Comparison of AGN bolometric luminosities derived using the different methods listed in Table A.1. The median and standard deviation of the difference (y − x) are indicated in the upper left corner of each panel. The dashed lines indicate the one-to-one relation. a: 14–195 keV and 12 μm results show a possible offset, comparable to their scatter (≃0.3 dex). The 5100 Å bolometric luminosity tends to be better consistent with both 14–195 keV (b) and 12 μm (c), although the scatters of both relations are considerable. Considering the uncertainty of the bolometric correction is large (∼0.5 dex), the different methods are relatively well consistent with each other.