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Fig. A.1.

image

StarHorse posterior CMD for 1% of the stars, comparing the results with the PARSEC 1.2S stellar models used to infer the results. Objects in unphysical regions of the posterior CMD result from poor median statistics of multi-modal posterior PDFs (see discussion in Sect. 3.4) and are flagged in the first digit of SH_OUTFLAG.

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