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Abstract:
ARGO is a "full coverage" air shower detector currently under construction in Tibet, China. One of the main goals of this experiment is to search for possible gamma-ray bursts (GRBs) with E>10GeV. In this work, the sensitivity in observing a GRB (with a certain significance) by ARGO is found to be dependent on the flux of the GRB, the slope and the energy cutoff of its spectrum, as well as its time duration and the zenith angle at the observation.
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References
|
[1]
|
. Meegan C A et al. Nature, 1992, 355: 143-1452. Metzger M R et al. Nature, 1997, 387: 878-8803. MA Xin-Hua et al. HEP NP, 2003, 27(11): 973-977(in Chinese)(马欣华等. 高能物理与核物理, 2003, 27(11): 973-977)4. Surdo A. Proc.28th ICRC. Tsukuba, Japan, 2003. 5|85. McEnery J E et al. 1999, Astro-Ph-99105496. ZHOU Xun-Xiu. Proc. 28th ICRC. Tsukuba, Japan, 2003.2757-27607. Adriani O et al. Nucl. Instrum. Methods in Physics Re-search, 2002, A488(1-2): 209-2258. Dingus B L et al. Proc. 25th ICRC. Durban, South Afria,1997. 30-329. CUI Shu-Wang et al. HEP NP, 2005, 29(1): 62-67 (in Chinese)(崔树旺等. 高能物理与核物理, 2005, 29(1): 62-67)10. CHEN Xin et al. HEP NP, 2004, 28(10): 1094-1098(in Chinese)(陈欣等. 高能物理与核物理, 2004, 28(10): 1094-1098)11. Hurley K et al. Nature, 1994, 372: 652-661
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