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April 2018 |
Second data release of the Hyper Suprime-Cam Subaru Strategic Program
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October 2019 |
The color-absolute magnitude relation for E and S0 galaxies. I - Calibration and tests for universality using Virgo and eight other nearby clusters
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August 1977 |
Deep learning
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May 2015 |
The Prism Multi-Object Survey (Primus). i. Survey Overview and Characteristics
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October 2011 |
The COSMOS2015 galaxy stellar mass function: Thirteen billion years of stellar mass assembly in ten snapshots⋆
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September 2017 |
The green valley is a red herring: Galaxy Zoo reveals two evolutionary pathways towards quenching of star formation in early- and late-type galaxies★
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March 2014 |
Secondary standard stars for absolute spectrophotometry
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March 1983 |
The STAGES view of red spirals and dusty red galaxies: mass-dependent quenching of star formation in cluster infall
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March 2009 |
Galaxy Zoo: morphological classifications for 120 000 galaxies in HST legacy imaging
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October 2016 |
The Evolution of the Star Formation Activity in Galaxies and Its Dependence on Environment
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May 2006 |
The ATLAS3D project - VII. A new look at the morphology of nearby galaxies: the kinematic morphology-density relation: The ATLAS3D project - VII. Morphology-density
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August 2011 |
How does galaxy environment matter? The relationship between galaxy environments, colour and stellar mass at 0.4 < z < 1 in the Palomar/DEEP2 survey: How does galaxy environment matter?
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December 2010 |
The evolution of disk galaxies and the origin of S0 galaxies
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April 1980 |
The DEEP2 galaxy redshift survey: evolution of the colour–density relation at 0.4 < z < 1.35
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March 2007 |
The bright-star masks for the HSC-SSP survey
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July 2017 |
Galaxy morphology in rich clusters - Implications for the formation and evolution of galaxies
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March 1980 |
The VIMOS VLT Deep Survey final data release: a spectroscopic sample of 35 016 galaxies and AGN out to z ~ 6.7 selected with 17.5 ≤ i AB ≤ 24.75
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October 2013 |
Galaxy And Mass Assembly (GAMA): end of survey report and data release 2
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July 2015 |
The colour-magnitude relation as a constraint on the formation of rich cluster galaxies
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October 1998 |
Physical Properties and Environments of Nearby Galaxies
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September 2009 |
Morphological Transformation from Galaxy Harassment
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March 1998 |
Fast and slow rotators in the densest environments: a SWIFT IFS study of the Coma cluster
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September 2013 |
Extragalactic science, cosmology, and Galactic archaeology with the Subaru Prime Focus Spectrograph
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February 2014 |
The Red‐Sequence Cluster Survey. I. The Survey and Cluster Catalogs for Patches RCS 0926+37 and RCS 1327+29
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March 2005 |
GALAXY STELLAR MASS ASSEMBLY BETWEEN 0.2 < z < 2 FROM THE S-COSMOS SURVEY
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January 2010 |
The Bimodal Galaxy Color Distribution: Dependence on Luminosity and Environment
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September 2004 |
Quenched fractions in the IllustrisTNG simulations: the roles of AGN feedback, environment, and pre-processing
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October 2020 |
The Morphology‐Density Relation in z ∼ 1 Clusters
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April 2005 |
Photometric Redshift with Bayesian Priors on Physical Properties of Galaxies
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February 2015 |
THE COSMOS2015 CATALOG: EXPLORING THE 1 < z < 6 UNIVERSE WITH HALF A MILLION GALAXIES
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June 2016 |
The Cosmic Evolution Survey (COSMOS): A Large‐Scale Structure at z = 0.73 and the Relation of Galaxy Morphologies to Local Environment
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September 2007 |
Galaxy morphology classification with deep convolutional neural networks
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April 2019 |
Mass Selection and the Evolution of the Morphology‐Density Relation from z = 0.8 to 0
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November 2007 |
The WiggleZ Dark Energy Survey: survey design and first data release
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January 2010 |
Galaxy formation through hierarchical clustering
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September 1991 |
The colour-magnitude relation for galaxies in the Coma cluster
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October 2001 |
Galactic Stellar and Substellar Initial Mass Function
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July 2003 |
Galaxy Zoo: disentangling the environmental dependence of morphology and colour
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October 2009 |
Preparing Red‐Green‐Blue Images from CCD Data
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Publications of the Astronomical Society of the Pacific, Vol. 116, Issue 816
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February 2004 |
A cluster finding algorithm based on the multiband identification of red sequence galaxies
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August 2014 |
First results on the cluster galaxy population from the Subaru Hyper Suprime-Cam survey. II. Faint end color–magnitude diagrams and radial profiles of red and blue galaxies at 0.1 < z < 1.1
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October 2017 |
The Cosmic Evolution Survey (COSMOS): Overview
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September 2007 |
Subaru Hyper Suprime-Cam excavates colossal over- and underdense structures over 360 deg2 out to z = 1
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March 2021 |
The SAMI Pilot Survey: the kinematic morphology–density relation in Abell 85, Abell 168 and Abell 2399
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July 2014 |
Do star formation rates of galaxy clusters depend on mass? Blue/late-type fractions and total star formation rates of 115 galaxy clusters as a function of cluster virial mass: Do SFRs of galaxy clusters depend on mass?
