UPPER LIMITS on the RATES of BINARY NEUTRON STAR and NEUTRON STAR-BLACK HOLE MERGERS from ADVANCED LIGO'S FIRST OBSERVING RUN

Research output: Contribution to journalArticleResearchpeer review

Authors

  • The LIGO Scientific Collaboration
  • The Virgo Collaboration
  • B. Allen
  • Karsten Danzmann
  • Michele Heurs
  • Harald Lück
  • Daniel Steinmeyer
  • Henning Fedor Cornelius Vahlbruch
  • Benno Willke
  • Holger Wittel
  • Peter Aufmuth
  • A. Bisht
  • Stefan Kaufer
  • Christian Krüger
  • J. D. Lough
  • A. Sawadsky
  • Aditya Singh Mehra

External Research Organisations

  • California Institute of Caltech (Caltech)
  • Louisiana State University
  • American University Washington DC
  • Universita di Salerno
  • Monte S. Angelo University Federico II
  • University of Florida
  • Universite de Savoie
  • University of Sannio
  • Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
  • National Institute for Subatomic Physics (Nikhef)
  • LIGO Laboratory
  • Instituto Nacional de Pesquisas Espaciais
  • Istituto Nazionale di Fisica Nucleare (INFN)
  • Inter-University Centre for Astronomy and Astrophysics India
  • Tata Institute of Fundamental Research (TIFR HYD)
  • University of Wisconsin Milwaukee
  • University of Pisa
  • Sezione di Pisa
  • Australian National University
  • Carson College of Business
  • University of Birmingham
  • University of Glasgow
  • Seoul National University
  • University of Melbourne
  • Tsinghua University
  • University of Western Australia
  • Observatoire Côte d'Azur
  • Rochester Institute of Technology
  • Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA)
  • Northwestern University
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Details

Original languageEnglish
Article numberL21
JournalAstrophysical Journal Letters
Volume832
Issue number2
Publication statusPublished - 23 Nov 2016

Keywords

    binaries: general, gamma-ray burst: general, gravitational waves, stars: black holes, stars: neutron

ASJC Scopus subject areas

Cite this

UPPER LIMITS on the RATES of BINARY NEUTRON STAR and NEUTRON STAR-BLACK HOLE MERGERS from ADVANCED LIGO'S FIRST OBSERVING RUN. / The LIGO Scientific Collaboration; The Virgo Collaboration; Allen, B. et al.
In: Astrophysical Journal Letters, Vol. 832, No. 2, L21, 23.11.2016.

