J/ApJ/929/61ivo://CDS.VizieR/J/ApJ/929/61doi:10.26093/cds/vizier.19290061CDSDamjanov I.Sohn J.Utsumi Y.Geller M.J.Dell'Antonio I.2024-11-06T20:25:03Z2024-04-09T09:38:33ZCDS support team

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

cds-question@unistra.frgalaxiescatalogsvisible-astronomyspectroscopysloan-photometryredshiftedgalaxy-kinematicssurveysWe use surveys covering the redshift range 0.05<z<3.8 to explore quiescent galaxy scaling relations and the redshift evolution of the velocity dispersion, size, and dynamical mass at fixed stellar mass. For redshift z<0.6, we derive mass-limited samples and demonstrate that these large samples enhance constraints on the evolution of the quiescent population. The constraints include 2985 new velocity dispersions from the SHELS F2 survey. In contrast with the known substantial evolution of size with redshift, evolution in the velocity dispersion is negligible. The dynamical-to-stellar-mass ratio increases significantly as the universe ages, in agreement with recent results that combine high-redshift data with the Sloan Digital Sky Survey. Like other investigators, we interpret this result as an indication that the dark matter fraction within the effective radius increases as a result of the impact of the minor mergers that are responsible for size growth. We emphasize that dense redshift surveys covering the range 0.07<z<1 along with strong and weak lensing measurements could remove many ambiguities in evolutionary studies of the quiescent population.2022ApJ...929...61Dhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/929/61CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toII/282 : The SDSS Photometric Catalog, Release 6 (Adelman-McCarthy+, 2007)II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009)V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16) (Ahumada+, 2020)J/MNRAS/371/703 : MILES library of empirical spectra (Sanchez-Blazquez+, 2006)J/ApJS/172/615 : GALFIT result for GEMS galaxies (Haussler+, 2007)J/MNRAS/382/109 : Massive galaxies in Extended Groth Strip (Trujillo+, 2007)J/A+A/524/A6 : Evolution of spectral early-type galaxies (Saglia+, 2010)J/ApJ/739/L44 : Structural data for gal. between 0.2<z<2.7 (Damjanov+, 2011)J/ApJS/196/11 : Bulge+disk decompositions of SDSS galaxies (Simard+, 2011)J/ApJ/775/106 : CANDELS passive and massive early-type gal. (Cassata+, 2013)J/ApJ/771/85 : Dynamical masses of z~2 quiescent gal. (van de Sande+, 2013)J/MNRAS/441/203 : Massive quiescent ETG in clusters (Delaye+ 2014)J/ApJS/213/35 : SHELS: complete galaxy redshift survey (Geller+, 2014)J/ApJ/821/101 : Stellar MFP for massive quiescent z<0.7 gal. (Zahid+, 2016)J/ApJS/229/20 : MMT/Hectospec redshift survey for Abell 2029 (Sohn+, 2017)J/ApJS/234/21 : Hectospec survey of galaxies in COSMOS (Damjanov+, 2018)J/ApJ/872/91 : SHELS galaxy sizes using Subaru/HSC (Damjanov+, 2019)J/ApJ/905/170 : Mass-based structural param. for 3D-HST gal. (Mosleh+, 2020)J/ApJ/902/17 : Sp. of quiescent gal. in 9 lensing clusters (Sohn+, 2020)J/ApJ/909/129 : HectoMAP redshift survey DR1 (Sohn+, 2021)J/MNRAS/501/1028 : Galaxies at z=1-3 lensed by six HFF clusters (Yang+, 2021)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/929/61https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/929/61http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/929/61https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/929/61https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/929/61http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/929/61GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/929/61/table2 (*The Smithsonian Hectospec Lensing Survey (SHELS) F2 sample)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/929/61/table2?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/929/61/table2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/929/61/table2?GETtext/xml+votable180.050000true138.70035530.736426940.0055555555555555565/1241 6/4941-4943 4954 4961 4973 4976 4978https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/929/61?format=asciiOpticaldefaultJ/ApJ/929/61/table2*The Smithsonian Hectospec Lensing Survey (SHELS) F2 samplerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintobjIDSDSS objIDmeta.id;meta.mainprimaryRAJ2000[138.7/141.1] Right Ascension (J2000)degpos.eq.ra;meta.mainindexedDEJ2000[28.8/31.1] Declination (J2000)degpos.eq.dec;meta.mainindexedrmag[12.6/20.8] Extinction-corrected SDSS r-band Petrosian magnitudemagphot.mag;em.opt.Rfloate_rmag[0.002/36.2] Mean error for rmagmagstat.error;phot.magfloatz[0.013/3.41] Redshiftsrc.redshiftdoublee_z[1e-5/0.002] Mean error for zstat.error;src.redshiftdoubledn4000[0.3/16394] The D_n_4000 spectral indexspect.indexdoublee_dn4000[0/924]? Mean error for dn4000 (1)stat.errorfloatnullablelogMass[7/13] Log of the stellar masslog(solMass)phys.massfloatE_logMass[0.009/1] Upper error limit for logMasslog(solMass)stat.error;stat.maxfloate_logMass[0.009/1.1] Lower error limit for logMasslog(solMass)stat.error;phys.massfloatQDisplay the quiescent sample data (link to Table 3)meta.ref.urlcharSHELSDisplay data from Geller+ 2014, J/ApJS/213/35meta.ref.urlcharSloanDisplay the SDSS-DR17 data for this objectmeta.ref.urlcharSimbadNameSimbad column added by the CDSmeta.idcharnullableJ/ApJ/929/61/table3SHELS F2 quiescent samplerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRe[1/51.3] Circularized half-light radius (1)kpcphys.size.radiusfloate_Re[0.002/1] Mean error for Rekpcstat.errorfloatb/a[0.05/1] Axis ratio (2)phys.angSize;arith.ratiofloatobjIDSDSS objIDmeta.id;meta.maine_b/a[0.0001/0.05] Mean error for b/astat.errorfloatn[0.3/6] Sersic indexstat.fit.paramfloate_n[0/0.7] Mean error for nstat.errorfloatsigma[/592]? Velocity dispersion within 3kpc (3)km/sphys.veloc.dispersionfloatnullablee_sigma[/17343]? Mean error for sigmakm/sstat.errorfloatnullableMLS[0/1] Inclusion in the stellar mass limited sample; 1=YESmeta.codeint