Disk masses binned by incident FUV flux (in units of G₀). Blue points show the median dust mass in each bin, with uncertainties; the empirical 95th percentile disk mass is shown as a bold, dark blue line. The dashed gray line represents an empirical fit to the relation between the median dust mass and the FUV radiation field for the Survey of Orion Disks with ALMA (SODA) sample. The points in orange and green represent, for σ Ori and the Orion Nebula Cluster (ONC) respectively, the median and 95% disk mass (as lines), for the central 90% of the FUV distribution in these regions.