Multi-messenger observations of a binary neutron star merger

LIGO Scientific Collaboration and Virgo Collaboration; Fermi GBM; INTEGRAL; Icecube Collaboration; AstroSat Cadmium Zinc Telluride Imager Team; IPN Collaboration; The Insight-HXMT Collaboration; ANTARES Collaboration; The Swift Collaboration; AGILE Team; The 1M2H Team; The Dark Energy Camera GW-EM Collaboration and the DES Collaboration; DLT40 Collaboration; GRAWITA: GRAvitational Wave Inaf TeAm; The Fermi Large Area Telescope Collaboration; ATCA: Australia Telescope Compact Array; ASKAP: Australian SKA Pathfinder; Las Cumbres Observatory Collaboration; OzGrav, DWF (Deeper, Wider, Faster program), AST3, and CAASTRO Collaborations; The VINROUGE Collaboration; MASTER Collaboration; J-GEM; GROWTH, JAGWAR, Caltech-NRAO, TTU-NRAO, and NuSTAR Collaborations; Pan-STARRS; The MAXI Team; TZAC Consortium; KU Collaboration; Nordic Optical Telescope; ePESSTO; GROND; Texas Tech University; SALT Group; TOROS: Transient Robotic Observatory of the South Collaboration; The BOOTES Collaboration; MWA: Murchison Widefield Array; The CALET Collaboration; IKI-GW Follow-up Collaboration; H.E.S.S. Collaboration; LOFAR Collaboration; LWA: Long Wavelength Array; HAWC Collaboration; The Pierre Auger Collaboration; ALMA Collaboration; Euro VLBI Team; Pi of the Sky Collaboration; The Chandra Team at McGill University; DFN: Desert Fireball Network; ATLAS; High Time Resolution Universe Survey; RIMAS and RATIR; SKA South Africa/MeerKAT

doi:10.3847/2041-8213/aa91c9

Multi-messenger observations of a binary neutron star merger

LIGO Scientific Collaboration and Virgo Collaboration
, Fermi GBM
, INTEGRAL
, Icecube Collaboration
, AstroSat Cadmium Zinc Telluride Imager Team
, IPN Collaboration
, The Insight-HXMT Collaboration
, ANTARES Collaboration
, The Swift Collaboration
, AGILE Team
, The 1M2H Team
, The Dark Energy Camera GW-EM Collaboration and the DES Collaboration
, DLT40 Collaboration
, GRAWITA: GRAvitational Wave Inaf TeAm
, The Fermi Large Area Telescope Collaboration
, ATCA: Australia Telescope Compact Array
, ASKAP: Australian SKA Pathfinder
, Las Cumbres Observatory Collaboration
, OzGrav, DWF (Deeper, Wider, Faster program), AST3, and CAASTRO Collaborations
, The VINROUGE Collaboration

MASTER Collaboration, J-GEM, GROWTH, JAGWAR, Caltech-NRAO, TTU-NRAO, and NuSTAR Collaborations, Pan-STARRS, The MAXI Team, TZAC Consortium, KU Collaboration, Nordic Optical Telescope, ePESSTO, GROND, Texas Tech University, SALT Group, TOROS: Transient Robotic Observatory of the South Collaboration, The BOOTES Collaboration, MWA: Murchison Widefield Array, The CALET Collaboration, IKI-GW Follow-up Collaboration, H.E.S.S. Collaboration, LOFAR Collaboration, LWA: Long Wavelength Array, HAWC Collaboration, The Pierre Auger Collaboration, ALMA Collaboration, Euro VLBI Team, Pi of the Sky Collaboration, The Chandra Team at McGill University, DFN: Desert Fireball Network, ATLAS, High Time Resolution Universe Survey, RIMAS and RATIR, SKA South Africa/MeerKAT

