J/ApJS/206/8ivo://CDS.VizieR/J/ApJS/206/8doi:10.26093/cds/vizier.22060008CDSMuzzin A.Marchesini D.Stefanon M.Franx M.Milvang-Jensen B.,Dunlop J.S.Fynbo J.P.U.Brammer G.Labbe I.van Dokkum P.2018-05-29T12:14:43Z2016-11-18T12:03:42ZCDS support team

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

cds-question@unistra.frgalaxiesphotometryinfrared-photometryredshiftedvisible-astronomybroad-band-photometryultraviolet-photometrysurveysWe present a catalog covering 1.62deg^2^ of the COSMOS/UltraVISTA field with point-spread function (PSF) matched photometry in 30 photometric bands. The catalog covers the wavelength range 0.15-24{mu}m including the available GALEX, Subaru, Canada-France-Hawaii Telescope, VISTA, and Spitzer data. Catalog sources have been selected from the DR1 UltraVISTA K_s_ band imaging that reaches a depth of K_s,tot_=23.4 AB (90% completeness). The PSF-matched catalog is generated using position-dependent PSFs ensuring accurate colors across the entire field. Also included is a catalog of photometric redshifts (z_phot_) for all galaxies computed with the EAZY code. Comparison with spectroscopy from the zCOSMOS 10k bright sample shows that up to z~1.5 the z_phot_ are accurate to {Delta}z/(1+z)=0.013, with a catastrophic outlier fraction of only 1.6%. The z_phot_ also show good agreement with the z_phot_ from the NEWFIRM Medium Band Survey out to z~3. A catalog of stellar masses and stellar population parameters for galaxies determined using the FAST spectral energy distribution fitting code is provided for all galaxies. Also included are rest-frame U-V and V-J colors, L_2800_ and L_IR_. The UVJ color-color diagram confirms that the galaxy bi-modality is well-established out to z~2. Star-forming galaxies also obey a star-forming "main sequence" out to z~2.5, and this sequence evolves in a manner consistent with previous measurements. The COSMOS/UltraVISTA K_s_-selected catalog covers a unique parameter space in both depth, area, and multi-wavelength coverage and promises to be a useful tool for studying the growth of the galaxy population out to z~3-4.2013ApJS..206....8Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/206/8CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toB/eso : ESO Science Archive Catalog (ESO, 1991-2016)VIII/95 : Herschel Multi-tiered Extragalactic Survey (Oliver+, 2012)II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012)II/284 : COSMOS Multi-Wavelength Photometry Catalog (Capak+, 2007)VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)J/ApJ/777/18 : Stellar mass functions of galaxies to z=4 (Muzzin+, 2013)J/ApJ/771/85 : Dynamical masses of z~2 quiescent gal. (van de Sande+, 2013)J/A+A/544/A156 : UltraVISTA Catalogue Release DR1 (McCracken+, 2012)J/MNRAS/415/3831 : AzTEC/ASTE source catalogue (Aretxaga+, 2011)J/ApJ/735/86 : NEWFIRM MBS: photometric catalogs (Whitaker+, 2011)J/ApJS/188/384 : The VLA-COSMOS survey. IV. (Schinnerer+, 2010)J/AJ/138/1261 : Spitzer/MIPS observations of the COSMOS field (Frayer+, 2009)J/ApJS/184/218 : The zCOSMOS 10k-bright spectroscopic sample (Lilly+, 2009)J/ApJS/184/158 : Chandra COSMOS survey I. (Elvis+, 2009)J/ApJ/682/985 : FIREWORKS photometry of GOODS CDF-S (Wuyts+, 2008)J/MNRAS/385/2225 : AzTEC millimetre survey of COSMOS field (Scott+, 2008)J/ApJS/172/70 : zCOSMOS-bright catalog (Lilly+, 2007)J/ApJS/172/46 : VLA-COSMOS survey. II. (Schinnerer+, 2007)J/ApJS/172/29 : XMM-Newton survey in COSMOS field. I. (Hasinger+, 2007)J/ApJ/655/51 : HDFS IRAC observations of 2<z<3.5 galaxies (Wuyts+, 2007)J/AJ/131/1184 : A recalibration of optical photometry (Maiz-Apellaniz+, 2006)J/AJ/125/1107 : Ultra-deep near-IR observation in HDF-S (Labbe+, 2003)http://www.strw.leidenuniv.nl/galaxyevolution/ULTRAVISTA/ : UltraVISTA homehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/206/8https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/206/8http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/206/8https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/206/8https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/206/8http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/206/8GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJS/206/8/catalog (*UVISTA photometric catalog v4.1)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/206/8/catalog?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/206/8/catalog?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/206/8/catalog?GETtext/xml+votable180.050000true150.372651.6093940.0055555555555555565/6814 6/27245 27247 273446.772611666688002e-21 1.4134638842407062e-18https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/206/8?format=asciiInfraredOpticalUVdefaultJ/ApJS/206/8/m05FAST stellar masses and SPS parameters for Maraston C. (2005MNRAS.362..799M) modelsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/262615] Running sequence numbermeta.id;meta.mainintprimaryz[0.01/6]? Photometric redshift from EASYsrc.redshift.photfloatnullableltau[7/10]? Best-fit value of log({tau}) (1)log(yr)stat.fit.paramfloatnullablemetal[0.02]? Metallicity (fixed at 0.020)phys.abund.Zfloatnullablelage[7/10.1]? Best-fit value of log(t) (1)log(yr)time.agefloatnullableAv[0/4]? Best-fit value of A_v_phys.absorptionfloatnullablelmass[-1/14.3]? Best-fit value of log(M_star_/M_{sun}_)log(solMass)phys.massfloatnullablelsfr[-36/4.8]? Best-fit value of log(sfr) from the SEDlog(solMass.yr**-1)phys.SFRfloatnullablelssfr[-43/-1]? Best-fit value of log(ssfr) from the SEDlog(yr**-1)phys.SFRfloatnullablela2t[-3/3.1] la2t valuestat.fit.paramfloatchi2[-1/189] {chi}^2^ of best-fitting modelstat.param;meta.modelleddoubleJ/ApJS/206/8/153-155U-V EASY rest-frame colorsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/262615] Running sequence numbermeta.id;meta.mainintprimaryzpk[/6]? Photometric redshift from the peak of the P(z) distributionsrc.redshift.photdoublenullableDM[/47]? Distance modulusphot.mag.distModfloatnullableNf[/20]? Number of filters used for the fitmeta.numberintnullablechi2[/2009]? Best-fit {chi}^2^stat.fit.chi2;meta.modelleddoublenullableL153[/826698]? EAZY-interpolated U-V color index (1)phot.color;em.opt;em.optdoublenullableL155[/5.59709e+06]? EAZY-interpolated U-V color index (1)phot.color;em.opt;em.optdoublenullableJ/ApJS/206/8/155-161V-J EASY rest-frame colorsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/262615] Running sequence numbermeta.id;meta.mainintprimaryzpk[/6]? Photometric redshift from the peak