Fig. 15.
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Cumulative distribution of rotation periods in the context of RV selection biases. Red solid: rotation period distribution of stars discarded in the planet occurrence analysis of Ribas et al. (2023); green dashed: stars in common with Ribas et al. (2023) that are not known to be planet hosts; blue dot-dashed: known planet hosts in Ribas et al. (2023).
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