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Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/48814
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dc.contributor.authorAbbott, B.-
dc.contributor.authorAbbott, R.-
dc.contributor.authorAdhikari, R.-
dc.contributor.authorAgresti, J.-
dc.contributor.authorAjith, P.-
dc.contributor.authorAllen, B.-
dc.contributor.authorAllen, G.-
dc.contributor.authorAmin, R.-
dc.contributor.authorAnderson, S.-
dc.contributor.authorAnderson, W.-
dc.contributor.authorAraya, M.-
dc.contributor.authorArmandula, H.-
dc.contributor.authorAshley, M.-
dc.contributor.authorAulbert, C.-
dc.contributor.authorBabak, S.-
dc.contributor.authorBalasubramanian, R.-
dc.contributor.authorBallmer, S.-
dc.contributor.authorBantilan, H.-
dc.contributor.authorBarish, B.-
dc.contributor.authorBarker, C.-
dc.contributor.authoret al.-
dc.date.issued2006-
dc.identifier.citationClassical and Quantum Gravity, 2006; 23(8 Special Issue S1):S29-S39-
dc.identifier.issn0264-9381-
dc.identifier.issn1361-6382-
dc.identifier.urihttp://hdl.handle.net/2440/48814-
dc.description.abstractWe report on a search for gravitational-wave bursts in data from the three LIGO interferometric detectors during their third science run. The search targets sub-second 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 Hz−1/2. No gravitational-wave signals were detected in the eight days of analysed data.-
dc.description.statementofresponsibilityB. Abbott...D. Ottaway...et al., LIGO Scientific Collaboration-
dc.language.isoen-
dc.publisherIOP Publishing Ltd-
dc.rights© 2006 IOP Publishing-
dc.source.urihttp://dx.doi.org/10.1088/0264-9381/23/8/s05-
dc.titleSearch for gravitational-wave bursts in LIGO's third science run-
dc.typeJournal article-
dc.identifier.doi10.1088/0264-9381/23/8/S05-
pubs.publication-statusPublished-
dc.identifier.orcidOttaway, D. [0000-0001-6794-1591]-
Appears in Collections:Aurora harvest
Physics publications

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