Fig. B.1.
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Zoomed-in version of Figure 10, showing only massive quenched galaxies at z = 2, 3, and 4. The time between the peak in sub-millimetre flux density and subsequent quenching is lowest for the highest-redshift MQs, on average. The median tquench − tsubmm − peak timescales are 0.9 Gyr, 0.6 Gyr, and 0.4 Gyr for MQs selected at z = 2, 3, and 4, respectively.
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