Fig. 8.

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Distribution of the galaxies in DECODE’s catalogue on the M⋆ − Mh plane at redshifts z = 0, 1 and 2, for the halo quenching scenario. The colour bar represents the star formation rate of the galaxies. The red dotted, solid and dashed lines show the scenarios with no quenching, halo quenching-only, and both halo and low-mass quenching, respectively. We also show the stellar mass-halo mass relations from Moster et al. (2018) (violet dash-dotted lines) and Behroozi et al. (2019) (yellow dotted lines), at the same redshifts.
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