The size distribution of galaxies in the Sloan Digital Sky Survey

Abstract

abridged: We use a complete sample of about 140,000 galaxies from the Sloan Digital Sky Survey (SDSS) to study the size distribution of galaxies and its dependence on their luminosity, stellar mass, and morphological type. The large SDSS database provides statistics of unprecedented accuracy. For each type of galaxy, the size distribution at given luminosity (or stellar mass) is well described by a log-normal function, characterized by its median $\bar{R}$ and dispersion ${\sigma }_{\ln R}$. For late-type galaxies, there is a characteristic luminosity at $M_{r,0}\sim -20.5$ (assuming $h=0.7$) corresponding to a stellar mass $M_0\sim 10^{10.6}\Msun$. Galaxies more massive than $M_0$ have $\bar{R}\propto M^{0.4}$ and ${\sigma }_{\ln R}\sim 0.3$, while less massive galaxies have $\bar{R}\propto M^{0.15}$ and ${\sigma }_{\ln R}\sim 0.5$. For early-type galaxies, the $\bar{R}$ - $M$ relation is significantly steeper, $\bar{R}\propto M^{0.55}$, but the ${\sigma }_{\ln R}$ - $M$ relation is similar to that of late-type galaxies. Faint red galaxies have sizes quite independent of their luminosities.

42 pages, 18 figures, 2 tables; replaced with the version accepted by MNRAS

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• Starburst to quiescent from HST/ALMA: Stars and dust unveil minor mergers in submillimeter galaxies at $z\sim 4.5$
• Tracing the Mass-Dependent Star Formation History of Late-Type Galaxies using X-ray Emission: Results from the Chandra Deep Fields
• CLASH-VLT: Environment-driven evolution of galaxies in the z=0.209 cluster Abell 209
• Intrinsic Alignments of Galaxies in the Illustris Simulation
• Environmental dependence of bulge-dominated galaxy sizes in hierarchical models of galaxy formation. Comparison with the local Universe
• A 5x10^9 Solar Mass Black Hole in NGC 1277 from Adaptive Optics Spectroscopy
• Rates and Properties of Strongly Gravitationally Lensed Supernovae and their Host Galaxies in Time-Domain Imaging Surveys
• On the self-regulation of intense star-formation in galaxies at z=1-3
• The role of dry mergers for the formation and evolution of brightest cluster galaxies
• The Dramatic Size and Kinematic Evolution of Massive Early-Type Galaxies
• Avoiding progenitor bias: The structural and mass evolution of Brightest Group and Cluster Galaxies in Hierarchical models since z~1
• The Bivariate Size-luminosity Relations for Lyman Break Galaxies at z ~ 4 - 5
• The SINS/zC-SINF Survey of z~2 Galaxy Kinematics: Rest-frame Morphology, Structure, and Colors from Near-infrared Hubble Space Telescope Imaging
• Early results from GLASS-JWST. V: the first rest-frame optical size-luminosity relation of galaxies at $z>7$
• The stellar mass-size relation for the most isolated galaxies in the local Universe
• Major mergers are not the dominant trigger for high-accretion AGNs at z = 2
• Brightest cluster galaxies in cosmological simulations: achievements and limitations of AGN feedback models
• The structure of post-starburst galaxies at $0.5<z<2$: evidence for two distinct quenching routes at different epochs
• On The Robustness of z=0-1 Galaxy Size Measurements Through Model and Non-Parametric Fits
• Simulations of single and two-component galaxy decompositions for spectroscopically selected galaxies from the Sloan Digital Sky Survey
• Morphologies and Color Gradients of Luminous Evolved Galaxies at z~1.5
• Simulations of Dust in Interacting Galaxies I: Dust Attenuation
• Photometric mass and mass decomposition in early-type lens galaxies
• Tidal Disruption Events and Gravitational Waves from Intermediate-mass Black Holes in Evolving Globular Clusters Across Space and Time
• The fate of high-redshift massive compact galaxies
• The effect of the environment on the stellar mass - size relation of present-day galaxies
• Minor vs Major Mergers: The Stellar Mass Growth of Massive Galaxies from z=3 using Number Density Selection Techniques
• Effective Models for Statistical Studies of Galaxy-Scale Gravitational Lensing
• An EAGLE's View of Ex-situ Galaxy Growth
• Catalog of Visually Classified Galaxies in the Local ($z\sim 0.01$) Universe
• Precision Scaling Relations for Disk Galaxies in the Local Universe
• The information content of stellar halos: Stellar population gradients and accretion histories in early-type Illustris galaxies
• ALFALFA HI Data Stacking III. Comparison of environmental trends in HI gas mass fraction and specific star formation rate
• Spiral arm pitch angle and galactic shear rate in N-body simulations of disc galaxies
• On the Populations of Radio Galaxies with Extended Morphology at z<0.3
• The Millennium Galaxy Catalogue: Exploring the Color-Concentration Bimodality via Bulge-Disc Decomposition
• The influence of environment on satellite galaxies in the GAEA semi-analytic model
• The relationship between fine galaxy stellar morphology and star formation activity in cosmological simulations: a deep learning view
• The unusual NIV]-emitter galaxy GDS J033218.92-275302.7: star formation or AGN-driven winds from a massive galaxy at z=5.56
• Quantitative Morphological Analysis of the HDF--North and HDF-South. I. Early- and Late-type Luminosity-Size Relations of galaxies out to z~1
• The Dissipative Merger Progenitors of Elliptical Galaxies
• The properties of (sub)millimetre-selected galaxies as revealed by CANDELS HST WFC3/IR imaging in GOODS-South
• Associating Fast Radio Bursts with Their Host Galaxies
• Evolution of galaxy size--stellar mass relation from the Kilo Degree Survey
• Morphologies of ~190,000 Galaxies at z=0-10 Revealed with HST Legacy Data. III. Continuum Profile and Size Evolution of Lya Emitters
• Wet Compaction to a Blue Nugget: a Critical Phase in Galaxy Evolution
• Angular momentum distribution of hot gas and implications for disk galaxy formation
• Integrating human and machine intelligence in galaxy morphology classification tasks
• The early early type: discovery of a passive galaxy at z=3
• Dissecting the size-mass and ${\Sigma }_1$-mass relations at 1.0 < z < 2.5: galaxy mass profiles and color gradients as a function of spectral shape
• Baryonic Conversion Tree: The global assembly of stars and dark matter in galaxies from the SDSS
• Testing the predictions of the cold dark matter model for the sizes, colours, morphologies and luminosities of galaxies with the SDSS
• On the Elevation and Suppression of Star Formation within Galaxies
• ALMA 26 Arcmin${}^2$ Survey of GOODS-S at One-millimeter (ASAGAO): Average Morphology of High-$z$ Dusty Star-Forming Galaxies is an Exponential-Disk ($n\simeq 1$)
• Dark halo response and the stellar initial mass function in early-type and late-type galaxies
• The evolution of the mass-size relation to z=3.5 for UV-bright galaxies and sub-mm galaxies in the GOODS-NORTH field
• How to get cool in the heat: comparing analytic models of hot, cold, and cooling gas in haloes and galaxies with EAGLE
• Physics of Galactic Metals: Evolutionary Effects due to Production, Distribution, Feedback & Interaction with Black Holes
• Massive black hole binaries in LISA: multimessenger prospects and electromagnetic counterparts
• The Sizes of Quasar Host Galaxies with the Hyper Suprime-Cam Subaru Strategic Program
• Disk evolution since z=1 in a CDM Universe
• BayeSED: A General Approach to Fitting the Spectral Energy Distribution of Galaxies
• Early-type galaxies at z = 1.3. I. The Lynx supercluster: cluster and groups at z=1.3. Morphology and color-magnitude relation
• HST/WFC3 grism observations of $z\sim 1$ clusters: The cluster vs. field stellar mass-size relation and evidence for size growth of quiescent galaxies from minor mergers
• The evolution of galaxy size and morphology at z~0.5-3.0 in the GOODS-N region with HST/WFC3 data
• The Small Scatter in BH-Host Correlations & The Case for Self-Regulated BH Growth
• Testing Yukawa-like potentials from f(R)-gravity in elliptical galaxies
• Modeling Fast Radio Burst Dispersion and Scattering Properties in the First CHIME/FRB Catalog
• The Decomposed Bulge and Disk Size-Mass Relations of Massive Galaxies at 1<z<3 in CANDELS
• A new population of recently quenched elliptical galaxies in the SDSS
• Puffing up early-type galaxies by baryonic mass loss: numerical experiments
• The impact of quenching on galaxy profiles in the Simba simulation
• On the formation time scale of massive cluster ellipticals based on deep near-IR spectroscopy at z~2
• The low frequency of dual AGNs versus the high merger rate of galaxies: A phenomenological model
• The growth of disks and bulges during hierarchical galaxy formation. I: fast evolution vs secular processes
• 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 mass, colour, and structural evolution of today's massive galaxies since z~5
• The CALIFA view on stellar angular momentum across the Hubble sequence
• Comparing galaxy formation in semi-analytic models and hydrodynamical simulations
• What Sets the Sizes of the Faintest Galaxies?
