The characteristics and development status of the control and housekeeping electronics of FRIDA

J. J. Díaz; R. Flores-Meza; Beatriz Sánchez; Jesús Patrón

doi:10.1117/12.2056342

8 July 2014 The characteristics and development status of the control and housekeeping electronics of FRIDA

J. J. Díaz, R. Flores-Meza, Beatriz Sánchez, Jesús Patrón

Author Affiliations +

Proceedings Volume 9147, Ground-based and Airborne Instrumentation for Astronomy V; 914733 (2014) https://doi.org/10.1117/12.2056342
Event: SPIE Astronomical Telescopes + Instrumentation, 2014, Montréal, Quebec, Canada

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.

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J. J. Díaz, R. Flores-Meza, Beatriz Sánchez, and Jesús Patrón "The characteristics and development status of the control and housekeeping electronics of FRIDA", Proc. SPIE 9147, Ground-based and Airborne Instrumentation for Astronomy V, 914733 (8 July 2014); https://doi.org/10.1117/12.2056342

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