Fig. 26.

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Variation in σNMAD as a function of the cut applied in r-band magnitude separately for red and blue galaxies. Each panel shows results for a different way of classifying the galaxies, using the strength of the 4000 Å break (top), the specific instantaneous SFR (middle), and the equivalent width of Hα (bottom). Solid lines correspond to σNMAD values at 100% completeness (no cut in odds), and dotted lines indicate σNMAD values for a cut in odds corresponding to 50% completeness.
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