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Fig. C.3.

Fig. C.3. Refer to the following caption and surrounding text.

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Best orbital solution for the AB outer orbit for the two assumed astrometric uncertainty values for data take before 1991. The solid black line corresponds to Solution I, and the dashed blue line to Solution II. The grey dots represent the astrometric measurements. A sketch of the mid-March disc position in the sky plane, based on the disc geometry adopted by Faruqi et al. (2025), is overplotted for both solutions.

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