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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