Properties of the formed moons as a function of the size of the circumplanetary disks. Panel A shows the average number, panel B shows the average individual mass, and panel C shows the average eccentricity of the moons. Solid and dotted lines display the SC and the PC simulations, respectively. Black and gray lines are the simulations with cold and hot disks around M_pl = 10 M_J host planets. Vertical error bars indicate the standard deviation from the average values, which come from 10 simulations for each disk size. Red and orange lines display simulations with M_pl = 2 M_J and 5 M_J host planets, respectively. The colors of the shading indicate the same stellar distances as in Fig. 3.