Mocking integral field unit observations and metallicity diagnostics from cosmological simulations

Open Access

Fig. 7.

Lower panel: Median predicted N2, R23, $\hat{R}$ ${\hat {\mathrm {R}}}$ , O3N2 and N2O2 as a function of the ionization parameter. The shaded regions indicate the interquartile range (25th–75th percentiles) of the line ratios in each ionization parameter bin. Additionally, we indicate the Spearman parameter (r_S) and p-value for each indicator. Upper panel: Distribution of the median log(U) per spaxel.

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