• The Sloan Lens ACS Survey. XI. Beyond Hubble resolution: size, luminosity and stellar mass of compact lensed galaxies at intermediate redshift
• The Number Density of Quiescent Compact Galaxies at Intermediate Redshift
• From the Top Down and Back Up Again: Star Cluster Structure from Hierarchical Star Formation
• On the spectro-photometric properties of the bulk of the radio-loud AGN population
• The age dependence of the size-stellar mass relation and some implications
• The number density of superdense early-type galaxies at 1<z<2 and the local cluster galaxies
• High Resolution Imaging of PHIBSS z~2 Main Sequence Galaxies in CO J=1-0
• How large are the globular cluster systems of early-type galaxies and do they scale with galaxy halo properties?
• Early-type galaxies in the PEARS survey: Probing the stellar populations at moderate redshift
• Dissipationless collapses in MOND
• Spectroscopic Confirmation of an Ultra Massive and Compact Galaxy at z=3.35: A Detailed Look at an Early Progenitor of Local Most Massive Ellipticals
• Introducing EMP-Pathfinder: modelling the simultaneous formation and evolution of stellar clusters in their host galaxies
• hCOSMOS: a dense spectroscopic survey of $r⩽21.3$ galaxies in the COSMOS field
• A spectroscopic sample of massive, evolved z~2 galaxies: Implications for the evolution of the mass-size relation
• Constraints on Quenching of $z\lesssim 2$ Massive Galaxies from the Evolution of the average Sizes of Star-Forming and Quenched Populations in COSMOS
• Blasts from the Past: Supernova Shock Breakouts among X-Ray Transients in the XMM-Newton Archive
• Early-type galaxies at z~1.3. IV. Scaling relations in different environments
• Local Analogs for High-redshift Galaxies: Resembling the Physical Conditions of the Interstellar Medium in High-redshift Galaxies
• Disk galaxies with broken luminosity profiles from cosmological simulations
• AGN Jet-induced Feedback in Galaxies. II. Galaxy colours from a multicloud simulation
• The stability of stellar disks in Milky-Way sized dark matter halos
• Cosmic Evolution of Stellar Disk Truncations: From z~1 to the Local Universe
• EGG: hatching a mock Universe from empirical prescriptions
• Gemini K-band NIRI Adaptive Optics Observations of Massive Galaxies at 1 < z < 2
• The Structural Evolution of Milky Way-like Star Forming Galaxies since z~1.3
• Morphologies of Two Massive Old Galaxies at z ~ 2.5
• A near-infrared morphological comparison of high-redshift submm and radio galaxies: massive star-forming discs vs relaxed spheroids
• Bivariate Galaxy Luminosity Functions in the Sloan Digital Sky Survey
• Formation of galaxies in ΛCDM cosmologies. I. The fine structure of disc galaxies
• The size-star formation relation of massive galaxies at 1.5<z<2.5
• The Red Sequence Luminosity Function in Massive Intermediate Redshift Galaxy Clusters
• Rotation rates, sizes, and star formation efficiencies of a representative population of simulated disc galaxies
• Expected number of massive galaxy relics in the present-day Universe
• On the formation of massive galaxies: A simultaneous study of number density, size and intrinsic colour evolution in GOODS
• Massive Galaxies are Larger in Dense Environments: Environmental Dependence of Mass-Size Relation of Early-Type Galaxies
• Numerical convergence of hydrodynamical simulations of galaxy formation: the abundance and internal structure of galaxies and their cold dark matter haloes
• What Determines the Sizes of Bars in Spiral Galaxies?
• The evolutionary sequence of sub-mm galaxies: from diffuse discs to massive compact ellipticals?
• Constraining the star formation and the assembly histories of normal and compact early-type galaxies at 1<z<2
• Formation and evolution of dwarf early-type galaxies in the Virgo cluster II. Kinematic Scaling Relations
• Nature of H-alpha selected galaxies at z>2. II. Clumpy galaxies and compact star-forming galaxies
• The structural and size evolution of star-forming galaxies over the last 11 Gyrs
• The hot circumgalactic medium in the eROSITA All-Sky Survey I. X-ray surface brightness profiles
• Rapid growth of seed black holes during early bulge formation
• Galapagos-2/Galfitm/GAMA -- multi-wavelength measurement of galaxy structure: separating the properties of spheroid and disk components in modern surveys
• The Lyman alpha reference sample: IV. Morphology at low and high redshift
• The effects of the cluster environment on the galaxy mass-size relation in MACSJ J1206.2-0847
• GASP XXXIII. The ability of spatially resolved data to distinguish among the different physical mechanisms affecting galaxies in low-density environments
• Structural properties of discs and bulges of early-type galaxies
• The Mass Dependence of Star Formation Histories in Barred Spiral Galaxies
• The SDSS-UKIDSS Fundamental Plane of Early-type Galaxies
• Early-type galaxy density profiles from IllustrisTNG: I. Galaxy correlations and the impact of baryons
• Sizes and ages of SDSS ellipticals: Comparison with hierarchical galaxy formation models
• Compact groups from the Millennium Simulations: I. Their Nature and the completeness of the Hickson sample
• Galaxy Sizes Since $z=2$ from the Perspective of Stellar Mass Distribution within Galaxies
• SPIDER - VI. The Central Dark Matter Content of Luminous Early-Type Galaxies: Benchmark Correlations with Mass, Structural Parameters and Environment
• The MUSE Hubble Ultra Deep Field Survey: XII. MgII emission and absorption in star-forming galaxies
• Red nuggets grow inside-out: evidence from gravitational lensing
• The Size Evolution of Passive Galaxies: Observations from the Wide Field Camera 3 Early Release Science Program
• Realistic mock observations of the sizes and stellar mass surface densities of massive galaxies in FIRE-2 zoom-in simulations
• Shallow Dark Matter Cusps in Galaxy Clusters
• Hubble Space Telescope Observations of Field Ultracool Dwarfs at High Galactic Latitude
• The VLA Survey of the Chandra Deep Field South. II. Identification and host galaxy properties of submillijansky sources
• The evolution of the size-mass relation at $z$=1-3 derived from the complete Hubble Frontier Fields data set
• The new semianalytic code GalICS 2.0 - Reproducing the galaxy stellar mass function and the Tully-Fisher relation simultaneously
• The Mass Scale of High-Redshift Galaxies: Virial Mass Estimates Calibrated with Stellar Dynamical Models from LEGA-C
• Age and metallicity gradients support hierarchical formation for M87
• X-shooter Spectroscopy and HST Imaging of 15 Ultra Massive Quiescent Galaxies at $z\gtrsim 2$
• Spatially Resolved Colors and Stellar Population Properties in Early-Type Galaxies at z ~ 1.5
• Formation of disk galaxies in preheated media: a preventative feedback model
• GOODS-ALMA 2.0: Starbursts in the main sequence reveal compact star formation regulating galaxy evolution prequenching
• WATCAT: a tale of wide-angle tailed radio galaxies
• Spatially Resolved Stellar Populations of $0.3<z<6.0$ Galaxies in WHL0137-08 and MACS0647+70 Clusters as Revealed by JWST: How do Galaxies Grow and Quench Over Cosmic Time?
