@article{caltechauthors68705,
          volume = {93},
          number = {12},
           month = {June},
          author = {S. Adri{\'a}n-Mart{\'i}nez and B. P. Abbott and R. Abbott and M. R. Abernathy and R. X. Adhikari and S. B. Anderson and K. Arai and M. C. Araya and J. C.  Barayoga and B. C. Barish and B. K. Berger and G. Billingsley and J. K. Blackburn and R. Bork and A. F. Brooks and C. Cahillane and T. Callister and C. B. Cepeda and R. Chakraborty and T. Chalermsongsak and P. Couvares and D. C. Coyne and V. Dergachev and R. W. P. Drever and P. Ehrens and T. Etzel and S. E. Gossan and K. E. Gushwa and E. K. Gustafson and E. D. Hall and A. W. Heptonstall and K. A. Hodge and M. Isi and J. B. Kanner and W. Kells and V. Kondrashov and W. Z. Korth and D. B. Kozak and A. Lazzarini and T. G. F. Li and M. Mageswaran and E. Maros and D. V. Martynov and J. N. Marx and G. McIntyre and J. McIver and S. Meshkov and M. Pedraza and A. Perreca and L. R. Price  and E. A. Quintero and D. H. Reitze and N. A. Robertson and J. G. Rollins and S. Sachdev and E. J. Sanchez and P. Schmidt and Z. Shao and A. Singer and N. D. Smith and R. J. E. Smith and R. Taylor and M. P. Thirugnanasambandam and C. V. Torres and C. I. Torrie and G. Vajente and S. Vass and L. Wallace and A. J. Weinstein and S. E. Whitcomb and R. D. Williams and C. C. Wipf and H. Yamamoto and L. Zhang and M. E. Zucker and J. Zweizig and Y. Chen and W. Engels and C. D. Ott and K. S. Thorne},
            note = {{\copyright} 2016 American Physical Society. Received 21 February 2016; published 23 June 2016.

The authors acknowledge the financial support of the
funding agencies: Centre National de la Recherche
Scientifique (CNRS), Commissariat {\`a} l?{\'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), R{\'e}gion {\^I}lede-
France (DIM-ACAV), R{\'e}gion Alsace (contrat CPER),
R{\'e}gion Provence-Alpes-C{\^o}te d?Azur, D{\'e}partement 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; Stichting voor
Fundamenteel Onderzoek der Materie (FOM), 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
Econom{\'i}a y Competitividad (MINECO), Prometeo and
Grisol{\'i}a programs of Generalitat Valenciana and
MultiDark, Spain; Agence de l?Oriental and CNRST,
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. We acknowledge
the support from the following agencies: U.S.
National Science Foundation-Office of Polar Programs,
U.S. National Science Foundation-Physics Division,
University of Wisconsin Alumni Research Foundation,
the Grid Laboratory Of Wisconsin (GLOW) grid infrastructure
at the University of Wisconsin - Madison, the
Open Science Grid (OSG) grid infrastructure; U.S.
