Fig. 1.
Top: distance distribution of WDs from the catalog of Gentile Fusillo et al. (2019) compared to the distribution of OCs listed in Cantat-Gaudin et al. (2018a). Middle: comparison of the parallax error distribution of the WDs and OC member stars listed in Cantat-Gaudin et al. (2018a). Bottom: comparison of the average proper motion error (average of the RA and Dec components) of the WDs and OC members.
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