TDCOSMO. VII. Boxyness/discyness in lensing galaxies : Detectability and impact on
arXiv:2112.03932 · doi:10.1051/0004-6361/202141551
Abstract
In the context of gravitational lensing, the density profile of lensing galaxies is often considered to be perfectly elliptical. Potential angular structures are generally ignored, except to explain flux ratios anomalies. Surprisingly, the impact of azimuthal structures on extended images of the source has not been characterized, nor its impact on the H0 inference. We address this task by creating mock images of a point source embedded in an extended source, lensed by an elliptical galaxy on which multipolar components are added to emulate boxy/discy isodensity contours. Modeling such images with a density profile free of angular structure allow us to explore the detectability of image deformation induced by the multipoles in the residual frame. Multipole deformations are almost always detectable for our highest signal-to-noise mock data. However the detectability depends on the lens ellipticity and Einstein radius, on the S/N of the data, and on the specific lens modeling strategy. Multipoles also introduce small changes to the time delays. We therefore quantify how undetected multipoles would impact H0 inference. When no multipoles are detected in the residuals, the impact on H0 for a given lens is in general less than a few km/s/Mpc, but in the worst case scenario, combining low S/N in the ring and large intrinsic boxyness/discyness, the bias on H0 can reach 10-12 km/s/Mpc. If we now look at the inference on H0 from a population of lensing galaxies, having a distribution of multipoles representative of what is found in the light-profile of elliptical galaxies, we then find a systematic bias on H0 < 1%. The comparison of our mock systems to the state-of-the-art time delay lens sample studied by the H0LiCOW and TDCOSMO collaborations, indicates that multipoles are currently unlikely to be a source of substantial systematic bias on the inferred value of H0 from time-delay lenses.
Accepted for publication in A&A; 21 pages ; content indentical to previous version, only form improvements thanks to A&A language editing ; link to the notebook associated https://github.com/TDCOSMO/TD_data_public
References in corpus (19)
- The NumPy array: a structure for efficient numerical computation
- Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
- Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
- The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
- The Halos of Satellite Galaxies: the Companion of the Massive Elliptical Lens SL2S J08544-0121
- The Hubble Constant from Infrared Surface Brightness Fluctuation Distances
- How well can cold-dark-matter substructures account for the observed radio flux-ratio anomalies?
- Using The Baryonic Tully-Fisher Relation to Measure
- Over-constrained Gravitational Lens Models and the Hubble Constant
- Strong lensing signatures of self-interacting dark matter in low-mass halos
- Isophotal Shapes of Elliptical/S0 Galaxies from the Sloan Digital Sky Survey
- Multi wavelength study of the gravitational lens system RXS J1131-1231: II Lens model and source reconstruction
- Large-Scale Gravitational Lens Modeling with Bayesian Neural Networks for Accurate and Precise Inference of the Hubble Constant
- SLITronomy: towards a fully wavelet-based strong lensing inversion technique
- The UV--mid-IR Spectral Energy Distribution of a z=1.7 Quasar Host Galaxy
- The impact of mass map truncation on strong lensing simulations
- Multipole Gravitational Lensing and High-order Perturbations on the Quadrupole Lens
- Unlensing HST Observations of the Einstein Ring 1RXS J1131-1231: A Bayesian Analysis
- Isophote Shapes of Early-Type Galaxies in Massive Clusters at and 0
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