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Fig. 1.


Pulse profile for PSR J2055+3829 at 1.4 GHz, formed by integrating 48.8 h of coherently dedispersed observations with the Nançay Radio Telescope and the NUPPI backend. Profiles recorded at orbital phases between 0.1 and 0.4 were excluded from the summation to avoid contamination of the integrated profile from dispersive delays caused by ionized material near the companion star. To improve readability we divided the number of phase bins by four to form a profile with 512 phase bins.

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