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Galaxy mass modelling from multiwavelength JWST strong lens analysis: dark matter substructure, angular mass complexity, or both?

Lange, Samuel C.; Amvrosiadis, Aristeidis; Nightingale, James W.; He, Qiuhan; Frenk, Carlos S.; Robertson, Andrew; Cole, Shaun; Massey, Richard; Cao, Xiaoyue; Li, Ran; Wang, Kaihao

Galaxy mass modelling from multiwavelength JWST strong lens analysis: dark matter substructure, angular mass complexity, or both? Thumbnail


Authors

Profile image of Sam Lange

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

Profile image of Qiuhan He

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

Andrew Robertson

Xiaoyue Cao

Ran Li

Kaihao Wang



Abstract

We analyse two galaxy-scale strong gravitational lenses, SPT0418-47 and SPT2147-50, using JWST NIRCam imaging across multiple filters. To account for angular complexity in the lens mass distribution, we introduce multipole perturbations with orders m = 1, 3, 4. Our results show strong evidence for angular mass complexity in SPT2147, with multipole strengths of 0.3–1.7 per cent for m = 3, 4 and 2.4–9.5 per cent for m = 1, while SPT0418 shows no such preference. We also test lens models that include a dark matter substructure, finding a strong preference for a substructure in SPT2147-50 with a Bayes factor of ▲log(ε)∼ 60 when multipoles are not included. Including multipoles reduces the Bayes factor to ▲log(ε)∼ 11, still corresponding to a 5σ detection of a subhalo with an NFW (Navarro–Frenk–White) mass of log10(M200/M☉) = 10.87+−00..7153. While SPT2147-50 may represent the fourth detection of a dark matter substructure in a strong lens, further analysis is needed to confirm that the signal is not due to systematics associated with the lens mass model.

Citation

Lange, S. C., Amvrosiadis, A., Nightingale, J. W., He, Q., Frenk, C. S., Robertson, A., Cole, S., Massey, R., Cao, X., Li, R., & Wang, K. (2025). Galaxy mass modelling from multiwavelength JWST strong lens analysis: dark matter substructure, angular mass complexity, or both?. Monthly Notices of the Royal Astronomical Society, 539(2), 704-726. https://doi.org/10.1093/mnras/staf491

Journal Article Type Article
Acceptance Date Mar 18, 2025
Online Publication Date Mar 28, 2025
Publication Date 2025-05
Deposit Date May 27, 2025
Publicly Available Date May 27, 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 539
Issue 2
Pages 704-726
DOI https://doi.org/10.1093/mnras/staf491
Public URL https://durham-repository.worktribe.com/output/3964827

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