FRIDA: THE AO SECOND GENERATION INSTRUMENT FOR GTC, STATUS REPORT

Belen Rosado Sanchez, Juan Antonio Diaz Acosta,Luis Alvarez,V Bringas,N Cardiel, Acela Maria Boffill Corrales,S Cuevas,Oscar Chapa, J J Diaz,Stephen S Eikenberry, M C Elichemoral, Carlos Espejo,R Flores,Francisco Garzon,Peter L Hammersley,C Keiman, Gerardo Lara, J A L Opez, Pedro Juan Tarraga Lopez,Daniel Sanchez Lucero, Herminia Arrazola Moreno,S Pascual,Jesus Patron,A Prieto, Angel Garcia Rodriguez, J Uribe,Andrew J Watson

Revista Mexicana de Astronomia y Astrofisica-Serie de Conferencias（2013）

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摘要

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 0.9-2.4 mu m. FRIDA is a collaborative project between the main GTC partners, namely, Spain, Mexico and University of Florida. The present paper provides an updated overview of the instrument development.

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关键词

instrumentation: spectrographs

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