• Morphology Dependence Of Stellar Age in Quenched Galaxies at Redshift ~ 1.2: Massive Compact Galaxies Are Older Than More Extended Ones
• Pan-STARRS1: Galaxy Clustering in the Small Area Survey 2
• Faint progenitors of luminous $z\sim 6$ quasars: why don't we see them?
• Predicting the Properties of the Remnants of Dissipative Galaxy Mergers
• Color gradients and half-mass radii of galaxies out to $z=2$ in the CANDELS/3D-HST fields: further evidence for important differences in the evolution of mass-weighted and light-weighted sizes
• KROSS-SAMI: A Direct IFS Comparison of the Tully-Fisher Relation Across 8 Gyr Since $z\approx 1$
• An X-ray Detected Group of Quiescent Early-type Galaxies at z=1.6 in the Chandra Deep Field South
• The Mass Profile and Shape of Bars in the Spitzer Survey of Stellar Structure in Galaxies (S4G): Search for an Age Indicator for Bars
• How the central black hole may shape its host galaxy through AGN feedback
• Galaxy sizes as a function of environment at intermediate redshift from the ESO Distant Cluster Survey
• A New View of the Size-Mass Distribution of Galaxies: Using $r_{20}$ and $r_{80}$ instead of $r_{50}$
• On the central stellar mass density and the inside-out growth of early-type galaxies
• A universal stellar-mass and size relation of galaxies in GOODS-N region
• Constraining Satellite Galaxy Stellar Mass Loss and Predicting Intrahalo Light I: Framework and Results at Low Redshift
• Hubble Space Telescope Imaging of Post-Starburst Quasars
• A bias in cosmic shear from galaxy selection: results from ray-tracing simulations
• The Large-Scale Environments of Type Ia Supernovae: Evidence for a Metallicity Bias in the Rate or Luminosity of Prompt Ia Events
• Time Evolution of Galaxy Scaling Relations in Cosmological Simulations
• Redshift evolution of the dynamical properties of massive galaxies from SDSS-III/BOSS
• The diverse formation histories of simulated disc galaxies
• Towards a radially-resolved semi-analytic model for the evolution of disc galaxies tuned with machine learning
• A Detection of the Environmental Dependence of the Sizes and Stellar Haloes of Massive Central Galaxies
• Structural and Dynamical Properties of Galaxies in a Hierarchical Universe: Sizes and Specific Angular Momenta
• The edges of galaxies: Tracing the limits of star formation
• One Plane for All: Massive Star-Forming and Quiescent Galaxies Lie on the Same Mass Fundamental Plane at z~0 and z~0.7
• Where are compact groups in the local Universe?
• The build-up of pseudobulges in a hierarchical universe
• A Compact Early-type Galaxy at z = 0.6 Under a Magnifying Lens: Evidence For Inside-out Growth
• INSPIRE: INvestigating Stellar Population In RElics -- I. Survey presentation and pilot program
• The Grism Lens-Amplified Survey from Space (GLASS). IX. The dual origin of low-mass cluster galaxies as revealed by new structural analyses
• Mass of the dynamically hot inner stellar halo predicts the ancient accreted stellar mass
• Galaxy density profiles and shapes -- I. simulation pipeline for lensing by realistic galaxy models
• Emission lines in early-type galaxies: active nuclei or stars?
• Satellite Accretion Onto Massive Galaxies With Central Black Holes
• The growth of galactic bulges through mergers in LCDM haloes revisited. I. Present-day properties
• Isolated elliptical galaxies in the local Universe
• The starburst-AGN connection: the role of young stellar populations in fueling supermassive black holes
• The Fornax Deep Survey with VST. X. The assembly history of the bright galaxies and intra-group light in the Fornax A subgroup
• The Star Formation Histories of Red-Sequence Galaxies, Mass-to-Light Ratios and the Fundamental Plane
• Are ultra-diffuse galaxies Milky Way-sized?
