J/MNRAS/486/4166ivo://CDS.VizieR/J/MNRAS/486/4166doi:10.26093/cds/vizier.74864166CDSSmith M.W.L.Clark C.J.R.De Looze I.Lamperti I.Saintonge A.,Wilson C.D.Accurso G.Brinks E.Bureau M.Chung E.J.Cigan P.J.,Clements D.L.Dharmawardena T.Fanciullo L.Gao Y.Gao Y.Gear W.K.,Gomez H.L.Greenslade J.Hwang H.S.Kemper F.Lee J.C.Li C.Lin L.,Liu L.Molnar D.C.Mok A.Pan H.-A.Sargent M.Scicluna P.,Smith C.M.A.Urquhart S.Williams T.G.Xiao T.Yang C.Zhu M.2024-08-19T20:18:23Z2022-12-09T13:44:22ZCDS support team

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

cds-question@unistra.frgalaxiesphotometrycatalogsinfrared-photometrymillimeter-astronomysubmillimeter-astronomyWe present the SCUBA-2 850{mu}m component of JINGLE, the new JCMT large survey for dust and gas in nearby galaxies, which with 193 galaxies is the largest targeted survey of nearby galaxies at 850{mu}m. We provide details of our SCUBA-2 data reduction pipeline, optimized for slightly extended sources, and including a calibration model adjusted to match conventions used in other far-infrared (FIR) data. We measure total integrated fluxes for the entire JINGLE sample in 10 infrared/submillimetre bands, including all WISE, Herschel-PACS, Herschel-SPIRE, and SCUBA-2 850{mu}m maps, statistically accounting for the contamination by CO(J=3-2) in the 850{mu}m band. Of our initial sample of 193 galaxies, 191 are detected at 250{mu}m with a >=5{sigma} significance. In the SCUBA-2 850{mu}m band we detect 126 galaxies with >=3{sigma} significance. The distribution of the JINGLE galaxies in FIR/sub-millimetre colour-colour plots reveals that the sample is not well fit by single modified-blackbody models that assume a single dust-emissivity index ({beta}). Instead, our new 850{mu}m data suggest either that a large fraction of our objects require {beta}<1.5, or that a model allowing for an excess of sub-mm emission (e.g. a broken dust emissivity law, or a very cold dust component~<10K) is required. We provide relations to convert FIR colours to dust temperature and {beta} for JINGLE-like galaxies. For JINGLE the FIR colours correlate more strongly with star-formation rate surface-density rather than the stellar surface-density, suggesting heating of dust is greater due to younger rather than older stellar-populations, consistent with the low proportion of early-type galaxies in the sample.2019MNRAS.486.4166Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/486/4166CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/MNRAS/481/3497 : JINGLE, Survey overview and first results (Saintonge+, 2018)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/486/4166https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/486/4166http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/486/4166https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/486/4166https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/486/4166http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/486/4166GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/486/4166/jingle (JINGLE catalog)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/486/4166/jingle?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/486/4166/jingle?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/486/4166/jingle?GETtext/xml+votable180.050000true199.071412525.40669720.0055555555555555565/2593-2594 2610 6/10253 10259 10264 10267 10269 10271 10282 10285-10286 10289-10294 10296-10297 10302 10336 10342 10345-10346 10348 10350-10351 10368 10371 10380-10381 10383-10385 10389 10391 10393-10398 10400-10402 10404 10415 10419 10421-10423 10428-10429 10432 10434 10438-10439 10444-10446 10449 10464-10466 21845 21847 21849 21852-21854 21879 25596 25917 25919 25935 25944 25946-25947 25961 25964 25966 25976 26005 26051 26254-26255 26275-26276 