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Fig. 14


From the first to the fourth row, the γ-ray light curve multiplicity (left column) and peak separation (right column) as a function of α and ζ for LAT pulsars and PC, SG, OG, and OPC models are shown respectively. Big triangles and small points refer to LAT and simulated pulsars, respectively.

This figure is made of several images, please see below:

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