The mass-metallicity relation at z~0.7

D. Crampton; D. Le Borgne; H.-W. Chen; I. Hook; I. Jorgensen; K. Glazebrook; P. McCarthy; R. Abraham; R. Carlberg; R. Marzke

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The mass-metallicity relation at z~0.7

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arxiv astro-ph/0412041 v1 pith:KDCCTWAQ submitted 2004-12-01 astro-ph

S. Savaglio , K. Glazebrook , D. Le Borgne , S. Juneau , R. Abraham , D. Crampton , P. McCarthy , H.-W. Chen

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R. Marzke R. Carlberg I. Jorgensen I. Hook R. Murowinski

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keywords mass-metallicityrelationsampledeepgalaxiesredshiftsurveycanada-france

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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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