We no longer require hyper-galaxies to increase the noise in regions of an image fit which are poor, because multi-Gaussian expansions leave far fewer residuals for a galaxy fit.
The functionality associated with this takes up a lot of the source code and is cumbersome to maintain. However, I did not want to remove it entirely, because it may be necessary in the future.
All hyper functionality has therefore been isolated to a legacy module, out the way.
I have also removed all high-level examples for hyper function (e.g. in the workspace), removes the image sky / noise map features, removed it from SLaM pipelines.
Any functionality associated with adapting a pixelization mesh / regularization now uses the term adapt instead of hyper (e.g. HyperSetup -> AdaptSetup, hyper_dataset -> adapt_dataset).
We no longer require hyper-galaxies to increase the noise in regions of an image fit which are poor, because multi-Gaussian expansions leave far fewer residuals for a galaxy fit.
The functionality associated with this takes up a lot of the source code and is cumbersome to maintain. However, I did not want to remove it entirely, because it may be necessary in the future.
All hyper functionality has therefore been isolated to a
legacymodule, out the way.I have also removed all high-level examples for hyper function (e.g. in the workspace), removes the image sky / noise map features, removed it from SLaM pipelines.
Any functionality associated with adapting a pixelization mesh / regularization now uses the term
adaptinstead of hyper (e.g.HyperSetup->AdaptSetup,hyper_dataset->adapt_dataset).