Analysis of LIGO data for gravitational waves from binary neutron stars

B. Abbott, C.A. Cantley, LIGO Scientific Collaboration

Research output: Contribution to journalArticle

97 Citations (Scopus)

Abstract

We report on a search for gravitational waves from coalescing compact binary systems in the Milky Way and the Magellanic Clouds. The analysis uses data taken by two of the three LIGO interferometers during the first LIGO science run and illustrates a method of setting upper limits on inspiral event rates using interferometer data. The analysis pipeline is described with particular attention to data selection and coincidence between the two interferometers. We establish an observational upper limit of R<1.7×102 per year per Milky Way Equivalent Galaxy (MWEG), with 90% confidence, on the coalescence rate of binary systems in which each component has a mass in the range 1–3M⊙.
LanguageEnglish
Article number122001
Number of pages16
JournalPhysical Review D
Volume69
Issue number12
DOIs
Publication statusPublished - 15 Jun 2004

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LIGO (observatory)
binary stars
gravitational waves
neutron stars
interferometers
coalescing
Magellanic clouds
confidence
galaxies

Keywords

  • Milky Way Equivalent Galaxy
  • gravitational waves
  • binary systems
  • Milky Way

Cite this

Abbott, B. ; Cantley, C.A. ; LIGO Scientific Collaboration. / Analysis of LIGO data for gravitational waves from binary neutron stars. In: Physical Review D. 2004 ; Vol. 69, No. 12.
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Analysis of LIGO data for gravitational waves from binary neutron stars. / Abbott, B.; Cantley, C.A.; LIGO Scientific Collaboration.

In: Physical Review D, Vol. 69, No. 12, 122001, 15.06.2004.

Research output: Contribution to journalArticle

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AU - LIGO Scientific Collaboration

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KW - Milky Way Equivalent Galaxy

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