GRID: a student project to monitor the transient gamma-ray sky in the multi-messenger astronomy era | |
Wen, Jiaxing1,2,3; Long, Xiangyun4,5; Zheng, Xutao1,2; An, Yu6; Cai, Zhengyang4,5; Cang, Jirong1,2; Che, Yuepeng7; Chen, Changyu1,2; Chen, Liangjun6; Chen, Qianjun1,2 | |
刊名 | EXPERIMENTAL ASTRONOMY |
2019-08-01 | |
卷号 | 48期号:1页码:77-95 |
关键词 | Gamma-ray bursts Gravitational waves Scintillation detector SiPM CubeSat |
ISSN号 | 0922-6435 |
DOI | 10.1007/s10686-019-09636-w |
通讯作者 | Feng, Hua(hfeng@tsinghua.edu.cn) ; Zeng, Ming(mingzeng@tsinghua.edu.cn) ; Zhang, Bin-Bin(bbzhang@nju.edu.cn) |
英文摘要 | The Gamma-Ray Integrated Detectors (GRID) is a space mission concept dedicated to monitoring the transient gamma-ray sky in the energy range from 10 keV to 2 MeV using scintillation detectors onboard CubeSats in low Earth orbits. The primary targets of GRID are the gamma-ray bursts (GRBs) in the local universe. The scientific goal of GRID is, in synergy with ground-based gravitational wave (GW) detectors such as LIGO and VIRGO, to accumulate a sample of GRBs associated with the merger of two compact stars and study jets and related physics of those objects. It also involves observing and studying other gamma-ray transients such as long GRBs, soft gamma-ray repeaters, terrestrial gamma-ray flashes, and solar flares. With multiple CubeSats in various orbits, GRID is unaffected by the Earth occultation and serves as a full-time and all-sky monitor. Assuming a horizon of 200 Mpc for ground-based GW detectors, we expect to see a few associated GW-GRB events per year. With about 10 CubeSats in operation, GRID is capable of localizing a faint GRB like 170817A with a 90% error radius of about 10 degrees, through triangulation and flux modulation. GRID is proposed and developed by students, with considerable contribution from undergraduate students, and will remain operated as a student project in the future. The current GRID collaboration involves more than 20 institutes and keeps growing. On August 29th, the first GRID detector onboard a CubeSat was launched into a Sun-synchronous orbit and is currently under test. |
WOS关键词 | NEUTRON-STAR ; ELECTROMAGNETIC COUNTERPART ; KILONOVA ; BURSTS ; NUCLEOSYNTHESIS ; PERFORMANCE ; EMISSION |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | SPRINGER |
WOS记录号 | WOS:000481758700005 |
内容类型 | 期刊论文 |
源URL | [http://libir.pmo.ac.cn/handle/332002/28071] |
专题 | 中国科学院紫金山天文台 |
通讯作者 | Feng, Hua; Zeng, Ming; Zhang, Bin-Bin |
作者单位 | 1.Tsinghua Univ, Dept Engn Phys, Beijing 100084, Peoples R China 2.Tsinghua Univ, Ctr Astrophys, Beijing 100084, Peoples R China 3.China Acad Engn Phys, Laser Fus Res Ctr, Sci & Technol Plasma Phys Lab, Mianyang 621900, Sichuan, Peoples R China 4.Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China 5.Tsinghua Univ, Ctr Astrophys, Beijing 100084, Peoples R China 6.Guangxi Univ, Dept Phys, Guangxi Key Lab Relativist Astrophys, Nanning 530004, Guangxi, Peoples R China 7.Ningbo Univ Technol, Sch Elect & Informat Engn, Ningbo 315211, Zhejiang, Peoples R China 8.Shanghai Jiao Tong Univ, Dept Instruments Sci & Engn, Shanghai 200240, Peoples R China 9.Ningbo Univ, Sch Mat Sci & Chem Engn, Ningbo 315211, Zhejiang, Peoples R China 10.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210093, Jiangsu, Peoples R China |
推荐引用方式 GB/T 7714 | Wen, Jiaxing,Long, Xiangyun,Zheng, Xutao,et al. GRID: a student project to monitor the transient gamma-ray sky in the multi-messenger astronomy era[J]. EXPERIMENTAL ASTRONOMY,2019,48(1):77-95. |
APA | Wen, Jiaxing.,Long, Xiangyun.,Zheng, Xutao.,An, Yu.,Cai, Zhengyang.,...&Zhu, Zonghong.(2019).GRID: a student project to monitor the transient gamma-ray sky in the multi-messenger astronomy era.EXPERIMENTAL ASTRONOMY,48(1),77-95. |
MLA | Wen, Jiaxing,et al."GRID: a student project to monitor the transient gamma-ray sky in the multi-messenger astronomy era".EXPERIMENTAL ASTRONOMY 48.1(2019):77-95. |
个性服务 |
查看访问统计 |
相关权益政策 |
暂无数据 |
收藏/分享 |
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。
修改评论