26279 26282 26286 26956 26962 26965-26966 26971 26996 27300 27303 27305 27324 27648 27650 28118 28127 409592.3390025583187276e-22 6.513807192489934e-20https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/486/4166?format=asciiInfraredMillimeterdefaultJ/MNRAS/486/4166/jingleJINGLE catalogSimbadNameSimbad column added by the CDSmeta.idcharnullablee_FW4.6Error on FW4.6mJystat.errordoubleACFW4.6? WISE 4.6um Aperture Correction Factorinstr.paramdoublenullableSNRW12WISE 12um Peak Signal-To-Noise Ratiostat.snrdoubleFW12? WISE 12um Flux DensitymJyphot.flux.density;em.IR.8-15umdoublenullablee_FW12Error on FW12mJystat.errordoubleACFW12? WISE 12um Aperture Correction Factorinstr.paramdoublenullableSNRW22WISE 22um Peak Signal-To-Noise Ratiostat.snrdoubleFW22? WISE 22um Flux DensitymJyphot.flux.density;em.IR.15-30umdoublenullablee_FW22Error on FW22mJystat.errordoubleACFW22? WISE 22um Aperture Correction Factorinstr.paramdoublenullableSNRP100? PACS 100um Peak Signal-To-Noise Ratiostat.snrfloatnullableFP100? PACS 100um Flux DensitymJyphot.flux.density;em.IR.60-100umdoublenullablee_FP100? Error on FP100mJystat.errordoublenullableACFP100? PACS 100um Aperture Correction Factorinstr.paramdoublenullableSNRP160? PACS 160um Peak Signal-To-Noise Ratiostat.snrdoublenullableFP160? PACS 160um Flux DensitymJyphot.flux.density;em.mm.1500-3000GHzdoublenullablee_FP160? Error on FP160mJystat.errordoublenullableACFP160? PACS 160um Aperture Correction Factorinstr.paramdoublenullablemetS250[0/1] SPIRE 250um Extraction Method (2)meta.codeintSNRS250SPIRE 250um Peak Signal-To-Noise Ratiostat.snrdoubleFS250? SPIRE 250um Flux DensitymJyphot.flux.density;em.mm.750-1500GHzdoublenullablee_FS250Error on FS250mJystat.errordoubleACF250? SPIRE 250um Aperture Correction Factorinstr.paramdoublenullablemetS350[0/1] SPIRE 250um Extraction Method (2)meta.codeintSNRS350SPIRE 350um Peak Signal-To-Noise Ratiostat.snrfloatFS350? SPIRE 350um Flux DensitymJyphot.flux.density;em.mm.750-1500GHzdoublenullablee_FS350Error on FS350mJystat.errordoubleACF350? SPIRE 350um Aperture Correction Factorinstr.paramdoublenullablemetS500[0/1] SPIRE 500um Extraction Method (2)meta.codeintSNRS500SPIRE 500um Peak Signal-To-Noise Ratiostat.snrfloatFS500? SPIRE 500um Flux DensitymJyphot.flux.density;em.mm.400-750GHzdoublenullablee_FS500Error on FS500mJystat.errordoubleACF500? SPIRE 500um Aperture Correction Factorinstr.paramdoublenullablemetS850SCUBA2 850um Extraction Method (2)meta.codeintSNRS850SCUBA2 850um Peak Signal-To-Noise Ratiostat.snrfloatFSCO32SCUBA2 850um Predicted CO(3-2) Flux Density ContaminationmJyphot.flux.density;em.mm.200-400GHzfloatFS850? SCUBA2 850um Flux Density (CO(3-2) Corrected)mJyphot.flux.density;em.mm.200-400GHzdoublenullablee_FS850Error on FS850mJystat.errordoubleACFS850? SCUBA2 850um Aperture Correction Factorinstr.paramdoublenullableFCFS850? SCUBA2 850um Filter Correction Factorinstr.paramdoublenullablea250? Aperture Major Radius at 250um (3)arcsecphys.angSizefloatnullableb250? Aperture Minor Radius at 250um (3)arcsecphys.angSize;srcfloatnullableAperPA? Aperture Position Angledegpos.posAng;instr.fovdoublenullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintID[0/192] JINGLE Catalogue IDmeta.idintFlagph[0-2] Photometry Flag (1)meta.code.errorintSNRW3.4WISE 3.4um Peak Signal-To-Noise Ratiostat.snrdoubleFW3.4? WISE 3.4um Flux DensitymJyphot.mag;em.IR.3-4umdoublenullablee_FW3.4Error on FW3.4mJystat.errordoubleACFW3.4? WISE 3.4um Aperture Correction Factorinstr.paramdoublenullableSNRW4.6WISE 4.6um Peak Signal-To-Noise Ratiostat.snrdoubleFW4.6? WISE 4.6um Flux DensitymJyphot.mag;em.IR.4-8umdoublenullable_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.main_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainNameSDSS name (JHHMMSS.ss+DDMMSS.s)meta.id;meta.mainchar