J/MNRAS/372/1621ivo://CDS.VizieR/J/MNRAS/372/1621doi:10.26093/cds/vizier.73721621CDSCoppin K.Chapin E.L.Mortier A.M.J.Scott S.E.Borys C.Dunlop J.S.,Halpern M.Hughes D.H.Pope A.Scott D.Serjeant S.Wagg J.,Alexander D.M.Almaini O.Aretxaga I.Babbedge T.Best P.N.Blain A.,Chapman S.Clements D.L.Crawford M.Dunne L.Eales S.A.Edge A.C.,Farrah D.Gaztanaga E.Gear W.K.Granato G.L.Greve T.R.Fox M.,Ivison R.J.Jarvis M.J.Jenness T.Lacey C.Lepage K.Mann R.G.,Marsden G.Martinez-Sansigre A.Oliver S.Page M.J.Peacock J.A.,Pearson C.P.Percival W.J.Priddey R.S.Rawlings S.Rowan-Robinson M.,Savage R.S.Seigar M.Sekiguchi K.Silva L.Simpson C.Smail I.,Stevens J.A.Takagi T.Vaccari M.Van Kampen E.Willott C.J.2024-07-03T20:14:27Z2008-12-12T14:28:47ZCDS support team

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

cds-question@unistra.frsurveysmillimeter-astronomysubmillimeter-astronomyWe present maps, source catalogue and number counts of the largest, most complete and unbiased extragalactic submillimetre survey: the 850-m SCUBA Half-Degree Extragalactic Survey (SHADES). Using the Submillimetre Common-User Bolometer Array (SCUBA) on the James Clerk Maxwell Telescope (JCMT), SHADES mapped two separate regions of sky: the Subaru/XMM-Newton Deep Field (SXDF) and the Lockman Hole East (LH). Encompassing 93 per cent of the overall acquired data (i.e. data taken up to 2004 February 1), these SCUBA maps cover 720arcmin^2^ with a rms noise level of about 2mJy and have uncovered >100 submillimetre galaxies. In order to ensure the utmost robustness of the resulting source catalogue, data reduction was independently carried out by four subgroups within the SHADES team, providing an unprecedented degree of reliability with respect to other SCUBA catalogues available from the literature. Individual source lists from the four groups were combined to produce a robust 120-object SHADES catalogue; an invaluable resource for follow-up campaigns aiming to study the properties of a complete and consistent sample of submillimetre galaxies. For the first time, we present deboosted flux densities for each submillimetre galaxy found in a large survey. Extensive simulations and tests were performed separately by each group in order to confirm the robustness of the source candidates and to evaluate the effects of false detections, completeness and flux density boosting. Corrections for these effects were then applied to the data to derive the submillimetre galaxy source counts. SHADES has a high enough number of detected sources that meaningful differential counts can be estimated, unlike most submillimetre surveys which have to consider integral counts. We present differential and integral source number counts and find that the differential counts are better fit with a broken power law or a Schechter function than with a single power law; the SHADES data alone significantly show that a break is required at several mJy, although the precise position of the break is not well constrained. We > also find that a 850-m survey complete down to 2mJy would resolve > 20-30 per cent of the far-infrared background into point sources.2006MNRAS.372.1621Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/372/1621CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/MNRAS/370/1057 : Blank-field SCUBA surveys (Scott+ 2006)J/MNRAS/379/1571 : SCUBA Half-Degree Extragalactic Survey. IV (Aretxaga+, 2007)J/MNRAS/380/199 : SCUBA Half-Degree Extragalactic Survey. III (Ivison+, 2007)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/372/1621https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/372/1621http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/372/1621https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/372/1621https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/372/1621http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/372/1621GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/372/1621/table2 (The 850-um SHADES catalogue for the LH and SXDF regions)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/372/1621/table2?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/372/1621/table2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/372/1621/table2?GETtext/xml+votable180.050000true163.005916757.41194440.0055555555555555566/6069 17690https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/372/1621?format=asciiRadiodefaultJ/MNRAS/372/1621/table2The 850-um SHADES catalogue for the LH and SXDF regionsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint[CCM2006]Name (LOCK850.NNN or SXDF850.NNN)meta.id;meta.maincharRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainS850umFlux density at 850ummJyphot.flux.density;em.mm.200-400GHzfloatE_S850umError on S850um (Upper limit)mJystat.error;stat.maxfloate_S850umError on S850um (Lower limit)mJystat.errorfloatS/Nmap signal-to-noise rationstat.snr;obs.fieldfloatMapS850Map noise estimate at 850ummJystat.snr;instr.det.noisefloatl_S450umLimit flag on S450ummeta.code.errorcharS450umFlux density at 450um (3{sigma} limit)mJyphot.flux.density;em.mm.400-750GHzintn_S450um[g] Note on S450um (1)meta.notecharComComments (2)meta.noteNotesIndividual notes (1)meta.notecharPapIIIDisplay the data from Paper III (Ivison et al. 2007, Cat. J/MNRAS/380/199)meta.ref.urlcharPapIVDisplay the data from Paper IV (Aretxaga et al. 2007, Cat. J/MNRAS/379/1571)meta.ref.urlcharSHADESSHADES designation (JHHMMSS+DDMMSS)meta.idchar