9 August 2016 MEGARA spectrograph mechanics and opto-mechanics in the AIV phase
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Abstract
MEGARA (Multi-Espectrógrafo en GTC de Alta Resolución para Astronomía) is the future optical Integral-Field Unit (IFU) and Multi-Object Spectrograph (MOS) for the GTC 10.4m telescope. The spectrograph is currently being integrated in the laboratory for a pre-shipping review in September 2016. This paper presents the current status and final performance of the spectrograph mechanics and opto-mechanics, composed of the mechanisms and the large optomechanical elements mounts.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Manuel Maldonado-Medina, Manuel Maldonado-Medina, Ana Pérez-Calpena, Ana Pérez-Calpena, María Luisa García Vargas, María Luisa García Vargas, Ernesto Sánchez-Blanco , Ernesto Sánchez-Blanco , Ismael Martínez Delgado, Ismael Martínez Delgado, Armando Gil de Paz, Armando Gil de Paz, Xabier Arrillaga Echaniz, Xabier Arrillaga Echaniz, Jesús Gallego Maestro, Jesús Gallego Maestro, Esperanza Carrasco Licea, Esperanza Carrasco Licea, Jorge Iglesias-Páramo, Jorge Iglesias-Páramo, Francisco Sánchez-Moreno, Francisco Sánchez-Moreno, } "MEGARA spectrograph mechanics and opto-mechanics in the AIV phase", Proc. SPIE 9908, Ground-based and Airborne Instrumentation for Astronomy VI, 99088S (9 August 2016); doi: 10.1117/12.2233041; https://doi.org/10.1117/12.2233041
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