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Fig. 7

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Top: distribution of galaxy stellar masses in the control sample (black solid line) and in the structure (red dashed line). Bottom: same as in the top panel, but for the distribution of SFR. In both panels, the solid point with the error bar shows the typical error on and SFR. The possible systematic offset in the SFR computation due to the choice of different SFHs (see Sect. 2.1) is not included.

This figure is made of several images, please see below:

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