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Fig. 3.
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Pulse profile for PSR J1841−0500 as observed by Camilo et al. (2012) at 4.8 GHz. The panels are as for PSR B1931+24 in Figure 2. For the RVM fit, we also display the solution shifted by 90 deg (solid and dashed lines) as this pulsar shows clear orthogonal jumps.
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