Abstract
LIRIS is a near-infrared (0.9–2.4 microns) intermediate resolution spectrograph (R = 1000 – 8000) 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 4.2 m William Herschel Telescope (WHT) at the Observatorio del Roque de Los Muchachos (ORM, La Palma).
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Manchado A., Fuentes F.J., Prada F. et al., 1998, SPIE, 3354, 448
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© 2001 Springer Science+Business Media Dordrecht
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Manchado, A. et al. (2001). LIRIS (Long-Slit Intermediate Resolution Infrared Spectrograph). In: Zamorano, J., Gorgas, J., Gallego, J. (eds) Highlights of Spanish Astrophysics II. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-1776-2_78
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DOI: https://doi.org/10.1007/978-94-017-1776-2_78
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