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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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