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The z = 7.08 Quasar ULAS J1120+0641 May Never Reach a “Normal” Black Hole to Stellar Mass Ratio
Meredith A. Stone, George H. Rieke, Jianwei 建伟 Lyu 吕, Michael K. Florian, Kevin N. Hainline, Yang Sun and Yongda Zhu The Astrophysical Journal 993(2) 168 (2025) https://doi.org/10.3847/1538-4357/ae062a
Spectral Variability Studies in Active Galactic Nuclei: Exploring Continuum and Emission Line Regions in the Age of LSST and JWST
Swayamtrupta Panda, Paola Marziani, Bożena Czerny, Alberto Rodríguez-Ardila and Francisco Pozo Nuñez Universe 9(12) 492 (2023) https://doi.org/10.3390/universe9120492
Characterising SMSS J2157–3602, the most luminous known quasar, with accretion disc models
Samuel Lai (赖民希), Christian Wolf, Christopher A Onken and Fuyan Bian (边福彦) Monthly Notices of the Royal Astronomical Society 521(3) 3682 (2023) https://doi.org/10.1093/mnras/stad651
The disk–torus system in active galactic nuclei: possible evidence of highly spinning black holes
A novel black hole mass scaling relation based on coronal gas, and its dependence with the accretion disc
Almudena Prieto, Alberto Rodríguez-Ardila, Swayamtrupta Panda and Murilo Marinello Monthly Notices of the Royal Astronomical Society 510(1) 1010 (2021) https://doi.org/10.1093/mnras/stab3414
Cosmic Spin and Mass Evolution of Black Holes and Its Impact
WISDOM project – VI. Exploring the relation between supermassive black hole mass and galaxy rotation with molecular gas
Mark D Smith, Martin Bureau, Timothy A Davis, et al. Monthly Notices of the Royal Astronomical Society 500(2) 1933 (2020) https://doi.org/10.1093/mnras/staa3274