Fig. C.3
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Periodogram of the RV residuals of HD189567, after sequentially removing, from top to bottom, the instrumental RV offsets, the 14.3 d Keplerian signal, a linear detrending with FWHM and polynomial drift, and lastly the 33.7 d Keplerian signal. False alarm probability (FAP) thresholds are shown as horizontal lines for FAP=10%, 1% and 0.1%.
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