Near Infrared Camera Comissioning for ARC 3.5M Telescope

Details Near Infrared Camera Comissioning for ARC 3.5M Telescope Near Infrared Camera Comissioning for ARC 3.5M Telescope

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...205.4911h&link_type=abstract

American Astronomical Society Meeting 205, #49.11; Bulletin of the American Astronomical Society, Vol. 36, p.1420

Astronomy and Astrophysics

Astronomy

Scientific paper

A near-infrared camera is being commissioned for the ARC 3.5 meter telescope that will operate in both an imaging and a narrow band, full field spectroscopic mode. The 4.5' x 4.5' field-of-view is imaged onto a new-generation, low-noise Rockwell Hawaii-1RG 1024x1024 HgCdTe detector. High resolution (R 10,000) spectroscopy is accomplished by employing a Queensgate (now IC Optical) cryogenic Fabry-Perot etalon. The instrument is housed in a large Dewar of innovative, light-weight design. This presentation describes the as-built opto-mechanical system for the instrument and the initial commissioning results at Apache Point Observatory in New Mexico.

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