J/ApJ/799/148ivo://CDS.VizieR/J/ApJ/799/148doi:10.26093/cds/vizier.17990148CDSBezanson R.Franx M.van Dokkum P.G.2018-01-05T08:56:17Z2015-07-10T15:18:16ZCDS support team

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

cds-question@unistra.frredshiftedgalaxy-kinematicsgalaxiesspectroscopyScaling relations between galaxy structures and dynamics have been studied extensively for early- and late-type galaxies, both in the local universe and at high redshifts. The abundant differences between the properties of disky and elliptical, or star-forming and quiescent, galaxies seem to be characteristic of the local universe; such clear distinctions begin to disintegrate as observations of massive galaxies probe higher redshifts. In this paper we investigate the existence of the mass fundamental plane of all massive galaxies ({sigma}>~100km/s). This work includes local galaxies (0.05<z<0.07) from the Sloan Digital Sky Survey, in addition to 31 star-forming and 72 quiescent massive galaxies at intermediate redshift (z~0.7) with absorption-line kinematics from deep Keck-DEIMOS spectra and structural parameters from Hubble Space Telescope imaging. In two-parameter scaling relations, star-forming and quiescent galaxies differ structurally and dynamically. However, we show that massive star-forming and quiescent galaxies lie on nearly the same mass fundamental plane, or the relationship between stellar mass surface density, stellar velocity dispersion, and effective radius. The scatter in this relation (measured about log{sigma}) is low: 0.072dex (0.055dex intrinsic) at z~0 and 0.10dex (0.08dex intrinsic) at z~0.7. This 3D surface is not unique: virial relations, with or without a dependence on luminosity profile shapes, can connect galaxy structures and stellar dynamics with similar scatter. This result builds on the recent finding that mass fundamental plane has been stable for early-type galaxies since z~2. As we now find that this also holds for star-forming galaxies to z~0.7, this implies that these scaling relations of galaxies will be minimally susceptible to progenitor biases owing to the evolving stellar populations, structures, and dynamics of galaxies through cosmic time.2015ApJ...799..148Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/799/148CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toB/hst : HST Archived Exposures Catalog (STScI, 2007)II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009)J/ApJS/206/10 : CANDELS multiwavelength catalog (Galametz+, 2013)J/ApJ/777/18 : Stellar mass functions of galaxies to z=4 (Muzzin+, 2013)J/ApJ/775/106 : CANDELS passive & massive early-type galaxies (Cassata+, 2013)J/ApJ/771/85 : Dynamical mass of z~2 quiescent galaxies (van de Sande+, 2013)J/AJ/145/77 : Imaging & spectroscopy in 3 galaxy clusters (Jorgensen+, 2013)J/MNRAS/427/1666 : Massive galaxies in CANDELS-UDS field (Bruce+, 2012)J/ApJS/203/24 : Galaxies structural param. in CANDELS (van der Wel+, 2012)J/ApJS/196/11 : Bulge+disk decompositions of SDSS galaxies (Simard+, 2011)J/ApJ/735/86 : NEWFIRM MBS: photometric catalogs (Whitaker+, 2011)J/ApJ/724/714 : Velocity dispersions of MS1054-03, Coma gal. (Holden+, 2010)J/MNRAS/398/1129 : Central galaxies in groups and clusters (Guo+, 2009)J/ApJS/183/295 : A K-selected catalog of the ECDFS from MUSYC (Taylor+, 2009)J/ApJS/176/1 : Subaru/XMM-Newton deep survey (SXDS). II. (Furusawa+, 2008)J/ApJ/653/1027 : TKRS/GOODS-N Field galaxies (Weiner+, 2006)J/ApJ/638/725 : Fundamental manifold of spheroids (Zaritsky+, 2006)http://www.sdss.org/ : SDSS home pagehttp://www.mpa-garching.mpg.de/SDSS/DR7/ : MPA-JHU DR7 home pagehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/799/148https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/799/148http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/799/148https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/799/148https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/799/148http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/799/148GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/799/148/table1 (DEIMOS z~0.7 sample - Galaxy properties)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/799/148/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/799/148/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/799/148/table1?GETtext/xml+votable180.050000true150.103582.197925830.0055555555555555566/17690 27258https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/799/148?format=asciiOpticaldefaultJ/ApJ/799/148/table1DEIMOS z~0.7 sample - Galaxy propertiesSimbadNameSimbad column added by the CDSmeta.idcharz[0.3/1.1] Redshiftsrc.redshiftfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDIdentifier ({C/U}NNNNN) (1)meta.idcharRAJ2000Right Ascension in decimal degrees (J2000)degpos.eq.ra;meta.mainDEJ2000Declination in decimal degrees (J2000)degpos.eq.dec;meta.mainRe[0.6/15.6] Circularized effective radiuskpcphys.size.radiusfloatn[0.7/6] Sersic index (2)stat.fit.paramfloatFilterFilter used in the observation ("ACS-F814W" or "WFC3-F160W") (2)instr.setup;obscharlogM[9.9/11.6] Log stellar masslog(solMass)phys.massfloatsig.A[85/284] Velocity dispersion measured in the aperturekm/sphys.veloc.dispersioninte_sig.A[3/34] Uncertainty in sigmaAkm/sstat.errorintsig.Re[88/291] Aperture corrected velocity dispersionkm/sphys.veloc.dispersioninte_sig.Re[3/36] Uncertainty in sigmaRekm/sstat.errorinttExp[20400/49200] Exposure timestime.duration;obs.exposureintHCatSources within 1" from the HST-UDS and -COSMOS catalogs (van der Wel+, 2012, J/ApJS/203/24 and Whitaker+, 2011, J/ApJ/735/86)meta.ref.urlintnullableSloanDisplay the online SDSS data for the nearest objectmeta.ref.urlchar