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Fig. B.1.

image

Posterior pdfs for four stars in our sample (their Gaia EDR3 source_id is displayed at top of each panel). The thick black solid line represents p(d | o, mKsΘKM, ΘSM, ΘCMD). The coloured thin lines illustrate the different components of the pdfs. The correlation terms in the covariance matrix of Eq. (B.12) are neglected here for illustrative purposes. The distributions are scaled so that they peak at unity.

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