Gallo and Sesana estimate the local black hole mass function between 10^5 and 10^6 solar masses by folding GAMA galaxy counts together with X-ray occupation fraction constraints, finding a normalization uncertainty of about one dex.
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Exploring the local black hole mass function below $10^6$ solar masses
Gallo and Sesana estimate the local black hole mass function between 10^5 and 10^6 solar masses by folding GAMA galaxy counts together with X-ray occupation fraction constraints, finding a normalization uncertainty of about one dex.