Issue |
EAS Publications Series
Volume 20, 2006
Mass Profiles and Shapes of Cosmological Structures
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Page(s) | 161 - 166 | |
DOI | https://doi.org/10.1051/eas:2006064 | |
Published online | 19 May 2006 |
G.A. Mamon, F. Combes, C. Deffayet and B. Fort (eds)
EAS Publications Series, 20 (2006) 161-166
Gravitational Lensing & Stellar Dynamics
Kapteyn Astronomical Institute,
PO Box 800, 9700 AV Groningen, The Netherlands
Strong gravitational lensing and stellar dynamics provide two complementary and orthogonal constraints on the density profiles of galaxies. Based on spherically symmetric, scale-free, mass models, it is shown that the combination of both techniques is powerful in breaking the mass-sheet and mass-anisotropy degeneracies. Second, observational results are presented from the Lenses Structure & Dynamics (LSD) Survey and the Sloan Lens ACS (SLACS) Survey collaborations to illustrate this new methodology in constraining the dark and stellar density profiles, and mass structure, of early-type galaxies to redshifts of unity.
© EAS, EDP Sciences, 2006