Probing the Star Formation Main Sequence Down to 108 M ⊙ at 1.0 < z < 3.0

Probing the Star Formation Main Sequence Down to 108 M ⊙ at 1.0 < z < 3.0

We investigate the star formation main sequence (MS; SFR– M _⋆ ) down to 10 ^8−9 M _⊙ using a sample of 34,061 newly discovered ultrafaint (27 mag ≲ i ≲ 30 mag) galaxies at 1 < z < 3 detected in the GOODS-N field. Virtually none of these galaxies are contained in previous public catalogs, effe...

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Bibliographic Details
Main Authors: Rosa M. Mérida, Pablo G. Pérez-González, Patricia Sánchez-Blázquez, Ángela García-Argumánez, Marianna Annunziatella, Luca Costantin, Alejandro Lumbreras-Calle, Belén Alcalde-Pampliega, Guillermo Barro, Néstor Espino-Briones, Anton M. Koekemoer
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
High-redshift galaxies
Dwarf galaxies
Galaxy formation
Galaxy evolution
Galaxies
Star formation
Online Access:https://doi.org/10.3847/1538-4357/acc7a3

Internet

https://doi.org/10.3847/1538-4357/acc7a3

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