Fig. 2

Excess distribution (left) and distribution of uncertainties on the disk-to-star flux ratio (right). The Gaussian overplotted on the excess distribution has a width of σ = 1 and is used to guide the eye and illustrates that the data are consistent with this ideal behavior. Vertical dashed lines are plotted at fCSE/σf = − 3 and fCSE/σf = + 3 for the excess distribution and at the median uncertainty (2.5 × 10-3) for the uncertainty distribution.
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