An advanced cooled grating spectrometer for UKIRT-CGS4

Details An advanced cooled grating spectrometer for UKIRT-CGS4 An advanced cooled grating spectrometer for UKIRT-CGS4

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989irsa.rept..563m&link_type=abstract

In ESA, Infrared Spectroscopy in Astronomy p 563-566 (SEE N90-19084 11-89)

Astronomy and Astrophysics

Astronomy

Cooling Systems, Design Analysis, Gratings (Spectra), Infrared Radiation, Infrared Spectrometers, Infrared Telescopes, Infrared Imagery, Spectral Resolution, United Kingdom

Scientific paper

The main features of the Cooled Grating Spectrometer (CGS4), for the United Kingdom Infrared Telescope (UKIRT), are described. The CGS4 for use at 1 to 5 microns is designed to fully utilize foreseeable arrays and to take maximum advantage of the solid imaging detectors. The spectrometer can use low dispersion first order grating in a back-to-back configuration with a high dispersion echelle, giving wavelength resolutions from approximately 1,000 to 24,000.

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