Absorbed X-ray (2−10 keV) X-ray luminosity against the 12 μm luminosity. Color- and shape-coding as in Fig. 1. The typical errors are on the order of 30% and 20% for the IR and X-ray luminosity, respectively, including the uncertainties in the model fitting. The hatched diagram represents the 1σ envelope of the local (Gandhi et al. 2009) relation. The dotted line corresponds to a factor of 30 lower X-ray luminosity as is typical in many Compton-thick nuclei. The numbers of interesting sources correspond to the sequence numbers in Tables 1 and 2.