Fig. 3

Cluster membership probabilities for M 67 (top), NGC 654 (middle), and a cluster-free section of sky (bottom). Blue circles are the astrometric probabilities, green circles are the photometric probabilities, and red circles are the inferred joint distribution; the x-axis is the star’s identifying index (sorted by increasing joint probability). Typical variances for the estimated probabilities are on the order of –0.03.
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