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Fig. B.2.

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Same as Fig. 4, but we show the data vector for the individual cosmologies from our Cosmology Training Set, colour-coded by their respective value of S8 (dotted lines) and the measured values in the DES-Y1 survey (black). For a better visibility, all values are divided by the mean of our Covariance Training Set. In addition, we predict with the GPR Emulator a data vector where Ωm is increased by 80% with respect to the cosmology of the Covariance Training Set (dashed line), one where S8 is increased by 10% (dash-dotted line), and one where Ωm is increased by 80% and simultaneously S8 is decreased by 10% (solid line).

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