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21 August 1998 Phoenix: a cryogenic high-resolution 1- to 5-μm infrared spectrograph
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We describe a cryogenic, high-resolution spectrograph (Phoenix) for the 1-5 micrometers region. Phoenix is an echelle spectrograph of the near-Littrow over-under configuration without cross dispersion. The foreoptics include Lyot re- imaging, discrete and circular variable order sorting filters, a selection of slits, and optics for post-slit and Lyot imaging. The entire instrument is cooled to 50 K using two closed cycle coolers. The detector is a Hughes-Santa Barbara 512 X 1024 InSb array. Resolution of 65,000 has been obtained. Throughput without slit losses is 13 percent at 2.3 micrometers . Recent results are discussed. Phoenix is a facility instrument of the National Optical Astronomy Observatories and will be available at CTIO, KPNO, and Gemini.
© (1998) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Kenneth Harry Hinkle, Randy W. Cuberly, Neil A. Gaughan, Julie B. Heynssens, Richard R. Joyce, Stephen T. Ridgway, Paul Schmitt, and Jorge E. Simmons "Phoenix: a cryogenic high-resolution 1- to 5-μm infrared spectrograph", Proc. SPIE 3354, Infrared Astronomical Instrumentation, (21 August 1998);


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