Skip to main content
OSTI.GOVU.S. Department of Energy Office of Scientific and Technical Information
U.S. Department of Energy
Office of Scientific and Technical Information
 

Subaru Hyper Suprime-Cam revisits the large-scale environmental dependence on galaxy morphology over 360 deg2 at z = 0.3–0.6

Journal Article · · Publications of the Astronomical Society of Japan
DOI:https://doi.org/10.1093/pasj/psab097· OSTI ID:1982718
; ; ;

This study investigates the role of large-scale environments on the fraction of spiral galaxies at z = 0.3–0.6 sliced to three redshift bins of Δz = 0.1. Here, we sample 276220 massive galaxies in a limited stellar mass of 5 × 1010 solar mass (~M*) over 360 deg2, as obtained from the Second Public Data Release of the Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP). By combining projected two-dimensional density information (Shimakawa et al. 2021, MNRAS, 503, 3896) and the CAMIRA cluster catalog (Oguri et al. 2018, PASJ, 70, S20), we investigate the spiral fraction across large-scale overdensities and in the vicinity of red sequence clusters. We adopt transfer learning to reduce the cost of labeling spiral galaxies significantly and then perform stacking analysis across the entire field to overcome the limitations of sample size. Here we employ a morphological classification catalog by the Galaxy Zoo Hubble (Willett et al., 2017, MNRAS, 464, 4176) to train the deep learning model. Based on 74103 sources classified as spirals, we find moderate morphology–density relations on a 10 comoving Mpc scale, thanks to the wide-field coverage of HSC-SSP. Clear deficits of spiral galaxies have also been confirmed, in and around 1136 red sequence clusters. Furthermore, we verify whether there is a large-scale environmental dependence on rest-frame u - r colors of spiral galaxies; such a tendency was not observed in our sample.

Research Organization:
US Department of Energy (USDOE), Washington, DC (United States). Office of Science, Sloan Digital Sky Survey (SDSS)
Sponsoring Organization:
USDOE
OSTI ID:
1982718
Journal Information:
Publications of the Astronomical Society of Japan, Vol. 73, Issue 6; ISSN 0004-6264
Publisher:
Astronomical Society of Japan
Country of Publication:
United States
Language:
English

References (125)

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

Similar Records

Subaru Hyper Suprime-Cam revisits the large-scale environmental dependence on galaxy morphology over 360 deg2 at z = 0.3–0.6
Journal Article · 2021 · Publications of the Astronomical Society of Japan · OSTI ID:1826839
+1 more
Passive spiral galaxies deeply captured by Subaru Hyper Suprime-Cam
Journal Article · 2022 · Publications of the Astronomical Society of Japan · OSTI ID:1867980
+4 more
King Ghidorah Supercluster: Mapping the light and dark matter in a new supercluster at z = 0.55 using the subaru hyper suprime-cam
Journal Article · 2022 · Monthly Notices of the Royal Astronomical Society: Letters · OSTI ID:1902179
+1 more

Related Subjects

Astronomy &amp; Astrophysics