Fig. 1.
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Flare energy as a function of spot group area for solar flares (black dots) and superflares of G-type stars from the Kepler sample by Okamoto et al. (2021). Left panel: Original Sun-like sample from Okamoto et al. (2021). Right panel: Updated solar observations based on the rescaling discussed in Hudson et al. (2024) (purple dots) and updated stellar sample utilizing the updated spot group area function from Herbst et al. (2021) (blue dots and associated errors).
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