Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function

Abstract

We explore the inter-relationships between mass, star-formation rate and environment in the SDSS, zCOSMOS and other surveys. The differential effects of mass and environment are completely separable to z ~ 1, indicating that two distinct processes are operating, "mass-quenching" and "environment-quenching". Environment-quenching, at fixed over-density, evidently does not change with epoch to z ~ 1, suggesting that it occurs as large-scale structure develops in the Universe. The observed constancy of the mass-function shape for star-forming galaxies, demands that the mass-quenching of galaxies around and above M*, must be proportional to their star-formation rates at all z < 2. We postulate that this simple mass-quenching law also holds over a much broader range of stellar mass and epoch. These two simple quenching processes, plus some additional quenching due to merging, then naturally produce (a) a quasi-static Schechter mass function for star-forming galaxies with a value of M* that is set by the proportionality between the star-formation and mass-quenching rates, (b) a double Schechter function for passive galaxies with two components: the dominant one is produced by mass-quenching and has exactly the same M* as the star-forming galaxies but an alpha shallower by +1, while the other is produced by environment effects and has the same M* and alpha as the star-forming galaxies, and is larger in high density environments. Subsequent merging of quenched galaxies modifies these predictions somewhat in the denser environments, slightly increasing M* and making alpha more negative. All of these detailed quantitative relationships between the Schechter parameters are indeed seen in the SDSS, lending strong support to our simple empirically-based model. The model naturally produces for passive galaxies the "anti-hierarchical" run of mean ages and alpha-element abundances with mass.

66 pages, 19 figures, 1 movie, accepted for publication in ApJ. The movie is also available at http://www.exp-astro.phys.ethz.ch/zCOSMOS/MF_simulation_d1_d4.mov

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• The morphological transformation and the quenching of galaxies
• Satellite quenching was not important for z$\sim$1 clusters: most quenching occurred during infall
• On the evolution of the central density of quiescent galaxies
• The Close AGN Reference Survey (CARS): No obvious signature of AGN feedback on star formation, but subtle trends
• The stellar mass - halo mass relation from galaxy clustering in VUDS: a high star formation efficiency at z~3
• Massive central galaxies of galaxy groups in the Romulus simulations: an overview of galaxy properties at z=0
• UV to submillimetre luminosity functions of TNG50 galaxies
• Star Formation Quenching in Green Valley Galaxies at $0.5\lesssim z\lesssim 1.0$ and Constraints with Galaxy Morphologies
• Too dense to go through: The importance of low-mass clusters for satellite quenching
• On the relative effect of nodes and filaments of the cosmic web on the quenching of galaxies and the orientation of their spin
• A Catalog of Host Galaxies for WISE-Selected AGN: Connecting Host Properties with Nuclear Activity and Identifying Contaminants
• The environment of radio sources in the VLA-COSMOS Survey field
• Galaxy evolution in the mid-infrared green valley: a case of the A2199 supercluster
• On the formation of massive quiescent galaxies with diverse morphologies in the TNG50 simulation
• The JCMT Nearby Galaxies Legacy Survey -- XI. -- Environmental Variations in the Atomic and Molecular Gas Radial Profiles of Nearby Spiral Galaxies
• SDSS-IV MaNGA: The Roles of AGNs and Dynamical Processes in Star Formation Quenching in Nearby Disk Galaxies
• What drives galaxy quenching? A deep connection between galaxy kinematics and quenching in the local Universe
• Flows around galaxies. I. The dependency of galaxy connectivity on cosmic environments and effects on the star-formation rate
• The cosmic web of X-ray active galactic nuclei seen through the eROSITA Final Equatorial Depth Survey (eFEDS)
• In and out star formation in z~1.5 quiescent galaxies from rest-frame UV spectroscopy and the far-infrared
• Revealing impacts of stellar mass and environment on galaxy quenching
• Galaxy evolution in merging clusters: The passive core of the "Train Wreck" cluster of galaxies, A520
• The Properties of Radio Galaxies and the Effect of Environment in Large Scale Structures at $z\sim 1$
• Compact, bulge dominated structures of spectroscopically confirmed quiescent galaxies at z~3
• ODIN: Where Do Lyman-alpha Blobs Live? Contextualizing Blob Environments within the Large-Scale Structure
• The SAGA Survey. IV. The Star Formation Properties of 101 Satellite Systems around Milky Way-mass Galaxies
• The Stellar Mass Function in CANDELS and Frontier Fields: the build-up of low mass passive galaxies since z~3
• Observations of the Initial Formation and Evolution of Spiral galaxies at $1<z<3$ in the CANDELS fields
• Changing Ionization Conditions in SDSS Galaxies with AGN as a Function of Environment from Pairs to Clusters
• Star formation and quenching among the most massive galaxies at z~1.7
• Brightest group galaxies and the large-scale environment
• Active Galactic Nuclei from HeII: a more complete census of AGN in SDSS galaxies yields a new population of low-luminosity AGN in highly star-forming galaxies
• Galaxy And Mass Assembly (GAMA): Timescales for galaxies crossing the green valley
• SDSS-IV MaNGA: Internal mass distributions and orbital structures of early-type galaxies and their dependence on environment
• The GOGREEN survey: Dependence of galaxy properties on halo mass at z > 1 and implications for environmental quenching
• Galaxy populations in the Hydra I cluster from the VEGAS survey I. Optical properties of a large sample of dwarf galaxies
• The MaNGA FIREFLY Value-Added-Catalogue: resolved stellar populations of 10,010 nearby galaxies
• The Intrinsic Scatter of Galaxy Scaling Relations
• HST/WFC3 grism observations of $z\sim 1$ clusters: Evidence for rapid outside-in environmental quenching from spatially resolved H$\alpha$ maps
• Environmental dependence of the galaxy stellar mass function in the Dark Energy Survey Science Verification Data
• On the environmental influence of groups and clusters of galaxies beyond the virial radius: Galactic conformity at few Mpc scales
• The interstellar medium and feedback in the progenitors of the compact passive galaxies at z~2
• Resolved Star Formation on Sub-galactic Scales in a Merger at z=1.7
• Kinematic analysis of EAGLE simulations: Evolution of ${\lambda }_{Re}$ and its connection with mergers and gas accretion
• VIS3COS: III. environmental effects on the star formation histories of galaxies at z~0.8 seen in [OII], H$\delta$, and Dn4000
• Color-Magnitude Distribution of Face-on Nearby Galaxies in SDSS DR7
• Quantifying the suppression of the (un)-obscured star formation in galaxy cluster cores at 0.2$\lesssim$$z$$\lesssim$0.9
• Spectroscopic Confirmation of two Extremely Massive Protoclusters BOSS1244 and BOSS1542 at $z=2.24$
• The definition of environment and its relation to the quenching of galaxies at z=1-2 in a hierarchical Universe
• Fraction of Clumpy Star-Forming Galaxies at $0.5\le z\le 3$ in UVCANDELS: Dependence on Stellar Mass and Environment
• Demonstrating Diversity in Star Formation Histories with the CSI Survey
• COSMOS2020: UV selected galaxies at $z\ge 7.5$
• The SAMI galaxy survey: galaxy size can explain the offset between star-forming and passive galaxies in the mass-metallicity relationship
• WALLABY Pre-Pilot Survey: The effects of tidal interaction on radial distribution of color in galaxies of the Eridanus supergroup
• Molecular Gas Reservoirs in Massive Quiescent Galaxies at $\mathrm{z}\sim 0.7$ Linked to Late Time Star Formation
• BUDHIES IV: Deep 21-cm neutral Hydrogen, optical and UV imaging data of Abell 963 and Abell 2192 at z $\simeq$ 0.2
• Implications of the Environments of Radio-detected AGN in a Complex Protostructure at z$\sim$3.3
• Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
• A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE).XIV. The main sequence relation in a rich environment down to M_star ~ 10^6 Mo
• GOGREEN: a critical assessment of environmental trends in cosmological hydrodynamical simulations at z ~ 1
