LeMoN: Lens Modelling with Neural networks -- I. Automated modelling of strong gravitational lenses with Bayesian Neural Networks
arXiv:2210.10793 · doi:10.1093/mnras/stad1325
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 datasets 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 datasets of 10.000 images each. We obtain accuracies comparable to previous studies present in the current literature and an average modelling time of just 0.5s per lens. Finally, we apply the LeMoN algorithm to a pilot dataset 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).
arXiv commentSubmitted to MNRAS; The code will be available on GitHub upon acceptance of the paper
References in corpus (70)
- SciPy 1.0--Fundamental Algorithms for Scientific Computing in Python
- H0LiCOW XIII. A 2.4% measurement of from lensed quasars: tension between early and late-Universe probes
- Spectroscopic Target Selection for the Sloan Digital Sky Survey: The Luminous Red Galaxy Sample
- Rotation-invariant convolutional neural networks for galaxy morphology prediction
- The COSMOS Survey: Hubble Space Telescope / Advanced Camera for Surveys (HST/ACS) Observations and Data Processing
- A Bayesian approach to strong lensing modelling of galaxy clusters
- Direct Detection of CDM Substructure
- The Sloan Lens ACS Survey. X. Stellar, Dynamical, and Total Mass Correlations of Massive Early-type Galaxies
- The Sloan Lens ACS Survey. III - The Structure and Formation of Early-type Galaxies and their Evolution since z~1
- The Sloan Lens ACS Survey. I. A Large Spectroscopically Selected Sample of Massive Early-Type Lens Galaxies
- Evidence for substructure in lens galaxies?
- COSMOS2020: A panchromatic view of the Universe to from two complementary catalogs
- Strong Lensing by Galaxies
- The Sloan Lens ACS Survey. V. The Full ACS Strong-Lens Sample
- Massive Dark-matter halos and Evolution of Early-type Galaxies to z=1
- Gravitational Lensing
- The initial mass function of early-type galaxies
- Improving galaxy morphologies for SDSS with Deep Learning
- The population of galaxy-galaxy strong lenses in forthcoming optical imaging surveys
- Lenstronomy: multi-purpose gravitational lens modelling software package
- Bayesian Strong Gravitational-Lens Modeling on Adaptive Grids: Objective Detection of Mass Substructure in Galaxies
- Shear and Ellipticity in Gravitational Lenses
- Fast Automated Analysis of Strong Gravitational Lenses with Convolutional Neural Networks
- Dark Matter Contraction and the Stellar Content of Massive Early-type Galaxies: Disfavoring "Light" Initial Mass Functions
- Inference of the Cold Dark Matter substructure mass function at z=0.2 using strong gravitational lenses
- Finding Strong Gravitational Lenses in the Kilo Degree Survey with Convolutional Neural Networks
- Pixel-based correction for Charge Transfer Inefficiency in the Hubble Space Telescope Advanced Camera for Surveys
- The Sloan Digital Sky Survey Quasar Lens Search. I. Candidate Selection Algorithm
- The SL2S Galaxy-scale Lens Sample. V. Dark Matter Halos and Stellar IMF of Massive Early-type Galaxies out to Redshift 0.8
- The Strong Gravitational Lens Finding Challenge
- Cosmological constraints with deep learning from KiDS-450 weak lensing maps
- Classifying Radio Galaxies with Convolutional Neural Network
- Uncertainties in Parameters Estimated with Neural Networks: Application to Strong Gravitational Lensing
- Dark matter halos of massive elliptical galaxies at are well described by the Navarro-Frenk-White profile
- The SL2S Galaxy-scale Lens Sample. III. Lens Models, Surface Photometry and Stellar Masses for the final sample
- AutoLens: Automated Modeling of a Strong Lens's Light, Mass and Source
- LinKS: Discovering galaxy-scale strong lenses in the Kilo-Degree Survey using Convolutional Neural Networks
- The Sloan Lens ACS Survey. XIII. Discovery of 40 New Galaxy-Scale Strong Lenses
