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Fig. 6
P − Ṗ diagram including the pulsars observed by Fermi/LAT and plot of the predicted γ-ray luminosity in the range 0.1 − 10 GeV for a random sample of pulsars. Gamma-ray luminosity Lγ versus the spindown luminosity Lsp for two random samples of millisecond and young pulsars. The lines Lγ = Lsp and 
are also shown.
This figure is made of several images, please see below:
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