• Stacked star formation rate profiles of bursty galaxies exhibit 'coherent' star formation
• The Stripe 82 Massive Galaxy Project III: A Lack of Growth Among Massive Galaxies
• CLEAR: The Evolution of Spatially Resolved Star Formation in Galaxies between $0.5\lesssim z\lesssim 1.7$ using H$\alpha$ Emission Line Maps
• The dark side of galaxy stellar populations I: The stellar-to-halo mass relation and the velocity dispersion - halo mass relation
• A declining major merger fraction with redshift in the local Universe from the largest-yet catalog of major and minor mergers in SDSS
• From starburst to quiescence: post-starburst galaxies and their large-scale clustering over cosmic time
• Characterising the evolving $K$-band luminosity function using the UltraVISTA, CANDELS and HUDF surveys
• Properties of Galaxies in Cosmic Filaments around the Virgo Cluster
• The environment of AGN dwarf galaxies at z$\sim$0.7 from the VIPERS survey
• DustPedia - the relationships between stars, gas and dust for galaxies residing in different environments
• The evolution of the cluster optical galaxy luminosity function between z=0.4 and 0.9 in the DAFT/FADA survey
• From Blue Cloud to Red Sequence: Evidence of Morphological Transition Prior to Star Formation Quenching
• The Properties of Hα Emission-Line Galaxies at z = 2.24
• The miniJPAS survey: The role of group environment in quenching the star formation
• Characterizing circumgalactic gas around massive ellipticals at z~0.4 III. The galactic environment of a chemically-pristine Lyman limit absorber
• The role of mass and environment in the build up of the quenched galaxy population since cosmic noon
• The hot circumgalactic media of massive cluster satellites in the TNG-Cluster simulation: existence and detectability
• Hector - a new massively multiplexed IFS instrument for the Anglo-Australian Telescope
• Missing Giants: Predictions on Dust-Obscured Galaxy Stellar Mass Assembly Throughout Cosmic Time
• CO($J$=1-0) mapping survey of 64 galaxies in the Fornax cluster with the ALMA Morita array
• The energy distribution of the first supernovae
• SuperBoRG: Search for The Brightest of Reionizing Galaxies and Quasars in HST Parallel Imaging Data
• UV dust attenuation as a function of stellar mass and its evolution with redshift
• A census of radio-selected AGN on the COSMOS field and of their FIR properties
• DETECTIFz galaxy groups in the REFINE survey -- 1. Group detection and quenched fraction evolution at $z<2.5$
• Galaxy And Mass Assembly (GAMA): Bivariate functions of H$\alpha$ star forming galaxies
• MIGHTEE-HI: the HI Size-Mass relation over the last billion years
• Galaxy clusters and groups in the ALHAMBRA Survey
• Determining the Halo Mass Scale where Galaxies Lose Their Gas
• Characterizing Protoclusters and Protogroups at z $\sim$ 2.5 Using Ly$\alpha$ Tomography
• Implications of a Temperature Dependent IMF II: An Updated View of the Star-Forming Main Sequence
• The Morphological Transformation of Red Sequence Galaxies in Clusters since $z\sim 1$
• Quenching in Cosmic Sheets: Tracing the Impact of Large Scale Structure Collapse on the Evolution of Dwarf Galaxies
• Planck's Dusty GEMS. III. A massive lensing galaxy with a bottom-heavy stellar initial mass function at z=1.5
• Large Scale Structures in COSMOS2020: Evolution of Star Formation Activity in Different Environments at 0.4 < z < 4
• S2COSMOS: Evolution of Gas Mass with Redshift Using Dust Emission
• What is Important? Morphological Asymmetries are Useful Predictors of Star Formation Rates of Star-forming Galaxies in SDSS Stripe 82
• Being WISE II: Reducing the Influence of Star Formation History on the Mass-to-Light Ratio of Quiescent Galaxies
• Star Formation and AGN Feedback in the Local Universe: Combining LOFAR and MaNGA
• Properties of brightest group galaxies in cosmic web filaments
• Galaxy and Mass Assembly (GAMA): Formation and Growth of Elliptical Galaxies in the Group Environment
• Mass and Environment as Drivers of Galaxy Evolution III: The constancy of the faint-end slope and the merging of galaxies
• Across the Green Valley with HST grisms: colour evolution, crossing time-scales and the growth of the red sequence at $z=1.0-1.8$
• Revisiting Attenuation Curves: the Case of NGC 3351
• A universal correlation between star-formation activity and molecular gas properties across environments
• Spectral Energy Distributions for 258 Local Volume Galaxies
• Predicting emission line fluxes and number counts of distant galaxies for cosmological surveys
• A Uniform History for Galaxy Evolution
• Exploring over 700 massive quiescent galaxies at z = 2-7: Demographics and stellar mass functions
• ZFIRE: Similar Stellar Growth in H$\alpha$-emitting Cluster and Field Galaxies at z~2
• Coevolution of metallicity and star formation in galaxies to z=3.7: II. A theoretical model
• Observational Evidence for Enhanced Black Hole Accretion in Giant Elliptical Galaxies
• The relation between morphology, star formation history, and environment in local universe galaxies
• Galaxy and Mass Assembly: luminosity and stellar mass functions in GAMA groups
• A 16 deg${}^2$ survey of emission-line galaxies at z<1.6 from HSC-SSP PDR2 and CHORUS
• Estimating dust attenuation from galactic spectra. II. Stellar and gas attenuation in star-forming and diffuse ionized gas regions in MaNGA
• Reconstructing the Assembly of Massive Galaxies. II. Galaxies Develop Massive and Dense Stellar Cores as They Evolve and Head Toward Quiescence at Cosmic Noon
• Galaxy properties in the cosmic web of EAGLE simulation
• Photometric Objects around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. I. Methods
• A complete spectroscopic catalogue of local galaxies in the Northern spring sky -- Gas properties and nuclear activity in different environments
• WEAVE-StePS. A stellar population survey using WEAVE at WHT
• The GOGREEN Survey: Constraining the Satellite Quenching Timescale in Massive Clusters at $\mathbf{z}\gtrsim 1$
• The HectoMAP Cluster Survey: Spectroscopically Identified Clusters and their Brightest Cluster Galaxies (BCGs)
• Deep spectroscopy of nearby galaxy clusters: II. The Hercules cluster
• S-PLUS DR1 galaxy clusters and groups catalogue using PzWav
• Galaxy Morphologies Revealed with Subaru HSC and Super-Resolution Techniques I: Major Merger Fractions of L_UV~3-15 L_UV* Dropout Galaxies at z~4-7
• Continuous wavelet analysis of matter clustering using the Gaussian-derived wavelet
• The ALHAMBRA survey : $B-$band luminosity function of quiescent and star-forming galaxies at $0.2\le z<1$ by PDF analysis
• AGN-driven quenching of satellite galaxies
• MUSE sneaks a peek at extreme ram-pressure stripping events -- V. Towards a complete view of the galaxy cluster A1367
• Spatially resolved properties of galaxies from CANDELS+MUSE: Radial extinction profile and insights on quenching
• The Elephant in the Bathtub: when the physics of star formation regulate the baryon cycle of galaxies
• The CAVITY project. The spatially resolved stellar population properties of galaxies in voids
• Investigating the Projected Phase Space of Gaussian and Non-Gaussian Clusters
• OMEGA -- OSIRIS Mapping of Emission-line Galaxies in A901/2: II. -- Environmental influence on integrated star formation properties and AGN activity
• Shaping physical properties of galaxy subtypes in the VIPERS survey: environment matters
• MIGHTEE-HI: The HI mass-stellar mass relation over the last billion years
• The submillimetre view of massive clusters at z~0.8-1.6
• Star-formation quenching of cluster galaxies as traced by metallicity, presence of active galactic nuclei, and galactic conformity
• 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
• Local and large-scale effects on the astrophysics of void-galaxies
• The Fornax3D project: Environmental effects on the assembly of dynamically cold disks in Fornax cluster galaxies
• The SAMI -- Fornax Dwarfs Survey II: The Stellar Mass Fundamental Plane and the Dark Matter fraction of Dwarf Galaxies
• The Three Hundred project: connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
• The evolution of star formation activity in galaxy groups
• The Tully-Fisher relation in dense groups at $z\sim 0.7$ in the MAGIC survey
• SDSS-IV MaNGA: Environmental dependence of the Mgb/<Fe>-sigma_* relation for nearby galaxies
• Formation of an ultra-diffuse galaxy in the stellar filaments of NGC3314A: caught in act?
