Table A.1.
11 sources with X-ray redshift estimates.
| PID | zx | zph | sp | ID(H14) |
|---|---|---|---|---|
| 19 | 1.92 (1.90–1.94) | 1.980 (1.47–2.6) | L | 105024 |
| 32 | 1.90 (1.74–1.96) | 3.163 (0–4.27) | E | 105036 |
| 88 (a) | 1.12 (1.1–1.14) | 0.345, 1.360 | L | 59030 |
| 95 | 0.86 (0.85–0.87) | 1.478 (0.91–1.78) | EL | 105046 |
| 103 | 2.00 (1.98–2.02) | 1.976 (1.92–2.02) | L | 60464 |
| 142 | 2.25 (2.15–2.37) | 2.509 (2.03–2.69) | E | 63777 |
| 166 | 1.37 (1.32–1.43) | 1.688 (1.55–1.71) (b) | EL | 9360 |
| 213 | 3.17 (3.08–3.31) | 2.167 (1.44–5.74) | E | 105100 |
| 215 (c) | 2.66 (2.65–2.67) | 2.513 (2.45–2.61) | L | 15377 |
| 252 | 1.52 (1.49–1.56) | 1.907 (1.82–1.95) | E | 19476 |
| 338 | 2.02 (2.00–2.07) | 1.018 (0.09–2.58) | E | 105136 |
Notes. Table columns are PID, X-ray redshift zx and the 68% error interval in parenthesis, photometric redshifts, and the 68% error interval from (Hsu et al. 2014, =H14), X-ray spectral feature which drives zx estimate: E: Fe K absorption edge; L: Fe K line, source ID number of Chandra counterpart in H14.
Another photometric redshift from Straatman et al. (2016) is zph = 1.37.
There are two Chandra sources in the XMM error circle. One of them has a spectroscopic redshift but is fainter in X-ray. The other brighter X-ray source only has photometric redshifts shown here and zph = 2.6 from Straatman et al. (2016), and seems to be the source of a strong Fe K line detected in the XMM-Newton spectrum. See text for further details.
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