Insight-hxmt observations of the first binary neutron star merger gw170817
文献类型：期刊论文
| 作者 | Li, Tipei1,2,3; Xiong, ShaoLin1; Zhang, ShuangNan1,3; Lu, FangJun1; Song, LiMing1; Cao, XueLei1; Chang, Zhi1; Chen, Gang1; Chen, Li4; Chen, TianXiang1 |
| 刊名 | Science china-physics mechanics & astronomy
 |
| 出版日期 | 2018-03-01 |
| 卷号 | 61期号:3页码:8 |
| 关键词 | Gw170817 Bns merger Gravitational wave electromagnetic counterpart |
| ISSN号 | 1674-7348 |
| DOI | 10.1007/s11433-017-9107-5 |
| 通讯作者 | Zhang, shuangnan(zhangsn@ihep.ac.cn) |
| 英文摘要 | Finding the electromagnetic (em) counterpart of binary compact star merger, especially the binary neutron star (bns) merger, is critically important for gravitational wave (gw) astronomy, cosmology and fundamental physics. on aug. 17, 2017, advanced ligo and fermi/gbm independently triggered the first bns merger, gw170817, and its high energy em counterpart, grb 170817a, respectively, resulting in a global observation campaign covering gamma-ray, x-ray, uv, optical, ir, radio as well as neutrinos. the high energy x-ray telescope (he) onboard insight-hxmt (hard x-ray modulation telescope) is the unique high-energy gamma-ray telescope that monitored the entire gw localization area and especially the optical counterpart (sss17a/at2017gfo) with very large collection area (similar to 1000 cm(2)) and microsecond time resolution in 0.2-5 mev. in addition, insight-hxmt quickly implemented a target of opportunity (too) observation to scan the gw localization area for potential x-ray emission from the gw source. although insight-hxmt did not detect any significant high energy (0.2-5 mev) radiation from gw170817, its observation helped to confirm the unexpected weak and soft nature of grb 170817a. meanwhile, insight-hxmt/he provides one of the most stringent constraints (similar to 10(-7) to 10(-6) erg/cm(2)/s) for both grb170817a and any other possible precursor or extended emissions in 0.2-5 mev, which help us to better understand the properties of em radiation from this bns merger. therefore the observation of insight-hxmt constitutes an important chapter in the full context of multi-wavelength and multi-messenger observation of this historical gw event. |
| WOS关键词 | GAMMA-RAY BURSTS |
| WOS研究方向 | Physics |
| WOS类目 | Physics, Multidisciplinary |
| 语种 | 英语 |
| WOS记录号 | WOS:000423576900004 |
| 出版者 | SCIENCE PRESS |
| URI标识 | http://www.irgrid.ac.cn/handle/1471x/2177941 |
| 专题 | 高能物理研究所 |
| 通讯作者 | Zhang, ShuangNan |
| 作者单位 | 1.Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China 2.Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China 3.Chinese Acad Sci, Univ Chinese Acad Sci, Beijing 100049, Peoples R China 4.Beijing Normal Univ, Dept Astron, Beijing 100088, Peoples R China 5.Tsinghua Univ, Dept Engn Phys, Beijing 100084, Peoples R China |
| 推荐引用方式 GB/T 7714 | Li, Tipei,Xiong, ShaoLin,Zhang, ShuangNan,et al. Insight-hxmt observations of the first binary neutron star merger gw170817[J]. Science china-physics mechanics & astronomy,2018,61(3):8. |
| APA | Li, Tipei.,Xiong, ShaoLin.,Zhang, ShuangNan.,Lu, FangJun.,Song, LiMing.,...&Zou, ChangLin.(2018).Insight-hxmt observations of the first binary neutron star merger gw170817.Science china-physics mechanics & astronomy,61(3),8. |
| MLA | Li, Tipei,et al."Insight-hxmt observations of the first binary neutron star merger gw170817".Science china-physics mechanics & astronomy 61.3(2018):8. |
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来源：高能物理研究所
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