J/MNRAS/368/1223ivo://CDS.VizieR/J/MNRAS/368/1223doi:10.26093/cds/vizier.73681223CDSHill T.Thompson M.A.Burton M.G.Walsh A.J.Minier V.Cunningham M.R.,Pierce-Price D.2024-07-02T20:17:17Z2006-12-11T21:42:09ZCDS support team

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

cds-question@unistra.frh-ii-regionsastrophysical-masersradio-astronomyradio-sourcesmillimeter-astronomysubmillimeter-astronomyWe report the results of a submillimetre continuum emission survey targeted towards 78 star formation regions, 72 of which are devoid of methanol maser and UC HII regions, identified in the Swedish ESO Submillimetre Telescope (SEST)/SEST IMaging Bolometer Array (SIMBA) millimetre continuum survey of Hill et al. (2005, Cat. <J/MNRAS/363/405>). At least 45 per cent of the latter sources, dubbed 'mm-only', detected in this survey are also devoid of the mid-infrared MSX emission. The 450- and 850-um continuum emission was mapped using the Submillimetre Common User Bolometer Array (SCUBA) instrument on the James Clerk Maxwell Telescope (JCMT). Emission is detected towards 97 per cent of the 78 sources targeted as well as towards 28 other SIMBA sources lying in the SCUBA fields. In total, we have identified 212 cores in this submillimetre survey, including 106 previously known from the SIMBA survey. Of the remaining 106 sources, 53 result from resolving a SIMBA source into multiple submillimetre components, whilst the other 53 sources are submillimetre cores, not seen in the SIMBA. Additionally, we have identified two further mm-only sources in the SIMBA images. Of the total 405 sources identified in the SIMBA survey, 255 are only seen at millimetre wavelengths.2006MNRAS.368.1223Hhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/368/1223CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/MNRAS/363/405 : SIMBA observations of cold cores (Hill+, 2005)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/368/1223https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/368/1223http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/368/1223https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/368/1223https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/368/1223http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/368/1223GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/368/1223/table3 (Parameters for the 212 submillimetre continuum sources found in the SCUBA survey)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/368/1223/table3?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/368/1223/table3?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/368/1223/table3?GETtext/xml+votable180.050000true266.47625-28.7355560.005555555555555556Cone search capability for table J/MNRAS/368/1223/table4 (171 SIMBA sources with corresponding SCUBA data and the dust grain emissivity index beta.)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/368/1223/table4?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/368/1223/table4?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/368/1223/table4?GETtext/xml+votable180.050000true92.27708321.8408330.0055555555555555566/14353 24325 28829-28831 28890 28896 28912-28913 28918-28919 29070 29090-29092 29094 29096-29097 29100-29101 29103 29114-29116 29160 29461 29505 29510-29511 29529 29532-29533 29535 29553 30218-30219 30241 30256 30259 30262-30263 30268-30269 30312-30313 30318-30319 30405 30420 30693-30694https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/368/1223?format=asciiRadiodefaultJ/MNRAS/368/1223/table3Parameters for the 212 submillimetre continuum sources found in the SCUBA surveyrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000Peak right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Peak declination (J2000)pos.eq.dec;meta.main[HTB2006]Source name (1)meta.id;meta.maincharXSimbad column added by the CDSmeta.ref.urlcharTracerTracer (G2)meta.notecharTargetIdentifier SIMBA targetmeta.idcharF450um? Integrated 450um fluxJyphot.flux.density;em.mm.400-750GHzfloatnullablen_F450um[aefgpxznN ] Note on F450um (G1)meta.notecharFP450um? Peak 450um fluxJyphot.flux.density;em.mm.400-750GHzfloatnullablen_FP450um[n] Note on FP450um (G1)meta.notecharF850um? Integrated 850um flux (in Jy/beam)Jyphot.flux.density;em.mm.200-400GHzfloatnullablen_F850um[adgpxzN ] Note on F850um (G1)meta.notecharFP850um? Peak 850um flux (in Jy/beam)Jyphot.flux.density;em.mm.200-400GHzfloatnullableCorIndicates the SIMBA association for the submillimetre cores detected in this survey (4)meta.codecharJ/MNRAS/368/1223/table4171 SIMBA sources with corresponding SCUBA data and the dust grain emissivity index beta.RefReference (6)meta.bibcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000Peak right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Peak declination (J2000)pos.eq.dec;meta.mainn_[HBM2005][*] * for sources not in Paper Imeta.notechar[HBM2005]Source name (1)meta.id;meta.maincharXSimbad column added by the CDSmeta.ref.urlcharTracerTracer (G2)meta.notecharF1200um? Integrated flux at 1200umJyphot.flux.density;em.mm.200-400GHzfloatnullablen_F1200um[ag] Note on F1200um (G1)meta.notecharF850um? Integrated flux at 850umJyphot.flux.density;em.mm.200-400GHzfloatnullablel_F450umLimit flag on F450ummeta.code.errorcharF450um? Integrated flux at 450umJyphot.flux.density;em.mm.400-750GHzfloatnullablen_F450um[nNe] Note on F450um (G1)meta.notecharNote[lac] SIMBA core resolved into multiple components by SCUBA (5)meta.notecharbeta10K? Dust emissivity exponent beta at Tdust=10K (error are typically 20%)stat.fit.paramfloatnullablebeta20K? Dust emissivity exponent beta at Tdust=20K (error are typically 30%)stat.fit.paramfloatnullablebeta30K? Dust emissivity exponent beta at Tdust=30K (error are typically 30%)stat.fit.paramfloatnullablebeta40K? Dust emissivity exponent beta at Tdust=40K (error are typically 30%)stat.fit.paramfloatnullablebeta50K? Dust emissivity exponent beta at Tdust=50K (error are typically 30%)stat.fit.paramfloatnullablePapIData from Paper I, Cat. <J/MNRAS/363/405>meta.ref.urlchar