Probing the Star Formation Main Sequence down to \(10^{8}\) M\(_\odot\) at \(1.0<z<3.0\)

We investigate the star formation main sequence (MS) (SFR-M\(_{\star}\)) down to 10\(^{8-9}\mathrm{M}_\odot\) using a sample of 34,061 newly-discovered ultra-faint (\(27\lesssim i \lesssim 30\) mag) galaxies at \(1

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Bibliographic Details
Published in:arXiv.org 2023-03
Main Authors: Mérida, Rosa M, Pérez-González, Pablo G, Sánchez-Blázquez, Patricia, García-Argumánez, Ángela, Annunziatella, Marianna, Costantin, Luca, Lumbreras-Calle, Alejandro, Alcalde-Pampliega, Belén, Barro, Guillermo, Espino-Briones, Néstor, Koekemoer, Anton M
Format: Article
Language:English
Subjects:
Star & galaxy formation
Star formation
Starburst galaxies
Stellar populations
Online Access:Get full text
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Description
Summary:We investigate the star formation main sequence (MS) (SFR-M\(_{\star}\)) down to 10\(^{8-9}\mathrm{M}_\odot\) using a sample of 34,061 newly-discovered ultra-faint (\(27\lesssim i \lesssim 30\) mag) galaxies at \(1
ISSN:2331-8422
DOI:10.48550/arxiv.2303.16234