Weak Gravitational Lensing: Current Status and Future Prospects

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dc.creatorKaiser, Nick
dc.date1995-09-05
dc.date.accessioned2026-07-07T02:20:07Z
dc.date.available2026-07-07T02:20:07Z
dc.descriptionIn this review I will describe progress that has been made in determining masses of galaxy clusters using `weak lensing' and how this technique my be applied in the future to determine the dark matter distribution both on supercluster scales and on the scale of galaxy haloes.
dc.descriptionplain latex; 15 pages; 6 postscript figures
dc.identifierhttps://arxiv.org/abs/astro-ph/9509019
dc.identifierhttp://arxiv.org/abs/astro-ph/9509019
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10113
dc.subjectAstrophysics
dc.titleWeak Gravitational Lensing: Current Status and Future Prospects
dc.typetext

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