Data Reduction Pipeline for GTC/FRIDA

Details Data Reduction Pipeline for GTC/FRIDA Data Reduction Pipeline for GTC/FRIDA

2009-11-30

arxiv.org/abs/0911.5437v1

Multi-wavelength Astronomy and Virtual Observatory, Proceedings of the EURO-VO Workshop, 2009, Eds. D. Baines and P. Osuna, Eu

Astronomy and Astrophysics

Astrophysics

Instrumentation and Methods for Astrophysics

2 pages, 3 figures, Proceedings of the EURO-VO Workshop "Multi-wavelength Astronomy and Virtual Observatory", held at the Euro

Scientific paper

FRIDA (inFRared Imager and Dissector for the Adaptative optics system of the GTC) will be a NIR (1-2.5microns) imager and Integral Field Unit spectrograph to operate with the Adaptative Optics system of the 10.4m 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.

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