Show simple item record

dc.contributor.authorWard-Thompson, D.
dc.contributor.authorDi Francesco, J.
dc.contributor.authorHatchell, J.
dc.contributor.authorHogerheijde, M.R.
dc.contributor.authorNutter, D.
dc.contributor.authorBastien, P.
dc.contributor.authorBasu, S.
dc.contributor.authorBonnell, I.
dc.contributor.authorBowey, J.
dc.contributor.authorBrunt, C.
dc.contributor.authorBuckle, J.
dc.contributor.authorButner, H.
dc.contributor.authorCavanagh, B.
dc.contributor.authorChrysostomou, A.
dc.date.accessioned2010-06-30T10:20:31Z
dc.date.available2010-06-30T10:20:31Z
dc.date.issued2007
dc.identifier.citationWard-Thompson , D , Di Francesco , J , Hatchell , J , Hogerheijde , M R , Nutter , D , Bastien , P , Basu , S , Bonnell , I , Bowey , J , Brunt , C , Buckle , J , Butner , H , Cavanagh , B & Chrysostomou , A 2007 , ' The James Clerk Maxwell Telescope Legacy Survey of Nearby Star-forming Regions in the Gould Belt ' , Publications of the Astronomical Society of the Pacific , vol. 119 , no. 858 , pp. 855-870 . https://doi.org/10.1086/521277
dc.identifier.issn0004-6280
dc.identifier.otherPURE: 178516
dc.identifier.otherPURE UUID: dff8c785-2e55-4b44-a873-dd97684589a9
dc.identifier.otherdspace: 2299/4609
dc.identifier.otherScopus: 35348843912
dc.identifier.urihttp://hdl.handle.net/2299/4609
dc.descriptionOriginal article can be found at: http://www.journals.uchicago.edu/toc/pasp/current Copyright ASP/ University of Chicago Press. DOI: 10.1086/521277
dc.description.abstractThis paper describes a James Clerk Maxwell Telescope (JCMT) legacy survey that has been awarded roughly 500 hr of observing time to be carried out from 2007 to 2009. In this survey, we will map with SCUBA-2 (Submillimetre Common-User Bolometer Array 2) almost all of the well-known low-mass and intermediate-mass star-forming regions within 0.5 kpc that are accessible from the JCMT. Most of these locations are associated with the Gould Belt. From these observations, we will produce a flux-limited snapshot of star formation near the Sun, providing a legacy of images, as well as point-source and extended-source catalogs, over almost 700 deg2 of sky. The resulting images will yield the first catalog of prestellar and protostellar sources selected by submillimeter continuum emission, and should increase the number of known sources by more than an order of magnitude. We will also obtain with the array receiver HARP (Heterodyne Array Receiver Program) CO maps, in three CO isotopologues, of a large typical sample of prestellar and protostellar sources.We will then map the brightest hundred sources with the SCUBA-2 polarimeter (POL-2), producing the first statistically significant set of polarization maps in the submillimeter. The images and source catalogs will be a powerful reference set for astronomers, providing a detailed legacy archive for future telescopes, including ALMA, Herschel, and JWST.en
dc.language.isoeng
dc.relation.ispartofPublications of the Astronomical Society of the Pacific
dc.rightsOpen
dc.titleThe James Clerk Maxwell Telescope Legacy Survey of Nearby Star-forming Regions in the Gould Belten
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted2007
rioxxterms.versionofrecordhttps://doi.org/10.1086/521277
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record