It would be useful to have the option to return the covariance in mass and redshift bins. If we could do this, we could test the ideal case where we know the true mass and true redshift. This is the basic sanity check for the cluster implementation in FireCrown, so we could also use it for TJPCov.
It would be useful to have the option to return the covariance in mass and redshift bins. If we could do this, we could test the ideal case where we know the true mass and true redshift. This is the basic sanity check for the cluster implementation in FireCrown, so we could also use it for TJPCov.