Geoff C-F Chen
SHARP – VIII. J0924+0219 lens mass distribution and time-delay prediction through adaptive-optics imaging
Chen, Geoff C-F; Fassnacht, Christopher D; Suyu, Sherry H; Koopmans, Léon VE; Lagattuta, David J; McKean, John P; Auger, Matt W; Vegetti, Simona; Treu, Tommaso
Authors
Christopher D Fassnacht
Sherry H Suyu
Léon VE Koopmans
Dr David Lagattuta david.j.lagattuta@durham.ac.uk
Post Doctoral Research Associate
John P McKean
Matt W Auger
Simona Vegetti
Tommaso Treu
Abstract
Strongly lensed quasars can provide measurements of the Hubble constant (H0) independent of any other methods. One of the key ingredients is exquisite high-resolution imaging data, such as Hubble Space Telescope (HST) imaging and adaptive-optics (AO) imaging from ground-based telescopes, which provide strong constraints on the mass distribution of the lensing galaxy. In this work, we expand on the previous analysis of three time-delay lenses with AO imaging (RX J1131−1231, HE 0435−1223, and PG 1115+080), and perform a joint analysis of J0924+0219 by using AO imaging from the Keck telescope, obtained as part of the Strong lensing at High Angular Resolution Program (SHARP) AO effort, with HST imaging to constrain the mass distribution of the lensing galaxy. Under the assumption of a flat Λ cold dark matter (ΛCDM) model with fixed Ωm = 0.3, we show that by marginalizing over two different kinds of mass models (power-law and composite models) and their transformed mass profiles via a mass-sheet transformation, we obtain ΔtBA=6.89+0.8−0.7h−1σ^2v d, ΔtCA=10.7+1.6−1.2h−1σ^2v d, and ΔtDA=7.70+1.0−0.9h−1σ^2v d, where h=H0/100kms−1Mpc−1 is the dimensionless Hubble constant and σ^v=σobv/(280kms−1) is the scaled dimensionless velocity dispersion. Future measurements of time delays with 10 per cent uncertainty and velocity dispersion with 5 per cent uncertainty would yield a H0 constraint of ∼15 per cent precision.
Citation
Chen, G. C.-F., Fassnacht, C. D., Suyu, S. H., Koopmans, L. V., Lagattuta, D. J., McKean, J. P., Auger, M. W., Vegetti, S., & Treu, T. (2022). SHARP – VIII. J0924+0219 lens mass distribution and time-delay prediction through adaptive-optics imaging. Monthly Notices of the Royal Astronomical Society, 513(2), 2349-2359. https://doi.org/10.1093/mnras/stac1081
Journal Article Type | Article |
---|---|
Acceptance Date | Feb 22, 2022 |
Online Publication Date | Apr 27, 2022 |
Publication Date | 2022-06 |
Deposit Date | Jun 16, 2022 |
Publicly Available Date | Jun 16, 2022 |
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 | 513 |
Issue | 2 |
Pages | 2349-2359 |
DOI | https://doi.org/10.1093/mnras/stac1081 |
Public URL | https://durham-repository.worktribe.com/output/1201688 |
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Copyright Statement
This article has been accepted for publication in Monthly notices of the Royal Astronomical Society. ©: 2021 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
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