Fig. A.2.

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Completeness of retired galaxies in terms of z, and M*. The coloured map illustrates the 5th percentile of sSFR9 on each z–M* bin. Each bin includes the (uncorrected) fraction of retired galaxies with respect to the total, based on the classification that maximises the F-score. The dashed and solid lines denote the mass completeness limit above which retired galaxies are detected. Each line tracks the lower envelope that satisfies sSFR9 < 10−11 yr−1 and sSFR8 < 3 × 10−11 yr−1, based on the 5th and 1st percentiles, respectively.
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