J/ApJ/719/763ivo://CDS.VizieR/J/ApJ/719/763doi:10.26093/cds/vizier.17190763CDSVieira J.D.Crawford T.M.Switzer E.R.Ade P.A.R.Aird K.A.,Ashby M.L.N.Benson B.A.Bleem L.E.Brodwin M.Carlstrom J.E.,Chang C.L.Cho H.-M.Crites A.T.de Haan T.Dobbs M.A.Everett W.,George E.M.Gladders M.Hall N.R.Halverson N.W.High F.W.,Holder G.P.Holzapfel W.L.Hrubes J.D.Joy M.Keisler R.Knox L.,Lee A.T.Leitch E.M.Lueker M.Marrone D.P.McIntyre V.McMahon J.J.,Mehl J.Meyer S.S.Mohr J.J.Montroy T.E.Padin S.Plagge T.,Pryke C.Reichardt C.L.Ruhl J.E.Schaffer K.K.Shaw L.Shirokoff E.,Spieler H.G.Stalder B.Staniszewski Z.Stark A.A.Vanderlinde K.,Walsh W.Williamson R.Yang Y.Zahn O.Zenteno A.2012-07-25T11:48:57Z2012-07-06T10:21:24ZCDS support team

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

cds-question@unistra.frmillimeter-astronomysubmillimeter-astronomyactive-galactic-nucleisurveysWe report the results of an 87deg^2^ point-source survey centered at R.A. 5h30m, decl. -55{deg} taken with the South Pole Telescope at 1.4 and 2.0mm wavelengths with arcminute resolution and milli-Jansky depth. Based on the ratio of flux in the two bands, we separate the detected sources into two populations, one consistent with synchrotron emission from active galactic nuclei and the other consistent with thermal emission from dust. We present source counts for each population from 11 to 640mJy at 1.4mm and from 4.4 to 800mJy at 2.0mm. The 2.0mm counts are dominated by synchrotron-dominated sources across our reported flux range; the 1.4mm counts are dominated by synchrotron-dominated sources above ~15mJy and by dust-dominated sources below that flux level. We detect 141 synchrotron-dominated sources and 47 dust-dominated sources at signal-to-noise ratio S/N>4.5 in at least one band. All of the most significantly detected members of the synchrotron-dominated population are associated with sources in previously published radio catalogs. Some of the dust-dominated sources are associated with nearby (z<<1) galaxies whose dust emission is also detected by the Infrared Astronomy Satellite. However, most of the bright, dust-dominated sources have no counterparts in any existing catalogs. We argue that these sources represent the rarest and brightest members of the population commonly referred to as submillimeter galaxies (SMGs).2010ApJ...719..763Vhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/719/763CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toVIII/81 : Sydney University Molonglo Sky Survey (SUMSS V2.1) (Mauch+ 2008)IX/29 : ROSAT All-Sky Survey Faint Source Catalog (Voges+ 2000)IX/10 : ROSAT All-Sky Bright Source Catalogue (1RXS) (Voges+ 1999)II/156 : IRAS Faint Source Catalog, |b| > 10, Version 2.0 (Moshir+ 1989)J/MNRAS/413/2314 : Radio and mid-IR counterpart of submm galaxies (Biggs+,J/ApJ/712/942 : z>4 submillimeter galaxies (Michalowski+, 2010)J/MNRAS/401/160 : AzTEC survey of the SHADES fields. I. (Austermann+, 2010)J/ApJ/699/1610 : Spitzer survey of submillimeter galaxies (Hainline+, 2009)J/MNRAS/385/1656 : Extragalactic radio-sources at 95GHz (Sadler+, 2008)J/MNRAS/385/2225 : AzTEC millimetre survey of COSMOS field (Scott+, 2008)J/ApJ/622/772 : Redshift survey of submillimeter galaxies (Chapman+, 2005)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/719/763https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/719/763http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/719/763https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/719/763https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/719/763http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/719/763GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/719/763/table5 (Point sources above 3{sigma} at 1.4mm or 2.0mm in an 87 square degree South Pole Telescope (SPT) field centered at 05:30-55{deg} (J2000))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/719/763/table5?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/719/763/table5?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/719/763/table5?GETtext/xml+votable180.050000true74.787-58.9530.0055555555555555564/2115 2116 2117 2118 5/8455 8459 8476 8477 8478 8512 8513 8514 6/33813 33815 33817 33818 33819 33829 33830 33831 33833 33916 33917 33918 33941 33984 33985 33988 33989 34000 34001 34060 34061 34062 34064 34065 34066 34080 34081 34082 39042 39048 39050 39072 39074 39080 39082 39424 39426 39432 39434 39456 394589.932212984278052e-23 1.4188866158993417e-22https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/719/763?format=asciiRadiodefaultJ/ApJ/719/763/table5Point sources above 3{sigma} at 1.4mm or 2.0mm in an 87 square degree South Pole Telescope (SPT) field centered at 05:30-55{deg} (J2000)S1.4rRaw 1.4mm flux densitymJyphot.flux.density;em.mm.200-400GHzfloatS1.4bDe-boosted 1.4mm flux densitymJyphot.flux.density;em.mm.200-400GHzfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSPT-SSource identification (JHHMMSS+DDMM.m)meta.id;meta.maincharRAJ2000Right Ascension in decimal degrees (J2000)degpos.eq.ra;meta.mainDEJ2000Declination in decimal degrees (J2000)degpos.eq.dec;meta.mainS/N2Signal-to-noise of 2.0mm datastat.snrfloatS2.0rRaw 2.0mm flux densitymJyphot.flux.density;em.mm.100-200GHzfloatS2.0bDe-boosted 2.0mm flux densitymJyphot.flux.density;em.mm.100-200GHzfloatE_S2.0bUpper limit uncertainty in S2.0bmJystat.error;stat.maxfloate_S2.0bLower limit uncertainty in S2.0bmJystat.errorfloatS/N1Signal-to-noise of 1.4mm datastat.snrfloatE_S1.4bUpper limit uncertainty in S1.4bmJystat.error;stat.maxfloate_S1.4bLower limit uncertainty in S1.4bmJystat.errorfloatSpI.rRaw spectral index (1)spect.indexfloatSpI.bDe-boosted spectral indexspect.indexfloatE_SpI.bUpper limit uncertainty in SpI.bstat.error;stat.maxfloate_SpI.bLower limit uncertainty in SpI.bstat.errorfloatP(1.66)[0/1] Fraction of spectral index posterior probability above 1.66 (2)stat.fit.goodnessfloatType[sync/dust] Source classification (3)src.classcharSUMSS[0/1157] Nearest source in SUMSS (Cat. VIII/81)arcsecpos.angDistanceintRASS[3/2167] Nearest source in RASS (Cat. IX/10 and Cat. IX/29)arcsecpos.angDistanceIRAS[1/2180] Nearest source in IRAS (Cat. II/156)arcsecpos.angDistanceint