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Fig. 6


Distribution of ALLSMOG galaxies as a function of the gas-phase metallicity computed using five different strong-line calibrations (details in Sect. 4.1.2). As in Figs. 4 and 5, the full sample is represented by the coloured histogram, and the hatched histogram traces the non-detections. The detection fraction per bin is shown at the bottom of the histograms.

This figure is made of several images, please see below:

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