A Semi-analytic Ray-tracing Algorithm for Weak Lensing
arXiv:1012.1625 · doi:10.1111/j.1365-2966.2011.18754.x
Abstract
We propose a new ray-tracing algorithm to measure the weak lensing shear and convergence fields directly from N-body simulations. We calculate the deflection of the light rays lensed by the 3-D mass density field or gravitational potential along the line of sight on a grid-by-grid basis, rather than using the projected 2-D lens planes. Our algorithm uses simple analytic formulae instead of numerical integrations in the computation of the projected density field along the line of sight, and so is computationally efficient, accurate and straightforward to implement. This will prove valuable in the interpretation of data from the next generation of surveys that will image many thousands of square degrees of sky.
13 pages, 5 figures
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- CMB weak-lensing beyond the Born approximation: a numerical approach
- The Accuracy of Weak Lensing Simulations
- Weak lensing by voids in weak lensing maps
- Cosmological test of gravity using weak lensing voids
- ICE-COLA: fast simulations for weak lensing observables
- Weak lensing by galaxy troughs with modified gravity
- Studying the precision of ray tracing techniques with Szekeres models
- Methods for studying the accuracy of light propagation in N-body simulations
- Multiple Lensing of the Cosmic Microwave Background anisotropies
- RAY-RAMSES: a code for ray tracing on the fly in N-body simulations
- Born-corrections to weak lensing of the cosmic microwave background temperature and polarisation anisotropies
- Retrieving the three-dimensional matter power spectrum and galaxy biasing parameters from lensing tomography
- Influence of the local Universe on weak gravitational lensing surveys
- Proca-stinated Cosmology II: Matter, Halo, and Lensing Statistics in the vector Galileon
- A Hamiltonian, post-Born, three-dimensional, on-the-fly ray tracing algorithm for gravitational lensing
- Ringing the universe with cosmic emptiness: void properties through a combined analysis of stacked weak gravitational and Doppler lensing