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Environmental Evidence for Overly Massive Black Holes in Low-mass Galaxies and a Black Hole–Halo Mass Relation at z ∼ 5

JWST observations have unveiled faint active galactic nuclei (AGNs) at high redshift that provide insights into the formation of supermassive black holes (SMBHs). However, disentangling their stellar from AGN light is challenging. Here, we use an empirical approach to infer the average stellar mass...

Whakaahuatanga katoa

I tiakina i:
Ngā kaituhi matua: Jorryt Matthee, Rohan P. Naidu, Gauri Kotiwale, Lukas J. Furtak, Ivan Kramarenko, Ruari Mackenzie, Jenny Greene, Angela Adamo, Rychard J. Bouwens, Claudia Di Cesare, Anna-Christina Eilers, Anna de Graaff, Kasper E. Heintz, Daichi Kashino, Michael V. Maseda, Sandro Tacchella, Alberto Torralba
Hōputu: Artigo
Reo:Inglês
I whakaputaina: IOP Publishing 2025-01-01
Rangatū:The Astrophysical Journal
Ngā marau:
AGN host galaxies
High-redshift galaxies
Early universe
Quasars
Emission line galaxies
Galaxies
Urunga tuihono:https://doi.org/10.3847/1538-4357/ade886
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