Fig. 6

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Posterior distributions and correlation between the anomalistic period and periastron precession rate where the chains converged. The middle plot shows the strong correlation between these two free parameters, as in Eq. (12). On the sides, are the corresponding histograms of the posterior distributions. As can be seen from the histograms on the sides, many chains converged to various positive and negative peaks, as predicted by the semi-grid method and reported in Table 5.
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