PMO OpenIR
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; Chen, Ziyun8,9; Cheng, Yingjie10; Deng, Litao6; Deng, Wei6; Ding, Wenqing11; Du, Hangci4,5; Duan, Lian12; Gan, Quan4,5; Gao, Tai12; Gao, Zhiying12; Han, Wenbin1,2; Han, Yiying12; He, Xinbo13; He, Xinhao14; Hou, Long12; Hu, Fan15; Hu, Junling6; Huang, Bo6; Huang, Dongyang1,2; Huang, Xuefeng6; Jia, Shihai1,2; Jiang, Yuchen1,2; Jin, Yifei1,2; Li, Ke12; Li, Siyao14; Li, Yurong12; Liang, Jianwei1,2; Liang, Yuanyuan12; Lin, Wei1,2; Liu, Chang1,2; Liu, Gang1,2; Liu, Mengyuan12; Liu, Rui16; Liu, Tianyu12; Liu, Wanqiang4,5; Lu, Di'an1,2; Lu, Peiyibin1,2; Lu, Zhiyong1,2; Luo, Xiyu12; Ma, Sizheng4,5; Ma, Yuanhang1,2; Mao, Xiaoqing12; Mo, Yanshan6; Nie, Qiyuan1,2; Qu, Shuiyin12; Shan, Xiaolong17; Shi, Gengyuan18; Song, Weiming10; Sun, Zhigang9,19; Tan, Xuelin6; Tang, Songsong12; Tao, Mingrui12; Wang, Boqin1,2; Wang, Yue1,2; Wang, Zhiang20; Wu, Qiaoya14; Wu, Xuanyi4,5; Xia, Yuehan6; Xiao, Hengyuan4,5; Xie, Wenjin6; Xu, Dacheng1,2; Xu, Rui1,2; Xu, Weili12; Yan, Longbiao12; Yan, Shengyu6; Yang, Dongxin1,2; Yang, Hang21; Yang, Haoguang11; Yang, Yi-Si10; Yang, Yifan4,5; Yao, Lei4,5; Yu, Huan1,2; Yu, Yangyi1,2; Zhang, Aiqiang1,2; Zhang, Bingtao1,2; Zhang, Lixuan21; Zhang, Maoxing1,2; Zhang, Shen12; Zhang, Tianliang1,2; Zhang, Yuchong4,5; Zhao, Qianru12; Zhao, Ruining21; Zheng, Shiyu17; Zhou, Xiaolong10; Zhu, Runyu15; Zou, Yu1,2; An, Peng7; Cai, Yifu22; Chen, Hongbing9; Dai, Zigao10; Fan, Yizhong23; Feng, Changqing20; Feng, Hua1,2,24; Gao, He21; Huang, Liang25; Kang, Mingming12; Li, Lixin26; Li, Zhuo26; Liang, Enwei6; Lin, Lin21; Lin, Qianqian27; Liu, Congzhan28; Liu, Hongbang6; Liu, Xuewen12; Liu, Yinong1,2; Lu, Xiang6; Mao, Shude24; Shen, Rongfeng13; Shu, Jing29; Su, Meng30; Sun, Hui31; Tam, Pak-Hin13; Tang, Chi-Pui32; Tian, Yang1,2; Wang, Fayin10; Wang, Jianjun7; Wang, Wei27; Wang, Zhonghai12; Wu, Jianfeng14; Wu, Xuefeng23; Xiong, Shaolin28; Xu, Can25; Yu, Jiandong7; Yu, Wenfei33; Yu, Yunwei34; Zeng, Ming1,2; Zeng, Zhi1,2; Zhang, Bin-Bin10,35; Zhang, Bing36; Zhao, Zongqing3; Zhou, Rong12; Zhu, Zonghong21
2019-08-01
Source PublicationEXPERIMENTAL ASTRONOMY
ISSN0922-6435
Volume48Issue:1Pages:77-95
Corresponding AuthorFeng, Hua(hfeng@tsinghua.edu.cn) ; Zeng, Ming(mingzeng@tsinghua.edu.cn) ; Zhang, Bin-Bin(bbzhang@nju.edu.cn)
AbstractThe 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.
KeywordGamma-ray bursts Gravitational waves Scintillation detector SiPM CubeSat
DOI10.1007/s10686-019-09636-w
WOS KeywordNEUTRON-STAR ; ELECTROMAGNETIC COUNTERPART ; KILONOVA ; BURSTS ; NUCLEOSYNTHESIS ; PERFORMANCE ; EMISSION
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000481758700005
PublisherSPRINGER
Citation statistics
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/28072
Collection中国科学院紫金山天文台
Corresponding AuthorFeng, Hua; Zeng, Ming; Zhang, Bin-Bin
Affiliation1.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
11.Tsinghua Univ, Sch Aerosp Engn, Beijing 100084, Peoples R China
12.Sichuan Univ, Coll Phys Sci & Technol, Chengdu 610065, Sichuan, Peoples R China
13.Sun Yat Sen Univ, Sch Phys & Astron, Zhuhai 519082, Peoples R China
14.Xiamen Univ, Dept Astron, Xiamen 361005, Fujian, Peoples R China
15.Univ Sci & Technol Beijing, Sch Math & Phys, Beijing 100083, Peoples R China
16.Tsinghua Univ, Dept Foreign Languages & Literatures, Beijing 100084, Peoples R China
17.Tsinghua Univ, Dept Elect Engn, Beijing 100084, Peoples R China
18.Tsinghua Univ, Sch Software, Beijing 100084, Peoples R China
19.Ningbo Univ, Fac Elect Engn & Comp Sci, Ningbo 315211, Zhejiang, Peoples R China
20.Univ Sci & Technol China, Sch Phys Sci, Dept Modern Phys, Hefei 230026, Anhui, Peoples R China
21.Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China
22.Univ Sci & Technol China, Sch Phys Sci, Dept Astron, Hefei 230026, Anhui, Peoples R China
23.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China
24.Tsinghua Univ, Dept Astron, Beijing 100084, Peoples R China
25.Lanzhou Univ, Sch Phys Sci & Technol, Lanzhou 730000, Gansu, Peoples R China
26.Peking Univ, Sch Phys, Dept Astron, Kavli Inst Astron & Astrophys, Beijing 100087, Peoples R China
27.Wuhan Univ, Sch Phys & Technol, Wuhan 430072, Hubei, Peoples R China
28.Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China
29.Chinese Acad Sci, Inst Theoret Phys, Beijing 100190, Peoples R China
30.Univ Hong Kong, Dept Phys, Hong Kong, Peoples R China
31.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
32.Macau Univ Sci & Technol, State Key Lab Lunar & Planetary Sci, Macau, Peoples R China
33.Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China
34.Cent China Normal Univ, Inst Astrophys, Wuhan 430079, Hubei, Peoples R China
35.Nanjing Univ, Minist Educ, Key Lab Modern Astron & Astrophys, Nanjing, Jiangsu, Peoples R China
36.Univ Nevada, Dept Phys & Astron, Las Vegas, NV 89154 USA
Recommended Citation
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.
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