Self-consistent JWST Census of Star Formation and AGN Activity at z = 5.5–13.5

Self-consistent JWST Census of Star Formation and AGN Activity at z = 5.5–13.5

The cosmic star formation history (CSFH) and cosmic active galactic nuclei (AGN) luminosity history (CAGNH) are self consistently measured at z  = 5.5–13.5. This is achieved by analyzing galaxies detected by the James Webb Space Telescope from $\approx 400\,{{\rm{arcmin}}}^{2}$ fields from the Prime...

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Bibliographic Details
Main Authors: Jordan C. J. D’Silva, Simon P. Driver, Claudia D. P. Lagos, Aaron S. G. Robotham, Nathan J. Adams, Christopher J. Conselice, Brenda Frye, Nimish P. Hathi, Thomas Harvey, Anton M. Koekemoer, Rafael Ortiz III, Massimo Ricotti, Clayton Robertson, Michael J. Rutkowski, Ross M. Silver, Stephen M. Wilkins, Christopher N. A. Willmer, Rogier A. Windhorst, Seth H. Cohen, Rolf A. Jansen, Jake Summers, Dan Coe, Norman A. Grogin, Madeline A. Marshall, Mario Nonino, Nor Pirzkal, Russell E. Ryan Jr., Haojing Yan
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Active galactic nuclei
Star formation
James Webb Space Telescope
Galaxy formation
Galaxy evolution
Online Access:https://doi.org/10.3847/1538-4357/adf19e
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https://doi.org/10.3847/1538-4357/adf19e

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