The Very Knotty Lenser: exploring the role of regularization in source and potential reconstructions using Gaussian Process Regression
arXiv:2202.09378 · doi:10.1093/mnras/stac1924
Abstract
Reconstructing lens potentials and lensed sources can easily become an underconstrained problem, even when the degrees of freedom are low, due to degeneracies, particularly when potential perturbations superimposed on a smooth lens are included. Regularization has traditionally been used to constrain the solutions where the data failed to do so, e.g. in unlensed parts of the source. In this exploratory work, we go beyond the usual choices of regularization and adopt observationally motivated priors for the source brightness. We also perform a similar comparison when reconstructing lens potential perturbations, which are assumed to be stationary, i.e. permeate the entire field of view. We find that physically motivated priors lead to lower residuals, avoid overfitting, and are decisively preferred within a Bayesian quantitative framework in all the examples considered. For the perturbations, choosing the wrong regularization can have a detrimental effect that even high-quality data cannot correct for, while using a purely smooth lens model can absorb them to a very high degree and lead to biased solutions. Finally, our new implementation of the semi-linear inversion technique provides the first quantitative framework for measuring degeneracies between the source and the potential perturbations.
25 pages, 21 figures, 5 tables, submitted to MNRAS
References in corpus (13)
- The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
- Theory of Star Formation
- Too big to fail? The puzzling darkness of massive Milky Way subhaloes
- Properties of galaxies reproduced by a hydrodynamic simulation
- High-resolution mass models of dwarf galaxies from LITTLE THINGS
- The Structure & Dynamics of Massive Early-type Galaxies: On Homology, Isothermality and Isotropy inside one Effective Radius
- Bayesian Strong Gravitational-Lens Modeling on Adaptive Grids: Objective Detection of Mass Substructure in Galaxies
- Is there a "too big to fail" problem in the field?
- The SINFONI Nearby Elliptical Lens Locator Survey: Discovery of two new low-redshift strong lenses and implications for the initial mass function in giant early-type galaxies
- On the Power Spectrum of Dark Matter Substructure in Strong Gravitational Lenses
- The inner mass power spectrum of galaxies using strong gravitational lensing: beyond linear approximation
- Statistical and systematic uncertainties in pixel-based source reconstruction algorithms for gravitational lensing
- SLITronomy: towards a fully wavelet-based strong lensing inversion technique
Cited by in corpus (6)
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- Modeling lens potentials with continuous neural fields in galaxy-scale strong lenses
- Interlopers speak out: studying the dark universe using small-scale lensing anisotropies