Table 3
Chandra spectral fits.
LID | z | NH | P1/P2 | cstat/d.o.f. | EW | Flux | log LX | log LXunabs |
1022 cm-2 | keV | 10-15 erg cm-2 s-1 | erg s-1 | erg s-1 | ||||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
|
||||||||
117 | 1.51 |
![]() |
0.02 | 392/390 |
![]() |
![]() |
![]() |
43.41 |
170 | 1.22 | < 0.8 | < 0.2 | 93/117 | < 1.2 |
![]() |
![]() |
41.50 |
199 | 2.45 |
![]() |
<0.02 | 162/205 |
![]() |
![]() |
![]() |
43.52 |
230 | 2.61 |
![]() |
0.001 | 119/135 | < 0.43 |
![]() |
![]() |
44.82 |
293 | 3.88 |
![]() |
<0.002 | 195/228 | <1.0 |
![]() |
![]() |
43.31 |
326 | 3.10 | < 7 | < 0.01 | 211/287 | < 0.3 |
![]() |
![]() |
43.45 |
397 | 2.28 |
![]() |
<0.04 | 309/324 | < 0.2 |
![]() |
![]() |
43.56 |
Notes. The columns are: (1) Chandra ID from the Luo et al. (2010) catalogue. (2) Redshift. (3) Intrinsic column density. (4) Ratio between the power-law normalizations in case of a double power-law model. (5) C-stat value to degrees of freedom ratio. (6) Fe Kα rest-frame equivalent width. (7) Observed flux in the 2–10 keV band. (8) Observed luminosity in the 2–10 keV band. (9) Unabsorbed luminosity in the 2–10 keV band.
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