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Publication Details
AFRICAN RESEARCH NEXUS
SHINING A SPOTLIGHT ON AFRICAN RESEARCH
earth and planetary sciences
The MOSDEF Survey: The Evolution of the Mass-Metallicity Relation from z = 0 to z ∼ 3.3
Astrophysical Journal, Volume 914, No. 1, Article 19, Year 2021
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Description
We investigate the evolution of galaxy gas-phase metallicity (O/H) over the range z = 0-3.3 using samples of ∼300 galaxies at z ∼ 2.3 and ∼150 galaxies at z ∼ 3.3 from the MOSDEF survey. This analysis crucially utilizes different metallicity calibrations at z ∼ 0 and z > 1 to account for evolving interstellar medium (ISM) conditions. We find significant correlations between O/H and stellar mass (M ∗) at z ∼ 2.3 and z ∼ 3.3. The low-mass power-law slope of the mass-metallicity relation (MZR) is remarkably invariant over z = 0-3.3, such that O/H ∝ M∗0.30 at all redshifts in this range. At fixed M ∗, O/H decreases with increasing redshift as dlog(O/H)/dz = -0.11 ± 0.02. We find no evidence that the fundamental metallicity relation between M ∗, O/H, and star formation rate evolves out to z ∼ 3.3. We employ analytic chemical evolution models to place constraints on the mass and metal loading factors of galactic outflows. The efficiency of metal removal increases toward lower M ∗ at fixed redshift and toward higher redshift at fixed M ∗. These models suggest that the slope of the MZR is primarily set by the scaling of the outflow metal loading factor with M ∗, not by the change in gas fraction as a function of M ∗. The evolution toward lower O/H at fixed M ∗ with increasing redshift is driven by both higher gas fraction (leading to stronger dilution of ISM metals) and higher metal removal efficiency. These results suggest that the processes governing the smooth baryonic growth of galaxies via gas flows and star formation hold in the same form over at least the past 12 Gyr. © 2021. The American Astronomical Society. All rights reserved..
Authors & Co-Authors
Sanders, Ryan L.
United States, Davis
University of California, Davis
Shapley, Alice E.
United States, Los Angeles
University of California, Los Angeles
Reddy, Naveen A.
United States, Riverside
University of California, Riverside
Kriek, Mariska T.
United States, Berkeley
University of California, Berkeley
Siana, Brian D.
United States, Riverside
University of California, Riverside
Coil, Alison L.
United States, La Jolla
University of California, San Diego
Mobasher, Bahram
United States, Riverside
University of California, Riverside
Shivaei, Irene
United States, Tucson
The University of Arizona
Dav́e, Romeel
United Kingdom, Edinburgh
The University of Edinburgh
Azadi, Mojegan
United States, Cambridge
Harvard-smithsonian Center for Astrophysics
Price, Sedona H.
Germany, Garching Bei Munchen
Max Planck Institute for Extraterrestrial Physics
Leung, Gene C.K.
United States, Austin
The University of Texas at Austin
Freeman, William R.
United States, Riverside
University of California, Riverside
Fetherolf, Tara
United States, Riverside
University of California, Riverside
Barro, Guillermo
United States, Stockton
University of the Pacific, California
Statistics
Citations: 97
Authors: 15
Affiliations: 12
Identifiers
Doi:
10.3847/1538-4357/abf4c1
ISSN:
0004637X
Study Design
Cross Sectional Study
Study Approach
Quantitative