Fig. 10
STELLA light curves (upper panel), CaII H&K and H-α activity indicators (middle panel), and TERRA RVs (lower panel) phase folded using the same period P = 2.741 d and reference epoch of the STELLA V band photometry andKepler/K2 light curve in Fig. 1. Subplots for the light curves and RVs show the residuals O–C of the best-fit sine function obtained with the GLS software.
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