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AutoLens: automated modeling of a strong lens’s light, mass and source

Nightingale, J. W.; Dye, S.; Massey, Richard J.

AutoLens: automated modeling of a strong lens’s light, mass and source Thumbnail


Authors

J. W. Nightingale

SIMON DYE Simon.Dye@nottingham.ac.uk
Associate Professor

Richard J. Massey



Abstract

This work presents AutoLens, the first entirely automated modeling suite for the analysis of galaxy-scale strong gravitational lenses. AutoLens simultaneously models the lens galaxy’s light and mass whilst reconstructing the extended source galaxy on an adaptive pixel-grid. The method’s approach to source-plane discretization is amorphous, adapting its clustering and regularization to the intrinsic properties of the lensed source. The lens’s light is fitted using a superposition of Sersic functions, allowing AutoLens to cleanly deblend its light from the source. Single component mass models representing the lens’s total mass density profile are demonstrated, which in conjunction with light modeling can detect central images using a centrally cored profile. Decomposed mass modeling is also shown, which can fully decouple a lens’s light and dark matter and determine whether the two component are geometrically aligned. The complexity of the light and mass models are automatically chosen via Bayesian model comparison. These steps form AutoLens’s automated analysis pipeline, such that all results in this work are generated without any user-intervention. This is rigorously tested on a large suite of simulated images, assessing its performance on a broad range of lens profiles, source morphologies and lensing geometries. The method’s performance is excellent, with accurate light, mass and source profiles inferred for data sets representative of both existing Hubble imaging and future Euclid wide-field observations.

Journal Article Type Article
Acceptance Date May 3, 2018
Online Publication Date May 22, 2018
Publication Date Aug 21, 2018
Deposit Date Jun 13, 2018
Publicly Available Date Jun 13, 2018
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Oxford University Press
Peer Reviewed Peer Reviewed
Volume 478
Issue 4
Pages 4738-4784
DOI https://doi.org/10.1093/mnras/sty1264
Keywords gravitational lensing, galaxies: structure
Public URL https://nottingham-repository.worktribe.com/output/933405
Publisher URL https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/sty1264/5001434
Additional Information This article has been accepted for publication inMonthly Notices of the Royal Astronomical Society Published by Oxford University Press on behalf of the Royal Astronomical Society.

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