LIRIS (Long-slit Intermediate Resolution Infrared Spectrograph): Assembly Integration and verification

Bibcode
2003SPIE.4841..160M
DOI
10.1117/12.458920
Manchado, A.; Barreto, Mary; Acosta-Pulido, Jose; Ballesteros Ramirez, Ezequiel; Correa, Santiago; Delgado, Jose M.; Dominguez-Tagle, Carlos; Hernández, Elvio; Lopez, Roberto L.; Manescau, Antonio; Moreno, Heidi; Prada, Francisco; Redondo, Pablo; Sanchez de la Rosa, Vicente; Sosa, Nicolas A.; Tenegi, Fabio
Bibliographical reference

Instrument Design and Performance for Optical/Infrared Ground-based Telescopes. Edited by Iye, Masanori; Moorwood, Alan F. M. Proceedings of the SPIE, Volume 4841, pp. 160-168 (2003).

Advertised on:
3
2003
Number of authors
16
IAC number of authors
16
Citations
2
Refereed citations
1
Description
LIRIS is a near-infrared (0.9 - 2.4 microns) intermediate resolution spectrograph (R = 1000-3000) conceived as a common user instrument for the (WHT) at the Observatorio del Roque de los Muchachos (ORM) La Palma. LIRIS is now being assembled, integrated and virified at the Instituto Astrofisico de Canarias (IAC). LIRIS will have imaging, long-slit and multi-object spectroscopy working modes. Coronography and polarimetry capabilities will eventually be added. Image capability will allow easy target acquisition.
Type
Non-refereed

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