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Fig. 1.

image

Disk mass vs stellar mass after correcting the disk masses for the Gaia estimated distances and using the stellar masses derived here. Orange circles are used for targets observed with X-shooter, gray symbols for targets not observed, circles for ALMA detections, downward facing triangles for ALMA upper limits. The shaded regions delimit the disk mass ranges where the sample is complete with respect to the Barenfeld et al. (2016) one. The dashed gray lines delimit the bins used in the discussion. For the objects not observed with X-shooter, the distances, disk, and stellar masses from the literature are adopted.

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