The role of filaments in the large-scale conformity signal

arXiv:2607.22838 · astro-ph.GA · Submitted 2026-07-24 · Read on arXiv

Daniela Palma, Ivan Lacerna, Noelia Pérez, Luis Pereyra, Antonio D. Montero-Dorta, Constanza A. Soto-Suárez, Laerte Sodré, M. Celeste Artale, Amrutha Belwadi, Facundo Rodriguez, Nelvy Choque-Challapa

astro-ph.GA

Submitted: 2026-07-24

Comments: 20 pages, 15 figures. Revised version submitted to Astronomy & Astrophysics

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

Terminology

• Robustness — 5× in this paper · explained in 5 episodes
• Trace — 5× in this paper · explained in 2 episodes
• Consistency — 3× in this paper · explained in 3 episodes
• AGN — 2× in this paper · explained in 1 episode
• AGN Feedback — 2× in this paper · explained in 1 episode
• Abundance — 2× in this paper · explained in 1 episode
• Clustering — 1× in this paper · explained in 2 episodes

Sources

• Connecting clustering and the cosmic web:Observational constraints on secondary halo bias
• Environmental history of filament galaxies: stellar mass assembly and star-formation of filament galaxies

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