ARGO-YBJ constraints on very high energy emission from GRBs
ARGO-YBJ Collaboration
刊名ASTROPARTICLE PHYSICS
2009
卷号32期号:1页码:47-52
关键词GAMMA-RAY BURSTS DETECTOR TEV CALIBRATION SEARCH ARRAY
学科分类Astronomy & Astrophysics; Physics
DOI10.1016/j.astropartphys.2009.05.005
通讯作者Chen, SZ (reprint author), Chinese Acad Sci, Key Lab Particle Astrophys, Inst High Energy Phys, POB 918, Beijing 100049, Peoples R China.
英文摘要The ARGO-YBJ (Astrophysical Radiation Ground-based Observatory at YangBajing) experiment is designed for very high energy gamma-astronomy and cosmic ray researches. Due to the full coverage of a large area (5600 m(2)) with resistive plate chambers at a very high altitude (4300 m a.s.l.), the ARGO-YBJ detector is used to search for transient phenomena, such as Gamma-ray bursts (GRBs). Because the ARGO-YBJ detector has a large field of view (similar to 2 sr) and is operated with a high duty cycle (>90%), it is well suited for GRB surveying and can be operated in searches for high energy GRBs following alarms set by satellite-borne observations at lower energies. In this paper, the sensitivity of the ARGO-YBJ detector for GRB detection is estimated. Upper limits to fluence with 99% confidence level for 26 GRBs inside the field of view from June 2006 to January 2009 are set in the two energy ranges 10-100 GeV and 10 GeV-1 TeV. (C) 2009 Elsevier B.V. All rights reserved.
类目[WOS]Astronomy & Astrophysics ; Physics, Particles & Fields
收录类别SCI
语种英语
WOS记录号WOS:000270699200004
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被引频次:20[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ihep.ac.cn/handle/311005/212909
专题中国科学院高能物理研究所_粒子天体物理中心_期刊论文
作者单位中国科学院高能物理研究所
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ARGO-YBJ Collaboration. ARGO-YBJ constraints on very high energy emission from GRBs[J]. ASTROPARTICLE PHYSICS,2009,32(1):47-52.
APA ARGO-YBJ Collaboration.(2009).ARGO-YBJ constraints on very high energy emission from GRBs.ASTROPARTICLE PHYSICS,32(1),47-52.
MLA ARGO-YBJ Collaboration."ARGO-YBJ constraints on very high energy emission from GRBs".ASTROPARTICLE PHYSICS 32.1(2009):47-52.
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