The ATLAS 1.4 GHz survey

Details The ATLAS 1.4 GHz survey The ATLAS 1.4 GHz survey

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atnf.prop.3171h&link_type=abstract

ATNF proposal C1967, Semester: April, 2010

Computer Science

Star Formation, Active Galactic Nuclei / Quasars, Surveys And Studies Of Distant Galaxies, Atca

Scientific paper

Following the very successful observations during 2009OCTS for this large project, we request 500 h to complete the observations over both ATLAS survey areas at 1.4 GHz using CABB. The sensitivity limitations previously imposed by the bright confusing source have now been resolved, and we aim to (1) use CABB to achieve the originally proposed sensitivity over the full ATLAS survey regions (CDFS and ELAIS-S1) at 1.4 GHz; (2) measure the evolution in both active nucleus and star formation dominated systems over significant fractions of cosmic time (up to 80% the age of the universe for star formers, and the whole of cosmic history for active nuclei); and (3) test new analysis techniques and confusion mitigation strategies for ASKAP continuum surveys, such as EMU.

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