Table 3.
Best-fit parameters of the X-ray spectral analysis.
XID | Model | C-stat/d.o.f. | NH | Γ | EFe line | EW | F[2−10 keV] | L[2−10 keV] |
---|---|---|---|---|---|---|---|---|
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
42 | Transmission | 146.9/172 | ![]() |
1.8 | ![]() |
![]() |
![]() |
![]() |
Reflection | 154.8/173 | – | 1.8 | ![]() |
![]() |
![]() |
![]() |
|
MYTorus | 151.8/177 | ![]() |
1.8 | 6.4 | ![]() |
![]() |
![]() |
|
170 | Transmission | 355.7/391 | ![]() |
1.8 | 6.4 | < 141 | ![]() |
![]() |
Reflection | 972.5/389 | – | 1.8 | 6.4 | ![]() |
![]() |
![]() |
|
MYTorus | 354.3/389 | ![]() |
1.8 | 6.4 | <150 | ![]() |
![]() |
|
337 | Transmission | 207.4/240 | ![]() |
1.8 | ![]() |
![]() |
![]() |
![]() |
Reflection | 197.4/242 | – | 1.8 | 6.32 | <503 | ![]() |
![]() |
|
MYTorus | 190.7/241 | ![]() |
1.8 | 6.4 | ![]() |
![]() |
![]() |
|
539 | Transmission | 29.2/45 | ![]() |
1.8 | 6.91![]() |
![]() |
![]() |
![]() |
Reflection | 32.4/47 | – | 1.8 | 6.9 | <2089 | ![]() |
![]() |
|
MYTorus | 30.9/45 | ![]() |
1.8 | ![]() |
![]() |
![]() |
![]() |
|
551 | Transmission | 268.1/307 | ![]() |
1.8 | ![]() |
![]() |
![]() |
![]() |
Reflection | 282.1/309 | – | 1.8 | ![]() |
![]() |
![]() |
![]() |
|
MYTorus | 276.5/316 | ![]() |
1.8 | 6.4 | ![]() |
![]() |
![]() |
|
666 | Transmission | 83.6/113 | ![]() |
1.8 | ![]() |
![]() |
![]() |
![]() |
Reflection | 87.9/114 | – | 1.8 | ![]() |
![]() |
![]() |
![]() |
|
MYTorus | 85.9/115 | >39 | 1.8 | 6.4 | ![]() |
![]() |
>3.4 | |
746 | Transmission | 372.7/382 | ![]() |
1.8 | 6.4 | <100 | ![]() |
![]() |
Reflection | 492.8/376 | – | 1.8 | ![]() |
<325 | ![]() |
![]() |
|
MYTorus | 368.8/382 | ![]() |
1.8 | 6.4 | <204 | ![]() |
![]() |
Notes. (1) X-ray source ID (see Table 1); (2) model used to fit the source spectrum; (3) ratio between the Cash statistic value and the number of degrees of freedom; (4) column density in units of 1023 cm−2; (5) spectral index; (6) rest-frame energy of the iron emission line in keV; (7) rest-frame equivalent width of the iron line in eV; (8) observed flux in the hard (2−10 keV) band, in units of 10−15 erg cm−2 s−1; and (9) rest-frame absorption corrected luminosity in the hard (2−10 keV) band, in units of 1044 erg s−1. Errors are given at the 90% confidence level.
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