
doi: 10.1063/1.3149457
handle: 11577/2447346
As is well known, the Crab pulsar displays a light curve with a characteristic double peak profile having a period of 33 milliseconds. Its pulse profile has been extensively monitored by several authors; it is also used for testing high‐speed photon counters. We have studied the optical light curve of the Crab pulsar by means of a novel photon counting instrument, that has the capability to provide data with exceptionally high temporal resolution and time tagging accuracy of each incoming photon.
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