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Fig. 8
Fractions of passive (solid lines) and star-forming (dashed line) galaxies as functions of group richness (top) and luminosity (bottom) in four large-scale density bins. The fractions are calculated in richness bins of two galaxies and luminosity bins of 5 × 1010 h-2 L⊙.
This figure is made of several images, please see below:
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