Evolution of synthetic planets in the disk model given by disk-wind evolution (a) and viscous evolution (b). The colour of each point denotes a particular timestep since the begining of the simulation (t₀ = 1 Myr). The faded circles are synthetic planets that do not result in PDS 70-like planets at a time of 4 Myr after the beginning of the simulation. The squares show the successful PDS 70b synthetic planets, and the diamonds show the successful PDS 70c planets. The black circles and error bars are the values for PDS 70 b and c, as shown in Table 1. The grey lines connect the points from individual synthetic planets. The wind model can reproduce both planets b and c, although it over estimates the mass of planet b. The viscous model cannot reproduce planet c and underestimates the radial location of planet b. The inset of panel b shows the collection of successful synthetic planets for both the viscous and wind models. See the text for more details.