DeepVoid: A Deep Learning Void Detector

Abstract We present DeepVoid, an application of deep learning trained on a physical definition of cosmic voids to detect voids in density fields and galaxy distributions. By semantically segmenting the IllustrisTNG simulation volume using the tidal tensor, we train a deep convolutional neural network to classify local structure using a U-Net architecture for training and prediction. The model achieves a void F1 score of 0.96 and a Matthews correlation coefficient over all structural classes of 0.81 for dark matter particles in IllustrisTNG with interparticle spacing of λ = 0.33 h −1 Mpc. We then apply the machine learning technique of curriculum learning to enable the model to classify structure in data with significantly larger intertracer separation. At the highest tracer separation tested, λ = 10 h −1 Mpc, the model achieves a void F1 score of 0.89 and a Matthews correlation coefficient of 0.6 on IllustrisTNG subhalos.

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Publication Details

Journal
The Astrophysical Journal
Published
2026-02-04
DOI
https://doi.org/10.3847/1538-4357/ae2c80
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
0.00
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article

DeepVoid: A Deep Learning Void Detector

Kelly A. Douglass, Mark C. Neyrinck, Shunichi Kumagai, Miguel A. Aragón-Calvo et al.
The Astrophysical Journal
Dark Matter and Cosmic Phenomena
article

DeepVoid: A Deep Learning Void Detector

Kelly A. Douglass, Mark C. Neyrinck, Shunichi Kumagai, Miguel A. Aragón-Calvo, S. BenZvi, Michael S. Vogeley
article en

Abstract

Abstract We present DeepVoid, an application of deep learning trained on a physical definition of cosmic voids to detect voids in density fields and galaxy distributions. By semantically segmenting the IllustrisTNG simulation volume using the tidal tensor, we train a deep convolutional neural network to classify local structure using a U-Net architecture for training and prediction. The model achieves a void F1 score of 0.96 and a Matthews correlation coefficient over all structural classes of 0.81 for dark matter particles in IllustrisTNG with interparticle spacing of λ = 0.33 h −1 Mpc. We then apply the machine learning technique of curriculum learning to enable the model to classify structure in data with significantly larger intertracer separation. At the highest tracer separation tested, λ = 10 h −1 Mpc, the model achieves a void F1 score of 0.89 and a Matthews correlation coefficient of 0.6 on IllustrisTNG subhalos.

The Astrophysical JournalVol. 998(1)
Openalex Percentile: Top 96%
Dark Matter and Cosmic Phenomena
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