Fig. 1
Radial velocity measurements of the HD 59686 system. Note that a jitter of 19.83 m s-1 was added in quadrature to the formal RV uncertainties, and this is reflected in the plot. Upper left: lick RVs together with the best Keplerian fit to the data. Upper right: RV residuals from the fit. Lower left: phased RV variations and Keplerian fit for the ~7 MJup planet HD 59686 Ab after subtracting the signal of the stellar companion. Lower right: RV data and Keplerian fit for the ~0.5 M⊙ stellar object HD 59686 B after subtracting the planetary signal.
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