English

On the Magnfication Relations in Quadruple Lenses: A Moment Approach

Astrophysics 2009-10-31 v1

Abstract

We present a new method of studying quadruple lenses in elliptical power-law potentials parameterized by ψ(x,y)(x2+y2/q2)β/2/β(0β<2)\psi(x,y) \propto (x^2+y^2/q^2)^{\beta/2}/\beta (0 \leq \beta < 2). For this potential, the moments of the four image positions weighted by signed magnifications (magnification times parity) have very simple properties. In particular, we find that the zeroth moment -- the sum of four signed magnifications satisfies 2/(2β)\simeq 2/(2-\beta); the relation is exact for β=0\beta=0 (point-lens) and β=1\beta=1 (isothermal potential), independent of the axial ratio. Similar relations can be derived when a shear is present along the major or minor axes. These relations, however, do not hold well for the closely-related elliptical density distributions. For a singular isothermal elliptical density distribution without shear, the sum of signed magnifications for quadruple lenses is 2.8\approx 2.8, again nearly independent of the ellipticity. For the same distribution with shear, the total signed magnification is around 2-3 for most cases, but can be significantly different for some combinations of the axial ratio and shear where more than four images can appear.

Keywords

Cite

@article{arxiv.astro-ph/9906323,
  title  = {On the Magnfication Relations in Quadruple Lenses: A Moment Approach},
  author = {Hans J. Witt and Shude Mao},
  journal= {arXiv preprint arXiv:astro-ph/9906323},
  year   = {2009}
}

Comments

16 pages, 4 figures, submitted to MNRAS