Correction made to the normalisation of the simulated v_kick versus ẽ distributions of young objects (the figure shows the example of τ_c ≤ 10 Myr). The top panel shows the amount of objects per eccentricity bin for progrades (blue) and retrogrades (red) orbits, as well as the corrected amounts used for the normalisation (lightblue and lightred, respectively). The bottom panel shows the kick distributions for the five ẽ bins closest to 1 (indicated by colour), normalised using the corrected values shown above.