NYU-VAGC: a galaxy catalog based on new public surveys

Abstract

Here we present the New York University Value-Added Galaxy Catalog (NYU-VAGC), a catalog of local galaxies (mostly below a redshift of about 0.3) based on a set of publicly-released surveys (including the 2dFGRS, 2MASS, PSCz, FIRST, and RC3) matched to the Sloan Digital Sky Survey (SDSS) Data Release 2. Excluding areas masked by bright stars, the photometric sample covers 3514 square degrees and the spectroscopic sample covers 2627 square degrees (with about 85% completeness). Earlier, proprietary versions of this catalog have formed the basis of many SDSS investigations of the power spectrum, correlation function, and luminosity function of galaxies. We calculate and compile derived quantities (for example, K-corrections and structural parameters for galaxies). The SDSS catalog presented here is photometrically recalibrated, reducing systematic calibration errors across the sky from about 2% to about 1%. We include an explicit description of the geometry of the catalog, including all imaging and targeting information as a function of sky position. Finally, we have performed eyeball quality checks on a large number of objects in the catalog in order to flag deblending and other errors. This catalog is complementary to the SDSS Archive Servers, in that NYU-VAGC's calibration, geometrical description, and conveniently small size are specifically designed for studying galaxy properties and large-scale structure statistics using the SDSS spectroscopic catalog.

arXiv commentaccepted by AJ; full resolution version available at http://sdss.physics.nyu.edu/vagc/va_paper.ps; data files available at http://sdss.physics.nyu.edu/vagc/

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• The Spatial Clustering of ROSAT All-Sky Survey AGN: I. The cross-correlation function with SDSS Luminous Red Galaxies
• SDSS-IV MaNGA: Inside-out vs. outside-in quenching in different local environments
• A Correction to the Standard Galactic Reddening Map: Passive Galaxies as Standard Crayons
• IMF radial gradients in most massive early-type galaxies
• The clustering of luminous red galaxies at z $\sim$ 0.7 from eBOSS and BOSS data
• The galaxy luminosity function in groups and clusters: the faint-end upturn and the connection to the field luminosity function
• 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
• Isophotal Shapes of Elliptical/S0 Galaxies from the Sloan Digital Sky Survey
• The effect of the environment on the stellar mass - size relation of present-day galaxies
• Three-Point Correlation Functions of SDSS Galaxies: Luminosity and Color Dependence in Redshift and Projected Space
• The star formation activity in cosmic voids
• The meaning of WISE colours - I. The Galaxy and its satellites
• Active Galactic Nucleus Pairs from the Sloan Digital Sky Survey. II. Evidence for Tidally Enhanced Star Formation and Black Hole Accretion
• The Millennium Galaxy Catalogue: The local supermassive black hole mass function in early- and late-type galaxies
• A Spectroscopic Survey of Faint Quasars in the SDSS Deep Stripe: I. Preliminary Results from the Co-added Catalog
• Stellar Populations of Elliptical Galaxies in the Local Universe
• NIHAO VI. The hidden discs of simulated galaxies
• The growth of luminous red galaxies by merging
• The Space Density of Extended Ultraviolet (XUV) Disks in the Local Universe and Implications for Gas Accretion on to Galaxies
• The Intrinsic Shape of Galaxies in SDSS/Galaxy Zoo
• The pre-processing of subhaloes in SDSS groups and clusters
• Linking bar- and interaction-driven molecular gas concentration with centrally-enhanced star formation in EDGE-CALIFA galaxies
• On the Populations of Radio Galaxies with Extended Morphology at z<0.3
• The ANTARES Astronomical Time-Domain Event Broker
• Updated 34-Band Photometry for the SINGS/KINGFISH Samples of Nearby Galaxies
• Correlating galaxy colour and halo concentration: A tunable Halo Model of galactic conformity
• Constraining the Projected Radial Distribution of Galactic Satellites with the Sloan Digital Sky Survey
• The Weak Lensing Radial Acceleration Relation: Constraining Modified Gravity and Cold Dark Matter theories with KiDS-1000
• Cosmic Web Reconstruction through Density Ridges: Method and Algorithm
• Non-linearity and environmental dependence of the star forming galaxies Main Sequence
• The Massive End of the Stellar Mass Function
• The Relation Between Galaxy Morphology and Environment in the Local Universe: An RC3-SDSS Picture
• Bayesian High-Redshift Quasar Classification from Optical and Mid-IR Photometry
• Do Bars Trigger Activity in Galactic Nuclei?
• Three-Point Correlation Functions of SDSS Galaxies: Constraining Galaxy-Mass Bias
• The clustering of SDSS galaxy groups: mass and color dependence
• Plunging fireworks: Why do infalling galaxies light up on the outskirts of clusters?
• The Sloan Digital Sky Survey Peculiar Velocity Catalogue
• On the universality of void density profiles
• RCSED - A Value-Added Reference Catalog of Spectral Energy Distributions of 800,299 Galaxies in 11 Ultraviolet, Optical, and Near-Infrared Bands: Morphologies, Colors, Ionized Gas and Stellar Populations Properties
• Testing adiabatic contraction with SDSS elliptical galaxies
• Testing the predictions of the cold dark matter model for the sizes, colours, morphologies and luminosities of galaxies with the SDSS
• The cross-correlation between galaxies of different luminosities and Colors
• Inferring the star formation histories of the most massive and passive early-type galaxies at z<0.3
• Topology of structure in the Sloan Digital Sky Survey: model testing
• A Dichotomy in Satellite Quenching Around L* Galaxies
• The Bright End of the Luminosity Function of Red Sequence Galaxies
• The Hierarchical Origins of Observed Galaxy Morphology
• Mapping the Real Space Distributions of Galaxies in SDSS DR7: II. Measuring the growth rate, clustering amplitude of matter and biases of galaxies at redshift $0.1$
• The Redshift-Space Cluster-Galaxy Cross-Correlation Function: I. Modeling Galaxy Infall onto Millennium Simulation Clusters and SDSS Groups
• The Extreme Small Scales: Do Satellite Galaxies Trace Dark Matter?
• A new population of recently quenched elliptical galaxies in the SDSS
• The Gas-Phase Metallicity of Central and Satellite Galaxies in the SDSS
• The Cosmic Thermal History Probed by Sunyaev-Zeldovich Effect Tomography
• Host Galaxies of Type Ic and Broad-lined Type Ic Supernovae from the Palomar Transient Factory: Implication for Jet Production
• SDSS-IV MaNGA: Radial Gradients in Stellar Population Properties of Early-Type and Late-Type Galaxies
• The Spatial Clustering of Low Luminosity AGN
• Ultraviolet Extinction at High Galactic Latitudes
• Central and Satellite Colors in Galaxy Groups: A Comparison of the Halo Model and SDSS Group Catalogs
• Constraining the HI-Halo Mass Relation From Galaxy Clustering
• Cosmic Web Reconstruction through Density Ridges: Catalogue
• Bar-induced central star formation as revealed by integral field spectroscopy from CALIFA
• The UNAM-KIAS Catalog of Isolated Galaxies
• Extragalactic Imprints in Galactic Dust Maps
• Early-type galaxies in the PEARS survey: Probing the stellar populations at moderate redshift
• Euclid preparation: XIX. Impact of magnification on photometric galaxy clustering
• Planck intermediate results. XXXVII. Evidence of unbound gas from the kinetic Sunyaev-Zeldovich effect
• Constraining the Star Formation Histories in Dark Matter Halos: I. Central Galaxies
• A multiscale approach to environment and its influence on the colour distribution of galaxies
• Galaxy Morphology Network: A Convolutional Neural Network Used to Study Morphology and Quenching in $\sim 100,000$ SDSS and $\sim 20,000$ CANDELS Galaxies
• HI Content and Optical Properties of Field Galaxies from the ALFALFA Survey. II. Multivariate Analysis of a Galaxy Sample in Low Density Environments
• A Self-Calibrating Halo-Based Group Finder: Application to SDSS
• The Accretion of Gas onto Galaxies as Traced by their Satellites
• Clustering of Luminous Red Galaxies III: Detection of the Baryon Acoustic Peak in the 3-point Correlation Function
• Evolution of blue E/S0 galaxies from z~1: merger remnants or disk rebuilding galaxies?
