Top: Overlapping fraction of AGNs also identified by our DL method as a function of the adopted cut on the X-ray or the rest-frame 6 μm luminosity for the X-ray and MIR-selected AGNs. The solid lines show the overlapping fraction by applying a cut at f_AGN > 0.2, while the dashed lines show the overlapping fraction if we select AGNs by requiring f_AGN > 0.1. Bottom: AGN luminosity in the JWST/NIRCam F150W filter versus the X-ray luminosity or the rest-frame 6 μm luminosity, for the X-ray-selected or MIR-selected AGNs. The dash-dotted lines show the respective linear fits.