• 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
• The Role of Dissipation in the Scaling Relations of Cosmological Merger Remnants
• Galaxy Size and Mass Build-up in the First 2 Gyrs of Cosmic History from Multi-Wavelength JWST NIRCam Imaging
• Quiescent Galaxy Size and Spectroscopic Evolution: Combining HSC Imaging and Hectospec Spectroscopy
• Galaxy sizes and the galaxy-halo connection -- I: the remarkable tightness of the size distributions
• The Pan-STARRS1 Small Area Survey 2
• The Environmental Dependence of the Luminosity-Size Relation for Galaxies
• Star-forming galaxies as the origin of the IceCube PeV neutrinos
• The metallicity of galactic winds
• The Impact of Gas Stripping and Stellar Mass Loss on Satellite Galaxy Evolution
• Globular clusters as tracers of the dark matter halo: insights from the E-MOSAICS simulations
• Weak Lensing with Sizes, Magnitudes and Shapes
• JWST CEERS probes the role of stellar mass and morphology in obscuring galaxies
• The galaxy luminosity - size relation and selection biases in the Hubble Ultra Deep Field
• Supermassive Black Holes and Their Host Galaxies - I. Bulge luminosities from dedicated near-infrared data
• The rest-frame optical sizes of massive galaxies with suppressed star formation at $z\sim 4$
• Stellar Disks in Aquarius Dark Matter Haloes
• The effect of baryon cooling on the statistics of giant arcs and multiple quasars
• Post-Newtonian constraints on Lorentz-violating gravity theories with a MOND phenomenology
• A combined VANDELS and LEGA-C study: the evolution of quiescent galaxy size, stellar mass and age from $\text{z}=0.6$ to $\text{z}=1.3$
• On the cosmic evolution of the specific star formation rate
• The origin of bulges and discs in the CALIFA survey: I. Morphological evolution
• Globular Clusters Formed within Dark Halos I: present-day abundance, distribution and kinematics
• The Evolutionary Pathways of Disk-, Bulge-, and Halo-dominated Galaxies
• Inverse stellar population age gradients of post-starburst galaxies at z=0.8 with LEGA-C
• Radius Dependent Luminosity Evolution of Blue Galaxies in GOODS-N
• Structures in the fundamental plane of early-type galaxies
• A New Empirical Method to Infer the Starburst History of the Universe from Local Galaxy Properties
• Quasar Photometric Redshifts and Candidate Selection: A New Algorithm Based on Optical and Mid-Infrared Photometric Data
• Photometric properties and luminosity function of nearby massive early-type galaxies
• The redshift distribution of cosmological samples: a forward modeling approach
• Gravitational Potential and Surface Density Drive Stellar Populations -- II. Star-Forming Galaxies
• $R_{\mathrm{e}}$. I. Understanding galaxy sizes, associated luminosity densities, and the artificial division of the early-type galaxy population
• Evolution of the brightest cluster galaxies: the influence of morphology, stellar mass and environment
• The ALMA-CRISTAL survey: Widespread dust-obscured star formation in typical star-forming galaxies at z=4-6
• The angular momentum of disc galaxies: implications for gas accretion, outflows, and dynamical friction
• Combining Size and Shape in Weak Lensing
• The Origin of Exponential Star-forming Disks
• Small-scale galaxy clustering in the EAGLE simulation
• Disk Galaxy Scaling Relations in the SFI++: Intrinsic Scatter and Applications
• Massive Low Surface Brightness Galaxies in the EAGLE Simulation
• Calibrated, cosmological hydrodynamical simulations with variable IMFs I: Method and effect on global galaxy scaling relations
• The gas-phase metallicities of star-forming galaxies in aperture-matched SDSS samples follow potential rather than mass or average surface density
• Deep GMOS Spectroscopy of Extremely Red Galaxies in GOODS-South: Ellipticals, Mergers and Red Spirals at 1<z<2
• Further constraining galaxy evolution models through the Size Function of SDSS Early-type galaxies
• Imprints of recoiling massive black-holes on the hot gas of early type galaxies
• 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)
• The Size-Mass relation at Rest-Frame $1.5\mu$m from JWST/NIRCam in the COSMOS-WEB and PRIMER-COSMOS fields
• Galaxy and Mass Assembly (GAMA): Accurate number densities & environments of massive ultracompact galaxies at 0.02 < z < 0.3
• The Relationship Between Brightest Cluster Galaxy Star Formation and the Intracluster Medium in CLASH
• The abundance of compact quiescent galaxies since z ~ 0.6
• Resolving the baryon-fraction profile in lensing galaxies
• Measurement of the B-band Galaxy Luminosity Function with Approximate Bayesian Computation
• Balmer Break Galaxy Candidates at $z\sim 6$: a Potential View on the Star-Formation Activity at $z\gtrsim 14$
• GAMA+KiDS: Empirical correlations between halo mass and other galaxy properties near the knee of the stellar-to-halo mass relation
• VIS3COS: II. Nature and nurture in galaxy structure and morphology
• Stellar populations of galaxies in the ALHAMBRA survey up to $z\sim 1$. IV. Properties of quiescent galaxies on the stellar mass$-$size plane
• The size evolution of galaxy discs formed within Lambda Cold Dark Matter haloes
• Compact, bulge dominated structures of spectroscopically confirmed quiescent galaxies at z~3
• From HI to Stars: HI Depletion in Starbursts and Star-Forming Galaxies in the ALFALFA H-alpha Survey
• The new class of FR0 radio galaxies
• Star formation and quenching among the most massive galaxies at z~1.7
• Brightest group galaxies and the large-scale environment
• Rotation Curves of Galaxies and Their Dependence on Morphology and Stellar Mass
• Adaptive Optics Rest-Frame V-band Imaging of Lyman Break Galaxies at z~3: High-surface Density Disk-like Galaxies ?
• VIMOS Public Extragalactic Redshift Survey (VIPERS). The distinct build-up of dense and normal massive passive galaxies
• The Intrinsic Scatter of Galaxy Scaling Relations
• Galaxy And Mass Assembly (GAMA): Bulge-disk decomposition of KiDS data in the nearby universe
• The Compact UV Size of Green Pea Galaxies As Local Analogs of High-redshift Ly$\alpha$-Emitters
• The galaxy size - halo mass scaling relations and clustering properties of central and satellite galaxies
• How Robust Are the Size Measurements of High-redshift Compact Galaxies?
• The structural properties of classical bulges and discs from z~2
• Size distribution of galaxies in SDSS DR7: weak dependence on halo environment
• Leveraging 3D-HST Grism Redshifts to Quantify Photometric Redshift Performance
• A Fundamental Line for Elliptical Galaxies
• Rapid build-up of the stellar content in the protocluster core SPT2349$-$56 at $z=4.3$
• Massive quiescent galaxies at $z\sim 3$: a comparison of selection, stellar population and structural properties with simulation predictions
• SPIDER - V. Measuring Systematic Effects in Early-Type Galaxy Stellar Masses from Photometric SED Fitting
• Kinematic analysis of EAGLE simulations: Evolution of ${\lambda }_{Re}$ and its connection with mergers and gas accretion
• The galaxy size to halo spin relation of disk galaxies in cosmological hydrodynamical simulations
• The imprint of dark matter haloes on the size and velocity dispersion evolution of early-type galaxies
• The Evolution of Galaxies at Constant Number Density: A Less Biased View of Star Formation, Quenching, and Structural Formation
• CEERS: Spatially Resolved UV and mid-IR Star Formation in Galaxies at 0.2 < z < 2.5: The Picture from the Hubble and James Webb Space Telescopes
• Morphological evolution in situ: Disk-dominated cluster red sequences at z ~ 1.25
• Revisiting the Size-Luminosity Relation in the Era of Ultra Diffuse Galaxies
• The Compact Structures of Massive $z\sim 0.7$ Post-Starburst Galaxies in the SQuIGG$\vec{L}$E Sample
• Polar-ring galaxies: the SDSS view on the symbiotic galaxies
• Dark-ages reionization and galaxy formation simulation--VII. The sizes of high-redshift galaxies
• GAlaxy Light profile convolutional neural NETworks (GaLNets). I. fast and accurate structural parameters for billion galaxy samples
• The population of early-type galaxies: how it evolves with time and how it differs from passive and late-type galaxies
• The SAMI galaxy survey: galaxy size can explain the offset between star-forming and passive galaxies in the mass-metallicity relationship
• Intrinsic Shape of Star-Forming BzK Galaxies II: Rest-Frame UV and Optical Structures in GOODS-South and SXDS
• Color-magnitude relations of late-type galaxies
• Colour gradients in normal and compact early-type galaxies at 1<z<2
• Scaling relations of cluster elliptical galaxies at z~1.3. Distinguishing luminosity and structural evolution
• The size-luminosity relation of lensed galaxies at $z=6-9$ in the Hubble Frontier Fields
