Example of the results of our clustering procedure for NGC 2682 (upper panels) and Blanco 1 (lower panels). For each cluster, the three scatter plots represent (from left to right) a comparison between the members from CAN+20 (in orange) and ours (in blue) in proper motion space, in equatorial coordinate space, and in the color magnitude diagram. Rightmost panel: a Venn diagram for both clusters, in which the number of members in both studies is compared with members from CAN+20 in red, our members in green, and the overlap in orange.