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Scientific paper
Feb 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..745..669d&link_type=abstract
HIGH ENERGY GAMMA-RAY ASTRONOMY: 2nd International Symposium on High Energy Gamma-Ray Astronomy. AIP Conference Proceedings, Vo
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1
Gamma-Ray Sources, Gamma-Ray Bursts, Neutrino, Muon, Pion, And Other Elementary Particle Detectors, Cosmic Ray Detectors
Scientific paper
The ARGO-YBJ experiment, currently under construction at the YangBaJing Laboratory (Tibet, P.R. China, 4300 m a.s.l.), could be upgraded with a large (~ 2500 m2) muon detector both to extend the sensitivity to γ-ray sources to energies greater than ~ 20 TeV and to perform a cosmic ray primary composition study. In this paper we present an evaluation of the rejection power for proton-induced showers achievable with the upgraded ARGO-YBJ detector. Minimum detectable γ-ray fluxes are calculated for different experimental setups.
Di Girolamo Tristano
di Sciascio Giuseppe
Fratini K.
Megna Ralph
Saggese L.
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