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Fast Calculation of a Family of Elliptical Gravitational Lens Models

  • Authors: Rennan Barkana

Barkana 1998 The Astrophysical Journal 502 531.

  • Provider: AAS Journals

Caption: Fig. 3.

Properties of the four images of a source placed directly behind the lens center, for SPEMDs and corresponding SPEPs. Several different power‐law indices η are considered. Left: Distance y of the images on the y‐axis over the distance x of the images on the x‐axis. Right: Magnification ratio Ay/Ax of the two types of images. In each case the appropriate quantity is plotted as a function of ellipticity, with the SPEMD as the solid curve and the SPEP as the dashed curve.

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