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Proceedings Paper

Near-infrared camera and Fabry-Perot spectrometer (NIC-FPS)
Author(s): Fred R. Hearty; Jon Morse; Stephane Beland; James Green; Nathaniel J. Cunningham; Robert Valentine; Meredith Drosback; Cynthia S. Froning; Patrick Hartigan; J. C. Barentine
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Paper Abstract

A near-infrared instrument is being built 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' fild-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 report describes the as-built opto-mechanical system for the instrument and the work remaining before deployment at Apache Point Observatory in New Mexico.

Paper Details

Date Published: 30 September 2004
PDF: 10 pages
Proc. SPIE 5492, Ground-based Instrumentation for Astronomy, (30 September 2004); doi: 10.1117/12.551703
Show Author Affiliations
Fred R. Hearty, Univ. of Colorado/Boulder (United States)
Jon Morse, Arizona State Univ. (United States)
Stephane Beland, Univ. of Colorado/Boulder (United States)
James Green, Univ. of Colorado/Boulder (United States)
Nathaniel J. Cunningham, Univ. of Colorado/Boulder (United States)
Robert Valentine, Univ. of Colorado/Boulder (United States)
Meredith Drosback, Univ. of Colorado/Boulder (United States)
Cynthia S. Froning, Univ. of Colorado/Boulder (United States)
Patrick Hartigan, Rice Univ. (United States)
J. C. Barentine, New Mexico State Univ. (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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