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dc.contributor.authorPerera, T.A.
dc.contributor.authorChapin, E.L.
dc.contributor.authorAustermann, J.E.
dc.contributor.authorScott, K.S.
dc.contributor.authorWilson, G.W.
dc.contributor.authorHalpern, M.
dc.contributor.authorPope, A.
dc.contributor.authorScott, D.
dc.contributor.authorYun, M.S.
dc.contributor.authorLowenthal, J.D.
dc.contributor.authorMorrison, G.
dc.contributor.authorAretxaga, I.
dc.contributor.authorBock, J.J.
dc.contributor.authorCoppin, Kristen
dc.contributor.authorCrowe, M.
dc.contributor.authorFrey, L.
dc.contributor.authorHughes, D.H.
dc.contributor.authorKang, Y.
dc.contributor.authorKim, S.
dc.contributor.authorMauskopf, P. D.
dc.date.accessioned2014-01-27T13:30:30Z
dc.date.available2014-01-27T13:30:30Z
dc.date.issued2008-12-01
dc.identifier.citationPerera , T A , Chapin , E L , Austermann , J E , Scott , K S , Wilson , G W , Halpern , M , Pope , A , Scott , D , Yun , M S , Lowenthal , J D , Morrison , G , Aretxaga , I , Bock , J J , Coppin , K , Crowe , M , Frey , L , Hughes , D H , Kang , Y , Kim , S & Mauskopf , P D 2008 , ' An AzTEC 1.1 mm survey of the GOODS-N field - I : Maps, catalogue and source statistics ' , Monthly Notices of the Royal Astronomical Society , vol. 391 , no. 3 , pp. 1227-1238 . https://doi.org/10.1111/j.1365-2966.2008.13902.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 2712846
dc.identifier.otherPURE UUID: b2ad50c3-fe97-4a7c-8445-3f634d9a77e7
dc.identifier.otherScopus: 57249091444
dc.identifier.otherORCID: /0000-0002-0729-2988/work/30423109
dc.identifier.urihttp://hdl.handle.net/2299/12683
dc.descriptioncopyright Royal Astronomical Society
dc.description.abstractWe have conducted a deep and uniform 1.1 mm survey of the Great Observatories Origins Deep Survey-North (GOODS-N) field with AzTEC on the James Clerk Maxwell Telescope. Here, we present the first results from this survey including maps, the source catalogue and 1.1 mm number counts. The results presented here were obtained from a 245 arcmin region with a near uniform coverage to a depth of 0.96-1.16 mJy beam. Our robust catalogue contains 28 source candidates detected with S/N ≥ 3.75, only ∼1- 2 of which are expected to be spurious detections. Of these source candidates, eight are also detected by Submillimetre Common-User Bolometer Array (SCUBA) at 850 μm in regions where there is a good overlap between the two surveys. The major advantage of our survey over that with SCUBA is the uniformity of coverage. We calculate number counts using two different techniques: the first using a frequentist parameter estimation and the second using a Bayesian method. The two sets of results are in good agreement. We find that the 1.1 mm differential number counts are well described in the 2-6 mJy range by the functional form dN/dS = N′(S′/S) exp(-S/S′) with fitted parameters S′ = 1.25 ± 0.38 mJy and dN/dS = 300 ± 90 mJy deg at 3 mJy.en
dc.format.extent12
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleAn AzTEC 1.1 mm survey of the GOODS-N field - I : Maps, catalogue and source statisticsen
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=57249091444&partnerID=8YFLogxK
rioxxterms.versionSMUR
rioxxterms.versionofrecordhttps://doi.org/10.1111/j.1365-2966.2008.13902.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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