Fig. 3
Maximum contribution of microlensing to the measurements of the RM effect for different combination of planet mass and the position of the projection of the planet on the disk of the star. From top to bottom, the stellar rotational velocity is equal to 2, 5, and 10 km s-1, respectively. The detection limit of HARPS, ESPRESSO at VLT and HIRES at E-ELT are also shown for comparison.
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