Fig. C.7.
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Dependence of the ⟨ℳapn⟩ and ξκ to changes of baryonic and cosmological parameters. We scaled the model vectors using the same model just for a GrO case, disentangling the effect of the baryons. The θap = {θap, 1, θap, 2, θap, 3} values for the lowest panel are increasing from left to right as in Fig. 4, increasing first θap, 3, then θap, 2 and lastly θap, 1.
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