First upper limits from LIGO on gravitational wave bursts

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

Research output: Contribution to journalArticle

100 Citations (Scopus)

Abstract

We report on a search for gravitational wave bursts using data from the first science run of the Laser Interferometer Gravitational Wave Observatory (LIGO) detectors. Our search focuses on bursts with durations ranging from 4 to 100 ms, and with significant power in the LIGO sensitivity band of 150 to 3000 Hz. We bound the rate for such detected bursts at less than 1.6 events per day at a 90% confidence level. This result is interpreted in terms of the detection efficiency for ad hoc waveforms (Gaussians and sine Gaussians) as a function of their root-sum-square strain hrss; typical sensitivities lie in the range hrss∼10−19–10−17strain/√Hz, depending on the waveform. We discuss improvements in the search method that will be applied to future science data from LIGO and other gravitational wave detectors.
LanguageEnglish
Article number102001
Number of pages21
JournalPhysical Review D
Volume69
Issue number10
DOIs
Publication statusPublished - 15 May 2004

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LIGO (observatory)
gravitational waves
bursts
waveforms
sensitivity
detectors
confidence

Keywords

  • gravitational waves
  • LIGO
  • interferometric detection

Cite this

Abbott, B. ; Cantley, C.A. ; LIGO Scientific Collaboration. / First upper limits from LIGO on gravitational wave bursts. In: Physical Review D. 2004 ; Vol. 69, No. 10.
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First upper limits from LIGO on gravitational wave bursts. / Abbott, B.; Cantley, C.A.; LIGO Scientific Collaboration.

In: Physical Review D, Vol. 69, No. 10, 102001, 15.05.2004.

Research output: Contribution to journalArticle

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