Fig. 16.
Star-to-star comparison to the distance scale of the open cluster sample of Cantat-Gaudin et al. (2018a): relative distance difference as a function of cluster distance (for 60 284 stars with membership probabilities Pmemb = 1). Only 1% of the flag-cleaned stars in this sample show distance deviations greater than 50% (defined by the short-dashed grey lines).
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