Explanation of the exceptionally strong timing noise of PSR J0337+1715 by a circum-ternary planet and consequences for gravity tests

Open Access

Fig. D.1.

Correlation plot of the posterior distribution function of the PL3 model using the corresponding MCMC-generated sample, and restricted to $\bar{f}$ ${\bar{f}}$ , $\bar{\cdot} f$ ${\bar{\cdot}}f$ as well as PL3 specific parameters.

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