Physics
Scientific paper
Dec 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ncimc...7..682m&link_type=abstract
(Convegno Nazionale di Fisica Cosmica, 2nd, L'Aquila, Italy, May 29-June 1, 1984) Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol
Physics
9
Cosmic Ray Showers, Gamma Ray Bursts, Gamma Ray Telescopes, High Energy Interactions, Scintillation Counters, Energy Spectra, Radiant Flux Density, Statistical Analysis, Temporal Distribution
Scientific paper
The results of a search for cosmic gamma-ray bursts of primary energies E01 greater than 5 GeV and E04 greater than 20 TeV over time scales t = 1-100 ms, performed using the four-liquid-scintillation-counter EAS array (Morello and Navarra, 1981) at Plateau Rosa (elevation 3500 m) on 215 days during 1979-1982, are presented in tables and graphs and discussed. No counting-rate excess significantly above the statistical fluctuation is observed, although satellite detectors report at least 10 observable bursts during the operating period. Upper limits for the high-energy burst flux are established as phi1(E greater than E01) less than 0.00004 times t to the 0.36 erg/sq cm and phi4(E greater than E04) less than 0.000016 erg/sq cm for t less than 100 ms.
Morello C.
Navarra Gianni
Periale L.
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