The last 20-GHz follow-up of the AT20G survey

Details The last 20-GHz follow-up of the AT20G survey The last 20-GHz follow-up of the AT20G survey

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atnf.prop.1168e&link_type=abstract

ATNF proposal C1049, Semester: October, 2007

Computer Science

Extragalactic, Atca

Scientific paper

We propose a follow-up of the Australia Telescope 20 GHz (AT20G) survey candidates in the declination range -15 < Dec < 0 in order to characterise (a) the high-frequency source population; improve radio source spectral evolution models; (c) quantify the discrete source contribution to the CMB anisotropies; (d) provide a network of high-frequency calibrators. In the coming term we ask for time to confirm a list of 2000 candidates from the upcoming Aug/Sep 2007 survey campaign. We also ask for time to clean up bad flux densities and positions for 600 confirmed sources from previous runs. This observation will complete the AT20G survey. 5 and 8GHz observations of this sample will be done with the VLA.

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