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Fig. C.1.


Left panel: marginal posterior distribution of the CO model for the FWHM, i, and PA, exploring the full range of space parameters (see text). We note that the PA varies from 75° to 255° for graphical reasons to keep the distribution in a single curve. The vertical dashed lines represent the 16th, 50th, and 84th percentiles reported on the top of each marginal posterior distribution plot. Right panel: same as left panel but for a more constrained range of parameters.

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