EIGER. VI. The Correlation Function, Host Halo Mass, and Duty Cycle of Luminous Quasars at z ≳ 6

We expect luminous ( M _1450 ≲ −26.5) high-redshift quasars to trace the highest-density peaks in the early Universe. Here, we present observations of four z ≳ 6 quasar fields using JWST/NIRCam in the imaging and wide-field slitless spectroscopy mode and report a wide range in the number of detected...

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Autors principals:	Anna-Christina Eilers, Ruari Mackenzie, Elia Pizzati, Jorryt Matthee, Joseph F. Hennawi, Haowen Zhang, Rongmon Bordoloi, Daichi Kashino, Simon J. Lilly, Rohan P. Naidu, Robert A. Simcoe, Minghao Yue, Carlos S. Frenk, John C. Helly, Matthieu Schaller, Joop Schaye
Format:	Artigo
Idioma:	Inglês
Publicat:	IOP Publishing 2024-01-01
Col·lecció:	The Astrophysical Journal
Matèries:	Quasars Supermassive black holes Clustering Astrostatistics techniques Galaxy dark matter halos High-redshift galaxy clusters
Accés en línia:	https://doi.org/10.3847/1538-4357/ad778b
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