Data Reduction Pipelines for MIPS

Details Data Reduction Pipelines for MIPS Data Reduction Pipelines for MIPS

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...203.2217w&link_type=abstract

American Astronomical Society Meeting 203, #22.17; Bulletin of the American Astronomical Society, Vol. 35, p.1245

Astronomy and Astrophysics

Astronomy

Scientific paper

The Multiband Imaging Photometer for SIRTF (MIPS) is the longest-wavelength instrument on SIRTF, providing broadband imaging at 24, 70 and 160 microns as well as low-resolution spectroscopy between 52 and 99 microns. We will present an overview of the MIPS data reduction pipelines for both the Si:As (24 micron) and the Ge:Ga (70 and 160 micron) arrays. We will outline the expected data products and post-processing tools available to the user.

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