Moderate Galaxy-Galaxy Lensing
arXiv:1201.1960 · doi:10.1111/j.1365-2966.2012.20438.x
Abstract
We study moderate gravitational lensing where a background galaxy is magnified substantially, but not multiply imaged, by an intervening galaxy. We focus on the case where both the lens and source are elliptical galaxies. The signatures of moderate lensing include isophotal distortions and systematic shifts in the fundamental plane and Kormendy relation, which can potentially be used to statistically determine the galaxy mass profiles. These effects are illustrated using Monte Carlo simulations of galaxy pairs where the foreground galaxy is modelled as a singular isothermal sphere model and observational parameters appropriate for the Large Synoptic Survey Telescope (LSST). The range in radius probed by moderate lensing will be larger than that by strong lensing, and is in the interesting regime where the density slope may be changing.
8 pages, 12 figures, MNRAS, comments welcome
References in corpus (4)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- The Structure & Dynamics of Massive Early-type Galaxies: On Homology, Isothermality and Isotropy inside one Effective Radius
- Isophotal Shapes of Elliptical/S0 Galaxies from the Sloan Digital Sky Survey
- Direct Measurements of the magnification produced by galaxy clusters as gravitational lenses