AAS 203rd Meeting, January 2004
Session 46 Instrumentation for HST and Sirtf
Poster, Tuesday, January 6, 2004, 9:20am-6:30pm, Grand Hall

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[46.08] SIRTF Infrared Spectrometer Data Processing at the SIRTF Science Center

P.W. Morris (IRS Instrument Support Team, SSC), F. Fang, R. Narron (IRS Downlink Operations Group, SSC), IRS Instrument Support Team, SSC Downlink Opertations Team

The SIRTF Infrared Spectrometer (IRS) produces spectroscopy over the 5.3 - 40 micron range at low (~70) and moderate (~650) spectral resolutions, using four independent 128x128 format Si BiB arrays operated to provide unprecedented sensitivities for astronomical applications. We will present an overview of the IRS data reduction pipelines at the SIRTF Science Center, at the levels of basic detector calibrations, photometric and spectral calibrations, and spectral extraction, and outline the data products expected to be available to users.

The author(s) of this abstract have provided an email address for comments about the abstract: sirtf@sirtf.ipac.caltech.edu

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Bulletin of the American Astronomical Society, 35#5
© 2003. The American Astronomical Soceity.