Table 11
Power law and absorption edges fit results.
| Source | Type | z | Γ | NH | E | τ | f2−10 keV | Log L2−10 keV | χ2/d.o.f. | Probability | Sample |
| 1022 | 10-13 | ||||||||||
| cm-2 | keV | erg cm-2 s-1 | erg s-1 | % | |||||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) |
|
|
|||||||||||
| XBSJ100926.5+533426 | AGN1 | 1.718 |
2.02
|
< 0.18 |
2.09
|
0.63
|
0.73 | 45.18 | 40/37 | 34.5 | BSS |
| XBSJ102412.3+042023 | AGN1 | 1.458 |
2.01
|
< 0.17 |
3.25
|
0.9
|
0.53 | 44.87 | 37/33 | 28.9 | BSS |
| XBSJ204159.2–321439 | AGN1 | 0.738 |
2.08
|
< 0.10 |
2.10
|
0.70
|
1.05 | 44.45 | 27/26 | 42.3 | BSS |
Notes. Columns: (1) source name; (2) class; (3) redshift; (4) photon index; (5) intrinsic column density; (6) threshold energy; (7) absorption depth at threshold; (8) observed flux in the 2 − 10 keV band, de-absorbed by our Galaxy; (9) intrinsic luminosity in the 2 − 10 keV band; (10) χ2 to number of degrees of freedom; (11) null hypothesis probability; (12) sample the source belongs to.
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