The mass-metallicity relation at z ~ 0.7

DOIResolve DOI: http://doi.org/10.1063/1.1913959
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TypeArticle
Proceedings titleThe Spectral Energy Distributions of Gas-Rich Galaxies: Confronting Models with Data; International Workshop
Series titleAIP Conference Proceedings; no. 761
ConferenceInternational Workshop on The Spectral Energy Distribution of Gas Rich Galaxies: Confronting Models with Data, October 4-8, 2004, Heidelberg, Germany
ISBN0-7354-0246-9
Pages425428; # of pages: 4
AbstractThe 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.
Publication date
AffiliationNational Research Council Canada; NRC Herzberg Institute of Astrophysics
Peer reviewedYes
NPARC number9722390
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Record identifier18b7362d-d8fa-4637-a53f-8d03cc69c622
Record created2009-07-17
Record modified2016-05-09
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