Abstract
The lens equation, derived in Chap. 4 and discussed in some detail in the previous chapter, defines a surjective mapping \( f:{{\mathbb{R}}^{2}} \to {{\mathbb{R}}^{2}},x \mapsto y \) from the lens plane to the source plane. We assume here that it is differentiable as often as is needed. If \( {{y}^{{(0)}}} = f({\text{ }}{{x}^{{(0)}}}) \) is the image of x (0)) and if the Jacobian D = det A of the derivative \( A = \frac{{\partial y}}{{\partial x}} = \frac{{\partial ({\text{ }}{{y}_{1}},{\text{ }}{{y}_{2}})}}{{\partial ({\text{ }}{{x}_{1}},{\text{ }}{{x}_{2}})}} \) of does not vanish at x(0), there exist neighborhoods of and on which f is bijective, i.e., the lens mapping is locally invertible. For an infinitesimal displacement dy of the source, the corresponding image position in the lens plane changes by \( dx = {{A}^{{ - 1}}}({{x}^{{(0)}}})dy. \)
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© 1992 Springer-Verlag New York Inc.
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Schneider, P., Ehlers, J., Falco, E.E. (1992). Lensing near critical points. In: Gravitational Lenses. Astronomy and Astrophysics Library. Springer, New York, NY. https://doi.org/10.1007/978-1-4612-2756-4_6
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DOI: https://doi.org/10.1007/978-1-4612-2756-4_6
Publisher Name: Springer, New York, NY
Print ISBN: 978-1-4612-7655-5
Online ISBN: 978-1-4612-2756-4
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