Maps for the growth and migration of planets around stars of 1 M_⊙ (left) and 0.1 M_⊙ (right) and at disk turbulent α_t = 10⁻³ (top) and 10⁻⁴ (bottom). The initial time t₀ and initial location r₀ are shownin x and y axis. The color corresponds to the final mass of the planet, and the black line represents the final location of the planet. The water ice line and the transition radius are labeled as magenta and cyan dashed lines. The parameters are adopted from run_D3 for the left panel and run_M3 for the right panel, respectively. We would like to note that the disk lifetimes in above two cases are longer than 3 Myr. Jupiter-mass planets can form around a 1 M_⊙ star while Earth-mass planets can form around a 0.1 M_⊙ star.