Current SRD yaml files assume the "Eisenstein & Hu" power spectrum although the right one to assume is "HaloFit" if one wants to reproduce the SRD plots. Te rason behind choosing EH is that when doing the MCMC, CAMB (or CLASS?) give trouble with certain wa/w0 combinations. We should check if the newer versions of CCL provide an elegant exit for this problem already.
Current SRD yaml files assume the "Eisenstein & Hu" power spectrum although the right one to assume is "HaloFit" if one wants to reproduce the SRD plots. Te rason behind choosing EH is that when doing the MCMC, CAMB (or CLASS?) give trouble with certain wa/w0 combinations. We should check if the newer versions of CCL provide an elegant exit for this problem already.