The Chang-Refsdal lens revisited

• Published in: Monthly notices of the Royal Astronomical Society 2006-06, Vol.369 (1), p.317-334
• Main Authors: An, Jin H., Evans, N. Wyn
• Format: Article
• Language: English
• Subjects: Astronomy; Earth, ocean, space; Exact sciences and technology; gravitational lensing; methods: analytical; Optics; Telescopes
• ISSN: 0035-8711; 1365-2966
• DOI: 10.1111/j.1365-2966.2006.10303.x

This paper provides a complete theoretical treatment of the point-mass lens perturbed by constant external shear, often called the Chang-Refsdal lens. We show that simple invariants exist for the products of the (complex) positions of the four images, as well as moment sums of their signed magnifications. The image topographies and equations of the caustics and critical curves are also studied. We derive the fully analytic expressions for pre-caustics, which are the loci of non-critical points that map to the caustics under the lens mapping. They constitute boundaries of the region in the image domain that maps on to the interior of the caustics. The areas under the critical curves, caustics and pre-caustics are all evaluated, which enables us to calculate the mean magnification of the source within the caustics. Additionally, the exact analytic expression for the magnification distribution for the source in the triangular caustics is derived, as well as a useful approximate expression. Finally, we find that the Chang-Refsdal lens with additional convergence greater than unity (the 'overfocusing case') can exhibit third-order critical behaviour, if the 'reduced shear' is exactly equal to , and that the number of images for N-point masses with non-zero constant shear cannot be greater than 5N− 1.