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December 2004 |
Hyper Suprime-Cam: Camera dewar design
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September 2017 |
Optimizing automatic morphological classification of galaxies with machine learning and deep learning using Dark Energy Survey imaging
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February 2020 |
Mass and Environment as Drivers of Galaxy Evolution. ii. the Quenching of Satellite Galaxies as the Origin of Environmental Effects
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August 2012 |
Photometric redshifts for Hyper Suprime-Cam Subaru Strategic Program Data Release 1
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October 2017 |
Environmental Effects on Late‐Type Galaxies in Nearby Clusters
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April 2006 |
Matplotlib: A 2D Graphics Environment
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January 2007 |
Gradient-based learning applied to document recognition
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January 1998 |
A Modified Magnitude System that Produces Well-Behaved Magnitudes, Colors, and Errors Even for Low Signal-to-Noise Ratio Measurements
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September 1999 |
NINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE ( WMAP ) OBSERVATIONS: COSMOLOGICAL PARAMETER RESULTS
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September 2013 |
Spin parity of spiral galaxies II: a catalogue of 80 k spiral galaxies using big data from the Subaru Hyper Suprime-Cam survey and deep learning
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July 2020 |
The build-up of the colour-magnitude relation as a function of environment
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September 2005 |
The SAMI Galaxy Survey: Mass as the Driver of the Kinematic Morphology–Density Relation in Clusters
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July 2017 |
The X-CLASS survey: A catalogue of 1646 X-ray-selected galaxy clusters up to z ∼ 1.5
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August 2021 |
Galaxy stellar mass functions of different morphological types in clusters, and their evolution between z= 0.8 and 0: Galaxy stellar mass functions and morphologies
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February 2011 |
SDSS-IV MaNGA: Probing the Kinematic Morphology–Density Relation of Early-type Galaxies with MaNGA
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December 2017 |
The morphology-density relation in the Sloan Digital Sky Survey: Morphology-density relation in the SDSS
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November 2003 |
The MASSIVE Survey – VII. The relationship of angular momentum, stellar mass and environment of early-type galaxies
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June 2017 |
MOONS: the Multi-Object Optical and Near-infrared Spectrograph for the VLT
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July 2014 |
The VIMOS Public Extragalactic Survey (VIPERS): First Data Release of 57 204 spectroscopic measurements
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January 2014 |
The Evolution of Dusty Star Formation and Stellar Mass Assembly in Clusters: Results from the IRAC 3.6, 4.5, 5.8, and 8.0 μm Cluster Luminosity Functions
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October 2008 |
Using transfer learning to detect galaxy mergers
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May 2018 |
The 13th Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-IV Survey Mapping Nearby Galaxies at Apache Point Observatory
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December 2017 |
The Environment of Passive Spiral Galaxies in the SDSS
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August 2003 |
The evolution of large-scale structure in a universe dominated by cold dark matter
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May 1985 |
The on-site quality-assurance system for Hyper Suprime-Cam: OSQAH†
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September 2017 |
A new classification system for galaxies
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June 1976 |
The evolution of galaxies in clusters. V - A study of populations since Z approximately equal to 0.5
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October 1984 |
The Effects of Environment on Morphological Evolution at 0 < z < 1.2 in the COSMOS Survey
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September 2007 |
The environmental dependence of the relations between stellar mass, structure, star formation and nuclear activity in galaxies: Galaxy structure, star formation and nuclear activity
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August 2004 |
Galaxy evolution in groups and clusters: star formation rates, red sequence fractions and the persistent bimodality: Galaxy evolution in groups and clusters
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May 2012 |
The Evolution of Spiral, s0, and Elliptical Galaxies in Clusters
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May 2009 |
The Hyper Suprime-Cam software pipeline
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October 2017 |
Disc colours in field and cluster spiral galaxies at 0.5 ≲ z ≲ 0.8
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April 2016 |
Prime Focus Spectrograph (PFS) for the Subaru telescope: overview, recent progress, and future perspectives
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conference
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August 2016 |
Galaxy bimodality versus stellar mass and environment
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December 2006 |
redMaPPer. I. ALGORITHM AND SDSS DR8 CATALOG
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April 2014 |
THE PHASE SPACE AND STELLAR POPULATIONS OF CLUSTER GALAXIES AT z ∼ 1: SIMULTANEOUS CONSTRAINTS ON THE LOCATION AND TIMESCALE OF SATELLITE QUENCHING
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November 2014 |
Galaxy Zoo: reproducing galaxy morphologies via machine learning★: Galaxy Zoo: morphology via machine learning
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April 2010 |
