Fig. 17.
Ionisation parameter log(q) as a function of log(EW(Hα)) dividing all the spaxels used in this work into bins of 0.15 dex and then separating the galaxies into bins of metallicity, as reported in the legend. The shaded regions represent the 16th and 84th percentiles of the distribution in each stellar mass bin taking into account the number of galaxies lying in the bin.
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