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Session overview and AzTEC instrument performance

By Peter A. R. Ade, I. Aretxaga, J. Austerman, J. J. Bock, D. Hughes, Y. Kang, S. Kim, J. Lowenthal, Philip Daniel Mauskopf, K. Scott and M. Yun

Abstract

AzTEC is a new 144 element bolometer receiver destined as a first-generation instrument for the Large Millimeter Telescope. >From November 2005 and through January 2006, AzTEC made science observations at the 15m James Clerk Maxwell Telescope (JCMT). Approximately 1/2 of the available time was spent mapping the submillimeter galaxy population in blank and biased fields. Overall, over 1 square degree of sky was mapped with uniform coverage in each of five primary fields making this the largest set of surveys of the submillimeter galaxy population ever performed. Hundreds of new submillimeter galaxies have been detected. Here we discuss the instrument, our mapping technique, and a brief summary of the data reduction process. We conclude with a brief summary of the overall impact of these surveys on our understanding of the submillimeter galaxy population

Topics: QB
OAI identifier: oai:http://orca.cf.ac.uk:41381
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