Paper
16 August 2000 Phoenix: operation and performance of a cryogenic high-resolution 1- to 5-μm infrared spectrograph
Author Affiliations +
Abstract
At the 1998 SPIE meeting we described a cryogenic, high- resolution spectrograph for use in the 1-5 micrometers region. At that time Phoenix had been used at Kitt Peak for about a year. In the intervening two years we have worked extensively with the instrument and have modified a few aspects of the design to bring the operational characteristics more closely into agreement with the original specifications. Changes to the instrument since 1998 that resulted in significant improvements in performance will be discussed. We will review the current operational characteristics of the spectrograph. Phoenix is a facility instrument of the National Optical Astronomy Observatory with use planned at Gemini South and CTIO.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Kenneth Harry Hinkle, Richard R. Joyce, Nigel Sharp, and Jeff A. Valenti "Phoenix: operation and performance of a cryogenic high-resolution 1- to 5-μm infrared spectrograph", Proc. SPIE 4008, Optical and IR Telescope Instrumentation and Detectors, (16 August 2000); https://doi.org/10.1117/12.395529
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KEYWORDS
Head

Cryogenics

Spectrographs

Collimators

Silicon

Sensors

Telescopes

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