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Fig. 4.

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Star-forming ratio as a function of r for galaxies in four different M* ranges (different panels). The red line represents galaxies that are embedded in substructures with at least two galaxies with log M*(M) > 10.15. The black line represents single galaxies that orbit the cluster alone. Central BCGs are excluded. The coloured bands represent the 68% confidence intervals obtained with Poisson statistics (see Sect. 3).

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