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Fig. 9

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HD 147379 planet search. Top and middle panels: GLS periodograms of the HARPS-N YARARA-V1 RV time-series, in a model with correlated noise and with no Keplerian in the model (k0) and one Keplerian (k1) at a period of 86.5 days. Bottom panel: RV measurements phase-folded on the 86.5 days signal.
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