Fig. A.1
Model of completeness as a function of stellar mass and radial position in the ONC according to Eq. (A.1) and using the parameters from Table A.1. From right to left the graphs represent increasing radii in steps of 0.25 pc from the centre to 2.5 pc, the outer boundary of the ONC. The solid (red), dashed (blue), and dotted (black) lines are grouped in steps of 1 pc, respectively.
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