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Pc)) Fig. 5 In each plot the distribution is that of the overall radio pulsar population. Overplotted in each case are up to 11 impulses denoting the parameter values of the original PMPS RRATs. The ˙ B, E, ˙ τ, BLC , distance and DM. In some cases the abscissa is plotted parameters plotted are: P, P, linearly, in some as a base-10 logarithm P˙ and none of these can fall into a ‘normal’ area of P − P˙ space. They will either be high B sources (possibly in the magnetar region) or old ‘dying’ pulsars.

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