Department of Energy, and National Energy Research
Scientific Computing Center, the Louisiana Optical
Network Initiative (LONI) grid computing resources;
Natural Sciences and Engineering Research Council of
Canada, WestGrid and Compute/Calcul Canada; Swedish
Research Council, Swedish Polar Research Secretariat,
Swedish National Infrastructure for Computing (SNIC),
and Knut and Alice Wallenberg Foundation, Sweden;
German Ministry for Education and Research (BMBF),
Deutsche Forschungsgemeinschaft (DFG), Helmholtz
Alliance for Astroparticle Physics (HAP), Research
Department of Plasmas with Complex Interactions
(Bochum), Germany; Fund for Scientific Research
(FNRS-FWO), FWO Odysseus programme, Flanders
Institute to encourage scientific and technological research
in industry (IWT), Belgian Federal Science Policy Office
(Belspo); University of Oxford, United Kingdom; Marsden
Fund, New Zealand; Australian Research Council;
Japan Society for Promotion of Science (JSPS); the
Swiss National Science Foundation (SNSF), Switzerland;
National Research Foundation of Korea (NRF); Danish
National Research Foundation, Denmark (DNRF). The
authors 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, Department of Science and
Technology, India, Science \& Engineering Research
Board (SERB), India, Ministry of Human Resource
Development, India, the Spanish Ministerio de Econom{\'i}a
y Competitividad, the Conselleria d?Economia i
Competitivitat and Conselleria d?Educaci{\'o}, Cultura i
Universitats of the Govern de les Illes Balears, the
National Science Centre of Poland, the European
Commission, 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 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, Canadian Institute for
Advanced Research, the Brazilian Ministry of Science,
Technology, and Innovation, Russian Foundation for Basic
Research, the Leverhulme Trust, the Research Corporation,
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. This article has LIGO document number
LIGO-P1500271. },
           title = {High-energy Neutrino follow-up search of Gravitational Wave Event GW150914 with ANTARES and IceCube},
       publisher = {American Physical Society},
            year = {2016},
         journal = {Physical Review D},
           pages = {Art. No. 122010},
             url = {http://resolver.caltech.edu/CaltechAUTHORS:20160628-092040474},
        abstract = {We present the high-energy-neutrino follow-up observations of the first gravitational wave transient GW150914 observed by the Advanced LIGO detectors on September 14, 2015. We search for coincident neutrino candidates within the data recorded by the IceCube and Antares neutrino detectors. A possible joint detection could be used in targeted electromagnetic follow-up observations, given the significantly better angular resolution of neutrino events compared to gravitational waves. We find no neutrino candidates in both temporal and spatial coincidence with the gravitational wave event. Within {$\pm$}500  s of the gravitational wave event, the number of neutrino candidates detected by IceCube and Antares were three and zero, respectively. This is consistent with the expected atmospheric background, and none of the neutrino candidates were directionally coincident with GW150914. We use this nondetection to constrain neutrino emission from the gravitational-wave event.}
}

