Fig. 4.

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SED-derived DTM ratio, DTMSED = log AV − (log NHI + [M/H]tot) (top), and depletion-derived DTMmass ratio (bottom) as a function of dust-corrected metallicity [M/H]tot. The symbol notation follows Fig. 3. Median relations at five discrete redshifts are also shown from the L-Galaxies MM simulation (Yates et al., in prep.). We observe a potential anticorrelation of DTMSED with metallicity and a stronger, positive correlation of DTMmass with increasing metallicity.
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