Highlights of the ARGO-YBJ Experiment at 4,300 m a.s.l.
文献类型：期刊论文
| 作者 | ARGO-YBJ Collaboration |
| 刊名 | BRAZILIAN JOURNAL OF PHYSICS
 |
| 出版日期 | 2014 |
| 卷号 | 44期号:5页码:494-503 |
| 关键词 | GAMMA-RAY OBSERVATION COSMIC-RAYS GALACTIC PLANE CRAB-NEBULA ENERGY-SPECTRUM TEV EMISSION ANISOTROPY MILAGRO PULSAR |
| 通讯作者 | Cao, Z (reprint author), Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, POB 918, Beijing 100049, Peoples R China. |
| 英文摘要 | The ARGO-YBJ experiment in Tibet, China has been operated to survey the northern sky for gamma ray sources, transient or steady, for nearly 6 years. Many astrophysics observational results will be highlighted in this paper, such as the sky survey results, extended source observation, diffuse gamma rays from the galactic plane, and emission mechanism of AGNs and their flares. As the unique detector for EAS with a continuously sensitive area of 5,600 m (2), the ARGO-YBJ array catches almost all particles in the central part of showers. The high-quality data set for showers above few TeV has been used for cosmic ray measurements such as the energy spectrum and composition. All those results are summarized here. As one of the next generation ground-based high-altitude air shower detector, LHAASO is briefly introduced as the successor of ARGO-YBJ in the end of the paper. |
| 学科主题 | Physics |
| 类目[WOS] | Physics, Multidisciplinary |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000342165000007 |
| 公开日期 | 2016-02-25 |
| 源URL | [http://ir.ihep.ac.cn/handle/311005/213785]  |
| 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. Highlights of the ARGO-YBJ Experiment at 4,300 m a.s.l.[J]. BRAZILIAN JOURNAL OF PHYSICS,2014,44(5):494-503. |
| APA | ARGO-YBJ Collaboration.(2014).Highlights of the ARGO-YBJ Experiment at 4,300 m a.s.l..BRAZILIAN JOURNAL OF PHYSICS,44(5),494-503. |
| MLA | ARGO-YBJ Collaboration."Highlights of the ARGO-YBJ Experiment at 4,300 m a.s.l.".BRAZILIAN JOURNAL OF PHYSICS 44.5(2014):494-503. |
入库方式： OAI收割
来源：高能物理研究所
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