Fig. 3.

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Stellar mass completeness as a function of redshift for central galaxies (black dash-dotted line) and the control sample (magenta dashed line) within a stellar mass range 8.5 ≤ log(M⋆/M⊙) ≤ 11.5 (1703 central galaxies and 5086 galaxies in the control sample). The completeness has been estimated using the 95% percentile of stellar mass at redshift bins with a width of 0.005 and applying a logarithmic fit of the form log10(M⋆/M⊙) = A + B log10(z) over the redshift range.
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