Fig. 6.
Hi-z LBGs (filled dots, top) and Low-zZ galaxies (filled boxes, middle) dust formation rate diagram, sMdust vs. sSFR, colour-coded in IRX. Like in Fig. 5, colour-coding the data points helps towards interpreting the sequence as an evolutionary sequence with low-IRX objects at high sSFR and again at low sSFR. In the middle range, IRX is higher. Low-zZ galaxies (filled dots, bottom) dust formation rate diagram, sMdust vs. sSFR, colour-coded in metallicity.
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