Fig. 7.
Similar to figures 5 and 6, the quenching efficiency ε is plotted as a function of redshift for different mass ranges in four panels for field (dotted), group (dashed), and cluster (solid) galaxies, respectively. In general, the slope of the quenching efficiency decreases with the increasing masses, implying that the quenching effect is stronger for less-massive galaxies. (Color online)

Similar to figures 5 and 6, the quenching efficiency ε is plotted as a function of redshift for different mass ranges in four panels for field (dotted), group (dashed), and cluster (solid) galaxies, respectively. In general, the slope of the quenching efficiency decreases with the increasing masses, implying that the quenching effect is stronger for less-massive galaxies. (Color online)

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