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Fig. 2

image

Phases. Variations of the MBL according to different parameters, with the same fixed parameters as in Fig. 1. Top: the impacting parameters are the exoplanet diameter (left) and the stellar diameter (right). Bottom: the impacting parameters are the spot temperature (left) and the exoplanet location on the stellar disk (right), for which θp = 0.15 mas. MBL are calculated for 20° (triangles) and (diamonds) variations.

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