FRIDA: Near Infrared Imager and Integral Field Spectroscopy for GTC

Bibcode
2007RMxAC..28...69L
López, J. A.; Bringas, V.; Cuevas, S.; Díaz, J. J.; Eikenberry, S.; Espejo, C.; Flores, R.; Fuentes, F. J.; Gallego, J.; Garzón, F.; Hammersley, P.; Pelló, R.; Prieto, A.; Sánchez, B.; Watson, A. M.
Referencia bibliográfica

The 3rd Mexico-Korea Conference on Astrophysics: Telescopes of the Future and San Pedro Mártir (Eds. Stan Kurtz, José Franco, Seungsoo Hong, Guillermo García-Segura, Alfredo Santillán, Jongsoo Kim, & Inwoo Han) Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias) Vol. 28, pp. 69-72 (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
0
Número de citas referidas
0
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
Técnicas

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