A duty cycle, δ, as a function of spin period for Galactic pulsars (gray circles), previously known Magellanic Cloud pulsars (orange triangles), and the five pulsars reported in this work (green triangles). The shaded regions and contours show the 50%, 80%, and 95% highest-density regions of a 2D Gaussian kernel-density estimate fitted to the Galactic population in ﹩({\mathrm{log}}_{10}P,{\mathrm{log}}_{10}\delta )﹩ space.