The CSE decomposition of certain mass profiles was hard-coded to only go to a certain radii (e.g. around 7.5"), because we wrote them for galaxy scale lenses.
This branch updates the implementation to work over much larger scales, based on the input grid, for galaxy cluster / weak lensing science.
The first PR push is only for the NFW, I will update all other profiles (including those using an MGE) before merging.
The CSE decomposition of certain mass profiles was hard-coded to only go to a certain radii (e.g. around 7.5"), because we wrote them for galaxy scale lenses.
This branch updates the implementation to work over much larger scales, based on the input grid, for galaxy cluster / weak lensing science.
The first PR push is only for the
NFW, I will update all other profiles (including those using an MGE) before merging.