INTEGRAL observation of the Crab pulsar

In this paper, we present the timing and spectral analysis of several observations of the Crab pulsar with INTEGRAL. All these observations, when summed together provide an high-statistics data set which can be used for accurate phase resolved spectroscopy of the pulsed emission over the energy range 3–350 keV. In particular, we present the light curves in several energy ranges and phase-resolved spectral analysis of the pulsed emission.