FRIDA: The first instrument for the adaptive optics system of GTC

Bibcode
2007RMxAC..29...18L
López, J. A.; Bringas, V.; Cuevas, S.; Díaz, J. J.; Eikenberry, S. S.; Espejo, C.; Flores, R.; Fuentes, F. J.; Gallego, J.; Garzón, F.; Hammersley, P.; Pelló, R.; Prieto, A.; Sánchez, B.; Watson, A.
Referencia bibliográfica

First Light Science with the GTC (Eds. R. Guzmán, C. Packham, J. M. Rodríguez-Espinosa, & S. Torres-Peimbert) Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias) Vol. 29, pp. 18-20 (2007) (http://www.astroscu.unam.mx/~rmaa/)

Fecha de publicación:
6
2007
Número de autores
15
Número de autores del IAC
0
Número de citas
3
Número de citas referidas
1
Descripción
FRIDA (inFRrared Imager and Dissector for the Adaptive optics system of the Gran Telescopio Canarias) is being designed as a diffraction limited instrument with broad and narrow band imaging and integral field spectroscopy capabilities to operate in the wavelength range 0.9 - 2.5 μm. FRIDA is a collaborative project between the main GTC partners, namely, Spain, México and Florida. The main design characteristics of FRIDA are described in this contribution.
Tipo
Sin árbitro
Instrumentación

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