arxiv: 1605.09660 · v1 · pith:NXHJ57E4new · submitted 2016-05-31 · 🌌 astro-ph.IM

FRIDA: diffraction-limited imaging and integral-field spectroscopy for the GTC

Alan M. Watson , Jos\'e A. Acosta-Pulido , Luis C. \'Alvarez-N\'u\~nez , Vicente Bringas-Rico , Nicol\'as Cardiel , Salvador Cuevas , Oscar Chapa , Jos\'e Javier D\'iaz Garc\'ia

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Stephen S. Eikenberry Carlos Espejo Rub\'en A. Flores-Meza Jorge Fuentes-Fern\'andez Jes\'us Gallego Jos\'e Leonardo Garc\'es Medina Francisco Garz\'on L\'opez Peter Hammersley Carolina Keiman Gerardo Lara Jos\'e Alberto L\'opez Pablo L. L\'opez Diana Lucero Heidy Moreno Arce Sergio Pascual Ramirez Jes\'us Patr\'on Recio Almudena Prieto Alberto Jos\'e Rodr\'iguez Jos\'e Marco de la Rosa Beatriz S\'anchez Jorge A. Uribe Francisco V\'aldez Berriozabal

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keywords fridadiffraction-limitedimagingintegral-fieldmodeadaptive-opticsapplicationsarcsec

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FRIDA 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.

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FRIDA: diffraction-limited imaging and integral-field spectroscopy for the GTC

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