The slope and scatter of the star-forming main sequence at z ∼ 5: Reconciling observations with simulations

Galaxies exhibit a tight correlation between their star formation rate (SFR) and stellar mass over a wide redshift range known as the star-forming main sequence (SFMS). With JWST, the SFMS can now be investigated at high redshifts down to masses of ∼106 M⊙, using sensitive star formation rate tracer...

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Detalhes bibliográficos

Principais autores:	Di Cesare Claudia, Matthee Jorryt, Naidu Rohan P., Torralba Alberto, Kotiwale Gauri, Kramarenko Ivan G., Blaizot Jeremy, Rosdahl Joakim, Leja Joel, Iani Edoardo, Adamo Angela, Covelo-Paz Alba, Furtak Lukas J., Heintz Kasper E., Mascia Sara, Navarrete Benjamín, Oesch Pascal A., Romano Michael, Shivaei Irene, Tacchella Sandro
Formato:	Artigo
Idioma:	Inglês
Publicado em:	EDP Sciences 2026-03-01
coleção:	Astronomy & Astrophysics
Assuntos:	galaxies: evolution galaxies: high-redshift galaxies: star formation
Acesso em linha:	https://www.aanda.org/articles/aa/full_html/2026/03/aa57790-25/aa57790-25.html
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