| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1780534 | New Astronomy Reviews | 2006 | 8 Pages |
Abstract
OSIRIS (OH-Suppressing Infra-Red Integral-field Spectrograph) is a new facility instrument for the Keck Observatory. After seeing first light in February 2005, OSIRIS is currently undergoing commissioning. OSIRIS provides the capability of performing three-dimensional spectroscopy in the near-infrared z, J, H, and K bands at the resolution limit of the Keck II telescope, which is equipped with adaptive optics and a laser guide star. The science case for OSIRIS is summarized, and the instrument and associated data reduction software are described.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
A. Quirrenbach, J. Larkin, M. Barczys, T. Gasaway, C. Iserlohe, A. Krabbe, M. McElwain, I. Song, J. Weiss, S. Wright,