Abstract
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 modeling.
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Schramm, T. & Kayser, R. 1995, A&A, 299, 1
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© 1996 International Astronomical Union
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Schramm, T. (1996). Beltrami Equation and Cluster Lensing. In: Kochanek, C.S., Hewitt, J.N. (eds) Astrophysical Applications of Gravitational Lensing. International Astronomical Union / Union Astronomique Internationale, vol 173. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0221-3_41
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DOI: https://doi.org/10.1007/978-94-009-0221-3_41
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