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FRIDA (inFrared Imager and Dissector for Adaptative optics) is a second-generation instrument for the 10 m Gran Telescopio de Canarias (GTC) and the first proposed for working with its Adaptative Optics system.

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FRIDA DRP

This is FRIDA DRP, the data reduction pipeline for FRIDA.

FRIDA (inFrared Imager and Dissector for Adaptative optics) is a second-generation instrument for the 10m GTC (Gran Telescopio Canarias) and the first proposed for working with its Adaptive Optics system.

The software is under development. It is possible that changes may be made that render the code backward incompatible. For the time being, it is recommended to install the development version. This code makes use of the numina package, which contains common functionality for different GTC instrument pipelines.

Installing and running the development version

Please follow the instructions available in the online documentation.

Licensing

FRIDA DRP is distributed under GNU GPL, either version 3 of the License, or (at your option) any later version. See the file LICENSE.txt for details.

Authors

Maintainers: Nicolás Cardiel <[email protected]>, Sergio Pascual: <[email protected]>

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FRIDA (inFrared Imager and Dissector for Adaptative optics) is a second-generation instrument for the 10 m Gran Telescopio de Canarias (GTC) and the first proposed for working with its Adaptative Optics system.

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