High resolution spectroscopy with CSHELL |
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| Authors: | T. P. Greene A. T. Tokunaga J. S. Carr |
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| Affiliation: | (1) Institute for Astronomy, University of Hawai'i, Hilo, USA;(2) Department of Astronomy, Ohio State University, Columbus, USA |
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| Abstract: | CSHELL, the NASA Infrared Telescope Facility Cryogenic Echelle Spectrograph was designed to fill a need for high sensitivity, high resolution, long slit near-infrared spectroscopy. Scientific programs in the areas of comets, planetary atmospheres, young stellar objects, the interstellar medium, and galactic dynamics have been pursued with CSHELL and are described herein. The future of the instrument is also discussed. |
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| Keywords: | Infrared Spectroscopy CSHELL NASA IRTF |
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