Growth and migration of single protoplanets in disks of a long lifetime at different turbulent levels and pebble-to-gas mass flux ratios around stars of M_★ = 0.1 M_⊙. Three turbulent coefficients of α_t = 10⁻² (upper), 10⁻³ (middle) and 10⁻⁴ (lower) and two pebble-to-gas flux ratios of ξ_p/g = 1% (left) and 2% (right) are shown. The planet and disk parameters are listed in Table 1. The dashed line represents the pebble isolation mass at the time when the planet born at 1 au reaches this value. The increasing sizes of the dots denote the disk evolution at one Myr intervals. Compared to Fig. 2, more massive planets from in disk with a longer lifetime.