Total mass-loss rate, Ṁ(t), of the discs modelled with FARGO as a function of t∕t_park, where t_park is the time it takes the planet to get parked in each simulation. The lines are plotted starting from the times at which the planet is released and photoevaporation is activated. The total mass-loss rates are averaged over 100 orbits. Top panel: Ṁ_tot in the primordial discs, while the bottom one corresponds to transition discs.