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Fig. 4


Probability density distributions of galaxy g − r colours (left panel), probabilities of being late type (pl, middle panel), and star formations rates (SFRs, in log M/yr, right panel) for high (h, log   Ms ≥ 10.25, solid lines) and low (l, log   Ms < 10.25, dashed lines) stellar mass galaxies in the superclusters of filament (F, red lines) and spider (S, blue lines) morphology.

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