AGN X-ray coronae at high luminosity: A broadband study of RBS 229 and PG 1407+265

arXiv:2609.01265 · astro-ph.HE · Submitted 2026-09-01 · Read on arXiv

astro-ph.HE

Submitted: 2026-09-01

Updated: 2026-09-01

Comments: 17 pages, 11 figures, accepted for publication in Astronomy & Astrophysics

DOI: 10.1051/0004-6361/202660733

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

Terminology

• AGN — 38× in this paper · explained in 1 episode
• Calibration — 8× in this paper · explained in 7 episodes
• Optical Monitor — 4× in this paper
• Abundance — 2× in this paper · explained in 1 episode
• Consistency — 1× in this paper · explained in 3 episodes
• Core — 1× in this paper · explained in 2 episodes
• Trace — 1× in this paper · explained in 2 episodes
• alpha — 1× in this paper · explained in 1 episode

Sources

• Supermassive Black Hole Winds in X-rays: SUBWAYS V. Properties of hot coronae in quasars at intermediate redshift

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