J/AJ/143/125ivo://CDS.VizieR/J/AJ/143/125doi:10.26093/cds/vizier.51430125CDSMelbourne J.Soifer B.T.Desai V.Pope A.Armus L.Dey A.,Bussmann R.S.Jannuzi B.T.Alberts S.2017-06-19T07:58:03Z2013-07-28T16:05:35ZCDS support team

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

cds-question@unistra.frgalaxiesinfrared-sourcesredshiftedinfrared-photometrymillimeter-astronomyphotometrysubmillimeter-astronomyDust-obscured galaxies (DOGs) are a subset of high-redshift (z~2) optically-faint ultra-luminous infrared galaxies (ULIRGs, e.g., L_IR_>10^12^L_{sun}_). We present new far-infrared photometry, at 250, 350, and 500{mu}m (observed-frame), from the Herschel Space Telescope for a large sample of 113 DOGs with spectroscopically measured redshifts. Approximately 60% of the sample are detected in the far-IR. The Herschel photometry allows the first robust determinations of the total infrared luminosities of a large sample of DOGs, confirming their high IR luminosities, which range from 10^11.6^L_{sun}_<L_IR_(8-1000{mu}m)<10^13.6^L_{sun}_. 90% of the Herschel-detected DOGs in this sample are ULIRGs and 30% have L_IR_>10^13L{sun}. The rest-frame near-IR (1-3{mu}m) spectral energy distributions (SEDs) of the Herschel-detected DOGs are predictors of their SEDs at longer wavelengths.2012AJ....143..125Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/143/125CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJ/744/150 : MIR-selected (bump & power-law DOGs) ULIRGs (Bussmann+, 2012)J/MNRAS/423/197 : MIPS photometry for Herschel SAG2 Programs (Bendo+, 2012)J/MNRAS/417/2239 : SPIRE (f250um>17.4mJy) GOODS-N galaxies (Symeonidis+, 2011)J/MNRAS/409/L13 : Herschel-SPIRE radio galaxies (Chapman+, 2010)J/ApJ/716/530 : Mid-IR variability from the SDWFS (Kozlowski+, 2010)J/MNRAS/409/2 : Herschel sources SED model parameters (Rowan-Robinson+, 2010)J/MNRAS/409/L13 : Herschel-SPIRE radio galaxies (Chapman+, 2010)J/ApJ/692/422 : MAMBO observations of SWIRE sources (Lonsdale+, 2009)J/A+A/508/117 : Spitzer selected starbursts at z~2 (Fiolet+, 2009)J/ApJ/701/428 : The Spitzer Deep, Wide-Field Survey (SDWFS) (Ashby+, 2009)J/ApJ/658/778 : Spitzer mid-IR spectroscopy of z~2 ULIRGs (Yan+, 2007)J/ApJ/622/772 : Redshift survey of submillimeter galaxies (Chapman+, 2005)http://herschel.esac.esa.int/logrepgen/observationlist.do : Herschelhttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/143/125https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/143/125http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/143/125https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/143/125https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/143/125http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/143/125GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/AJ/143/125/DOGs (Sample of 113 dust-obscured galaxies (DOGs))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/143/125/DOGs?https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/143/125/DOGs?