CRIRES: cryogenic high-resolution infrared echelle spectrograph for the VLT

Details CRIRES: cryogenic high-resolution infrared echelle spectrograph for the VLT CRIRES: cryogenic high-resolution infrared echelle spectrograph for the VLT

Aug 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998spie.3354..599w&link_type=abstract

Proc. SPIE Vol. 3354, p. 599-605, Infrared Astronomical Instrumentation, Albert M. Fowler; Ed.

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The instrument ensemble at ESO's Very Large Telescope will be extended by a high-resolution echelle spectrograph for the 1-5 micrometers wavelength range. Primary design goals are high spectral resolution, wide coverage and high sensitivity. Several novel features are introduced with this instrument. At the same time, development time and risk will be minimized through the use of concepts available from earlier ESO VLT instruments.

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