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Fig. 6.

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Comparison of distribution of photometric and structural properties – absolute magnitude Mg, Sérsic index n, effective radius Re, axis ratio, central surface brightness μ0, g, and (g − i)0 color – between the UDGs (green) and the non-UDGs (gray) in the MATLAS dwarfs sample. The samples are divided by nucleation status: nucleated (empty gray/hashed green) and nonnucleated (filled gray/green). All dwarfs are shown for Mg while only galaxies in the range of the UDGs luminosity, −15.5 < Mg < −11.5, are considered for the other parameters.

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