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/143/125/DOGs?GETtext/xml+votable180.050000true216.4092083335.315391670.0055555555555555565/2287 2628 6/9145 9146 9147 10516 10517 105183.2031150387835462e-22 3.3785437584409506e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/143/125?format=asciiOpticalInfraredRadiodefaultJ/AJ/143/125/DOGsSample of 113 dust-obscured galaxies (DOGs)SimbadNameSimbad column added by the CDSmeta.idcharF5.8[3.4/953.1] Spitzer/IRAC 5.8{mu}m flux densityuJyphot.flux.density;em.IR.4-8umfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSSTGalaxy ID (JHHMMSS.s+DDMMSS)meta.id;meta.maincharn_SST[a] New Dust-obscured galaxy (1)meta.notecharRAJ2000[14] Hour of Right Ascension (J2000)pos.eq.ra;meta.mainDEJ2000[32/35] Degree of Declination (J2000)pos.eq.dec;meta.mainz[0.75/4.41] Redshiftsrc.redshiftfloatR-24[14.04/22.31] The optical to mid-infrared R-[24] color index (Vega system)magphot.color;em.opt;em.IRfloatF24/FRMid-infrared to-optical flux ratio F{nu}(24{mu}m)/F{nu}(R)phot.flux;arith.ratiodoublel_BWmagUpper limit on BWmagmeta.code.errorcharBWmag[21.6/27.1] The B_W_ band magnitude (Vega system)magphot.mag;em.opt.Bfloate_BWmag? Uncertainty on BWmagmagstat.error;phot.magfloatnullablel_RmagUpper limit on Rmagmeta.code.errorcharRmag[21.76/26.1] The R band magnitude (Vega system)magphot.mag;em.opt.Rfloatu_RmagUncertainty flag on Rmagmeta.code.errorchare_Rmag? Rmag uncertaintymagstat.error;phot.mag;em.opt.Rfloatnullablel_ImagUpper limit on Imagmeta.code.errorcharImag[19.03/25.4] The I band magnitude (Vega system)magphot.mag;em.opt.Ifloate_Imag? Uncertainty on Imagmagstat.error;phot.mag;em.opt.Ifloatnullablel_F3.6Upper limit on F3.6meta.code.errorcharF3.6[3.8/237.1] Spitzer/IRAC 3.6{mu}m flux densityuJyphot.mag;em.IR.3-4umfloate_F3.6? Uncertainty on F3.6uJystat.errorfloatnullablel_F4.5Upper limit on F4.5meta.code.errorcharF4.5[2.4/490.2] Spitzer/IRAC 4.5{mu}m flux densityuJyphot.mag;em.IR.4-8umfloate_F4.5? Uncertainty on F4.5uJystat.errorfloatnullablel_F5.8Upper limit on F5.8meta.code.errorchare_F5.8? Uncertainty on F5.8uJystat.errorfloatnullablel_F8.0Upper limit on F8.0meta.code.errorcharF8.0[7.4/1873.5] Spitzer/IRAC 8.0{mu}m flux densityuJyphot.flux.density;em.IR.8-15umfloate_F8.0? Uncertainty on F8.0uJystat.errorfloatnullableF24[0.33/6.89] Spitzer/MIPS 24{mu}m flux densitymJyphot.flux.density;em.IR.15-30umfloate_F24Uncertainty on F24mJystat.errorfloatl_F250Upper limit on F250 (2)meta.code.errorcharF250[10.6/96] Herschel/SPIRE 250{mu}m flux densitymJyphot.flux.density;em.mm.750-1500GHzfloate_F250? Uncertainty on F250mJystat.errorfloatnullablel_F350Upper limit on F350 (2)meta.code.errorcharF350[7.4/93] Herschel/SPIRE 350{mu}m flux densitymJyphot.flux.density;em.mm.750-1500GHzfloate_F350? Uncertainty on F350mJystat.errorfloatnullablef_F350[s] s=saturatedmeta.codecharl_F500Upper limit on F500 (2)meta.code.errorcharF500[15/94.4] Herschel/SPIRE 500{mu}m flux densitymJyphot.flux;em.IRfloate_F500? Uncertainty on F500mJystat.errorfloatnullableSEDSED plot for this sourcemeta.ref.urlcharSED1Type of spectral energy distribution (SED) in the rest-frame near-infrared (Bump or PL) (3)src.classcharSED2Type of SED in the mid/far-infrared (4)src.classcharl_LIR1Upper limit on LIR1meta.code.errorcharLIR1Total infrared luminosity L_IR_(8-1000{mu}m)solLumphys.luminosity;em.IRdoubleLIR2Model predicted infrared luminosity (Chary & Elbaz, 2001ApJ...556..562C)solLumphys.luminosity;em.IRdoublel_IR8Upper limit on IR8meta.code.errorcharIR8Ratio of infrared luminosity to rest-frame 8{mu}m luminosity (L(8-1000{mu}m)/{nu}L_{nu}_(8{mu}m))phys.luminosity;arith.ratiofloatT? Far-infrared dust temperatureKphys.temperatureintnullableSDWFSSimbad column added by the CDSmeta.ref.urlintnullable