• 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
• A new spin on disks of satellite galaxies
• Estimation of galactic model parameters in high latitudes with SDSS
• Halo Histories vs. Galaxy Properties at z=0 II: Large-Scale Galactic Conformity
• Bivariate Galaxy Luminosity Functions in the Sloan Digital Sky Survey
• Evidence of pre-processing and a dependence on dynamical state for low-mass satellite galaxies
• Velocity Dispersion, Size, Sérsic Index and $D_{n}4000$: The Scaling of Stellar Mass with Dynamical Mass for Quiescent Galaxies
• Stellar mass-to-light ratio gradients in galaxies: correlations with mass
• Self-similarity and universality of void density profiles in simulation and SDSS data
• A large sample of low surface brightness disk galaxies from the SDSS. I: The sample and the stellar populations
• A Serendipitous XMM Survey of the SDSS: the evolution of the colour-magnitude diagram of X-ray AGN from z=0.8 to z=0.1
• New Approaches To Photometric Redshift Prediction Via Gaussian Process Regression In The Sloan Digital Sky Survey
• Direct Minkowski Functional analysis of large redshift surveys: a new high--speed code tested on the luminous red galaxy Sloan Digital Sky Survey-DR7 catalogue
• The SAMI Pilot Survey: Stellar Kinematics of Galaxies in Abell 85, 168 and 2399
• Galaxy Clustering Topology in the Sloan Digital Sky Survey Main Galaxy Sample: a Test for Galaxy Formation Models
• Clustering of luminous red galaxies II: small scale redshift space distortions
• The DEEP2 Galaxy Redshift Survey: The Evolution of Void Statistics from z~1 to z~0
• Photometric Redshift Probability Distributions for Galaxies in the SDSS DR8
• A New Test of the Statistical Nature of the Brightest Cluster Galaxies
• Massive Galaxies are Larger in Dense Environments: Environmental Dependence of Mass-Size Relation of Early-Type Galaxies
• SPIDER X - Environmental effects in central and satellite early-type galaxies through the stellar fossil record
• Mergers in Galaxy Groups - I. Structure and Properties of Elliptical Remnants
• The spatial clustering of ROSAT All-Sky Survey Active Galactic Nuclei IV. More massive black holes reside in more massive dark matter halos
• Cosmic web dependence of galaxy clustering and quenching in SDSS
• Measuring the X-ray luminosities of SDSS DR7 clusters from RASS
• The Stellar Mass Components of Galaxies: Comparing Semi-Analytical Models with Observation
• The dependence of the galaxy stellar-to-halo mass relation on galaxy morphology
• Constraining the Cosmic Baryon Distribution with Fast Radio Burst Foreground Mapping
• Alignment between filaments and galaxy spins from the MaNGA integral-field survey
• A z=1.82 Analog of Local Ultra-massive Elliptical Galaxies
• Prediction of galaxy halo masses in SDSS DR7 via a machine learning approach
• 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
• The HI Mass Function and Velocity Width Function of Void Galaxies in the Arecibo Legacy Fast ALFA Survey
• The Galaxy Optical Luminosity Function from the AGN and Galaxy Evolution Survey (AGES)
• Precision Measurements of the Cluster Red Sequence using an Error Corrected Gaussian Mixture Model
• Environmental dependence of AGN activity. I.: the effects of host galaxy
• 3D Genus Topology of Luminous Red Galaxies
• Elucidating Galaxy Assembly Bias in SDSS
• The MOND Fundamental Plane
• Halpha3: an Halpha imaging survey of HI selected galaxies from ALFALFA. III. Nurture shapes up the Hubble sequence in the Great Wall
• The Strikingly Similar Relation between Satellite and Central Galaxies and Their Dark Matter Halos Since z=2
• The complete census of optically selected AGNs in the Coma Supercluster: the dependence of AGN activity on the local environment
• Stellar, gas and dark matter content of barred galaxies
• Modelling the Transfer Function for the Dark Energy Survey
• Young ages and other intriguing properties of massive compact galaxies in the Local Universe
• Are rotating planes of satellite galaxies ubiquitous?
• The Jubilee ISW Project II: observed and simulated imprints of voids and superclusters on the cosmic microwave background
• Galactic Satellite Systems: Radial Distribution and Environment Dependence of Galaxy Morphology
• Very large scale correlations in the galaxy distribution
• The Star-Formation Main Sequence: The Dependence of Specific Star Formation Rate and Its Dispersion on Galaxy Stellar Mass
• Spatially Resolved Galaxy Star Formation and its Environmental Dependence I
• SDSS-IV MaNGA: Stellar initial mass function variation inferred from Bayesian analysis of the integral field spectroscopy of early type galaxies
• Characterizing Dust Attenuation in Local Star Forming Galaxies: Inclination Effects and the 2175Å Feature
• Euclid. V. The Flagship galaxy mock catalogue: a comprehensive simulation for the Euclid mission
• A Candidate Dual AGN at z=1.175
• Building a Predictive Model of Galaxy Formation - I: Phenomenological Model Constrained to the $z=0$ Stellar Mass Function
• The Dependence of Star Formation Activity on Stellar Mass Surface Density and Sersic Index in zCOSMOS Galaxies at 0.5<z<0.9 Compared with SDSS Galaxies at 0.04<z<0.08
• On the evidence for large-scale galactic conformity in the local Universe
• How Massive are Massive Compact Galaxies?
