LIRIS (long-slit intermediate-resolution infrared spectrograph): project status

Details LIRIS (long-slit intermediate-resolution infrared spectrograph): project status LIRIS (long-slit intermediate-resolution infrared spectrograph): project status

Aug 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000spie.4008.1162m&link_type=abstract

Proc. SPIE Vol. 4008, p. 1162-1171, Optical and IR Telescope Instrumentation and Detectors, Masanori Iye; Alan F. Moorwood; Eds.

Physics

Instrumentation and Detectors

5

Scientific paper

LIRIS is a near-IR intermediate resolution spectrograph with added capabilities for multi-object, imaging, coronography, and polarimetry. This instrument is now being constructed at the IAC, and upon complexion will be installed on the 4.2m William Herschel Telescope at the Observatorio del Roque de Los Muchachos. The optical system uses lenses and is based on a classical collimator/camera design. Grisms are used as the dispersion elements. The plate scale matches the median seeing at the ORM. The detector is a Hawaii 1024 X 1024 HgCdTe array operating at 60K.

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