High-Eddington AGN at z~0.06-0.16 lie above the mm/X-ray correlation of low-luminosity sources; mm emission instead tracks bolometric luminosity linearly, suggesting a two-component coronal electron population.
Finally, the SFR values for PG 0026+129 and PG 0052+251 were determined by Y
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The Millimeter/X-ray Relation in Rapidly Accreting Supermassive Black Holes at z <0.16
High-Eddington AGN at z~0.06-0.16 lie above the mm/X-ray correlation of low-luminosity sources; mm emission instead tracks bolometric luminosity linearly, suggesting a two-component coronal electron population.