Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube

Research output: Contribution to journalArticleResearchpeer review

Authors

  • The LIGO Scientific Collaboration
  • The Virgo Collaboration
  • ANTARES Collaboration
  • Icecube Collaboration
  • V. B. Adya
  • S. L. Danilishin
  • K. Danzmann
  • M. M. Hanke
  • J. Hennig
  • Michele Heurs
  • H. Lück
  • D. Steinmeyer
  • H. Vahlbruch
  • L. W. Wei
  • D. M. Wilken
  • B. Willke
  • H. Wittel
  • Christoph Affeldt
  • Gerald Bergmann
  • Nina Bode
  • P. Booker
  • Marc Brinkmann
  • M. Cabero
  • T. Dent
  • O. de Varona
  • S. Doravari
  • S. Hochheim
  • J. Junker
  • Kai S. Karvinen
  • S. Khan
  • R. Kirchhoff
  • Patrick Koch
  • S. M. Köhlenbeck
  • N. Koper
  • Volker Kringel
  • G. Kuehn
  • S. Leavey
  • J. Lehmann
  • James Lough
  • Moritz Mehmet
  • Arunava Mukherjee
  • M. Nery
  • F. Ohme
  • P. Oppermann
  • M. Phelps
  • O. Puncken
  • A. Rüdiger
  • Emil Schreiber
  • B. W. Schulte
  • Y. Setyawati
  • M. Standke
  • M. Steinke
  • Fabian Thies
  • Michael Weinert
  • F. Wellmann
  • Peter Weßels
  • Maximilian H. Wimmer
  • W. Winkler
  • J. Woehler
  • D. S. Wu
  • Peter Aufmuth
  • Aparna Bisht
  • Steffen Kaufer

External Research Organisations

  • University of Strasbourg
  • Universitat Politècnica de Catalunya
  • Sezione di Genova
  • Polytechnic University of Valencia
  • Universite d'Aix-Marseille
  • Observatoire de Paris (OBSPARIS)
  • Universitat de Valencia
  • University of Copenhagen
  • Oskar Klein Centre
  • Stockholm University
  • University of Wisconsin
  • University of California at Berkeley
  • Lawrence Berkeley National Laboratory
  • University of Maryland
  • Erlangen Centre for Astroparticle Physics
  • Friedrich-Alexander-Universität Erlangen-Nürnberg (FAU Erlangen-Nürnberg)
  • Pennsylvania State University
  • Technical University of Munich (TUM)
  • Southern University and A&M College
  • Stony Brook University (SBU)
  • Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
  • Carson College of Business
  • University of Adelaide
  • California Institute of Caltech (Caltech)
  • University of Florida
  • Observatoire de la Côte d’Azur (OCA)
  • Tata Institute of Fundamental Research (TIFR HYD)
  • Inje University
  • Seoul National University
  • Radboud University Nijmegen (RU)
  • The Chinese University of Hong Kong
  • Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA)
  • Northwestern University
  • Inter-University Centre for Astronomy and Astrophysics India
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Details

Original languageEnglish
Article number134
JournalAstrophysical Journal
Volume870
Issue number2
Publication statusPublished - 16 Jan 2019

Keywords

    gravitational waves, neutrinos

ASJC Scopus subject areas

Cite this

Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube. / The LIGO Scientific Collaboration; The Virgo Collaboration; ANTARES Collaboration et al.
In: Astrophysical Journal, Vol. 870, No. 2, 134, 16.01.2019.

