Fig. 6.
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2D ex situ stellar mass fraction maps for 30 randomly selected galaxies in each group, based on the classification we developed. Each map shows the median of 10 samples predicted by the diffusion model, trained on the MaNGIA mock dataset and conditioned on the stellar mass density and kinematic maps of the corresponding MaNGA galaxy. The different groups display different spatial distributions in their ex situ stellar mass fraction, following our classification scheme.
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