The mass-metallicity relation at z ∼ 0.7.
In: AIP Conference Proceedings; 2005, Vol. 761 Issue 1, p425-428, 4p; Jg. 761 (2005-04-11) 1, S. 425-428
Konferenz
Zugriff:
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. © 2005 American Institute of Physics [ABSTRACT FROM AUTHOR]
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Titel: |
The mass-metallicity relation at z ∼ 0.7.
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Autor/in / Beteiligte Person: | Savaglio, S. ; Glazebrook, K. ; Le Borgne, D. ; Juneau, S. ; Abraham, R. G. ; Crampton, D. ; McCarthy, P. J. P. ; Chen, H. W. ; Marzke, R. ; Carlberg, R. G. ; Jørgensen, I. ; Roth, K. ; Hook, I. ; Murowinski, R. |
Quelle: | AIP Conference Proceedings; 2005, Vol. 761 Issue 1, p425-428, 4p; Jg. 761 (2005-04-11) 1, S. 425-428 |
Veröffentlichung: | 2005 |
Medientyp: | Konferenz |
ISSN: | 0094-243X (print) |
DOI: | 10.1063/1.1913959 |
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