• The dark side of galaxy stellar populations I: The stellar-to-halo mass relation and the velocity dispersion - halo mass relation
• The dichotomy of dark matter fraction and total mass density slope of galaxies over five dex in mass
• Moderate Steepening of Galaxy Cluster Dark Matter Profiles by Baryonic Pinching
• Strong spiral arms drive secular growth of pseudo bulges in disk galaxies
• Angular size test on the expansion of the Universe
• Ultramassive dense early-type galaxies: velocity dispersions and number density evolution since z=1.6
• Stellar Velocity Dispersion for a Strongly-Lensed, Intermediate-Mass Quiescent Galaxy at z=2.8
• Partial stellar tidal disruption events and their rates
• The morphological mix of dwarf galaxies in the nearby Universe
• The Evolutionary Sequence of Post-Starburst Galaxies
• What boost galaxy mergers in two massive galaxy protoclusters at z = 2.24
• Morphological evolution and galactic sizes in the L-Galaxies SA model
• What is Important? Morphological Asymmetries are Useful Predictors of Star Formation Rates of Star-forming Galaxies in SDSS Stripe 82
• The PAU Survey: Measurement of Narrow-band galaxy properties with Approximate Bayesian Computation
• Pitfalls when observationally characterizing the relative formation rates of stars and stellar clusters in galaxies
• Mass distribution and orbital anisotropy of early-type galaxies: constraints from the Mass Plane
• Massive relic galaxies prefer dense environments
• Generating Synthetic Cosmological Data with GalSampler
• Understanding the Unique Assembly History of Central Group Galaxies
• Galaxy collisions as a mechanism of ultra diffuse galaxy (UDG) formation
• The PAndAS View of the Andromeda Satellite System. IV Global properties
• Inferring galaxy dark halo properties from visible matter with Machine Learning
• Intrinsic Shape of Star-Forming BzK Galaxies at z~2 in GOODS-N
• The metal enrichment of passive galaxies in cosmological simulations of galaxy formation
• ZFIRE: Similar Stellar Growth in H$\alpha$-emitting Cluster and Field Galaxies at z~2
• Scaling relations for globular cluster systems in early-type galaxies
• The scaling relation between baryonic mass and stellar disc size of morphologically late-type galaxies
• Size magnification as a complement to Cosmic Shear
• The spectral energy distribution of the hyperluminous, hot dust-obscured galaxy W2246$-$0526
• The Formation History of Subhalos and the Evolution of Satellite Galaxies
• The inner structure of very massive elliptical galaxies: implications for the inside-out formation mechanism of z~2 galaxies
• Simulating JWST/NIRCam Color Selection of High-Redshift Galaxies
• Star Formation History in Barred Spiral Galaxies. AGN Feedback
• The rapid transition from star-formation to AGN dominated rest-frame UV light at z ~ 4
• Ellipticals at $z=0$ from Self-Consistent Hydrodynamical Simulations: Comparison with SDSS Structural and Kinematical Data
• SH$\alpha$DE: Survey description and mass-kinematics scaling relations for dwarf galaxies
• Two phase galaxy formation: The Gas Content of Normal Galaxies
• Sersic Properties of Disc Galaxy Mergers
• Modelling the accretion and feedback of supermassive black hole binaries in gas-rich galaxy mergers
• Reconstructing the Assembly of Massive Galaxies. II. Galaxies Develop Massive and Dense Stellar Cores as They Evolve and Head Toward Quiescence at Cosmic Noon
• Loss of star forming gas in SDSS galaxies
• SEAGLE--II: Constraints on feedback models in galaxy formation from massive early type strong lens galaxies
• Exploring Proxies for the Supermassive Black Hole Mass Function: Implications for Pulsar Timing Arrays
• H-ATLAS/GAMA: Quantifying the Morphological Evolution of the Galaxy Population Using Cosmic Calorimetry
• Introducing the AIDA-TNG project: galaxy formation in alternative dark matter models
• Compact molecular gas emission in local LIRGs among low- and high-z galaxies
• Importance of Mock Observations in Validating Galaxy Properties for Cosmological Simulations
• On the HI Content of MaNGA Major Merger Pairs
• SQuIGG$\vec{L}$E Survey: Massive z$\sim$0.6 Post-Starburst Galaxies Exhibit Flat Age Gradients
• The Link Between Morphology and Structure of Brightest Cluster Galaxies: Automatic Identification of cDs
• The Evolution of Sizes and Specific Angular Momenta in Hierarchical Models of Galaxy Formation and Evolution
• Calibrating cosmological simulations with implicit likelihood inference using galaxy growth observables
• Taking the Milky Way for a spin: disc formation in the ARTEMIS simulations
• Exploring Relations Between BCG \& Cluster Properties in the SPectroscopic IDentification of eROSITA Sources Survey from $0.05<z<0.3$
• MaNGA galaxy properties -- I. An extensive optical, mid-infrared photometric, and environmental catalogue
• SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES) IV: Spatial clustering and halo masses of 450-$\mu$m-selected sub-millimeter galaxies
• Physical properties of galaxies: toward a consistent comparison between hydrodynamical simulations and SDSS
• Mergers of supermassive and intermediate-mass black holes in galactic nuclei from disruptions of star clusters
• Constraining the Noise-Free Distribution of Halo Spin Parameters
• Stellar mass as the "glocal" driver of galaxies' stellar population properties
• Compact E+A Galaxies as a Progenitor of Massive Compact Quiescent Galaxies at 0.2<z< 0.8
• Mock galaxy redshift catalogues from simulations: implications for Pan-STARRS1
• SDSS-IV MaNGA: galaxy gas-phase metallicity gradients vary across the mass-size plane
• Clustering Constraints on the Relative Sizes of Central and Satellite Galaxies
• Dark Matter and IMF normalization in Virgo dwarf early-type galaxies
• High Redshift Massive Quiescent Galaxies are as Flat as Star Forming Galaxies: The Flattening of Galaxies and the Correlation with Structural Properties in CANDELS/3D-HST
• The evolution of late-type galaxies from CASSOWARY lensing systems
• Galaxy size trends as a consequence of cosmology
• Evolution of the Fundamental Plane of 0.2<z<1.2 Early-type galaxies in the EGS
• High-redshift quasar host galaxies with adaptive optics
• Massive black holes in stellar systems: 'quiescent' accretion and luminosity
• The low-metallicity QSO HE 2158-0107: A massive galaxy growing by the accretion of nearly pristine gas from its environment?
• Mass and size growth of early-type galaxies by dry mergers in cluster environments
• The evolution of disc galaxies with and without classical bulges since z~1
• Frequent Spin Reorientation of Galaxies due to Local Interactions
• A unified scenario for the origin of spiral and elliptical galaxy structural scaling laws
• The signature of dissipation in the mass-size relation: are bulges simply spheroids wrapped in a disc?
• Similarities and uniqueness of Ly$\alpha$ emitters among star-forming galaxies at z=2.5
• The discrepancy between dynamical and stellar masses in massive compact galaxies traces non-homology
• The SAMI Galaxy Survey: The role of disc fading and progenitor bias in kinematic transitions
• DAWN JWST Archive: Morphology from profile fitting of over 340 000 galaxies in major fields
• The host galaxies of luminous type 2 AGN at $z\sim$0.3-0.4
• The structure of massive quiescent galaxies at z~3 in the CANDELS-COSMOS field
• Measuring Dark Matter in Galaxies: The Mass Fraction Within 5 Effective Radii
• Cosmological Simulations of Massive Compact High-z Galaxies
• Constraining the epoch of reionization from the observed properties of the high-z Universe
• Setting firmer constraints on the evolution of the most massive, central galaxies from their local abundances and ages
• The Prevalence of Type III Disc Breaks in HI-rich and Low-spin Galaxies
• The half mass radius of MaNGA galaxies: Effect of IMF gradients
• MaNGA galaxy properties -- II. A detailed comparison of observed and simulated spiral galaxy scaling relations
• The ALHAMBRA survey: tight dependence of the optical mass-to-light ratio on galaxy colour up to z = 1.5
• Colour gradients of low-redshift galaxies in the DESI Legacy Imaging Survey
• Galaxy evolution by color-log(n) type since redshift unity in the Hubble Ultra Deep Field
• The Nature of Low Surface Brightness Galaxies in the Hyper Suprime-Cam Survey
• The Dearth of Difference between Central and Satellite Galaxies III. Environmental Dependence of Mass-Size and Mass-Structure Relations
• VLT/X-Shooter Near-Infrared Spectroscopy and HST Imaging of Gravitationally-Lensed z~2 Compact Quiescent Galaxies
• COMP2CAT: hunting compact double radio sources in the local Universe
• Dependence of the Fundamental Plane of Early-type Galaxies on Age and Internal Structure
• The specific angular momenta of superthin galaxies: Cue to their origin?
