Abstract
AbstractUsing the high speed 2-d TRIFFID photometer, we have obtained phase resolved photometry of the Crab pulsar inUBVthat allows us to flux the unpulsed light curve component. Following de-extinction, weighted least-square fitting indicates a power-law exponent ofα= −0.62 ± 0.49. This is steeper than that reported for the peak components and its origin remains unclear with respect to contemporary magnetospheric theory.
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