• Properties of satellite galaxies in the SDSS photometric survey: luminosities, colours and projected number density profiles
• Stellar mass functions of galaxies, disks and spheroids at z~0.1
• Star Formation Quenching Timescale of Central Galaxies in a Hierarchical Universe
• The H alpha Galaxy Survey. IV. Star formation in the local Universe
• The HI Morphology and Stellar Properties of Strongly Barred Galaxies: support for bar quenching in massive spirals
• Halo Histories vs. Galaxy Properties at z=0, I: The Quenching of Star Formation
• The properties of early-type galaxies in the Ursa Major cluster
• Red star-forming and blue passive galaxies in clusters
• ADDGALS: Simulated Sky Catalogs for Wide Field Galaxy Surveys
• The 2dF-SDSS LRG and QSO Survey: The Star Formation Histories of Luminous Red Galaxies
• An X-ray Detected Group of Quiescent Early-type Galaxies at z=1.6 in the Chandra Deep Field South
• Broadband Intensity Tomography: Spectral Tagging of the Cosmic UV Background
• The Large-Scale Environments of Type Ia Supernovae: Evidence for a Metallicity Bias in the Rate or Luminosity of Prompt Ia Events
• Detecting Radio-AGN signatures in Red geysers
• The nature of assembly bias - III. Observational properties
• AGN and their host galaxies in the local Universe: two mass independent Eddington ratio distribution functions characterize black hole growth
• Using 21cm Absorption in Small Impact Parameter Galaxy-QSO Pairs to Probe Low-Redshift Damped and Sub-Damped Lyman-alpha System
• Galaxy-galaxy weak-lensing measurement from SDSS: II. host halo properties of galaxy groups
• Mg II Absorption Characteristics of a Volume-Limited Sample of Galaxies at z ~ 0.1
• The Dearth of Difference between Central and Satellite Galaxies I. Perspectives on star formation quenching and AGN activities
• Dozens of compact and high velocity-dispersion early-type galaxies in Sloan Digital Sky Survey
• The Dependence of AGN Activity on Environment in SDSS
• Updated Results on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• Constraining the last 7 billion years of galaxy evolution in semi-analytic models
• The galaxy counts-in-cells distribution from the SDSS
• Point spread function tails and the measurements of diffuse stellar halo light around edge-on disc galaxies
• Satellite Quenching, Galaxy Inner Density and the Halo Environment
• A Deep Proper Motion Catalog Within the Sloan Digital Sky Survey Footprint. II. The White Dwarf Luminosity Function
• Eppur si muove: Positional and kinematic correlations of satellite pairs in the low Z universe
• The statistical nature of the brightest group galaxies
• Where are compact groups in the local Universe?
• One Plane for All: Massive Star-Forming and Quiescent Galaxies Lie on the Same Mass Fundamental Plane at z~0 and z~0.7
• The galaxy-subhalo connection in low-redshift galaxy clusters from weak gravitational lensing
• Stellar mass-gap as a probe of halo assembly history and concentration: youth hidden among old fossils
• The PAU Survey: Photometric redshifts using transfer learning from simulations
• The dependence of the pairwise velocity dispersion on galaxy properties
• Evidence of ongoing AGN-driven feedback in a quiescent post starburst E+A galaxy
• Central galaxies in different environments: Do they have similar properties?
• Environmental Effects on the Metal Enrichment of Low Mass Galaxies in Nearby Clusters
• Galaxy Zoo: major galaxy mergers are not a significant quenching pathway
• Emission-lines calibrations of the Star Formation Rate from the Sloan Digital Sky Survey
• The clustering of X-ray selected AGN at z=0.1
• Quiescent Galaxy Size and Spectroscopic Evolution: Combining HSC Imaging and Hectospec Spectroscopy
• Galaxy Zoo: Evidence for rapid, recent quenching within a population of AGN host galaxies
• FLIMFLAM DR1: The First Constraints on the Cosmic Baryon Distribution from 8 FRB sightlines
• The Red Dead Redemption Survey of Circumgalactic Gas About Massive Galaxies. I. Mass and Metallicity of the Cool Phase
• A weak gravitational lensing recalibration of the scaling relations linking the gas properties of dark halos to their mass
• 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 Environmental Dependence of the Luminosity-Size Relation for Galaxies
• Breaking the self-averaging properties of spatial galaxy fluctuations in the Sloan Digital Sky Survey - Data Release Six
• Measuring the distance-redshift relation with the baryon acoustic oscillations of galaxy clusters
• Does the Galaxy-Halo Connection Vary with Environment?
• A comparative study of satellite galaxies in Milky Way-like galaxies from HSC, DECaLS and SDSS
• Testing cold dark matter with the low mass Tully-Fisher relation
• The boundary of cosmic filaments
• Massive Star-Forming Galaxies Have Converted Most of Their Halo Gas into Stars
• How are galaxies assigned to halos? Searching for assembly bias in the SDSS galaxy clustering
• A High Resolution Atlas of Composite SDSS Galaxy Spectra
• The environment of barred galaxies in the low-redshift Universe
• Structural and Stellar Population Properties vs. Bulge Types in Sloan Digital Sky Survey Central Galaxies
• Dark Energy Survey Year 3 results: Marginalisation over redshift distribution uncertainties using ranking of discrete realisations
• Hubble Space Telescope Observations of Two Faint Dwarf Satellites of Nearby LMC Analogs from MADCASH
• The Conditional Colour-Magnitude Distribution: I. A Comprehensive Model of the Colour-Magnitude-Halo Mass Distribution of Present-Day Galaxies
• Mapping the real space distributions of galaxies in SDSS DR7: I. Two Point Correlation Functions
• The Faint End of the Luminosity Function and Low Surface Brightness Galaxies
• Triggering the Untriggered: The First Einstein Probe-Detected Gamma-Ray Burst 240219A and Its Implications
• No evidence for modifications of gravity from galaxy motions on cosmological scales
• Photometric Redshifts from SDSS Images with an Interpretable Deep Capsule Network
• Constraining star formation rates in cool-core brightest cluster galaxies
• The hot circumgalactic medium in the eROSITA All-Sky Survey II. Scaling relations between X-ray luminosity and galaxies' mass
• Using Multipoles of the Correlation Function to Measure H(z), D_A(z), and β(z) from Sloan Digital Sky Survey Luminous Red Galaxies
• Color Dependence in the Spatial Distribution of Satellite Galaxies
• Towards Accurate Modelling of Galaxy Clustering on Small Scales: Testing the Standard $\Lambda \mathrm{CDM}$ + Halo Model
• The redshift distribution of cosmological samples: a forward modeling approach
• Radio Detection of Radio-Quiet Galaxies
• The stellar halo of isolated central galaxies in the Hyper Suprime-Cam imaging survey
• A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey
• The Fundamental Plane of massive quiescent galaxies out to z~2
• Connections between galaxy mergers and Starburst: evidence from local Universe
• Automated bar detection in local disc galaxies from the SDSS - The colors of bars
• The effect of dry mergers on the color-magnitude relation of early-type galaxies
• SDSS-IV MaNGA: Uncovering the Angular Momentum Content of Central and Satellite Early-type Galaxies
• Investigating the Stellar Mass Growth Histories of Satellite Galaxies as a Function of Infall Time using Phase-Space
• The Optical Green Valley vs Mid-IR Canyon in Compact Groups
• SDSS-IV MaNGA: spatially resolved dust attenuation in spiral galaxies
• The effect of cosmic web filaments on galaxy evolution
• Precision Spectrophotometry at the Level of 0.1%
• Optical Properties of Host Galaxies of Extragalactic Nuclear Water Masers
• ACCESS: NIR Luminosity Function and Stellar Mass Function of Galaxies in the Shapley Supercluster Environment