of the P(z) distributionsrc.redshift.photdoublenullableDM[/47]? Distance modulusphot.mag.distModfloatnullableNf[/20]? Number of filters used for the fitmeta.numberintnullablechi2[/1730]? Best-fit {chi}^2^stat.fit.chi2;meta.modelleddoublenullableL155[/261250]? EAZY-interpolated V-J color index (1)phot.color;em.opt;em.IRdoublenullableL161[/1.06681e+06]? EAZY-interpolated V-J color index (1)phot.color;em.opt;em.IRdoublenullableJ/ApJS/206/8/catalog*UVISTA photometric catalog v4.1recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/262615] Running sequence numbermeta.id;meta.mainintprimaryRAJ2000[149.3/150.8] Right ascension (J2000)degpos.eq.ra;meta.mainindexedDEJ2000[1.6/2.9] Declination (J2000)degpos.eq.dec;meta.mainindexedxpixX position of object in the Ks imagepixpos.cartesian.x;instr.detdoubleypixY position of object in the Ks imagepixpos.cartesian.y;instr.detdoubleFKstot[-41/644028] Total Ks-band flux with apcor already applied (1)phot.mag;em.IR.Kdoublee_FKstot[0.1/53] Kstot uncertaintystat.errorfloatFKs[0.01/75226] UltraVISTA Ks flux (2)0.3631uJyphot.mag;em.IR.Kdoublee_FKs[0.6/17] FKs uncertainty0.3631uJystat.errorfloatFH[-16/93819] UltraVISTA H flux (2)0.3631uJyphot.flux.density;em.IR.Hdoublee_FH[0.5/13] FH uncertainty0.3631uJystat.errorfloatFJ[-19.1/64555] UltraVISTA J flux (2)0.3631uJyphot.flux.density;em.IR.Jdoublee_FJ[0.3/10.3] FJ uncertainty0.3631uJystat.errorfloatFY[-14.8/116197] UltraVISTA Y (broadband at 1020nm) flux (2)0.3631uJyphot.flux.density;em.IRdoublee_FY[0.3/17] FY uncertainty0.3631uJystat.errorfloatFch4[-5255/44148]? Spitzer/IRAC 8um flux (2)0.3631uJyphot.flux.density;em.IR.8-15umdoublenullablee_Fch4[3.9/103098]? Fch4 uncertainty0.3631uJystat.errordoublenullableFch3[-1501/63780]? Spitzer/IRAC 5.8um flux (2)0.3631uJyphot.flux.density;em.IR.4-8umdoublenullablee_Fch3[4.1/3195]? Fch3 uncertainty0.3631uJystat.errordoublenullableFch2[-223/26394]? Spitzer/IRAC 4.5um flux (2)0.3631uJyphot.flux.density;em.IR.4-8umdoublenullablee_Fch2[0.6/1322]? Fch2 uncertainty0.3631uJystat.errordoublenullableFch1[-218/23086]? Spitzer/IRAC 3.6um flux (2)0.3631uJyphot.mag;em.IR.3-4umdoublenullablee_Fch1[0.5/1156]? Fch1 uncertainty0.3631uJystat.errordoublenullableFzp[-7/2060]? Subaru/SuprimeCam z+ flux (2)0.3631uJyphot.mag;em.opt.Idoublenullablee_Fzp[0.1/2]? Fzp uncertainty0.3631uJystat.errorfloatnullableFip[-6.2/514]? Subaru/SuprimeCam i+ flux (2)0.3631uJyphot.flux.density;em.opt.Ifloatnullablee_Fip[0.08/0.8]? Fip uncertainty0.3631uJystat.errorfloatnullableFrp[-17/876]? Subaru/SuprimeCam r+ flux (2)0.3631uJyphot.flux.density;em.opt.Rfloatnullablee_Frp[0.05/1.3]? Frp uncertainty0.3631uJystat.errorfloatnullableFV[-6.6/1175]? Subaru/SuprimeCam V_j_ flux (2)0.3631uJyphot.flux.density;em.opt.Vdoublenullablee_FV[0.05/1.3]? FV uncertainty0.3631uJystat.errorfloatnullableFgp[-46/1249]? Subaru/SuprimeCam g+ flux (2)0.3631uJyphot.mag;em.opt.Bdoublenullablee_Fgp[0.05/0.8]? Fgp uncertainty0.3631uJystat.errorfloatnullableFB[-7.4/1138]? Subaru/SuprimeCam B_j_ flux (2)0.3631uJyphot.flux.density;em.opt.Bdoublenullablee_FB[0.03/1.2]? FB uncertainty0.3631uJystat.errorfloatnullableFu[-54.1/16050] CFHT/MegaCam u* flux (2)0.3631uJyphot.flux.density;em.opt.Udoublee_Fu[0.03/14.2] Fu