California Institute of Technology
Louisiana State University
Salerno
Complesso Universitario di Monte S.Angelo
University of Florida
Monash University
LIGO Livingston Observatory
IN2P3 Institut National de Physique Nucleaire et de Physique des Particules
University of Sannio at Benevento
Complesso Universitario di Monte Sant'Angelo
Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
University of Mississippi
University of Illinois
University of Cambridge
Science Park
LIGO, Massachusetts Institute of Technology
Instituto Nacional de Pesquisas Espaciais
Gran
Laboratori Nazionali del Gran Sasso
The Inter-University Centre for Astronomy and Astrophysics
Tata Institute of Fundamental Research
University of Wisconsin-Milwaukee
Leibniz Universität Hannover
Università di Pisa
INFN
Australian National University
University of the West of Scotland
Université Paris-Saclay
California State University
European Gravitational Observatory (EGO)
Chennai Mathematical Institute
Università di Roma Tor Vergata
Gran Sasso Science Institute
Universität Hamburg
Cardiff University
Embry-Riddle Aeronautical University
APC - AstroParticule et Cosmologie
Korea Institute of Science and Technology Information
West Virginia University
Università di Perugia
INFN
Syracuse University
University of Minnesota Twin Cities
University of Glasgow
LIGO Hanford Observatory
Institute for Particle and Nuclear Physics
NASA/Goddard Space Flight Center
Columbia University in the City of New York
Stanford University
Dipartimento di Fisica
University of Padua
Lendulet Astrophysics Research Group
Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences
Rochester Institute of Technology
University of Birmingham
RRCAT
Lomonosov Moscow State University
University of Strathclyde
Pennsylvania State University
University of Western Australia
Radboud University Nijmegen
Observatoire de la Côte d'Azur
UMR6082
Washington State University
University of Oregon
Laboratoire Kastler Brossel
Carleton College, USA
University of Adelaide
Astronomical Observatory Warsaw University
Vrije University Amsterdam
University of Maryland
Georgia Institute of Technology
Université Claude Bernard Lyon 1
Università degli Studi di Genova
University of Tokyo
Tsinghua University
Texas Tech University at Lubbock
Kenyon College
University of Valencia
Centro Studi e Ricerche Enrico Fermi
National Tsing Hua University
Northwestern University
Canadian Institute for Theoretical Astrophysics
University of Chicago
Pusan National University
Chinese University of Hong Kong
Osservatorio Astronomico di Padova
Trento Institute for Fundamental Physics and Applications
University of Melbourne
Università di Roma la Sapienza
Université Libre de Bruxelles
Sonoma State University
Montana State University
Universitat de les Illes Balears
University of Texas Rio Grande Valley
Bellevue College
Institute for Plasma Research India

Research output: Contribution to journal › Article › peer-review

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174 Downloads (Pure)

Abstract

On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of ~1.7 s with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg² at a luminosity distance of 40± ₈ ⁸ Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 M_☉. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at ~40 Mpc) less than 11 hours after the merger by the One-Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ∼10 days. Following early non-detections, X-ray and radio emission were discovered at the transient's position ~9 and ~16 days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC 4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta.

Original language	English
Article number	L12
Number of pages	59
Journal	Astrophysical Journal Letters
Volume	848
Issue number	2
DOIs	https://doi.org/10.3847/2041-8213/aa91c9
Publication status	Published - 01 Jan 2017

Access to Document

10.3847/2041-8213/aa91c9

103923925 Published articleFinal published version, 2.04 MBLicence: CC BY

Cite this

LIGO Scientific Collaboration and Virgo Collaboration, Fermi GBM, INTEGRAL, Icecube Collaboration, AstroSat Cadmium Zinc Telluride Imager Team, IPN Collaboration, The Insight-HXMT Collaboration, ANTARES Collaboration, The Swift Collaboration, AGILE Team, The 1M2H Team, The Dark Energy Camera GW-EM Collaboration and the DES Collaboration, DLT40 Collaboration, GRAWITA: GRAvitational Wave Inaf TeAm, The Fermi Large Area Telescope Collaboration, ATCA: Australia Telescope Compact Array, ASKAP: Australian SKA Pathfinder, Las Cumbres Observatory Collaboration, OzGrav, DWF (Deeper, Wider, Faster program), AST3, and CAASTRO Collaborations, ... SKA South Africa/MeerKAT (2017). Multi-messenger observations of a binary neutron star merger. Astrophysical Journal Letters, 848(2), Article L12. https://doi.org/10.3847/2041-8213/aa91c9