• Galaxy clustering and projected density profiles as traced by satellites in photometric surveys: Methodology and luminosity dependence
• Measurement of the pairwise kinematic Sunyaev-Zeldovich effect with Planck and BOSS data
• The extended Baryon Oscillation Spectroscopic Survey: measuring the cross-correlation between the MgII flux transmission field and quasars and galaxies at $z=0.59$
• SDSS-IV MANGA: A Star Formation -- Baryonic Mass Relation at Kpc Scales
• The best fit for the observed galaxy Counts-in-Cell distribution function
• The nature of red dwarf galaxies
• The morphological transformation and the quenching of galaxies
• Massive central galaxies of galaxy groups in the Romulus simulations: an overview of galaxy properties at z=0
• Star Formation and Substructure in Galaxy Clusters
• Ultra deep sub-kpc view of nearby massive compact galaxies
• Minkowski Functionals of Convergence Maps and the Lensing Figure of Merit
• Tomographic Alcock-Paczynski Test with Redshift-Space Correlation Function: Evidence for the Dark Energy Equation of State Parameter w>-1
• Small- and Large-Scale Galactic Conformity in SDSS DR7
• Brightest galaxies as halo centre tracers in SDSS DR7
• IQ-Collaboratory 1.1: the Star-Forming Sequence of Simulated Central Galaxies
• Effect of local and large-scale environments on nuclear activity and star formation
• Tracing the Filamentary Structure of the Galaxy Distribution at z~0.8
• The EFIGI catalogue of 4458 nearby galaxies with morphology II. Statistical properties along the Hubble sequence
• The gas-phase metallicities of star-forming galaxies in aperture-matched SDSS samples follow potential rather than mass or average surface density
• The Mass Dependance of Satellite Quenching in Milky Way-like Halos
• Spectral Properties of Galaxies in Void Regions
• Fourier Phase Analysis of SDSS Galaxies
• Probing hot gas around luminous red galaxies through the Sunyaev-Zel'dovich effect
• The nature of the SDSS galaxies in various classes based on morphology, colour and spectral features -- I. Optical properties
• Modeling Galaxy-Galaxy Weak Lensing with SDSS Groups
• An observational proxy of halo assembly time and its correlation with galaxy properties
• Revealing the cosmic web dependent halo bias
• Dissecting the Red Sequence. IV. The Role of Truncation in the Two-Dimensional Family of Early-Type Galaxy Star Formation Histories
• Using Galaxy Pairs to Probe Star Formation During Major Halo Mergers
• The dependence of galaxy clustering on tidal environment in the Sloan Digital Sky Survey
• The dependence of AGN activity on stellar and halo mass in Semi-Analytic Models
• Alignments of Group Galaxies with Neighboring Groups
• Galaxy Bias and ${\sigma }_8$ from Counts in Cells from the SDSS Main Sample
• Groups in the Millennium Simulation and in SDSS DR7
• Automated Morphological Classification of SDSS Red Sequence Galaxies
• BSG alignment of SDSS galaxy groups
• Stellar populations of galaxies in the ALHAMBRA survey up to $z\sim 1$. IV. Properties of quiescent galaxies on the stellar mass$-$size plane
• Updated void catalogs of the SDSS DR7 main sample
• Detected fluctuations in SDSS LRG magnitudes: Bulk flow signature or systematic?
• Surface photometry of WINGS galaxies with GASPHOT
• The influence of halo assembly on galaxies and galaxy groups
• Size distribution of galaxies in SDSS DR7: weak dependence on halo environment
• Galaxy groups in the 2MASS Redshift Survey
• Growth of bulges in disc galaxies since $z\sim 1$
• Galaxy clustering dependence on the $\left[\mathrm{O}\mathrm{II}\right]$ emission line luminosity in the local Universe
• Differences in Halo-Scale Environments between Type 1 and Type 2 AGNs at Low Redshift
• Increasing the Lensing Figure of Merit through Higher Order Convergence Moments
• Structure in the 3D Galaxy Distribution: I. Methods and Example Results
• The metallicity distributions in high-latitudes with SDSS
• Galaxy and Mass Assembly (GAMA): Colour and luminosity dependent clustering from calibrated photometric redshifts
• ELUCID V. Lighting dark matter halos with galaxies
• The Role of Environment on the Formation of Early-Type Galaxies
• Halo Occupation Distribution Modeling of Green Valley Galaxies
• 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
• Alignment of galaxy spins in the vicinity of voids
• Local and global environmental effects on galaxies and active galactic nuclei
• The SZ flux-mass ($Y$-$M$) relation at low halo masses: improvements with symbolic regression and strong constraints on baryonic feedback
• The UV-Optical Color Dependence of Galaxy Clustering in the Local Universe
• Bivariate Luminosity Function of Galaxy Pairs
• Testing the presence of multiple photometric components in nearby early-type galaxies using SDSS
• Galactic conformity measured in semi-analytic models
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Never mind the gaps: comparing techniques to restore homogeneous sky coverage
• Testing the Modern Merger Hypothesis via the Assembly of Massive Blue Elliptical Galaxies in the Local Universe
• A Fundamental Line for Elliptical Galaxies
• Probing the galaxy-halo connection with total satellite luminosity
• The effect of environment on the structure of disc galaxies
• Implications of the remarkable homogeneity of galaxy groups and clusters
• The Relation between Dynamical Mass-to-Light Ratio and Color for Massive Quiescent Galaxies out to z~2 and Comparison with Stellar Population Synthesis Models
• The weak imprint of environment on the stellar populations of galaxies
• Mass segregation trends in SDSS galaxy groups
• The HST/ACS Coma Cluster Survey - VII. Structure and Assembly of Massive Galaxies in the Center of the Coma Cluster
• Optical and Infrared Diagnostics of SDSS galaxies in the SWIRE Survey
• Observational constraints on the physics behind the evolution of AGN since z ~ 1
• Color-Magnitude Distribution of Face-on Nearby Galaxies in SDSS DR7
• An accurate method to determine the systematics due to the peculiar velocities of galaxies in measuring the Hubble constant from gravitational wave standard sirens
• Targeting supermassive black hole binaries and gravitational wave sources for the pulsar timing array
• Rise and fall of post-starburst galaxies in Magneticum Pathfinder
• Euclid preparation: XII. Optimizing the photometric sample of the Euclid survey for galaxy clustering and galaxy-galaxy lensing analyses
• The Sloan Nearby Cluster Weak Lensing Survey
• A new methodology to test galaxy formation models using the dependence of clustering on stellar mass
• Measuring Coherent Motions in the Universe
• Evidence of Galaxy Assembly Bias in SDSS DR7 Galaxy Samples from Count Statistics
• Testing the accuracy of clustering redshift with simulations
• The Galaxy Cross-Correlation Function as a Probe of the Spatial Distribution of Galactic Satellites
• The dark side of galaxy stellar populations I: The stellar-to-halo mass relation and the velocity dispersion - halo mass relation
• Color-magnitude relations of late-type galaxies
• From Blue Cloud to Red Sequence: Evidence of Morphological Transition Prior to Star Formation Quenching
• The evolution of the scatter of the cosmic average color-magnitude relation: Demonstrating consistency with the ongoing formation of elliptical galaxies
• The bivariate gas-stellar mass distributions and the mass functions of early- and late-type galaxies at $z\sim 0$
• Color Magnitude Relation and Morphology of Low-Redshift ULIRGs in SDSS
• Satellite galaxies around present-day massive ellipticals
• Stellar mass versus stellar velocity dispersion: which is better for linking galaxies to their dark matter halos?
