Development of the FRIDA control software during the Integration and Testing phases
The FRIDA instrument is an integral field spectrograph and camera, both designedto work in high spatial resolution, at the diffraction limit of GTC (Gran Telescopio Canarias), in the range of 1 - 2.5 microns. FRIDA is a general purpose instrument for the entire GTC community, its construction approved by the Scientific Advisory Committee of GTC in
José Alfonso
López Aguerri
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