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dc.contributor.authorParker, Q.A.
dc.contributor.authorPhillipps, S.
dc.contributor.authorPierce, M.J.
dc.contributor.authorHartley, M.
dc.contributor.authorRead, M.
dc.contributor.authorMacGillivray, H.T.
dc.contributor.authorTritton, S.B.
dc.contributor.authorCass, C.P.
dc.contributor.authorCannon, R.D.
dc.contributor.authorCohen, M.
dc.contributor.authorDrew, J.E.
dc.contributor.authorFrew, D.J.
dc.contributor.authorHopewell, E.C.
dc.contributor.authorMader, S.
dc.contributor.authorMalin, D.F.
dc.contributor.authorMasheder, M.R.W.
dc.contributor.authorMorgan, D.H.
dc.contributor.authorMorris, R.A.H.
dc.contributor.authorRusseil, D.
dc.contributor.authorRussell, K.S.
dc.contributor.authorWalker, R.N.F.
dc.contributor.authorHambly, N.C.
dc.date.accessioned2008-01-02T10:00:14Z
dc.date.available2008-01-02T10:00:14Z
dc.date.issued2005
dc.identifier.citationParker , Q A , Phillipps , S , Pierce , M J , Hartley , M , Read , M , MacGillivray , H T , Tritton , S B , Cass , C P , Cannon , R D , Cohen , M , Drew , J E , Frew , D J , Hopewell , E C , Mader , S , Malin , D F , Masheder , M R W , Morgan , D H , Morris , R A H , Russeil , D , Russell , K S , Walker , R N F & Hambly , N C 2005 , ' The AAO/UKST SuperCOSMOS Ha survey ' , Monthly Notices of the Royal Astronomical Society , vol. 362 , no. 2 , pp. 689-710 . https://doi.org/10.1111/j.1365-2966.2005.09350.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 144267
dc.identifier.otherPURE UUID: 3a75745c-d3ef-47c5-a747-57f17324b7ff
dc.identifier.otherdspace: 2299/1288
dc.identifier.otherScopus: 24944579866
dc.identifier.urihttp://hdl.handle.net/2299/1288
dc.descriptionThe definitive version is available at www.blackwell-synergy.com. Copyright Blackwell Publishing DOI : 10.1111/j.1365-2966.2005.09350.x
dc.description.abstractThe UK Schmidt Telescope (UKST) of the Anglo-Australian Observatory completed a narrow-band H plus [NII] 6548, 6584°A survey of the Southern Galactic Plane and Magellanic Clouds in late 2003. The survey, which was the last UKST wide-field pho- tographic survey, and the only one undertaken in a narrow band, is now an on-line digital data product of the Wide-Field Astronomy Unit of the Royal Observatory Ed- inburgh (ROE). The survey utilised a high specification, monolithic H interference band-pass filter of exceptional quality. In conjunction with the fine grained Tech-Pan film as a detector it has produced a survey with a powerful combination of area cover- age (4000 square degrees), resolution (∼1 arcsecond) and sensitivity (≤5 Rayleighs), reaching a depth for continuum point sources of R ≃ 20.5. The main survey consists of 233 individual fields on a grid of centres separated by 4◦ at declinations below +2◦ and covers a swathe approximately 20◦ wide about the Southern Galactic Plane. The original survey films were scanned by the SuperCOSMOS measuring machine at the Royal Observatory, Edinburgh to provide the on-line digital atlas called the SuperCOSMOS H Survey (SHS).en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.rightsOpen
dc.titleThe AAO/UKST SuperCOSMOS Ha surveyen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted2005
rioxxterms.versionofrecordhttps://doi.org/10.1111/j.1365-2966.2005.09350.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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