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Caption: Figure 5.
AGN bolometric luminosity as a function of the infrared luminosity for the 21 X-ray detected DOGs (CT candidates: blue stars; moderately obscured AGNs: green triangles) with an FIR SED-decomposition fit that led to the determination of the IR luminosity. Error bars in luminosities are obtained directly from the errors in the fluxes, accounting for the observed spread in bolometric correction in X-rays. The numbers next to the symbols correspond to the DOG ID # from Riguccini et al. (2015), also listed in Table 2. The lower and upper solid lines represent 10% and 50% of the infrared luminosity, respectively.
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