It would be useful to have functions in the library that take an array of galaxy numbers per shell (as e.g. produced by partition()), potentially a list of biases, and return the expected angular power spectra for angular clustering (from redshifts()) and lensing (from MultiPlaneConvergence).
Note that multi_plane_matrix() already implements the way to get the lensing contributions from each shell. This function would be a small extension to that, incorporating the (diagonal) matrix of biased angular clustering, and applying both directly to the input Cls.
It would be useful to have functions in the library that take an array of galaxy numbers per shell (as e.g. produced by
partition()), potentially a list of biases, and return the expected angular power spectra for angular clustering (fromredshifts()) and lensing (fromMultiPlaneConvergence).Note that
multi_plane_matrix()already implements the way to get the lensing contributions from each shell. This function would be a small extension to that, incorporating the (diagonal) matrix of biased angular clustering, and applying both directly to the input Cls.