Fig. 17.

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Histograms of stellar mass (top left panel), bulge-to-disc ratio within the galaxy effective radius (top right panel), color (bottom left panel), and SFR (bottom right panel) using the four VMC overdensity classes (see Sect. 5.1 and Table 5). For each class in each histogram, the leftmost and rightmost bins contain all objects with values below and above the corresponding limits, respectively.
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