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Optical observations of LIGO source GW 170817 by the Antarctic Survey Telescopes at Dome A, Antarctica
Hu, Lei1,2,3; Wu, Xuefeng1,2,3; Andreoni, Igor4,5,6; Ashley, Michael C. B.7; Cooke, Jeff4,5,8; Cui, Xiangqun2,9; Du, Fujia9; Dai, Zigao10,11; Gu, Bozhong9; Hu, Yi2,12; Lu, Haiping9; Li, Xiaoyan9; Li, Zhengyang9; Liang, Ensi10,11; Liu, Liangduan10,11; Ma, Bin2,12; Shang, Zhaohui2,12,13; Sun, Tianrui1,2,14; Suntzeff, N. B.15; Tao, Charling16,17,18; Uddin, Syed A.1,2,8; Wang, Lifan1,2,15; Wang, Xiaofeng17,18; Wen, Haikun9; Xiao, Di10,11; Xu, Jin9; Yang, Ji1; Yang, Shihai9; Yuan, Xiangyan2,9; Zhou, Hongyan19; Zhang, Hui10,11; Zhou, Jilin10,11; Zhu, Zonghong20,21
2017-11-15
Source PublicationSCIENCE BULLETIN
Volume62Issue:21Pages:1433-1438
AbstractThe LIGO detection of gravitational waves (GW) from merging black holes in 2015 marked the beginning of a new era in observational astronomy. The detection of an electromagnetic signal from a GW source is the critical next step to explore in detail the physics involved. The Antarctic Survey Telescopes (AST3), located at Dome A, Antarctica, is uniquely situated for rapid response time-domain astronomy with its continuous night-time coverage during the austral winter. We report optical observations of the GW source (GW 170817) in the nearby galaxy NGC 4993 using AST3. The data show a rapidly fading transient at around 1 day after the GW trigger, with the i-band magnitude declining from 17.23 +/- 0.13 magnitude to 17.72 +/- 0.09 magnitude in similar to 1.8 h. The brightness and time evolution of the optical transient associated with GW 170817 are broadly consistent with the predictions of models involving merging binary neutron stars. We infer from our data that the merging process ejected about similar to 10(-2) solar mass of radioactive material at a speed of up to 30% the speed of light. (C) 2017 Science China Press. Published by Elsevier B.V. and Science China Press. All rights reserved.
SubtypeArticle
KeywordGravitational Waves Binary Neutron Stars Gamma-ray Bursts
WOS HeadingsScience & Technology
Funding OrganizationNational Basic Research Program (973 Program) of China(2013CB834900) ; National Basic Research Program (973 Program) of China(2013CB834900) ; Chinese Polar Environment Comprehensive Investigation & Assessment Program(CHINARE2016-02-03) ; Chinese Polar Environment Comprehensive Investigation & Assessment Program(CHINARE2016-02-03) ; National Natural Science Foundation of China(11573014 ; National Natural Science Foundation of China(11573014 ; Key Research Program of Frontier Sciences(QYZDY-SSW-SLH010 ; Key Research Program of Frontier Sciences(QYZDY-SSW-SLH010 ; Strategic Priority Research Program "multi-waveband gravitational wave Universe"(XDB23040000) ; Strategic Priority Research Program "multi-waveband gravitational wave Universe"(XDB23040000) ; Youth Innovation Promotion Association of Chinese Academy of Sciences(2011231) ; Youth Innovation Promotion Association of Chinese Academy of Sciences(2011231) ; Tsinghua University ; Tsinghua University ; Nanjing University ; Nanjing University ; Beijing Normal University ; Beijing Normal University ; University of New South Wales ; University of New South Wales ; Texas AM University ; Texas AM University ; Australian Antarctic Division ; Australian Antarctic Division ; National Collaborative Research Infrastructure Strategy (NCRIS) of Australia ; National Collaborative Research Infrastructure Strategy (NCRIS) of Australia ; Chinese Academy of Sciences through the Center for Astronomical Mega-Science ; Chinese Academy of Sciences through the Center for Astronomical Mega-Science ; National Astronomical Observatory of China (NAOC) ; National Astronomical Observatory of China (NAOC) ; Robert Martin Ayers Sciences Fund ; Robert Martin Ayers Sciences Fund ; Australian Research Council (ARC) Centre of Excellence for Gravitational Wave Discovery (OzGrav)(CE170100004) ; Australian Research Council (ARC) Centre of Excellence for Gravitational Wave Discovery (OzGrav)(CE170100004) ; ARC Centre of