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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/5270
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dc.contributor.authorHancock, Paul J.-
dc.contributor.authorRoberts, Paul-
dc.contributor.authorKesteven, Michael J.-
dc.contributor.authorSubrahmanyan, Ravi-
dc.contributor.author+16 Co-authors-
dc.date.accessioned2012-08-29T06:42:13Z-
dc.date.available2012-08-29T06:42:13Z-
dc.date.issued2011-11-
dc.identifier.citationExperimental Astronomy, 2011, Vol.32, 147en
dc.identifier.issn0922-6435-
dc.identifier.issn1572-9508 (Online)-
dc.identifier.urihttp://hdl.handle.net/2289/5270-
dc.descriptionRestricted Accessen
dc.description.abstractThe Australia Telescope 20 GHz (AT20G) survey is a large area (2 π sr), sensitive (40 mJy), high frequency (20 GHz) survey of the southern sky. The survey was conducted in two parts: an initial fast scanning survey, and a series of more accurate follow-up observations. The follow-up survey catalog has been presented by Murphy et al. (MNRAS 402:2403, 2010). In this paper we discuss the hardware setup and scanning survey strategy as well as the production of the scanning survey catalog.en
dc.language.isoenen
dc.publisherSpringer Verlagen
dc.relation.urihttp://adsabs.harvard.edu/abs/2011ExA....32..147Hen
dc.relation.urihttp://arxiv.org/abs/1109.1886en
dc.relation.urihttp://dx.doi.org/10.1007/s10686-011-9257-yen
dc.rights2011 Springer Verlagen
dc.subjectInterferometryen
dc.subjectSurveysen
dc.subjectCatalogsen
dc.titleThe Australia telescope 20 GHz survey: hardware, observing strategy, and scanning survey catalogen
dc.typeArticleen
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