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dc.contributor.authorJenness, T.
dc.contributor.authorStevens, J. A.
dc.contributor.authorArchibald, E.N.
dc.contributor.authorEconomou, F.
dc.contributor.authorJessop, N.
dc.contributor.authorRobson, E.I.
dc.date.accessioned2007-08-17T12:33:26Z
dc.date.available2007-08-17T12:33:26Z
dc.date.issued2002-10
dc.identifier.citationJenness , T , Stevens , J A , Archibald , E N , Economou , F , Jessop , N & Robson , E I 2002 , ' Towards the automated reduction and calibration of SCUBA data from the James Clerk Maxwell Telescope ' , Monthly Notices of the Royal Astronomical Society , vol. 336 , no. 1 , pp. 14-21 . https://doi.org/10.1046/j.1365-8711.2002.05604.x
dc.identifier.issn0035-8711
dc.identifier.otherdspace: 2299/475
dc.identifier.otherORCID: /0000-0002-4010-8310/work/62747610
dc.identifier.urihttp://hdl.handle.net/2299/475
dc.descriptionThe definitive version is available at www.blackwell-synergy.com '.--Copyright Blackwell Publishing. DOI : 10.1046/j.1365-8711.2002.05604.x
dc.description.abstractThe Submillimetre Common User Bolometer Array (SCUBA) instrument has been op- erating on the James Clerk Maxwell Telescope (JCMT) since 1997. The data archive is now sufficiently large that it can be used to investigate instrumental properties and the variability of astronomical sources. This paper describes the automated calibra- tion and reduction scheme used to process the archive data with particular emphasis on ‘jiggle-map’ observations of compact sources. We demonstrate the validity of our automated approach at both 850- and 450-μm and apply it to several of the JCMT sec- ondary flux calibrators.We determine light curves for the variable sources IRC+10216 and OH 231.8. This automation is made possible by using the ORAC-DR data reduc- tion pipeline, a flexible and extensible data reduction pipeline that is used on UKIRT and the JCMT.en
dc.format.extent548422
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleTowards the automated reduction and calibration of SCUBA data from the James Clerk Maxwell Telescopeen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1046/j.1365-8711.2002.05604.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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