Fig. 4.
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Cumulative distributions of SERSIC (left) and SHAPE_R (right) for AGNs and matched control galaxies in the 8.5 ≤ log(MBH/M⊙) < 9.0 bin. The vertical lines indicate the sample medians. Owing to the small number of AGNs with reliable DESI morphology, especially for SHAPE_R, this comparison is intended as a qualitative illustration only.
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