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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1316
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dc.contributor.authorDamour, Thibault-
dc.contributor.authorIyer, B.R.-
dc.contributor.authorSathyaprakash, B.S.-
dc.date.accessioned2006-06-08T06:02:51Z-
dc.date.available2006-06-08T06:02:51Z-
dc.date.issued2000-10-15-
dc.identifier.citationPhysical Review D, 2000, Vol.62, 084036en
dc.identifier.issn1550-2368 (online)-
dc.identifier.issn1550-7998-
dc.identifier.urihttp://hdl.handle.net/2289/1316-
dc.description.abstractFrequency-domain filters for time-windowed gravitational waves from inspiraling compact binaries are constructed which combine the excellent performance of our previously developed time-domain P approximants with the analytic convenience of the stationary phase approximation without a serious loss in event rate. These Fourier-domain representations incorporate the “edge oscillations” due to the (assumed) abrupt shutoff of the time-domain signal caused by the relativistic plunge at the last stable orbit. These new analytic approximations, the SPP approximants, are not only effectual for detection and faithful for parameter estimation, but are also computationally inexpensive to generate (and are faster by factors up to 10, as compared to the corresponding time-domain templates). The SPP approximants should provide data analysts the Fourier-domain templates for massive black hole binaries of total mass m≲40M⊙, the most likely sources for LIGO and VIRGO.en
dc.format.extent429779 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherThe American Physical Societyen
dc.relation.urihttp://link.aps.org/abstract/PRD/v62/e084036en
dc.rights(2000) by the American Physical Societyen
dc.titleFrequency-domain P-approximant filters for time-truncated inspiral gravitational wave signals from compact binariesen
dc.typeArticleen
Appears in Collections:Research Papers (TP)

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