Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/3724
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dc.contributor.authorSubrahmanyan, Ravi-
dc.contributor.authorEkers, R.D.-
dc.contributor.authorSaripalli, Lakshmi-
dc.contributor.authorSadler, E.M.-
dc.date.accessioned2009-02-04T10:54:28Z-
dc.date.available2009-02-04T10:54:28Z-
dc.date.issued2007-
dc.identifier.citationProceedings of a conference: From planets to dark energy: the modern radio universe held in Manchester, UK. Proceedings of Science, MRU-055, SISSAen
dc.identifier.issn1824-8039-
dc.identifier.urihttp://hdl.handle.net/2289/3724-
dc.descriptionOpen Accessen
dc.description.abstractWe have made a radio survey—the Australia Telescope Low Brightness Survey (ATLBS)—of 8.4 square degrees sky area, using the Australia Telescope Compact Array in the 20-cm band, in an observing mode designed to provide wide-field images with exceptional sensitivity in surface brightness, and thereby explore a new parameter space in radio source populations. The goals of this survey are to quantify the distribution in angular sizes, particularly at weak surface brightness levels: this has implications for the confusion in deep surveys with the SKA. The survey is expected to lead to a census of the radio emission associated with low-power radio galaxies at redshifts 1–3, without any missing extended emission, and hence a study of the cosmic evolution of low-power radio galaxies to higher redshift and a comprehensive study of the AGN feedback during the intense black hole growth phase during this redshift range.en
dc.language.isoenen
dc.publisherSISSAen
dc.relation.urihttp://adsabs.harvard.edu/abs/2007mru..confE..55Sen
dc.relation.urihttp://pos.sissa.it/cgi-bin/reader/conf.cgi?confid=52en
dc.rights2007 The authorsen
dc.titleA deep survey of the low-surface-brightness radio skyen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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