LIRIS (Long-slit Intermediate Resolution Infrared Spectrograph): assembly integration and verification

Arturo Manchado-Torres; Mary Barreto; Jose Acosta-Pulido; Ezequiel Ballesteros Ramirez; Santiago Correa; Jose Miguel Delgado; Carlos Dominguez-Tagle; Elvio Hernandez; Roberto L. Lopez; Antonio Manescau; Heidi Moreno; Francisco Prada; Pablo Redondo; Vicente Sanchez de la Rosa; Nicolas A. Sosa; Fabio Tenegi

doi:10.1117/12.458920

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7 March 2003 LIRIS (Long-slit Intermediate Resolution Infrared Spectrograph): Assembly Integration and verification

Arturo Manchado-Torres, Mary Barreto, Jose Acosta-Pulido, Ezequiel Ballesteros Ramirez, Santiago Correa, Jose Miguel Delgado, Carlos Dominguez-Tagle, Elvio Hernandez, Roberto L. Lopez, Antonio Manescau, Heidi Moreno, Francisco Prada, Pablo Redondo, Vicente Sanchez de la Rosa, Nicolas A. Sosa, Fabio Tenegi

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Proceedings Volume 4841, Instrument Design and Performance for Optical/Infrared Ground-based Telescopes; (2003) https://doi.org/10.1117/12.458920
Event: Astronomical Telescopes and Instrumentation, 2002, Waikoloa, Hawai'i, United States

Abstract

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.

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Arturo Manchado-Torres, Mary Barreto, Jose Acosta-Pulido, Ezequiel Ballesteros Ramirez, Santiago Correa, Jose Miguel Delgado, Carlos Dominguez-Tagle, Elvio Hernandez, Roberto L. Lopez, Antonio Manescau, Heidi Moreno, Francisco Prada, Pablo Redondo, Vicente Sanchez de la Rosa, Nicolas A. Sosa, and Fabio Tenegi "LIRIS (Long-slit Intermediate Resolution Infrared Spectrograph): Assembly Integration and verification", Proc. SPIE 4841, Instrument Design and Performance for Optical/Infrared Ground-based Telescopes, (7 March 2003); https://doi.org/10.1117/12.458920

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