Data Reduction Pipeline for GTC/FRIDA

Bibcode
2009mavo.proc..105E
Eliche-Moral, M. C.; Cardiel, N.; Pascual, S.; Gallego, J.
Referencia bibliográfica

Multi-wavelength Astronomy and Virtual Observatory, Proceedings of the EURO-VO Workshop, held at the European Space Astronomy Centre of ESA, Villafranca del Castillo, Spain, 1-3 December, 2008, Eds.: D. Baines and P. Osuna, Published by the European Space Agency., p.105

Fecha de publicación:
7
2009
Número de autores
4
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
FRIDA (inFRared Imager and Dissector for the Adaptive optics system of the GTC) will be a NIR (1-2.5 μm) imager and Integral Field Unit spectrograph to operate with the Adaptive Optics system of the 10.4 m GTC telescope. FRIDA will offer broad and narrow band diffraction-limited imaging and integral field spectroscopy at low, intermediate and high spectral resolution. The Extragalactic Astrophysics and Astronomical Instrumentation group of the Universidad Complutense de Madrid (GUAIX) is developing the Data Reduction Pipeline for FRIDA. Specific tools for converting output, reduced datacubes to the standard Euro3D FITS format will be developed, in order to allow users to exploit existing VO applications for analysis. FRIDA is to be commissioned on the telescope in 2011.
Tipo
Sin árbitro

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