Fig. 6.

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Corner plot showing the posterior distributions of the orbital and PK parameters and the correlations between them for PSR J0955−6150 obtained from the non-linear timing of the pulsar with the DDH binary model using TEMPONEST. The off-diagonal elements show the correlation between the parameters and are marked contours that define the 39%, 86%, and 98% confidence levels, while the diagonal elements show the marginalised 1D posterior distributions of the parameters with the shaded region indicating nominal 1σ or 68.27% of the probability.
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