the central galaxy on the satellite populations of groups and clusters
• The Evaporation and Survival of Cluster Galaxies' Coronae Part I: The Effectiveness of Isotropic Thermal Conduction Including Saturation
• The Color and Stellar Mass Dependence of Small-scale Galaxy Clustering in SDSS-III BOSS
• Dark against luminous matter around isolated central galaxies: a comparative study between modern surveys and Illustris-TNG
• Beyond Ultra-diffuse Galaxies. II. Environmental Quenching of Mass-Size Outliers among the Satellites of Milky Way Analogs
• Autocorrelations of stellar light and mass in the low-redshift Universe
• Using large galaxy surveys to distinguish z~0.5 quiescent galaxy models
• Backsplash galaxies and their impact on galaxy evolution: a three-stage, four-type perspective
• The Properties of Type Ia Supernova Host Galaxies from the Sloan Digital Sky Survey
• Galaxy assembly bias in the stellar-to-halo mass relation for red central galaxies from SDSS
• PRIMUS: Clustering of Star-forming and Quiescent Central Galaxies at $0.2<z<0.9$
• Herschel-ATLAS/GAMA:How does the far-IR luminosity function depend on galaxy group properties?
• Measuring the X-ray luminosities of DESI groups from eROSITA Final Equatorial-Depth Survey: I. X-ray luminosity -- halo mass scaling relation
• The PAU Survey: galaxy stellar population properties estimates with narrowband data
• Reconstructing Orbits of Galaxies in Extreme Regions (ROGER) III: galaxy evolution patterns in projected phase space around massive X-ray clusters
• The dependence of low redshift galaxy properties on environment
• Hyenas: X-ray Bubbles and Cavities in the Intra-Group Medium
• Small-Scale Conformity of the Virgo Cluster Galaxies
• Identification of 4876 Bent-Tail Radio Galaxies in the FIRST Survey Using Deep Learning Combined with Visual Inspection
• PRIMUS: The Effect of Physical Scale on the Luminosity-Dependence of Galaxy Clustering via Cross-Correlations
• Assembly bias evidence in close galaxy pairs
• A general approach to quenching and galactic conformity
• Understanding Galaxy Formation and Evolution
• Finding proto-clusters to trace galaxy evolution: I. The finder and its performance
• Are early-type galaxies quenched by present-day environment? A study of dwarfs in the Fornax Cluster
• Star-forming and Quiescent Central Galaxies Cluster Similarly: Implications for the Galaxy-Halo Connection
• The XXL Survey XLV. Linking the ages of optically selected groups to their X-ray emission
• The EDGE-CALIFA survey: Star formation relationships for galaxies at different stages of their evolution
• The Halo Masses of Galaxies to $z\sim 3$: A Hybrid Observational and Theoretical Approach
• The properties and environment of very young galaxies in the local Universe
• Quantifying galactic morphological transformations in the cluster environment
• The Environments of Low and High Luminosity Radio Galaxies at Moderate Redshifts
• Structure and large scale environment of galaxy pairs in the S-PLUS DR4
• The fragility of thin discs in galaxies -- I. Building tailored N-body galaxy models
• The Circular Velocity Function of Group Galaxies
• Clusters and Groups of Galaxies in the Simulated Local Universe
• The WiggleZ Dark Energy Survey: Galaxy Evolution at 0.25 < z < 0.75 Using The Second Red-Sequence Cluster Survey (RCS-2)
• The Spatial Range of Conformity
• Unravelling the orbits of cluster galaxy populations according to their dominant gas ionization source
• Unraveling emission line galaxy conformity at z~1 with DESI early data
• Modeling Star Formation Histories of Changing-Look AGN Host Galaxies with Prospector
• How do uncertainties in galaxy formation physics impact field-level galaxy bias?
• Satellites and central galaxies in SDSS: the influence of interactions on their properties
• Small-Scale Dynamical Coherence Accompanied with Galaxy Conformity
• The Compactness of Galaxy Groups in the Sloan Digital Sky Survey
• Interactions of galaxies outside clusters and massive groups
• Compact groups of galaxies in GAMA -- Probing the densest minor systems at intermediate redshifts
• Insights into environmental quenching at $z\sim 1$: an enhancement of faint, low-mass passive galaxies in clusters
• FASHI: An untargeted survey of the 21 cm HI absorption galaxies with FAST
• Mock Observations: Three Different Types of Galaxy Alignment in TNG100 Simulations
• The VANDELS Survey: Star formation and quenching in two over-densities at 3 < z < 4
• Searching for Conformity Across Cosmic Time with Local Group and Local Volume Star Formation Histories
• Observing Correlations Between Dark Matter Accretion and Galaxy Growth: II. Testing the Impact of Galaxy Mass, Star Formation Indicator, and Neighbour Colours
• The conformity of HI galaxies in ALFALFA-SDSS sample
• More than just halo mass: Modelling how the red galaxy fraction depends on multiscale density in a HOD framework
• Exploring the stellar populations of backsplash galaxies
• 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?
• Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
• Mock Observations: Morphological Analysis of Galaxies in TNG100 Simulations
• Mergers and Disk Survival in LCDM
• Spatial clustering in the ESO-Sculptor Survey: two-point correlation functions by galaxy type at redshifts 0.1 - 0.5
• DESI Emission-line Galaxies: Clustering Dependence on Stellar Mass and [OII] Luminosity
• Environmental Quenching of Low Surface Brightness Galaxies near Milky Way mass Hosts
• The environmental dependence of the stellar mass fundamental plane of early-type galaxies
• Strong Conformity and Assembly Bias: Towards a Physical Understanding of the Galaxy-Halo Connection in SDSS Clusters
• Mechanisms Affecting Galaxies Nearby and Environmental Trends (MAGNET)
• CosmoGLINT: Cosmological Generative Model for Line Intensity Mapping with Transformer
• The Swift AGN and Cluster Survey. II. Cluster Confirmation with SDSS Data
• Insights into the dependence of galaxy properties on the environment with explainable machine learning models
• GLACE survey: galaxy activity in ZwCl0024+1652 cluster from strong optical emission lines
• Winds versus jets: a comparison between black hole feedback modes in simulations of idealized galaxy groups and clusters
• Clustering Property of Wolf-Rayet Galaxies in the SDSS
• Emergence of red, star-forming galaxies (red misfits) in a ΛCDM universe
• Environmental Invariance of the Galaxy Size-Mass Relation
• Morphological Transformation and Star Formation Quenching of Massive Galaxies at 0.5 < z < 2.5 in 3D-HST/CANDELS
• A semi-analytical perspective on massive red galaxies: I. Assembly history, environment & redshift evolution
• Forged by Feedback: Stellar Properties of Brightest Group Galaxies in Cosmological Simulations
• The origin of ionized gas in retired galaxies: dynamical clues
• SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass
• The interplay between AGN feedback and precipitation of the intracluster medium in simulations of galaxy groups and clusters
• Quantifying the Poor Purity and Completeness of Morphological Samples Selected by Galaxy Colour
• Mapping Nearby Galaxies with Apache Point Observatory: Group and field galaxies' morphologies in the colour-magnitude plane
• Alignment of the central galaxies with the environment
• Breaking down the link between luminous and dark matter in massive galaxies