@article{e19a8ecdc0894b24b67edef6a3b048a7,

title = "Multi-messenger observations of a binary neutron star merger",

abstract = "On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of \textasciitilde{}1.7 s with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg2 at a luminosity distance of 40± 8 8 Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 M☉. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at \textasciitilde{}40 Mpc) less than 11 hours after the merger by the One-Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ∼10 days. Following early non-detections, X-ray and radio emission were discovered at the transient's position \textasciitilde{}9 and \textasciitilde{}16 days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC 4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta.",

keywords = "Gravitational waves, Stars: neutron",

author = "\{LIGO Scientific Collaboration and Virgo Collaboration\} and \{Fermi GBM\} and INTEGRAL and \{Icecube Collaboration\} and \{AstroSat Cadmium Zinc Telluride Imager Team\} and \{IPN Collaboration\} and \{The Insight-HXMT Collaboration\} and \{ANTARES Collaboration\} and \{The Swift Collaboration\} and \{AGILE Team\} and \{The 1M2H Team\} and \{The Dark Energy Camera GW-EM Collaboration and the DES Collaboration\} and \{DLT40 Collaboration\} and \{GRAWITA: GRAvitational Wave Inaf TeAm\} and \{The Fermi Large Area Telescope Collaboration\} and \{ATCA: Australia Telescope Compact Array\} and \{ASKAP: Australian SKA Pathfinder\} and \{Las Cumbres Observatory Collaboration\} and \{OzGrav, DWF (Deeper, Wider, Faster program), AST3, and CAASTRO Collaborations\} and \{The VINROUGE Collaboration\} and \{MASTER Collaboration\} and J-GEM and \{GROWTH, JAGWAR, Caltech-NRAO, TTU-NRAO, and NuSTAR Collaborations\} and Pan-STARRS and \{The MAXI Team\} and \{TZAC Consortium\} and \{KU Collaboration\} and \{Nordic Optical Telescope\} and ePESSTO and GROND and \{Texas Tech University\} and \{SALT Group\} and \{TOROS: Transient Robotic Observatory of the South Collaboration\} and \{The BOOTES Collaboration\} and \{MWA: Murchison Widefield Array\} and \{The CALET Collaboration\} and \{IKI-GW Follow-up Collaboration\} and \{H.E.S.S. Collaboration\} and \{LOFAR Collaboration\} and \{LWA: Long Wavelength Array\} and \{HAWC Collaboration\} and \{The Pierre Auger Collaboration\} and \{ALMA Collaboration\} and \{Euro VLBI Team\} and \{Pi of the Sky Collaboration\} and \{The Chandra Team at McGill University\} and \{DFN: Desert Fireball Network\} and ATLAS and \{High Time Resolution Universe Survey\} and \{RIMAS and RATIR\} and \{SKA South Africa/MeerKAT\} and Abbott, \{B. P.\} and R. Abbott and Abbott, \{T. D.\} and F. Acernese and K. Ackley and C. Adams and T. Adams and P. Addesso and Adhikari, \{R. X.\} and Adya, \{V. B.\} and C. Affeldt and M. Afrough and B. Agarwal and M. Agathos and K. Agatsuma and N. Aggarwal and Aguiar, \{O. D.\} and L. Aiello and A. Ain and P. Ajith and B. Allen and G. Allen and A. Allocca and Altin, \{P. A.\} and A. Amato and A. Ananyeva and Anderson, \{S. B.\} and Anderson, \{W. G.\} and Angelova, \{S. V.\} and S. Antier and S. Appert and K. Arai and Araya, \{M. C.\} and Areeda, \{J. S.\} and N. Arnaud and Arun, \{K. G.\} and S. Ascenzi and G. Ashton and M. Ast and Aston, \{S. M.\} and P. Astone and Atallah, \{D. V.\} and P. Aufmuth and C. Aulbert and K. AultONeal and C. Austin and A. Avila-Alvarez and S. Babak and P. Bacon and Bader, \{M. K.M.\} and S. Bae and Baker, \{P. T.