J/ApJ/596/748ivo://CDS.VizieR/J/ApJ/596/748doi:10.26093/cds/vizier.15960748CDSThompson R.I.2006-10-08T12:05:06Z2006-10-08T12:01:59ZCDS support team

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

cds-question@unistra.frgalaxiesphotometryredshiftedinfrared-photometryThe original analysis of the star formation history in the NICMOS deep images of the northern Hubble Deep Field (NHDF) is extended to the entire NHDF utilizing NICMOS and WFPC2 archival data. The roughly constant star formation rate from redshifts 16 found in this study is consistent with the original results. Star formation rates from this study, Lyman break galaxies, and submillimeter observations are now in concordance. The spike of star formation at redshift 2 due to two ultraluminous IR galaxies in the small deep NICMOS field is smoothed out in the larger area results presented here. The larger source base of this study allows comparison with predictions from hierarchical galaxy formation models. In general, the observation are consistent with the predictions. The observed luminosity functions at redshifts 16 are presented for future comparisons with theoretical galaxy evolution calculations. Mid- and far-infrared properties of the sources are also calculated and compared with observations. A candidate for the VLA source VLA 3651+1221 is discussed.2003ApJ...596..748Thttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/596/748CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/AJ/112/1335 : Hubble Deep Field observations (Williams+ 1996)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/596/748https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/596/748http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/596/748https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/596/748https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/596/748http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/596/748GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/596/748/table2 (Listing of measured quantities)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/596/748/table2?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/596/748/table2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/596/748/table2?GETtext/xml+votable180.050000true189.1592916762.207861110.005555555555555556HST6/11252https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/596/748?format=asciiOpticalInfrareddefaultJ/ApJ/596/748/table2Listing of measured quantitiesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint[T2003]NICMOS identificationmeta.id;meta.mainintprimaryWFPC-IDWFPC identificationmeta.idcharzRedshift (photometric)src.redshift.photfloatE(B-V)Extinctionmagphot.color.excessfloatSFRStar Formation RatesolMass/yrphys.SFRdoubleLum? LuminositysolLumphys.luminositydoublenullableFracLuminosity fraction removed by extinction and re-emitted in the mid and far infraredphys.absorptionfloatISO6? The ISO 6 micron fluxmJyphot.flux.density;em.IR.4-8umdoublenullableISO15? The ISO 15 micron fluxmJyphot.flux.density;em.IR.8-15umdoublenullableSCUBA? The SCUBA 850 micron fluxmJyphot.flux.density;em.mm.200-400GHzdoublenullableTNumSelected template number (1)src.class.colorfloatChi2The {chi}^2^ valuestat.valuefloatF160W? Total AB magnitude in the F160W filtermagphot.mag;em.IR.HfloatnullableApmagThe 0.6" diameter F160W filter magnitudemagphot.mag;em.IR.HfloatRAJ2000Hour of Right Ascension (J2000)pos.eq.ra;meta.mainDEJ2000Degree of Declination (J2000)pos.eq.dec;meta.mainJ/ApJ/596/748/table3Properties of Galaxies with F160W Magnitudes Significantly Brighter than Predicted L* MagnitudesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint[T2003]Sequential numbermeta.recordintWFPC-IDWFPC identificationmeta.idcharzRedshift (photometric)src.redshift.photfloatF160WAB magnitude in the F160W filtermagphot.mag;em.IR.HfloatE(B-V)Extinctionmagphot.color.excessfloatTNumTemplate used for spectral energy distributionsrc.class.colorfloatLumLuminositysolLumphys.luminositydouble