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Fig. 11.

image

Left panel: black-hole mass, M bh β −1(M ), versus total stellar mass, M (M ), for HerMES-SWIRE sources and for RIFSCz sources with z < 0.3 (smaller points), with AGN dust tori. QSOs are excluded by the requirement that there be a stellar mass estimate, so these are all Type 2 AGN. Circled points are Herschel extreme starbursts. Right panel: M bh/(βM ) versus z for HerMES-SWIRE sources and for RIFSCz sources with z < 0.3, with AGN dust tori.

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