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Issue A&A
Volume 458, Number 2, November I 2006
Page(s) 349 - 356
Section Cosmology (including clusters of galaxies)
DOI http://dx.doi.org/10.1051/0004-6361:20054582



A&A 458, 349-356 (2006)
DOI: 10.1051/0004-6361:20054582

Combining weak and strong lensing in cluster potential reconstruction

M. Cacciato1, 2, M. Bartelmann3, M. Meneghetti3 and L. Moscardini1, 4

1  Dipartimento di Astronomia, Università di Bologna, via Ranzani 1, 40127 Bologna, Italy
    e-mail: marcello.cacciato@studio.unibo.it
2  Max-Planck-Institut für Astronomie, Königstuhl  17, 69117 Heidelberg, Germany
3  Zentrum für Astronomie, ITA, Universität Heidelberg, Albert-Überle-Str. 2, 69120 Heidelberg, Germany
4  INFN, Sezione di Bologna, Italy

(Received 24 November 2005 / Accepted 2 August 2006)

Abstract
We propose a method for recovering the two-dimensional gravitational potential of galaxy clusters which combines data from weak and strong gravitational lensing. A first estimate of the potential from weak lensing is improved at the approximate locations of critical curves. The method can be fully linearised and does not rely on the existence and identification of multiple images. We use simulations to show that it recovers the surface-mass density profiles and distributions very accurately,even if critical curves are only partially known and if their location is realistically uncertain. We further describe how arcs at different redshifts can be combined, and how deviations from weak lensing can be included.


Key words: gravitational lensing -- galaxies: clusters: general -- cosmology: theory



© ESO 2006


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