Table 2
Joint XMM and Chandra spectral fits of the full sample of Compton-thick candidates.
Power-law | Reflection | |||||||||
|
||||||||||
PID | cts | cts | z | N H | Γ | EW | c-stat | Γ | EW | c-stat |
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
|
||||||||||
48 | 7736 | 4172 | 0.298 |
![]() |
![]() |
![]() |
3622/3010 |
![]() |
<0.013 | 4078/3011 |
66 | 1044 | 215 | 1.185 |
![]() |
1.8 |
![]() |
3614/3010 | 1.8 |
![]() |
3666/3012 |
144 | 848 | 407 | 3.700 |
![]() |
![]() |
![]() |
3477/3010 |
![]() |
![]() |
3477/3011 |
147 | 1207 | 593 | 1.537 |
![]() |
![]() |
![]() |
3485/3010 |
![]() |
![]() |
3487/3011 |
214 | 2921 | 1921 | 2.0 |
![]() |
![]() |
![]() |
3498/3010 |
![]() |
![]() |
3582.5/3011 |
222 | 1694 | 1021 | 0.424 |
![]() |
![]() |
![]() |
3477/3010 | 1.8 | <0.15 | 3702/3012 |
245 | 460 | 259 | 2.68 |
![]() |
![]() |
<0.37 | 3388/3010 |
![]() |
<0.44 | 3404/3011 |
289 | 3790 | 2295 | 0.607 |
![]() |
![]() |
![]() |
3330/3010 | 1.8 | <0.10 | 4263/3012 |
324 | 733 | 104 | 1.222 | <0.60 |
![]() |
![]() |
3425/3010 | 1.8 |
![]() |
3457/3012 |
Notes.The columns are: (1) XMM-Newton ID. (2) Net XMM-Newton counts (all three modules). (3) Net Chandra counts. (4) Redshift; two or three decimal digits denote photometric or spectroscopic redshift respectively. (5) NH column density in units of 1022 cm-2. (6) Photon index. (7) Equivalent-width in units of keV; the energy of the line has been fixed at a rest-frame energy of 6.4 keV. (8) c-statistic value/degrees of freedom. (9) Photon-index for the PEXRAV model. (10) Equivalent-width of the FeKα line in the PEXRAV model. The line energy is fixed to 6.4 keV. (11) c-statistic value/degrees of freedom. All errors refer to the 90% confidence level.
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