Computer Science – Performance
Scientific paper
Apr 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aipc..220..257t&link_type=abstract
AIP Conf. Proc., No. 220, p. 257 - 264
Computer Science
Performance
Detectors: Cosmic Rays, Detectors: Gamma Rays
Scientific paper
The Tibet ASγ experiment, which has started since January, 1990, is located at an altitude of 4300 m at Yangbaging in Tibet, China (90.5°E, 30.1°N). The air-shower array is composed of 49 scintillation counters for fast timing, each counter having an area of 0.5 m2, in a grid pattern with a spacing of 15 m and 16 density detectors. The analysis of experimental data shows that the performance of array is realized as expected by the Monte Carlo simulation. The detection threshold energy for γ-rays is ≡40 TeV; the peak energy 20 TeV. The angular resolution around 100 TeV is ≡0.5°. The systematic error of arrival direction is considerably smaller than the angular resolution in the concerned energy region.
Amenomori Michihiro
Bai Z. W.
Cao Zhoujian
Ding Lin-Kai
Feng Zhao-Yang
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