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The evolution of the mass-metallicity relations from the VANDELS survey and the GAEA Semi-Analytic model

In this work, we study the evolution of the mass-metallicity relations (MZRs) as predicted by the GAlaxy Evolution and Assembly (GAEA) semi-analytic model. We contrast these predictions with recent results from the VANDELS survey, that allows us to expand the accessible redshift range for the stella...

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Published in:arXiv.org 2021-04
Main Authors: Fontanot, Fabio, Calabrò, Antonello, Talia, Margherita, Mannucci, Filippo, Castellano, Marco, Cresci, Giovanni, Gabriella De Lucia, Gallazzi, Anna, Hirschmann, Michaela, Pentericci, Laura, Xie, Lizhi, Amorin, Ricardo, Bolzonella, Micol, Bongiorno, Angela, Cucciati, Olga, Cullen, Fergus, Fynbo, Johan P U, Hathi, Nimish, Hibon, Pascale, McLure, Ross J, Pozzetti, Lucia
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creator Fontanot, Fabio
Calabrò, Antonello
Talia, Margherita
Mannucci, Filippo
Castellano, Marco
Cresci, Giovanni
Gabriella De Lucia
Gallazzi, Anna
Hirschmann, Michaela
Pentericci, Laura
Xie, Lizhi
Amorin, Ricardo
Bolzonella, Micol
Bongiorno, Angela
Cucciati, Olga
Cullen, Fergus
Fynbo, Johan P U
Hathi, Nimish
Hibon, Pascale
McLure, Ross J
Pozzetti, Lucia
description In this work, we study the evolution of the mass-metallicity relations (MZRs) as predicted by the GAlaxy Evolution and Assembly (GAEA) semi-analytic model. We contrast these predictions with recent results from the VANDELS survey, that allows us to expand the accessible redshift range for the stellar MZR up to \(z\sim3.5\). We complement our study by considering the evolution of the gas-phase MZR in the same redshift range. We show that GAEA is able to reproduce the observed evolution of the \(z
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subjects Galactic evolution
Mathematical models
Metallicity
Red shift
Star & galaxy formation
Star formation rate
Stellar evolution
Stellar mass
title The evolution of the mass-metallicity relations from the VANDELS survey and the GAEA Semi-Analytic model
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