DeepVoid: A Deep Learning Void Detector
arXiv:2504.21134 · doi:10.3847/1538-4357/ae2c80
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 . We then apply the machine learning technique of curricular learning to enable the model to classify structure in data with significantly larger intertracer separation. At the highest tracer separation tested, , the model achieves a void F1 score of 0.89 and a Matthews correlation coefficient of 0.6 on IllustrisTNG subhalos.
23 pages, 9 figures. Submitted to the Astrophysical Journal on 4/25/25. Accepted on 12/11/2025. Published on 02/04/2026
References in corpus (70)
- Planck 2015 results. XIII. Cosmological parameters
- The Seventh Data Release of the Sloan Digital Sky Survey
- Populating a cluster of galaxies - I. Results at z=0
- E pur si muove: Galiliean-invariant cosmological hydrodynamical simulations on a moving mesh
- Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
- The Baryon Oscillation Spectroscopic Survey of SDSS-III
- First results from the IllustrisTNG simulations: matter and galaxy clustering
- First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies
- First results from the IllustrisTNG simulations: the galaxy color bimodality
- First results from the IllustrisTNG simulations: A tale of two elements -- chemical evolution of magnesium and europium
- First results from the IllustrisTNG simulations: radio haloes and magnetic fields
- Euclid. I. Overview of the Euclid mission
- Properties of Dark Matter Haloes in Clusters, Filaments, Sheets and Voids
- A hierarchy of voids: Much ado about nothing
- ZOBOV: a parameter-free void-finding algorithm
- Tracing the cosmic web
- A Dynamical Classification of the Cosmic Web
- An Imprint of Super-Structures on the Microwave Background due to the Integrated Sachs-Wolfe Effect
- A Cosmic Watershed: the WVF Void Detection Technique
- DESI Bright Galaxy Survey: Final Target Selection, Design, and Validation
- The Multiscale Morphology Filter: Identifying and Extracting Spatial Patterns in the Galaxy Distribution
- Cosmic Voids in Sloan Digital Sky Survey Data Release 7
- Target Selection and Validation of DESI Luminous Red Galaxies
- Voids in the PSCz Survey and the Updated Zwicky Catalog
- Precision cosmography with stacked voids
- Learning to Predict the Cosmological Structure Formation
- The Aspen--Amsterdam Void Finder Comparison Project
- Target Selection and Validation of DESI Quasars
- A kinematic classification of the cosmic web
- Target Selection and Validation of DESI Emission Line Galaxies
- Counting voids to probe dark energy
- Voids in massive neutrino cosmologies
- The Hierarchical Structure and Dynamics of Voids
- Beyond BAO: improving cosmological constraints from BOSS with measurement of the void-galaxy cross-correlation
- The High Latitude Spectroscopic Survey on the Nancy Grace Roman Space Telescope
- Simulating nonlinear cosmological structure formation with massive neutrinos
- ORIGAMI: Delineating Halos using Phase-Space Folds
- Reconstructing the Cosmic Velocity and Tidal Fields with Galaxy Groups Selected from the Sloan Digital Sky Survey
- Fast cosmic web simulations with generative adversarial networks
- A robust public catalogue of voids and superclusters in the SDSS Data Release 7 galaxy surveys
- The Void Size Function in Dynamical Dark Energy Cosmologies
- Precision cosmology with voids in the final BOSS data
- Galaxy And Mass Assembly (GAMA): The galaxy luminosity function within the cosmic web
- Simulating Voids
- Cosmological Reconstruction From Galaxy Light: Neural Network Based Light-Matter Connection
- Alignments of Voids in the Cosmic Web
- On the linearity of tracer bias around voids
- The lensing and temperature imprints of voids on the Cosmic Microwave Background
- Void Lensing as a Test of Gravity
- Testing cosmology with a catalogue of voids in the BOSS galaxy surveys
- Euclid: Cosmological forecasts from the void size function
- Classifying the Large Scale Structure of the Universe with Deep Neural Networks
- Cosmological exploitation of the size function of cosmic voids identified in the distribution of biased tracers
- Cosmic voids in modified gravity scenarios
- The Integrated Sachs-Wolfe effect in gravity
- Cosmological constraints from the BOSS DR12 void size function
- The nature of voids: II. Tracing underdensities with biased galaxies
- A volumetric deep Convolutional Neural Network for simulation of mock dark matter halo catalogues
- Field Level Neural Network Emulator for Cosmological N-body Simulations
- An interpretable machine learning framework for dark matter halo formation
- The part and the whole: voids, supervoids, and their ISW imprint
- Halo abundances within the cosmic web
- DIVE in the cosmic web: voids with Delaunay Triangulation from discrete matter tracer distributions
- Cosmology with cosmic web environments I. Real-space power spectra
- Updated void catalogs of the SDSS DR7 main sample
- Observational Constraints on Dynamical Dark Energy Models
- Guess the cheese flavour by the size of its holes: A cosmological test using the abundance of Popcorn voids
- Velocity profiles of matter and biased tracers around voids
- Classification of cosmic structures for galaxies with deep learning: connecting cosmological simulations with observations
- A Comparison of Void-Finding Algorithms using Crossing Numbers