Table 1.
Spectral fits results for candidate CT AGN.
| LID | z | log NH | Γ | P1/P2 | Flux | log LX | log LXunabs | CT probability | PC |
|---|---|---|---|---|---|---|---|---|---|
| cm−2 | 10−15 erg cm−2 s−1 | erg s−1 | erg s−1 | (%) | |||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) |
| 96 | 0.310 |
 |
 |
0.004 | 1.48 | 41.4 | 42.9 | 96.7 | CT |
| 130 | 1.327 |
 |
 |
< 0.001 | 1.38 | 42.3 | 44.2 | 98.4 | nCT |
| 137 | 1.544 |
 |
 |
0.027 | 1.40 | 42.47 | 43.7 | 95.0 | CT |
| 138 | 0.738 |
 |
 |
0.014 | 0.92 | 41.9 | 43.4 | 100.0 | noCT |
| 142 | 1.86 |
 |
 |
0.15 | 0.68 | 42.8 | 43.6 | 94.5 | noCT |
| 164 | 0.729 |
 |
 |
0.09 | 0.87 | 41.9 | 42.9 | 100.0 | noCT |
| 170 | 1.22 |
 |
 |
0.04 | 0.12 | 41.7 | 43.0 | 99.4 | nCT |
| 178 | 0.738 |
 |
 |
0.007 | 1.32 | 41.9 | 43.2 | 92.9 | CT |
| 180 | 3.660 |
 |
 |
0.006 | 1.28 | 43.3 | 44.2 | 90.0 | CT |
| 195 | 1.41 |
 |
 |
0.008 | 1.00 | 42.1 | 43.7 | 98.3 | CT |
| 196 | 0.670 |
 |
 |
0.004 | 0.70 | 41.58 | 43.34 | 99.9 | CT |
| 266 | 0.954 |
 |
 |
0.093 | 0.33 | 41.8 | 42.8 | 99.4 | noCT |
| 282 | 2.223 |
 |
 |
0.040 | 0.36 | 42.7 | 43.9 | 99.9 | CT |
| 287 | 1.037 |
 |
 |
0.052 | 0.77 | 42.2 | 43.4 | 97.2 | CT |
| 309 | 2.578 |
 |
 |
0.001 | 0.98 | 42.8 | 44.6 | 100.0 | CT |
| 312 | 1.309 |
 |
 |
0.085 | 0.36 | 42.3 | 43.2 | 100.0 | noCT |
| 313 | 1.608 |
 |
 |
0.012 | 1.51 | 42.4 | 43.9 | 99.3 | CT |
| 327 | 1.096 |
 |
 |
0.082 | 0.18 | 41.7 | 42.7 | 99.6 | ... |
| 337 | 2.470 |
 |
 |
0.002 | 0.55 | 42.3 | 44.2 | 99.6 | CT |
| 389 | 1.74 |
 |
 |
0.006 | 1.68 | 42.6 | 44.3 | 100.0 | nCT |
Notes. The columns are: (1) Chandra ID from the Luo et al. (2010) catalog. (2) Redshift (two decimal and three decimal digits denote photometric and spectroscopic redshifts, respectively). (3) Intrinsic column density. (4) Photon index (f corresponds to fixed photon index). (5) Ratio between the scattered and the torus components. (6) Observed flux in the 2−10 keV band. (7) Observed luminosity in the 2−10 keV band. (8) Unabsorbed luminosity in the 2−10 keV band. (9) Probability of the source being Compton-thick. (10) Previous classification from Buchner et al. (2014), Brightman et al. (2014), and/or Liu et al. (2017): Compton-thick (CT), near-CT (NH > 5 × 1023, nCT), not a CT (noCT).
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