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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Autores principales:	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
Formato:	Artigo
Lenguaje:	Inglês
Publicado:	IOP Publishing 2024-01-01
Colección:	The Astrophysical Journal
Materias:	Quasars Supermassive black holes Clustering Astrostatistics techniques Galaxy dark matter halos High-redshift galaxy clusters
Acceso en línea:	https://doi.org/10.3847/1538-4357/ad778b
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