Fig. 10
Variation of the 12 + log(O/H) abundance in the integrated galaxy (black data points) as a function of the adopted F([Oii] λ3727)/F(Hβ) ratio. The fluxes are relative to F(Hβ) = 100. The continuum lines corresponds to the integrated values of 7.53 and the dotted lines show the uncertainties associated with these values. More details are in the text.
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