Table 1.
Best-fit parameters for the nine objects with spectroscopic redshifts where a significant Fe Kα line is detected at 6.4 keV.
| XID | z | CNTS | NH | Γ | EW (keV) |
|---|---|---|---|---|---|
| 2 | 0.628 | 827 |
 |
 |
 |
| 4 | 2.013 | 259 | < 4 |
 |
 |
| 8 | 2.78 | 102 |
 |
1.9 |
 |
| 31 | 2.377 | 154 | < 2.7 |
 |
 |
| 44 | 1.486 | 195 |
 |
 |
 |
| 70 | 0.764 | 228 |
 |
 |
 |
| 73 | 2.171 | 226 | < 4.3 |
 |
 |
| 114 | 0.533 | 159 | < 0.9 |
 |
 |
| 115 | 0.76 | 76 |
 |
1.9 |
 |
Notes. The counts are the net full counts; the photon index Γ is free to vary if there are more than 150 net counts of the source, while it is fixed if there are fewer than 150. The column density NH is shown in units of 1022 cm−2. The equivalent width of the emission line is shown in keV. Errors are at the 90% confidence level.
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