J/AJ/145/77ivo://CDS.VizieR/J/AJ/145/77doi:10.26093/cds/vizier.51450077CDSJorgensen I.Chiboucas K.2021-02-10T08:39:05Z2014-05-16T05:57:05ZCDS support team

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

cds-question@unistra.frgalaxy-clustersgalaxiesspectroscopyinfrared-photometryvisible-astronomybroad-band-photometrygalaxy-kinematicsredshiftedhst-photometryWe present an analysis of stellar populations and evolutionary history of galaxies in three similarly rich galaxy clusters MS0451.6-0305 (z=0.54), RXJ0152.7-1357 (z=0.83), and RXJ1226.9+3332 (z=0.89). Our analysis is based on high signal-to-noise ground-based optical spectroscopy and Hubble Space Telescope imaging for a total of 17-34 members in each cluster. Using the dynamical masses together with the effective radii and the velocity dispersions, we find no indication of evolution of sizes or velocity dispersions with redshift at a given galaxy mass. We establish the Fundamental Plane (FP) and scaling relations between absorption line indices and velocity dispersions. We confirm that the FP is steeper at z~0.86 compared to the low-redshift FP, indicating that under the assumption of passive evolution the formation redshift, z_form_, depends on the galaxy velocity dispersion (or alternatively mass). At a velocity dispersion of {sigma}=125km/s (Mass=10^10.55^M_{sun}_) we find z_form_=1.24+/-0.05, while at {sigma}=225km/s (Mass=10^11.36^M_{sun}_) the formation redshift is z_form_=1.95^+0.3^_-0.2_, for a Salpeter initial mass function. The three clusters follow similar scaling relations between absorption line indices and velocity dispersions as those found for low-redshift galaxies. The zero point offsets for the Balmer lines depend on cluster redshifts. However, the offsets indicate a slower evolution, and therefore higher formation redshift, than the zero point differences found from the FP, if interpreting the data using a passive evolution model. Specifically, the strength of the higher order Balmer lines H{delta} and H{gamma} implies z_form_>2.8. The scaling relations for the metal indices in general show small and in some cases insignificant zero point offsets, favoring high formation redshifts for a passive evolution model.2013AJ....145...77Jhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/145/77CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toV/139 : The SDSS Photometric Catalog, Release 9 (Adelman-McCarthy+, 2012)J/ApJ/725/1252 : Confirmed members of RX J0152.7-1357 (Demarco+, 2010)J/ApJ/724/714 : Velocity dispersions of MS1054-03 & Coma gal. (Holden+, 2010)J/ApJS/184/271 : Photometry of galaxies in 3 clusters (Chiboucas+, 2009)J/ApJ/671/1503 : Cl 0024+16 and MS 0451-03 spectrophotometry (Moran+, 2007)J/ApJ/665/1067 : Velocities in Cl 0024+16 and MS 0451-03 (Moran+, 2007)J/AJ/130/445 : X-ray-luminous galaxy cluster RX J0142.0+2131 Barr+, 2005)J/AJ/127/2455 : Gemini Deep Deep Survey (GDDS) (Abraham+, 2004)J/ApJ/498/195 : Spectroscopic survey of CL 1358+62 (Fisher+ 1998)J/MNRAS/273/1097 : CCD photometry for E and S0 galaxies (Jorgensen+ 1995)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/145/77https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/145/77http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/145/77https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/145/77https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/145/77http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/145/77GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/AJ/145/77/MS0451 (Combined table from original tables)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/145/77/MS0451?https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/145/77/MS0451?