Aristeidis Amvrosiadis aristeidis.amvrosiadis@durham.ac.uk
Post Doctoral Research Associate
Aristeidis Amvrosiadis aristeidis.amvrosiadis@durham.ac.uk
Post Doctoral Research Associate
James Nightingale james.w.nightingale@durham.ac.uk
Academic Visitor
Dr Qiuhan He qiuhan.he@durham.ac.uk
Post Doctoral Research Associate
Dr Andrew Robertson andrew.robertson@durham.ac.uk
Academic Visitor
Sam Lange samuel.c.lange@durham.ac.uk
PGR Student Doctor of Philosophy
Professor Carlos Frenk c.s.frenk@durham.ac.uk
Professor
Professor Shaun Cole shaun.cole@durham.ac.uk
Director of the Institute for Computational Cosmology
Professor Richard Massey r.j.massey@durham.ac.uk
Professor
Adriano Poci adriano.poci@durham.ac.uk
Academic Visitor
The surface brightness distribution of massive early-type galaxies (ETGs) often deviates from a perfectly elliptical shape. To capture these deviations in their isophotes during an ellipse fitting analysis, Fourier modes of order are often used. In such analyses, the centre of each ellipse is treated as a free parameter which may result in offsets from the centre of light, particularly for ellipses in the outer regions. This complexity is not currently accounted for in the mass models used in either strong gravitational lensing or galactic dynamical studies. In this work, we adopt a different approach, using the Fourier mode to account for this complexity while keeping the centres of all perturbed ellipses fixed, showing that it fits the data equally well. We applied our method to the distribution of light emission to a sample of ETGs from the MASSIVE survey and found that the majority have low amplitudes, below 2 per cent. Five out of the 30 galaxies we analysed have high amplitudes, ranging from 2 to 10 per cent in the outer parts ( kpc), all of which have a physically associated companion. Based on our findings, we advocate the use of the multipole in the mass models used in strong lensing and dynamical studies, particularly for galaxies with recent or ongoing interactions.
Amvrosiadis, A., Nightingale, J. W., He, Q., Robertson, A., Lange, S., Frenk, C. S., Cole, S., Massey, R., & Poci, A. (2025). Lopsidedness in early-type galaxies: the role of the m = 1 multipole in isophote fitting and strong lens modelling. Monthly Notices of the Royal Astronomical Society, 540(4), 3281-3288. https://doi.org/10.1093/mnras/staf857
Journal Article Type | Article |
---|---|
Acceptance Date | Apr 30, 2025 |
Online Publication Date | Jun 4, 2025 |
Publication Date | 2025-07 |
Deposit Date | Jul 1, 2025 |
Publicly Available Date | Jul 1, 2025 |
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 | 540 |
Issue | 4 |
Pages | 3281-3288 |
DOI | https://doi.org/10.1093/mnras/staf857 |
Keywords | galaxies: elliptical and lenticular, gravitational lensing: strong, galaxies: structure |
Public URL | https://durham-repository.worktribe.com/output/4125246 |
Published Journal Article
(1.6 Mb)
PDF
Publisher Licence URL
http://creativecommons.org/licenses/by/4.0/
FLASH: Faint Lenses from Associated Selection with Herschel
(2023)
Journal Article
Abell 1201: detection of an ultramassive black hole in a strong gravitational lens
(2023)
Journal Article
About Durham Research Online (DRO)
Administrator e-mail: dro.admin@durham.ac.uk
This application uses the following open-source libraries:
Apache License Version 2.0 (http://www.apache.org/licenses/)
Apache License Version 2.0 (http://www.apache.org/licenses/)
SIL OFL 1.1 (http://scripts.sil.org/OFL)
MIT License (http://opensource.org/licenses/mit-license.html)
CC BY 3.0 ( http://creativecommons.org/licenses/by/3.0/)
Powered by Worktribe © 2025
Advanced Search