• SDSS-IV MaNGA: Signatures of halo assembly in kinematically misaligned galaxies
• Ultramassive dense early-type galaxies: velocity dispersions and number density evolution since z=1.6
• The DESI PRObabilistic Value-Added Bright Galaxy Survey (PROVABGS) Mock Challenge
• The first constraint from SDSS galaxy-galaxy weak lensing measurements on interacting dark energy models
• Morphological evolution and galactic sizes in the L-Galaxies SA model
• The Velocity Dispersion Function for Quiescent Galaxies in the Local Universe
• Forward Modeling Populations of Flares from Tidal Disruptions of Stars by Super-massive Black Holes
• HI Content and Optical Properties of Field Galaxies from the ALFALFA Survey. I.Selection of a Control Sample
• Shocks or Photoionization: Direct Temperature Measurements of the Low-Ionization Gas in Quiescent Galaxies
• Measurement of $H(z)$ and $D_A(z)$ from the two-dimensional power spectrum of Sloan Digital Sky Survey luminous red galaxies
• A Robust Distance Measurement and Dark Energy Constraints from the Spherically-Averaged Correlation Function of Sloan Digital Sky Survey Luminous Red Galaxies
• Hosts and triggers of AGNs in the Local Universe
• The Transparency of Galaxy Clusters
• Conditional HI mass functions and the HI-to-halo mass relation in the local Universe
• Massive relic galaxies prefer dense environments
• Detection of spatial correlations of fundamental plane residuals, and cosmological implications
• Euclid: The selection of quiescent and star-forming galaxies using observed colours
• Crawling the Cosmic Network: Exploring the Morphology of Structure in the Galaxy Distribution
• Alignment between satellite and central galaxies in the SDSS DR7: dependence on large-scale environment
• A New Technique for Galaxy Photometric Redshifts in the Sloan Digital Sky Survey
• Extinction properties of lensing galaxies
• Revealing the Nature of Extreme Coronal-line Emitter SDSS J095209.56+214313.3
• Simulations of isolated dwarf galaxies formed in dark matter halos with different mass assembly histories
• Stellar Mass and color dependence of the three-point correlation function of galaxies in the local universe
• Connecting optical and X-ray tracers of galaxy cluster relaxation
• DESCQA: An Automated Validation Framework for Synthetic Sky Catalogs
• A complete spectroscopic catalogue of local galaxies in the Northern spring sky -- Gas properties and nuclear activity in different environments
• Morphological Segregation in the Surroundings of Cosmic Voids
• An Analysis Framework for Understanding the Origin of Nuclear Activity in Low-Power Radio Galaxies
• Dark matter halos of barred disk galaxies
• Estimating dust attenuation from galactic spectra. II. Stellar and gas attenuation in star-forming and diffuse ionized gas regions in MaNGA
• Red-channel (6000-8000 Å) nuclear spectra of 376 local galaxies
• The Thermal Sunyaev-Zel'dovich Effect from Massive, Quiescent 0.5 $\le$ z $\le$ 1.5 Galaxies
• RedMaPPer: Evolution and Mass Dependence of the Conditional Luminosity Functions of Red Galaxies in Galaxy Clusters
• The Isophotal Structure of Early-Type Galaxies in the SDSS: Dependence on AGN Activity and Environment
• The stellar mass in and around isolated central galaxies: connections to the total mass distribution through galaxy-galaxy lensing in the Hyper Suprime-Cam survey
• Halpha3: an Halpha imaging survey of HI selected galaxies from ALFALFA. V: The Coma Supercluster survey completion
• The Nuclear Activities of Nearby S0 Galaxies
• Survival of pure disk galaxies over the last 8 billion years
• A Deep Proper Motion Catalog Within The Sloan Digital Sky Survey Footprint
• Compact Groups of Galaxies in Sloan Digital Sky Survey and LAMOST Spectral Survey: I. The Catalogs
• Red Misfits in the Sloan Digital Sky Survey: Properties of Star-forming Red Galaxies
• The cosmic shallows I: interaction of CMB photons in extended galaxy halos
• The distribution of faint satellites around central galaxies in the CFHT Legacy Survey
• Robust automatic photometry of local galaxies from SDSS Dissecting the color magnitude relation with color profiles
• Rejuvenation triggers nuclear activity in nearby galaxies
• The dependence of subhalo abundance matching on galaxy photometry and selection criteria
• Probing star formation and ISM properties using galaxy disk inclination I: Evolution in disk opacity since $z\sim 0.7$
• Constraining Star Formation and AGN in z~2 Massive Galaxies using High Resolution MERLIN Radio Observations
• On the dependence of galaxy morphologies on galaxy mergers
• Critical Examinations of QSO Redshift Periodicities and Associations with Galaxies in Sloan Digital Sky Survey Data
• Main Sequence Scatter is Real: The Joint Dependence of Galaxy Clustering on Star Formation and Stellar Mass
• Compact Groups of Galaxies in Sloan Digital Sky Survey and LAMOST Spectral Survey. II. Dynamical Properties of Isolated and Embedded Groups
• Investigating the Projected Phase Space of Gaussian and Non-Gaussian Clusters
• Low redshift quasars in the SDSS Stripe 82. Host galaxy colors and close environment
• NUV-IR colours of red sequence galaxies in local clusters
• The Stellar Mass Fundamental Plane and Compact Quiescent Galaxies at z < 0.6
• A new method to measure galaxy bias by combining the density and weak lensing fields
• Physical properties of galaxies: toward a consistent comparison between hydrodynamical simulations and SDSS
• Global dust attenuation in disc galaxies: strong variation with specific star formation and stellar mass, and the importance of sample selection
• Observed versus modelled u,g,r,i,z-band photometry of local galaxies - Evaluation of model performance
• The hot circumgalactic medium in the eROSITA All-Sky Survey III. Star-forming and quiescent galaxies
• The Circumnuclear Star-forming Activities along the Hubble Sequence
• Maturing Satellite Kinematics into a Competitive Probe of the Galaxy-Halo Connection
• Groups of Galaxies in AEGIS: The 200 ksec Chandra Extended X-ray Source catalogue
• The evolution of star formation activity in galaxy groups
• Galaxy-Galaxy Weak Lensing Measurements from SDSS: I. Image Processing and Lensing signals
• The evolution of disc galaxies with and without classical bulges since z~1
• A finer view of the conditional galaxy luminosity function and magnitude-gap statistics
• The discrepancy between dynamical and stellar masses in massive compact galaxies traces non-homology
• On the Clustering of Faint Red Galaxies
• Simulating the Mass-Metallicity Relation from z=1
• On the relation between Seyfert 2 accretion rate and environment at z < 0.1
• The similar stellar populations of quiescent spiral and elliptical galaxies
• The intrinsic SFRF and sSFRF of galaxies: comparing SDSS observation with IllustrisTNG simulation
