Explaining JWST Counts with Galaxy Formation Models

A distinct power-law break is apparent at m _AB  ∼ 21 in the deep near-infrared PEARLS-JWST galaxy counts. The break becomes more pronounced at longer wavelengths, with the slope flattening smoothly with apparent magnitude in the shortest band used at 0.9 μ m, and trending toward an increasingly bro...

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主要な著者:	Giorgio Manzoni, Tom Broadhurst, Jeremy Lim, Tao Liu, George Smoot, Carlton M. Baugh, Scott Tompkins, Rogier Windhorst, Simon Driver, Timothy Carleton, Brenda Frye, Leo Fung, Jiashuo Zhang, Seth H. Cohen, Christopher J. Conselice, Norman A. Grogin, Rolf A. Jansen, Anton M. Koekemoer, Rafael Ortiz III, Norbert Pirzkal, Christopher N. A. Willmer
フォーマット:	Artigo
言語:	Inglês
出版事項:	IOP Publishing 2025-01-01
シリーズ:	The Astrophysical Journal
主題:	Galaxy formation Galaxy counts Galaxy evolution Observational cosmology James Webb Space Telescope Astronomical simulations
オンライン･アクセス:	https://doi.org/10.3847/1538-4357/ade700
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