Comparison of the AGN bolometric luminosities obtained from the SED-fitting ($L_{\mathrm{bol}}^{\mathrm{sed}}$) and from X-ray spectral analysis ($L_{\mathrm{bol}}^{\mathrm{X}}$). The $L_{\mathrm{bol}}^{\mathrm{X}}$ were computed from the 2 − 10 keV rest-frame intrinsic luminosities using the Lusso et al. (2012) bolometric correction. Circles indicate X-ray-detected sources, while diamonds are the X-ray-undetected. For these sources, we have only an upper limit on their $L_{\mathrm{bol}}^{\mathrm{X}}$. The color code indicates the X/[Ne V] ratio for the X-ray-detected sources and upper limits for the X-ray-undetected sources. The orange line is the 1:1 correlation. The red line is the best-fit relation for the X-ray-detected sources obtained via orthogonal distance regression.