- Finding high-redshift strong lenses in DES using convolutional neural networks
- A deep learning approach to cosmological dark energy models
- Measuring the power spectrum of dark matter substructure using strong gravitational lensing
- The X-Shooter Lens Survey - I. Dark-Matter Domination and a Salpeter-type IMF in a Massive Early-type Galaxy
- The SL2S Galaxy-scale Gravitational Lens Sample. I. The alignment of mass and light in massive early-type galaxies at z=0.2-0.9
- A low-mass cut-off near the hydrogen burning limit for Salpeter-like initial mass functions in early-type galaxies
- The SWELLS Survey. I. A large spectroscopically selected sample of edge-on late-type lens galaxies
- New high-quality strong lens candidates with deep learning in the Kilo Degree Survey
- LensExtractor: A Convolutional Neural Network in Search of Strong Gravitational Lenses
- Survey of gravitationally-lensed objects in HSC imaging (SuGOHI). III. Statistical strong lensing constraints on the stellar IMF of CMASS galaxies
- An Ensemble of Bayesian Neural Networks for Exoplanetary Atmospheric Retrieval
- Central dark matter trends in early-type galaxies from strong lensing, dynamics and stellar populations
- Parameters Estimation for the Cosmic Microwave Background with Bayesian Neural Networks
- Automated galaxy-galaxy strong lens modelling: no lens left behind
- Hierarchical Inference With Bayesian Neural Networks: An Application to Strong Gravitational Lensing
- Testing Convolutional Neural Networks for finding strong gravitational lenses in KiDS
- Line-of-sight effects in strong gravitational lensing
- The use of convolutional neural networks for modelling large optically-selected strong galaxy-lens samples
- Deep Learning for Strong Lensing Search: Tests of the Convolutional Neural Networks and New Candidates from KiDS DR3
- HOLISMOKES -- IV. Efficient mass modeling of strong lenses through deep learning
- Up to 100,000 reliable strong gravitational lenses in future dark energy experiments
- Statistical strong lensing. I. Constraints on the inner structure of galaxies from samples of a thousand lenses
- GIGA-Lens: Fast Bayesian Inference for Strong Gravitational Lens Modeling
- Large-Scale Gravitational Lens Modeling with Bayesian Neural Networks for Accurate and Precise Inference of the Hubble Constant
- Using wavelets to capture deviations from smoothness in galaxy-scale strong lenses
- Strong lens modelling: comparing and combining Bayesian neural networks and parametric profile fitting
- The Very Knotty Lenser: exploring the role of regularization in source and potential reconstructions using Gaussian Process Regression
- Statistical strong lensing. II. Cosmology and galaxy structure with time-delay lenses
- A Systematic Review of Strong Gravitational Lens Modeling Software
- HOLISMOKES -- IX. Neural network inference of strong-lens parameters and uncertainties from ground-based images
- Gauging the dark matter fraction in a S0 galaxy at z=0.47 through gravitational lensing from deep HST/ACS imaging
- Discovery of two Einstein crosses from massive post--blue nugget galaxies at z>1 in KiDS
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- Galaxy Spectra neural Network (GaSNet). II. Using Deep Learning for Spectral Classification and Redshift Predictions
- Exploiting the diversity of modeling methods to probe systematic biases in strong lensing analyses
- Euclid preparation. LI. Forecasting the recovery of galaxy physical properties and their relations with template-fitting and machine-learning methods
- Lens Modeling of STRIDES Strongly Lensed Quasars using Neural Posterior Estimation
- Euclid preparation. Estimating galaxy physical properties using CatBoost chained regressors with attention
- Deep inference of simulated strong lenses in ground-based surveys
- Enhancing Gravitational Lens Study with Deep Learning: A Study on Effects of Dropout Regularization