Research output: Contribution to journalArticleResearchpeer review

The LIGO Scientific Collaboration, The Virgo Collaboration, Allen, B, Danzmann, K, Heurs, M, Lück, H, Steinmeyer, D, Vahlbruch, HFC, Willke, B, Wittel, H, Aufmuth, P, Bisht, A, Kaufer, S, Krüger, C, Lough, JD, Sawadsky, A & Singh Mehra, A 2016, 'UPPER LIMITS on the RATES of BINARY NEUTRON STAR and NEUTRON STAR-BLACK HOLE MERGERS from ADVANCED LIGO'S FIRST OBSERVING RUN', Astrophysical Journal Letters, vol. 832, no. 2, L21. https://doi.org/10.3847/2041-8205/832/2/L21
The LIGO Scientific Collaboration, The Virgo Collaboration, Allen, B., Danzmann, K., Heurs, M., Lück, H., Steinmeyer, D., Vahlbruch, H. F. C., Willke, B., Wittel, H., Aufmuth, P., Bisht, A., Kaufer, S., Krüger, C., Lough, J. D., Sawadsky, A., & Singh Mehra, A. (2016). UPPER LIMITS on the RATES of BINARY NEUTRON STAR and NEUTRON STAR-BLACK HOLE MERGERS from ADVANCED LIGO'S FIRST OBSERVING RUN. Astrophysical Journal Letters, 832(2), Article L21. https://doi.org/10.3847/2041-8205/832/2/L21
The LIGO Scientific Collaboration, The Virgo Collaboration, Allen B, Danzmann K, Heurs M, Lück H et al. UPPER LIMITS on the RATES of BINARY NEUTRON STAR and NEUTRON STAR-BLACK HOLE MERGERS from ADVANCED LIGO'S FIRST OBSERVING RUN. Astrophysical Journal Letters. 2016 Nov 23;832(2):L21. doi: 10.3847/2041-8205/832/2/L21
The LIGO Scientific Collaboration ; The Virgo Collaboration ; Allen, B. et al. / UPPER LIMITS on the RATES of BINARY NEUTRON STAR and NEUTRON STAR-BLACK HOLE MERGERS from ADVANCED LIGO'S FIRST OBSERVING RUN. In: Astrophysical Journal Letters. 2016 ; Vol. 832, No. 2.
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title = "UPPER LIMITS on the RATES of BINARY NEUTRON STAR and NEUTRON STAR-BLACK HOLE MERGERS from ADVANCED LIGO'S FIRST OBSERVING RUN",
keywords = "binaries: general, gamma-ray burst: general, gravitational waves, stars: black holes, stars: neutron",
author = "{The LIGO Scientific Collaboration} and {The Virgo Collaboration} and Abbott, {B. P.} and R. Abbott and Abbott, {T. D.} and Abernathy, {M. R.} 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. Agathos and K. Agatsuma and N. Aggarwal and Aguiar, {O. D.} and L. Aiello and A. Ain and P. Ajith and B. Allen and A. Allocca and Altin, {P. A.} and S. Bose and Brown, {D. D.} and Y. Chen and Danilishin, {S. L.} and Karsten Danzmann and Hanke, {M. M.} and J. Hennig and Michele Heurs and Lee, {H. M.} and Harald L{\"u}ck and Nguyen, {T. T.} and J. Schmidt and M. Shaltev and Daniel Steinmeyer and L. Sun and Vahlbruch, {Henning Fedor Cornelius} and M. Wang and X. Wang and Y. Wang and Wei, {L. W.} and Benno Willke and Holger Wittel and L. Zhang and Y. Zhang and M. Zhou and Peter Aufmuth and A. Bisht and Stefan Kaufer and Christian Kr{\"u}ger and Lough, {J. D.} and A. Sawadsky and {Singh Mehra}, Aditya",
note = "Funding information: 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 and Engineering Research Board (SERB), India, Ministry of Human Resource Development, India, the Spanish Ministerio de Economia y Competitividad, the Conselleria d'Economia i Competitivitat and Conselleria d'Educacio 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, Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP), 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.",
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month = nov,
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doi = "10.3847/2041-8205/832/2/L21",
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T1 - UPPER LIMITS on the RATES of BINARY NEUTRON STAR and NEUTRON STAR-BLACK HOLE MERGERS from ADVANCED LIGO'S FIRST OBSERVING RUN

AU - The LIGO Scientific Collaboration

AU - The Virgo Collaboration

AU - Abbott, B. P.

AU - Abbott, R.

AU - Abbott, T. D.

AU - Abernathy, M. R.

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 - 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 - Allocca, A.

AU - Altin, P. A.

AU - Bose, S.

AU - Brown, D. D.

AU - Chen, Y.

AU - Danilishin, S. L.

AU - Danzmann, Karsten

AU - Hanke, M. M.

AU - Hennig, J.

AU - Heurs, Michele

AU - Lee, H. M.

AU - Lück, Harald

AU - Nguyen, T. T.

AU - Schmidt, J.

AU - Shaltev, M.

AU - Steinmeyer, Daniel

AU - Sun, L.

AU - Vahlbruch, Henning Fedor Cornelius

AU - Wang, M.

AU - Wang, X.

AU - Wang, Y.

AU - Wei, L. W.

AU - Willke, Benno

AU - Wittel, Holger

AU - Zhang, L.

AU - Zhang, Y.

AU - Zhou, M.

AU - Aufmuth, Peter

AU - Bisht, A.

AU - Kaufer, Stefan

AU - Krüger, Christian

AU - Lough, J. D.

AU - Sawadsky, A.

AU - Singh Mehra, Aditya

N1 - Funding information: 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 and Engineering Research Board (SERB), India, Ministry of Human Resource Development, India, the Spanish Ministerio de Economia y Competitividad, the Conselleria d'Economia i Competitivitat and Conselleria d'Educacio 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, Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP), 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.

PY - 2016/11/23

Y1 - 2016/11/23

KW - binaries: general

KW - gamma-ray burst: general

KW - gravitational waves

KW - stars: black holes

KW - stars: neutron

UR - http://www.scopus.com/inward/record.url?scp=85000399268&partnerID=8YFLogxK

U2 - 10.3847/2041-8205/832/2/L21

DO - 10.3847/2041-8205/832/2/L21

M3 - Article

AN - SCOPUS:85000399268

VL - 832

JO - Astrophysical Journal Letters

JF - Astrophysical Journal Letters

SN - 2041-8205

IS - 2

M1 - L21

ER -

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