High resolution spectroscopy with CSHELL

Details High resolution spectroscopy with CSHELL High resolution spectroscopy with CSHELL

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994exa.....3..309g&link_type=abstract

Experimental Astronomy, vol. 3, no. 1-4, p. 309-312

Astronomy and Astrophysics

Astronomy

1

Astronomical Spectroscopy, Infrared Astronomy, Infrared Spectrometers, Infrared Spectroscopy, Near Infrared Radiation, Space Infrared Telescope Facility, Comets, Galactic Evolution, Interstellar Matter, Planetary Atmospheres, Star Formation

Scientific paper

The NASA Infrared Telescope Facility Cryogenic Echelle Spectrograph (CSHELL) 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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