Number of formed S-type planets as a function of binary semi-major axis (a_bin) from the grid of 5000 simulations presented in Sect. 3.4. The dashed black line illustrates the log-uniform distribution of a_bin adopted as the initial condition (multiplied by 0.5 for better visualisation). The different colours of the bars correspond to different ranges of planet mass, indicated in the legend of the figure. The simulations assumed one embryo per disc and did not include the gravitational perturbation from the secondary or orbital migration.