Collection of functions for astronomical image analysis and processing. These tools involves pure python, but also are integrated with CASA (https://casa.nrao.edu/)
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Improve the background modelling for radio images. #7
Compare results when the background is fixed to be the residual map from deconvolution and when is set to be a multiplicative scalar of it (e.g. an additional parameter to me minimised)
Compare results with a simple flat-sky model
Compare results when a bkg estimator is used as a model of the background
The following experiments must be conducted: