Deep Source Count Observations with SHARC II: Reduction Software and Latest Results

Details Deep Source Count Observations with SHARC II: Reduction Software and Latest Results Deep Source Count Observations with SHARC II: Reduction Software and Latest Results

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...20311906k&link_type=abstract

American Astronomical Society Meeting 203, #119.06; Bulletin of the American Astronomical Society, Vol. 35, p.1405

Astronomy and Astrophysics

Astronomy

Scientific paper

We present latest results from a year long campaign of deep observations at 350μ m of various pre-selected fields (CUDSS3hr, MIPS14hr, SSA17) to a target 3σ of 15mJy. These observations were taken with the SHARC II instrument at the Caltech Submillimeter Observatory and much effort has gone into characterizing the instrument, with different sets of reduction software being written. We detail our own IDL-based reduction software - CIRRUS - and the future work to be done on this front. The observation results will be used to place constraints on source count models.

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