| DOI | Resolve DOI: https://doi.org/10.1063/1.1913959 |
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| Author | Search for: Savaglio, S.; Search for: Glazebrook, K.; Search for: Borgne, D. Le; Search for: Juneau, S.1; Search for: Abraham, R.; Search for: Crampton, David1; Search for: McCarthy, P.; Search for: Chen, Hui; Search for: Marzke, R.; Search for: Carlberg, R.; Search for: Jorgensen, I.; Search for: Hook, I.; Search for: Murowinski, R.1 |
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| Affiliation | - National Research Council of Canada. NRC Herzberg Institute of Astrophysics
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| Format | Text, Article |
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| Conference | International Workshop on The Spectral Energy Distribution of Gas Rich Galaxies: Confronting Models with Data, October 4-8, 2004, Heidelberg, Germany |
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| Abstract | The 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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| Publication date | 2005-04-11 |
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| Peer reviewed | Yes |
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| NPARC number | 9722390 |
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| Export citation | Export as RIS |
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| Report a correction | Report a correction (opens in a new tab) |
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| Record identifier | 18b7362d-d8fa-4637-a53f-8d03cc69c622 |
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| Record created | 2009-07-17 |
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| Record modified | 2020-04-07 |
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