Fig. 6.
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Quiescent fraction fQ for galaxies in three local environments as a function of stellar mass (left) and the infall proxy dR (right). The bin sizes are Δlog M★/M⊙ = 0.5 and ΔdR = 0.6, respectively. Cluster, group, and isolated galaxies are shown as red, orange, and blue curves, respectively. Shaded squares indicate the uncertainties in fQ.
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