Decomposed fluxes and luminosities.
Notes. Estimated fluxes in the 4−8 keV and 10−30 keV bands in units of 10−13 erg s−1 cm−2, and the intrinsic luminosities in unit of 1042 erg s−1, corrected for absorption and reflection for the SW and N nuclei, based on the two-component decomposition (Model (iii) in Table 1 and Fig. 2b). The Fe K emission-line flux is excluded from the measured fluxes.
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