Observations of southern sky gamma ray sources at Egamma greater than or equal to 300 GeV

Details Observations of southern sky gamma ray sources at Egamma greater than or equal to 300 GeV Observations of southern sky gamma ray sources at Egamma greater than or equal to 300 GeV

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974csgr.conf..279g&link_type=abstract

In ESRO The Context and Status of Gamma Ray Astronomy p 279-285 (SEE N75-25813 16-93)

Astronomy and Astrophysics

Astronomy

1

Energy Spectra, Gamma Rays, Radio Sources (Astronomy), Southern Hemisphere, Active Galaxies, Cerenkov Radiation, Compton Effect, Flux Density, Galactic Radiation, Models, Pulse Amplitude, Radiation Sources, Signal To Noise Ratios, Sky Radiation, X Ray Sources

Scientific paper

Results of three year observations of the active radio galaxy and X-ray source Cen A (NGC-5128) are reported. The Narrabri optical reflectors were used to detect the atmospheric Cerenkov light from extensive air showers with the double-beam technique allowing partial cosmic ray rejection. An improved timing system was employed and detected pulse heights were recorded so that spectral information is available. Preliminary results are presented, including evidence for the detection of Cen A(NGC-5128). Possible source models and some implications are discussed.

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