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Fig. 5


Probability density distributions of stellar masses (log   Ms, in log   M), (left panel) and probabilities of being late type (pl, right panel), for red, low SFR galaxies (red lines), blue, high SFR galaxies (blue lines), and for red, high SFR galaxies (grey lines) in the superclusters of filament (solid lines) and spider (dashed lines) morphology. High SFR galaxies have log   SFR ≥ −0.5, and low SFR galaxies have log   SFR < −0.5. Lines in the left panel denote the same populations as in the right panel.

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