Proceedings Paper
The characteristics and development status of the control and housekeeping electronics of FRIDA| Format | Member Price | Non-Member Price |
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Paper Abstract
FRIDA (inFRared Imager and Dissector for the Adaptive optics system of the Gran Telescopio Canarias) is a diffraction
limited instrument that will offer broad and narrow band imaging and integral field spectroscopy with low, intermediate
and high spectral resolutions in the 0.9 - 2.5 μm wavelength range. FRIDA will be installed at a Nasmyth focus of GTC,
behind the AO system. The characteristics and development status of the Control and Housekeeping Electronics are
described in this contribution.
FRIDA is a collaborative project between the IAC (Spain), UNAM (México), UCM (Spain) and the UF (Florida), lead
by UNAM.
Paper Details
Date Published: 8 July 2014
PDF: 7 pages
Proc. SPIE 9147, Ground-based and Airborne Instrumentation for Astronomy V, 914733 (8 July 2014);
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: 7 pages
Proc. SPIE 9147, Ground-based and Airborne Instrumentation for Astronomy V, 914733 (8 July 2014);
Show Author Affiliations
J. J. Díaz, Instituto de Astrofísica de Canarias (Spain)
R. Flores-Meza, Univ. Nacional Autónoma de México (Mexico)
R. Flores-Meza, Univ. Nacional Autónoma de México (Mexico)
Beatriz Sánchez, Univ. Nacional Autónoma de México (Mexico)
Jesús Patrón, Instituto de Astrofísica de Canarias (Spain)
Jesús Patrón, Instituto de Astrofísica de Canarias (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)
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