M∗-independent quantity as a function of oxygen abundance 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 panel corresponds to a different strong-line metallicity calibration method (see Sect. 4.1.2). We refer to the caption of Fig. 8 for an explanation of the symbols and lines shown in the plot. The results of the regression analysis are reported in Table A.1.
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