J/ApJ/546/694ivo://CDS.VizieR/J/ApJ/546/694doi:10.26093/cds/vizier.15460694CDSThompson R.I.Weymann R.J.Storrie-Lombardi L.J.2001-05-11T21:20:53Z2001-05-11T21:19:02ZCDS support team

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

cds-question@unistra.frgalaxiesphotometryredshiftedextinctioninfrared-photometryWe present the results of an extensive analysis of the star formation rates determined from the NICMOS deep images of the northern Hubble Deep Field. We use SED template fitting photometric techniques to determine both the redshift and the extinction for each galaxy in our field. Measurement of the individual extinctions provides a correction for star formation hidden by dust obscuration. We determine star formation rates for each galaxy based on the 1500{AA} UV flux and add the rates in redshift bins of width 1.0 centered on integer redshift values.2001ApJ...546..694Thttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/546/694CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/AJ/112/1335 : Hubble Deep Field observations (Williams+ 1996)J/AJ/117/17 : Hubble Deep Field near-IR obs. (Thompson+, 1999)J/ApJ/538/493 : HDF-South NICMOS field (Yahata+, 2000)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/546/694https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/546/694http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/546/694https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/546/694https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/546/694http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/546/694GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/546/694/table1 (Listing of measured quantities)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/546/694/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/546/694/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/546/694/table1?GETtext/xml+votable180.050000true189.170041762.20266670.005555555555555556HST6/11252https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/546/694?format=asciiOpticalInfrareddefaultJ/ApJ/546/694/table1Listing of measured quantitiesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNICMOSNICMOS identification number (1)meta.id;meta.maindouble[WBD96]WFPC identification number from Williams et al., 1996, Cat. <J/AJ/112/1335>meta.idcharzRedshiftsrc.redshiftfloatE(B-V)(B-V) color excessmagphot.color.excessfloatSFRStar formation rate determined in Section 5solMass/yrphys.SFRfloatLumBolometric luminosity (2)solLumphys.luminositydoubleFracFraction of the luminosity removed by extinction and re-emitted in the mid & far-IRphys.luminosity;arith.ratiofloatSCUBA? The SCUBA 850 microns fluxmJyphot.flux.density;em.mm.200-400GHzdoublenullableTempTemplate number of best fit between 1.0 (early-cold) and 6.0 (late-hot)stat.fit.paramfloatChi2Modified Chi^2^ of the fit from Equ. 1 (3)stat.fit.paramfloatTotmag? The F160W AB magnitude (4)magphot.mag;em.UV.100-200nmfloatnullableApmag? The 0.6" diameter aperture F160W magnitude See note (5)magphot.mag;em.UV.100-200nmfloatnullableRAJ2000Right Ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.main