Low Energy Gamma Ray Observation of the Crab and Cygnus Region with the "miso" Telescope

Details Low Energy Gamma Ray Observation of the Crab and Cygnus Region with the "miso" Telescope Low Energy Gamma Ray Observation of the Crab and Cygnus Region with the "miso" Telescope

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....9...26p&link_type=abstract

Proceedings from the 18th International Cosmic Ray Conference, held in Bangalore, India, 22 August - 3 September, 1983. Volume

Physics

Scientific paper

During two balloon flights of the MISO telescope in 1979 and 1980, the Crab Nebula and Cygnus X-1 were studied in the hard X ray - soft γ ray energy band. The Crab Nebula was observed in 1980 and its spectrum was measured up to 2 MeV. Cygnus X-1 was observed on both occasions and was found to be in different hard X-ray states: in a superlow state in 1979 and in a low state 1980. No γ ray excess from this source was measured above few hundred keV.

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