Fig. 8.
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sSFR as a function of stellar mass for galaxies with M⋆ ≥ 108 M⊙. To increase the statistics satellites galaxies within the same mass range are also included. The dashed line depicts the adopted limit for star-forming galaxies of log10(sSFR yr−1) = 10−10.8. Galaxies tend to have lower sSFR at the higher mass end (see also Fig. 9).
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