• Star Formation in Simulated Galaxies: Understanding the Transition to Quiescence at $3\times 10^{10}$ M${}_{\odot }$
• Synergies between low- and intermediate-redshift galaxy populations revealed with unsupervised machine learning
• The role of major mergers in the size growth of intermediate-mass spheroids
• The evolutionary pathways of disk galaxies with different sizes
• Energy transfer from baryons to dark matter as a unified solution to small-scale structure issues of the $\Lambda$CDM model
• The role of quenching time in the evolution of the mass-size relation of passive galaxies from the WISP survey
• HerMES : SPIRE detection of high redshift massive compact galaxies in GOODS-N field
• Central velocity dispersion catalog of LAMOST-DR7 galaxies
• The mass-dependent star formation histories of disk galaxies: infall model versus observations
• New insights into the structure of early-type galaxies: the Photometric Plane at z~0.3
• Bulge formation through disc instability -- I
• The impact of environment on size: Galaxies are 50% smaller in the Fornax Cluster compared to the field
• The Physical Origin of the Mass-Size Relation and Its Scatter of Disk Galaxies
• Compact star-forming galaxies preferentially quenched to become PSBs in $z<1$ clusters
• Hot versus Cold: the Dichotomy in Spherical Accretion of Cooling Flows onto Supermassive Black Holes in Elliptical Galaxies, Galaxy Groups and Clusters
• K-CLASH: spatially-resolving star-forming galaxies in field and cluster environments at $z\approx 0.2$-$0.6$
• On the limits of measuring the bulge and disk properties of local and high-redshift massive galaxies
• Compact Quiescent Galaxies at Intermediate Redshifts
• Compact galaxies and the size-mass galaxy distribution from a colour-selected sample at 0.04 < z < 0.15 supplemented by ugrizYJHK photometric redshifts
• JADES: Rest-frame UV-to-NIR Size Evolution of Massive Quiescent Galaxies from Redshift z=5 to z=0.5
• The Properties of Massive Star-forming galaxies with Outside-in Assembly Mode
• Analysis of the galaxy size versus stellar mass relation
• The local environmental dependence of galaxy properties in the volume-limited sample of Main Galaxies from the SDSS Data Release 5
• Galaxy Properties in Clusters: Dependence on the Environment and the Cluster Identification Techniques
• HST F160W Imaging of Very Massive Galaxies at $1.5<z<3.0$: Diversity of Structures and the Effect of Close Pairs on Number Density Estimates
• Color gradients reflect an inside-out growth in early-type galaxies of the cluster MACS J1206.2-0847
• Magnitude and size evolution of bulgeless galaxies
• Stellar Metallicity Gradients in SDSS galaxies
• The Mass-Radius Relation for Star-Forming Galaxies at z ~ 1.5-3.0
• The THESAN-ZOOM project: central starbursts and inside-out quenching govern galaxy sizes in the early Universe
• The OTELO survey as a morphological probe. Last ten Gyr of galaxy evolution. The mass--size relation up to z=2
• The Size-Mass Relation of Post-Starburst Galaxies in the Local Universe
• PHANGS-ALMA: Arcsecond CO(2-1) Imaging of Nearby Star-Forming Galaxies
• Serendipitous discovery of a massive cD galaxy at z=1.096: Implications for the early formation and late evolution of cD galaxies
• When Should We Treat Galaxies as Isolated?
• Dust accretion and destruction in galaxy groups and clusters
• The Coevolution of Massive Quiescent Galaxies and Their Dark Matter Halos over the Last 6 Billion Years
• The Effect of Halo Mass on the HI Content of Galaxies in Groups and Clusters
• A physical model for the origin of the diffuse cosmic infrared background
• A possible signature of the influence of tidal perturbations in dwarf galaxy scaling relations
• Compact groups from semi-analytical models of galaxy formation -- I: a comparative study of frequency and nature
• A Nearby Analog of z~2 Compact Quiescent Galaxies with a Rotating Disk
• Simulation-based inference of deep fields: galaxy population model and redshift distributions
• The fall of CSS100217: a tidal disruption-induced low state in an apparently hostless active galactic nucleus
• Angular momentum evolution of stellar disks at high redshifts
• Pseudo-Evolution of Galaxies in LCDM Cosmology
• The mass dependence of structure, star formation rate, and mass assembly mode at 0.5<z< 2.5
• The SFR-radius connection: data and implications for wind strength and halo concentration
• Correlation of structure and stellar properties of galaxies in Stripe 82
• The Puzzling Origin of Massive Compact Galaxies in MaNGA
• Drivers of asymmetry in synthetic H I emission-line profiles of galaxies in the EAGLE simulation
• Scaling relations of z~0.25-1.5 galaxies in various environments from the morpho-kinematic analysis of the MAGIC sample
• The size--mass and other structural parameter ($n,{\mu }_z,R_z$) relations for local bulges/spheroids from multicomponent decompositions
• Accurate Computation of the Screening of Scalar Fifth Forces in Galaxies
• Demographics of Tidal Disruption Events with L-Galaxies: I. Volumetric TDE rates and the abundance of Nuclear Star Clusters
• The supermassive black hole merger driven evolution of high-redshift red nuggets into present-day cored early-type galaxies
• MOIRCS Deep Survey. VII: NIR Morphologies of Star-forming Galaxies at Redshift z~1
• Denser Environments Cultivate Larger Galaxies: A Comprehensive Study beyond the Local Universe with 3 Million Hyper Suprime-Cam Galaxies
• Empirical Evidence of Non-Minimally Coupled Dark Matter in the Dynamics of Local Spiral Galaxies?
• A new gas cooling model for semi-analytical galaxy formation models
• Black hole mass measurement using molecular gas kinematics: what ALMA can do
• Simulating Deep Hubble Images With Semi-empirical Models of Galaxy Formation
• Surface photometry and structure of high redshift disk galaxies in the HDF-S NICMOS field
• Tilted outer and inner structures in edge-on galaxies?
