1995/07/24 by Schramm, T
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9507093
4 pages latex, 2 figures, uuencoded, compressed tar-file
arxiv created 1995/07/24 · arxiv updated 2009/12/01
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.