Tracing Galaxy Bias Through the Cosmic Web: The Role of Filaments

arXiv:2608.25060 · astro-ph.GA, astro-ph.CO · Submitted 2026-08-25 · Read on arXiv

astro-ph.GA, astro-ph.CO

Submitted: 2026-08-25

Updated: 2026-08-25

Comments: Submitted to A&A, 14 pages, 13 figures

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Clustering — 6× in this paper · explained in 2 episodes
• Trace — 5× in this paper · explained in 2 episodes
• Anisotropy — 3× in this paper · explained in 3 episodes
• Accuracy — 1× in this paper · explained in 1 episode
• Alignment — 1× in this paper · explained in 1 episode
• Fidelity — 1× in this paper · explained in 2 episodes
• Matter Power Spectrum — 1× in this paper · explained in 2 episodes
• Non-Gaussianity — 1× in this paper · explained in 2 episodes
• Primordial non-Gaussianity — 1× in this paper · explained in 2 episodes
• Robustness — 1× in this paper · explained in 5 episodes

Sources

• The Galaxy Bias Profile of Cosmic Voids:A Comparison of Void Finders
• The role of filaments in the large-scale conformity signal
• The Evolution of the Spin Alignments of Dark Matter Halos in the Cosmic Web
• Large Scale Structure and the Cosmic Web

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