Table 5.
Sources with an AGN signature in IR or X-rays.
| No. | Galaxy | AGNbol | [Ne v] | PAH | X |
|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | ||
| 45 | UGC 08387 | 0.03 ± 0.01 | Y | N | N |
| 57 | IRAS F06076−2139 (S) | − | N | N | C |
| 68 | IRAS F16164−0746 | 0.05 ± 0.01 | Y | N | C |
| 71 | NGC 2623 | 0.10 ± 0.03 | Y | N | C |
| 72 | IC 5298 | 0.33 ± 0.05 | Y | N | A |
| 79 | NGC 5256 (NE) | 0.23 ± 0.07(u) | Y(u) | N | A |
| 79 | NGC 5256 (SW) | 0.23 ± 0.07(u) | Y(u) | N | L |
| 82 | NGC 0034 | 0.04 ± 0.02 | N | N | A |
| 85 | IRAS F17138−1017 | 0.07 ± 0.04 | N | N | C |
| 100 | NGC 7130 | 0.22 ± 0.04 | Y | N | LA |
| 105 | NGC 7592 (W) | 0.20 ± 0.06 | Y(u) | N | N |
| 106 | NGC 6286 | 0.11 ± 0.06 | N | N | A* |
| 107 | NGC 4922 (N) | 0.17 ± 0.05 | Y | N | A |
| 114 | NGC 0232 | 0.09 ± 0.03 | Y | N | N |
| 120 | CGCG 049−057 | 0.04 ± 0.02 | N | N | C |
| 121 | NGC 1068 | 1.00 ± 0.01 | Y | − | L |
| 127 | MCG−03−34−064 | 0.88 ± 0.04 | Y | Y | LA |
| 136 | MCG −01−60−022 | 0.08 ± 0.06 | N | − | CA |
| 142 | NGC 5135 | 0.24 ± 0.06 | Y | N | L |
| 144 | IC 0860 | 0.06 ± 0.03 | N | N | C |
| 163 | NGC 4418 | 0.48 ± 0.22 | N | Y | N |
| 169 | ESO 343−IG013 (N) | 0.09 ± 0.04 | N | N | C |
| 191 | ESO 420−G013 | 0.25 ± 0.04 | Y | N | N |
| 194 | ESO 432−IG006 (NE) | 0.12 ± 0.04 | N | N | A |
| 194 | ESO 432−IG006 (SW) | 0.09 ± 0.05 | N | N | A |
| 198 | NGC 1365 | 0.38 ± 0.03 | N | N | CLA |
Notes. Column (1): Contribution of the AGN to the bolometric luminosity of the galaxy (Díaz-Santos et al. 2017). Column (2): Detection of the [Ne v] line (Petric et al. 2011). Column (3): EW of the 6.2 μm PAH feature < 0.1 μm (Stierwalt et al. 2013). Column (4): X-ray AGN selection criteria. C: X-ray color (HR > −0.3); L: Detection of 6.4 KeV line. A: Absorbed AGN feature. Y: Source meets the criterion. N: Source does not meet the criterion. (u) Unresolved detection in a multiple system.
Only in the NuSTAR data (Ricci et al. 2016). See Appendix A for details on particular sources.
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