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Fig. 11.
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Distribution of mass M200c and SFR of our sample of 570 simulated high-z SF halos, coloured by their fate at z = 0 (top left panel), their redshift (top right panel), their number of SF galaxy members with galaxies are SFR > 10 M⊙ yr−1 (bottom left panel), and their SFR fraction (as defined in Eq. (4), bottom right panel).
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