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Fig. 4
RV variability in m s-1 over the 8-day span of the dataset about the mean (dotted line – 13.232 km s-1). The red line shows the predicted RV contribution of the planet over the same timeframe using the reported ephemeris (Mayor et al. 2004). As in Fig. 3, the x-axis shows the time in Barycentric Julian Date.
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