Research output: Contribution to journalArticleResearchpeer review

The LIGO Scientific Collaboration, The Virgo Collaboration, ANTARES Collaboration, Icecube Collaboration, Adya, VB, Danilishin, SL, Danzmann, K, Hanke, MM, Hennig, J, Heurs, M, Lück, H, Steinmeyer, D, Vahlbruch, H, Wei, LW, Wilken, DM, Willke, B, Wittel, H, Affeldt, C, Bergmann, G, Bode, N, Booker, P, Brinkmann, M, Cabero, M, Dent, T, de Varona, O, Doravari, S, Hochheim, S, Junker, J, Karvinen, KS, Khan, S, Kirchhoff, R, Koch, P, Köhlenbeck, SM, Koper, N, Kringel, V, Kuehn, G, Leavey, S, Lehmann, J, Lough, J, Mehmet, M, Mukherjee, A, Nery, M, Ohme, F, Oppermann, P, Phelps, M, Puncken, O, Rüdiger, A, Schreiber, E, Schulte, BW, Setyawati, Y, Standke, M, Steinke, M, Thies, F, Weinert, M, Wellmann, F, Weßels, P, Wimmer, MH, Winkler, W, Woehler, J, Wu, DS, Aufmuth, P, Bisht, A & Kaufer, S 2019, 'Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube', Astrophysical Journal, vol. 870, no. 2, 134. https://doi.org/10.3847/1538-4357/aaf21d, https://doi.org/10.15488/5202
The LIGO Scientific Collaboration, The Virgo Collaboration, ANTARES Collaboration, Icecube Collaboration, Adya, V. B., Danilishin, S. L., Danzmann, K., Hanke, M. M., Hennig, J., Heurs, M., Lück, H., Steinmeyer, D., Vahlbruch, H., Wei, L. W., Wilken, D. M., Willke, B., Wittel, H., Affeldt, C., Bergmann, G., ... Kaufer, S. (2019). Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube. Astrophysical Journal, 870(2), Article 134. https://doi.org/10.3847/1538-4357/aaf21d, https://doi.org/10.15488/5202
The LIGO Scientific Collaboration, The Virgo Collaboration, ANTARES Collaboration, Icecube Collaboration, Adya VB, Danilishin SL et al. Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube. Astrophysical Journal. 2019 Jan 16;870(2):134. doi: 10.3847/1538-4357/aaf21d, 10.15488/5202
The LIGO Scientific Collaboration ; The Virgo Collaboration ; ANTARES Collaboration et al. / Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube. In: Astrophysical Journal. 2019 ; Vol. 870, No. 2.
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@article{396638dd62944d8684fd13ca74a33564,
title = "Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube",
keywords = "gravitational waves, neutrinos",
author = "{The LIGO Scientific Collaboration} and {The Virgo Collaboration} and {ANTARES Collaboration} and {Icecube Collaboration} and A. Albert and M. Andr{\'e} and M. Anghinolfi and M. Ardid and Aubert, {J. J.} and J. Aublin and T. Avgitas and B. Baret and J. Barrios-Mart{\'i} and M. Ahlers and M. Ahrens and Kelley, {J. L.} and Klein, {S. R.} and T. Schmidt and A. Schneider and J. Schneider and Weiss, {M. J.} and C. Wendt and M. Wolf and Xu, {X. W.} and Y. Xu and Adya, {V. B.} and S. Bose and Brown, {D. D.} and Y. Chen and Cheng, {H. P.} and Danilishin, {S. L.} and K. Danzmann and Hanke, {M. M.} and J. Hennig and Michele Heurs and A. Hreibi and S. Kumar and Lee, {H. K.} and J. Lee and X. Li and H. L{\"u}ck and P. Schmidt and D. Steinmeyer and L. Sun and H. Vahlbruch and Wang, {Y. F.} and Wei, {L. W.} and Wilken, {D. M.} and B. Willke and H. Wittel and L. Zhang and M. Zhou and Christoph Affeldt and Gerald Bergmann and Nina Bode and P. Booker and Marc Brinkmann and M. Cabero and T. Dent and {de Varona}, O. and S. Doravari and S. Hochheim and J. Junker and Karvinen, {Kai S.} and S. Khan and R. Kirchhoff and Patrick Koch and K{\"o}hlenbeck, {S. M.} and N. Koper and Volker Kringel and G. Kuehn and S. Leavey and J. Lehmann and James Lough and Moritz Mehmet and Arunava Mukherjee and M. Nery and F. Ohme and P. Oppermann and M. Phelps and O. Puncken and A. R{\"u}diger and Emil Schreiber and Schulte, {B. W.} and Y. Setyawati and M. Standke and M. Steinke and Fabian Thies and Michael Weinert and F. Wellmann and Peter We{\ss}els and Wimmer, {Maximilian H.} and W. Winkler and J. Woehler and Wu, {D. S.} and Peter Aufmuth and Aparna Bisht and Steffen Kaufer",
note = "Funding information: The ANTARES Collaboration acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat {\`a} l{\textquoteright}{\'e}nergie atomique et aux {\'e}nergies alternatives (CEA), Commission Europ{\'e}enne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), IdEx program and UnivEarthS Labex program at Sorbonne Paris Cit{\'e} (ANR-10-LABX-0023 and ANR-11-IDEX-0005-02), Labex OCEVU (ANR-11-LABX-0060) and the A*MIDEX project (ANR-11-IDEX-0001-02), R{\'e}gion Ile-de-Franc{\^e} (DIM-ACAV), R{\'e}gion Alsace (contrat CPER), R{\'e}gion Provence-Alpes-C{\^o}te d{\textquoteright}Azur, D{\'e}par-tement du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium f{\"u}r Bildung und Forschung (BMBF), Germany; Istituto Nazionale di Fisica Nucleare (INFN), Italy; Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia; National Authority for Scientific Research (ANCS), Romania; Ministerio de Econo-m{\'i}a y Competitividad (MINECO): Plan Estatal de Investiga-ci{\'o}n (refs. FPA2015-65150-C3-1-P, -2-P and -3-P, (MINECO/ FEDER)), Severo Ochoa Centre of Excellence and MultiDark Consolider (MINECO), and Prometeo and Grisol{\'i}a programs (Generalitat Valenciana), Spain; Ministry of Higher Education, Scientific Research and Professional Training, Morocco. