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Fig. 13.
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Distribution of stellar masses for the 49 UDGs (green) and 1258 traditional dwarf (non-UDGs) galaxies (gray) with GALFIT parameters and (g − r) colors, based on the Bell et al. (2003) color-mass relation. The samples are divided by nucleation status: nucleated (empty gray/hashed green) and nonnucleated (filled gray/green).
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