Open Access

Fig. 7


Phase-folded transit light curves of planets (from top to bottom) b, c, d, e, f, and g. The best transit model is shown in red. The time scale is not the same between the first three and last three plots. The coverage of the last transit is not as good as in Christiansen et al. (2018) due to the differences in the pipeline used to correct for K2 systematics.

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