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities. The IceCube Collaboration gratefully acknowledges the following support: USA—U.S. National Science Foundation-Office of Polar Programs, U.S. National Science Foundation-Physics Division, Wisconsin Alumni Research Foundation, Center for High Throughput Computing (CHTC) at the University of Wisconsin-Madison, Open Science Grid (OSG), Extreme Science and Engineering Discovery Environment (XSEDE), U.S. Department of Energy-National Energy Research Scientific Computing Center, Particle astrophysics research computing center at the University of Maryland, Institute for Cyber-Enabled Research at Michigan State University, and Astroparticle physics computational facility at Marquette University; Belgium—Funds for Scientific Research (FRS-FNRS and FWO), FWO Odysseus and Big Science programmes, and Belgian Federal Science Policy Office (Belspo); Germany—Bundesministerium f{\"u}r Bildung und Forschung (BMBF), Deutsche Forschungsgemeinschaft (DFG), Helmholtz Alliance for Astroparticle Physics (HAP), Initiative and Networking Fund of the Helmholtz Association, Deutsches Elektronen Synchrotron (DESY), and High Performance Computing cluster of the RWTH Aachen; Sweden—Swedish Research Council, Swedish Polar Research Secretariat, Swedish National Infrastructure for Computing (SNIC), and Knut and Alice Wallenberg Foundation; Australia—Australian Research Council; Canada— Natural Sciences and Engineering Research Council of Canada, Calcul Qu{\'e}bec, Compute Ontario, Canada Foundation for Innovation, WestGrid, and Compute Canada; Denmark—Villum Fonden, Danish National Research Foundation (DNRF); New Zealand—Marsden Fund; Japan—Japan Society for Promotion of Science (JSPS) and Institute for Global Prominent Research (IGPR) of Chiba University; Korea—National Research Foundation of Korea (NRF); Switzerland—Swiss National Science Foundation (SNSF). The LIGO Scientific Collaboration and the Virgo Collaboration gratefully acknowledge the support of the United States National Science Foundation (NSF) for the construction and operation of the LIGO Laboratory and Advanced LIGO as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck-Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS) and the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, for the construction and operation of the Virgo detector and the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies as well as by the Council of Scientific and Industrial Research of India, the Department of Science and Technology, India, the Science & Engineering Research Board (SERB), India, the Ministry of Human Resource Development, India, the Spanish Agencia Estatal de Investigaci{\'o}n, the Vice-presid{\`e}ncia i Conselleria d{\textquoteright}Innovaci{\'o} Recerca i Turisme and the Conselleria d{\textquoteright}Educaci{\'o} i Universitat del Govern de les Illes Balears, the Conselleria d{\textquoteright}Educaci{\'o} Investigaci{\'o} Cultura i Esport de la Generalitat Valenciana, the National Science Centre of Poland, the Swiss National Science Foundation (SNSF), the Russian Foundation for Basic Research, the Russian Science Foundation, the European Commission, the European Regional Development Funds (ERDF), the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, the Hungarian Scientific Research Fund (OTKA), the Lyon Institute of Origins (LIO), the Paris Il? e-de-France Region, the National Research, Development and Innovation Office Hungary (NKFI), the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation, the Natural Science and Engineering Research Council Canada, the Canadian Institute for Advanced Research, the Brazilian Ministry of Science, Technology, Innovations, and Communications, the International Center for Theoretical Physics South American Institute for Fundamental Research (ICTP-SAIFR), the Research Grants Council of Hong Kong, the National Natural Science Foundation of China (NSFC), the Leverhulme Trust, the Research Corporation, the Ministry of Science and Technology (MOST), Taiwan and the Kavli Foundation. The authors gratefully acknowledge the support of the NSF, STFC, MPS, INFN, CNRS, and the State of Niedersachsen/Germany for provision of computational resources.",
year = "2019",
month = jan,
day = "16",
doi = "10.3847/1538-4357/aaf21d",
language = "English",
volume = "870",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "IOP Publishing Ltd.",
number = "2",

