Issue |
A&A
Volume 673, May 2023
|
|
---|---|---|
Article Number | A33 | |
Number of page(s) | 60 | |
Section | Numerical methods and codes | |
DOI | https://doi.org/10.1051/0004-6361/202244534 | |
Published online | 03 May 2023 |
HOLISMOKES
X. Comparison between neural network and semi-automated traditional modeling of strong lenses
1
Max-Planck-Institut für Astrophysik,
Karl-Schwarzschild Str. 1,
85748
Garching, Germany
e-mail: schuldt@mpa-garching.mpg.de
2
Technical University of Munich, TUM School of Natural Sciences, Department of Physics,
James-Franck-Str. 1,
85748
Garching, Germany
3
Academia Sinica Institute of Astronomy and Astrophysics (ASIAA),
11F of ASMAB, No.1, Section 4, Roosevelt Road,
Taipei
10617, Taiwan
4
Ruhr University Bochum, Faculty of Physics and Astronomy, Astronomical Institute (AIRUB), German Centre for Cosmological Lensing,
44780
Bochum, Germany
5
Pyörrekuja 5 A,
04300
Tuusula, Finland
Received:
18
July
2022
Accepted:
8
March
2023
Modeling of strongly gravitationally lensed galaxies is often required in order to use them as astrophysical or cosmological probes. With current and upcoming wide-field imaging surveys, the number of detected lenses is increasing significantly such that automated and fast modeling procedures for ground-based data are urgently needed. This is especially pertinent to short-lived lensed transients in order to plan follow-up observations. Therefore, we present in a companion paper a neural network predicting the parameter values with corresponding uncertainties of a singular isothermal ellipsoid (SIE) mass profile with external shear. In this work, we also present a newly developed pipeline glee_auto.py that can be used to model any galaxy-scale lensing system consistently. In contrast to previous automated modeling pipelines that require high-resolution space-based images, glee_auto.py is optimized to work well on ground-based images such as those from the Hyper-Suprime-Cam (HSC) Subaru Strategic Program or the upcoming Rubin Observatory Legacy Survey of Space and Time. We further present glee_tools.py, a flexible automation code for individual modeling that has no direct decisions and assumptions implemented on the lens system setup or image resolution. Both pipelines, in addition to our modeling network, minimize the user input time drastically and thus are important for future modeling efforts. We applied the network to 31 real galaxy-scale lenses of HSC and compare the results to traditional, Markov chain Monte Carlo sampling-based models obtained from our semi-autonomous pipelines. In the direct comparison, we find a very good match for the Einstein radius. The lens mass center and ellipticity show reasonable agreement. The main discrepancies pretrain to the external shear, as is expected from our tests on mock systems where the neural network always predicts values close to zero for the complex components of the shear. In general, our study demonstrates that neural networks are a viable and ultra fast approach for measuring the lens-galaxy masses from ground-based data in the upcoming era with ~105 lenses expected.
Key words: gravitational lensing: strong / methods: data analysis
© The Authors 2023
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
This article is published in open access under the Subscribe to Open model.
Open Access funding provided by Max Planck Society.
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