ARGO-YBJ constraints on very high energy emission from GRBs
文献类型：期刊论文
| 作者 | ARGO-YBJ Collaboration |
| 刊名 | ASTROPARTICLE PHYSICS
 |
| 出版日期 | 2009 |
| 卷号 | 32期号:1页码:47-52 |
| 关键词 | GAMMA-RAY BURSTS DETECTOR TEV CALIBRATION SEARCH ARRAY |
| 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. |
| 学科主题 | Astronomy & Astrophysics; Physics |
| 类目[WOS] | Astronomy & Astrophysics ; Physics, Particles & Fields |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000270699200004 |
| 公开日期 | 2016-02-25 |
| 源URL | [http://ir.ihep.ac.cn/handle/311005/212909]  |
| 专题 | 高能物理研究所_粒子天体物理中心 |
| 作者单位 | 中国科学院高能物理研究所 |
| 推荐引用方式 GB/T 7714 | 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. |
入库方式： OAI收割
来源：高能物理研究所
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