EAS-TOP - Results of gamma-ray astronomy at 10 exp 14 eV

Details EAS-TOP - Results of gamma-ray astronomy at 10 exp 14 eV EAS-TOP - Results of gamma-ray astronomy at 10 exp 14 eV

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ncimc..15..723a&link_type=abstract

Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol. 15 C, no. 5, p. 723-733.

Astronomy and Astrophysics

Astronomy

Cosmic Ray Showers, Gamma Ray Astronomy, Angular Resolution, Crab Nebula, Pulsars, Radio Bursts, Radio Sources (Astronomy)

Scientific paper

The EAS-TOP Extensive Air Shower array, on top of the underground Gran Sasso Laboratory, is fully operating as a gamma-ray astronomy observatory since the beginning of 1989. After showing the measured angular resolution of the detector, we present the results obtained from the analysis of 280 days of measurements in 1989-1990, with the purpose of investigating possible emission (d.c. and sporadic) from the candidate sources in the Northern Hemisphere at an energy, greater than 200 TeV.

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