Learning the cosmic web: graph-based classification of simulated galaxies by their dark matter environments

ABSTRACT We present a novel graph-based machine learning classifier for identifying the dark matter cosmic web environments of galaxies. Large galaxy surveys offer comprehensive statistical views of how galaxy properties are shaped by large-scale structure, but this requires robust classifications of galaxies’ cosmic web environments. Using stellar mass-selected IllustrisTNG-300 galaxies, we apply a three-stage, simulation-based framework to link galaxies to the total (mainly dark) underlying matter distribution. Here, we apply the following three steps: First, we assign the positions of simulated galaxies to a void, wall, filament, or cluster environment using the T-web classification of the underlying matter distribution. Secondly, we construct a Delaunay triangulation of the galaxy distribution to summarize the local geometric structure with ten graph metrics for each galaxy. Thirdly, we train a graph attention network (GAT) on each galaxy’s graph metrics to predict its cosmic web environment. For galaxies with stellar mass $\mathrm{\gt 10^9 {\rm M}_{\odot }}$, our GAT+ model achieves an accuracy of $85~{{\rm per\ cent}}$, outperforming graph-agnostic multilayer perceptrons and graph convolutional networks. Our results demonstrate that graph-based representations of galaxy positions provide a powerful and physically meaningful way to infer dark matter environments. We plan to apply this simulation-based graph modelling to investigate how the properties of observed galaxies from the Dark Energy Spectroscopic Instrument (DESI) survey are influenced by their dark matter environments.