• Do galaxies die? Different views from simulations and observations in the Local Universe
• Scaling relations for globular cluster systems in early-type galaxies. II. Is there an environmental dependence?
• 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 Pan-STARRS1 Medium-deep Survey: Star Formation Quenching in Group and Cluster Environments
• Rest-Frame Near-Infrared Radial Light Profiles up to z=3 from JWST/NIRCam: Wavelength Dependence of the Sérsic Index
• Pre- and post-processing of cluster galaxies out to $5\times R_{200}$: The extreme case of A2670
• A Framework for Empirical Galaxy Phenomenology: The Scatter in Galaxy Ages and Stellar Metallicities
• eROSITA clusters dynamical state and their impact on the BCG luminosity
• The Contribution of Evolved Stars to PAH Heating and Implications for Estimating Star Formation Rates
• The stellar mass function of quiescent galaxies in 2 < z < 2.5 protoclusters
• Some Die Filthy Rich: The Diverse Molecular Gas Contents of Post-starburst Galaxies Probed by Dust Absorption
• Constraining the duration of ram pressure stripping features in the optical from the direction of jellyfish galaxy tails
• Quantifying the Origin and Distribution of Intracluster Light in a Fornax-like Cluster
• DAWN JWST Archive: Morphology from profile fitting of over 340 000 galaxies in major fields
• The evolution of compact massive quiescent and starforming galaxies derived from the $R_e-R_h$ and $M_{\mathrm{star}}-M_h$ relations
• Dynamics and Metallicity of Far-IR Selected Galaxies
• CSST large-scale structure analysis pipeline: I. constructing reference mock galaxy redshift surveys
• Ram Pressure Candidates in UNIONS
• The building up of observed stellar scaling relations of massive galaxies and the connection to black hole growth in the TNG50 simulation
• Modeling Redshift-Space Clustering with Abundance Matching
• Environmental Effect on the Interstellar Medium in Galaxies across the Cosmic Web at z=0.73
• Dissect two-halo galactic conformity effect for central galaxies: The dependence of star formation activities on the large-scale environment
• Setting firmer constraints on the evolution of the most massive, central galaxies from their local abundances and ages
• The Impacts of Modeling Choices on the Inference of the Circumgalactic Medium Properties from Sunyaev-Zeldovich Observations
• Dissecting Nearby Galaxies with piXedfit: II. Spatially Resolved Scaling Relations Among Stars, Dust, and Gas
• On the accretion of a new group of galaxies onto Virgo: II. The effect of pre-processing on the stellar population content of dEs
• 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
• Satellite quenching and morphological transformation of galaxies in groups and clusters
• Deep Extragalactic VIsible Legacy Survey (DEVILS): The emergence of bulges and decline of disk growth since $z=1$
• The Fornax3D project: The environmental impact on gas metallicity gradients in Fornax cluster galaxies
• The Complete Local Volume Groups Sample -- IV. Star formation and gas content in group-dominant galaxies
• NUV signatures of environment driven galaxy quenching in SDSS groups
• Forensic reconstruction of galaxy colour evolution and population characterisation
• Mass and Environment as Drivers of Galaxy Evolution. IV. On the Quenching of Massive Central Disk Galaxies in The Local Universe
• Constraining the Stellar Populations and Star Formation Histories of Blue Compact Dwarf Galaxies with SED Fits
• Quenching depends on morphologies: implications from the ultraviolet-optical radial color distributions in Green Valley Galaxies
• Growing up in a megalopolis: Environmental effects on galaxy evolution in a supercluster at z~0.65 in UKIDSS UDS
• The SAGA Survey. V. Modeling Satellite Systems around Milky Way-mass Galaxies with Updated UniverseMachine
• The Dearth of Difference between Central and Satellite Galaxies III. Environmental Dependence of Mass-Size and Mass-Structure Relations
• Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. III. Accurate Measurement of Galaxy Stellar Mass Function with the Aid of Cosmological Redshift Surveys
• Deep Extragalactic VIsible Legacy Survey (DEVILS): Evolution of the ${\sigma }_{\mathrm{SFR}}$-M${}_{\star }$ relation and implications for self-regulated star formation
• Interrelation of the environment of Ly$\alpha$ emitters and massive galaxies at $2<z<4.5$
• The large molecular gas fraction of post-starburst galaxies at z > 1
• When the Well Runs Dry: Modeling Environmental Quenching of High-mass Satellites in Massive Clusters at \boldmath$z\gtrsim 1$
• The LEGA-C of nature and nurture in stellar populations of galaxies at z~0.6-1.0: D4000 and H-delta reveal different assembly histories for quiescent galaxies in different environments
• Star Formation in Simulated Galaxies: Understanding the Transition to Quiescence at $3\times 10^{10}$ M${}_{\odot }$
• Dependence of the Fundamental Plane of Early-type Galaxies on Age and Internal Structure
• The XXL Survey: XXXVII. The role of the environment in shaping the stellar population properties of galaxies at 0.1<z<0.5
• Synergies between low- and intermediate-redshift galaxy populations revealed with unsupervised machine learning
• HI Global Scaling Relations in the WISE-WHISP Survey
• The H$\alpha$ star formation main sequence in cluster and field galaxies at $z\sim 1.6$
• Effect of richness on AGN and star formation activities in SDSS galaxy groups
• The Chandra COSMOS Legacy Survey: clustering dependence of Type 2 AGN on host galaxy properties
• Nonparametric galaxy morphology from stellar and nebular emission with the CALIFA sample
• Galaxy quenching timescales from a forensic reconstruction of their colour evolution
• Witnessing the star-formation quenching in $L_{\ast }$ ellipticals
• The molecular gas resolved by ALMA in the low-metallicity dwarf merging galaxy Haro 11
• Deep Learning Assessment of galaxy morphology in S-PLUS DataRelease 1
• Do Galaxy Morphologies Really Affect the Efficiency of Star Formation during the Phase of Galaxy Transition?
