Fig. 7
Analysis of RVs for HD 200466A. Upper panels: measured RVs. Left panels: Lomb-Scargle periodogram. Right panels: temporal series of RVs and the residuals from the RV trend predicted by the binary orbital solution. Lower panels: RVs corrected for binary motion. Left panel: Lomb-Scargle periodogram of the residuals. Right panels: RVs of the residuals. Overplotted is the best Keplerian fit of RVs including the RV trend derived from HD 200466B and the residuals (Sect. 6).
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