Please use this identifier to cite or link to this item: http://hdl.handle.net/123456789/3371
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dc.contributor.authorMeena, A.K.-
dc.contributor.authorBagla, J.S.-
dc.date.accessioned2020-12-26T05:18:27Z-
dc.date.available2020-12-26T05:18:27Z-
dc.date.issued2020-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society (3), pp. 3294-3305en_US
dc.identifier.otherhttps://doi.org/10.1093/mnras/stz3632-
dc.identifier.urihttps://academic.oup.com/mnras/article/492/3/3294/5695756-
dc.identifier.urihttp://hdl.handle.net/123456789/3371-
dc.description.abstractThe number of strong lens systems is expected to increase significantly in ongoing and upcoming surveys. With an increase in the total number of such systems, we expect to discover many configurations that correspond to unstable caustics. In such cases, the instability can be used to our advantage for constraining the lens model. We have implemented algorithms for detection of different types of singularities in gravitational lensing. We apply our approach on a variety of lens models and then go on to test it with the inferred mass distribution for Abell 697 as an example application. We propose to represent lenses using A3-lines and singular points (A4 and D4) in the image plane. We propose this as a compact representation of complex lens systems that can capture all the details in a single snapshot.en_US
dc.language.isoenen_US
dc.publisherOxford Academicen_US
dc.subjectGravitational lensing: strongen_US
dc.subjectUnstable causticsen_US
dc.subjectSingular pointsen_US
dc.titleFinding singularities in gravitational lensingen_US
dc.typeArticleen_US
Appears in Collections:Research Articles

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