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The mass-metallicity relation at z ∼ 0.7
conference contribution
posted on 2024-08-06, 12:09 authored by S. Savaglio, Karl GlazebrookKarl Glazebrook, D. Le Borgne, S. Juneau, R. G. Abraham, D. Crampton, P. J.P. McCarthy, H. W. Chen, R. Marzke, R. G. Carlberg, I. Jøgensen, K. Roth, I. Hook, R. MurowinskiThe ISM metallicity and the stellar mass are examined in a sample of 66 galaxies at 0.4 < z < 1, selected from the Gemini Deep Deep Survey (GDDS) and the Canada-France Redshift Survey (CFRS). We observe a mass-metallicity relation similar to that seen in z ~ 0.1 SDSS galaxies, but displaced towards higher masses and/or lower metallicities. Using this sample, and a small sample of z ~ 2.3 LBGs, a redshift dependent mass-metallicity relation is proposed which describes the observed results.
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735402469ISSN
0094-243XJournal title
AIP Conference ProceedingsConference name
AIPVolume
761Issue
1Pagination
3 ppPublisher
American Institute of PhysicsCopyright statement
Copyright © 2005 American Institute of Physics. The published version is reproduced in accordance with the copyright policy of the publisher.Language
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