GUI - Post-analysis Options

Once the modellings have been generated (by LIME for instance), hyper-spectral cubes (.fits files) can be analysed directly in GASS.

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It is possible, using GASS, to directly compare the models and the observations, and to retrieve the best fit of a set of models. This can be performed both for spectral or dust emission.

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Moment maps (0 and 1) can be displayed directly using the interface.

 

GASS can also simulate interferometric observations (more informations in the GASS paper).