Fig. 11.
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Histogram distributions of multimode (M, panel a), intensity (I, panel b), and deviation (D, panel c) for different types of massive galaxies. Color bars at the top of each panel show the median values of M, I, and D for each galaxy type. Notably, the MID median values gradually increase from SPH to IRR types, reflecting a systematic trend of different galaxy types in the MID parameter space.
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