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/145/77/MS0451?GETtext/xml+votable180.050000true73.552625-3.05561110.005555555555555556Cone search capability for table J/AJ/145/77/RXJ1226 (Combined table from original tables)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/145/77/RXJ1226?https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/145/77/RXJ1226?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/145/77/RXJ1226?GETtext/xml+votable180.050000true186.77837533.59158330.0055555555555555566/22915 285352.040811542443644e-19 4.653515163505597e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/145/77?format=asciiOpticalInfrareddefaultJ/AJ/145/77/MS0451Combined table from original tablesnSerSersic indexstat.fit.paramfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintGalaxy[12/3906] Galaxy ID numbermeta.id;meta.mainintRAJ2000Hour of Right Ascension (J2000) (G1)pos.eq.ra;meta.mainDEJ2000Degree of Declination (J2000) (G1)pos.eq.dec;meta.maing'mag? SDSS g'-band total magnitude (only for Table13) (G2)magphot.mag;em.opt.Bfloatnullabler'magSDSS r'-band total magnitude (G2)magphot.mag;em.opt.Rfloati'magSDSS i'-band total magnitude (G2)magphot.mag;em.opt.Ifloatz'magSDSS z'-band total magnitude (G2)magphot.mag;em.opt.Ifloatg'-r'? SDSS g'-r' color index (only for Table13) (G2)magphot.color;em.opt.B;em.opt.Rfloatnullabler'-i'SDSS r'-i' color index (G2)magphot.color;em.opt.R;em.opt.Ifloati'-z'SDSS i'-z' color index (G2)magphot.color;em.opt.I;em.opt.Ifloatmag1Total magnitude m_tot,dev_ (1)magphot.mag;em.optfloatReff1Log of the effective radius logr_e,dev_ (1)log(arcsec)phys.angSizefloat<mu1>Mean surface brightness within the effective radius <{mu}>_e,dev_ (1)mag.arcsec**-2phot.mag.sbfloatmag2Total magnitude m_tot,ser_ (2)magphot.mag;em.optfloatReff2Log of the effective radius logr_e,ser_ (2)log(arcsec)phys.angSizefloat<mu2>Mean surface brightness within the effective radius <{mu}>_e,ser_ (2)mag.arcsec**-2phot.mag.sbfloatPA[-85.5/85.9] Position angle of the major axis measured from North through Eastdegpos.posAngfloatEllEllipticitysrc.ellipticityfloatzRedshiftsrc.redshiftfloatMadopted Membership (1=galaxy is a member of the cluster; 0=galaxy is not a member)meta.code.membercharsigma1? Log of velocity dispersion log{sigma} (3)log(km.s**-1)phys.veloc.dispersionfloatnullablee_sigma1? {sigma} uncertainty in sigma1log(km.s**-1)stat.errorfloatnullablesigma2? Log of velocity dispersion log{sigma}_cor_ (4)log(km.s**-1)phys.veloc.dispersionfloatnullableB8V? Fraction of the template star of spectral type B8V in the spectrastatfloatnullableG1V? Fraction of the template star of spectral type G1V in the spectrastatfloatnullableK0III? Fraction of the template star of spectral type K0III in the spectrastatfloatnullablechi2? {chi}^2^stat.fit.chi2floatnullableS/N? Signal-to-noise ratio per {AA} in the rest frame of the galaxy (5)stat.snr;src.class.starGalaxyfloatnullableCN3883? The CN3883 line index (7)magspect.indexfloatnullablee_CN3883? Uncertainty in CN3883 (8)magstat.errorfloatnullableCaHK? The CaHK line index; in {AA} (7)0.1nmspect.indexfloatnullablee_CaHK? Uncertainty in CaHK; in {AA} (8)0.1nmstat.errorfloatnullableD4000? The D4000 line index (7)spect.index;spect.linefloatnullablee_D4000? Uncertainty in D4000 (8)stat.errorfloatnullableHdA? The H{delta}_A_ line index; in {AA} (7)0.1nmspect.indexfloatnullablee_HdA? Uncertainty in HdA; in {AA} (8)0.1nmstat.errorfloatnullableCN1? The CN_1_ line index (7)magspect.index;spect.linefloatnullablee_CN1? Uncertainty in CN1 (8)magstat.errorfloatnullableCN2? The CN_2_ line index (7)magspect.index;spect.linefloatnullablee_CN2? Uncertainty in CN2 (8)magstat.errorfloatnullableG4300? The G4300 line index; in {AA} (7)0.1nmspect.line.eqWidthfloatnullablee_G4300? Uncertainty in G4300; in {AA} (8)0.1nmstat.errorfloatnullableHgA? The H{gamma}_A_ line index; in {AA} (7)0.1nmspect.index;em.line.Hgammafloatnullablee_HgA? Uncertainty in HgA; in {AA} (8)0.1nmstat.errorfloatnullableFe4383? The Fe4383 line index; in {AA} (7)0.1nmspect.line.eqWidthfloatnullablee_Fe4383? Uncertainty in Fe4383; in {AA} (8)0.1nmstat.errorfloatnullableC4668? The C4668 line index; in {AA} (7)0.1nmspect.indexfloatnullablee_C4668? Uncertainty in C4668; in {AA} (8)0.1nmstat.errorfloatnullableHb? The H{beta} line index; in {AA} (7)0.1nmspect.line.eqWidthfloatnullablee_Hb? Uncertainty in Hb; in {AA} (8)0.1nmstat.errorfloatnullableHbG? The H{beta}_G_ line index; in {AA} (7)0.1nmspect.index;em.line.Hbetafloatnullablee_HbG? Uncertainty in HbG; in {AA} (8)0.1nmstat.errorfloatnullableMgb? The Mgb line index; in {AA} (7)0.1nmspect.line.eqWidthfloatnullablee_Mgb? Uncertainty in Mgb; in {AA} (8)0.1nmstat.errorfloatnullableFe5270? The Fe5270 line index; in {AA} (7)0.1nmspect.line.eqWidthfloatnullablee_Fe5270? Uncertainty in Fe5270; in {AA} (8)0.1nmstat.errorfloatnullableFe5335? The Fe5335 line index; in {AA} (7)0.1nmspect.line.eqWidthfloatnullablee_Fe5335? Uncertainty in Fe5335; in {AA} (8)0.1nmstat.errorfloatnullableEW? [OII] equivalent width (7)0.1nmspect.line.eqWidthfloatnullablee_EW? Uncertainty in EW; in {AA} (8)0.1nmstat.error;spect.line.eqWidthfloatnullableJ/AJ/145/77/RXJ1226Combined table from original tablesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintGalaxy[12/3906] Galaxy ID numbermeta.id;meta.mainintf_Galaxy[b] Listed at the same position as the galaxies are superimposed, as seen by two overlapping spectra in the slit (only for Table14)meta.codecharRAJ2000Hour of Right Ascension (J2000) (G1)pos.eq.ra;meta.mainDEJ2000Degree of Declination (J2000) (G1)pos.eq.dec;meta.mainr'magSDSS r'-band total magnitude (G2)magphot.mag;em.opt.Rfloati'magSDSS i'-band total magnitude (G2)magphot.mag;em.opt.Ifloatz'magSDSS z'-band total magnitude (G2)magphot.mag;em.opt.Ifloatr'-i'SDSS r'-i' color index (G2)magphot.color;em.opt.R;em.opt.Ifloati'-z'SDSS i'-z' color index (G2)magphot.color;em.opt.I;em.opt.IfloatzRedshiftsrc.redshiftfloatMadopted Membership (1=galaxy is a member of the cluster; 0=galaxy is not a member)meta.code.membercharsigma1? Log of velocity dispersion log{sigma} (3)log(km.s**-1)phys.veloc.dispersionfloatnullablee_sigma1? {sigma} uncertainty in sigma1log(km.s**-1)stat.errorfloatnullablesigma2? Log of velocity dispersion log{sigma}_cor_ (4)log(km.s**-1)phys.veloc.dispersionfloatnullableB8V? Fraction of the template star of spectral type B8V in the spectrastatfloatnullableG1V? Fraction of the template star of spectral type G1V in the spectrastatfloatnullableK0III? Fraction of the template star of spectral type K0III in the spectrastatfloatnullablechi2? {chi}^2^stat.fit.chi2floatnullableS/N? Signal-to-noise ratio per {AA} in the rest frame of the galaxy (5)stat.snr;src.class.starGalaxyfloatnullableRefReference for data (only for Table23) (6)meta.ref;pos.framecharCN3883? The CN3883 line index (7)magspect.indexfloatnullablee_CN3883? Uncertainty in CN3883 (8)magstat.errorfloatnullableCaHK? The CaHK line index; in {AA} (7)0.1nmspect.indexfloatnullablee_CaHK? Uncertainty in CaHK; in {AA} (8)0.1nmstat.errorfloatnullableD4000? The D4000 line index (7)spect.index;spect.linefloatnullablee_D4000? Uncertainty in D4000 (8)stat.errorfloatnullableHdA? The H{delta}_A_ line index; in {AA} (7)0.1nmspect.indexfloatnullablee_HdA? Uncertainty in HdA; in {AA} (8)0.1nmstat.errorfloatnullableCN1? The CN_1_ line index (7)magspect.index;spect.linefloatnullablee_CN1? Uncertainty in CN1 (8)magstat.errorfloatnullableCN2? The CN_2_ line index (7)magspect.index;spect.linefloatnullablee_CN2? Uncertainty in CN2 (8)magstat.errorfloatnullableG4300? The G4300 line index; in {AA} (7)0.1nmspect.line.eqWidthfloatnullablee_G4300? Uncertainty in G4300; in {AA} (8)0.1nmstat.errorfloatnullableHgA? The H{gamma}_A_ line index; in {AA} (7)0.1nmspect.index;em.line.Hgammafloatnullablee_HgA? Uncertainty in HgA; in {AA} (8)0.1nmstat.errorfloatnullableFe4383? The Fe4383 line index; in {AA} (7)0.1nmspect.line.eqWidthfloatnullablee_Fe4383? Uncertainty in Fe4383; in {AA} (8)0.1nmstat.errorfloatnullableC4668? The C4668 line index; in {AA} (7)0.1nmspect.indexfloatnullablee_C4668? Uncertainty in C4668; in {AA} (8)0.1nmstat.errorfloatnullableEW? [OII] equivalent width (7)0.1nmspect.line.eqWidthfloatnullablee_EW? Uncertainty in EW; in {AA} (8)0.1nmstat.error;spect.line.eqWidthfloatnullableJ/AJ/145/77/table3GMOS-N observationsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintClusterCluster namemeta.ref;pos.framecharprimaryProgramProgram identifiermeta.id;obscharDateUT datetime.epochcharDTypeData typemeta.codecharf_PType[a] Director's Discretionary timemeta.codecharPTypeProgram typeinstr.setupcharJ/AJ/145/77/table4GMOS-N imaging datarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintClusterCluster namemeta.ref;pos.framecharprimaryProgramProgram identifier(s)meta.id;obscharFiltFilter used (g', r', i', or z')instr.setup;instr.filtercharN1Number of exposuremeta.numberintExp1Exposure timestime.duration;obs.exposureintn_Exp1Note on exposuremeta.notecharN2? Number of exposuremeta.numberintnullableExp2? Exposure timestime.duration;obs.exposureintnullablen_Exp2Note on exposuremeta.notecharFWHMFull Width at Half Maximum (1)arcsecspect.line.widthfloatSBSky brightnessmag.arcsec**-2phot.mag.sbfloatAgGalactic extinctionmagphys.absorption.galfloatJ/AJ/145/77/table5GMOS-N spectroscopic datarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintClusterCluster namemeta.ref;pos.framecharprimaryProgramProgram identifier(s)meta.id;obscharExp1Exposure timestime.duration;obs.exposureintExp2? Second exposure timestime.duration;obs.exposureintnullableNNumber of individual exposuresmeta.numberintf_N[f] A fifth exposure was taken but contains no significant signal from the science targetsmeta.codecharFWHMFull Width at Half Maximum (1)arcsecspect.line.widthfloatResMedian instrumental resolution; in {AA} (2)0.1nmspect.resolutionfloatRes2The equivalent resolution in km/s at 4300{AA} in the rest frame of the clusterskm/sspect.resolutionintWidthSlit width (3)arcsecspect.line.widthfloatLengthExtraction length (3)arcsecphys.angSizefloatRadRadius in an equivalent circular aperture (4)arcsecstat.fit.paramfloatLength0Slit length (beginning)arcsecinstr.setupfloatLength1? Slit length (end)arcsecinstr.setupfloatnullableS/NSignal-to-noise ratio (5)stat.snrintJ/AJ/145/77/table7HST/ACS imaging datarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintClusterCluster namemeta.ref;pos.framecharprimaryNNumber of fieldsmeta.numberintFiltFilter (F814W, F775W, or F814W)meta.id;instr.filtercharExpTotal exposure timestime.duration;obs.exposureintProgramProgram identifier (9836, 9290, or 9033)meta.id;obsintSimbadSimbad column added by the CDSmeta.ref.urlchar