Table 3
Joint XMM-Newton and Chandra spectral fits to the four more probable Compton-thick sources Power-law + FeKα line (PLCABS+GA) leaving the relative XMM-Newton and Chandra normalization and the energy of the line free.
| PID | N H | Γ | E | E W X | E W C | c |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) |
|
|
||||||
| 66 |
|
|
|
|
|
3560/3008 |
| 144 |
|
|
|
|
|
3475/3008 |
| 147 |
|
|
|
|
|
3477/3008 |
| 324 | <0.45 |
|
|
|
|
3402/3008 |
Notes.The columns are: (1) XMM-Newton ID. (2) Column density (in units of 1022). (3) Photon index as derived from the PLCABS model. (4) FeKα line energy. (5) XMM-Newton rest-frame EW of the FeKα line. (6) Chandra rest-frame EW of the FeKα line. (7) c-statistic value and degrees of freedom. Note: the model is the same as that used in Table 2 except here, the FeKα line energy is free and the Chandra and XMM-Newton power-law normalizations are not tied to each other.
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