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.
Authors
- Kelly A. Douglass (ORCID: https://orcid.org/0000-0002-9540-546X)
- Mark C. Neyrinck (ORCID: https://orcid.org/0000-0002-2618-5790)
- Shunichi Kumagai (ORCID: https://orcid.org/0000-0002-0352-7903)
- Miguel A. Aragón-Calvo (ORCID: https://orcid.org/0000-0003-0615-3975)
- S. BenZvi (ORCID: https://orcid.org/0000-0001-5537-4710)
- Michael S. Vogeley (ORCID: https://orcid.org/0000-0001-7416-9800)
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