Corner plot of a subset of the RM parameters. The contours show the 1, 2, and 3σ levels. Only 99% of the distribution is shown for clarity. The sky-projected obliquity angle (λ) is correlated with the impact parameter (b) but seems to be minimally impacted by the the RV trend line parameters (γ and ﹩\dot{\gamma }﹩), with the exemption of the largest λ values (with a near-flat RM signal near egress) corresponding to a tighter RV trend line solution. Remaining, unshown parameters are similarly Gaussian distributed with little correlation between parameters.