Gravitational lensing model degeneracies: Is steepness all-important?
arXiv:astro-ph/0608496 · doi:10.1086/508798
Abstract
In gravitational lensing, steeper mass profiles generically produce longer time delays but smaller magnifications, without necessarily changing the image positions or magnification ratios between different images. This is well known. We find in this paper, however, that even if steepness is fixed, time delays can still have significant model dependence, which we attribute to shape modeling degeneracies. This conclusion follows from numerical experiments with models of 35 galaxy lenses. We suggest that varying and twisting ellipticities, features that are explored by pixelated lens models but not so far by parametric models, have an important effect on time delays.
To appear in ApJ
References in corpus (1)
Cited by in corpus (9)
- Gravitational Lens Time Delays: A Statistical Assessment of Lens Model Dependences and Implications for the Global Hubble Constant
- LensPerfect: Gravitational Lens Massmap Reconstructions Yielding Exact Reproduction of All Multiple Images
- A New Estimate of the Hubble Time with Improved Modeling of Gravitational Lenses
- Lens Galaxy Properties of SBS1520+530: Insights from Keck Spectroscopy and AO Imaging
- Radial density profiles of time-delay lensing galaxies
- A generalisation of the mass-sheet degeneracy producing ring-like artefacts in the lens mass distribution
- Steepened inner density profiles of group galaxies via interactions: An N-body analysis
- Lensed Image Angles: New Statistical Evidence for Substructure
- The Hubble constant from galaxy lenses: impacts of triaxiality and model degeneracies