Mass as a function of semi-major axis of all planets in all populations using ε = 0.9 (left two columns) or ε = 0.5 (right two columns). In these two groups the left column always gives the results for the pebble accretion model and the right column the product of the planetesimal accretion model. Each line represents a starting time. The colour-coding expresses the gas fraction for each planet at the end of the formation stage.