Fig. 3.
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Distribution of the maximum S870 flux density reached by each modelled galaxy across its entire formation history, S870, max (first row), and when it occurred (second row; redshift distribution), for massive quiescent galaxies (MQs) selected at z = 2, 3, and 4 (from left to right). The minimum S870, max reached by any of the MQs is indicated by the vertical dashed black line.
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