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. 9.

(a) Compares histograms for the range distributions for the KOI and non-KOI samples, (b) CFDs for the two cases. The KOIs appear systematically more active than the non-KOIs, which is confirmed by statistical testing (K-S p < 10⁻⁶). We discuss our interpretation of this difference in Section 3.3.

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