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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

SHARP – VIII. J0924+0219 lens mass distribution and time-delay prediction through adaptive-optics imaging Thumbnail


Authors

Geoff C-F Chen

Christopher D Fassnacht

Sherry H Suyu

Léon VE Koopmans

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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