A $χ^2$ veto for continuous gravitational wave searches

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dc.creatorde la Jordana, Llucia Sancho
dc.creatorSintes, Alicia M.
dc.date2008-04-07
dc.date2009-02-27
dc.date.accessioned2026-07-07T12:49:42Z
dc.date.available2026-07-07T12:49:42Z
dc.description$χ^2$ vetoes are commonly used in searching for gravitational waves, in particular for broad-band signals, but they can also be applied to narrow-band continuous wave signals, such as those expected from rapidly rotating neutron stars. In this paper we present a $χ^2$ veto adapted to the Hough transform searches for continuous gravitational wave signals; we characterize the $χ^2$-significance plane for different frequency bands; and discuss the expected performance of this veto in LIGO analysis.
dc.descriptionFinal version, 12th Gravitational Waves Data Analysis Workshop
dc.identifierhttps://arxiv.org/abs/0804.1007
dc.identifierhttp://arxiv.org/abs/0804.1007
dc.identifierClass.Quant.Grav.25:184014,2008
dc.identifierdoi:10.1088/0264-9381/25/18/184014
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/222465
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleA $χ^2$ veto for continuous gravitational wave searches
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