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dc.contributor.authorSCOPE Collaboration
dc.contributor.authorEden, D. J.
dc.contributor.authorLiu, Tie
dc.contributor.authorKim, Kee-Tae
dc.contributor.authorLiu, S. -Y.
dc.contributor.authorTatematsu, K.
dc.contributor.authorFrancesco, J. Di
dc.contributor.authorWang, K.
dc.contributor.authorThompson, M. A.
dc.contributor.authorFuller, G. A.
dc.contributor.authorLi, Di
dc.contributor.authorRistorcelli, I.
dc.contributor.authorKang, Sung-ju
dc.contributor.authorHirano, N.
dc.contributor.authorJohnstone, D.
dc.contributor.authorLin, Y.
dc.contributor.authorHe, J. H.
dc.contributor.authorKoch, P. M.
dc.contributor.authorSanhueza, Patricio
dc.contributor.authorQin, S. -L.
dc.contributor.authorZhang, Q.
dc.contributor.authorGoldsmith, P. F.
dc.contributor.authorN., J. Evans II
dc.contributor.authorYuan, J.
dc.contributor.authorZhang, C. -P.
dc.contributor.authorWhite, G. J.
dc.contributor.authorChoi, Minho
dc.contributor.authorLee, Chang Won
dc.contributor.authorToth, L. V.
dc.contributor.authorMairs, S.
dc.contributor.authorYi, H. -W.
dc.contributor.authorTang, M.
dc.contributor.authorSoam, A.
dc.contributor.authorPeretto, N.
dc.contributor.authorSamal, M. R.
dc.contributor.authorFich, M.
dc.contributor.authorParsons, H.
dc.contributor.authorMalinen, J.
dc.contributor.authorBendo, G. J.
dc.contributor.authorRivera-Ingraham, A.
dc.contributor.authorLiu, H. -L.
dc.contributor.authorWouterloot, J.
dc.contributor.authorLi, P. S.
dc.contributor.authorQian, L.
dc.contributor.authorRawlings, J.
dc.contributor.authorRawlings, M. G.
dc.contributor.authorFeng, S.
dc.contributor.authorWang, B.
dc.contributor.authorLi, Dalei
dc.contributor.authorLiu, M.
dc.contributor.authorChrysostomou, A.
dc.date.accessioned2019-06-04T01:02:20Z
dc.date.available2019-06-04T01:02:20Z
dc.date.issued2019-05-01
dc.identifier.citationSCOPE Collaboration , Eden , D J , Liu , T , Kim , K-T , Liu , S -Y , Tatematsu , K , Francesco , J D , Wang , K , Thompson , M A , Fuller , G A , Li , D , Ristorcelli , I , Kang , S , Hirano , N , Johnstone , D , Lin , Y , He , J H , Koch , P M , Sanhueza , P , Qin , S -L , Zhang , Q , Goldsmith , P F , N. , J E II , Yuan , J , Zhang , C -P , White , G J , Choi , M , Lee , C W , Toth , L V , Mairs , S , Yi , H -W , Tang , M , Soam , A , Peretto , N , Samal , M R , Fich , M , Parsons , H , Malinen , J , Bendo , G J , Rivera-Ingraham , A , Liu , H -L , Wouterloot , J , Li , P S , Qian , L , Rawlings , J , Rawlings , M G , Feng , S , Wang , B , Li , D , Liu , M & Chrysostomou , A 2019 , ' SCOPE : SCUBA-2 Continuum Observations of Pre-protostellar Evolution - Survey Description and Compact Source Catalogue ' , Monthly Notices of the Royal Astronomical Society , vol. 485 , no. 2 , pp. 2895–2908 . https://doi.org/10.1093/mnras/stz574
dc.identifier.issn0035-8711
dc.identifier.otherArXiv: http://arxiv.org/abs/1902.10180v1
dc.identifier.otherORCID: /0000-0001-5392-909X/work/62748202
dc.identifier.urihttp://hdl.handle.net/2299/21358
dc.description© 2019 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society.
dc.description.abstractWe present the first release of the data and compact-source catalogue for the JCMT Large Program SCUBA-2 Continuum Observations of Pre-protostellar Evolution (SCOPE). SCOPE consists of 850 μm continuum observations of 1235 Planck Galactic Cold Clumps (PGCCs) made with the Submillimetre Common-User Bolometer Array 2 on the James Clerk Maxwell Telescope. These data are at an angular resolution of 14.4 arcsec, significantly improving upon the 353 GHz resolution of Planck at 5 arcmin, and allowing for a catalogue of 3528 compact sources in 558 PGCCs. We find that the detected PGCCs have significant sub-structure, with 61 per cent of detected PGCCs having three or more compact sources, with filamentary structure also prevalent within the sample. A detection rate of 45 per cent is found across the survey, which is 95 per cent complete to Planck column densities of N H2 > 5 × 10 21 cm −2. By positionally associating the SCOPE compact sources with young stellar objects, the star formation efficiency, as measured by the ratio of luminosity to mass, in nearby clouds is found to be similar to that in the more distant Galactic Plane, with the column density distributions also indistinguishable from each other.en
dc.format.extent14
dc.format.extent3544138
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.subjectISM: Clouds
dc.subjectStars: Formation
dc.subjectSubmillimetre: ISM
dc.subjectSurveys
dc.subjectAstronomy and Astrophysics
dc.subjectSpace and Planetary Science
dc.titleSCOPE : SCUBA-2 Continuum Observations of Pre-protostellar Evolution - Survey Description and Compact Source Catalogueen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=85067119048&partnerID=8YFLogxK
dc.identifier.urlhttps://arxiv.org/abs/1902.10180
rioxxterms.versionofrecord10.1093/mnras/stz574
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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