Gamma rays of energy or = 10(15) eV from CYG X-3

Details Gamma rays of energy or = 10(15) eV from CYG X-3 Gamma rays of energy or = 10(15) eV from CYG X-3

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....1...67k&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 1 p 67-70 (SEE N85-33902 22-93)

Mathematics

Probability

1

Cosmic Ray Showers, Gamma Rays, Radiation Sources, Stars, Correlation, Data Acquisition, Estimates, Time

Scientific paper

The experimental data of extensive air showers observed at Akeno have been analyzed to detect the gamma ray signal from Cyg X-3. After muon poor air showers are selected, the correlation of data acquisition time with 4.8 hours X-ray period is studied, giving the data concentration near the phase 0.6, the time of X-ray maximum. The probability that uniform backgrounds create the distribution is 0.2%. The time averaged integral gamma ray flux is estimated as (1.1 + or - 0.4)x 10 to the -14th power cm(-2) sec(-1) for Eo 10 to the 15th power eV and (8.8 + or - 5.0)x 10 to the 14th power cm(-2) sec(-1) for Eo 6 x 10 to the 14th power eV.

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