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dc.contributor.authorNettke, W.
dc.contributor.authorScott, D.
dc.contributor.authorGibb, A. G.
dc.contributor.authorThompson, M.
dc.contributor.authorChrysostomou, A.
dc.contributor.authorEvans, A.
dc.contributor.authorHill, T.
dc.contributor.authorJenness, T.
dc.contributor.authorJoncas, G.
dc.contributor.authorMoore, T.
dc.contributor.authorSerjeant, S.
dc.contributor.authorUrquhart, J.S.
dc.contributor.authorVaccari, M.
dc.contributor.authorWeferling, B.
dc.contributor.authorWhite, G.
dc.contributor.authorZhu, M.
dc.date.accessioned2017-06-01T13:02:45Z
dc.date.available2017-06-01T13:02:45Z
dc.date.issued2017-06-01
dc.identifier.citationNettke , W , Scott , D , Gibb , A G , Thompson , M , Chrysostomou , A , Evans , A , Hill , T , Jenness , T , Joncas , G , Moore , T , Serjeant , S , Urquhart , J S , Vaccari , M , Weferling , B , White , G & Zhu , M 2017 , ' The SCUBA-2 Ambitious Sky Survey: a catalogue of beam-sized sources in the Galactic longitude range 120deg-140deg ' , Monthly Notices of the Royal Astronomical Society , vol. 468 , pp. 250-260 . https://doi.org/10.1093/mnras/stx339
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 11676894
dc.identifier.otherPURE UUID: fe8f44e0-8ace-4da6-8631-a038f9c2bf2f
dc.identifier.otherBibtex: urn:d9140e530a34a583a757e1f52aa722a9
dc.identifier.otherScopus: 85017220843
dc.identifier.otherORCID: /0000-0001-5392-909X/work/42466470
dc.identifier.urihttp://hdl.handle.net/2299/18261
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
dc.description.abstractThe SCUBA-2 Ambitious Sky Survey (SASSy) is composed of shallow 850-µm imaging using the Submillimetre Common-User Bolometer Array 2 (SCUBA-2) on the James Clerk Maxwell Telescope. Here we describe the extraction of a catalogue of beam-sized sources from a roughly 120 deg2 region of the Galactic plane mapped uniformly (to an rms level of about 40 mJy), covering longitude 120◦ < l < 140◦ and latitude |b| < 2. ◦9. We used a matched-filtering approach to increase the signal-to-noise ratio (S/N) in these noisy maps and tested the efficiency of our extraction procedure through estimates of the false discovery rate, as well as by adding artificial sources to the real images. The primary catalogue contains a total of 189 sources at 850 µm, down to an S/N threshold of approximately 4.6. Additionally, we list 136 sources detected down to S/N = 4.3, but recognize that as we go lower in S/N, the reliability of the catalogue rapidly diminishes. We perform follow-up observations of some of our lower significance sources through small targeted SCUBA-2 images and list 265 sources detected in these maps down to S/N = 5. This illustrates the real power of SASSy: inspecting the shallow maps for regions of 850-µm emission and then using deeper targeted images to efficiently find fainter sources. We also perform a comparison of the SASSy sources with the Planck Catalogue of Compact Sources and the IRAS Point Source Catalogue, to determine which sources discovered in this field might be new, and hence potentially cold regions at an early stage of star formation.en
dc.format.extent11
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.subjectsurveys: ISM
dc.subjectclouds: submillimetre
dc.subjectgalaxies: submillimetre
dc.subjectISM: submillimetre: stars
dc.titleThe SCUBA-2 Ambitious Sky Survey: a catalogue of beam-sized sources in the Galactic longitude range 120deg-140degen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.identifier.urlhttps://arxiv.org/abs/1703.01930
rioxxterms.versionVoR
rioxxterms.versionofrecordhttps://doi.org/10.1093/mnras/stx339
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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