Table 6.
Six broad Fe K line sources.
| PID | z | σ | EW | F1−5 |
|---|---|---|---|---|
| keV | keV | 10−14 erg s−1 cm−2 | ||
| 33 | 1.843 |
 |
 |
3.0 |
| 62 | 2.561 |
 |
 |
0.78 |
| 203 | 0.543 |
 |
 |
7.6 |
| 308 | 0.733 |
 |
 |
1.2 |
| 319 | 0.734 |
 |
 |
7.5 |
| 337 | 0.837 |
 |
 |
2.8 |
Notes. Six unobscured sources in which broad Fe K emission is detected, out of the 21 bright sources. When a Gaussian of the centroid energy of 6.4 keV is fitted, and the 90% confidence interval of the line width is positive, the source made this table. The line EW is measured in the galaxy rest frame. The source flux in the observed 1–5 keV range, F1−5, is shown for reference.
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