Details
| Originalsprache | Englisch |
|---|---|
| Aufsatznummer | 134 |
| Fachzeitschrift | Astrophysical Journal |
| Jahrgang | 870 |
| Ausgabenummer | 2 |
| Publikationsstatus | Veröffentlicht - 16 Jan. 2019 |
ASJC Scopus Sachgebiete
- Physik und Astronomie (insg.)
- Astronomie und Astrophysik
- Erdkunde und Planetologie (insg.)
- Astronomie und Planetologie
Zitieren
- Standard
- Harvard
- Apa
- Vancouver
- BibTex
- RIS
in: Astrophysical Journal, Jahrgang 870, Nr. 2, 134, 16.01.2019.
Publikation: Beitrag in Fachzeitschrift › Artikel › Forschung › Peer-Review
}
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 -