Resulting kick estimates (blue and red solid lines) for the young pulsars in the sample of Verbunt et al. (2017, blue and left column) and the expanded sample of Igoshev (2020, red and right column), similar to Fig. 6 but excluded pulsars with τ_kin > τ_c + 5 Myr. We fitted log-normal distributions (solid light blue/red) to the results in each panel, and to the results corresponding to the ages analysed by the literature we also fitted Maxwellians and double-Maxwellians (dashed light blue/red and grey lines). The corresponding distributions posed by Verbunt et al. (2017) and Igoshev (2020) are also shown (dotted light blue/red and grey lines).