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Cited article:

From Sub-Solar to Super-Solar Chemical Abundances along the Quasar Main Sequence

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Discovery of a hyperluminous quasar at z = 1.62 with Eddington ratio >3 in the eFEDS field confirmed by KOOLS-IFU on Seimei Telescope

Yoshiki Toba, Keito Masu, Naomi Ota, Zhen-Kai Gao, Masatoshi Imanishi, Anri Yanagawa, Satoshi Yamada, Itsuki Dosaka, Takumi Kakimoto, Seira Kobayashi, Neiro Kurokawa, Aika Oki, Sorami Soga, Kohei Shibata, Sayaka Takeuchi, Yukana Tsujita, Tohru Nagao, Masayuki Tanaka, Yoshihiro Ueda and Wei-Hao Wang
Publications of the Astronomical Society of Japan 76 (6) 1173 (2024)
https://doi.org/10.1093/pasj/psae078

Chemical abundances along the quasar main sequence

A. Floris, P. Marziani, S. Panda, M. Sniegowska, M. D’Onofrio, A. Deconto-Machado, A. del Olmo and B. Czerny
Astronomy & Astrophysics 689 A321 (2024)
https://doi.org/10.1051/0004-6361/202450458

Exploring the links between quasar winds and radio emission along the main sequence at high redshift

A. Deconto-Machado, A. del Olmo and P. Marziani
Astronomy & Astrophysics 691 A15 (2024)
https://doi.org/10.1051/0004-6361/202449976

Accretion/Ejection Phenomena and Emission-Line Profile (A)symmetries in Type-1 Active Galactic Nuclei

Paola Marziani
Symmetry 15 (10) 1859 (2023)
https://doi.org/10.3390/sym15101859