The mass-metallicity relation at z ≁ 0.7

被引：0
|
作者：
Savaglio, S [1 ]
Glazebrook, K [1 ]
Le Borgne, D [1 ]
Juneau, S [1 ]
Abraham, RG [1 ]
Crampton, D [1 ]
McCarthy, PJP [1 ]
Chen, HW [1 ]
Marzke, R [1 ]
Carlberg, RG [1 ]
Jorgensen, I [1 ]
Roth, K [1 ]
Hook, I [1 ]
Murowinski, R [1 ]
机构：
[1] Johns Hopkins Univ, Baltimore, MD 21218 USA
来源：
SPECTRAL ENERGY DISTRIBUTIONS OF GAS-RICH GALAXIES: CONFRONTING MODELS WITH DATA | 2005年 / 761卷
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
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 similar to 0.1 SDSS galaxies, but displaced towards higher masses and/or lower metallicities. Using this sample, and a small sample of z similar to 2.3 LBGs, a redshift dependent mass-metallicity relation is proposed which describes the observed results.
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页码：425 / 428
页数：4
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