Publication:
MEGARA MOS: where are my positioners and fibers pointing to?

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2018
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Pérez Calpena, Ana
Sánchez-Blanco Mancera, Ernesto
Gómez Álvarez, Pedro
Martínez Delgado, Ismael
Castillo Morales, África
Gil de Paz, Armando
Arrillaga, Xabier, Xabier
García Vargas, Marisa Luisa
Carrasco Licea, Esperanza
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SPIE-Int Soc Optical Engineering
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Abstract
MEGARA is an integral-field and multi-object medium-resolution spectrograph for the GTC 10.4m telescope, which was commissioned on June - August 2017. MEGARA offers two observing modes, the LCB mode, a large central IFU; and a Multi-Object Spectrograph (MOS) mode, composed by 92 robotic positioners carrying 7-fiber minibundles each. This paper presents the models and measurements developed for the alignment between the image of the telescope pupil and the 100-itm fiber cores during the integration and verification at the laboratory. On the one hand, the error in the positioner-minibundles assembly was optimized with the aim of achieving a fiber-to-fiber flux homogeneity better than 10%. On the other hand, the positioner pointing was characterized in order to achieve a pointing precision of 1/5 of the spaxel size (which has been designed to be 0.62 arcsec). The on-sky measurements obtained during the commissioning to verify our laboratory results are also presented.
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© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only. Conference on Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation (III. 2018. Austin, TX)
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