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