Convenient filtering techniques for LIGO strain of the GW150914 event

dc.creatorMoreschi, Osvaldo Mario
dc.date.accessioned2021-02-12T20:43:36Z
dc.date.accessioned2022-10-15T14:12:11Z
dc.date.available2021-02-12T20:43:36Z
dc.date.available2022-10-15T14:12:11Z
dc.date.created2021-02-12T20:43:36Z
dc.date.issued2019-04-18
dc.identifierMoreschi, Osvaldo Mario; Convenient filtering techniques for LIGO strain of the GW150914 event; IOP Publishing; Journal of Cosmology and Astroparticle Physics; 2019; 4; 18-4-2019; 1-18
dc.identifier1475-7516
dc.identifierhttp://hdl.handle.net/11336/125661
dc.identifierCONICET Digital
dc.identifierCONICET
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4395389
dc.description.abstractWe present a new strategy for the pre-processing filtering techniques of the LIGO strain of the GW150914 [1,2] event that intends to extract as much physical information as possible, minimizing the use of prior assumptions, and avoiding intense deformations of the astrophysical signal. The new techniques allow us to reveal more low frequency signal at earlier times, that it has been overlooked.
dc.languageeng
dc.publisherIOP Publishing
dc.relationinfo:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1903.00546
dc.relationinfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/1475-7516/2019/04/032
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1088/1475-7516/2019/04/032
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/restrictedAccess
dc.subjectGRAVITATIONAL WAVE DETECTORS
dc.subjectGRAVITATIONAL WAVES/EXPERIMENTS
dc.titleConvenient filtering techniques for LIGO strain of the GW150914 event
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:ar-repo/semantics/artículo
dc.typeinfo:eu-repo/semantics/publishedVersion


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