}

Download

TY - JOUR

T1 - Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube

AU - The LIGO Scientific Collaboration

AU - The Virgo Collaboration

AU - ANTARES Collaboration

AU - Icecube Collaboration

AU - Albert, A.

AU - André, M.

AU - Anghinolfi, M.

AU - Ardid, M.

AU - Aubert, J. J.

AU - Aublin, J.

AU - Avgitas, T.

AU - Baret, B.

AU - Barrios-Martí, J.

AU - Ahlers, M.

AU - Ahrens, M.

AU - Kelley, J. L.

AU - Klein, S. R.

AU - Schmidt, T.

AU - Schneider, A.

AU - Schneider, J.

AU - Weiss, M. J.

AU - Wendt, C.

AU - Wolf, M.

AU - Xu, X. W.

AU - Xu, Y.

AU - Adya, V. B.

AU - Bose, S.

AU - Brown, D. D.

AU - Chen, Y.

AU - Cheng, H. P.

AU - Danilishin, S. L.

AU - Danzmann, K.

AU - Hanke, M. M.

AU - Hennig, J.

AU - Heurs, Michele

AU - Hreibi, A.

AU - Kumar, S.

AU - Lee, H. K.

AU - Lee, J.

AU - Li, X.

AU - Lück, H.

AU - Schmidt, P.

AU - Steinmeyer, D.

AU - Sun, L.

AU - Vahlbruch, H.

AU - Wang, Y. F.

AU - Wei, L. W.

AU - Wilken, D. M.

AU - Willke, B.

AU - Wittel, H.

AU - Zhang, L.

AU - Zhou, M.

AU - Affeldt, Christoph

AU - Bergmann, Gerald

AU - Bode, Nina

AU - Booker, P.

AU - Brinkmann, Marc

AU - Cabero, M.

AU - Dent, T.

AU - de Varona, O.

AU - Doravari, S.

AU - Hochheim, S.

AU - Junker, J.

AU - Karvinen, Kai S.

AU - Khan, S.

AU - Kirchhoff, R.

AU - Koch, Patrick

AU - Köhlenbeck, S. M.

AU - Koper, N.

AU - Kringel, Volker

AU - Kuehn, G.

AU - Leavey, S.

AU - Lehmann, J.

AU - Lough, James

AU - Mehmet, Moritz

AU - Mukherjee, Arunava

AU - Nery, M.

AU - Ohme, F.

AU - Oppermann, P.

AU - Phelps, M.

AU - Puncken, O.

AU - Rüdiger, A.

AU - Schreiber, Emil

AU - Schulte, B. W.

AU - Setyawati, Y.

AU - Standke, M.

AU - Steinke, M.

AU - Thies, Fabian

AU - Weinert, Michael

AU - Wellmann, F.

AU - Weßels, Peter

AU - Wimmer, Maximilian H.

AU - Winkler, W.

AU - Woehler, J.

AU - Wu, D. S.

