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S. Wachter, D. Frayer, D. Padgett, F. Masci, D. Henderson, W. Latter (SIRTF Science Center), MIPS Team
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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Bulletin of the American Astronomical Society, 35#5
© 2003. The American Astronomical Soceity.