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Fast Calculation of Gravitational Lensing Properties of Elliptical Navarro-Frenk-White and Hernquist Density Profiles

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arxiv 2106.11464 v2 pith:PH2YYBKI submitted 2021-06-22 astro-ph.IM astro-ph.GA

classification astro-ph.IMastro-ph.GA
keywords densityellipticalgravitationallensingprofilespropertiesapproachcalculation
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abstract

We present a new approach for fast calculation of gravitational lensing properties, including the lens potential, deflection angles, convergence, and shear, of elliptical Navarro-Frenk-White (NFW) and Hernquist density profiles, by approximating them by superpositions of elliptical density profiles for which simple analytic expressions of gravitational lensing properties are available. This model achieves high fractional accuracy better than $10^{-4}$ in the range of the radius normalized by the scale radius of $10^{-4}-10^3$. These new approximations are $\sim 300$ times faster in solving the lens equation for a point source compared with the traditional approach resorting to expensive numerical integrations, and are implemented in {\tt glafic} software.

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  1. Lambda as a Probe of Lensing Consistency

    astro-ph.CO 2026-07 conditional novelty 6.0 of 10

    Spatially resolved λ(r) from the mass-sheet degeneracy quantifies the radial transition in reliability between strong and weak lensing mass reconstructions of galaxy clusters.

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