Stellar mass distribution of accretors in the Sco-Cen clusters vs. cluster age (Baraffe et al. 2015-BpRp). The plot shows the stellar masses of all cluster members with pEW <  − 1.0 nm as derived in Sect. 2.5 (Table 2), and the cluster median both before (orange) and after (blue) applying the 0.06 < M_⋆ < 0.22 M_⊙ cut (red lines). The median mass is only shown if there are at least four cluster members in the chosen mass range. We note this filtering by stellar mass results in similar median stellar masses for all clusters.