lemon: LEns MOdelling with Neural networks – I. Automated modelling of strong gravitational lenses with Bayesian Neural Networks

Author:

Gentile Fabrizio12ORCID,Tortora Crescenzo3ORCID,Covone Giovanni345ORCID,Koopmans Léon V E6ORCID,Li Rui7,Leuzzi Laura12,Napolitano Nicola R37ORCID

Affiliation:

1. Department of Physics and Astronomy (DIFA), University of Bologna , Via Gobetti 93/2, I-40129 Bologna, Italy

2. INAF – Osservatorio di Astrofisica e Scienza dello Spazio , Via Gobetti 93/3, I-40129 Bologna, Italy

3. INAF – Osservatorio Astronomico di Capodimonte , Salita Moiariello, 16, I-80131 Napoli, Italy

4. Dipartimento di Fisica ‘Ettore Pancini’, Università di Napoli Federico II , Compl. Univ. Monte S. Angelo, Via Cinthia, I-80126 Napoli, Italy

5. INFN, Sezione di Napoli , C.U. Monte S. Angelo, Via Cinthia, I-80126 Napoli, Italy

6. Kapteyn Astronomical Institute, University of Groningen , P.O Box 800, NL-9700 AV Groningen, the Netherlands

7. School of Physics and Astronomy, Sun Yat-sen University Zhuhai Campus , Daxue Road 2, 519082 Tangjia, Zhuhai, Guangdong, China

Abstract

ABSTRACT The unprecedented number of gravitational lenses expected from new-generation facilities such as the ESA Euclid telescope and the Vera Rubin Observatory makes it crucial to rethink our classical approach to lens-modelling. In this paper, we present lemon (Lens Modelling with Neural networks): a new machine-learning algorithm able to analyse hundreds of thousands of gravitational lenses in a reasonable amount of time. The algorithm is based on a Bayesian Neural Network: a new generation of neural networks able to associate a reliable confidence interval to each predicted parameter. We train the algorithm to predict the three main parameters of the singular isothermal ellipsoid model (the Einstein radius and the two components of the ellipticity) by employing two simulated data sets built to resemble the imaging capabilities of the Hubble Space Telescope and the forthcoming Euclid satellite. In this work, we assess the accuracy of the algorithm and the reliability of the estimated uncertainties by applying the network to several simulated data sets of 104 images each. We obtain accuracies comparable to previous studies present in the current literature and an average modelling time of just ∼0.5 s per lens. Finally, we apply the lemon algorithm to a pilot data set of real lenses observed with HST during the SLACS program, obtaining unbiased estimates of their SIE parameters. The code is publicly available on GitHub (https://github.com/fab-gentile/LEMON).

Funder

MIUR

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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