Fig. B.1
Top panel: out-of-transit master stellar spectrum at the Na doublet and Hα lines. The strong interstellar Na absorption, indicated by the gray shadow, can be noticed on the red side of the stellar Na absorption. The wavelength is in the stellar rest frame. Bottom panel: transmission spectrum without the CLV and RM correction. The best-fit planet absorption presented in Fig. 9 has been removed. The red line shows the combined CLV and RM model.
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