• Merger-induced star formation in low-metallicity dwarf galaxy NGC 4809/4810
• The SAMI Galaxy Survey: galaxy spin is more strongly correlated with stellar population age than mass or environment
• The PAU Survey: Measurements of the 4000 Å spectral break with narrow-band photometry
• The Stellar-to-Halo Mass Ratios of Passive and Star-Forming Galaxies at z~2-3 from the SMUVS survey
• Evidence for gas-phase metal deficiency in massive protocluster galaxies at z~2.2
• Deep Extragalactic VIsible Legacy Survey (DEVILS): Stellar Mass Growth by Morphological Type since $z=1$
• A Sample of Dust Attenuation Laws for DES Supernova Host Galaxies
• Discrepancies Between JWST Observations and Simulations of Quenched Massive Galaxies at $z>3$: A Comparative Study With IllustrisTNG and ASTRID
• The effect of disk inclination on the Main Sequence of star forming galaxies
• Dead or Alive? How Bursty Star Formation and Patchy Dust Can Cause Temporary Quiescence in High Redshift Galaxies
• Euclid preparation. The Cosmic Dawn Survey (DAWN) of the Euclid Deep and Auxiliary Fields
• A single galaxy population? statistical evidence that the Star-Forming Main Sequence might be the tip of the iceberg
• The first all-sky survey of star-forming galaxies with eROSITA: Scaling relations and a population of X-ray luminous starbursts
• Connecting galaxy structure and star formation: the role of environment in formation of S0 galaxies
• Examining transitional galaxies to understand the role of clusters and their dynamical status in galaxy quenching
• Quasar Sightline and Galaxy Evolution (QSAGE) survey -- II. Galaxy overdensities around UV luminous quasars at z=1-2
• Ageing and Quenching through the ageing diagram: predictions from simulations and observational constraints
• The Global Environment of Small Galaxy Systems
• Rapidly quenched galaxies in the Simba cosmological simulation and observations
• Merger Histories and Environments of Dwarf AGN in IllustrisTNG
• ViCTORIA project: MeerKAT HI observations of the ram pressure stripped galaxy NGC 4523
• Nature versus nurture: relic nature and environment of the most massive passive galaxies at $z<0.5$
• JADES: Rest-frame UV-to-NIR Size Evolution of Massive Quiescent Galaxies from Redshift z=5 to z=0.5
• Implications of a Temperature Dependent IMF III: Mass Growth and Quiescence
• Impact of cosmic filaments on the gas accretion rate of dark matter halos
• Reconstructing the galaxy density field with photometric redshifts: II. Environment-dependent galaxy evolution since $z\simeq 3$
• Mid-Infrared Outbursts in Nearby Galaxies: Nuclear Obscuration and Connections to Hidden Tidal Disruption Events and Changing-Look Active Galactic Nuclei
• The bright end of the galaxy luminosity function at $z\simeq 7$ from the VISTA VIDEO survey
• What Regulates Galaxy Evolution? Open Questions in Our Understanding of Galaxy Formation and Evolution
• The impact of stellar bars on star-formation quenching: Insights from a spatially resolved analysis in the local Universe
• Discovering Large-Scale Structure at $2<z<5$ in the C3VO Survey
• Exploring Galaxy Evolution Time-Scales in Clusters: Insights from the Projected Phase Space
• COSMOS-Web: A history of galaxy migrations over the stellar mass-star formation rate plane
• The role of stochastic and smooth processes in regulating galaxy quenching
• Green valley galaxies in the cosmic web: internal versus environmental quenching
• The role of environment in galaxy evolution in the SERVS Survey I: density maps and cluster candidates
• Subaru Hyper Suprime-Cam revisits the large-scale environmental dependence on galaxy morphology over 360 deg${}^2$ at z=0.3-0.6
• How the Galaxy-Halo Connection Depends on Large-Scale Environment
• The Complex Gaseous and Stellar environments of the nearby dual AGN Mrk 739
• Starbursts with suppressed velocity dispersion revealed in a forming cluster at z=2.51
• Panchromatic Photometry of Low-redshift, Massive Galaxies Selected from SDSS Stripe 82
• Semi-analytic spectral fitting: simultaneously modelling the mass accumulation and chemical evolution in MaNGA spiral galaxies
• Detection of anisotropic satellite quenching in galaxy clusters up to $z\sim 1$
• SITELLE Hα Imaging Spectroscopy of z~0.25 Clusters: Emission Line Galaxy Detection and Ionized Gas Offset in Abell 2390 & Abell 2465
• The miniJPAS survey: The galaxy populations in the most massive cluster in miniJPAS, mJPC2470-1771
• COSMOS-Web: The emergence of the Hubble Sequence
• The quenched mass portion of star-forming galaxies and the origin of the star formation sequence slope
• Environmental impacts on dust temperature of star-forming galaxies in the local Universe
• A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) XV. The Halpha luminosity function of the Virgo cluster
• Quenching or Bursting: Star Formation Acceleration--A New Methodology for Tracing Galaxy Evolution
• Environments of dwarf galaxies with optical AGN characteristics
• Implications of Increased Central Mass Surface Densities for the Quenching of Low-mass Galaxies
• Quenching, bursting and galaxy shapes: colour transformation as a function of morphology
• Galaxy And Mass Assembly: Group and field galaxy morphologies in the star-formation rate - stellar mass plane
• MAGIC: Muse gAlaxy Groups In Cosmos -- A survey to probe the impact of environment on galaxy evolution over the last 8 Gyr
• Environmental dependence of AGN activity and star formation in galaxy clusters from Magneticum simulations
• Compact Galaxies at Intermediate Redshifts Quench Faster than Normal-sized Galaxies
• The origin of star-gas misalignments in simulated galaxies
• Scaling relations of z~0.25-1.5 galaxies in various environments from the morpho-kinematic analysis of the MAGIC sample
• Resolved Stellar Mass Maps of Galaxies in the Hubble Frontier Fields: Evidence for Mass Dependency in Environmental Quenching
• Evidence for anisotropic quenching in massive galaxy clusters at $z\approx 0.5$
• Misalignment between cold gas and stellar components in early-type galaxies
• The effect of the environment on the structure, morphology and star-formation history of intermediate-redshift galaxies
• Early results from GLASS-JWST. XX: Unveiling a population of "red-excess'' galaxies in Abell2744 and in the coeval field
• A spectroscopic study of a rich cluster at z=1.52 with Subaru $\&$ LBT: the environmental impacts on the mass-metallicity relation
• On the nature of Small Galaxy Systems
• The Nature and Evolution of Early Massive Quenched Galaxies in the Simba-C Simulation
• The Infrared Medium-Deep Survey II: How to Trigger Radio-AGN? Hints from Their Environments
• A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE).XI. Two dimensional H$\alpha$ kinematics of the edge-on ram pressure stripped galaxy NGC 4330
• The Subtle Effects of Mergers on Star Formation in Nearby Galaxies
• Subaru Hyper Suprime-Cam excavates colossal over- and under-dense structures over 360 deg2 out to z=1
• Spatially resolved signature of quenching in star-forming galaxies
• The Host Galaxies of Radio AGN: New Views from Combining LoTSS and MaNGA Observations
• The Local Cluster Survey II: Disk-Dominated Cluster Galaxies with Suppressed Star Formation
• Do cluster properties affect the quenching rate?