Excellence for All-sky Astrophysics (CAASTRO)(CE110001020) ; ARC Centre of Excellence for All-sky Astrophysics (CAASTRO)(CE110001020) ; Centre of Excellence for All-sky Astrophysics in 3-Dimensions (ASTRO-3D)(CE170100013) ; Centre of Excellence for All-sky Astrophysics in 3-Dimensions (ASTRO-3D)(CE170100013) ; Australian Astronomical Observatory (AAO) ; Australian Astronomical Observatory (AAO) ; ARC(FT130101219) ; ARC(FT130101219) ; National Basic Research Program (Project 973) of China(2014CB845800) ; National Basic Research Program (Project 973) of China(2014CB845800) ; Strategic Priority Research Program of the Chinese Academy of Sciences(XDB23000000) ; Strategic Priority Research Program of the Chinese Academy of Sciences(XDB23000000) ; 11673068 ; 11673068 ; QYZDB-SSW-SYS005) ; QYZDB-SSW-SYS005) ; 11325313 ; 11325313 ; 11633002 ; 11633002 ; 11433009 ; 11433009 ; 11725314 ; 11725314 ; 11633001 ; 11633001 ; 11373014) ; 11373014) ; National Basic Research Program (973 Program) of China(2013CB834900) ; National Basic Research Program (973 Program) of China(2013CB834900) ; Chinese Polar Environment Comprehensive Investigation & Assessment Program(CHINARE2016-02-03) ; Chinese Polar Environment Comprehensive Investigation & Assessment Program(CHINARE2016-02-03) ; National Natural Science Foundation of China(11573014 ; National Natural Science Foundation of China(11573014 ; Key Research Program of Frontier Sciences(QYZDY-SSW-SLH010 ; Key Research Program of Frontier Sciences(QYZDY-SSW-SLH010 ; Strategic Priority Research Program "multi-waveband gravitational wave Universe"(XDB23040000) ; Strategic Priority Research Program "multi-waveband gravitational wave Universe"(XDB23040000) ; Youth Innovation Promotion Association of Chinese Academy of Sciences(2011231) ; Youth Innovation Promotion Association of Chinese Academy of Sciences(2011231) ; Tsinghua University ; Tsinghua University ; Nanjing University ; Nanjing University ; Beijing Normal University ; Beijing Normal University ; University of New South Wales ; University of New South Wales ; Texas AM University ; Texas AM University ; Australian Antarctic Division ; Australian Antarctic Division ; National Collaborative Research Infrastructure Strategy (NCRIS) of Australia ; National Collaborative Research Infrastructure Strategy (NCRIS) of Australia ; Chinese Academy of Sciences through the Center for Astronomical Mega-Science ; Chinese Academy of Sciences through the Center for Astronomical Mega-Science ; National Astronomical Observatory of China (NAOC) ; National Astronomical Observatory of China (NAOC) ; Robert Martin Ayers Sciences Fund ; Robert Martin Ayers Sciences Fund ; Australian Research Council (ARC) Centre of Excellence for Gravitational Wave Discovery (OzGrav)(CE170100004) ; Australian Research Council (ARC) Centre of Excellence for Gravitational Wave Discovery (OzGrav)(CE170100004) ; ARC Centre of Excellence for All-sky Astrophysics (CAASTRO)(CE110001020) ; ARC Centre of Excellence for All-sky Astrophysics (CAASTRO)(CE110001020) ; Centre of Excellence for All-sky Astrophysics in 3-Dimensions (ASTRO-3D)(CE170100013) ; Centre of Excellence for All-sky Astrophysics in 3-Dimensions (ASTRO-3D)(CE170100013) ; Australian Astronomical Observatory (AAO) ; Australian Astronomical Observatory (AAO) ; ARC(FT130101219) ; ARC(FT130101219) ; National Basic Research Program (Project 973) of China(2014CB845800) ; National Basic Research Program (Project 973) of China(2014CB845800) ; Strategic Priority Research Program of the Chinese Academy of Sciences(XDB23000000) ; Strategic Priority Research Program of the Chinese Academy of Sciences(XDB23000000) ; 11673068 ; 11673068 ; QYZDB-SSW-SYS005) ; QYZDB-SSW-SYS005) ; 11325313 ; 11325313 ; 11633002 ; 11633002 ; 11433009 ; 11433009 ; 11725314 ; 11725314 ; 11633001 ; 11633001 ; 11373014) ; 11373014)
DOI10.1016/j.scib.2017.10.006
WOS KeywordCOMPACT OBJECT MERGERS ; SITE
Indexed BySCI
Language英语
