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A Detailed Gravitational Lens Model Based on Submillimeter Array and Keck Adaptive Optics Imaging of a Herschel-ATLAS Sub-millimeter Galaxy at z=4.243

dc.contributor.authorS. Bussmann, R.
dc.contributor.authorA. Gurwell, M.
dc.contributor.authorFu, Hai
dc.contributor.authorSmith, Daniel
dc.contributor.authorDye, S.
dc.contributor.authorAuld, R.
dc.contributor.authorBaes, M.
dc.contributor.authorJ. Baker, A.
dc.contributor.authorBonfield, D.
dc.contributor.authorCava, A.
dc.contributor.authorL. Clements, D.
dc.contributor.authorCooray, A.
dc.contributor.authorCoppin, Kristen
dc.contributor.authorDannerbauer, H.
dc.contributor.authorDariush, A.
dc.contributor.authorDe Zotti, G.
dc.contributor.authorDunne, L.
dc.contributor.authorEales, S.
dc.contributor.authorFritz, J.
dc.contributor.authorHopwood, R.
dc.contributor.authorIbar, E.
dc.contributor.authorJ. Ivison, R.
dc.contributor.authorJarvis, M.J.
dc.contributor.authorKim, S.
dc.contributor.authorL. Leeuw, L.
dc.contributor.authorMaddox, S.
dc.contributor.authorJ. Michalowski, M.
dc.contributor.authorNegrello, M.
dc.contributor.authorPascale, E.
dc.contributor.authorPohlen, M.
dc.contributor.authorA. Riechers, D.
dc.contributor.authorRigby, E.
dc.contributor.authorScott, Douglas
dc.contributor.authorTemi, P.
dc.contributor.authorP. Van der Werf, P.
dc.contributor.authorVerma, A.
dc.contributor.authorWardlow, J.
dc.contributor.authorWilner, D.
dc.date.accessioned2013-02-06T11:00:08Z
dc.date.available2013-02-06T11:00:08Z
dc.date.issued2012-09-10
dc.identifier.citationS. Bussmann , R , A. Gurwell , M , Fu , H , Smith , D , Dye , S , Auld , R , Baes , M , J. Baker , A , Bonfield , D , Cava , A , L. Clements , D , Cooray , A , Coppin , K , Dannerbauer , H , Dariush , A , De Zotti , G , Dunne , L , Eales , S , Fritz , J , Hopwood , R , Ibar , E , J. Ivison , R , Jarvis , M J , Kim , S , L. Leeuw , L , Maddox , S , J. Michalowski , M , Negrello , M , Pascale , E , Pohlen , M , A. Riechers , D , Rigby , E , Scott , D , Temi , P , P. Van der Werf , P , Verma , A , Wardlow , J & Wilner , D 2012 , ' A Detailed Gravitational Lens Model Based on Submillimeter Array and Keck Adaptive Optics Imaging of a Herschel-ATLAS Sub-millimeter Galaxy at z=4.243 ' , The Astrophysical Journal , vol. 756 , no. 2 , 134 . https://doi.org/10.1088/0004-637X/756/2/134
dc.identifier.issn0004-637X
dc.identifier.otherPURE: 1328470
dc.identifier.otherPURE UUID: cafdccfd-a5ee-4053-bfa9-eb380006bdd7
dc.identifier.otherScopus: 84865609973
dc.identifier.otherArXiv: http://arxiv.org/abs/1207.2724v1
dc.identifier.otherORCID: /0000-0002-0729-2988/work/30423069
dc.identifier.otherORCID: /0000-0001-9708-253X/work/69424339
dc.identifier.urihttp://hdl.handle.net/2299/9919
dc.descriptionCopyright 2012 Elsevier B.V., All rights reserved.
dc.description.abstractWe present high-spatial resolution imaging obtained with the Submillimeter Array (SMA) at 880 μm and the Keck Adaptive Optics (AO) system at KS-band of a gravitationally lensed sub-millimeter galaxy (SMG) at z = 4.243 discovered in the Herschel Astrophysical Terahertz Large Area Survey.en
dc.format.extent11
dc.language.isoeng
dc.relation.ispartofThe Astrophysical Journal
dc.titleA Detailed Gravitational Lens Model Based on Submillimeter Array and Keck Adaptive Optics Imaging of a Herschel-ATLAS Sub-millimeter Galaxy at z=4.243en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=84865609973&partnerID=8YFLogxK
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1088/0004-637X/756/2/134
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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