\} and F. Baldaccini and G. Ballardin and Ballmer, \{S. W.\} and S. Banagiri and Barayoga, \{J. C.\} and Barclay, \{S. E.\} and Barish, \{B. C.\} and D. Barker and K. Barkett and F. Barone and B. Barr and L. Barsotti and M. Barsuglia and D. Barta and Barthelmy, \{S. D.\} and J. Bartlett and I. Bartos and R. Bassiri and A. Basti and Batch, \{J. C.\} and M. Bawaj and Bayley, \{J. C.\} and M. Bazzan and B. B{\'e}csy and C. Beer and M. Bejger and I. Belahcene and Bell, \{A. S.\} and Berger, \{B. K.\} and G. Bergmann and Bero, \{J. J.\} and Berry, \{C. P.L.\} and D. Bersanetti and A. Bertolini and J. Betzwieser and S. Bhagwat and R. Bhandare and Bilenko, \{I. A.\} and G. Billingsley and Billman, \{C. R.\} and J. Birch and R. Birney and O. Birnholtz and S. Biscans and S. Biscoveanu and A. Bisht and M. Bitossi and C. Biwer and Bizouard, \{M. A.\} and Blackburn, \{J. K.\} and J. Blackman and Blair, \{C. D.\} and Blair, \{D. G.\} and Blair, \{R. M.\} and S. Bloemen and O. Bock and N. Bode and M. Boer and G. Bogaert and A. Bohe and F. Bondu and E. Bonilla and R. Bonnand and Boom, \{B. A.\} and R. Bork and V. Boschi and S. Bose and K. Bossie and Y. Bouffanais and A. Bozzi and C. Bradaschia and Brady, \{P. R.\} and M. Branchesi and Brau, \{J. E.\} and T. Briant and A. Brillet and M. Brinkmann and V. Brisson and P. Brockill and Broida, \{J. E.\} and Brooks, \{A. F.\} and Brown, \{D. A.\} and Brown, \{D. D.\} and S. Brunett and Buchanan, \{C. C.\} and A. Buikema and T. Bulik and Bulten, \{H. J.\} and A. Buonanno and D. Buskulic and C. Buy and Byer, \{R. L.\} and M. Cabero and L. Cadonati and G. Cagnoli and C. Cahillane and \{Calder{\'o}n Bustillo\}, J. and Callister, \{T. A.\} and E. Calloni and Camp, \{J. B.\} and M. Canepa and P. Canizares and Cannon, \{K. C.\} and H. Cao and J. Cao and Capano, \{C. D.\} and E. Capocasa and F. Carbognani and S. Caride and Carney, \{M. F.\} and \{Casanueva Diaz\}, J. and C. Casentini and S. Caudill and M. Cavagli{\`a} and F. Cavalier and R. Cavalieri and G. Cella and Cepeda, \{C. B.\} and P. Cerd{\'a}-Dur{\'a}n and G. Cerretani and E. Cesarini and Chamberlin, \{S. J.\} and M. Chan and S. Chao and P. Charlton and E. Chase and E. Chassande-Mottin and D. Chatterjee and K. Chatziioannou and Cheeseboro, \{B. D.\} and Chen, \{H. Y.\} and X. Chen and Y. Chen and Cheng, \{H. P.\} and H. Chia and A. Chincarini and A. Chiummo and T. Chmiel and Cho, \{H. S.\} and M. Cho and Chow, \{J. H.\} and N. Christensen and Q. Chu and Chua, \{A. J.K.\} and S. Chua and Chung, \{A. K.W.\} and S. Chung and G. Ciani and R. Ciolfi and Cirelli, \{C. E.\} and A. Cirone and F. Clara and Clark, \{J. A.\} and P. Clearwater and F. Cleva and C. Cocchieri and E. Coccia and Cohadon, \{P. F.\} and D. Cohen and A. Colla and Collette, \{C. G.\} and Cominsky, \{L. R.\} and M. Constancio and L. Conti and Cooper, \{S. J.\} and P. Corban and Corbitt, \{T. R.\} and I. Cordero-Carri{\'o}n and Corley, \{K. R.\} and N. Cornish and A. Corsi and S. Cortese and Costa, \{C. A.\} and Coughlin, \{M. W.\} and Coughlin, \{S. B.\} and Coulon, \{J. P.\} and Countryman, \{S. T.\} and P. Couvares and Covas, \{P. B.\} and Cowan, \{E. E.\} and Coward, \{D. M.\} and Cowart, \{M. J.\} and Coyne, \{D. C.\} and R. Coyne and Creighton, \{J. D.E.\} and Creighton, \{T. D.\} and J. Cripe and Crowder, \{S. G.\} and Cullen, \{T. J.\} and A. Cumming and L. Cunningham and E. Cuoco and \{Dal Canton\}, T. and G. D{\'a}lya and Danilishin, \{S. L.\} and S. D'Antonio and K. Danzmann and A. Dasgupta",

