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Fig. 3

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Validation data results for the ffNN-based stellar evolution emulator. The histograms and summary statistics of the residuals , over the validation data k = 1, …, Nval are shown, for YL in panel a, for YT in panel b, and for Yg in panel c. We calculate the mean , the standard deviation σϵ, the most extremal underprediction ϵ+, and the most extremal overprediction ϵ. Overall, the distribution of residuals is globally symmetric around near 0, with a sharper peak than a Gaussian, reminiscent of a Cauchy distribution.

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