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GW150914: First results from the search for binary black hole coalescence with Advanced LIGO

  • (LIGO Scientific Collaboration and Virgo Collaboration)
  • California Institute of Technology
  • Louisiana State University
  • University of Salerno
  • National Institute for Nuclear Physics
  • University of Florida
  • National Science Foundation
  • Université Savoie Mont Blanc
  • Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
  • National Institute for Subatomic Physics
  • Instituto Nacional de Pesquisas Espaciais
  • Inter-University Centre for Astronomy and Astrophysics India
  • Tata Institute of Fundamental Research
  • University of Wisconsin-Milwaukee
  • Leibniz University Hannover
  • University of Pisa
  • Australian National University
  • University of Mississippi
  • California State University Fullerton
  • Université Paris-Saclay
  • SPIC Science Foundation
  • University of Rome Tor Vergata
  • University of Southampton
  • University of Hamburg
  • Université de Paris
  • Montana State University
  • University of Perugia
  • European Gravitational Observatory
  • Syracuse University
  • University of Glasgow

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

Abstract

On September 14, 2015, at 0950:45 UTC the two detectors of the Laser Interferometer Gravitational-Wave Observatory (LIGO) simultaneously observed the binary black hole merger GW150914. We report the results of a matched-filter search using relativistic models of compact-object binaries that recovered GW150914 as the most significant event during the coincident observations between the two LIGO detectors from September 12 to October 20, 2015 GW150914 was observed with a matched-filter signal-to-noise ratio of 24 and a false alarm rate estimated to be less than 1 event per 203000 years, equivalent to a significance greater than 5.1 σ.

Original languageEnglish
Article number122003
JournalPhysical Review D
Volume93
Issue number12
DOIs
StatePublished - 7 Jun 2016
Externally publishedYes

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