Funding OrganizationNational Basic Research Program (973 Program) of China(2013CB834900) ; National Basic Research Program (973 Program) of China(2013CB834900) ; Chinese Polar Environment Comprehensive Investigation & Assessment Program(CHINARE2016-02-03) ; Chinese Polar Environment Comprehensive Investigation & Assessment Program(CHINARE2016-02-03) ; National Natural Science Foundation of China(11573014 ; National Natural Science Foundation of China(11573014 ; Key Research Program of Frontier Sciences(QYZDY-SSW-SLH010 ; Key Research Program of Frontier Sciences(QYZDY-SSW-SLH010 ; Strategic Priority Research Program "multi-waveband gravitational wave Universe"(XDB23040000) ; Strategic Priority Research Program "multi-waveband gravitational wave Universe"(XDB23040000) ; Youth Innovation Promotion Association of Chinese Academy of Sciences(2011231) ; Youth Innovation Promotion Association of Chinese Academy of Sciences(2011231) ; Tsinghua University ; Tsinghua University ; Nanjing University ; Nanjing University ; Beijing Normal University ; Beijing Normal University ; University of New South Wales ; University of New South Wales ; Texas AM University ; Texas AM University ; Australian Antarctic Division ; Australian Antarctic Division ; National Collaborative Research Infrastructure Strategy (NCRIS) of Australia ; National Collaborative Research Infrastructure Strategy (NCRIS) of Australia ; Chinese Academy of Sciences through the Center for Astronomical Mega-Science ; Chinese Academy of Sciences through the Center for Astronomical Mega-Science ; National Astronomical Observatory of China (NAOC) ; National Astronomical Observatory of China (NAOC) ; Robert Martin Ayers Sciences Fund ; Robert Martin Ayers Sciences Fund ; Australian Research Council (ARC) Centre of Excellence for Gravitational Wave Discovery (OzGrav)(CE170100004) ; Australian Research Council (ARC) Centre of Excellence for Gravitational Wave Discovery (OzGrav)(CE170100004) ; ARC Centre of Excellence for All-sky Astrophysics (CAASTRO)(CE110001020) ; ARC Centre of Excellence for All-sky Astrophysics (CAASTRO)(CE110001020) ; Centre of Excellence for All-sky Astrophysics in 3-Dimensions (ASTRO-3D)(CE170100013) ; Centre of Excellence for All-sky Astrophysics in 3-Dimensions (ASTRO-3D)(CE170100013) ; Australian Astronomical Observatory (AAO) ; Australian Astronomical Observatory (AAO) ; ARC(FT130101219) ; ARC(FT130101219) ; National Basic Research Program (Project 973) of China(2014CB845800) ; National Basic Research Program (Project 973) of China(2014CB845800) ; Strategic Priority Research Program of the Chinese Academy of Sciences(XDB23000000) ; Strategic Priority Research Program of the Chinese Academy of Sciences(XDB23000000) ; 11673068 ; 11673068 ; QYZDB-SSW-SYS005) ; QYZDB-SSW-SYS005) ; 11325313 ; 11325313 ; 11633002 ; 11633002 ; 11433009 ; 11433009 ; 11725314 ; 11725314 ; 11633001 ; 11633001 ; 11373014) ; 11373014) ; National Basic Research Program (973 Program) of China(2013CB834900) ; National Basic Research Program (973 Program) of China(2013CB834900) ; Chinese Polar Environment Comprehensive Investigation & Assessment Program(CHINARE2016-02-03) ; Chinese Polar Environment Comprehensive Investigation & Assessment Program(CHINARE2016-02-03) ; National Natural Science Foundation of China(11573014 ; National Natural Science Foundation of China(11573014 ; Key Research Program of Frontier Sciences(QYZDY-SSW-SLH010 ; Key Research Program of Frontier Sciences(QYZDY-SSW-SLH010 ; Strategic Priority Research Program "multi-waveband gravitational wave Universe"(XDB23040000) ; Strategic Priority Research Program "multi-waveband gravitational wave Universe"(XDB23040000) ; Youth Innovation Promotion Association of Chinese Academy of Sciences(2011231) ; Youth Innovation Promotion Association of Chinese Academy of Sciences(2011231) ; Tsinghua University ; Tsinghua University ; Nanjing University ; Nanjing University ; Beijing Normal University ; Beijing Normal University ; University of New South Wales ; University of New South Wales ; Texas AM University ; Texas AM University ; Australian Antarctic Division ; Australian Antarctic Division ; National Collaborative Research Infrastructure Strategy (NCRIS) of Australia ; National Collaborative Research