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B.","Lazzarini, A.","Li, T. G. F.","Mageswaran, M.","Maros, E.","Martynov, D. V.","Marx, J. N.","McIntyre, G.","McIver, J.","Meshkov, S.","Pedraza, M.","Perreca, A.","Price, L. R.","Quintero, E. A.","Reitze, D. H.","Robertson, N. A.","Rollins, J. G.","Sachdev, S.","Sanchez, E. J.","Schmidt, P.","Shao, Z.","Singer, A.","Smith, N. D.","Smith, R. J. E.","Taylor, R.","Thirugnanasambandam, M. P.","Torres, C. V.","Torrie, C. I.","Vajente, G.","Vass, S.","Wallace, L.","Weinstein, A. J.","Whitcomb, S. E.","Williams, R. D.","Wipf, C. C.","Yamamoto, H.","Zhang, L.","Zucker, M. E.","Zweizig, J.","Chen, Y.","Engels, W.","Ott, C. D.","Thorne, K. 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2016 American Physical Society. Received 21 February 2016; published 23 June 2016. The authors 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), Région \\^Ilede- France (DIM-ACAV), Région Alsace (contrat CPER), Région Provence-Alpes-C\\^ote d?Azur, Département du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium für Bildung und Forschung (BMBF), Germany; Istituto Nazionale di Fisica Nucleare (INFN), Italy; Stichting voor Fundamenteel Onderzoek der Materie (FOM), 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 Economía y Competitividad (MINECO), Prometeo and Grisolía programs of Generalitat Valenciana and MultiDark, Spain; Agence de l?Oriental and CNRST, 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. We acknowledge the support from the following agencies: U.S. National Science Foundation-Office of Polar Programs, U.S. National Science Foundation-Physics Division, University of Wisconsin Alumni Research Foundation, the Grid Laboratory Of Wisconsin (GLOW) grid infrastructure at the University of Wisconsin - Madison, the Open Science Grid (OSG) grid infrastructure; U.S. Department of Energy, and National Energy Research Scientific Computing Center, the Louisiana Optical Network Initiative (LONI) grid computing resources; Natural Sciences and Engineering Research Council of Canada, WestGrid and Compute/Calcul Canada; Swedish Research Council, Swedish Polar Research Secretariat, Swedish National Infrastructure for Computing (SNIC), and Knut and Alice Wallenberg Foundation, Sweden; German Ministry for Education and Research (BMBF), Deutsche Forschungsgemeinschaft (DFG), Helmholtz Alliance for Astroparticle Physics (HAP), Research Department of Plasmas with Complex Interactions (Bochum), Germany; Fund for Scientific Research (FNRS-FWO), FWO Odysseus programme, Flanders Institute to encourage scientific and technological research in industry (IWT), Belgian Federal Science Policy Office (Belspo); University of Oxford, United Kingdom; Marsden Fund, New Zealand; Australian Research Council; Japan Society for Promotion of Science (JSPS); the Swiss National Science Foundation (SNSF), Switzerland; National Research Foundation of Korea (NRF); Danish National Research Foundation, Denmark (DNRF). The authors 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, Department of Science and Technology, India, Science & Engineering Research Board (SERB), India, Ministry of Human Resource Development, India, the Spanish Ministerio de Economía y Competitividad, the Conselleria d?Economia i Competitivitat and Conselleria d?Educació, Cultura i Universitats of the Govern de les Illes Balears, the National Science Centre of Poland, the European Commission, 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 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, Canadian Institute for Advanced Research, the Brazilian Ministry of Science, Technology, and Innovation, Russian Foundation for Basic Research, the Leverhulme Trust, the Research Corporation, 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. This article has LIGO document number LIGO-P1500271. ","title":"High-energy Neutrino follow-up search of Gravitational Wave Event GW150914 with ANTARES and IceCube","publisher":"American Physical Society","year":"2016","journal":"Physical Review D","pages":"Art. No. 122010","url":"http://resolver.caltech.edu/CaltechAUTHORS:20160628-092040474","abstract":"We present the high-energy-neutrino follow-up observations of the first gravitational wave transient GW150914 observed by the Advanced LIGO detectors on September 14, 2015. We search for coincident neutrino candidates within the data recorded by the IceCube and