Fig. B.1.

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StarHorse posterior probability distributions for four example stars. In the off-diagonal sub-panels we show the two-dimensional projections of the five-dimensional posterior PDF (mass, age, metallicity, distance, and extinction) as approximated by a three-component Gaussian mixture model as black contours, while the diagonal panels show the 1D posterior approximations. The blue vertical lines show the median values directly inferred from the full posterior (available in the CDS tables and through ADQL).
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