Please use this identifier to cite or link to this item: http://hdl.handle.net/123456789/4448
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dc.contributor.authorMeena, Ashish Kumar-
dc.contributor.authorBagla, Jasjeet Singh-
dc.date.accessioned2023-08-10T09:36:13Z-
dc.date.available2023-08-10T09:36:13Z-
dc.date.issued2022-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 515(3), 4151-4160.en_US
dc.identifier.urihttps://doi.org/10.1093/mnras/stac1080-
dc.identifier.urihttp://hdl.handle.net/123456789/4448-
dc.descriptionOnly IISER Mohali authors are available in the record.en_US
dc.description.abstractWe study the image formation near point singularities (swallowtail and umbilics) in the simulated strongly lensed images of Hubble Ultra Deep Field (HUDF) by the Hubble Frontier Fields (HFF) clusters. In this work, we only consider nearly half of the brightest (a total of 5271) sources in the HUDF region. For every HFF cluster, we constructed 11 realizations of strongly lensed HUDF with an arbitrary translation of the cluster centre within the central region of HUDF and an arbitrary rotation. In each of these realizations, we visually identify the characteristic/exotic image formation corresponding to the different point singularities. We find that our current results are consistent with our earlier results based on different approaches. We also study time delay in these exotic image formations and compare it with typical five-image geometries. We find that the typical time delay in exotic image formations is an order of magnitude smaller than the typical time delay in a generic five-image geometry.en_US
dc.language.isoen_USen_US
dc.publisherOxford Academicen_US
dc.subjectExotic imageen_US
dc.subjectstrong gravitationalen_US
dc.subjectclusters of galaxiesen_US
dc.subjectHUDFen_US
dc.titleExotic image formation in strong gravitational lensing by clusters of galaxies – III. Statistics with HUDFen_US
dc.typeArticleen_US
Appears in Collections:Research Articles

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