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Fig. 7
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Synthetic LCs for stars with different rotation rates as they would be observed in the Kepler passband at an inclination of i = 90°. We show non-nested cases (p = 0) with rotation rate values of 1Ω⊙ (blue), 2Ω⊙ (orange), 4Ω⊙ (green), and 8Ω⊙ (red).
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