• Tracing the cosmic velocity field at z ~ 0.1 from galaxy luminosities in the SDSS DR7
• Black Hole - Bulge Relationship of Post-Starburst Quasars at z \sim 0.3
• Counts-in-Cylinders in the Sloan Digital Sky Survey with Comparisons to N-body Simulations
• The IMACS Cluster Building Survey: V. Further Evidence for Starburst Recycling from Quantitative Galaxy Morphologies
• Halo Histories vs. Galaxy Properties at z=0, III: The Properties of Star-Forming Galaxies
• Galaxy clustering with photometric surveys using PDF redshift information
• Constraining Delay Time Distribution of Binary Neutron Star Mergers from Host Galaxy Properties
• Modeling Redshift-Space Clustering with Abundance Matching
• The Nature of Obscuration in AGN: I. Insights from Host Galaxies
• Dissect two-halo galactic conformity effect for central galaxies: The dependence of star formation activities on the large-scale environment
• The cosmic web around the Coma cluster from constrained cosmological simulations: I. Filaments connected to Coma at $z=0$
• Satellite quenching and morphological transformation of galaxies in groups and clusters
• Wavelet analysis of baryon acoustic structures in the galaxy distribution
• Galactic Conformity in both Star-formation and Morphological Properties
• NUV signatures of environment driven galaxy quenching in SDSS groups
• Star Formation and Supercluster Environment of 107 Nearby Galaxy Clusters
• Multi-Scale Morphological Analysis of SDSS DR5 Survey using the Metric Space Technique
• The Differing Relationships Between Size, Mass, Metallicity and Core Velocity Dispersion of Central and Satellite Galaxies
• A Study of Central Galaxy Rotation with Stellar Mass and Environment
• The Dearth of Difference between Central and Satellite Galaxies III. Environmental Dependence of Mass-Size and Mass-Structure Relations
• Radial Star Formation Histories in 32 Nearby Galaxies
• Using Colors to Improve Photometric Metallicity Estimates for Galaxies
• Forward Modeling of Spectroscopic Galaxy Surveys: Application to SDSS
• The environmental dependence of rapidly-quenching and rejuvenating galaxies
• Color, Structure, and Star Formation History of Dwarf Galaxies over the last ~3 Gyr with GEMS and SDSS
• Star formation and morphological properties of galaxies in the Pan-STARRS $3\pi$ survey- I. A machine learning approach to galaxy and supernova classification
• The Baryonic Collapse Efficiency of Galaxy Groups in the RESOLVE and ECO Surveys
• Isophotal shapes of early-type galaxies to very faint levels
• Stellar mass versus velocity dispersion as tracer of the lensing signal around bulge-dominated galaxies
• Topology of Luminous Red Galaxies from the Sloan Digital Sky Survey
• Cosmological Information from the Small-scale Redshift Space Distortions
• A Virtual Observatory Census to Address Dwarfs Origins. AVOCADO - I. Science goals, sample selection and analysis tools
• Imaging of Three Possible Low Redshift Analogs to High Redshift Compact Red Galaxies
• The nature of the SDSS galaxies in various classes based on morphology, colour and spectral features - II. Multi-wavelength properties
• SDSS-IV MaNGA: Bayesian analysis of the star formation history of low-mass galaxies in the local Universe
• An Extensive Photometric Catalog of CALIFA Galaxies
• Connections between galaxy properties and halo formation time in the cosmic web
• Faint, Evolving Radio AGN in SDSS Luminous Red Galaxies
• BAT AGN Spectroscopic Survey -- XIII. The nature of the most luminous obscured AGN in the low-redshift universe
• Unsupervised Classification of Galaxies. I. ICA feature selection
• The Connection between Star-Forming Galaxies, AGN Host Galaxies and Early-Type Galaxies in the SDSS
• Spectro-Imaging Forward Model of Red and Blue Galaxies
• Compact galaxies and the size-mass galaxy distribution from a colour-selected sample at 0.04 < z < 0.15 supplemented by ugrizYJHK photometric redshifts
• Measuring the luminosity and virial black hole mass dependence of quasar-galaxy clustering at z ~ 0.8
• Central velocity dispersion catalog of LAMOST-DR7 galaxies
• Early-Type Galaxy Star Formation Histories in Different Environments
• The evolution of radial gradients of MaNGA quiescent elliptical galaxies: inside-out quenching or outer mass growth?
• In the crosshair: astrometric exoplanet detection with WFIRST's diffraction spikes
• Properties of X-ray selected Broad Absorption Line Quasars
• AXES-SDSS: comparison of SDSS galaxy groups with all-sky X-ray extended sources
• Constraining the scatter in the galaxy-halo connection at Milky Way masses
• Connecting SDSS central galaxies to their host halos using total satellite luminosity
• What Regulates Galaxy Evolution? Open Questions in Our Understanding of Galaxy Formation and Evolution
• Alignments of the Galaxies in and around the Virgo Cluster with the Local Velocity Shear
• Stellar Metallicity Gradients in SDSS galaxies
• Characteristic mass in galaxy quenching: environmental versus internal effects
• Testing galaxy formation models with galaxy stellar mass functions
• Galaxy Properties in Clusters: Dependence on the Environment and the Cluster Identification Techniques
• Two phase galaxy formation: The Evolutionary Properties of Galaxies
• The Global Environment of Small Galaxy Systems
• Satellites in the field and lens galaxies: SDSS/COSMOS vs. SLACS/CLASS
• Magnitude and size evolution of bulgeless galaxies
• Spatially Resolved Galaxy Star Formation and its Environmental Dependence II. Effect of the Morphology-Density Relation
• Unveiling the internal structure of Hercules supercluster
• The relation between galaxy density and radio jet power for 1.4 GHz VLA selected AGN in Stripe 82
• Performance study of Lagrangian methods: reconstruction of large scale peculiar velocities and baryonic acoustic oscillations
• Galaxy Concentrations are Trimodal
• Simulation-based inference of deep fields: galaxy population model and redshift distributions
• Galaxy evolution in compact groups I: Revealing a transitional galaxy population through a multiwavelength approach
• Distribution of Cold ($\lesssim 300$K) Atomic Gas in Galaxies: Results from the GBT HI Absorption Survey Probing the Inner Halos ($\rho <20$kpc) of Low-z Galaxies
• The Coevolution of Massive Quiescent Galaxies and Their Dark Matter Halos over the Last 6 Billion Years
• Exploring Galaxy Evolution Time-Scales in Clusters: Insights from the Projected Phase Space
• Red galaxies with pseudo-bulges in the SDSS: closer to disk galaxies or to classical bulges?
• Semi-analytic spectral fitting: simultaneously modelling the mass accumulation and chemical evolution in MaNGA spiral galaxies
• Group galaxy number density profiles far out: is the 'one-halo' term NFW out to $>10$ virial radii?
