Table 4
Low LX/L6 μm and low intrinsic X-ray luminosity sources with flat spectra.
| ID | z | f2 − 10 | LX |
|
Γ | C-stat | NH | C-stat |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
|
|
||||||||
| 96 | 0.310 | 0.76 | 41.23 | 10.07 |
|
503 | < 0.53 | 512 |
| 159 | 0.664 | 0.78 | 41.81 | 10.28 |
|
539 | < 0.24 | 549 |
| 166 | 0.340 | 0.54 | 41.12 | 9.61 |
|
438 |
|
440 |
| 178 | 0.735 | 1.22 | 41.76 | 10.32 |
|
452 |
|
449 |
| 208 | 0.738 | 0.72 | 41.92 | 10.55 |
|
488 | < 0.75 | 496 |
Notes. The columns are: (1) name in the catalogue of Luo et al. (2008); (2) spectroscopic redshift from Luo et al. (2010); (3) X-ray flux in the 2–10 keV band in units of 10-15 erg cm-2 s-1, as estimated from the X-ray spectroscopy; (4) logarithm of the obscured X-ray luminosity in the 2–10 keV band in units of erg s-1; (5) logarithm of the total 6 μm luminosity (star-formation and torus) in units of solar luminosity; (6) photon index Γ for column density fixed to NH = 0, as derived from the Chandra spectral fits; (7) corresponding C-statistic value; (8) column density in units of 1022 cm-2 for photon index fixed to Γ = 1.8; (9) corresponding C-statistic value; all errors refer to the 90% confidence level.
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