Fig. 1

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Luminosity series of a Sun-like star from the ZAMS up to TACHeB parametrized as function of stellar age, τ, (a) versus of the timescale-adapted evolutionary coordinate, , before (b) versus after (c) CHeB data augmentation and normalization to s. The original MIST data contains phase labels for each model, which the predictive models (the surrogate model and HNNI) do not see.
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