Poster
Abstract :
Based on the SLAP code (Sendra et al.
2005) we improve the lensing
reconstruction of the mass in a galaxy
cluster by integrating physical priors
in the code that greatly help to increse
the resolution of the solution and
reduce the uncertainties. The new code
is tested with simulated data (strong
lensing) that mimics real data. We
explore the improvements by comparing
the solutions obtained with and without
the new physical priors and discuss the
limitations of the new code.
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Bibliography
- Main
publications
- "Combined
reconstruction of weak and strong
lensing data with WSLAP"
Sendra et al. MNRAS, 375, 958 ( 2007)
- "Non-parametric
mass reconstruction of A1689 from
strong lensing data with the Strong
Lensing Analysis Package"
Sendra et al. 2005, MNRAS, 362, 1247
- "Non-parametric
inversion of strong lensing systems"
Sendra et al. 2005, MNRAS, 360, 477
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