• Tracing the co-evolution path of super massive black holes and spheroids with AKARI-selected ultra-luminous IR galaxies at intermediate redshifts
• Structures, stellar population properties, AGN fractions, and environments of massive compact galaxies at $1<z<2$ in 3D--{\it HST}/CANDELS
• Dynamical masses and non-homology of massive elliptical galaxies grown by dry mergers
• Fractal analysis of the large-scale stellar mass distribution in the Sloan Digital Sky Survey
• Post-starburst galaxies in SDSS-IV MaNGA: Two broad categories of evolutionary pathways
• Efficient exploration and calibration of a semi-analytical model of galaxy formation with deep learning
• Structural analysis of massive galaxies using HST deep imaging at z < 0.5
• Bayesian fitting of multi-Gaussian expansion models to galaxy images
• The Size Evolution of Elliptical Galaxies
• CSST Large-scale Structure Analysis Pipeline: II. the CSST Emulator for Slitless Spectroscopy (CESS)
• Massive Red Spiral Galaxies in SDSS-IV MaNGA Survey
• Chemical enrichment in isolated barred spiral galaxies
• Galaxy populations in groups and clusters: evidence for a characteristic stellar mass scale at $M_{\ast }\sim 10^{9.5}{M}_{\odot }$
• The color gradients of spiral disks in the Sloan Digital Sky Survey
• Size and Spectroscopic Evolution of HectoMAP Quiescent Galaxies
• Devouring the Milky Way Satellites: Modeling Dwarf Galaxies with Galacticus
• The connection between stellar mass, age and quenching timescale in massive quiescent galaxies at $z\simeq 1$
• 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
• The Size Function of Galaxy Disks out to z ~ 1 from the Canada-France-Hawaii-Telescope Legacy Survey
• FIGS: Spectral fitting constraints on the star formation history of massive galaxies since Cosmic Noon
• Stellar Mass Profiles of Quiescent Galaxies in Different Environments at $z\sim 0$
• The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship
• Leaving the dark ages with AMIGA
• Revisiting the census of low-luminosity AGN
• How to empirically model star formation in dark matter halos: I. Inferences about central galaxies from numerical simulations
• Pix2Prof: fast extraction of sequential information from galaxy imagery via a deep natural language 'captioning' model
• The power spectrum of systematics in cosmic shear tomography and the bias on cosmological parameters
• The merger history of massive spheroids since z~1 is size independent
• Field spheroid-dominated galaxies in a Λ-CDM Universe
• Galaxy mass-size segregation in the cosmic web from the CAVITY parent sample
• RABBITS -- II. The impact of AGN feedback on coalescing supermassive black holes in disc and elliptical galaxy mergers
• Dissecting the morphological and spectroscopic properties of galaxies in the local Universe: I. Elliptical galaxies
• Discovery of a Very Large (~20 kpc) Galaxy at z=3.72
• The most massive galaxies in clusters are already fully grown at $z\sim 0.5$
• The structural properties of nearby dwarf galaxies in low density environments -- size, surface brightness and colour gradients
• GABE: Galaxy Assembly with Binary Evolution
• Gaia transient detection efficiency: hunting for nuclear transients
• Beyond the galaxy luminosity function
• Ageing and Quenching through the ageing diagram II: physical characterization of galaxies
• Large Size Scatter of Passively Evolving Lensed Galaxies at z~2 in CLASH
• Probing galaxy evolution from $z=0$ to $z\simeq 10$ through galaxy scaling relations in three L-Galaxies flavours
• DHOST gravity in Ultra-diffuse galaxies -- Part II: NGC 1052-DF4 and Dragonfly 44
• Dark against luminous matter around isolated central galaxies: a comparative study between modern surveys and Illustris-TNG
• SEAGLE--III: Towards resolving the mismatch in the dark-matter fraction in early-type galaxies between simulations and observations
• Stellar Metallicity of Galaxies: New Insight on the Formation and Evolution of Low Surface Brightness Galaxies in the IllustrisTNG Simulation
• Growth of disc-like pseudo-bulges in SDSS DR7 since z = 0.1
• Galaxy And Mass Assembly (GAMA): Stellar-to-Dynamical Mass Relation I. Constraining the Precision of Stellar Mass Estimates
• The ASTRID Simulation at z=0: From Massive Black Holes to Large-scale Structure
• Is there substructure around M87?
• Follow-up survey for the binary black hole merger GW200224_222234 using Subaru/HSC and GTC/OSIRIS
• Smaller stellar disc scale lengths in rich environments
• Early-type galaxies at intermediate redshift observed with HST WFC3: perspectives on recent star-formation
• What drives the corpulence of galaxies? I. The formation of central compact dwarf galaxies in TNG50
• On The Fine Tuning and Physical Origin of Line-Locked Absorption Systems in Active Galaxies
• Physical and Morphological Properties of [O II] Emitting Galaxies in the HETDEX Pilot Survey
• Are compact groups hostile towards faint galaxies?
• The morphological dependent Tully-Fisher relation of spiral galaxies
• The stellar mass function and efficiency of galaxy formation with a varying initial mass function
• Radial Distribution of Near-UV Flux in Disc Galaxies in the range 0<z<1
• The changing ISM of massive elliptical galaxies and cosmic evolution of radio galaxies and quasars
• J-PLUS: the impact of bars on quenching time-scales in nearby green valley disc galaxies
• MUSE-ALMA Haloes IX: Morphologies and Stellar Properties of Gas-rich Galaxies
• Galaxy-halo size relation from Sloan Digital Sky Survey Data Release 7 and the ELUCID simulation
• Photometry and kinematics of dwarf galaxies from the Apertif HI survey
• PRIMER: JWST/MIRI reveals the evolution of star-forming structures in galaxies at z<2.5
• Interpreting the relation between the gamma-ray and infrared luminosities of star-forming galaxies
• Where Did the Outskirts Go? Outer Stellar Haloes as a Sensitive Probe of Supernova Feedback
• Constraints on the evolutionary mechanisms of massive galaxies since $z\sim 1$ from their velocity dispersions
• Dust Heating by Low-mass Stars in Massive Galaxies at z<1
• The mass-size relation of LRGs from BOSS and DECaLS
• Tully-Fisher Relation of Late-type Galaxies at $0.6\le z\le 2.5$
• Deep spectroscopy of nearby galaxy clusters: IV The quench of the star formation in galaxies in the infall region of Abell\ 85
• The evolution of galaxy sizes
• Angular momentum transfer and the size - mass relation in early - type galaxies
• A comprehensive study on the relation between the metal enrichment of ionised and atomic gas in star-forming galaxies
• On the Structure of the AGN Torus through the Fraction of Optically-Selected Type 1 AGNs
• MOIRCS Deep Survey V: A Universal Relation for Stellar Mass and Surface Brightness of Galaxies
• The evolution and dependence of the local mass-metallicity relation
• The Differential Assembly History of the Centers and Outskirts of Main Sequence Galaxies at $z\sim 2.3$
• SED-inferred properties and morphology of Lyman-break galaxies at $z\sim 1$ in the CDF-S
• A search for intermediate-mass black holes in compact stellar systems through optical emissions from tidal disruption events
• The detections of inflowing gas from narrow absorption lines at the parsec scale
• Luminosity Distribution of Dwarf Elliptical-like Galaxies
• The Spatial Distributions of Red and Blue Globular Clusters in Major Dry Merger Remnants
• Extinction and AGN over host galaxy contrast effects on the optical spectroscopic classification of AGN
• Extremely Low Molecular Gas Content in the Vicinity of a Red Nugget Galaxy at $z=1.91$
• Total and dark mass from observations of galaxy centers with Machine Learning
• WISDOM Project -- XIX. Figures of merit for supermassive black hole mass measurements using molecular gas and/or megamaser kinematics
• Evolution of massive quiescent galaxies via envelope accretion
• Measuring Structural Parameters Through Stacking Galaxy Images
