Rotation, activity, and stellar obliquities in a large uniform sample of Kepler solar analogs | Journal of Space Weather and Space Climate

Brightness Variations of the Sun and Sun-like Stars and Resulting Influences on their Environments

Open Access

Fig. 12.

(a) The distribution of measured rotation periods for the non-KOIs in our sample, (b–d) predicted distributions based on TRILEGAL population synthesis for the Kepler field combined with gyrochronology relations from Barnes (2007) (b), Mamajek & Hillenbrand (2008) (c), and Angus et al. (2015) (d). All of the gyrochronology relations, when applied to the TRILEGAL sample, underpredict the number of slow rotators in the sample.

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