Proper motions (in galactic coordinates) of the likely Sco-Cen association as presented in the study by Pecaut & Mamajek (2016). Blue data points refer to eRASS1 detected member, green data points to eRASS1 detected nonmembers, red data points refer to eRASS1 non-detected members, and magenta data points to eRASS1 nondetected nonmembers. The red polygon demarcates the selection region for Sco-Cen members chosen by Damiani et al. (2019) to identify Sco-Cen members.