Table 1
Candidate Compton-thick sources in the local sample based on the LX/L6 μm ratio.
| Name | z | LX | L6 μm | Fraction | CT | NH | EW |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
|
|
|||||||
| NGC 17 | 0.0196 | 41.29 | 43.82 | 0 | - |
|
0.440 |
| NGC 424 | 0.0118 | 41.60 | 43.93 | 1 | - |
|
<0.024 |
| NGC 1068 | 0.0380 | 41.11 | 44.14 | 0.74 | b | - | - |
| NGC 1194 | 0.0136 | 41.53 | 43.58 | 0.91 | - |
|
<0.059 |
| NGC 1320 | 0.0890 | 40.83 | 43.41 | 0.83 | a |
|
0.082 |
| NGC 1667 | 0.0152 | 40.62 | 43.69 | 0 | a |
|
0.391 |
| F 07599+6508 | 0.1488 | 41.90 | 45.79 | 0.96 | - | - | 0.027 |
| UGC 5101 | 0.0394 | 41.70 | 44.10 | 0 | - |
|
0.229 |
| Mrk 231 | 0.0422 | 42.28 | 45.23 | 0.95 | - |
|
0.011 |
| NGC 4968 | 0.0099 | 40.66 | 43.44 | 0.92 | a |
|
0.172 |
| NGC 5256 | 0.0279 | 41.62 | 44.07 | 0 | - |
|
0.608 |
| Mrk 273 | 0.0378 | 41.98 | 44.20 | 0 | - |
|
0.192 |
| Mrk 463 | 0.0504 | 42.46 | 45.03 | 0.98 | - |
|
< 0.008 |
| Mrk 848 | 0.0402 | 41.54 | 44.51 | 0.79 | - |
|
- |
| †2MASX J15504152 | 0.0303 | 41.87 | 43.79 | 0.48 | c |
|
- |
| NGC 6552 | 0.0265 | 41.79 | 44.55 | 0.95 | b | - | - |
| F 19254-7245 | 0.0617 | 42.23 | 44.60 | 0.88 | - |
|
0.064 |
| NGC 6890 | 0.0081 | 40.52 | 43.13 | 0.24 | c |
|
0.237 |
| NGC 7479 | 0.0079 | 40.57 | 43.92 | 0.70 | a |
|
- |
| NGC 7582 | 0.0053 | 41.05 | 43.44 | 0 | c | 0.04 | - |
| NGC 7674 | 0.0289 | 41.95 | 44.32 | 0.58 | c | - | 0.132 |
| ESO 286-IG019 | 0.0430 | 41.56 | 44.19 | 0.85 | - |
|
- |
| ESO 148-IG002 | 0.0446 | 41.78 | 44.07 | 0 | c | - | - |
Notes. The columns are: (1) name; (2) spectroscopic redshift; (3) logarithm of luminosity in the 2–10 keV band uncorrected for absorption in units of erg s-1; (4) logarithm of 6 μm luminosity in units of erg s-1; (5) fraction of the AGN contribution to the 6 μm luminosity; (6) compton-thick classification from Brightman & Nandra (2011a) based on: a: direct measurement of the column density; b: large EW of Fe Kα line; c: large reflection component; (7) NH column density in units of 1022 cm-2 from Brightman & Nandra (2011a); (8) EW of the 6.2 μm PAH in units of μm from Wu et al. (2009); .
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