Table 2
Results of the joint fit of XMM-Newton-pn+MOS+Chandra spectra for the CTKf sample.
| XMM ID | Ch. ID | z | Tot C | NH | F2−10 | Log (LI) | Log (LO) | Sc. % | EW | C/d.o.f. | ||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | ||
|
|
||||||||||||
| 2608 | 482 | 0.125 1 | 271 |
|
|
|
|
0.34 ± 0.15 |
|
542.6/579 | ||
| 60 211 | 368 | 0.511 2 | 85 |
|
|
|
|
1.62 ± 0.90 | <0.61 | 158.2/217 | ||
| 60 152 | 298 | 0.579 2 | 121 |
|
|
|
|
<0.41 |
|
189.4/236 | ||
| 54 514 | New | 0.707 2 | 265 |
|
|
|
|
1.58 ± 0.48 |
|
403.9/416 | ||
| 54 490 | 284 | 0.908 2 | 147 |
|
|
|
|
<1.50 |
|
258.7/261 | ||
| 60 342 | 576 | 0.941 3 | 72 |
|
|
|
|
<1.22 | <0.71 | 195.4/196 | ||
| 5511 | New | 1.023 3 | 202 |
|
|
|
|
6.78 ± 2.50 | <0.59 | 401.3/422 | ||
| 60 361 | New | 1.73 3 | 120 |
|
|
|
|
0.59 ± 0.45 |
|
335.2/382 | ||
| 70 082 | 747 | 2.429 3,* | 102 |
|
|
|
|
<2.01 | <1.301 | 402.0/418 | ||
| 70 145 | 708 | 2.548 3 | 123 |
|
|
|
|
2.72 ± 0.93 |
|
140.1/138 | ||
Notes. Sources are ordered by increasing redshift. Column: (1) XMM-Newton ID number; (2) Chandra ID; (3) redshift ( ); (4) total 0.3−10 keV net counts; (5) column density in units of 1024 cm-2; (6) 2−10 keV observed flux in units of 10-14 erg cm-2 s-1; (7) Log of the 2−10 keV rest frame absorption corrected luminosity, in units of erg s-1. The errors are obtained taking into account the errors on the observed luminosity and on the column density; (8) Log of the 2−10 keV rest frame observed luminosity, in units of erg s-1; (9) intensity of the scattered component, relative to the primary power-law; (10) equivalent width of the Fe Kα line, in units of keV, from the Pl fit; (11) best fit Cstat/d.o.f.
photometric from Salvato et al. (2011),
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