Fig. C.1
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Rotation-activity diagram as in Fig. 11, but here using the convective turnover timescale from Cranmer & Saar (2011). The vertical lines at Ro/Ro⊙ = 0.03 and 0.1 again represent the transition values from saturated to desaturated and desaturated to unsaturated stars, respectively. This is a consequence and a benefit of the usage of the rescaled Rossby number.
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