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dc.contributor.authorEden, D.~J.
dc.contributor.authorMoore, T. J. T.
dc.contributor.authorPlume, R.
dc.contributor.authorUrquhart, J.S.
dc.contributor.authorThompson, M. A.
dc.contributor.authorParsons, H.
dc.contributor.authorDempsey, J. T.
dc.contributor.authorRigby, A.~J.
dc.contributor.authorMorgan, L. K.
dc.contributor.authorThomas, H. S.
dc.contributor.authorBerry, D J
dc.contributor.authorBuckle, J.
dc.contributor.authorBrunt, Christopher M.
dc.contributor.authorButner, H. M.
dc.contributor.authorCarretero, D.
dc.contributor.authorChrysostomou, A.
dc.contributor.authorCurrie, M. J.
dc.contributor.authordeVilliers, H.~M.
dc.contributor.authorFich, M.
dc.contributor.authorGibb, A. G.
dc.contributor.authorHoare, M.G.
dc.contributor.authorJenness, T.
dc.contributor.authorManser, G.
dc.contributor.authorMottram, J.~C.
dc.contributor.authorNatario, C.
dc.contributor.authorOlguin, F.
dc.contributor.authorPeretto, N.
dc.contributor.authorPestalozzi, M.
dc.contributor.authorPolychroni, D.
dc.contributor.authorRedman, R.~O.
dc.contributor.authorSalji, C.
dc.contributor.authorSummers, L.~J.
dc.contributor.authorTahani, K.
dc.contributor.authorTraficante, A.
dc.contributor.authordiFrancesco, J.
dc.contributor.authorEvans, A.
dc.contributor.authorFuller, G. A.
dc.contributor.authorJohnstone, D.
dc.contributor.authorJoncas, G.
dc.contributor.authorLongmore, S.~N.
dc.contributor.authorMartin, Gary P
dc.contributor.authorRicher, J. S.
dc.contributor.authorWeferling, B.
dc.contributor.authorWhite, Glenn J.
dc.contributor.authorZhu, M.
dc.date.accessioned2017-08-03T14:20:06Z
dc.date.available2017-08-03T14:20:06Z
dc.date.issued2017-08-01
dc.identifier.citationEden , D J , Moore , T J T , Plume , R , Urquhart , J S , Thompson , M A , Parsons , H , Dempsey , J T , Rigby , A J , Morgan , L K , Thomas , H S , Berry , D J , Buckle , J , Brunt , C M , Butner , H M , Carretero , D , Chrysostomou , A , Currie , M J , deVilliers , H M , Fich , M , Gibb , A G , Hoare , M G , Jenness , T , Manser , G , Mottram , J C , Natario , C , Olguin , F , Peretto , N , Pestalozzi , M , Polychroni , D , Redman , R O , Salji , C , Summers , L J , Tahani , K , Traficante , A , diFrancesco , J , Evans , A , Fuller , G A , Johnstone , D , Joncas , G , Longmore , S N , Martin , G P , Richer , J S , Weferling , B , White , G J & Zhu , M 2017 , ' The JCMT Plane Survey : First complete data release - emission maps and compact source catalogue ' , Monthly Notices of the Royal Astronomical Society , vol. 469 , no. 2 , pp. 2163-2183 . https://doi.org/10.1093/mnras/stx874
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 11698451
dc.identifier.otherPURE UUID: e7c17207-5190-4127-88b0-8fdb34c59056
dc.identifier.otherArXiv: http://arxiv.org/abs/1704.02982v1
dc.identifier.otherORCID: /0000-0001-5392-909X/work/42466472
dc.identifier.urihttp://hdl.handle.net/2299/19111
dc.descriptionThis article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. © 2017 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. Full version of Table 3 available from http://www.canfar.phys.uvic.ca/vosui/#/JPSPR1
dc.description.abstractWe present the first data release of the James Clerk Maxwell Telescope (JCMT) Plane Survey (JPS), the JPS Public Release 1 (JPSPR1). JPS is an 850-um continuum survey of six fields in the northern inner Galactic Plane in a longitude range of l=7-63, made with the Sub-millimetre Common-User Bolometer Array 2 (SCUBA-2). This first data release consists of emission maps of the six JPS regions with an average pixel-to-pixel noise of 7.19 mJy beam^-1, when smoothed over the beam, and a compact-source catalogue containing 7,813 sources. The 95 per cent completeness limits of the catalogue are estimated at 0.04 Jy beam^-1 and 0.3 Jy for the peak and integrated flux densities, respectively. The emission contained in the compact-source catalogue is 42 +- 5 per cent of the total and, apart from the large-scale (greater than 8') emission, there is excellent correspondence with features in the 500-um Herschel maps. We find that, with two-dimensional matching, 98 +- 2 per cent of sources within the fields centred at l=20, 30, 40 and 50 are associated with molecular clouds, with 91 +- 3 per cent of the l=30 and 40 sources associated with dense molecular clumps. Matching the JPS catalogue to Herschel 70-um sources, we find that 38 +- 1 per cent of sources show evidence of ongoing star formation. The images and catalogue will be a valuable resource for studies of star formation in the Galaxy and the role of environment and spiral arms in the star formation process.en
dc.format.extent24
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.rightsOpen
dc.subjectsurveys
dc.subjectstars: formation
dc.subjectISM: clouds
dc.subjectsubmillimetre: ISM
dc.titleThe JCMT Plane Survey : First complete data release - emission maps and compact source catalogueen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeFinal Published version
dcterms.dateAccepted2017-08-01
rioxxterms.versionVoR
rioxxterms.versionofrecordhttps://doi.org/10.1093/mnras/stx874
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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