Pinpointing the cosmic web between massive galaxy clusters I. The incidence of HI and OVI as WHIM tracers

arXiv:2610.11203 · astro-ph.CO · Submitted 2026-10-08 · Read on arXiv

astro-ph.CO

Submitted: 2026-10-08

Updated: 2026-10-08

Code: https://github.com/linetools/linetools

Terminology

• Trace — 16× in this paper · explained in 2 episodes
• Hubble Space Telescope — 2× in this paper
• Metallicity — 2× in this paper · explained in 3 episodes
• Velocity Dispersion — 2× in this paper · explained in 2 episodes
• AGN — 1× in this paper · explained in 1 episode
• Abundance — 1× in this paper · explained in 1 episode
• Active Galactic Nuclei (AGN) — 1× in this paper · explained in 1 episode
• Calibration — 1× in this paper · explained in 7 episodes
• Cosmic Origins Spectrograph — 1× in this paper
• N-body simulations — 1× in this paper · explained in 2 episodes
• Robustness — 1× in this paper · explained in 5 episodes
• Weak Lensing — 1× in this paper · explained in 2 episodes

Sources

• A Survey of H I and O VI Absorption Lines in the Outskirts of $z\lesssim0.3$ Galaxy Clusters

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