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

Bibcode
2024SPIE13096E..1YW
DOI
10.1117/12.3019191
Watson, Alan M.; Acosta-Pulido, José A.; Aguiar, Marta; Álvarez-Núñez, Luis C.; Béjar, Víctor J. S.; Cardiel, Nicolás.; Chapa, Oscar; Cuevas, Salvador; Díaz García, José Javier; Eikenberry, Stephen S.; Espejo, Carlos; Flores-Meza, Rubén. A.; Fuentes-Fernández, Jorge; Fujarte, José; Gallego, Jesús; Garcés Medina, José Leonardo; Garzón López, Francisco; Hammersley, Peter; Jovén Álvarez, Enrique; Keiman, Carolina; Lara, Gerardo; López, José Alberto; Matilla Blanco, Enol; Ortega, Carlos A.; Pascual Ramírez, Sergio; Patrón Recio, Jesús; Prieto, Almudena; Rodríguez, Berenice; Sánchez, Beatriz; Sánchez, Eleazar
Referencia bibliográfica

Ground-based and Airborne Instrumentation for Astronomy X

Fecha de publicación:
7
2024
Número de autores
30
Número de autores del IAC
9
Número de citas
0
Número de citas referidas
0
Descripción
FRIDA is a diffraction-limited imager and integral-field spectrograph for the adaptive-optics focus of the Gran Telescopio Canarias. In imaging mode FRIDA provides scales of 10, 20 and 40 mas/pixel and in IFS mode spectral resolutions of about 1200, 4000 and 30,000. Coronographic masks are available in both modes for highcontrast images. FRIDA is undergoing systems integration and is scheduled to complete system testing at the laboratory in December 2024 and to be delivered to the telescope shortly thereafter. In this contribution we present a summary of its design, fabrication, current status and potential scientific applications.
Tipo
Sin árbitro

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