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Probing the star formation main sequence down to 107 M⊙ at 1  <  z  <  9

The main sequence of star-forming galaxies (SFGMS or MS) is a fundamental scaling relation that provides a global framework for studying galaxy formation and evolution, as well as an insight into the complex star formation histories (SFHs) of individual galaxies. In this work, we combine large-area...

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Furkejuvvon:
Váldodahkkit: Mérida Rosa M., Sawicki Marcin, Iyer Kartheik G., Noirot Gaël, Willott Chris J., Bradač Maruša, Desprez Guillaume, Martis Nicholas S., Muzzin Adam, Rihtaršič Gregor, Sarrouh Ghassan T. E., Favaro Jeremy, Gaspar Gaia, Harshan Anishya, Judež Jon
Materiálatiipa: Artigo
Giella:Inglês
Almmustuhtton: EDP Sciences 2026-03-01
Ráidu:Astronomy & Astrophysics
Fáttát:
galaxies: evolution
galaxies: high-redshift
galaxies: photometry
galaxies: star formation
Liŋkkat:https://www.aanda.org/articles/aa/full_html/2026/03/aa57448-25/aa57448-25.html
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