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[1]  oai:arXiv.org:astro-ph/9507093  [pdf] - 93031
Beltrami Equation and Cluster Lensing: Characteristic Equations and Applications
Comments: 4 pages latex, 2 figures, uuencoded, compressed tar-file
Submitted: 1995-07-24
Arclets in clusters of galaxies can be used to determine the lens mapping and not only to constrain the mass density of the cluster. Multiply imaged arclets are therefore easily identified without further modelling.