Phase-averaged spectrum and simulated lightrcurve of the millisecond pulsar J1614-2230 as calculated using our model, along with the best-fit power-law plus exponential cutoff fit (Abdo et al. 2009). The parameters that were used are Δ = 0.25, Γ = 20, χ = ζ = π/2 for the millisecond pulsar (left). For the young pulsar in the supernova remnant 3C 58 we used Δ = Δ_lim, Γ = 80, χ = π/5 and ζ = π/2.