• Hickson-like compact groups inhabiting different environments
• The Influence of Environment on the Chemical Evolution in Low-mass Galaxies
• Reconstructing Orbits of Galaxies in Extreme Regions (ROGER) II: reliability of projected phase-space in our understanding of galaxy populations
• A systematic search for galaxy protocluster cores at the transition epoch of their star formation activity
• Dust in High-Redshift Galaxies: Reconciling UV Attenuation and IR Emission
• The connection between stellar mass, age and quenching timescale in massive quiescent galaxies at $z\simeq 1$
• Census of Gaseous Satellites around Local Spiral Galaxies
• Star formation histories of Coma Cluster galaxies matched to simulated orbits hint at quenching around first pericenter
• Linking galaxies to dark matter haloes at $z\sim 1$ : dependence of galaxy clustering on stellar mass and specific star formation rate
• Ram pressure stripping in clusters: Gravity can bind the ISM but not the CGM
• 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
• A new analytic ram pressure profile for satellite galaxies
• Galaxy and Mass Assembly (GAMA): Tracing galaxy environment using the marked correlation function
• The SAMI Galaxy Survey: Using concentrated star-formation and stellar population ages to understand environmental quenching
• Reconciling Mass Functions with the Star-Forming Main Sequence Via Mergers
• The AGORA High-Resolution Galaxy Simulations Comparison Project VII: Satellite quenching in zoom-in simulation of a Milky Way-mass halo
• Tracing the evolutionary pathways of dust and cold gas in high-z quiescent galaxies with SIMBA
• SDSS IV MaNGA: Characteristics of Edge-on Galaxies with a Counter-rotating Gaseous Disk
• The G-dwarf distribution in star-forming galaxies: a tug-of-war between infall and outflow
• 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 and Chemical Enrichment in Protoclusters
• JWST/NIRSpec spectroscopy of intermediate-mass quiescent galaxies at $z\sim 3-4$
• The dark side of galaxy stellar populations II: The dependence of star formation histories on halo mass and on the scatter of the main sequence
• An environment-dependent halo mass function as a driver for the early quenching of $z\ge 1.5$ cluster galaxies
• Environments of red nuggets at z~0.7 from the VIPERS survey
• Investigating the link between inner gravitational potential and star-formation quenching in CALIFA galaxies
• The causal effect of environment on halo mass and concentration
• The effect of the morphological quenching mechanism on star formation activity at 0.5 < z < 1.5 in 3D-HST/CANDELS
• 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
• Constraining quenching timescales in galaxy clusters by forward-modelling stellar ages and quiescent fractions in projected phase space
• First Resolved Dust Continuum Measurements of Individual Giant Molecular Clouds in the Andromeda Galaxy
• The Loneliest Galaxies in the Universe: A GAMA and GalaxyZoo Study on Void Galaxy Morphology
• SDSS-IV MaNGA: When is morphology imprinted on galaxies?
• VERTICO VI: Cold-gas asymmetries in Virgo cluster galaxies
• Probing galaxy evolution through HI 21-cm emission and absorption: current status and prospects with the Square Kilometre Array
• Correlation of the rate of Type Ia supernovae with the parent galaxy properties: Light and shadows
• BANG-MaNGA: A census of kinematic discs and bulges across mass and star formation in the local Universe
• MusE GAs FLOw and Wind (MEGAFLOW) VII. A NOEMA pilot program to probe molecular gas in galaxies with measured circumgalactic gas flows
• Ageing and Quenching through the ageing diagram II: physical characterization of galaxies
• From Halos to Galaxies. VI. Improved halo mass estimation for SDSS groups and measurement of the halo mass function
• LARgE Survey. I. Dead Monsters: the Massive End of the Passive Galaxy Stellar Mass Function at Cosmic Noon
• The SAMI Galaxy Survey: The contribution of different kinematic classes to the stellar mass function of nearby galaxies
• The Atomic Hydrogen Content of Galaxies as a function of Group-Centric Radius
• Probing galaxy evolution from $z=0$ to $z\simeq 10$ through galaxy scaling relations in three L-Galaxies flavours
• Star formation history and transition epoch of cluster galaxies based on the Horizon-AGN simulation
• Insights on star formation histories and physical properties of $1.2\le z\lesssim 4$ Herschel-detected galaxies
• Galaxy populations in the most distant SPT-SZ clusters -- II. Galaxy structural properties in massive clusters at 1.4<z<1.7
• BreakBRD Galaxies I: Global Properties of Spiral Galaxies with Central Star Formation in Red Disks
• Double Trouble: Two spectroscopically confirmed low-mass quiescent galaxies at z>5 in overdensities
• The mass-dependent UVJ diagram at cosmic noon: A challenge for galaxy evolution models and dust radiative transfer
• Consistent analysis of the AGN LF in X-ray and MIR in the XMM-LSS field
• Environmental cluster effects and galaxy evolution: The HI properties of the Abell clusters A85/A496/A2670
• PAC in DESI. I. Galaxy Stellar Mass Function into the $10^6{\mathrm{M}}_{\odot }$ Frontier
• PAC.V. The Roles of Mass and Environment in the Quenching of Galaxies
• Age and Metallicity of galaxies in different environments of the Coma supercluster
• SDSS-IV MaNGA: Unveiling Galaxy Interaction by Merger Stages with Machine Learning
• The MeerKAT Galaxy Clusters Legacy Survey: star formation in massive clusters at 0.15 < z < 0.35
• Resolved star formation in TNG100 central and satellite galaxies
• CALSAGOS: Clustering ALgorithmS Applied to Galaxies in Overdense Systems
• From haloes to galaxies. III. The gas cycle of local galaxy populations
• MOSEL and IllustrisTNG: Massive Extended Galaxies at z=2 Quench Later Than Normal-size Galaxies
• Euclid preparation. LI. Forecasting the recovery of galaxy physical properties and their relations with template-fitting and machine-learning methods
• Connecting the growth of galaxies to the large-scale environment in a massive node of the Cosmic Web at z~3
• Early-type galaxies at intermediate redshift observed with HST WFC3: perspectives on recent star-formation
• VST-GAME: Galaxy Assembly as a function of Mass and Environment with VST. Photometric assessment and density field of MACSJ0416
• The extragalactic $\gamma$-ray background: imprints from the physical properties and evolution of star-forming galaxy populations
• Measuring the X-ray luminosities of DESI groups from eROSITA Final Equatorial-Depth Survey: I. X-ray luminosity -- halo mass scaling relation
• The XXL survey. XLIX. Linking the members star formation histories to the cluster mass assembly in the z=1.98 galaxy cluster XLSSC 122
• Star Formation Properties of Sloan Digital Sky Survey BOSS Void Galaxies in the Hyper Suprime-Cam Survey
