Cumulative number of pulsars with pseudo-luminosity greater than a given pseudo-luminosity (L₁₂₈₄) as a function of the pseudo-luminosity. This figure is adapted from Fig. 3 in Martsen et al. (2022). We have used the known pulsar values as quoted in Martsen et al. (2022) and added the radiometer flux based estimates (see Sect. 3.7) for the ten new pulsars. It is evident that the linear trend tapers when going from right to left.