note = "Includes bibliographical references.",

year = "2017",

month = jan,

day = "1",

doi = "10.3847/2041-8213/aa91c9",

language = "English",

volume = "848",

journal = "Astrophysical Journal Letters",

issn = "2041-8205",

publisher = "American Astronomical Society",

number = "2",

}

LIGO Scientific Collaboration and Virgo Collaboration, Fermi GBM, INTEGRAL, Icecube Collaboration, AstroSat Cadmium Zinc Telluride Imager Team, IPN Collaboration, The Insight-HXMT Collaboration, ANTARES Collaboration, The Swift Collaboration, AGILE Team, The 1M2H Team, The Dark Energy Camera GW-EM Collaboration and the DES Collaboration, DLT40 Collaboration, GRAWITA: GRAvitational Wave Inaf TeAm, The Fermi Large Area Telescope Collaboration, ATCA: Australia Telescope Compact Array, ASKAP: Australian SKA Pathfinder, Las Cumbres Observatory Collaboration, OzGrav, DWF (Deeper, Wider, Faster program), AST3, and CAASTRO Collaborations, The VINROUGE Collaboration, MASTER Collaboration, J-GEM, GROWTH, JAGWAR, Caltech-NRAO, TTU-NRAO, and NuSTAR Collaborations, Pan-STARRS, The MAXI Team, TZAC Consortium, KU Collaboration, Nordic Optical Telescope, ePESSTO, GROND, Texas Tech University, SALT Group, TOROS: Transient Robotic Observatory of the South Collaboration, The BOOTES Collaboration, MWA: Murchison Widefield Array, The CALET Collaboration, IKI-GW Follow-up Collaboration, H.E.S.S. Collaboration, LOFAR Collaboration, LWA: Long Wavelength Array, HAWC Collaboration, The Pierre Auger Collaboration, ALMA Collaboration, Euro VLBI Team, Pi of the Sky Collaboration, The Chandra Team at McGill University, DFN: Desert Fireball Network, ATLAS, High Time Resolution Universe Survey, RIMAS and RATIR & SKA South Africa/MeerKAT 2017, 'Multi-messenger observations of a binary neutron star merger', Astrophysical Journal Letters, vol. 848, no. 2, L12. https://doi.org/10.3847/2041-8213/aa91c9

TY - JOUR

T1 - Multi-messenger observations of a binary neutron star merger

AU - LIGO Scientific Collaboration and Virgo Collaboration

AU - Fermi GBM

AU - INTEGRAL

AU - Icecube Collaboration

AU - AstroSat Cadmium Zinc Telluride Imager Team

AU - IPN Collaboration

AU - The Insight-HXMT Collaboration

AU - ANTARES Collaboration

AU - The Swift Collaboration

AU - AGILE Team

AU - The 1M2H Team

AU - The Dark Energy Camera GW-EM Collaboration and the DES Collaboration

AU - DLT40 Collaboration

AU - GRAWITA: GRAvitational Wave Inaf TeAm

AU - The Fermi Large Area Telescope Collaboration

AU - ATCA: Australia Telescope Compact Array

AU - ASKAP: Australian SKA Pathfinder

AU - Las Cumbres Observatory Collaboration

AU - OzGrav, DWF (Deeper, Wider, Faster program), AST3, and CAASTRO Collaborations

AU - The VINROUGE Collaboration

AU - MASTER Collaboration

AU - J-GEM

AU - GROWTH, JAGWAR, Caltech-NRAO, TTU-NRAO, and NuSTAR Collaborations

AU - Pan-STARRS

AU - The MAXI Team

AU - TZAC Consortium

AU - KU Collaboration

AU - Nordic Optical Telescope

AU - ePESSTO

AU - GROND

AU - Texas Tech University

AU - SALT Group

AU - TOROS: Transient Robotic Observatory of the South Collaboration

AU - The BOOTES Collaboration

AU - MWA: Murchison Widefield Array

AU - The CALET Collaboration

AU - IKI-GW Follow-up Collaboration

AU - H.E.S.S. Collaboration

AU - LOFAR Collaboration

AU - LWA: Long Wavelength Array

AU - HAWC Collaboration

AU - The Pierre Auger Collaboration

AU - ALMA Collaboration

AU - Euro VLBI Team

AU - Pi of the Sky Collaboration

AU - The Chandra Team at McGill University

AU - DFN: Desert Fireball Network

AU - ATLAS

AU - High Time Resolution Universe Survey

AU - RIMAS and RATIR

AU - SKA South Africa/MeerKAT

AU - Abbott, B. P.

AU - Abbott, R.

