SIRTF Infrared Spectrometer Data Processing at the SIRTF Science Center

Details SIRTF Infrared Spectrometer Data Processing at the SIRTF Science Center SIRTF Infrared Spectrometer Data Processing at the SIRTF Science Center

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...203.4608m&link_type=abstract

American Astronomical Society Meeting 203, #46.08; Bulletin of the American Astronomical Society, Vol. 35, p.1281

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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.

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