Sensitivity as a function of noise level using input data generated with 3 free parameters (exomoon radii, exomoon orbital phases, and noise levels, see Table 2; red curves) and with 14 free parameters (see Table 7; blue curves). The two methods are compared at a fixed exomoon radius of 1 R_⊕: ConvNet (solid curves) vs. ΔBIC (dashed curves). The sensitivity is plotted in bins of 50 ppm noise levels.