Same as Figs. 7a and b, but a linear stellar mass and luminosity correlation is adopted, with viscously heated and stellar irradiation disks in the left panel and pure stellar irradiation disks in the right panel. The characteristic disk size is fixed at 300 AU, and all embryos are assumed to start their growth at t₀ = 0 yr. The linear mass scaling between the planet and star can be obtained when the viscously heated inner disk regions are included. The planet masses are independent of their stellar masses when only stellar irradiated disks are considered.