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Lopsidedness in early-type galaxies: the role of the m = 1 multipole in isophote fitting and strong lens modelling

Amvrosiadis, A; Nightingale, J W; He, Q; Robertson, A; Lange, S; Frenk, C S; Cole, S; Massey, R; Poci, A

Lopsidedness in early-type galaxies: the role of the m = 1 multipole in isophote fitting and strong lens modelling Thumbnail


Authors

Profile image of Qiuhan He

Dr Qiuhan He qiuhan.he@durham.ac.uk
Post Doctoral Research Associate

Profile image of Sam Lange

Sam Lange samuel.c.lange@durham.ac.uk
PGR Student Doctor of Philosophy



Abstract

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.

Citation

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

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