Fig. 8
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RV observed data (red dots) vs. time. The inferred model is shown as a solid line, using as prior Ppeak = 94.13 d. The parameters resulting from the MCMC inference, as well as the corresponding mass lower limit, are collected in the bottom left box. The shaded region shows the confidence interval at 1σ (dark gray) and 2σ (light gray) for the hypothesis with a planet.
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