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Add functions to cosmo_val to perform the computation of pseudo-cls data vector and covariances in the tomographic case.
To do
Some of the implementation already exists in Euclid's FDQA.
It can be a good time to break the harmonic space related computation in elementary functions.
Add functions for the covariance based on OneCovariance.
See how to incorporate Gaussian simulations. This is quite heavy and MPI paralelisation worked great. Relying on MPI makes the incorporation to cosmo_val more complex. It maybe is better to have it as an external script.
Activity
cailmdaley commentedon Aug 31, 2026
Completed via #221/#240.