Baryonic assembly bias in X-ray-selected galaxy groups and clusters: insights from the Magneticum simulation

arXiv:2607.03746 · astro-ph.CO · Submitted 2026-07-04 · Read on arXiv

astro-ph.CO

Submitted: 2026-07-04

Updated: 2026-09-07

Comments: Accepted for publication in Astronomy & Astrophysics. 11 pages, 6 figures. Abstract adapted to ArXiv

Code: https://github.com/franciscovillaescusa/Pylians

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

Terminology

Clustering — 75× in this paper · explained in 2 episodes
Trace — 10× in this paper · explained in 2 episodes
Aperture — 6× in this paper · explained in 1 episode
AGN — 4× in this paper · explained in 1 episode
Robustness — 4× in this paper · explained in 5 episodes
AGN Feedback — 2× in this paper · explained in 1 episode
Abundance — 2× in this paper · explained in 1 episode
Calibration — 2× in this paper · explained in 7 episodes
Consistency — 2× in this paper · explained in 3 episodes
European Research Council — 2× in this paper
Accretion Shock — 1× in this paper · explained in 1 episode
Active Galactic Nuclei (AGN) — 1× in this paper · explained in 1 episode
Agenzia Spaziale Italiana — 1× in this paper
Core — 1× in this paper · explained in 2 episodes
Matter Power Spectrum — 1× in this paper · explained in 2 episodes
Metallicity — 1× in this paper · explained in 3 episodes
National Recovery and Resilience Plan — 1× in this paper
Weak Lensing — 1× in this paper · explained in 2 episodes

Sources

Modelling the uv/x-ray cosmic background with CUBA

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