Infrastructure Strategy (NCRIS) of Australia ; Chinese Academy of Sciences through the Center for Astronomical Mega-Science ; Chinese Academy of Sciences through the Center for Astronomical Mega-Science ; National Astronomical Observatory of China (NAOC) ; National Astronomical Observatory of China (NAOC) ; Robert Martin Ayers Sciences Fund ; Robert Martin Ayers Sciences Fund ; Australian Research Council (ARC) Centre of Excellence for Gravitational Wave Discovery (OzGrav)(CE170100004) ; Australian Research Council (ARC) Centre of Excellence for Gravitational Wave Discovery (OzGrav)(CE170100004) ; ARC Centre of Excellence for All-sky Astrophysics (CAASTRO)(CE110001020) ; ARC Centre of Excellence for All-sky Astrophysics (CAASTRO)(CE110001020) ; Centre of Excellence for All-sky Astrophysics in 3-Dimensions (ASTRO-3D)(CE170100013) ; Centre of Excellence for All-sky Astrophysics in 3-Dimensions (ASTRO-3D)(CE170100013) ; Australian Astronomical Observatory (AAO) ; Australian Astronomical Observatory (AAO) ; ARC(FT130101219) ; ARC(FT130101219) ; National Basic Research Program (Project 973) of China(2014CB845800) ; National Basic Research Program (Project 973) of China(2014CB845800) ; Strategic Priority Research Program of the Chinese Academy of Sciences(XDB23000000) ; Strategic Priority Research Program of the Chinese Academy of Sciences(XDB23000000) ; 11673068 ; 11673068 ; QYZDB-SSW-SYS005) ; QYZDB-SSW-SYS005) ; 11325313 ; 11325313 ; 11633002 ; 11633002 ; 11433009 ; 11433009 ; 11725314 ; 11725314 ; 11633001 ; 11633001 ; 11373014) ; 11373014)
WOS Research AreaScience & Technology - Other Topics
WOS SubjectMultidisciplinary Sciences
WOS IDWOS:000416211200004
Citation statistics
Cited Times:21[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/20286
Collection星系宇宙学研究部
Affiliation1.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China
2.Chinese Ctr Antarctic Astron, Nanjing 210008, Jiangsu, Peoples R China
3.Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230029, Anhui, Peoples R China
4.Swinburne Univ Technol, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia
5.Australian Res Council, Ctr Excellence Gravitat Wave Discovery OzGrav, Canberra, ACT, Australia
6.Australian Astron Observ, N Ryde, NSW 2113, Australia
7.Univ New South Wales, Sch Phys, Sydney, NSW 2052, Australia
8.Australian Res Council, Ctr Excellence All Sky Astrophys CAASTRO, Canberra, ACT, Australia
9.Nanjing Inst Astron Opt & Technol, Nanjing 210042, Jiangsu, Peoples R China
10.Nanjing Univ, Minist Educ, Sch Astron & Space Sci, Nanjing 210093, Jiangsu, Peoples R China
11.Nanjing Univ, Key Lab Modern Astron & Astrophys, Sch Astron & Space Sci, Nanjing 210093, Jiangsu, Peoples R China
12.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
13.Tianjin Normal Univ, Dept Phys, Tianjin 300074, Peoples R China
14.Shanghai Normal Univ, Shanghai Key Lab Astrophys, Shanghai 200234, Peoples R China
15.Texas A&M Univ, George P & Cynthia Woods Mitchell Inst Fundamenta, Dept Phys & Astron, 4242 TAMU, College Stn, TX 77843 USA
16.Aix Marseille Univ, CNRS, IN2P3, CPPM, Marseille, France
17.Tsinghua Univ, Phys Dept, Beijing 100084, Peoples R China
18.Tsinghua Univ, Tsinghua Ctr Astrophys THCA, Beijing 100084, Peoples R China
19.Polar Res Inst China, Shanghai 200136, Peoples R China
20.Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China
21.Wuhan Univ, Sch Phys & Technol, Wuhan 430072, Hubei, Peoples R China
Recommended Citation
GB/T 7714
Hu, Lei,Wu, Xuefeng,Andreoni, Igor,et al. Optical observations of LIGO source GW 170817 by the Antarctic Survey Telescopes at Dome A, Antarctica[J]. SCIENCE BULLETIN,2017,62(21):1433-1438.
APA Hu, Lei.,Wu, Xuefeng.,Andreoni, Igor.,Ashley, Michael C. B..,Cooke, Jeff.,...&Zhu, Zonghong.(2017).Optical observations of LIGO source GW 170817 by the Antarctic Survey Telescopes at Dome A, Antarctica.SCIENCE BULLETIN,62(21),1433-1438.
MLA Hu, Lei,et al."Optical observations of LIGO source GW 170817 by the Antarctic Survey Telescopes at Dome A, Antarctica".SCIENCE BULLETIN 62.21(2017):1433-1438.
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