AU - Abbott, T. D.

AU - Acernese, F.

AU - Ackley, K.

AU - Adams, C.

AU - Adams, T.

AU - Addesso, P.

AU - Adhikari, R. X.

AU - Adya, V. B.

AU - Affeldt, C.

AU - Afrough, M.

AU - Agarwal, B.

AU - Agathos, M.

AU - Agatsuma, K.

AU - Aggarwal, N.

AU - Aguiar, O. D.

AU - Aiello, L.

AU - Ain, A.

AU - Ajith, P.

AU - Allen, B.

AU - Allen, G.

AU - Allocca, A.

AU - Altin, P. A.

AU - Amato, A.

AU - Ananyeva, A.

AU - Anderson, S. B.

AU - Anderson, W. G.

AU - Angelova, S. V.

AU - Antier, S.

AU - Appert, S.

AU - Arai, K.

AU - Araya, M. C.

AU - Areeda, J. S.

AU - Arnaud, N.

AU - Arun, K. G.

AU - Ascenzi, S.

AU - Ashton, G.

AU - Ast, M.

AU - Aston, S. M.

AU - Astone, P.

AU - Atallah, D. V.

AU - Aufmuth, P.

AU - Aulbert, C.

AU - AultONeal, K.

AU - Austin, C.

AU - Avila-Alvarez, A.

AU - Babak, S.

AU - Bacon, P.

AU - Bader, M. K.M.

AU - Bae, S.

AU - Baker, P. T.

AU - Baldaccini, F.

AU - Ballardin, G.

AU - Ballmer, S. W.

AU - Banagiri, S.

AU - Barayoga, J. C.

AU - Barclay, S. E.

AU - Barish, B. C.

AU - Barker, D.

AU - Barkett, K.

AU - Barone, F.

AU - Barr, B.

AU - Barsotti, L.

AU - Barsuglia, M.

AU - Barta, D.

AU - Barthelmy, S. D.

AU - Bartlett, J.

AU - Bartos, I.

AU - Bassiri, R.

AU - Basti, A.

AU - Batch, J. C.

AU - Bawaj, M.

AU - Bayley, J. C.

AU - Bazzan, M.

AU - Bécsy, B.

AU - Beer, C.

AU - Bejger, M.

AU - Belahcene, I.

AU - Bell, A. S.

AU - Berger, B. K.

AU - Bergmann, G.

AU - Bero, J. J.

AU - Berry, C. P.L.

AU - Bersanetti, D.

AU - Bertolini, A.

AU - Betzwieser, J.

AU - Bhagwat, S.

AU - Bhandare, R.

AU - Bilenko, I. A.

AU - Billingsley, G.

AU - Billman, C. R.

AU - Birch, J.

AU - Birney, R.

AU - Birnholtz, O.

AU - Biscans, S.

AU - Biscoveanu, S.

AU - Bisht, A.

AU - Bitossi, M.

AU - Biwer, C.

AU - Bizouard, M. A.

AU - Blackburn, J. K.

AU - Blackman, J.

AU - Blair, C. D.

AU - Blair, D. G.

AU - Blair, R. M.

AU - Bloemen, S.

AU - Bock, O.

AU - Bode, N.

AU - Boer, M.

AU - Bogaert, G.

AU - Bohe, A.

AU - Bondu, F.

AU - Bonilla, E.

AU - Bonnand, R.

AU - Boom, B. A.

AU - Bork, R.

AU - Boschi, V.

AU - Bose, S.

AU - Bossie, K.

AU - Bouffanais, Y.

AU - Bozzi, A.

AU - Bradaschia, C.

AU - Brady, P. R.

AU - Branchesi, M.

AU - Brau, J. E.

AU - Briant, T.

AU - Brillet, A.

AU - Brinkmann, M.

AU - Brisson, V.

AU - Brockill, P.

AU - Broida, J. E.

AU - Brooks, A. F.

AU - Brown, D. A.

AU - Brown, D. D.

AU - Brunett, S.

AU - Buchanan, C. C.

AU - Buikema, A.

AU - Bulik, T.

AU - Bulten, H. J.

AU - Buonanno, A.

AU - Buskulic, D.

AU - Buy, C.

AU - Byer, R. L.

AU - Cabero, M.

AU - Cadonati, L.

AU - Cagnoli, G.

AU - Cahillane, C.

AU - Calderón Bustillo, J.

