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Fig. 8

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RV induced by a 30 MJup planet with a 7400-day-period (9 AU sep.) located at the position of β Pic b in 2003, when using the actual data sampling: grey crosses: without jitter noise, black squares: with a noise of 275 m/s. The grey line indicates the slope derived from the linear fitting of RV variations, and the black line indicates the slope of the β Pic real data deduced from linear fitting.

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