Stellar mass vs measured dust mass inside the disk. We show the dust masses of Upper Sco in green (Barenfeld et al. 2016), Lupus in orange (Ansdell et al. 2016), and the ALMA Herbig sample in blue. On the right a histogram is plotted of the distribution of the dust masses. The grey points are four of the six borderline stars (see Sect. 2). HD 53367 and Z CMa are missing because no stellar mass is available from Vioque et al. (2018) or Wichittanakom et al. (2020).