AU - Aufmuth, Peter

AU - Bisht, Aparna

AU - Kaufer, Steffen

N1 - Funding information: The ANTARES Collaboration acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat à l’énergie atomique et aux énergies alternatives (CEA), Commission Européenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), IdEx program and UnivEarthS Labex program at Sorbonne Paris Cité (ANR-10-LABX-0023 and ANR-11-IDEX-0005-02), Labex OCEVU (ANR-11-LABX-0060) and the A*MIDEX project (ANR-11-IDEX-0001-02), Région Ile-de-Francê (DIM-ACAV), Région Alsace (contrat CPER), Région Provence-Alpes-Côte d’Azur, Dépar-tement du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium für Bildung und Forschung (BMBF), Germany; Istituto Nazionale di Fisica Nucleare (INFN), Italy; Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia; National Authority for Scientific Research (ANCS), Romania; Ministerio de Econo-mía y Competitividad (MINECO): Plan Estatal de Investiga-ción (refs. FPA2015-65150-C3-1-P, -2-P and -3-P, (MINECO/ FEDER)), Severo Ochoa Centre of Excellence and MultiDark Consolider (MINECO), and Prometeo and Grisolía programs (Generalitat Valenciana), Spain; Ministry of Higher Education, Scientific Research and Professional Training, Morocco. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities. The IceCube Collaboration gratefully acknowledges the following support: USA—U.S. National Science Foundation-Office of Polar Programs, U.S. National Science Foundation-Physics Division, Wisconsin Alumni Research Foundation, Center for High Throughput Computing (CHTC) at the University of Wisconsin-Madison, Open Science Grid (OSG), Extreme Science and Engineering Discovery Environment (XSEDE), U.S. Department of Energy-National Energy Research Scientific Computing Center, Particle astrophysics research computing center at the University of Maryland, Institute for Cyber-Enabled Research at Michigan State University, and Astroparticle physics computational facility at Marquette University; Belgium—Funds for Scientific Research (FRS-FNRS and FWO), FWO Odysseus and Big Science programmes, and Belgian Federal Science Policy Office (Belspo); Germany—Bundesministerium für Bildung und Forschung (BMBF), Deutsche Forschungsgemeinschaft (DFG), Helmholtz Alliance for Astroparticle Physics (HAP), Initiative and Networking Fund of the Helmholtz Association, Deutsches Elektronen Synchrotron (DESY), and High Performance Computing cluster of the RWTH Aachen; Sweden—Swedish Research Council, Swedish Polar Research Secretariat, Swedish National Infrastructure for Computing (SNIC), and Knut and Alice Wallenberg Foundation; Australia—Australian Research Council; Canada— Natural Sciences and Engineering Research Council of Canada, Calcul Québec, Compute Ontario, Canada Foundation for Innovation, WestGrid, and Compute Canada; Denmark—Villum Fonden, Danish National Research Foundation (DNRF); New Zealand—Marsden Fund; Japan—Japan Society for Promotion of Science (JSPS) and Institute for Global Prominent Research (IGPR) of Chiba University; Korea—National Research Foundation of Korea (NRF); Switzerland—Swiss National Science Foundation (SNSF). The LIGO Scientific Collaboration and the Virgo Collaboration gratefully acknowledge the support of the United States National Science Foundation (NSF) for the construction and operation of the LIGO Laboratory and Advanced LIGO as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck-Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS) and the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, for the construction and operation of the Virgo detector and the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies as well as by the Council of Scientific and Industrial Research of India, the Department of Science and Technology, India, the Science & Engineering Research Board (SERB), India, the Ministry of Human Resource Development, India, the Spanish Agencia Estatal de Investigación, the Vice-presidència i Conselleria d’Innovació Recerca i Turisme and the Conselleria d’Educació i Universitat del Govern de les Illes Balears, the Conselleria d’Educació Investigació Cultura i Esport de la Generalitat Valenciana, the National Science Centre of Poland, the Swiss National Science Foundation (SNSF), the Russian Foundation for Basic Research, the Russian Science Foundation, the European Commission, the European Regional Development Funds (ERDF), the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, the Hungarian Scientific Research Fund (OTKA), the Lyon Institute of Origins (LIO), the Paris Il? e-de-France Region, the National Research, Development and Innovation Office Hungary (NKFI), the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation, the Natural Science and Engineering Research Council Canada, the Canadian Institute for Advanced Research, the Brazilian Ministry of Science, Technology, Innovations, and Communications, the International Center for Theoretical Physics South American Institute for Fundamental Research (ICTP-SAIFR), the Research Grants Council of Hong Kong, the National Natural Science Foundation of China (NSFC), the Leverhulme Trust, the Research Corporation, the Ministry of Science and Technology (MOST), Taiwan and the Kavli Foundation. The authors gratefully acknowledge the support of the NSF, STFC, MPS, INFN, CNRS, and the State of Niedersachsen/Germany for provision of computational resources.

PY - 2019/1/16

Y1 - 2019/1/16

KW - gravitational waves

KW - neutrinos

UR - http://www.scopus.com/inward/record.url?scp=85060246308&partnerID=8YFLogxK

U2 - 10.3847/1538-4357/aaf21d

DO - 10.3847/1538-4357/aaf21d

M3 - Article

AN - SCOPUS:85060246308

VL - 870

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 2

M1 - 134

ER -

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