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Fig. 2.
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Distribution of the AGN sample in the log MBH − log M★ plane colour-coded by log sSFR (in Gyr−1). The solid black line shows the best-fitting empirical MBH − M★ relation, while the dashed lines indicate the ±0.3 dex thresholds used to define the on–relation, overmassive, and undermassive subsets.
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