Using generalized PowerFlux methods to estimate the parameters of periodic gravitational waves

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dc.creatorMendell, Gregory
dc.creatorWette, Karl
dc.date2007-10-23
dc.date2008-05-16
dc.date.accessioned2026-07-07T11:38:18Z
dc.date.available2026-07-07T11:38:18Z
dc.descriptionWe investigate methods to estimate the parameters of the gravitational-wave signal from a spinning neutron star using Fourier transformed segments of the strain response from an interferometric detector. Estimating the parameters from the power, we find generalizations of the PowerFlux method. Using simulated elliptically polarized signals injected into Gaussian noise, we apply the generalized methods to estimate the squared amplitudes of the plus and cross polarizations (and, in the most general case, the polarization angle), and test the relative detection efficiencies of the various methods.
dc.description8 pages, presented at Amalid7, Sydney, Australia (July 2007), fixed minor typos and clarified discussion to match published CQG version; updated references
dc.identifierhttps://arxiv.org/abs/0710.4362
dc.identifierhttp://arxiv.org/abs/0710.4362
dc.identifierClass.Quant.Grav.25:114044,2008
dc.identifierdoi:10.1088/0264-9381/25/11/114044
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/199515
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleUsing generalized PowerFlux methods to estimate the parameters of periodic gravitational waves
dc.typetext

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