J/MNRAS/468/4006ivo://CDS.VizieR/J/MNRAS/468/4006doi:10.26093/cds/vizier.74684006CDSMackenzie T.P.Scott D.Bianconi M.Clements D.L.Dole H.A.,Flores-Cacho I.Guery D.Kneissl R.Lagache G.Marleau F.R.,Montier L.Nesvadba N.P.H.Pointecouteau E.Soucail G.2024-08-17T20:18:48Z2020-04-15T09:41:14ZCDS support team

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

cds-question@unistra.frgalaxy-clustersredshiftedmillimeter-astronomyphotometrysubmillimeter-astronomyWe present SCUBA-2 follow-up of 61 candidate high-redshift Planck sources. Of these, 10 are confirmed strong gravitational lenses and comprise some of the brightest such submm sources on the observed sky, while 51 are candidate proto-cluster fields undergoing massive starburst events. With the accompanying Herschel-Spectral and Photometric Imaging Receiver observations and assuming an empirical dust temperature prior of 34^+13^_-9_K, we provide photometric redshift and far-IR luminosity estimates for 172 SCUBA-2-selected sources within these Planck overdensity fields. The redshift distribution of the sources peak between a redshift of 2 and 4, with one-third of the sources having S_500_/S_350_>1. For the majority of the sources, we find far-IR luminosities of approximately 10^13^L_{sun}_, corresponding to star formation rates of around 1000M_{sun}_/yr. For S_850_>8mJy sources, we show that there is up to an order of magnitude increase in star formation rate density and an increase in uncorrected number counts of 6 for S_850_>8mJy when compared to typical cosmological survey fields. The sources detected with SCUBA-2 account for only approximately 5 per cent of the Planck flux at 353 GHz, and thus many more fainter sources are expected in these fields.2017MNRAS.468.4006Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/468/4006CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/468/4006https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/468/4006http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/468/4006https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/468/4006https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/468/4006http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/468/4006GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/468/4006/table1 (SCUBA-2-detected sources within the Planck proto-cluster candidate fields)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/468/4006/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/468/4006/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/468/4006/table1?GETtext/xml+votable180.050000true324.96272917-8.7880.0055555555555555566/4182 4456-4457 4599 4710 4726 5329 5412 5545 5550 5737 5890 6514 6520 7238 7364 8377 8857 9188 9575 9703 9722 9969 10133 10790 11335 11417 11557 16702 16725 16749 16861 16881 17107 17204 17206 17223 17314 17524 17722 18736 18949 26519 28390 35817 35820 36529 36553 48497 489832.3390025583187276e-22 2.3390025583187276e-22https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/468/4006?format=asciiMillimeterdefaultJ/MNRAS/468/4006/table1SCUBA-2-detected sources within the Planck proto-cluster candidate fieldsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintGalaxyGalaxy namemeta.id;meta.maincharRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainS850Flux density at 850ummJyphot.flux.density;em.mm.200-400GHzfloate_S850Flux density at 850um error (1)mJystat.errorfloatl_zphLimit flag on zph (2)meta.code.errorcharzphPhotometric redshiftsrc.redshiftfloatE_zph? Photometric redshift error (upper value) (3)stat.error;stat.maxfloatnullablee_zph? Photometric redshift error (lower value) (3)stat.errorfloatnullableLFIRFar-IR luminositylog(solLum)phys.luminosity;em.IRdoubleE_LFIR? Far-IR luminosity error (upper value) (3)log(solLum)stat.error;stat.maxdoublenullablee_LFIR? Far-IR luminosity error (lower value) (3)log(solLum)stat.errordoublenullablePLCK?[Y/N] In Planck beam ?meta.codechar