Precision photometry of early-type galaxies in the Coma and Virgo clusters: a test of the universality of the colour-magnitude relation - II. Analysis
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February 1992 |
Evolution of the colour-radius and morphology-radius relations in SDSS galaxy clusters
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February 2004 |
The Eleventh and Twelfth data Releases of the Sloan Digital sky Survey: Final data from Sdss-Iii
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July 2015 |
Hyper Suprime-Cam: Filters
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June 2018 |
The first appearance of the red sequence of galaxies in proto-clusters at 2 lsimzlsim 3
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June 2007 |
A young galaxy cluster in the old Universe
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August 2019 |
Morphology-dependent trends of galaxy age with environment in A 901/2 seen with COMBO-17
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March 2007 |
Galaxy Zoo: the dependence of morphology and colour on environment
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March 2009 |
MASS AND ENVIRONMENT AS DRIVERS OF GALAXY EVOLUTION IN SDSS AND zCOSMOS AND THE ORIGIN OF THE SCHECHTER FUNCTION
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August 2010 |
The Dependence of Galaxy Morphology and Structure on Environment and Stellar Mass
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January 2008 |
Morphological Studies of the Galaxy Populations in Distant “Butcher‐Oemler” Clusters with the Hubble Space Telescope . II. AC 103, AC 118, and AC 114 at z = 0.31
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April 1998 |
Evolution since z = 0.5 of the Morphology‐Density Relation for Clusters of Galaxies
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December 1997 |
How do galaxies get their gas?
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October 2005 |
Environments of galaxies in groups within the supercluster-void network
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September 2012 |
The fate of disc galaxies in IllustrisTNG clusters
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June 2020 |
The GOGREEN survey: the environmental dependence of the star-forming galaxy main sequence at 1.0 < z < 1.5
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March 2020 |
Astropy: A community Python package for astronomy
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September 2013 |
THE zCOSMOS 10k-BRIGHT SPECTROSCOPIC SAMPLE
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September 2009 |
Rotation-invariant convolutional neural networks for galaxy morphology prediction
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April 2015 |
The Prism Multi-Object Survey (Primus). ii. data Reduction and Redshift Fitting
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April 2013 |
A Wide‐Field Survey of Two z ∼ 0.5 Galaxy Clusters: Identifying the Physical Processes Responsible for the Observed Transformation of Spirals into S0s
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December 2007 |
THE 10k zCOSMOS: MORPHOLOGICAL TRANSFORMATION OF GALAXIES IN THE GROUP ENVIRONMENT SINCE z ∼1
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June 2010 |
The COSMOS Survey: Hubble Space Telescope Advanced Camera for Surveys Observations and Data Processing
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September 2007 |
Integrated Colors of Bright Galaxies in the u, b, V System.
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November 1960 |
EVOLUTION OF THE COLOR-MAGNITUDE RELATION IN GALAXY CLUSTERS AT z ∼ 1 FROM THE ACS INTERMEDIATE REDSHIFT CLUSTER SURVEY
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December 2008 |
Galaxy Morphology Network: A Convolutional Neural Network Used to Study Morphology and Quenching in ∼100,000 SDSS and ∼20,000 CANDELS Galaxies
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June 2020 |
Array programming with NumPy
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September 2020 |
Galaxy And Mass Assembly (GAMA): trends in galaxy colours, morphology, and stellar populations with large-scale structure, group, and pair environments
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June 2015 |
Galaxy evolution in groups and clusters: satellite star formation histories and quenching time-scales in a hierarchical Universe
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April 2013 |
A Computer-Generated Visual Morphology Catalog of ∼3,000,000 sdss Galaxies
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April 2016 |
EDisCS – the ESO distant cluster survey: Sample definition and optical photometry
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November 2005 |
The origin of dwarf galaxies, cold dark matter, and biased galaxy formation
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April 1986 |
The zCOSMOS redshift survey: the role of environment and stellar mass in shaping the rise of the morphology-density relation from z ~ 1
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June 2009 |
Evolution since z = 1 of the Morphology‐Density Relation for Galaxies
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February 2005 |
"Tuning Fork" Classification of Rich Clusters of Galaxies
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February 1971 |
The Second Data Release of the Sloan Digital Sky Survey
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July 2004 |
Transformation from spirals into S0s with bulge growth in groups of galaxies: Formation of S0 galaxies
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June 2011 |
Physical Models of Galaxy Formation in a Cosmological Framework
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August 2015 |
4MOST: 4-metre multi-object spectroscopic telescope
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October 2012 |
amico galaxy clusters in KiDS-DR3: sample properties and selection function
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January 2019 |
Transfer learning for galaxy morphology from one survey to another
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December 2018 |