High-luminosity RQ AGN deviate above the mm/X-ray correlation with a quadratic joint fit (0.32 dex scatter); mm emission correlates linearly with UV and bolometric luminosity.
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The Millimeter/X-ray Relation in Rapidly Accreting Supermassive Black Holes at $z < 0.16$
High-luminosity RQ AGN deviate above the mm/X-ray correlation with a quadratic joint fit (0.32 dex scatter); mm emission correlates linearly with UV and bolometric luminosity.