On the accuracy of the Perturbative Approach for Strong Lensing: Local Distortion for Pseudo-Elliptical Models
arXiv:1301.0060 · doi:10.1093/mnras/stt938
Abstract
The Perturbative Approach (PA) introduced by \citet{alard07} provides analytic solutions for gravitational arcs by solving the lens equation linearized around the Einstein ring solution. This is a powerful method for lens inversion and simulations in that it can be used, in principle, for generic lens models. In this paper we aim to quantify the domain of validity of this method for three quantities derived from the linearized mapping: caustics, critical curves, and the deformation cross section (i.e. the arc cross section in the infinitesimal circular source approximation). We consider lens models with elliptical potentials, in particular the Singular Isothermal Elliptic Potential and Pseudo-Elliptical Navarro--Frenk--White models. We show that the PA is exact for this first model. For the second, we obtain constraints on the model parameter space (given by the potential ellipticity parameter and characteristic convergence ) such that the PA is accurate for the aforementioned quantities. In this process we obtain analytic expressions for several lensing functions, which are valid for the PA in general. The determination of this domain of validity could have significant implications for the use of the PA, but it still needs to be probed with extended sources.
Accepted for publication in MNRAS
References in corpus (17)
- A Bayesian approach to strong lensing modelling of galaxy clusters
- Cosmological Constraints from Strong Gravitational Lensing in Galaxy Clusters
- The CFHTLS Strong Lensing Legacy Survey: I. Survey overview and T0002 release sample
- A New Survey for Giant Arcs
- Two New Large Separation Gravitational Lenses from SDSS
- Realistic simulations of gravitational lensing by galaxy clusters: extracting arc parameters from mock DUNE images
- A Systematic Search for High Surface Brightness Giant Arcs in a Sloan Digital Sky Survey Cluster Sample
- The Sloan Bright Arcs Survey : Discovery of Seven New Strongly Lensed Galaxies from z=0.66-2.94
- Lensview: Software for modelling resolved gravitational lens images
- The Sloan Bright Arcs Survey: Ten Strong Gravitational Lensing Clusters and Evidence of Overconcentration
- Gravitational arcs as a perturbation of the perfect ring
- Predicting the number of giant arcs expected in the next generation wide-field surveys from space
- Numerical investigation of lenses with substructures using the perturbative method
- Perturbative signature of substructures in strong gravitational lenses
- Domain of validity for pseudo-elliptical NFW lens models
- The SOAR Gravitational Arc Survey - I: Survey overview and photometric catalogs
- On Multiple Einstein Rings