Fig. 7
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Phase-folded filtered (top plots) and residual (bottom plots) RVs for transiting planets b (top panel) and c (middle panel), and for candidate planet e (bottom panel) of AU Mic. Red dots show the individual RV measurements with their error bars, while black stars indicate average RVs over 0.1 phase bins. As in Fig. 4, the dispersion of RV residuals is 10.1 m s−1.
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