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Fig. 12.

image

Corner plot (as in Fig. 4) showing the posterior distribution of the astrometric solution for the CCO in G347.3−0.5. For this target, a relative astrometric frame registration method was applied as described in the text. We therefore measured no absolute positions, but only relative source displacements, which correspond to the components of proper motion. See Table B.1 for constraints on all parameters.

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