save CDM+baryon linear power spectrum #33
Merged
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So far, the class interface allows to store the total (linear) matter power spectrum. However, there are applications like the halo mass function where the power spectrum of CDM+baryons is needed. The camb interface already allows to store the cdm+baryons linear power spectrum, this PR allows to do the same for class (using the same variable name
cdm_baryon_power_lin
). Thanks also to @asmaamaz