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LIRIS: Long Slit Intermediate-Resolution InfraRed Spectrograph
— Near-infrared imager and spectrograph —
First light (at ING): 15 February 2003.
Designed and built by: Instituto de Astrofísica de Canarias is the main builder and designer. Other collaborating institutions are the UK Astronomy Technology Centre and the Isaac Newton Group of Telescopes.
Description: LIRIS is a long-slit intermediate-resolution infrared spectrograph to be mounted on the Cassegrain focus of the 4.2 m William Herschel Telescope (WHT).