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The Mass–Metallicity Relation and Its Observational Effects at z ∼ 3–6

The correlation between galaxy stellar mass and gas-phase metallicity, known as the mass–metallicity relation (MZR), gives key insights into the processes that govern galaxy evolution. However, unquantified observational and selection biases can result in systematic errors in attempts to recover the...

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Autores principales: Zach Lewis, Michael V. Maseda, Anna de Graaff, Joel Leja, Bingjie Wang, Hans-Walter Rix, Ian McConachie, Nikko J. Cleri, Rachel Bezanson, Leindert A. Boogaard, Gabriel Brammer, Jenny E. Greene, Michaela Hirschmann, Harley Katz, Ivo Labbé, Jorryt Matthee, Tim B. Miller, Rohan P. Naidu, Pascal A. Oesch, David J. Setton, Katherine A. Suess, Andrea Weibel, Katherine E. Whitaker, Christina C. Williams
Formato: Artigo
Lenguaje:Inglês
Publicado: IOP Publishing 2026-01-01
Colección:The Astrophysical Journal
Materias:
Galaxy evolution
Chemical enrichment
Metallicity
Galaxy abundances
Scaling relations
Acceso en línea:https://doi.org/10.3847/1538-4357/ae7bfc
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