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V2required to move towards share XPCS/speckle analysis for CHX/CSXrequired to move towards share XPCS/speckle analysis for CHX/CSXV3lower priority, could be before V2 or after V2lower priority, could be before V2 or after V2_commonspecklepart of V2, but strictly related to a common repo (speckle + maybe scattering)part of V2, but strictly related to a common repo (speckle + maybe scattering)discussion
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See the issue below, as they are related, but this is to address a specific question of
np.histogram versus np.bincount raised in
#52
np.histogram is used for image based data because image normalization process creates floats (this is the case for csxtools get_fccd_images()). Some discussion of the various options would be good. Please add other options if I have missed one. We can consider multiple approaches too, but probably need to prioritize
- have 2 _process subfunctions: one for integer data (like Eiger detector) and one for float data
- convert floats to integers in a way that we agree.
- require input (whether images (aka full np.array) or compressed data) must be integers
@danielballan and others?
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V2required to move towards share XPCS/speckle analysis for CHX/CSXrequired to move towards share XPCS/speckle analysis for CHX/CSXV3lower priority, could be before V2 or after V2lower priority, could be before V2 or after V2_commonspecklepart of V2, but strictly related to a common repo (speckle + maybe scattering)part of V2, but strictly related to a common repo (speckle + maybe scattering)discussion