Dr Qiuhan He qiuhan.he@durham.ac.uk
Post Doctoral Research Associate
Unveiling lens light complexity with a novel multi-Gaussian expansion approach for strong gravitational lensing
He, Qiuhan; Nightingale, James W; Amvrosiadis, Aris; Robertson, Andrew; Cole, Shaun; Frenk, Carlos S; Massey, Richard; Li, Ran; Cao, Xiaoyue; Lange, Samuel C; França, João Paulo C
Authors
James Nightingale james.w.nightingale@durham.ac.uk
Academic Visitor
Aristeidis Amvrosiadis aristeidis.amvrosiadis@durham.ac.uk
Post Doctoral Research Associate
Dr Andrew Robertson andrew.robertson@durham.ac.uk
Academic Visitor
Professor Shaun Cole shaun.cole@durham.ac.uk
Director of the Institute for Computational Cosmology
Professor Carlos Frenk c.s.frenk@durham.ac.uk
Professor
Professor Richard Massey r.j.massey@durham.ac.uk
Professor
Ran Li
Xiaoyue Cao
Sam Lange samuel.c.lange@durham.ac.uk
PGR Student Doctor of Philosophy
João Paulo C França
Abstract
In a strong gravitational lensing system, the distorted light from a source is analysed to infer the properties of the lens. However, light emitted by the lens itself can contaminate the image of the source, introducing systematic errors in the analysis. We present a simple and efficient lens light model based on the well-tested multi-Gaussian expansion (MGE) method for representing galaxy surface brightness profiles, which we combine with a semi-linear inversion scheme for pixelized source modelling. Testing it against realistic mock lensing images, we show that our scheme can fit the lensed images to the noise level, with relative differences between the true input and best-fitting lens light model remaining below 5 per cent. We apply the MGE lens light model to 38 lenses from the HST SLACS sample. We find that the new scheme provides a good fit for the majority of the sample with only 3 exceptions – these show clear asymmetric residuals in the lens light. We examine the radial dependence of the ellipticity and position angles and confirm that it is common for a typical lens galaxy to exhibit twisting non-elliptical isophotes and boxy / disky isophotes. Our MGE lens light model will be a valuable tool for understanding the hidden complexity of the lens mass distribution.
Citation
He, Q., Nightingale, J. W., Amvrosiadis, A., Robertson, A., Cole, S., Frenk, C. S., Massey, R., Li, R., Cao, X., Lange, S. C., & França, J. P. C. (2024). Unveiling lens light complexity with a novel multi-Gaussian expansion approach for strong gravitational lensing. Monthly Notices of the Royal Astronomical Society, 532(2), 2441-2462. https://doi.org/10.1093/mnras/stae1577
Journal Article Type | Article |
---|---|
Acceptance Date | Jun 10, 2024 |
Online Publication Date | Jun 27, 2024 |
Publication Date | 2024-08 |
Deposit Date | Aug 2, 2024 |
Publicly Available Date | Aug 2, 2024 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 532 |
Issue | 2 |
Pages | 2441-2462 |
DOI | https://doi.org/10.1093/mnras/stae1577 |
Public URL | https://durham-repository.worktribe.com/output/2736422 |
Files
Published Journal Article
(6.4 Mb)
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Publisher Licence URL
http://creativecommons.org/licenses/by/4.0/
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