Fig. 3
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RV observations from CORALIE (green) and HARPS (blue and orange for nights 1 and 2, respectively, analyzed dataset). The black line is a Keplerian model as reported in Kuhn et al. (2016). The inset plot in the upper right corner zooms in on the transit in detail. A strong and roughly symmetrical velocity anomaly due to the RM effect is observed during transit.
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