Fig. 3.


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The results of our period-finding algorithm applied to an array of model stars with a range of magnitudes from 10 to 16 and noise from Gilliland et al. (2011). Artificial spots were added as described in the text. While period recovery begins to suffer for P > 30 d, errors are typically <20% for P < 40 d, even for the fainter stars in our sample (Kmag > 14, shown in black).

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