J/ApJ/517/148ivo://CDS.VizieR/J/ApJ/517/148doi:10.26093/cds/vizier.15170148CDSFlores H.Hammer F.Thuan T.X.Cesarsky C.Desert F.X.Omont A.,Lilly S .J.Eales S.Crampton D.Le Fevre O.2000-03-16T09:02:47Z2000-03-16T10:01:31ZCDS support team

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

cds-question@unistra.frgalaxiesinfrared-sourcesphotometryThe Canada-France Redshift Survey 1452+52 field has been deeply imaged with the Infrared Space Observatory using ISOCAM through the LW3 filter (1218 {mu}m). Careful data analysis and comparison with deep optical and radio data have allowed us to generate a catalog of 78 15 {mu}m sources with both radio and optical identifications. They are redder and lie at higher redshift than I-band-selected galaxies, with most of them being star-forming galaxies. We have considered the galaxies detected at radio and 15 {mu}m wavelengths, which potentially include all strong and heavily extincted starbursts, up to z=1. Spectral energy distributions (SEDs) for each of the sources have been derived using deep radio, mid-IR, near-IR, optical, and UV photometry. The sources were then spectrally classified by comparing with SEDs of well-known nearby galaxies. By deriving their far-IR luminosities by interpolation, we can estimate their star formation rate (SFR) in a way that does not depend sensitively on the extinction.1999ApJ...517..148Fhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/517/148CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJ/481/49 : CFRS XIV. Field galaxies up to z=1 (Hammer+ 1997)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/517/148https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/517/148http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/517/148https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/517/148https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/517/148http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/517/148GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/517/148/table1 (Optical counterparts of ISOCAM LW3 sources)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/517/148/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/517/148/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/517/148/table1?GETtext/xml+votable180.050000true214.42416752.4731390.005555555555555556ISO6/11424 11425https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/517/148?format=asciiInfrareddefaultJ/ApJ/517/148/table1Optical counterparts of ISOCAM LW3 sourcesRAJ2000Right Ascension (J2000)recnoRecord number assigned by the VizieR team. Should Not be used for identification.intCatalogCatalog object was obtained from (1)charISONameName in the ISO catalog of Flores et al. (1999A&A...343..389)intn_ISOName[g] Note on ISOName (2)charDEJ2000Declination (J2000)CFRS? Canada-France Redshift Survey numberfloatnullablen_zIndicates that a redshift of 0.7217 was given by Lilly+ (1995).charf_ISOName[s] Indicates object is a starcharz? RedshiftfloatnullableImag? I band isophotal magnitude in the AB systemmagfloatnullableVmag? V band isophotal magnitude in the AB systemmagfloatnullableKmag? K band isophotal magnitude in the AB systemmagfloatnullableDist? Distance between ISO source and optical or radio counterpartarcsecfloatnullableProbAssociated probability of coincidence of sourcesdoublef_ProbIndicates radio source with probability based on radio-source countscharFluxFlux density at 12-18 {mu}m within and 9'' apertureuJyinte_FluxUncertainty in FluxuJyint