• Exploring the evolution of star formation and dwarf galaxy properties with JWST/MIRI serendipitous spectroscopic surveys
• Local galaxies with compact cores as the possible descendants of massive compact quiescent galaxies at high redshift
• Connecting Star Formation Quenching with Galaxy Structure and Supermassive Black Holes through Gravitational Heating of Cooling Flows
• The morphologies and masses of extremely red galaxies in the Groth Strip survey
• Morphology and structure of BzK-selected galaxies at z~2 in the CANDELS-COSMOS field
• A Maximum Parsimony analysis of the effect of the environment on the evolution of galaxies
• Unveiling the formation route of the largest galaxies in the universe
• Beyond the stars: Linking H$\alpha$ sizes, kinematics, and star formation in galaxies at $z\approx 4-6$ with JWST grism surveys and $\text{geko}$
• Intrinsic correlations of galaxy sizes in a hydrodynamical cosmological simulation
• The Chocolate Chip Cookie Model: dust-to-metal ratio of HII regions
• Simulations of the accreted stellar halos of low-mass field galaxies
• Self-Similar Buildup and Inside-Out Growth: Tracing the Evolution of Intermediate to High-Mass Star-Forming Galaxies Since $z=2$
• A Morphology Catalog of Galaxies in CEERS: Evolution in the Size and Color Gradients of Galaxies Since Cosmic Dawn
• Mock Observations: Three Different Types of Galaxy Alignment in TNG100 Simulations
• Barions and $\Lambda$CDM Model Problems
• The JWST Emission Line Survey (JELS): The sizes and merger fraction of star-forming galaxies during the Epoch of Reionization
• Effects of Environment on the Size Evolution of Quiescent Galaxies: Comparing Galaxies in Clusters and in the Field at Two Rest-frame Wavelengths
• Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies
• Beyond diagnostic-diagrams: A critical exploration on the classification of ionization processes
• Cosmological parameters from lenses distance ratio
• Constraints on dynamically-formed massive black holes in Little Red Dots from X-ray non-detections
• The fragility of thin discs in galaxies -- II. Thin discs as tracers of the assembly history of galaxies
• The Type Ia Supernova and Asymptotic Giant Branch Stellar Ejecta-regulated Interstellar Medium of Massive Galaxies
• The stellar mass - physical effective radius relation for dwarf galaxies in low-density environments
• Euclid preparation. LXVII. Deep learning true galaxy morphologies for weak lensing shear bias calibration
• Photo-z optimization for measurements of the BAO radial direction
• Compact dust-obscured star-formation and the origin of the galaxy bimodality
• LEGA-C stellar populations scaling relations. I: Chemo-archaeological downsizing trends at z~0.7
• Cosmic quenching and scaling laws for the evolution of supermassive black holes and host galaxies
• Impact of galactic and intergalactic dust on the stellar EBL
• Environmental Quenching of Low Surface Brightness Galaxies near Milky Way mass Hosts
• Late growth of early-type galaxies in low-z massive clusters
• The size and mass evolution of the massive galaxies over cosmic time
• A High-resolution Far-infrared Survey to Probe Black Hole-Galaxy Co-evolution
• DELVE Milky Way Satellite Galaxy Census I: Satellite Population and Survey Selection Function in DES, DELVE, and Pan-STARRS
• 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
• Scaling Relations in Dissipationless Spiral-like Galaxy Mergers
• Do Galaxies Change in Size ? An Angular Size Test at Low Redshift with SDSS Data
• Past, present and Future of the Scaling Relations of Galaxies and Active Galactic Nuclei
• Correcting the fiber-aperture bias affecting galaxy stellar populations in the Sloan Digital Sky Survey. Aperture corrections to absorption indices based on CALIFA integral field observations
• Environmental Invariance of the Galaxy Size-Mass Relation
• The Formation of Dwarf Galaxy Disks
• X-ray properties of massive compact relic galaxies
• Can we constrain galaxy geometry parameters using spatially integrated SED fitting?
• SDSS-IV MaNGA: Stellar rotational support in disk galaxies vs. central surface density and stellar population age
• Morphology and structure of extremely red objects at $z\sim 1$ in the CANDELS-COSMOS field
• Deciphering galaxy images using machine vision -- Combining variational autoencoder and principal component analysis for feature extraction
• Panchromatic properties of galaxies in wide-field optical spectroscopic and photometric surveys
• Faint galaxies in the Zone of Avoidance revealed by JWST/NIRCam
• Disc instability and bar formation: view from the IllustrisTNG simulations
• On the Size Evolution of a Galactic Disk in Hierarchical Merging of Cold Dark Matter Halos
• Recent star formation in 0.5<z<1.5 quiescent galaxies
• Two-phase formation of galaxies: the coevolution between galaxies and dark matter halos
• The catalogue of virtual early-type galaxies from IllustrisTNG: validation and real observation consistency
• Extended Hernquist-Springel formalism for cosmic star formation
• The Evolution of the Hubble Sequence: morpho-kinematics of distant galaxies
• The LEGA-C galaxy survey: multiple quenching channels for quiescent galaxies at $z\sim 1$
• Structural evolution of quiescent galaxies at intermediate redshifts at UV and red rest-frame wavelengths
• The role of dark matter in the galaxy mass-size relationship
• The Kormendy relation of cluster galaxies in PPS regions
• Bar Evolution in Edge-on Galaxies: A Demographic Study of Boxy/Peanut Bulges
• xGASS: characterizing the slope and scatter of the stellar mass - angular momentum relation for nearby galaxies
• SQuIGGLE: Studying Quenching in Intermediate-z Galaxies -- Gas, AnguLar Momentum, and Evolution
• Disk Sizes in a LCDM Universe
• GalSBI-SPS: a stellar population synthesis-based galaxy population model for cosmology and galaxy evolution applications
• Quiescent Galaxy Size, Velocity Dispersion, and Dynamical Mass Evolution
• Galaxy Morphological Classification with Efficient Vision Transformer
• From the Densest Clusters to the Emptiest Voids: No Evidence For Environmental Effects on the Galaxy Size-Mass Relation at Low Redshift
• The role of HI in regulating size growth of local galaxies
• Velocity Dispersions and Stellar Populations of the Most Compact and Massive Early-Type Galaxies at Redshift ~1
• Size-Mass Relation Shows Its Colours: Contrasting Physical Imprints of Galaxy Evolution in Rest-Frame UV and Optical
• The multiwavelength structure of post-starburst galaxies at 0.5 < z < 3 with JWST PRIMER: compact morphologies and residual disturbances
• The 5 Gyr evolution of sub-M* galaxies
• Numerical approaches to star formation and SuperNovae energy feedback in simulations of galaxy clusters
• Testing the key role of the stellar mass-halo mass relation in galaxy merger rates and morphologies via DECODE, a novel Discrete statistical sEmi-empiriCal mODEl
• HI Gas and Star Formation in Major Galaxy Pairs from the FAST All-Sky HI Survey (FASHI)
• Everything Every Band All at Once I: A Global Morphology Catalog in Abell 2744 based on UNCOVER/MegaScience
• Spatially resolved stellar-to-total dynamical mass relation: Radial variations, gradients and profiles of galaxy stellar populations
• 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
• Prospects for measuring the Doppler magnification dipole with LSST and DESI
• Hierarchal formation and growth of galaxies through dynamical friction
• Fuzzy dark matter dynamical friction: stalling of globular clusters induced by dynamical heatings
• SF-R You Sure? The Conflicting Role of Star Formation Rates in Constraining the Evolution of Milky Way Analogues in Cosmological Simulations
• Observed structural parameters of EAGLE galaxies: reconciling the mass-size relation in simulations with local observations
• GalSBI: Phenomenological galaxy population model for cosmology using simulation-based inference