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Fig. 14.

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Number of objects per mass stellar mass bins (upper panel) and the fraction above ΣUDG defined in Sales et al. (2020) for a given stellar mass bin. Here, we consider only objects outside the main halo Rvir and inside the main halo FoF group. The colours are organised as in Fig. 3; the shaded area corresponds to the error of the mean in each bin.

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