Cumulative distribution of our sample in relation to the full Lupus disk population. Top panel: dust masses taken from Ansdell et al. 2016 of all Lupus disks detected in continuum (gray), Lupus disks resolved in continuum (blue) and our sample (red; see Sect. 2.2). Middle panel: same as above, but showing stellar masses derived from X-shooter spectra Alcalá et al. (2017), but recalculated using the new Gaia DR2 distances (see Appendix A in Alcalá et al. 2019). Bottom panel: same as above, but showing dust outer radii (R_mm).