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First upper limits from LIGO on gravitational wave bursts

Cusack, B J; McClelland, David; Scott, Susan M; Searle, Antony; Weinstein, A

Description

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...[Show more]

dc.contributor.authorCusack, B J
dc.contributor.authorMcClelland, David
dc.contributor.authorScott, Susan M
dc.contributor.authorSearle, Antony
dc.contributor.authorWeinstein, A
dc.date.accessioned2015-12-13T22:56:27Z
dc.date.available2015-12-13T22:56:27Z
dc.identifier.issn0264-9381
dc.identifier.urihttp://hdl.handle.net/1885/82802
dc.description.abstractWe 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 ∼ 10-19-10-17 strain/ √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.
dc.publisherInstitute of Physics Publishing
dc.sourceClassical and Quantum Gravity
dc.titleFirst upper limits from LIGO on gravitational wave bursts
dc.typeJournal article
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.citationvolume21
dc.date.issued2004
local.identifier.absfor029904 - Synchrotrons; Accelerators; Instruments and Techniques
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub11005
local.type.statusPublished Version
local.contributor.affiliationCusack, B J, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationMcClelland, David, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationScott, Susan M, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationSearle, Antony, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationWeinstein, A, California Institute of Technology
local.bibliographicCitation.issue2004
local.bibliographicCitation.startpageS677
local.bibliographicCitation.lastpageS684
local.identifier.doi10.1103/PhysRevD.69.102001
dc.date.updated2015-12-11T11:15:38Z
local.identifier.scopusID2-s2.0-24644447693
CollectionsANU Research Publications

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