Search for gravitational wave bursts in LIGO's third science run
LIGO Scientific Collaboration
TL;DR
This paper details a search for unmodeled gravitational wave bursts in LIGO's third science run data, achieving high sensitivity but detecting no signals in 8 days of observation.
Contribution
It presents a search methodology for unmodeled gravitational wave bursts in LIGO data with improved sensitivity during the third science run.
Findings
No gravitational wave bursts detected in the analyzed data
Set upper limits on burst event rates
Demonstrated the effectiveness of the search pipeline
Abstract
We report on a search for gravitational wave bursts in data from the three LIGO interferometric detectors during their third science run. The search targets subsecond bursts in the frequency range 100-1100 Hz for which no waveform model is assumed, and has a sensitivity in terms of the root-sum-square (rss) strain amplitude of hrss ~ 10^{-20} / sqrt(Hz). No gravitational wave signals were detected in the 8 days of analyzed data.
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