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High-energy γ-ray light curve of PSR0531 + 21
DOI: 10.1038/296723a0 Bibcode: 1982Natur.296..723W

Caraveo, P. A.; Bignami, G. F.; Hermsen, W. +8 more

The Crab pulsar (PSR0531 + 21) was one of the earliest identified sources of high-energy γ radiation1-6. As such it was selected as the first object of detailed study by ESA's γ-ray astronomy satellite COS B, launched in August 1975. The experiment and mission have been described elsewhere7. In the first 6 yr of operation COS…

1982 Nature
COS-B 43