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Fig. 8.
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Distribution of galaxies with (NGC 891, NGC 3044, NGC 3735, NGC 4217, and NGC 4631) and without (NGC 3079, NGC 3448, NGC 4157, NGC 4666, and NGC 5775) detected model preference, comparing their physical sizes and the number of beams that cover the galaxies after the described masking and weighting process.
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