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dc.contributor.authorEric V. Linder-
dc.date.accessioned2016-08-28T10:08:07Z-
dc.date.available2016-08-28T10:08:07Z-
dc.date.issued2013-
dc.identifier.issn1550-7998-
dc.identifier.otherOAK-10198-
dc.identifier.urihttps://dspace.ewha.ac.kr/handle/2015.oak/223810-
dc.description.abstractStrong gravitational lensing of time variable sources such as quasars and supernovae creates observable time delays between the multiple images. Time delays can provide a powerful cosmographic probe through the "time-delay distance" involving the ratio of lens, source, and lens-source distances. However, light curves of lensed images have measurement gaps, noise, systematics such as microlensing from substructure along an image line of sight, and no a priori functional model, making robust time-delay estimation challenging. Using Gaussian process techniques, we demonstrate success in accurate blind reconstruction of time delays and reduction in uncertainties for real data. © 2013 American Physical Society.-
dc.languageEnglish-
dc.titleRobust strong lensing time delay estimation-
dc.typeArticle-
dc.relation.issue12-
dc.relation.volume87-
dc.relation.indexSCIE-
dc.relation.indexSCOPUS-
dc.relation.journaltitlePhysical Review D - Particles, Fields, Gravitation and Cosmology-
dc.identifier.doi10.1103/PhysRevD.87.123512-
dc.identifier.wosidWOS:000320392200002-
dc.identifier.scopusid2-s2.0-84879080512-
dc.author.googleHojjati A.-
dc.author.googleKim A.G.-
dc.author.googleLinder E.V.-
dc.date.modifydate20180104081001-


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