• Machine learning technique for morphological classification of galaxies from SDSS. II. The image-based morphological catalogs of galaxies at 0.02<z<0.1
• Size, shade or shape? The contribution of galaxies of different types to the star-formation history of the Universe from SDSS-IV MaNGA
• Decoding the IRX-β dust attenuation relation in star-forming galaxies at intermediate redshift
• Environmental Effects on AGN activity via Extinction-free Mid-Infrared Census
• Probing the Mpc-scale environment of hyperluminous infrared galaxies at 2<z<4
• MAMBO -- An empirical galaxy and AGN mock catalogue for the exploitation of future surveys
• LARgE Survey -- II. The Dark Matter Halos and the Progenitors and Descendants of Ultra-Massive Passive Galaxies at Cosmic Noon
• Interpreting the relation between the gamma-ray and infrared luminosities of star-forming galaxies
• Galaxy And Mass Assembly (GAMA): The environmental impact on SFR and metallicity in galaxy groups
• A general approach to quenching and galactic conformity
• Measuring the Total Ultraviolet Light from Galaxy Clusters at z=0.5-1.6: The Balance of Obscured and Unobscured Star-Formation
• Critical Stellar Central Densities Drive Galaxy Quenching in the Nearby Universe
• A stochastic model to reproduce the star-formation history of individual galaxies in hydrodynamic simulations
• The kinematic bimodality: Efficient feedback and cold gas deficiency in slow-rotating galaxies
• Re-assessing the stellar population scaling relations of the galaxies in the Local Universe
• A systematic search for dormant galaxies at z~5-7 from the JWST NIRSpec archive
• A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) XVII. Statistical properties of individual HII regions in unperturbed systems
• Inferring redshift and galaxy properties via a multi-task neural net with probabilistic outputs: An application to simulated MOONS spectra
• The effect of local and large scale environment on the star formation histories of galaxies
• Thermal Regulation and the Star-Forming Main Sequence
• Cluster candidates with massive quiescent galaxies at $z\sim 2$
• The LAMOST Complete Spectroscopic Survey of Pointing Area (LaCoSSPAr) in the Southern Galactic Cap I. The Spectroscopic Redshift Catalog
• The correlations between galaxy properties in different environments of the cosmic web
• The Origin of Star Formation in Early-type Galaxies Inferred from Spatially Resolved Spectroscopy
• Unveiling the Universe with Emerging Cosmological Probes
• SEEDisCS II. Molecular gas in galaxy clusters and their large scale structure: low gas fraction galaxies, the case of CL1301.7$-$1139
• Optimizing high redshift galaxy surveys for environmental information
• Constraints on the galaxy "main sequence" at z>5: the stellar mass of HDF850.1
• The EDGE-CALIFA survey: Star formation relationships for galaxies at different stages of their evolution
• Topological data analysis reveals differences between simulated galaxies and dark matter haloes
• COSMOS-Web galaxy groups: Evolution of red sequence and quiescent galaxy fraction
• Star formation concentration as a tracer of environmental quenching in action: a study of the Eagle and C-Eagle simulations
• Spatially resolved self-consistent spectral modelling of jellyfish galaxies from MUSE with FADO: trends with mass and stripping intensity
• A Large Molecular Gas Reservoir in the Protocluster SPT2349$-$56 at $z=4.3$
• An Enigmatic 380 kpc Long Linear Collimated Galactic Tail
• Constraints on the Evolution of the Galaxy Stellar Mass Function II: Quenching Timescale of Galaxies and its Implication for their Star Formation Rate
• COSMOS2020: Disentangling the Role of Mass and Environment in Star Formation Activity of Galaxies at $0.4<z<4$
• Are early-type galaxies quenched by present-day environment? A study of dwarfs in the Fornax Cluster
• Test of Cosmic Web-feeding Model for Star Formation in Galaxy Clusters in the COSMOS Field
• Spitzer's View of the Candidate Cluster and Protocluster Catalog (CCPC)
• The recent star formation history of NGC 628 on resolved scales
• The SAMI Galaxy Survey: Trends in [α/Fe] as a Function of Morphology and Environment
• The properties and environment of very young galaxies in the local Universe
• The XXL Survey XLV. Linking the ages of optically selected groups to their X-ray emission
• Star-forming and Quiescent Central Galaxies Cluster Similarly: Implications for the Galaxy-Halo Connection
• HELLO project: High-$z$ Evolution of Large and Luminous Objects
• Recently Quenched Galaxies at z = 0.2 - 4.8 in the COSMOS UltraVISTA Field
• Evidence for Non-smooth Quenching in Massive Galaxies at $z\sim 1$
• The evolution of baryonic mass function of galaxies to z=3
• Modeling Star Formation Histories of Changing-Look AGN Host Galaxies with Prospector
• Cosmic Stillness: High Quiescent Galaxy Fractions Across Upper Mass Scales in the Early Universe to z = 7 with JWST
• Luminosity Distribution of Dwarf Elliptical-like Galaxies
• The miniJPAS survey. Evolution of the luminosity and stellar mass functions of galaxies up to $z\sim 0.7$
• Exploring the evolution of star formation and dwarf galaxy properties with JWST/MIRI serendipitous spectroscopic surveys
• Measuring Structural Parameters Through Stacking Galaxy Images
• The luminosity of cluster galaxies in the Cluster-EAGLE simulations
• Galaxy And Mass Assembly (GAMA): $\mathbf{z}\sim 0$ Galaxy Luminosity Function down to $\mathbf{L}\sim 10^6{\mathbf{L}}_{\odot }$ via Clustering Based Redshift Inference
• Testing galaxy formation models with the stellar mass-halo mass relations for star-forming and quiescent galaxies
• Targeting cluster galaxies for the 4MOST CHANCES Low-z sub-survey with photometric redshifts
• Estimation of the Galaxy Quenching Rate in the Illustris Simulation
• Quenching of Galaxies at Cosmic Noon: Understanding the Effect of Environment
• Red riding on hood: Exploring how galaxy colour depends on environment
• Galaxy Evolution in the Cluster Abell 85: New Insights from the Dwarf Population
• Exploring the interplay of dust and gas phases in DustPedia star-forming galaxies
• Star formation across cosmic time
• MIGHTEE-\HI: Possible interactions with the galaxy NGC~895
• Red Dragon: A Redshift-Evolving Gaussian Mixture Model for Galaxies
• H$\alpha$-based Star Formation Rates in and around z $\sim$ 0.5 EDisCS clusters
• The effects of environment on galaxies' dynamical structures: From simulations to observations
• Central star formation in an early-type galaxy I~Zw~81 in the Bootes void
• The impact of environment on the lives of disk galaxies as revealed by SDSS-IV MaNGA
• Shedding light on the star formation rate-halo accretion rate connection and halo quenching mechanism via DECODE, the Discrete statistical sEmi-empiriCal mODEl
