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Fig. 3.
Specific BHAR as a function of host galaxy stellar mass (left panel) for low (log λBHAR ≲ 32.6) and high (> 32.6) specific BHAR subsamples. The corresponding distribution in terms of Mstar, λBHAR, SFR, and spectroscopic redshift (right panel) are shown for the two AGN subsets.
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