Experimental results on gamma-ray sources at E0 = 10(13) - 10(14) eV

Details Experimental results on gamma-ray sources at E0 = 10(13) - 10(14) eV Experimental results on gamma-ray sources at E0 = 10(13) - 10(14) eV

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....1..127m&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 1 p 127-130 (SEE N85-33902 22-93)

Astronomy and Astrophysics

Astronomy

Cosmic Ray Showers, Gamma Ray Astronomy, Gamma Rays, Pulsars, Radiation Sources, Accuracy, Arrays, Data Processing, Detection, Histograms, Signal To Noise Ratios

Scientific paper

The detection of very high energy gamma ray sources has been reported in the last few years by means of extensive air shower observations. The Plateau Rosa array for the registration of the arrival directions of extensive air showers has been operating since 1980 and first results on Cygnus X-3 have been reported. Here, the status of observations of Cygnus X-3 and of the Crab Pulsar are reported.

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