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Fig. 10


CO(1–0) line luminosity as a function of the oxygen abundance in log-log scale for the sample of local star-forming galaxies defined by the ALLSMOG survey and by the sub-sample of COLD GASS selected in Sect. 5. Each plot corresponds to a different strong-line metallicity calibration method (see Sect. 4.1.2). Further explanation relevant to the quantity plotted on the y-axis, the symbols and the regression analysis can be found in the caption of Fig. 8 and in the text (Sect. 7).

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