Amy Etherington amy.etherington@durham.ac.uk
PGR Student Doctor of Philosophy
Beyond the bulge–halo conspiracy? Density profiles of early-type galaxies from extended-source strong lensing
Etherington, Amy; Nightingale, James W; Massey, Richard; Robertson, Andrew; Cao, XiaoYue; Amvrosiadis, Aristeidis; Cole, Shaun; Frenk, Carlos S; He, Qiuhan; Lagattuta, David J; Lange, Samuel; Li, Ran
Authors
James Nightingale james.w.nightingale@durham.ac.uk
Academic Visitor
Professor Richard Massey r.j.massey@durham.ac.uk
Professor
Dr Andrew Robertson andrew.robertson@durham.ac.uk
Academic Visitor
XiaoYue Cao
Aristeidis Amvrosiadis
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
Dr Qiuhan He qiuhan.he@durham.ac.uk
Post Doctoral Research Associate
Dr David Lagattuta david.j.lagattuta@durham.ac.uk
Post Doctoral Research Associate
Samuel Lange samuel.c.lange@durham.ac.uk
PGR Student Doctor of Philosophy
Ran Li
Abstract
Observations suggest that the dark matter and stars in early-type galaxies ‘conspire’ to produce a surprisingly simple distribution of total mass, ρ(r) ∝ ρ−γ, with γ ≈ 2. We measure the distribution of mass in 48 early-type galaxies that gravitationally lens a resolved background source. By fitting the source light in every pixel of images from the Hubble Space Telescope, we find a mean ⟨γ⟩=2.075+0.023−0.024 with an intrinsic scatter between galaxies of σγ=0.172+0.022−0.032 for the overall sample. This is consistent with and has similar precision to traditional techniques that employ spectroscopic observations to supplement lensing with mass estimates from stellar dynamics. Comparing measurements of γ for individual lenses using both techniques, we find a statistically insignificant correlation of −0.150+0.223−0.217 between the two, indicating a lack of statistical power or deviations from a power-law density in certain lenses. At fixed surface mass density, we measure a redshift dependence, ∂⟨γ⟩/z=0.345+0.322−0.296, that is consistent with traditional techniques for the same sample of Sloan Lens ACS and GALaxy-Lyα EmitteR sYstems (GALLERY) lenses. Interestingly, the consistency breaks down when we measure the dependence of γ on the surface mass density of a lens galaxy. We argue that this is tentative evidence for an inflection point in the total mass-density profile at a few times the galaxy effective radius – breaking the conspiracy.
Citation
Etherington, A., Nightingale, J. W., Massey, R., Robertson, A., Cao, X., Amvrosiadis, A., Cole, S., Frenk, C. S., He, Q., Lagattuta, D. J., Lange, S., & Li, R. (2023). Beyond the bulge–halo conspiracy? Density profiles of early-type galaxies from extended-source strong lensing. Monthly Notices of the Royal Astronomical Society, 521(4), 6005-6018. https://doi.org/10.1093/mnras/stad582
Journal Article Type | Article |
---|---|
Acceptance Date | Feb 16, 2023 |
Online Publication Date | Mar 7, 2023 |
Publication Date | 2023-06 |
Deposit Date | Aug 16, 2023 |
Publicly Available Date | Aug 16, 2023 |
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 | 521 |
Issue | 4 |
Pages | 6005-6018 |
DOI | https://doi.org/10.1093/mnras/stad582 |
Keywords | Space and Planetary Science; Astronomy and Astrophysics |
Public URL | https://durham-repository.worktribe.com/output/1719403 |
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Copyright Statement
© 2023 The Author(s).
Published by Oxford University Press on behalf of Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited
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