High-resolution infrared echelle spectrograph (CRIRES) for the VLT

Details High-resolution infrared echelle spectrograph (CRIRES) for the VLT High-resolution infrared echelle spectrograph (CRIRES) for the VLT

Aug 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000spie.4008.1076w&link_type=abstract

Proc. SPIE Vol. 4008, p. 1076-1083, Optical and IR Telescope Instrumentation and Detectors, Masanori Iye; Alan F. Moorwood; Eds.

Physics

Instrumentation and Detectors

1

Scientific paper

The 105 resolution spectrograph 'CRIRES' for the 1-5 micrometers wavelength range is under construction for ESO's Very Large Telescope. The Nasmyth-mounted instrument sues an adaptive optics front-end for light concentration and 0.2 arcsec spatial resolution in the main long-slit spectroscopy mode. Three detector arrays will be used for large single- order wavelength coverage. Many components for this large cryogenic spectrograph are based on developments for earlier ESO IR instruments.

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