Neural Network Prediction of Strong Lensing Systems with Domain Adaptation and Uncertainty Quantification

Fuente: arXiv
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Autores principales: Agarwal, Shrihan, Ćiprijanović, Aleksandra, Nord, Brian D.
Formato: Preprint
Publicado: 2024
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author Agarwal, Shrihan
Ćiprijanović, Aleksandra
Nord, Brian D.
author_facet Agarwal, Shrihan
Ćiprijanović, Aleksandra
Nord, Brian D.
contents Modeling strong gravitational lenses is computationally expensive for the complex data from modern and next-generation cosmic surveys. Deep learning has emerged as a promising approach for finding lenses and predicting lensing parameters, such as the Einstein radius. Mean-variance Estimators (MVEs) are a common approach for obtaining aleatoric (data) uncertainties from a neural network prediction. However, neural networks have not been demonstrated to perform well on out-of-domain target data successfully - e.g., when trained on simulated data and applied to real, observational data. In this work, we perform the first study of the efficacy of MVEs in combination with unsupervised domain adaptation (UDA) on strong lensing data. The source domain data is noiseless, and the target domain data has noise mimicking modern cosmology surveys. We find that adding UDA to MVE increases the accuracy on the target data by a factor of about two over an MVE model without UDA. Including UDA also permits much more well-calibrated aleatoric uncertainty predictions. Advancements in this approach may enable future applications of MVE models to real observational data.
format Preprint
id arxiv_https___arxiv_org_abs_2411_03334
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Neural Network Prediction of Strong Lensing Systems with Domain Adaptation and Uncertainty Quantification
Agarwal, Shrihan
Ćiprijanović, Aleksandra
Nord, Brian D.
Instrumentation and Methods for Astrophysics
Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
Artificial Intelligence
Machine Learning
Modeling strong gravitational lenses is computationally expensive for the complex data from modern and next-generation cosmic surveys. Deep learning has emerged as a promising approach for finding lenses and predicting lensing parameters, such as the Einstein radius. Mean-variance Estimators (MVEs) are a common approach for obtaining aleatoric (data) uncertainties from a neural network prediction. However, neural networks have not been demonstrated to perform well on out-of-domain target data successfully - e.g., when trained on simulated data and applied to real, observational data. In this work, we perform the first study of the efficacy of MVEs in combination with unsupervised domain adaptation (UDA) on strong lensing data. The source domain data is noiseless, and the target domain data has noise mimicking modern cosmology surveys. We find that adding UDA to MVE increases the accuracy on the target data by a factor of about two over an MVE model without UDA. Including UDA also permits much more well-calibrated aleatoric uncertainty predictions. Advancements in this approach may enable future applications of MVE models to real observational data.
title Neural Network Prediction of Strong Lensing Systems with Domain Adaptation and Uncertainty Quantification
topic Instrumentation and Methods for Astrophysics
Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
Artificial Intelligence
Machine Learning
url https://arxiv.org/abs/2411.03334