Maximum-Entropy Reconstruction of the Distribution of Mass in Cluster MS1054-03 from Weak Lensing Data

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dc.creatorMarshall, P. J.
dc.date2001-06-01
dc.date.accessioned2026-07-07T01:58:46Z
dc.date.available2026-07-07T01:58:46Z
dc.descriptionWeak gravitational lensing studies of clusters of galaxies provide complimentary information to that from X-ray data; the measured signal depends only on the cluster's projected mass, independent of dynamical assumptions. Here we apply a maximum-entropy method algorithm for reconstructing the two-dimensional density distribution to two sets of shear data for the high redshift cluster MS1054-03, courtesy of Clowe et al (2000) and Hoekstra et al (2000).
dc.description6 pages, with 11 bitmapped postscript figures. To appear in Proceedings of XXI Moriond Conference: Galaxy Clusters and the High Redshift Universe Observed in X-rays, edited by D. Neumann, F. Durret, & J. Tran Thanh Van. A version with uncompressed colour figures is available from http://www.mrao.cam.ac.uk/~pjm43/papers/
dc.identifierhttps://arxiv.org/abs/astro-ph/0106025
dc.identifierhttp://arxiv.org/abs/astro-ph/0106025
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2847
dc.subjectAstrophysics
dc.titleMaximum-Entropy Reconstruction of the Distribution of Mass in Cluster MS1054-03 from Weak Lensing Data
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