Observational and theoretical constraints on the formation and early evolution of the first dust grains in galaxies at 5 < z < 10

Open Access

Fig. 5.

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Hi-z LBGs (filled dots, top) and Low-zZ galaxies (filled boxes, panel) DFRD, sM_dust vs. sSFR, colour-coded by age. We see a sequence from top right to bottom left. Using a colour-coding system based on the age of the dominant stellar population, we see that this sequence corresponds to galaxies getting older and older from top right to bottom left.

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