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From the 1 of 7 linked papers with an AI index.

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20242026
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astro-ph.GA2026

Enabling Cosmic Web Analysis at Gigaparsec Scales: A Multi Block Approach for DisPerSE

Ankit Singh, Frazer Pearce, Meghan Gray +1

The paper introduces a frozen‑core, multi‑block technique that enables the DisPerSE filament finder to process gigaparsec‑scale cosmological simulations by preserving global topolo…

astro-ph.GA2026

Identifying group galaxies merging with massive clusters using machine learning

Rhys Jordan, Meghan E. Gray, Alfonso Aragón-Salamanca +3

The environment plays a critical role in galaxy evolution, with galaxy clusters and their infall regions offering diverse conditions that shape galaxies before they enter the dense…

astro-ph.GA2025

The life and times of dark matter haloes: what will I be when I grow up?

Julian Onions, Frazer Pearce, Alexander Knebe +6

Are the most massive objects in the Universe today the direct descendants of the most massive objects at higher redshift? We address this question by tracing the evolutionary histo…

astro-ph.GA2024

The effect of cosmic web filaments on galaxy evolution

Callum J. O'Kane, Ulrike Kuchner, Meghan E. Gray +1

Galaxy properties are known to be affected by their environment. This is well established for the extremes of the density scales, between the high-density cluster environment and t…

astro-ph.GA2024

Reconsidering the dynamical states of galaxy clusters using PCA and UMAP

Roan Haggar, Federico De Luca, Marco De Petris +10

Numerous metrics exist to quantify the dynamical state of galaxy clusters, both observationally and within simulations. Many of these correlate strongly with one another, but it is…