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

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

Author Affiliations +

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.

Citation Download Citation

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

ACCESS THE FULL ARTICLE

INSTITUTIONAL
Select your institution to access the SPIE Digital Library.

SELECT YOUR INSTITUTION

PERSONAL
Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.

PERSONAL SIGN IN

No SPIE Account? Create one

PURCHASE THIS CONTENT

SUBSCRIBE TO DIGITAL LIBRARY

50 downloads per 1-year subscription

Members: $195

Non-members: $335 ADD TO CART

25 downloads per 1 - year subscription

Members: $145

Non-members: $250 ADD TO CART

PURCHASE SINGLE ARTICLE

Includes PDF, HTML & Video, when available