AU - Callister, T. A.

AU - Calloni, E.

AU - Camp, J. B.

AU - Canepa, M.

AU - Canizares, P.

AU - Cannon, K. C.

AU - Cao, H.

AU - Cao, J.

AU - Capano, C. D.

AU - Capocasa, E.

AU - Carbognani, F.

AU - Caride, S.

AU - Carney, M. F.

AU - Casanueva Diaz, J.

AU - Casentini, C.

AU - Caudill, S.

AU - Cavaglià, M.

AU - Cavalier, F.

AU - Cavalieri, R.

AU - Cella, G.

AU - Cepeda, C. B.

AU - Cerdá-Durán, P.

AU - Cerretani, G.

AU - Cesarini, E.

AU - Chamberlin, S. J.

AU - Chan, M.

AU - Chao, S.

AU - Charlton, P.

AU - Chase, E.

AU - Chassande-Mottin, E.

AU - Chatterjee, D.

AU - Chatziioannou, K.

AU - Cheeseboro, B. D.

AU - Chen, H. Y.

AU - Chen, X.

AU - Chen, Y.

AU - Cheng, H. P.

AU - Chia, H.

AU - Chincarini, A.

AU - Chiummo, A.

AU - Chmiel, T.

AU - Cho, H. S.

AU - Cho, M.

AU - Chow, J. H.

AU - Christensen, N.

AU - Chu, Q.

AU - Chua, A. J.K.

AU - Chua, S.

AU - Chung, A. K.W.

AU - Chung, S.

AU - Ciani, G.

AU - Ciolfi, R.

AU - Cirelli, C. E.

AU - Cirone, A.

AU - Clara, F.

AU - Clark, J. A.

AU - Clearwater, P.

AU - Cleva, F.

AU - Cocchieri, C.

AU - Coccia, E.

AU - Cohadon, P. F.

AU - Cohen, D.

AU - Colla, A.

AU - Collette, C. G.

AU - Cominsky, L. R.

AU - Constancio, M.

AU - Conti, L.

AU - Cooper, S. J.

AU - Corban, P.

AU - Corbitt, T. R.

AU - Cordero-Carrión, I.

AU - Corley, K. R.

AU - Cornish, N.

AU - Corsi, A.

AU - Cortese, S.

AU - Costa, C. A.

AU - Coughlin, M. W.

AU - Coughlin, S. B.

AU - Coulon, J. P.

AU - Countryman, S. T.

AU - Couvares, P.

AU - Covas, P. B.

AU - Cowan, E. E.

AU - Coward, D. M.

AU - Cowart, M. J.

AU - Coyne, D. C.

AU - Coyne, R.

AU - Creighton, J. D.E.

AU - Creighton, T. D.

AU - Cripe, J.

AU - Crowder, S. G.

AU - Cullen, T. J.

AU - Cumming, A.

AU - Cunningham, L.

AU - Cuoco, E.

AU - Dal Canton, T.

AU - Dálya, G.

AU - Danilishin, S. L.

AU - D'Antonio, S.

AU - Danzmann, K.

AU - Dasgupta, A.

N1 - Includes bibliographical references.

PY - 2017/1/1

Y1 - 2017/1/1

N2 - On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of ~1.7 s with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg2 at a luminosity distance of 40± 8 8 Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 M☉. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at ~40 Mpc) less than 11 hours after the merger by the One-Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ∼10 days. Following early non-detections, X-ray and radio emission were discovered at the transient's position ~9 and ~16 days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC 4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta.

AB - On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of ~1.7 s with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg2 at a luminosity distance of 40± 8 8 Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 M☉. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at ~40 Mpc) less than 11 hours after the merger by the One-Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ∼10 days. Following early non-detections, X-ray and radio emission were discovered at the transient's position ~9 and ~16 days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC 4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta.

KW - Gravitational waves

KW - Stars: neutron

UR - https://www.scopus.com/pages/publications/85037171677

UR - https://www.scopus.com/pages/publications/85037171677#tab=citedBy

U2 - 10.3847/2041-8213/aa91c9

DO - 10.3847/2041-8213/aa91c9

M3 - Article

AN - SCOPUS:85037171677

SN - 2041-8205

VL - 848

JO - Astrophysical Journal Letters

JF - Astrophysical Journal Letters

IS - 2

M1 - L12

ER -

Multi-messenger observations of a binary neutron star merger

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