Fig. 13.

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Posterior probability distribution estimated trained on the D1 dataset (left) and training on the D3 dataset (right) (Table 2). These datasets both have the dn/dz selection but differ in the choice of fixing the cluster evolution γ parameters on their fiducial values. Four MDNs are trained per dataset each on a different survey area. These results are computed for the same target testing XOD, always of the appropriate survey size, that was produced having all 8 parameters free and with the dn/dz selection. We can see that fixing the γ parameters improves the accuracy of the NDE’s cosmological predictions.
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