Fig. 12
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Time evolution of X-ray (5–100 Å), EUV (100–920 Å), and total XUV luminosity of TOI 1430, according to Penz et al. (2008) and the X-ray/EUV scaling by Sanz-Forcada et al. (2022) (red lines) and according to Johnstone et al. (2021) (blue lines). Uncertainties on the age and X-ray luminosity of TOI 1430 are also indicated. The gray area is the original locus for dG stars in Penz et al. (2008).
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