J/MNRAS/411/505ivo://CDS.VizieR/J/MNRAS/411/505doi:10.26093/cds/vizier.74110505CDSChapin E.L.Chapman S.C.Coppin K.E.Devlin M.J.Dunlop J.S.,Greve T.R.Halpern M.Hasselfield M.F.Hughes D.H.Ivison R.J.,Marsden G.Moncelsi L.Netterfield C.B.Pascale E.Scott D.Smail I.,Viero M.Walter F.Weiss A.Werf P.V.D.2024-07-13T20:14:40Z2011-11-10T15:31:19ZCDS support team

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

cds-question@unistra.frgalaxiescatalogsx-ray-sourcesmillimeter-astronomysubmillimeter-astronomyWe present a joint analysis of the overlapping Balloon-borne Large Aperture Submillimetre Telescope (BLAST) 250, 350, 500um, and LABOCA 870um observations [from the LABOCA ECDFS Submm Survey (LESS) survey] of the Extended Chandra Deep Field-South. Out to z~3, the BLAST filters sample near the peak wavelength of thermal far-infrared (FIR) emission from galaxies (rest-frame wavelengths ~60-200um), primarily produced by dust heated through absorption in star-forming clouds. However, identifying counterparts to individual BLAST peaks is very challenging, given the large beams [full-width at half-maximum (FWHM) 36-60 arcsec]. In contrast, the ground-based 870um observations have a significantly smaller 19 arcsec FWHM beam, and are sensitive to higher redshifts (z~1-5, and potentially beyond) due to the more favourable negative K-correction. We use the LESS data, as well as deep Spitzer and VLA imaging, to identify 118 individual sources that produce significant emission in the BLAST bands.2011MNRAS.411..505Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/411/505CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJS/161/21 : Extended Chandra Deep Field-South survey (Lehmer+, 2005)J/AJ/131/2373 : Extended Chandra Deep Field-South survey (Virani+, 2006)J/other/Nat/458.737 : BLAST sources at 250, 350 and 500um (Devlin+, 2009)J/ApJ/727/1 : IRAC/MUSYC SIMPLE survey (Damen+, 2011)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/411/505https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/411/505http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/411/505https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/411/505https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/411/505http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/411/505GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/411/505/peak (Sub-mm peak catalog produced from matched-filtered maps that land within the coverage of the matching in each BLAST/LABOCA filter)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/411/505/peak?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/411/505/peak?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/411/505/peak?GETtext/xml+votable180.050000true53.1457917-27.92530560.005555555555555556Cone search capability for table J/MNRAS/411/505/matching (Combined catalog with maximum likelihood submm photometry, SED model fits and redshifts)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/411/505/matching?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/411/505/matching?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/411/505/matching?GETtext/xml+votable180.050000true52.8647083-27.744250.0055555555555555566/35935 359572.283270615984385e-22 7.945784137810954e-22https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/411/505?format=asciiX-rayRadiodefaultJ/MNRAS/411/505/peakSub-mm peak catalog produced from matched-filtered maps that land within the coverage of the matching in each BLAST/LABOCA filterSIDSID number (1)meta.idintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaWavelength (BLAST 250, 350, 500{mu}m, or LABOCA 870{mu}muminstr.filter;em.wl.centralintnullablePNamePreviously published name (2)meta.id;meta.maincharSeqMatch ID(s), in tablec5.datmeta.id;meta.maincharn_Seq[*] * when no matches (3)meta.notecharRAJ2000Submm peak centroid Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Submm peak centroid Declination (J2000)pos.eq.dec;meta.mainSFlux density, at 250, 350, 500 or 870um (4)mJyphot.flux.density;em.radiofloate_Srms uncertainty on Flux density (instrumental noise only)mJystat.errorfloatS/NSignal-to-noise ratio (5)stat.snrfloatJ/MNRAS/411/505/matchingCombined catalog with maximum likelihood submm photometry, SED model fits and redshiftsz? Redshiftsrc.redshiftfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeqSequential number, [CCC2011] NNN in Simbadmeta.id;meta.mainintprimaryS250Maximum likelihood flux density at 250ummJyphot.flux.density;em.mm.750-1500GHzinte_S250rms uncertainty on S250 (3)mJystat.errorintS350Maximum likelihood flux density at 350ummJyphot.flux.density;em.mm.750-1500GHzinte_S350rms uncertainty on S350 (3)mJystat.errorintS500Maximum likelihood flux density at 500ummJyphot.flux.density;em.mm.400-750GHzinte_S500rms uncertainty on S500 (3)mJystat.errorintS870Maximum likelihood flux density at 870ummJyphot.flux.density;em.mm.200-400GHzfloate_S870rms uncertainty on S870 (3)mJystat.errorfloatTobs? Observed temperature (4)Kphys.temperaturefloatnullablee_Tobs? rms uncertainty on TobsKstat.errorfloatnullableSTIR? 10-1000um total IR fluxes (log10) (4)log(W.m**-2)phot.flux.density;em.IRfloatnullablee_STIR? Fractional uncertainties in the total IR fluxes (5)stat.errorfloatnullableLTIR? Total IR luminosity (log10)log(solLum)phys.luminosity;em.IRfloatnullablef_z[*)p] Type of redshift (6)meta.codecharr_z[PCID] Redshift reference (7)meta.ref;pos.framecharn_z[a] Note on redshift for source 82 (8)meta.notecharSIMPLE? SIMPLE identification number (1)meta.idintnullableSID? SID870um identification number (1)meta.idintnullableSID250? submm SID for 250um peak (tablec1)meta.idintnullabler250? Radial separation for 250um peakarcsecpos.angDistancefloatnullableL250? Likelihood ratio for 250um peakstat.likelihood;arith.ratiofloatnullablePm250? Random association 24um/250um peak (2)stat.fit.goodnessfloatnullablePr250? Random association 1.4GHz/250um peak (2)stat.fit.goodnessfloatnullableSID350? submm SID for 350um peak (tablec2)meta.idintnullabler350? Radial separation for 350um peakarcsecpos.angDistancefloatnullableL350? Likelihood ratio for 350um peakstat.likelihood;arith.ratiofloatnullablePm350? Random association 24um/350um peak (2)stat.fit.goodnessfloatnullablePr350? Random association 1.4GHz/350um peak (2)stat.fit.goodnessfloatnullableSID500? submm SID for 500um peak (tablec3)meta.idintnullabler500? Radial separation for 500um peakarcsecpos.angDistancefloatnullableL500? Likelihood ratio for 500um peakstat.likelihood;arith.ratiofloatnullablePm500? Random association 24um/500um peak (2)stat.fit.goodnessfloatnullablePr500? Random association 1.4GHz/500um peak (2)stat.fit.goodnessfloatnullableSID870? submm SID for 870um peak (tablec4)meta.idintnullabler870? Radial separation for 870um peakarcsecpos.angDistancefloatnullableL870? Likelihood ratio for 870um peakstat.likelihood;arith.ratiofloatnullablePm870? Random association 24um/500um peak (2)stat.fit.goodnessfloatnullablePr870? Random association 1.4GHz/870um peak (2)stat.fit.goodnessfloatnullableRAJ2000IRAC Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000IRAC Declination (J2000)pos.eq.dec;meta.main