Table 4.
Correction for hidden BLRs and LX predictions.
| Name | L′(HαB) | fBLR |  |
 |
|---|---|---|---|---|
| (1) | (2) | (3) | (4) | |
| G01 | 44.24 | 0.15 | 45.07 (45.00) | 44.96 |
| G02 | 44.30 | 0.54 | 45.12 (45.03) | 45.16 |
| G03 | 44.53 | 0.19 | 45.31 (45.16) | 45.22 |
| G04 | 44.58 | 0.59 | 45.35 (45.18) | 45.32 |
Notes. (1) Broad Hα luminosity, corrected for the fraction of the BLR that is hidden (see text in Sect. 5.2.3). (2) Visible fraction of the BLRs. (3) 2−10 keV luminosity inferred from the LX − L(Hα) relation of Jin et al. (2012) and L′(HαB) in Col. (1). Those in parentheses are values corrected for a possible over-estimate that originates from an extrapolation of the relation (see text in Sect. 5.2.3). (4) 2−10 keV luminosity, estimated from the typical absorption-corrected X-ray to extinction-corrected [O III]λ5007 ratio of log (LX/L([O III])) = 1.32. Luminosities are logarithmic values in units of ergs per second. Uncertainty of these luminosities comes from the scatter of the relations adopted, about 0.3 dex.
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