Fig. 3
Plot showing the average emission profiles of the Crab pulsar at several frequencies observed at the WSRT arbitrarily aligned by the mainpulse peak. The first seven profiles are from the observations reported in this work, while profiles at 382, 608 and 1400 MHz are from the WSRT archives. The γ-ray profile is from Abdo et al. (2010). The arrow shows the location of the interpulse precursor emission component.
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