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Fig. 3

Recurrence of the shape classes described in Tables 2 and 3 and shown in Tables A.1 and A.2 for the γ-ray pulsars (top panels), radio pulsars (bottom panel), and each model for the whole simulated pulsar population and its visible subsample, as synthesised by Pierbattista et al. (2012).
This figure is made of several images, please see below:
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