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dc.contributor.authorMackenzie, Todd
dc.contributor.authorBraglia, Filiberto G.
dc.contributor.authorGibb, Andy G.
dc.contributor.authorScott, Douglas
dc.contributor.authorJenness, Tim
dc.contributor.authorSerjeant, Stephen
dc.contributor.authorThompson, Mark
dc.contributor.authorBerry, David
dc.contributor.authorBrunt, Christopher M.
dc.contributor.authorChapin, Edward
dc.contributor.authorChrysostomou, A.
dc.contributor.authorClements, Dave
dc.contributor.authorCoppin, Kristen
dc.contributor.authorEconomou, Frossie
dc.contributor.authorEvans, A.
dc.contributor.authorFriberg, Per
dc.contributor.authorGreaves, Jane
dc.contributor.authorHill, T.
dc.contributor.authorHolland, Wayne
dc.contributor.authorIvison, R. J.
dc.contributor.authorKnapen, Johan H.
dc.contributor.authorJackson, Neal
dc.contributor.authorJoncas, Gilles
dc.contributor.authorMorgan, Larry
dc.contributor.authorMortier, Angela
dc.contributor.authorPearson, Chris
dc.contributor.authorPestalozzi, Michele
dc.contributor.authorPope, Alexandra
dc.contributor.authorRicher, John
dc.contributor.authorUrquhart, J. S.
dc.contributor.authorVaccari, Mattia
dc.contributor.authorWeferling, Bernd
dc.contributor.authorWhite, Glenn
dc.contributor.authorZhu, Ming
dc.date.accessioned2011-09-20T15:01:05Z
dc.date.available2011-09-20T15:01:05Z
dc.date.issued2011-08
dc.identifier.citationMackenzie , T , Braglia , F G , Gibb , A G , Scott , D , Jenness , T , Serjeant , S , Thompson , M , Berry , D , Brunt , C M , Chapin , E , Chrysostomou , A , Clements , D , Coppin , K , Economou , F , Evans , A , Friberg , P , Greaves , J , Hill , T , Holland , W , Ivison , R J , Knapen , J H , Jackson , N , Joncas , G , Morgan , L , Mortier , A , Pearson , C , Pestalozzi , M , Pope , A , Richer , J , Urquhart , J S , Vaccari , M , Weferling , B , White , G & Zhu , M 2011 , ' A pilot study for the SCUBA-2 'All-Sky' Survey ' , Monthly Notices of the Royal Astronomical Society , vol. 415 , no. 2 , pp. 1950-1960 . https://doi.org/10.1111/j.1365-2966.2011.18840.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 366898
dc.identifier.otherPURE UUID: 4b4b4459-84ed-4de6-9377-f0b8b623fd96
dc.identifier.otherWOS: 000293756300077
dc.identifier.otherScopus: 79960576992
dc.identifier.otherORCID: /0000-0002-0729-2988/work/30423079
dc.identifier.otherORCID: /0000-0001-5392-909X/work/30970821
dc.identifier.urihttp://hdl.handle.net/2299/6458
dc.descriptionThe definitive version can be found at : http://onlinelibrary.wiley.com/ Copyright Royal Astronomical Society
dc.description.abstractWe have carried out a pilot study for the Submillimetre Common-User Bolometer Array 2 (SCUBA-2) 'All-Sky' Survey (SASSy), a wide and shallow mapping project at 850 mu m, designed to find rare objects, both Galactic and extragalactic. Two distinct sets of exploratory observations were undertaken and used to test the SASSy approach and data-reduction pipeline. The first was a 0 degrees.5 x 0 degrees.5 map around the nearby galaxy NGC 2559. The galaxy was easily detected at 156 mJy, but no other convincing sources are present in the map. Comparison with other galaxies with similar wavelength coverage indicates that NGC 2559 has relatively warm dust. The second observations cover 1 deg(2) around the W5-E H II region. As well as diffuse structure in the map, a filtering approach was able to extract 27 compact sources with signal-to-noise ratio greater than 6. By matching with data at other wavelengths we can see that the SCUBA-2 data can be used to discriminate the colder cores. Together these observations show that the SASSy project will be able to meet its original goals of detecting new bright sources which will be ideal for follow-up observations with other facilities.en
dc.format.extent11
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.subjectsurveys
dc.subjectsubmillimetre: galaxies
dc.subjectsubmillimetre: stars
dc.titleA pilot study for the SCUBA-2 'All-Sky' Surveyen
dc.contributor.institutionScience Learning Centre
dc.contributor.institutionSocial Sciences, Arts & Humanities Research Institute
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.date.embargoedUntil2011-12-01
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1111/j.1365-2966.2011.18840.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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