• Impact of cosmic web on the properties of galaxies in IllustrisTNG simulations
• Quenching vs. Quiescence: forming realistic massive ellipticals with a simple starvation model
• Insights into environmental quenching at $z\sim 1$: an enhancement of faint, low-mass passive galaxies in clusters
• Introducing cosmosTNG: simulating galaxy formation with constrained realizations of the COSMOS field
• Environmental impact on star-forming galaxies in a $z\sim 0.9$ cluster during course of galaxy accretion
• The Compactness of Galaxy Groups in the Sloan Digital Sky Survey
• Environmental effects on associations of dwarf galaxies
• Active Galactic Nuclei in the Green Valley at z$\sim$0.7
• Diving into dangerous tides: The impact of galaxy cluster tidal environments on satellite galaxy mass densities
• pop-cosmos: Insights from generative modeling of a deep, infrared-selected galaxy population
• The EDGE-CALIFA survey: The effect of active galactic nucleus feedback on the integrated properties of galaxies at different stages of their evolution
• Quantifying the Active Galactic Nuclei Fraction in Cosmic Voids via Mid-Infrared Variability
• Star formation and stellar & AGN feedback in the absence of accretion, not gas stripping, set the quenching timescale in satellite galaxies
• Star formation history of $0.1\le \text{z}\le 1.5$ mass-selected galaxies in the ELAIS-N1 Field
• Machine Learning Classification of COSMOS2020 Galaxies: Quiescent vs. Star-Forming
• Evolution of dwarf galaxy observable parameters
• A census of quiescent galaxies across $0.5<z<8$ with JWST/MIRI: Mass-dependent number density evolution of quiescent galaxies in the early Universe
• The inflow and outflow rate evolution of local Milky Way-mass star-forming galaxies since z=1.3
• Unveiling the gravitationally unstable disc of a massive star-forming galaxy using NOEMA and MUSE
• The Earliest Stage of Galactic Star Formation
• VALES VIII: Weak ionized gas outflows in star-forming galaxies at $z\sim 0.15$ traced with VLT/MUSE
• Touching the Stars: Using High-Resolution 3D Printing to Visualize Stellar Nurseries
• A MaNGA view of isolated galaxy mergers in the star-forming Main Sequence
• ZFIRE: The Beginning of the End for Massive Galaxies at z ~ 2 and Why Environment Matters
• Detection of extended millimeter emission in the host galaxy of 3C273 and its implications for QSO feedback via high dynamic range ALMA imaging
• Galaxy Manifold: Characterizing and understanding galaxies with two parameters
• Searching for Spectroscopic Signatures of Ongoing Quenching in SDSS Galaxies
• Structure and Kinematics of Star-forming Elliptical Galaxies in SDSS-MaNGA
• Quantifying the Impact of Incompleteness on Identifying and Interpreting Galaxy Protocluster Populations with the TNG-Cluster Simulation
• LeMMINGs. VI. Connecting nuclear activity to bulge properties of active and inactive galaxies: radio scaling relations and galaxy environment
• Investigating the Dominant Environmental Quenching Process in UVCANDELS/COSMOS Groups
• The Chocolate Chip Cookie Model: dust-to-metal ratio of HII regions
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• Galaxy Correlation Function and Local Density from Photometric Redshifts Using the Stochastic Order Redshift Technique (SORT)
• Stochastic Order Redshift Technique (SORT): a simple, efficient and robust method to improve cosmological redshift measurements
• Improved SED-Fitting Assumptions Result in Inside-Out Quenching at $z\sim 0.5$ and Quenching at All Radii Simultaneously at $z\sim 1$
• Born to be Starless: Revisiting the Missing Satellite Problem
• Brighter and More Massive Galaxies in the Vicinity of Lyman-alpha Nebulae
• The XMM-SERVS X-ray eXtended Galaxy Cluster (XVXGC) catalog
• Central Concentration of Asymmetric Features in Post-starburst Galaxies at $z\sim 0.8$
• Deep Extragalactic VIsible Legacy Survey (DEVILS): First Data Release Covering The D10 (COSMOS) Region
• Intrinsic and Environmental Effects on the Distribution of Star Formation in TNG100 Galaxies
• SG1120-1202: Mass-Quenching as Tracked by UV Emission in the Group Environment at z=0.37
• Boosting the evolutionary picture of Cl 0024+17 and MS 0451-03: A case study at intermediate-redshift
• The effect of environment on the properties of the most massive galaxies at $0.5<z<2.5$ in the cosmos-dash field
• The origin of the galaxy size-stellar metallicity relation: A semi-analytical perspective
• Fundamental relation in isolated galaxies, pairs, and triplets in the local universe
• Strong-lensing and kinematic analysis of CASSOWARY 31: can strong lensing constrain the masses of multi-plane lenses?
• Transforming galaxies with EASE: widespread structural changes enabled by short-lived spirals
• Bright siren without electromagnetic counterpart by LISA-Taiji-TianQin network
• The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes
• Exploring the stellar populations of backsplash galaxies
• MaNGA DynPop. VII. A Unified Bulge-Disk-Halo Model for Explaining Diversity in Circular Velocity Curves of 6000 Spiral and Early-Type Galaxies
• The distribution of local star formation activity as a function of galaxy stellar mass, environment and morphology
• Characterising EP241107a: Multiwavelength Observations of an Einstein Probe-detected Fast X-ray Transient
• The stellar mass function of quiescent and star-forming galaxies and its dependence on morphology in COSMOS-Web
• Effects of Environment on the Size Evolution of Quiescent Galaxies: Comparing Galaxies in Clusters and in the Field at Two Rest-frame Wavelengths
• Photometric variability in star-forming galaxies as evidence for low-mass AGN and a precursor to quenching
• Reconstructing galaxy star formation histories from COSMOS2020 photometry using simulation-based inference
• Pre-heating of the intergalactic medium by gravitational collapse and ultraviolet background
• The galaxy-environment connection revealed by constrained simulations
• Euclid Quick Data Release (Q1): The evolution of the passive-density and morphology-density relations between $z=0.25$ and $z=1$
• The COSMOS Wall at z$\sim$0.73: star-forming galaxies and their evolution in different environments
• The role of gas stripping in the quenching of satellite galaxies using SHARK v2.0
• Exploring Galaxy Properties of eCALIFA with Contrastive Learning
• Late growth of early-type galaxies in low-z massive clusters
• Impact of redshift distribution uncertainties on Lyman-break galaxy cosmological parameter inference
• A Bending in the Size-mass Relation of Star-forming Galaxies across $0.5<z<6.0$ at a Critical Stellar Mass of $10^{10}{M}_{\odot }$ Revealed by JWST
• Star Formation Rates in [Ne V] 3426 Å Selected Active Galactic Nuclei: Evidence for a Decrease along the Main Sequence?
