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First upper limits from LIGO on gravitational wave bursts

Alan J Weinstein (for the LIGO Scientific Collaboration)

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We report on a search for gravitational wave bursts using data from the first science run of the LIGO detectors. We focus on bursts with durations ranging from 4 ms 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 90% confidence level. This result is interpreted in terms of the detection efficiency for ad hoc wave forms (Gaussians and sine-Gaussians) as a function of their root-sum-square strain hrss; typical sensitivities lie in the range h_{\rm rss} \sim 10^{-19}\hbox{--} 10^{-17} \,{\rm strain}/\sqrt{\rm Hz} , depending on wave form. We discuss improvements in the search method that will be applied to future science data from LIGO and other gravitational wave detectors.


PACS

04.80.Nn Gravitational wave detectors and experiments

07.05.Kf Data analysis: algorithms and implementation; data management

95.30.Sf Relativity and gravitation

MSC

83C35 Gravitational waves

Subjects

Instrumentation and measurement

Gravitation and cosmology

Astrophysics and astroparticles

Dates

Issue 5 (7 March 2004)

Received 2 September 2003

Published 9 February 2004



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