FRIDA, the diffraction limited NIR imager and IFS for the Gran Telescopio Canarias: status report

Bibcode
2014SPIE.9147E..1PL
DOI
10.1117/12.2057236
López, J. A.; Acosta, J. A.; Alvarez, L. C.; Bringas, V.; Cardiel, N.; Clark, D. M.; Corrales, A.; Cuevas, S.; Chapa, O.; Díaz Garcia, J. J.; Eikenberry, S. S.; Eliche, C.; Espejo, C.; Flores, R.; Fuentes, J.; Gallego, J.; Garcés, J.; Garzón, F.; Hammersley, P.; Keiman, C.; Lara, G.; López, P.; Lucero, D.; Moreno, H.; Pascual, S.; Patrón, J.; Prieto, A.; Rodríguez, A.; Rodríguez, B.; Sánchez, B.; Torres, D.; Uribe, J.; Watson, A.
Referencia bibliográfica

Proceedings of the SPIE, Volume 9147, id. 91471P 15 pp. (2014).

Fecha de publicación:
7
2014
Número de autores
33
Número de autores del IAC
7
Número de citas
0
Número de citas referidas
0
Descripción
FRIDA is a diffraction limited imager and integral field spectrometer that is being built for the Gran Telescopio Canarias. FRIDA has been designed and is being built as a collaborative project between institutions from México, Spain and the USA. In imaging mode FRIDA will provide scales of 0.010, 0.020 and 0.040 arcsec/pixel and in IFS mode spectral resolutions R ~ 1000, 4,500 and 30,000. FRIDA is starting systems integration and is scheduled to complete fully integrated system tests at the laboratory by the end of 2015 and be delivered to GTC shortly after. In this contribution we present a summary of its design, fabrication, current status and potential scientific applications.
Tipo
Sin árbitro

Te puede interesar

  • Sin árbitro
    Study of basaltic asteroids through their phase curves
    Introduction Classified as type-V, the basaltic asteroids of the Main Belt (MB), for the most part, are connected to Vesta's dynamic family. However, since the discovery of the V-type asteroid (1459) Magnya in the outer MB, several new asteroids have been found in different regions, including V-types from inner regions not belonging to the Vesta
    Arcoverde, Plicida et al.

    Fecha de publicación:

    9
    2024
    Bibcode
    2024EPSC...17..999A
    Número de citas
    0
  • Sin árbitro
    The Multi Frequency Instrument 2 (MFI2): mechanical design, manufacture, integration, and commissioning of the MFI2 for the QUIJOTE facility in Tenerife (Canary Islands)
    The QUIJOTE (Q-U-I JOint TEnerife) experiment combines the operation of two radio-telescopes and three instruments working in the microwave bands from 10 to 47 GHz at the Teide Observatory, Tenerife, which has already been presented in previous SPIE meetings. The new Multi Frequency Instrument (MFI2) led by the Instituto de Astrofísica de Canarias
    Lorenzo-Hernández, Haroldo et al.

    Fecha de publicación:

    7
    2024
    Bibcode
    2024SPIE13096E..33L
    Número de citas
    0
  • Sin árbitro
    ANDES, the high-resolution spectrograph for the ELT: RIZ & UBV spectrographs' preliminary design, analysis, and integration of the vacuum vessel and thermal enclosure
    The RIZ & UBV visible spectrographs of the ANDES instrument, which are foreseen to be installed at the Extremely Large Telescope, require to be under a very stable high vacuum and at an extremely stable temperature of 1mK to reach the radial velocity goal of 10cm/s RMS over a 10-year period. The baseline design, integration and first analyses of
    Santos Diaz, P. et al.

    Fecha de publicación:

    7
    2024
    Bibcode
    2024SPIE13096E..4KS
    Número de citas
    0