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Proceedings Paper

Data reduction pipeline for OSIRIS, the new NIR diffraction-limited imaging field spectrograph for the Keck adaptive optics system
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Paper Abstract

OSIRIS is a near infrared diffraction limited imaging field spectrograph under development for the Keck observatory adaptive optics system and scheduled for commissioning in fall 2004. Based upon lenslet pupil imaging, diffraction grating, and a 2Kx2K Hawaii2 HgCdTe array, OSIRIS is a highly efficient instrument at the forefront of today's technology. OSIRIS will deliver per readout up to 4096 diffraction limited spectra in a complex interleaved format, requiring new challenges to be met regarding user interaction and data reduction. A data reduction software package is under development, aiming to provide the observer with a facility instrument allowing him to concentrate on science rather than dealing with instrumental as well as telescope and atmosphere related effects. Together with OSIRIS, a pipeline for basic data reduction will be provided for a new Keck instrument for the first time. A status report is presented here together with some aspects of the data reduction pipeline.

Paper Details

Date Published: 30 September 2004
PDF: 8 pages
Proc. SPIE 5492, Ground-based Instrumentation for Astronomy, (30 September 2004); doi: 10.1117/12.552592
Show Author Affiliations
Alfred Krabbe, Univ. zu Koln (Germany)
Tom Gasaway, Univ. of California/San Diego (United States)
Inseok Song, Univ. of California/Los Angeles (United States)
Christof Iserlohe, Univ. zu Koln (Germany)
Jason Weiss, Univ. of California/Los Angeles (United States)
James E. Larkin, Univ. of California/Los Angeles (United States)
Matthew Barczys, Univ. of California/Los Angeles (United States)
David Lafreniere, Univ. of California/Los Angeles (United States)

Published in SPIE Proceedings Vol. 5492:
Ground-based Instrumentation for Astronomy
Alan F. M. Moorwood; Masanori Iye, Editor(s)

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