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18 April 2024
 
  » arxiv » 0911.0002

 Article overview


The Australia Telescope 20 GHz Survey: The Source Catalogue
Tara Murphy ; Elaine M. Sadler ; Ronald D. Ekers ; Marcella Massardi ; Paul J. Hancock ; Elizabeth Mahony ; Roberto Ricci ; Sarah Burke-Spolaor ; Mark Calabretta ; Rajan Chhetri ; Gianfranco De Zotti ; Philip G. Edwards ; Jennifer A. Ekers ; Carole A. Jackson ; Michael J. Kesteven ; Emma Lindley ; Katherine Newton-McGee ; Chris Phillips ; Paul Roberts ; Robert J. Sault ; Lister Staveley-Smith ; Ravi Subrahmanyan ; Mark A. Walker ; Warwick E. Wilson ;
Date 30 Oct 2009
AbstractWe present the full source catalogue from the Australia Telescope 20 GHz (AT20G) Survey. The AT20G is a blind radio survey carried out at 20 GHz with the Australia Telescope Compact Array (ATCA) from 2004 to 2008, and covers the whole sky south of declination 0 deg. The AT20G source catalogue presented here is an order of magnitude larger than any previous catalogue of high-frequency radio sources, and includes 5890 sources above a 20 GHz flux-density limit of 40 mJy. All AT20G sources have total intensity and polarisation measured at 20 GHz, and most sources south of declination -15 deg also have near-simultaneous flux-density measurements at 5 and 8 GHz. A total of 1559 sources were detected in polarised total intensity at one or more of the three frequencies. We detect a small but significant population of non-thermal sources that are either undetected or have only weak detections in low-frequency catalogues. We introduce the term Ultra-Inverted Spectrum (UIS) to describe these radio sources, which have a spectral index alpha(5, 20) > +0.7 and which constitute roughly 1.2 per cent of the AT20G sample. The 20 GHz flux densities measured for the strongest AT20G sources are in excellent agreement with the WMAP 5-year source catalogue of Wright et al. (2009), and we find that the WMAP source catalogue is close to complete for sources stronger than 1.5 Jy at 23 GHz.
Source arXiv, 0911.0002
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