Antares neutrino detectors. A possible joint detection could be used in targeted electromagnetic follow-up observations, given the significantly better angular resolution of neutrino events compared to gravitational waves. We find no neutrino candidates in both temporal and spatial coincidence with the gravitational wave event. Within $\\pm$500  s of the gravitational wave event, the number of neutrino candidates detected by IceCube and Antares were three and zero, respectively. This is consistent with the expected atmospheric background, and none of the neutrino candidates were directionally coincident with GW150914. We use this nondetection to constrain neutrino emission from the gravitational-wave event.","bibtex":"@article{caltechauthors68705,\n volume = {93},\n number = {12},\n month = {June},\n author = {S. Adri{\\'a}n-Mart{\\'i}nez and B. P. Abbott and R. Abbott and M. R. Abernathy and R. X. Adhikari and S. B. Anderson and K. Arai and M. C. Araya and J. C. Barayoga and B. C. Barish and B. K. Berger and G. Billingsley and J. K. Blackburn and R. Bork and A. F. Brooks and C. Cahillane and T. Callister and C. B. Cepeda and R. Chakraborty and T. Chalermsongsak and P. Couvares and D. C. Coyne and V. Dergachev and R. W. P. Drever and P. Ehrens and T. Etzel and S. E. Gossan and K. E. Gushwa and E. K. Gustafson and E. D. Hall and A. W. Heptonstall and K. A. Hodge and M. Isi and J. B. Kanner and W. Kells and V. Kondrashov and W. Z. Korth and D. B. Kozak and A. Lazzarini and T. G. F. Li and M. Mageswaran and E. Maros and D. V. Martynov and J. N. Marx and G. McIntyre and J. McIver and S. Meshkov and M. Pedraza and A. Perreca and L. R. Price and E. A. Quintero and D. H. Reitze and N. A. Robertson and J. G. Rollins and S. Sachdev and E. J. Sanchez and P. Schmidt and Z. Shao and A. Singer and N. D. Smith and R. J. E. Smith and R. Taylor and M. P. Thirugnanasambandam and C. V. Torres and C. I. Torrie and G. Vajente and S. Vass and L. Wallace and A. J. Weinstein and S. E. Whitcomb and R. D. Williams and C. C. Wipf and H. Yamamoto and L. Zhang and M. E. Zucker and J. Zweizig and Y. Chen and W. Engels and C. D. Ott and K. S. Thorne},\n note = {{\\copyright} 2016 American Physical Society. Received 21 February 2016; published 23 June 2016.\r\n\r\nThe authors acknowledge the financial support of the\r\nfunding agencies: Centre National de la Recherche\r\nScientifique (CNRS), Commissariat {\\`a} l?{\\'e}nergie atomique\r\net aux {\\'e}nergies alternatives (CEA), Commission\r\nEurop{\\'e}enne (FEDER fund and Marie Curie Program),\r\nInstitut Universitaire de France (IUF), IdEx program and\r\nUnivEarthS Labex program at Sorbonne Paris Cit{\\'e} (ANR-\r\n10-LABX-0023 and ANR-11-IDEX-0005-02), R{\\'e}gion {\\^I}lede-\r\nFrance (DIM-ACAV), R{\\'e}gion Alsace (contrat CPER),\r\nR{\\'e}gion Provence-Alpes-C{\\^o}te d?Azur, D{\\'e}partement du Var\r\nand Ville de La Seyne-sur-Mer, France; Bundesministerium\r\nf{\\\"u}r Bildung und Forschung (BMBF), Germany; Istituto\r\nNazionale di Fisica Nucleare (INFN), Italy; Stichting voor\r\nFundamenteel Onderzoek der Materie (FOM), Nederlandse\r\norganisatie voor Wetenschappelijk Onderzoek (NWO), the\r\nNetherlands; Council of the President of the Russian\r\nFederation for young scientists and leading scientific\r\nschools supporting grants, Russia; National Authority for\r\nScientific Research (ANCS), Romania; Ministerio de\r\nEconom{\\'i}a y Competitividad (MINECO), Prometeo and\r\nGrisol{\\'i}a programs of Generalitat Valenciana and\r\nMultiDark, Spain; Agence de l?Oriental and CNRST,\r\nMorocco. We also acknowledge the technical support of\r\nIfremer, AIM and Foselev Marine for the sea operation and\r\nthe CC-IN2P3 for the computing facilities. We acknowledge\r\nthe support from the following agencies: U.S.