uncertainty0.3631uJystat.errorfloatFIA484[-257/2448]? Subaru/SuprimeCam IA484 flux (2)0.3631uJyphot.flux.density;em.opt.Vdoublenullablee_FIA484[0.07/8]? FIA484 uncertainty0.3631uJystat.errorfloatnullableFIA527[-316/3211]? Subaru/SuprimeCam IA527 flux (2)0.3631uJyphot.flux.density;em.opt.Vdoublenullablee_FIA527[0.07/9]? FIA527 uncertainty0.3631uJystat.errorfloatnullableFIA624[-412/3666]? Subaru/SuprimeCam IA624 flux (2)0.3631uJyphot.flux.density;em.opt.Rdoublenullablee_FIA624[0.09/8]? FIA624 uncertainty0.3631uJystat.errorfloatnullableFIA679[-582/5602]? Subaru/SuprimeCam IA679 flux (2)0.3631uJyphot.flux.density;em.opt.Rdoublenullablee_FIA679[0.1/8]? FIA679 uncertainty0.3631uJystat.errorfloatnullableFIA738[-206/3984]? Subaru/SuprimeCam IA738 flux (2)0.3631uJyphot.flux.density;em.opt.Rdoublenullablee_FIA738[0.1/9]? FIA738 uncertainty0.3631uJystat.errorfloatnullableFIA767[-1449/5859]? Subaru/SuprimeCam IA767 flux (2)0.3631uJyphot.flux.density;em.opt.Idoublenullablee_FIA767[0.1/10]? FIA767 uncertainty0.3631uJystat.errorfloatnullableFIB427[-871/7199]? Subaru/SuprimeCam IB427 flux (2)0.3631uJyphot.flux.density;em.opt.Vdoublenullablee_FIB427[0.07/17]? FIB427 uncertainty0.3631uJystat.errorfloatnullableFIB464[-1043/8397]? Subaru/SuprimeCam IB464 flux (2)0.3631uJyphot.flux.density;em.opt.Vdoublenullablee_FIB464[0.1/17]? FIB464 uncertainty0.3631uJystat.errorfloatnullableFIB505[-1476/7743]? Subaru/SuprimeCam IB505 flux (2)0.3631uJyphot.flux.density;em.opt.Vdoublenullablee_FIB505[0.09/15]? FIB505 uncertainty0.3631uJystat.errorfloatnullableFIB574[-566/7152]? Subaru/SuprimeCam IB574 flux (2)0.3631uJyphot.flux.density;em.opt.Vdoublenullablee_FIB574[0.1/13]? FIB574 uncertainty0.3631uJystat.errorfloatnullableFIB709[-645/5095]? Subaru/SuprimeCam IB709 flux (2)0.3631uJyphot.flux.density;em.opt.Rdoublenullablee_FIB709[0.1/9]? FIB709 uncertainty0.3631uJystat.errorfloatnullableFIB827[-1449/4860]? Subaru/SuprimeCam IB827 flux (2)0.3631uJyphot.flux.density;em.opt.Idoublenullablee_FIB827[0.1/10]? FIB827 uncertainty0.3631uJystat.errorfloatnullableFFUV[-1482/7734]? GALEX FUV flux (2)0.3631uJyphot.flux;em.UVdoublenullablee_FFUV[0.06/946]? FFUV uncertainty0.3631uJystat.errorfloatnullableFNUV[-6098/5495]? GALEX NUV flux (2)0.3631uJyphot.flux;em.UVdoublenullablee_FNUV[0.04/452]? FNUV uncertainty0.3631uJystat.errorfloatnullableF24[0.1/33412]? Spitzer/MIPS 24um flux (2)0.3631uJyphot.flux.density;em.IR.15-30umdoublenullablee_F24[0.1/14]? F24 uncertainty0.3631uJystat.errorfloatnullableKflag[0/6] SExtractor's FLAG output for the Ks-band image (3)meta.codefloatS/G[0/1] SExtractor's CLASS_STAR output from the Ks band image (>0.9: likely point source)meta.notefloatKKron[3/50] SExtractor's Kron radius in Ks-bandphys.size.radiusdoubleapcor[1/1.2] Aperture correction that has been applied to FLUX_AUTO to determine Ks_totphot.mag;arith.diffdoublezsp[0.01/2.1]? zCOSMOS spectroscopic redshiftsrc.redshiftdoublenullableCC[3/5]? Spectroscopic redshift quality flag (3<q_zsp<4: highest quality) (z_spec_cc) (4)meta.codedoublenullablezCOSMOS[7447/950074]? ID of the spectroscopic redshift in the zCOSMOS catalogmeta.idintnullableStar[0/1] Star/galaxy indicator determined from color-color plot (star=1, galaxy=0)src.class.starGalaxyintCont[0/1] Contamination: proximity to a bright star (contaminated=1, uncontaminated=0)meta.codeintnCont[0/21] Number of filters where object lies near gaps in photometry or near a saturated star; uncontaminated=0 (nan_contam) (5)meta.numberintOri[230/82870] ID number in the original catalogs generated from the 9 COSMOS subfields (orig_cat_id)meta.idintField[1/9] Subfield of the object (orig_cat_field)obs.fieldintUSE[0/1] Indicates galaxies with uncontaminated photometry and S/N>5 (6)meta.codeintDR1Display data from UltraVISTA DR1 catalog (McCracken+, 2012, J/A+A/544/A156) within 0.5"meta.ref.urlintnullableSimbadSimbad column added by the CDSmeta.ref.urlcharJ/ApJS/206/8/zout*EAZY photometric redshift catalog v4.1recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/262615] Running sequence numbermeta.id;meta.mainintprimaryzsp[0.01/2.1]? Spectroscopic redshift from zCOSMOSsrc.redshiftfloatnullableza[0.01/6]? Redshift where {chi}^2^ is minimized for all-template (1)src.redshift.photfloatnullablezm1[0.01/6]? Redshift marginalized over p(z|C)=exp{-0.5{chi}^2^} (1)src.redshift.photfloatnullablechia[1.4/3759]? {chi}^2^ value at z=zastat.fit.chi2doublenullablezp[0.01/6]? Redshift where likelihood is maximized after applying the prior, p(z|m_0_) (1)src.redshift.photfloatnullablechip[1.4/3759]? Original {chi}^2^ at z=zpstat.fit.chi2doublenullablezm2[0.01/6]? Redshift marginalized over p(z|C,m_0_)=p(z|C).p(z|m_0_) (1)src.redshift.photfloatnullableodds[-99/1] Redshift quality parameter (1)meta.code.qualfloatl68[0.01/6]? Lower 68% confidence interval on zpkstat.errorfloatnullableu68[0.02/6]? Upper 68% confidence interval on zpkstat.errorfloatnullablel95[0.01/6]? Lower 95% confidence interval on zpkstat.errorfloatnullableu95[0.02/6]? Upper 95% confidence interval on zpkstat.errorfloatnullablel99[0.01/6]? Lower 99% confidence interval on zpkstat.errorfloatnullableu99[0.02/6]? Upper 68% confidence interval on zpkstat.errorfloatnullableNf[8/29]? Number of filters used to determine zpkmeta.numberintnullableq_z[-99/3.26455e+212] z qualitymeta.code.qual;src.redshiftdoublezpk[0.01/6]? Photometric redshift from the peak of the P(z) distributionsrc.redshift.photdoublenullableProbpk[-99/1] Peak probabilitystat.fit.goodnessfloatzmc[0.01/6]? zmc value (1)src.redshift.photdoublenullableJ/ApJS/206/8/bc03FAST stellar masses and SPS parameters for Bruzual & Charlot (2003MNRAS.344.1000B) modelsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/262615] Running sequence numbermeta.id;meta.mainintprimaryz[0.01/6]? Photometric redshift from EASYsrc.redshift.photfloatnullableltau[7/10]? Best-fit value of log({tau}) (1)log(yr)stat.fit.paramfloatnullablemetal[0.02]? Metallicity (fixed at 0.020)phys.abund.Zfloatnullablelage[7/10.1]? Best-fit value of log(t) (1)log(yr)time.agefloatnullableAv[0/4]? Best-fit value of A_v_phys.absorptionfloatnullablelmass[-1/14.3]? Best-fit value of log(M_star_/M_{sun}_)log(solMass)phys.massfloatnullablelsfr[-36/4.8]? Best-fit value of log(sfr) from the SEDlog(solMass.yr**-1)phys.SFRfloatnullablelssfr[-43/-1]? Best-fit value of log(ssfr) from the SEDlog(yr**-1)phys.SFRfloatnullablela2t[-3/3.1] la2t valuestat.fit.paramfloatchi2[-1/189] {chi}^2^ of best-fitting modelstat.param;meta.modelleddouble