Shape-Preserving Evolution of the Global Ultraviolet Quasar Luminosity Function to z 7.5

arXiv:2606.22415 · astro-ph.CO · Submitted 2026-06-21 · Read on arXiv

Wenjie Wang, Zunli Yuan, Yu Luo, Longhua Qin

astro-ph.CO

Submitted: 2026-06-21

Comments: 25 pages, 10 figures, submitted to ApJ

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

Terminology

• AGN — 5× in this paper · explained in 1 episode
• Abundance — 4× in this paper · explained in 1 episode
• Robustness — 4× in this paper · explained in 5 episodes
• Active Galactic Nuclei (AGN) — 1× in this paper · explained in 1 episode
• Chebyshev Polynomials — 1× in this paper · explained in 2 episodes
• Markov Chain Monte Carlo — 1× in this paper

Sources

• Distance measures in cosmology
• The Steep-spectrum Radio-loud AGN Luminosity Function and Its Implications for Black Hole Growth and Star Formation

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