[O IV] and [Ne V]-weak AGNs Hidden by Compton-thick Material in Late
Mergers
[O IV] and [Ne V]-weak AGNs Hidden by Compton-thick Material in Late
Mergers
We study "buried" active galactic nuclei (AGNs) almost fully covered by circumnuclear material in ultra-/luminous infrared galaxies (U/LIRGs), which show weak ionized lines from narrow line regions. Employing an indicator of [O IV] 25.89-um or [Ne V] 14.32-um line to 12-um AGN luminosity ratio, we find 17 buried AGN candidates …