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Currently, the computation of Sigma_crit uses binned p(z)'s and effective lensing weights for each bin, as we've done it for the DES SV cosmic shear papers.
This isn't generally policeable and it lowers S/N because of the source/lens plane mixing.
The text was updated successfully, but these errors were encountered:
Currently, the computation of Sigma_crit uses binned p(z)'s and effective lensing weights for each bin, as we've done it for the DES SV cosmic shear papers.
This isn't generally policeable and it lowers S/N because of the source/lens plane mixing.
The text was updated successfully, but these errors were encountered: