Similar to Figure 9 but for the case where β = 3. In this case, all magnifications have comparable probability as predicted by Equation 11. The lensed LF (thick red line) lies a factor of ${\widehat{\mu }}^{\beta -1}$ above the nonlensed LF (blue line). The smaller number of events at high luminosity when compared to Figure 9 is due to the fact that the number of stars in the simulation is the same in both cases, but for the steeper LF there are more stars with lower luminosities. The number density if events concentrates around the CC, tracing the magnification.