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Fig. 7

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Variations of the bisector span of CoRoT-17 RV data as a function of the measured velocities (top) and the residuals to the Keplerian fit (bottom). The first plot shows no correlation, a good indication for the planetary hypothesis as opposed to a blend binary signal. The second plot shows a weak correlation, owing the lowest SNR data of the sample (open points show the data where SNR is less than 5).

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