• The Stellar Mass Assembly of Low Redshift, Massive, Central Galaxies in SDSS and the TNG300 simulation
• MOIRCS Deep Survey. VII: NIR Morphologies of Star-forming Galaxies at Redshift z~1
• The SRG/eROSITA all-sky survey. X-ray emission from the warm-hot phase gas in long cosmic filaments
• On the connection between shape and stellar population in early-type galaxies
• Cosmological Parameter Estimation from the Two-Dimensional Genus Topology -- Measuring the Expansion History using the Genus Amplitude as a Standard Ruler
• Genus statistics using the Delaunay tessellation field estimation method: (I) tests with the Millennium Simulation and the SDSS DR7
• Galaxy growth by merging in the nearby universe
• Orbital Dependence of Galaxy Properties in Satellite Systems of Galaxies
• Observing Correlations Between Dark Matter Accretion and Galaxy Growth: I. Recent Star Formation Activity in Isolated Milky Way-Mass Galaxies
• The Local Star Formation Rate Surface Density And Metallicity Relation For Star-forming Galaxies
• Satellite Alignment: III. Satellite Galaxies Spatial Distribution and their Dependence on Redshift with A Novel Galaxy Finder
• The SFR-radius connection: data and implications for wind strength and halo concentration
• Uncertainty in 2-point correlation function estimators and BAO detection in SDSS DR7
• Galaxy populations in groups and clusters: evidence for a characteristic stellar mass scale at $M_{\ast }\sim 10^{9.5}{M}_{\odot }$
• Massive Red Spiral Galaxies in SDSS-IV MaNGA Survey
• Late-formed halos prefer to host quiescent central galaxies. I. Observational results
• The differences between mass- and light-derived structural parameters over time for MaNGA Elliptical galaxies
• On the nature of Small Galaxy Systems
• Galaxy-group (halo) alignments from SDSS DR7 and the ELUCID simulation
• Halo Masses of MgII absorbers at z\sim 0.5 from SDSS DR7
• Fractal analysis of the large-scale stellar mass distribution in the Sloan Digital Sky Survey
• Global Properties of Neutral Hydrogen in Compact Groups
• A spectroscopic measure of the star-formation rate density in dwarf galaxies at z~1
• Quantifying the coherent outflows of galaxies around voids in the SDSS DR7
• Groups of two galaxies in SDSS: implications of colours on star formation quenching time-scales
• The power spectrum of systematics in cosmic shear tomography and the bias on cosmological parameters
• The Large-scale Effect of Environment on Galactic Conformity
• BASILISK: Bayesian Hierarchical Inference of the Galaxy-Halo Connection using Satellite Kinematics--I. Method and Validation
• Detection of a Multiphase Intragroup Medium: Results from the COS-IGrM Survey
• Comparing galaxy disk and star-formation properties in X-ray bright and faint groups and clusters
• The thermal and gravitational energy densities in the large-scale structure of the Universe
• Morphologies of galaxies within voids
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Constraining the Galaxy-Halo Connection with Optimal Statistics
• Stellar Mass Profiles of Quiescent Galaxies in Different Environments at $z\sim 0$
• Foreground and Source of a Cluster of Ultra-high Energy Cosmic Rays
• Influence of the Void Environment on Chemical Abundances in Dwarf Galaxies and Implications for Connecting Star Formation and Halo Mass
• Using the Modified Nearest Neighbor Method to Correct Fiber-collision Effects on Galaxy Clustering
• Population Gradients in the SDSS Galaxy Catalog. The role of merging
• Revisiting the clustering of narrow-line AGN in the local Universe: Joint dependence on stellar mass and color
• Nitrogen-to-Oxygen Abundance Ratio Variation In Quiescent Galaxies
• Asymmetry Revisited: The Effect of Dust Attenuation and Galaxy Inclination
• Molecular gas scaling relations for local star-forming galaxies in the low-$M_{\ast }$ regime
• Dark against luminous matter around isolated central galaxies: a comparative study between modern surveys and Illustris-TNG
• Structure in the 3D Galaxy Distribution: II. Voids and Watersheds of Local Maxima and Minima
• An accurate new method of calculating absolute magnitudes and K-corrections applied to the Sloan filter set
• From Halos to Galaxies. VI. Improved halo mass estimation for SDSS groups and measurement of the halo mass function
• The Properties of Type Ia Supernova Host Galaxies from the Sloan Digital Sky Survey
• The influence of Hickson-like compact group environment on galaxy luminosities
• Infrared Spectral Energy Distribution of Galaxies in the AKARI All Sky Survey: Correlations with Galaxy Properties, and Their Physical Origin
• BreakBRD Galaxies I: Global Properties of Spiral Galaxies with Central Star Formation in Red Disks
• Galaxy-galaxy lensing data: $f(T)$ gravity challenges General Relativity
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions and Lingering Tension
• Demographics of Sloan Digital Sky Survey galaxies along the Hubble sequence
• SUZAKU Observation of a New Merging Group of Galaxies at a Filamentary Junction
• The Luminosity and Stellar Mass Functions of Red W1-W2 Galaxies
• Nearby Galaxies in More Distant Contexts
• The co-evolution of strong AGN and central galaxies in different environments
• UV to FIR catalogue of a galaxy sample in nearby clusters: SEDs and environmental trends
• PAC.V. The Roles of Mass and Environment in the Quenching of Galaxies
• Probing star formation and ISM properties using galaxy disk inclination III: Evolution in dust opacity and clumpiness between redshift 0.0 < z < 0.7 constrained from UV to NIR
• The stellar mass function and efficiency of galaxy formation with a varying initial mass function
• Stellar Reddening Based Extinction Maps for Cosmological Applications
• The dependence of low redshift galaxy properties on environment
• The spatial distribution of satellites in galaxy clusters
• Exploring the links between star formation and minor companions around isolated galaxies
• Universal void density profiles from simulation and SDSS
• The less significant role of large-scale environment than optical AGN in nearby, isolated elliptical galaxies
• Re-assessing the stellar population scaling relations of the galaxies in the Local Universe
• The Ultraviolet Deep Imaging Survey of Galaxies in the Bootes Void I: catalog, color-magnitude relations and star formation
• Galaxy-halo size relation from Sloan Digital Sky Survey Data Release 7 and the ELUCID simulation
• Astrophysics in 2005
• A general approach to quenching and galactic conformity
• Constraints on the evolutionary mechanisms of massive galaxies since $z\sim 1$ from their velocity dispersions
• The dependence of cluster galaxy properties on the central entropy of their host cluster
• J-PLUS: the impact of bars on quenching time-scales in nearby green valley disc galaxies
• Are Milky-Way-like galaxies like the Milky Way? A view from SDSS-IV/MaNGA
• Red bulgeless galaxies in SDSS DR7. Are there any AGN hosts?
• The Metallicity measurement of Early-type Galaxies
• Effect of Bars on Evolution of SDSS Spiral Galaxies
• SDSS-IV MaNGA: Enhanced Star Formation in Galactic-scale Outflows
• Star-forming and Quiescent Central Galaxies Cluster Similarly: Implications for the Galaxy-Halo Connection
• Statistical properties of filaments in the cosmic web
• Systematic Survey of the Correlation between Northern HECR Events and SDSS Galaxies
• SDSS J121811.0+465501.2: a new Low Surface Brightness Galaxy with low metallicity
• A Pair of Early- and Late-Forming Galaxy Cluster Samples: a Novel Way of Studying Halo Assembly Bias Assisted by a Constrained Simulation
• The evolution and dependence of the local mass-metallicity relation
• How are Lyman $\alpha$ absorbers in the cosmic web related to gas-rich galaxies?
