AT 20 GHz (AT20G) follow-up

Details AT 20 GHz (AT20G) follow-up AT 20 GHz (AT20G) follow-up

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atnf.prop..528e&link_type=abstract

ATNF proposal C1049, Semester: October, 2006

Computer Science

Extragalactic, Atca

Scientific paper

We propose a follow-up of the Australia Telescope 20 GHz (AT20G) survey candidates in the declination range -30 < Dec < -15 in order to characterise (a) the high-frequency source population; (b) improve radio source spectral evolution models; (c) quantify the discrete source contribution to the CMB anisotropies; (d) provide a complete list of high-frequency calibrators. In the coming term we ask for time to confirm a list of 2000 candidates from the upcoming 2006 Aug/Sept survey campaign. This will complete follow-up observations for 75% of the southern sky. The final survey is expected to cover all the southern sky and detect about 10000 sources, being 100% complete down to S(20GHz) = 60 mJy.

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