Coherent network analysis for triggered gravitational wave burst searches

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dc.creatorHayama, Kazuhiro
dc.creatorMohanty, Soumya D.
dc.creatorRakhmanov, Malik
dc.creatorDesai, Shantanu
dc.date2007-09-06
dc.date.accessioned2026-07-07T11:42:17Z
dc.date.available2026-07-07T11:42:17Z
dc.descriptionSearches for gravitational wave bursts that are triggered by the observation of astronomical events require a different mode of analysis than all-sky, blind searches. For one, much more prior information is usually available in a triggered search which can and should be used in the analysis. Second, since the data volume is usually small in a triggered search, it is also possible to use computationally more expensive algorithms for tasks such as data pre-processing that can consume significant computing resources in a high data-volume un-triggered search. From the statistical point of view, the reduction in the parameter space search volume leads to higher sensitivity than an un-triggered search. We describe here a data analysis pipeline for triggered searches, called {\tt RIDGE}, and present preliminary results for simulated noise and signals.
dc.descriptionto appear on Classical & Quantum Gravity
dc.identifierhttps://arxiv.org/abs/0709.0940
dc.identifierhttp://arxiv.org/abs/0709.0940
dc.identifierClass.Quant.Grav.24:S681-S688,2007
dc.identifierdoi:10.1088/0264-9381/24/19/S30
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/200834
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleCoherent network analysis for triggered gravitational wave burst searches
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