J/ApJ/872/91ivo://CDS.VizieR/J/ApJ/872/91doi:10.26093/cds/vizier.18720091CDSDamjanov I.Zahid H.J.Geller M.J.Utsumi Y.Sohn J.Souchereau H.2020-10-16T12:05:07Z2020-08-26T15:10:54ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frgalaxiesspectroscopygalaxy-classification-systemsinfrared-photometryvisible-astronomyphotometryredshiftedWe explore the relationships between size, stellar mass, and average stellar population age (indicated by D_n_4000 indices) for a sample of ~11000 intermediate-redshift galaxies from the SHELS spectroscopic survey (Geller+ 2014, J/ApJS/213/35) augmented by high-resolution Subaru Telescope Hyper Suprime-Cam imaging. In the redshift interval 0.1<z<0.6, star-forming galaxies are on average larger than their quiescent counterparts. The mass-complete sample of ~3500M_*_>10^10^M_{sun}_ quiescent galaxies shows that the average size of a 10^11^M_{sun}_ quiescent galaxy increases by <~25% from z~0.6 to z~0.1. This growth rate is a function of stellar mass: the most massive (M_*_>10^10^M_{sun}_) galaxies grow significantly more slowly in size than quiescent systems an order of magnitude less massive that grow by 70% in the 0.1<~z<~0.3 redshift interval. For M_*_<10^11^M_{sun}_ galaxies, age and size are anticorrelated at fixed mass; more massive quiescent systems show no significant trend in size with average stellar population age. The evolution in absolute and fractional abundances of quiescent systems at intermediate redshift are also a function of galaxy stellar mass. The suite of evolutionary trends suggests that galaxies more massive than ~10^11^M_{sun}_ have mostly assembled their mass by z~0.6. Quiescent galaxies with lower stellar masses show more complex evolution that is characterized by a combination of individual quiescent galaxy size growth (through mergers) and an increase in the size of newly quenched galaxies joining the population at later times (progenitor bias). The low-mass population (M_*_~10^10^M_{sun}_) grows predominantly as a result of progenitor bias. For more massive (M_*_~5x10^10^M_{sun}_) quiescent galaxies, (predominantly minor) mergers and progenitor bias make more comparable contributions to the size growth. At intermediate redshift, quiescent size growth is mass-dependent; the most massive (M_*_>10^10^M_{sun}_) galaxies experience the least rapid increase in size from z~0.6 to z~0.1.2019ApJ...872...91Dhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/872/91CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toVII/86 : Groups of Galaxies. I. Nearby Groups (Huchra+ 1982)VII/84 : Groups of Galaxies. III. The CfA Survey (Geller+ 1983)II/344 : KiDS-ESO-DR2 multi-band source catalog (de Jong+, 2015)J/ApJ/604/521 : Luminosities & masses of gal. out to z~3 (Trujillo+, 2004)J/MNRAS/382/109 : Massive galaxies in Extended Groth Strip (Trujillo+, 2007)J/MNRAS/398/1129 : Central galaxies in groups and clusters (Guo+, 2009)J/ApJ/720/723 : Compact galaxies in the local universe (Taylor+, 2010)J/AJ/139/1857 : Sample of major galaxy pairs at z=0.08-0.38 (Woods+, 2010)J/ApJ/739/L44 : Structural data for gal. between 0.2<z<2.7 (Damjanov+, 2011)J/ApJ/775/106 : CANDELS passive and massive early-type gal. (Cassata+, 2013)J/A+A/556/A55 : Multi-color photometry of star-forming gal. (Ilbert+, 2013)J/ApJ/777/18 : Stellar mass functions of galaxies to z=4 (Muzzin+, 2013)J/ApJ/762/77 : PM2GC mass-limited sample surface photom. (Poggianti+, 2013)J/ApJ/771/85 : Dynamical masses of z~2 quiescent gal. (van de Sande+, 2013)J/ApJS/213/35 : SHELS: galaxy redshift survey for R<=20.6 (Geller+, 2014)J/ApJS/224/11 : SHELS: redshift survey of the F1 DLS field (Geller+, 2016)J/ApJS/225/27 : 3D-HST Survey: grism spectra master cat. (Momcheva+, 2016)J/ApJ/821/101 : Stellar MFP for massive quiescent z<0.7 gal. (Zahid+, 2016)J/ApJS/234/21 : Hectospec survey of gal. in COSMOS (Damjanov+, 2018)J/ApJ/855/100 : HectoMAP cluster survey. II. X-ray clusters (Sohn+, 2018)J/ApJ/856/172 : The HectoMAP cluster survey. I. (Sohn+, 2018)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/872/91https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/872/91http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/872/91https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/872/91https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/872/91http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/872/91GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/872/91/table1 (Structural properties of F2 DLS field Subaru-HSC galaxies)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/872/91/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/872/91/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/872/91/table1?GETtext/xml+votable180.050000true138.701267330.65196680.0055555555555555565/1241 6/4941 4942 4943 4954 4961 4973 4976 49782.762881831355591e-19 3.3785437584409506e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/872/91?format=asciiOpticalInfrareddefaultJ/ApJ/872/91/table1Structural properties of F2 DLS field Subaru-HSC galaxiesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSHELSSHELS Identifier, DDD.ddddddd+DD.ddddddd (1)meta.id;meta.maincharRmag[13.19/20.6] Deep Lens Survey (DLS) R-band magnitude (1)magphot.mag;em.opt.Rfloate_Rmag[0/9.99] Uncertainty in Rmagmagstat.error;phot.magfloatzspec[0.005/3.41] Spectroscopic redshift (1)src.redshiftdoublee_zspec[0/0.002] Uncertainty in zspecstat.errordoublere[0.005/14] Half-light radiiarcsecphys.size.radiusfloate_re[0.0002/0.8] Uncertainty in rearcsecstat.errorfloatb/a[0.0029/1] Axial ratios b/aphys.size.axisRatiofloate_b/a[0/0.82] Uncertainty in b/astat.errorfloatSloanDisplay the online SDSS data for the nearest objectmeta.ref.urlcharSimbadSimbad column added by the CDSmeta.ref.urlcharNEDNED column added by the CDSmeta.ref.urlchar_RAPositions from SHELS names (right ascension part)degpos.eq.ra;meta.main_DEPositions from SHELS names (declination part)degpos.eq.dec;meta.main