Fig. 3
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Inflection point period, PIP, vs. rotation period derived by McQ14 for 30 582 stars (upper panel) and S21 for 48 264 stars (lower panel). The solid black line shows the relation given in Eq. (1) with α = 0.217. Both panels exhibit an upper branch where the GPS method detects (slightly more than) the double of the inflection period.
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