Cryogenic high-resolution echelle spectrometer for the European Southern Observatory VLT

Details Cryogenic high-resolution echelle spectrometer for the European Southern Observatory VLT Cryogenic high-resolution echelle spectrometer for the European Southern Observatory VLT

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995spie.2475..279w&link_type=abstract

Proc. SPIE Vol. 2475, p. 279-285, Infrared Detectors and Instrumentation for Astronomy, Albert M. Fowler; Ed.

Astronomy and Astrophysics

Astronomy

1

Scientific paper

A cryogenic echelle spectrometer is planned for the ESO Very Large Telescope to perform high-resolution (R >= 100,000) observations in the 1 - 5 micrometers range. Primary design goals are optical quality to exploit the 8 m telescope advantage and large spectral field to exploit the sensitivity advantage of a dispersive instrument with a large detector array. The basic instrument uses established technology; some components potentially leading to enhanced performance or additional capabilities are under development.

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