
Proceedings Paper
MEGARA optical manufacturing processFormat | Member Price | Non-Member Price |
---|---|---|
$17.00 | $21.00 |
Paper Abstract
MEGARA is the future visible integral-field and multi-object spectrograph for the GTC 10.4-m telescope
located in La Palma. INAOE is a member of the MEGARA Consortium and it is in charge of the Optics
Manufacturing work package. MEGARA passed the Optics Detailed Design Review in May 2013, and the
blanks of the main optics have been already ordered and their manufacturing is in progress. Except for
the optical fibers and microlenses, the complete MEGARA optical system will be manufactured in
Mexico, shared between the workshops of INAOE and CIO. This includes a field lens, a 5-lenses collimator, a
7-lenses camera and a complete set of volume phase holographic gratings with 36 flat windows and 24 prisms,
being all these elements very large and complex. Additionally, the optical tests and the complete assembly of
the camera and collimator subsystems will be carried out in Mexico. Here we describe the current status of the
optics manufacturing process.
Paper Details
Date Published: 24 July 2014
PDF: 12 pages
Proc. SPIE 9147, Ground-based and Airborne Instrumentation for Astronomy V, 914771 (24 July 2014); doi: 10.1117/12.2055269
Published in SPIE Proceedings Vol. 9147:
Ground-based and Airborne Instrumentation for Astronomy V
Suzanne K. Ramsay; Ian S. McLean; Hideki Takami, Editor(s)
PDF: 12 pages
Proc. SPIE 9147, Ground-based and Airborne Instrumentation for Astronomy V, 914771 (24 July 2014); doi: 10.1117/12.2055269
Show Author Affiliations
E. Carrasco, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico)
G. Páez, Ctr. de Investigaciones en Óptica (Mexico)
F. Granados, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico)
E. Percino, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico)
E. Castillo-Domínguez, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico)
J. L. Avilés, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico)
G. Páez, Ctr. de Investigaciones en Óptica (Mexico)
F. Granados, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico)
E. Percino, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico)
E. Castillo-Domínguez, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico)
J. L. Avilés, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico)
M. L. García-Vargas, Fractal S.L.N.E (Spain)
A. Gil de Paz, Univ. Complutense de Madrid (Spain)
J. Gallego, Univ. Complutense de Madrid (Spain)
J. Iglesias-Páramo, Instituto de Astrofísica de Andalucía (Spain)
R. Cedazo, Univ. Politécnica de Madrid (Spain)
A. Gil de Paz, Univ. Complutense de Madrid (Spain)
J. Gallego, Univ. Complutense de Madrid (Spain)
J. Iglesias-Páramo, Instituto de Astrofísica de Andalucía (Spain)
R. Cedazo, Univ. Politécnica de Madrid (Spain)
Published in SPIE Proceedings Vol. 9147:
Ground-based and Airborne Instrumentation for Astronomy V
Suzanne K. Ramsay; Ian S. McLean; Hideki Takami, Editor(s)
© SPIE. Terms of Use
