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Implementing a semicoherent search for continuous gravitational waves using optimally constructed template banks

Wette, Karl; Walsh, S; Prix, R; Papa, M

Description

All-sky surveys for isolated continuous gravitational waves present a significant data-analysis challenge. Semicoherent search methods are commonly used to efficiently perform the computationally-intensive task of searching for these weak signals in the noisy data of gravitational-wave detectors such as LIGO and Virgo. We present a new implementation of a semicoherent search method, weave, that for the first time makes full use of a parameter-space metric to generate banks of search templates...[Show more]

dc.contributor.authorWette, Karl
dc.contributor.authorWalsh, S
dc.contributor.authorPrix, R
dc.contributor.authorPapa, M
dc.date.accessioned2019-09-24T06:14:05Z
dc.date.available2019-09-24T06:14:05Z
dc.identifier.issn2470-0010
dc.identifier.urihttp://hdl.handle.net/1885/170692
dc.description.abstractAll-sky surveys for isolated continuous gravitational waves present a significant data-analysis challenge. Semicoherent search methods are commonly used to efficiently perform the computationally-intensive task of searching for these weak signals in the noisy data of gravitational-wave detectors such as LIGO and Virgo. We present a new implementation of a semicoherent search method, weave, that for the first time makes full use of a parameter-space metric to generate banks of search templates at the correct resolution, combined with optimal lattices to minimize the required number of templates and hence the computational cost of the search. We describe the implementation of weave and associated design choices and characterize its behavior using semianalytic models.
dc.description.sponsorshipK. W. is supported by ARC Grant No. CE170100004
dc.format.mimetypeapplication/pdf
dc.language.isoen_AU
dc.publisherAmerican Physical Society
dc.rights© 2018 American Physical Society
dc.sourcePhysical Review D
dc.titleImplementing a semicoherent search for continuous gravitational waves using optimally constructed template banks
dc.typeJournal article
local.description.notesImported from ARIES
local.identifier.citationvolume97
dc.date.issued2018
local.identifier.absfor020105 - General Relativity and Gravitational Waves
local.identifier.ariespublicationu4485658xPUB1893
local.publisher.urlhttps://www.aps.org/
local.type.statusPublished Version
local.contributor.affiliationWette, Karl, College of Science, ANU
local.contributor.affiliationWalsh, S, University of Wisconsin
local.contributor.affiliationPrix, R, Max Planck Institute
local.contributor.affiliationPapa, M, Max Planck Institute for Gravitational Physics
dc.relationhttp://purl.org/au-research/grants/arc/CE170100004
local.bibliographicCitation.startpage123016-1
local.bibliographicCitation.lastpage123016-17
local.identifier.doi10.1103/PhysRevD.97.123016
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciences
dc.date.updated2019-03-12T07:31:34Z
local.identifier.scopusID2-s2.0-85049498660
local.identifier.thomsonID000436629300003
dcterms.accessRightsOpen Access
dc.provenancehttp://sherpa.ac.uk/romeo/issn/2470-0010/..."author can archive publisher's version/PDF" from SHERPA/RoMEO site (as at 24/09/19).
CollectionsANU Research Publications

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