Observation of γ-RAYS > 10**15 EV from Cygnus X-3

Physics

Scientific paper

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Scientific paper

The existence of pulsed emission of ultra-high energy γ-rays (>1015eV) from Cyg X-3 with the characteristic period of 4.8h, discovered by Samorski and Stamm (1983), is confirmed using data from three arrays at Haverah Park. The authors also provide strong evidence that the pulsed γ-ray spectrum steepens above 1016eV.

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