J/ApJ/675/234ivo://CDS.VizieR/J/ApJ/675/234doi:10.26093/cds/vizier.16750234CDSPerez-Gonzalez P.G.Rieke G.H.Villar V.Barro G.Blaylock M.,Egami E.Gallego J.Gil De Paz A.Pascual S.Zamorano J.Donley J.L.2010-09-26T12:18:55Z2010-09-10T16:06:11ZCDS support team

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

cds-question@unistra.frgalaxiesinfrared-sourcesphotometrystellar-massesUsing a sample of ~28000 sources selected at 3.6-4.5um with Spitzer observations of the Hubble Deep Field North, the Chandra Deep Field South, and the Lockman Hole (surveyed area ~664arcmin^2^), we study the evolution of the stellar mass content of the universe at 0<z<4. We calculate stellar masses and photometric redshifts, based on ~2000 templates built with stellar population and dust emission models fitting the ultraviolet to mid-infrared spectral energy distributions of galaxies with spectroscopic redshifts. We estimate stellar mass functions for different redshift intervals.2008ApJ...675..234Phttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/675/234CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/675/234https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/675/234http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/675/234https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/675/234https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/675/234http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/675/234GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticalInfrareddefaultJ/ApJ/675/234/table1Stellar mass functions for the global and star-forming population of galaxiesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintz0Redshift range: lower valuesrc.redshiftfloatz1Redshift range: upper valuesrc.redshiftfloatlogMLog of the masslog(solMass)phys.massfloatlogphi1? Log of IRAC stellar mass function (1)log(Mpc**-3)phys.densityfloatnullableE_logphi1? Upper limit uncertainty in logphi1 (1)log(Mpc**-3)stat.error;stat.maxfloatnullablee_logphi1? Lower limit uncertainty in logphi1 (1)log(Mpc**-3)stat.errorfloatnullablelogphi2? Log of I band stellar mass function (1)log(Mpc**-3)phys.densityfloatnullableE_logphi2? Upper limit uncertainty in logphi2 (1)log(Mpc**-3)stat.error;stat.maxfloatnullablee_logphi2? Lower limit uncertainty in logphi2 (1)log(Mpc**-3)stat.errorfloatnullablelogphi3? Log of MIPS stellar mass function (1)log(Mpc**-3)phys.densityfloatnullableE_logphi3? Upper limit uncertainty in logphi3 (1)log(Mpc**-3)stat.error;stat.maxfloatnullablee_logphi3? Lower limit uncertainty in logphi3 (1)log(Mpc**-3)stat.errorfloatnullable