Table 1
Sample properties.
| Num | Name | D(Mpc) | Slit width(arcsec)/Size(pc) | Type | Optical features | log (NH) | log (L(2–10 keV)) | X-ray Ref. | b/a |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) |
|
|
|||||||||
| 1 | NGC 1365 | 17.9 | 0.35/30 | S1.5 | 23.6 | 42.5 | (1, 11) | 0.5 | |
| 2 | NGC 1386 | 16.2 | 0.31/24 | S2 | E | >25.0 | 42.6 | (2, 3) | 0.4 |
| 3 | NGC 1808 | 11.5 | 0.35/19 | S2 | 22.9 | 40.4 | (3, 12) | 0.6 | |
| 4 | NGC 3081 | 32.5 | 0.65/102 | S2 | 23.9 | 42.5 | (2) | 0.8 | |
| 5 | NGC 3094 | 44.7 | 0.35/76 | S2 | 0.7 | ||||
| 6 | NGC 3281 | 45.7 | 0.35/77 | S2 | D, E | 24.3 | 43.4 | (1, 12) | 0.4 |
| 7 | NGC 4418 | 31.1 | 0.35/53 | S2 | E | >25.0 | 41.2 | (4) | 0.4 |
| 8 | NGC 4945 | 4.0 | 0.65/13 | S2 | D, E, M | 24.7 | 42.3 | (5, 12) | 0.4 |
| 9 | Centaurus A | 3.7 | 0.65/12 | S2 | D, E | 23.7 | 41.9 | (1, 13) | 0.4 |
| 10 | NGC 5135 | 58.6 | 0.70/199 | S2 | >25.0 | 43.1 | (2) | 0.7 | |
| 11 | Circinus | 4.2 | 0.35/7 | S2 | M | 24.6 | 42.6 | (6, 2) | 0.5 |
| 12 | NGC 5506 | 28.8 | 0.35/49 | S1.9 | D, E | 22.5 | 43.0 | (1, 3) | 0.2 |
| 13 | NGC 5643 | 16.9 | 0.35/29 | S2 | 23.8 | 42.6 | (7, 12) | 0.9 | |
| 14 | NGC 5728 | 29.1 | 0.35/49 | S1.9 | 23.6 | 43.3 | (6) | 0.6 | |
| 15 | IC 4518W | 69.6 | 0.70/236 | S2 | E, M | 24.3 | 42.6 | (8, 13) | 0.1 |
| 16 | ESO 103−G35 | 56.9 | 0.35/96 | S2 | E | 23.2 | 43.4 | (1, 12) | 0.4 |
| 17 | IC 5063 | 48.6 | 0.65/153 | S2 | D | 23.3 | 43.3 | (1, 12) | 0.7 |
| 18 | NGC 7130 | 69.2 | 0.70/235 | L2 | M | >25.0 | 43.1 | (10, 2) | 0.9 |
| 19 | NGC 7172 | 33.9 | 0.35/57 | S2 | D | 22.9 | 42.8 | (1, 3) | 0.6 |
| 20 | 3C 445 | 239.3 | 0.35/406 | S1.5 | 23.5 | 43.9 | (3) | 0.9 | |
| 21 | NGC 7479 | 33.8 | 0.35/57 | L1.9 | D, M | 24.3 | 42.0 | (3) | 0.8 |
| 22 | NGC 7582 | 20.6 | 0.70/70 | S2 | D, E | 23.0 | 42.6 | (2) | 0.4 |
Notes. The size of the region observed by T-ReCS is computed using the slit width. Optical features: (D) Dust features across the nuclear region; (E) Edge-on galaxies; (M) Merger.
Reference. The references for the X-ray results are: (1) Tueller et al. (2008); (2) Marinucci et al. (2012); (3) Brightman & Nandra (2011); (4) Maiolino et al. (2003); (5) Itoh et al. (2008); (6) Goulding et al. (2012); (7) Guainazzi et al. (2004); (8) Pereira-Santaella et al. (2011); (9) Moran et al. (1996); (10) Mullaney et al. (2011); (11) Risaliti et al. (2009); (12) Comastri (2004); and (13) de La Rosa et al. (2011).
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