The scatter in black hole mass at fixed stellar mass sets the low-mass slope of the quenched central galaxy mass function, and the observed slope requires a scatter of about 0.5 to 0.8 dex.
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On the signature of black holes on the quenched stellar mass function
The scatter in black hole mass at fixed stellar mass sets the low-mass slope of the quenched central galaxy mass function, and the observed slope requires a scatter of about 0.5 to 0.8 dex.