Upper limits of hard gamma-ray emission from six X-ray sources
M. Campbell, J. K. Alexander, Jr. Ball S. E., K. Greisen, D. Koch, B. McBreen
Abstract
M. Campbell, J. K. Alexander, Jr. Ball S. E., K. Greisen, D. Koch, B. McBreen
Abstract
The Cornell 100-inch gamma-ray telescope has been used to set upper limits for the gamma-ray flux above 400 MeV from the X-ray sources Cyg X-1, Cyg X-2, Cyg X-3, Cas A, Cas B, and Per X-1. An upper limit for the diffuse flux of the galactic disk was set which is consistent with OSO-3 and SAS-2 data. A new measurement of the atmospheric gamma-ray generation rate is presented.
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The Cornell 100-inch gamma-ray telescope has been used to set upper limits for the gamma-ray flux above 400 MeV from the X-ray sources Cyg X-1, Cyg X-2, Cyg X-3, Cas A, Cas B, and Per X-1. An upper limit for the diffuse flux of the galactic disk was set which is consistent with OSO-3 and SAS-2 data. A new measurement of the atmospheric gamma-ray generation rate is presented.
Key concepts: Physics, Astrophysics, Astronomy, Gamma ray, Flux (metallurgy), X-ray astronomy, Telescope, Gamma-ray astronomy