Observed X-ray luminosity in the rest-frame 2–10 keV band as a function of the 6 μm luminosity for fit AGN component. The solid purple, blue, and black lines represent the relation for Chen et al. (2017), Stern (2015), and Fiore et al. (2009), respectively. The dashed lines indicate the same relationships but where the X-ray luminosities are absorbed by a column density of N_H = 1.5 × 10²⁴ cm⁻². The shaded area represents the column density of absorbed gas is 1.5 × 10²⁴ cm⁻². The solid circles are 329 AGNs with a fit AGN component. The different colors represent the confidence coefficient of the 6 μm luminosity for a fit AGN component (or the fit AGN components). The cutting stars within the large circles represent CT-AGNs identified using the relationship between MIR and X-ray luminosities.