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Fig. 1

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Stellar parameters from Table 1 (shaded area) compared to Padova stellar evolution models (solid line) and Y2 models (dashed line). We note that the models differ slightly in their chemical composition. The bold regions on the tracks indicate the ratio of the stellar radius to the semi-major axis of the planetary orbit derived from its orbital period, the mass of the stellar model, and Kepler’s third law. The “+” symbols indicate 1 Gyr time steps.

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