• Machine Learning vs. Spectral Energy Distribution Fitting: A Comparative Analysis of Accuracy in Stellar Mass Estimation
• SEW: A full-spectrum linear fitting with stellar population synthesis method Based on "Equivalent Widths spectrum"
• Environmental Quenching of Low Surface Brightness Galaxies near Milky Way mass Hosts
• Assessing the connection between galactic conformity and assembly-type bias
• Major merger fraction along the massive galaxy quenching channel at 0.2$<z<$0.7
• A High-resolution Far-infrared Survey to Probe Black Hole-Galaxy Co-evolution
• Euclid preparation: TBD. Cosmic Dawn Survey: evolution of the galaxy stellar mass function across 0.2<z<6.5 measured over 10 square degrees
• SEMPER I. Radio Predictions for Star-Forming Galaxies at $0<z<5$
• The slope and scatter of the star forming main sequence at z~5 : reconciling observations with simulations
• The effects of star formation history in the SFR-M relation of HII galaxies
• Properties of Barred Galaxies with the Environment: II. The case of the Cosmic Web around the Virgo cluster
• MIGHTEE-HI: The star-forming properties of HI selected galaxies
• Dissecting the mass quenching in TNG50: Galaxy size determines the quenching mode
• From Halos to Galaxies. X: Decoding Galaxy SEDs with Physical Priors and Accurate Star Formation History Reconstruction
• Capivara: A Spectral-based Segmentation Method for IFU Data Cubes
• GLACE survey: galaxy activity in ZwCl0024+1652 cluster from strong optical emission lines
• SNITCH: Seeking a simple, informative star formation history inference tool
• Main sequence of star formation and colour bimodality considering galaxy environment
• Insights into the dependence of galaxy properties on the environment with explainable machine learning models
• CosmoGLINT: Cosmological Generative Model for Line Intensity Mapping with Transformer
• Isolated and group environment dependence of stellar mass and different star formation rates
• Cosmic Dragons: A Two-Component Mixture Model of COSMOS Galaxies
• COMAP Pathfinder -- Season 2 results IV. A stack on eBOSS/DESI quasars
• The Next Generation Virgo Cluster Survey (NGVS). XL. The Morphological Classification of Virgo Cluster Galaxies
• Sub-Gyr variability around the SFMS and its contribution to the scatter
• LEGA-C stellar populations scaling relations. II: Dissecting mass-complete archaeological trends and their evolution since z~0.7 with LEGA-C and SDSS
• Probing the influence of the protocluster environment on galaxy morphology at z = 2.23
• Tracing ionized gas kinematics in Lyman-Break Analogs. Implications for star formation compactness and outflow properties
• Dynamical properties and star formation history of a low-mass quenched galaxy at Cosmic Noon
• Star formation quenching precedes morphological transformation in COSMOS-WEB's richest galaxy groups
• The S-PLUS Fornax Project (S+FP): An extragalactic catalog covering $\sim$ 5 virial radii around NGC 1399 with galaxy properties
• Mechanisms Affecting Galaxies Nearby and Environmental Trends (MAGNET)
• The velocity dispersion function of red galaxies in four Hubble Frontier Fields galaxy clusters
• The CAVITY project. The spatially resolved SFR of galaxies in voids
• Blueberry and Green Pea galaxies live in low density environments
• A SHARP Look at Quenching and Bulge-Disk Growth in Massive Galaxies at Cosmic Noon
• SUNRISE-3D: Sharp UNveiling of AGN feedback Regulation and its Impact on Star-formation at the cosmic noon Epoch
• Nowhere Left to Hide: Uncovering All of the Massive Young Embedded Star Clusters in the Antennae with JWST
• The LEGA-C galaxy survey: multiple quenching channels for quiescent galaxies at $z\sim 1$
• Galaxy And Mass Assembly (GAMA): From filaments to voids, how extreme environment affects gas metallicity and SFR in galaxies
• Recent star formation in 0.5<z<1.5 quiescent galaxies
• Stellar population modelling of neutron stars and black holes: spatially-resolved graveyards in MaNGA/SDSS-IV galaxies
• Emergence of the Galaxy Morphology-Star Formation Activity-Clustercentric Radius Relations in Galaxy Clusters
• SDSS-IV MaNGA: Stellar rotational support in disk galaxies vs. central surface density and stellar population age
• Star-formation Properties of z ~ 1 Galaxy Clusters and Groups from Horizon Run 5
• What halts the growth of galaxies?
• Modelling gas around galaxy pairs and groups using the Q0107 quasar triplet
• Cluster environment quenches the star formation of low-mass satellite galaxies from the inside-out
• ALMA measures molecular gas reservoirs comparable to field galaxies in a low-mass galaxy cluster at z=1.3
• 3D intrinsic shapes of quiescent galaxies in observations and simulations
• Past, present and Future of the Scaling Relations of Galaxies and Active Galactic Nuclei
• A phylogenetic analysis of galaxies in the Coma Cluster and the field: a new approach to galaxy evolution
• On the signature of black holes on the quenched stellar mass function
• Exploring supermassive black hole physics and galaxy quenching across halo mass in FIRE cosmological zoom simulations
• Euclid preparation. Predicting star-forming galaxy scaling relations with the spectral stacking code SpectraPyle
• The gMOSS: the galaxy survey and galaxy populations of the large homogeneous field
• Detailed properties of gravitational-wave mergers from flyby perturbations of wide binary black holes in the field
• Noema formIng Cluster survEy (NICE): A Census of Star Formation and Cold Gas Properties in Massive protoclusters at 1.5<z<4
• Investigating the Impacts of AGN Activities on Dwarf Galaxies with FAST HI Observations
• On the hosts of neutron star mergers in the nearby Universe
• SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass
• The Journey to Dominance: How BCGs Evolve Differently from Other Massive Galaxies
• Size-Mass Relation Shows Its Colours: Contrasting Physical Imprints of Galaxy Evolution in Rest-Frame UV and Optical
• Morpho-kinematics of MACS J0416.1-2403 low mass galaxies
• Radar-Chart Analysis of Star-Formation Quenching Stages Across Circular Velocity Curve Classes in Nearby CALIFA Galaxies
• pop-cosmos: Star formation over 12 Gyr from generative modelling of a deep infrared-selected galaxy catalogue
• The peculiar filamentary HI structure of NGC 6145
• Spider-Webb: enhanced star formation in low-mass galaxies within the Spiderweb protocluster revealed by JWST Pa$\beta$ narrow-band imaging
• A Value-added Physical Properties Catalog for Low-redshift Galaxies from DESI Legacy Imaging Surveys DR10
• The galaxy starburst/main-sequence bimodality over five decades in stellar mass at z ~ 3-6.5
• The cosmic environment overtakes the local density in shaping galaxy star formation
• On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback
• Environmental Sculpting of Galaxy Structure at Fixed Stellar Mass: A Multi-Scale Analysis Across Cosmic Time using 3 Million HSC Galaxies
• Galaxy quenching across the Cosmic Web: disentangling mass and environment with SDSS DR18
• Euclid: A blue galaxy population and a brightest cluster galaxy in the making in a $z\sim 1.74$ MaDCoWS2 galaxy cluster candidate
• The influence of the Cosmic Web on the properties of dwarf galaxies in the Fornax-Eridanus Supercluster
• Resolved molecular gas and star-formation in massive unquenched spirals : I. UGC 8179
• Star-forming S0 Galaxies in SDSS-MaNGA: fading spirals or rejuvenated S0s?
• Galaxy and black hole coevolution in dark matter haloes not captured by cosmological simulations
• The miniJPAS survey: Dissecting galaxy properties across environments with spatially resolved photometry
• Testing a New Star Formation History Model from Principal Component Analysis to Facilitate Spectral Synthesis Modeling
• Testing subhalo abundance matching with galaxy kinematics
• Galaxy evolution on resolved scales: ageing and quenching in CALIFA
• Initial Investigations of the Outskirts of XLSSC 122
• Galaxy And Mass Assembly (GAMA): Deconstructing the galaxy stellar mass function by star formation and environment
• The origin of ionized gas in retired galaxies: dynamical clues
• Mocking IFU observations and metallicity diagnostics from cosmological simulations
• Euclid: Discovery of bright $z\simeq 7$ Lyman-break galaxies in UltraVISTA and Euclid COSMOS
• GalSBI-SPS: a stellar population synthesis-based galaxy population model for cosmology and galaxy evolution applications
• Identifying and Repairing Catastrophic Errors in Galaxy Properties Using Dimensionality Reduction
• The Nun Path: The Evolution and Quenching of Satellite Galaxies
• The Cosmic Rush Hour: Rapid Formation of Bright, Massive, Disky, Star-Forming Galaxies as Signatures of Early-Universe Physics
• Morphological Transformation and Star Formation Quenching of Massive Galaxies at 0.5 < z < 2.5 in 3D-HST/CANDELS
• The Kormendy relation of cluster galaxies in PPS regions
• Understanding the origin of early-type dwarfs: The spectrophotometric study of CGCG014-074
• 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
• A semi-analytical perspective on massive red galaxies: I. Assembly history, environment & redshift evolution
• BASS XXX: Distribution Functions of DR2 Eddington-ratios, Black Hole Masses, and X-ray Luminosities
• Ageing and Quenching: Influence of Galaxy Environment and Nuclear Activity in Transition Stage