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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Principais autores:	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:	Artigo
Jezik:	Inglês
Izdano:	IOP Publishing 2025-01-01
Serija:	The Astrophysical Journal
Teme:	Active galactic nuclei Star formation James Webb Space Telescope Galaxy formation Galaxy evolution
Online dostop:	https://doi.org/10.3847/1538-4357/adf19e
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