Weak Lensing Observations of High-Redshift Clusters of Galaxies

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dc.creatorClowe, D.
dc.creatorLuppino, G.
dc.creatorKaiser, N.
dc.creatorGioia, I.
dc.date1999-11-10
dc.date.accessioned2026-07-07T02:34:19Z
dc.date.available2026-07-07T02:34:19Z
dc.descriptionWe present results of a weak gravitational lensing survey of six X-ray selected high-redshift clusters of galaxies. We find that the masses of the clusters derived from weak lensing are comparable to those derived from the X-ray observations. We show that many of the clusters have significant substructure not observed in the X-ray observations and that for the more massive clusters a singular isothermal sphere does not provide a good fit to the radial mass profile.
dc.description5 pages, 1 figure, to be published in ASP Conference Series: Proceedings of Clustering at High Redshift, Les Rencontres Internationales de l'IGRAP
dc.identifierhttps://arxiv.org/abs/astro-ph/9911169
dc.identifierhttp://arxiv.org/abs/astro-ph/9911169
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15196
dc.subjectAstrophysics
dc.titleWeak Lensing Observations of High-Redshift Clusters of Galaxies
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