OSIRIS: AO-assisted integral-field spectroscopy at the Keck Observatory

Details OSIRIS: AO-assisted integral-field spectroscopy at the Keck Observatory OSIRIS: AO-assisted integral-field spectroscopy at the Keck Observatory

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006newar..49..639q&link_type=abstract

New Astronomy Reviews, Volume 49, Issue 10-12, p. 639-646.

Astronomy and Astrophysics

Astronomy

1

95.55.Br, 95.55.Qf, 95.75.Fg, 95.75.Mn

Scientific paper

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.

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