LIRIS: A Long-Slit Intermediate Resolution Infrared Sectrograph for the WHT

Acosta-Pulido, J.; Ballesteros, E.; Barreto, M.; Correa, S.; Delgado, J. M.; Dominguez-Tagle, C.; Hernandez, E.; Lopez, R.; Manchado, A.; Manescau, A.; Moreno, H.; Prada, F.; Redondo, P.; Sanchez, V.; Tenegi, F.
Bibliographical reference

The Newsletter of the Isaac Newton Group of Telescopes (ING Newsl.), issue no. 6, p. 22-24.

Advertised on:
10
2002
Number of authors
15
IAC number of authors
14
Citations
8
Refereed citations
8
Description
LIRIS is an Instituto de Astrofísica de Canarias (IAC) project that consists in a near-infrared (0.9-2.4microns) intermediate resolution spectrograph, conceived as a common user instrument for the WHT. LIRIS will have imaging, long-slit and multi-object spectroscopy observing modes (~1000-3000 Å). Coronography, and polarimetry capabilities will eventually be added. Image capability will allow easy target acquisition for spectroscopy.