• The clustering of galaxies with pseudo bulge and classical bulge in the local Universe
• The Galaxy Halo Connection in Modified Gravity Cosmologies: Environment Dependence of Galaxy Luminosity function
• The properties and environment of very young galaxies in the local Universe
• Cosmic Tidal Reconstruction with Halo Fields
• Constraining cosmological parameters using void statistics from the SDSS survey
• The Circular Velocity Function of Group Galaxies
• The galactic spin of AGN galaxies
• Anomalous anisotropic cross-correlations between WMAP CMB maps and SDSS galaxy distribution and implications on the dark flow scenario
• Quantifying galactic morphological transformations in the cluster environment
• Galaxy and halo properties around cosmic filaments from Sloan Digital Sky Survey Data Release 7 and the ELUCID simulation
• The Relative Role of Bars and Environments in AGN Triggering
• Unexpected clustering pattern in dwarf galaxies challenges formation models
• Measuring the growth of structure by matching dark matter haloes to galaxies with VIPERS and SDSS
• The impact of environment on the lives of disk galaxies as revealed by SDSS-IV MaNGA
• On the Constraints of Galaxy Assembly Bias in Velocity Space
• Joint constraints on galaxy bias and ${\sigma }_8$ through the N-pdf of the galaxy number density
• What determines the HI gas content in galaxies?: morphological dependence of the HI gas fraction across M*-SFR plane
• Constraining the optical depth of galaxies and velocity bias with cross-correlation between kinetic Sunyaev-Zeldovich effect and peculiar velocity field
• Stripping of the Hot Gas Halos in Member Galaxies of Abell 1795
• Estimating The Metallicity of Star-forming Early-type Galaxies
• Dependence of galactic bars on the tidal density field in the SDSS
• The Compactness of Galaxy Groups in the Sloan Digital Sky Survey
• Dependence of the ratio of total to visible mass on observable properties of SDSS MaNGA galaxies
• Interactions of galaxies outside clusters and massive groups
• eROSITA-RU Tidal Disruption Events with Keck-I/LRIS: Sample Selection, Optical Properties, and Host Galaxy Demographics
• Searching for Spectroscopic Signatures of Ongoing Quenching in SDSS Galaxies
• The evolution of low-mass central galaxies in the vicinity of massive structures and its impact on the two-halo conformity
• Upcoming searches for decaying dark matter with ULTRASAT ultraviolet maps
• Clustering properties and halo masses for central galaxies in the local Universe
• Shapes and Probabilities of Galaxy Clusters II: Comparisons with observations
• Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation
• Scaling laws in the stellar mass distribution and the transition to homogeneity
• Resolving the Host Galaxy of a Distant Blazar with LBT/LUCI1 + ARGOS
• Clustering of K-band selected local galaxies
• On the Dark Matter Halos of Optical and IR-selected AGN in the Local Universe
• An Improved Photometric Calibration of the Sloan Digital Sky Survey Imaging Data
• Assessment of SDSS-Derived Galaxy Morphologies Using HST Imaging
• BASILISK II. Improved Constraints on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• Measuring the Metallicity of Early-type Galaxies. I. Composite Region
• The breakBRD Breakdown: Using IllustrisTNG to Track the Quenching of an Observationally-Motivated Sample of Centrally Star-Forming Galaxies
• Star formation histories of massive red spiral galaxies in the local universe
• FPFS Shear Estimator: Systematic Tests on the Hyper Suprime-Cam Survey First Year Data
• Bayesian large-scale structure inference: initial conditions and the cosmic web
• Multiwavelength study of nearly face-on low surface brightness disk galaxies
• Structure in Galaxy Distribution. III. Fourier Transforming the Universe
• VISIONS: The VISTA Star Formation Atlas -- II. The data processing pipeline
• A Full Accounting of the Visible Mass in SDSS MaNGA Disk Galaxies
• Observing Correlations Between Dark Matter Accretion and Galaxy Growth: II. Testing the Impact of Galaxy Mass, Star Formation Indicator, and Neighbour Colours
• Nonparametric Inference via Bootstrapping the Debiased Estimator
• Measurement of the evolving galaxy luminosity and mass function using clustering-based redshift inference
• Counts-in-Cells of subhaloes in the IllustrisTNG simulations: the role of baryonic physics
• Counting quasar--radio source pairs to derive the millijansky radio luminosity function and clustering strength to z=3.5
• Does stellar mass assembly history vary with environment?
• Studying the dwarf galaxies in nearby groups of galaxies: spectroscopic and photometric data
• From Halos to Galaxies. X: Decoding Galaxy SEDs with Physical Priors and Accurate Star Formation History Reconstruction
• Cosmological constraints from galaxy multi-tracers in the nearby Universe
• Toward accurate measurement of property-dependent galaxy clustering I. Comparison of the Vmax method and the "shuffled" method
• Constraining $z\lesssim 2$ ultraviolet emission with the upcoming ULTRASAT satellite
• Interpreting deep learning-based stellar mass estimation via causal analysis and mutual information decomposition
• ZTF SN Ia DR2: Exploring SN Ia properties in the vicinity of under-dense environments
• SOMBI: Bayesian identification of parameter relations in unstructured cosmological data
• Star formation properties of galaxy cluster A1767
• Assessing the connection between galactic conformity and assembly-type bias
• An Order Statistics Approach to the Halo Model for Galaxies
• Non-parametric decompositions of disk galaxies in S${}^4$G using DiskFit
• 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
• Two categories of UV-upturn galaxies revealed by semi-analytic models
• LEGA-C stellar populations scaling relations. II: Dissecting mass-complete archaeological trends and their evolution since z~0.7 with LEGA-C and SDSS
• Measuring Mass of Gas in Central Galaxies using weak lensing and satellite kinematics in MOND
• Constraining AGN feedback model with SZ profile
• On the fairness of the main galaxy sample of SDSS
• VST-SMASH: VST Survey of Mass Assembly and Structural Hierarchy I. Survey presentation and deep photometry of IC 5332: tracing the mass assembly in the challenging faintest-end regime
• Particle Physics in the Sky and Astrophysics Underground: Connecting the Universe's Largest and Smallest Scales
• Toward accurate measurement of property-dependent galaxy clustering: II. Tests of the smoothed density-corrected $V_{\max }$ method
• Using the XMM Optical Monitor to Study Cluster Galaxy Evolution
• Panchromatic properties of galaxies in wide-field optical spectroscopic and photometric surveys
• Clustering Property of Wolf-Rayet Galaxies in the SDSS
• Are all post-starbursts mergers? HST reveals hidden disturbances in the majority of PSBs
• The Homogeneous Properties of Halpha-Selected Galaxies at (0.05<z<0.15)
• Hyper Suprime-Cam Y3 results: photo-$z$ bias calibration with lensing shear ratios and cosmological constraints from cosmic shear
• Quiescent Galaxy Size, Velocity Dispersion, and Dynamical Mass Evolution
• The Manticore Project II: Bayesian digital twins of cosmic structure across the SDSS and BOSS volumes
• Quenching Star Formation: Can AGN Do the Trick?
• Radial Distributions of Star Formation and Gas-phase Metallicity in Spiral-Elliptical Galaxy Pairs
• AVOCADO: A Virtual Observatory Census to Address Dwarfs Origins
• A MaNGA about the Legacy I: Connecting the Assembly of Stellar Halo with the Average Star Formation History in Low-Redshift Massive Galaxies
• ELUCID-DESI I: A Parallel MPI Implementation of the Initial Condition Solver for Large-Scale Reconstruction Simulations
• HI Gas and Star Formation in Major Galaxy Pairs from the FAST All-Sky HI Survey (FASHI)
• Passive spiral galaxies deeply captured by Subaru Hyper Suprime-Cam
• A novel Cosmic Filament catalogue from SDSS data
• Large-scale peculiar velocities through the galaxy luminosity function at z ~ 0.1
• IQ Collaboratory III: The Empirical Dust Attenuation Framework -- Taking Hydrodynamical Simulations with a Grain of Dust
• Galaxy and black hole coevolution in dark matter haloes not captured by cosmological simulations
• The Filament Rift: $\Lambda$CDM's Structural Challenge Against Observation
• From the Densest Clusters to the Emptiest Voids: No Evidence For Environmental Effects on the Galaxy Size-Mass Relation at Low Redshift
• SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass
• What best constrains galaxy evolution in the local Universe?
• Toward Understanding the Evolutionary Role of Star-forming Lenticular Galaxies: New HI Detections and Comparison with Quiescent S0s and Red Spirals
• On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback
• Bayesian inference of the initial conditions from large-scale structure surveys