Fig. 13.
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Cosmic evolution of SFR, M★, sSFR, and M200 of TNG300 galaxies are compared for C-LAEs split by environmental density δ5. The C-LAEs in the top 20% densest regions are shown in red (dot-dashed line), the middle 60% are shown in orange (solid line), and the bottom 20% are shown in blue (dotted line). The averages and standard deviation are computed the same as for Figure 9.
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