\r\nNational Science Foundation-Office of Polar Programs,\r\nU.S. National Science Foundation-Physics Division,\r\nUniversity of Wisconsin Alumni Research Foundation,\r\nthe Grid Laboratory Of Wisconsin (GLOW) grid infrastructure\r\nat the University of Wisconsin - Madison, the\r\nOpen Science Grid (OSG) grid infrastructure; U.S.\r\nDepartment of Energy, and National Energy Research\r\nScientific Computing Center, the Louisiana Optical\r\nNetwork Initiative (LONI) grid computing resources;\r\nNatural Sciences and Engineering Research Council of\r\nCanada, WestGrid and Compute/Calcul Canada; Swedish\r\nResearch Council, Swedish Polar Research Secretariat,\r\nSwedish National Infrastructure for Computing (SNIC),\r\nand Knut and Alice Wallenberg Foundation, Sweden;\r\nGerman Ministry for Education and Research (BMBF),\r\nDeutsche Forschungsgemeinschaft (DFG), Helmholtz\r\nAlliance for Astroparticle Physics (HAP), Research\r\nDepartment of Plasmas with Complex Interactions\r\n(Bochum), Germany; Fund for Scientific Research\r\n(FNRS-FWO), FWO Odysseus programme, Flanders\r\nInstitute to encourage scientific and technological research\r\nin industry (IWT), Belgian Federal Science Policy Office\r\n(Belspo); University of Oxford, United Kingdom; Marsden\r\nFund, New Zealand; Australian Research Council;\r\nJapan Society for Promotion of Science (JSPS); the\r\nSwiss National Science Foundation (SNSF), Switzerland;\r\nNational Research Foundation of Korea (NRF); Danish\r\nNational Research Foundation, Denmark (DNRF). The\r\nauthors gratefully acknowledge the support of the United\r\nStates National Science Foundation (NSF) for the construction\r\nand operation of the LIGO Laboratory and\r\nAdvanced LIGO as well as the Science and Technology\r\nFacilities Council (STFC) of the United Kingdom,\r\nthe Max-Planck-Society (MPS), and the State of Niedersachsen/Germany for support of the construction\r\nof Advanced LIGO and construction and operation of\r\nthe GEO600 detector. Additional support for Advanced\r\nLIGO was provided by the Australian Research Council.\r\nThe authors gratefully acknowledge the Italian Istituto\r\nNazionale di Fisica Nucleare (INFN), the French Centre\r\nNational de la Recherche Scientifique (CNRS) and the\r\nFoundation for Fundamental Research on Matter supported\r\nby the Netherlands Organisation for Scientific Research,\r\nfor the construction and operation of the Virgo detector and\r\nthe creation and support of the EGO consortium. The\r\nauthors also gratefully acknowledge research support from\r\nthese agencies as well as by the Council of Scientific and\r\nIndustrial Research of India, Department of Science and\r\nTechnology, India, Science \\& Engineering Research\r\nBoard (SERB), India, Ministry of Human Resource\r\nDevelopment, India, the Spanish Ministerio de Econom{\\'i}a\r\ny Competitividad, the Conselleria d?Economia i\r\nCompetitivitat and Conselleria d?Educaci{\\'o}, Cultura i\r\nUniversitats of the Govern de les Illes Balears, the\r\nNational Science Centre of Poland, the European\r\nCommission, the Royal Society, the Scottish Funding\r\nCouncil, the Scottish Universities Physics Alliance, the\r\nHungarian Scientific Research Fund (OTKA), the Lyon\r\nInstitute of Origins (LIO), the National Research\r\nFoundation of Korea, Industry Canada and the Province\r\nof Ontario through the Ministry of Economic Development\r\nand Innovation, the Natural Science and Engineering\r\nResearch Council Canada, Canadian Institute for\r\nAdvanced Research, the Brazilian Ministry of Science,\r\nTechnology, and Innovation, Russian Foundation for Basic\r\nResearch, the Leverhulme Trust, the Research Corporation,\r\nMinistry of Science and Technology (MOST), Taiwan and\r\nthe Kavli Foundation. The authors gratefully acknowledge\r\nthe support of the NSF, STFC, MPS, INFN, CNRS and the\r\nState of Niedersachsen/Germany for provision of computational\r\nresources. This article has LIGO document number\r\nLIGO-P1500271. },\n title = {High-energy Neutrino follow-up search of Gravitational Wave Event GW150914 with ANTARES and IceCube},\n publisher = {American Physical Society},\n year = {2016},\n journal = {Physical Review D},\n pages = {Art. No. 122010},\n url = {http://resolver.caltech.edu/CaltechAUTHORS:20160628-092040474},\n abstract = {We present the high-energy-neutrino follow-up observations of the first gravitational wave transient GW150914 observed by the Advanced LIGO detectors on September 14, 2015. We search for coincident neutrino candidates within the data recorded by the IceCube and Antares neutrino detectors. A possible joint detection could be used in targeted electromagnetic follow-up observations, given the significantly better angular resolution of neutrino events compared to gravitational waves. We find no neutrino candidates in both temporal and spatial coincidence with the gravitational wave event. Within {$\\pm$}500  s of the gravitational wave event, the number of neutrino candidates detected by IceCube and Antares were three and zero, respectively. This is consistent with the expected atmospheric background, and none of the neutrino candidates were directionally coincident with GW150914. We use this nondetection to constrain neutrino emission from the gravitational-wave event.}\n}\n\n","author_short":["Adrián-Martínez, S.","Abbott, B. P.","Abbott, R.","Abernathy, M. R.","Adhikari, R. X.","Anderson, S. B.","Arai, K.","Araya, M. C.","Barayoga, J. C.","Barish, B. C.","Berger, B. K.","Billingsley, G.","Blackburn, J. K.","Bork, R.","Brooks, A. F.","Cahillane, C.","Callister, T.","Cepeda, C. B.","Chakraborty, R.","Chalermsongsak, T.","Couvares, P.","Coyne, D. C.","Dergachev, V.","Drever, R. W. P.","Ehrens, P.","Etzel, T.","Gossan, S. E.","Gushwa, K. E.","Gustafson, E. K.","Hall, E. D.","Heptonstall, A. W.","Hodge, K. A.","Isi, M.","Kanner, J. B.","Kells, W.","Kondrashov, V.","Korth, W. Z.","Kozak, D. B.","Lazzarini, A.","Li, T. G. F.","Mageswaran, M.","Maros, E.","Martynov, D. V.","Marx, J. N.","McIntyre, G.","McIver, J.","Meshkov, S.","Pedraza, M.","Perreca, A.","Price, L. R.","Quintero, E. A.","Reitze, D. H.","Robertson, N. A.","Rollins, J. G.","Sachdev, S.","Sanchez, E. J.","Schmidt, P.","Shao, Z.","Singer, A.","Smith, N. D.","Smith, R. J. E.","Taylor, R.","Thirugnanasambandam, M. P.","Torres, C. V.","Torrie, C. I.","Vajente, G.","Vass, S.","Wallace, L.","Weinstein, A. J.","Whitcomb, S. E.","Williams, R. D.","Wipf, C. C.","Yamamoto, H.","Zhang, L.","Zucker, M. E.","Zweizig, J.","Chen, Y.","Engels, W.","Ott, C. D.","Thorne, K. S."],"key":"caltechauthors68705","id":"caltechauthors68705","bibbaseid":"adrinmartinez-abbott-abbott-abernathy-adhikari-anderson-arai-araya-etal-highenergyneutrinofollowupsearchofgravitationalwaveeventgw150914withantaresandicecube-2016","role":"author","urls":{"Paper":"http://resolver.caltech.edu/CaltechAUTHORS:20160628-092040474"},"downloads":0,"html":""},"search_terms":["high","energy","neutrino","follow","search","gravitational","wave","event","gw150914","antares","icecube","adrián-martínez","abbott","abbott","abernathy","adhikari","anderson","arai","araya","barayoga","barish","berger","billingsley","blackburn","bork","brooks","cahillane","callister","cepeda","chakraborty","chalermsongsak","couvares","coyne","dergachev","drever","ehrens","etzel","gossan","gushwa","gustafson","hall","heptonstall","hodge","isi","kanner","kells","kondrashov","korth","kozak","lazzarini","li","mageswaran","maros","martynov","marx","mcintyre","mciver","meshkov","pedraza","perreca","price","quintero","reitze","robertson","rollins","sachdev","sanchez","schmidt","shao","singer","smith","smith","taylor","thirugnanasambandam","torres","torrie","vajente","vass","wallace","weinstein","whitcomb","williams","wipf","yamamoto","zhang","zucker","zweizig","chen","engels","ott","thorne"],"keywords":[],"authorIDs":[],"dataSources":["87H4BDEWXjGHR2RTf"]}