Efficiently emulating distribution functions in gigaparsec volumes for varying cosmological parameters

arXiv:2604.17981 · astro-ph.CO, astro-ph.GA · Submitted 2026-04-20 · Read on arXiv

astro-ph.CO, astro-ph.GA

Submitted: 2026-04-20

Updated: 2026-09-27

Terminology

Abundance — 4× in this paper · explained in 1 episode
AGN — 3× in this paper · explained in 1 episode
AGN Feedback — 3× in this paper · explained in 1 episode
Accuracy — 3× in this paper · explained in 1 episode
Calibration — 3× in this paper · explained in 7 episodes
Clustering — 3× in this paper · explained in 2 episodes
Fidelity — 2× in this paper · explained in 2 episodes
Systematic Bias — 2× in this paper · explained in 3 episodes
Active Learning — 1× in this paper · explained in 6 episodes
Adam — 1× in this paper · explained in 2 episodes
Core — 1× in this paper · explained in 2 episodes
Matter Power Spectrum — 1× in this paper · explained in 2 episodes
Pruning — 1× in this paper · explained in 4 episodes
Simulation-based Inference — 1× in this paper · explained in 2 episodes
Trace — 1× in this paper · explained in 2 episodes
Transformer — 1× in this paper · explained in 2 episodes
Transformer Architecture — 1× in this paper · explained in 2 episodes

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