mROC curves produced by inserting a total of 40 exoplanets for a set of contrasts (6 × 10⁻⁴, 4 × 10⁻⁴ and 2 × 10⁻⁴ from top to bottom) at annuli of different separations in the ranges 3–4, 2–3, and 1–2 FWHM (left, middle, and right columns, respectively). The x-axis is the mean FP per map and the y-axis corresponds to the TPR computed using Eq. (2). The numbers next to each data point correspond to the threshold that was applied to compute the number of TPs and FPs for each binary map (as described in Fig. 4).