Measuring the gas reservoirs in 108 < M⋆ < 1011 M⊙ galaxies at 1 ≤ z ≤ 3

Context. Understanding the gas content in galaxies, along with its consumption and replenishment, is vital to our grasp of the evolution of the Universe. Numerous studies have addressed this notion, utilizing various observational tools and analytical methods. These include examining low-transition...

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Bibliographic Details
Published in:Astronomy and astrophysics (Berlin) 2024-06, Vol.686
Main Authors: Mérida, Rosa M, Gómez-Guijarro, Carlos, Pérez-González, Pablo G, Sánchez-Blázquez, Patricia, Elbaz, David, Franco, Maximilien, Lucas, Leroy, Magdis, Georgios E, Magnelli, Benjamin, Xiao, Mengyuan
Format: Article
Language:English
Subjects:
Far infrared radiation
Galaxies
Reservoirs
Star formation
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Summary:Context. Understanding the gas content in galaxies, along with its consumption and replenishment, is vital to our grasp of the evolution of the Universe. Numerous studies have addressed this notion, utilizing various observational tools and analytical methods. These include examining low-transition 12CO millimeter rotational lines and exploring the far-infrared and the (sub-)millimeter emission of galaxies. With the capabilities of present-day facilities, much of this research has been centered on relatively bright galaxies. Aims. This study is aimed at exploring the gas reservoirs of a more general type of galaxy population at 1.0 
ISSN:0004-6361
1432-0746
DOI:10.1051/0004-6361/202348661