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Fig. A.1.

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Top: Corner plot of the posterior distributions for all fitted parameters for the Keplerian orbital velocity models K_db and K_fb. The results for the two magnetic field polarities are shown in different colours, and their respected log-evidence values are reported in the legend. Bottom: Maximum likelihood estimators compared to the data. Points denote the fitting using observational timestamps, while lines are made in post-processing for visual aid.

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