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dc.contributor.authorCoppin, K.en_US
dc.contributor.authorChapin, E. L.en_US
dc.contributor.authorMortier, A. M. J.en_US
dc.contributor.authorScott, S. E.en_US
dc.contributor.authorBorys, C.en_US
dc.contributor.authorDunlop, J. S.en_US
dc.contributor.authorHalpern, M.en_US
dc.contributor.authorHughes, D. H.en_US
dc.contributor.authorPope, A.en_US
dc.contributor.authorScott, D.en_US
dc.contributor.authorSerjeant, S.en_US
dc.contributor.authorWagg, J.en_US
dc.contributor.authorAlexander, D. M.en_US
dc.contributor.authorAlmaini, O.en_US
dc.contributor.authorAretxaga, I.en_US
dc.contributor.authorBabbedge, T.en_US
dc.contributor.authorBest, P. N.en_US
dc.contributor.authorBlain, A.en_US
dc.contributor.authorChapman, S.en_US
dc.contributor.authorClements, D. L.en_US
dc.contributor.authorCrawford, M.en_US
dc.contributor.authorDunne, L.en_US
dc.contributor.authorEales, S. A.en_US
dc.contributor.authorEdge, A. C.en_US
dc.contributor.authorFarrah, D.en_US
dc.contributor.authorGaztanaga, E.en_US
dc.contributor.authorGear, W. K.en_US
dc.contributor.authorGranato, G. L.en_US
dc.contributor.authorGreve, T. R.en_US
dc.contributor.authorFox, M.en_US
dc.contributor.authorIvison, R. J.en_US
dc.contributor.authorJarvis, M. J.en_US
dc.contributor.authorJenness, T.en_US
dc.contributor.authorLacey, C.en_US
dc.contributor.authorLepage, K.en_US
dc.contributor.authorMann, R. G.en_US
dc.contributor.authorMarsden, G.en_US
dc.contributor.authorMartinez-Sansigre, A.en_US
dc.contributor.authorOliver, S.en_US
dc.contributor.authorPage, M. J.en_US
dc.contributor.authorPeacock, J. A.en_US
dc.contributor.authorPearson, C. P.en_US
dc.contributor.authorPercival, W. J.en_US
dc.contributor.authorPriddey, R. S.en_US
dc.contributor.authorRawlings, S.en_US
dc.contributor.authorRowan-Robinson, M.en_US
dc.contributor.authorSavage, R. S.en_US
dc.contributor.authorSeigar, M.en_US
dc.contributor.authorSekiguchi, K.en_US
dc.contributor.authorSilva, L.en_US
dc.contributor.authorSimpson, C.en_US
dc.contributor.authorSmail, I.en_US
dc.contributor.authorStevens, J. A.en_US
dc.contributor.authorTakagi, T.en_US
dc.contributor.authorVaccari, M.en_US
dc.contributor.authorvan Kampen, E.en_US
dc.contributor.authorWillott, C. J.en_US
dc.date.accessioned2014-03-12T19:20:49Z
dc.date.available2014-03-12T19:20:49Z
dc.date.issued2006-11-11en_US
dc.identifier.citationCoppin, K., E. L. Chapin, A. M. J. Mortier, S. E. Scott, et al. 2006. "The SCUBA HAlf Degree Extragalactic Survey (SHADES) -- II. Submillimetre maps, catalogue and number counts." Monthly Notices of the Royal Astronomical Society 372(4): 1621-1652en_US
dc.identifier.issn0035-8711en_US
dc.identifier.urihttp://dx.doi.org/10.1111/j.1365-2966.2006.10961.xen_US
dc.identifier.urihttp://hdl.handle.net/10222/45281
dc.description.abstractWe present the maps, source catalogue and number counts of the largest, most complete and unbiased extragalactic submillimetre survey ever undertaken: the 850-micron 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). These SCUBA maps cover 720 square arcmin with an RMS noise level of about 2 mJy 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 sub-groups drawn 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. We present differential and integral source number counts of submillimetre galaxies 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 an 850-micron survey complete down to 2 mJy would resolve 20-30 per cent of the Far-IR background into point sources. [abridged]en_US
dc.titleThe SCUBA HAlf Degree Extragalactic Survey (SHADES) -- II. Submillimetre maps, catalogue and number countsen_US
dc.title.alternativeMonthly Notices of the Royal Astronomical Societyen_US
dc.typearticleen_US
dc.identifier.volume372en_US
dc.identifier.issue4en_US
dc.identifier.startpage1621en_US
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