Cardiel López, NicolásGallego Maestro, JesúsPascual Ramírez, SergioWatson, Alan M.Acosta-Pulido, José A.Álvarez-Núñez, Luis C.Brigas Rico, VicenteCuevas, SalvadorChapa, ÓscarFuentes-Fernández, Jorge2023-06-182023-06-18© 2016 SPI20160277-786X10.1117/12.2233069https://hdl.handle.net/20.500.14352/23214FRIDA is a diffraction-limited imager and integral-field spectrometer that is being built for the adaptive-optics focus of the Gran Telescopio Canarias. In imaging mode FRIDA will provide scales of 0.010, 0.020 and 0.040 arcsec/pixel and in IFS mode spectral resolutions of 1500, 4000 and 30,000. FRIDA is starting systems integration and is scheduled to complete fully integrated system tests at the laboratory by the end of 2017 and to be delivered to GTC shortly thereafter. In this contribution we present a summary of its design, fabrication, current status and potential scientific applications.engjournal articlehttp://dx.doi.org/10.1117/12.2233069http://proceedings.spiedigitallibrary.org/open access52Adaptive opticsInfrared imagingInfrared spectroscopyIntegral-field spectroscopyAstrofísicaAstronomía (Física)