Table 1
Spitzer IRS properties of the high-τ 9.7 μm AGN in the 12 μm sample.
| Name | z | Type | τ | log [νL6 μm] | AGN | EW(6.2) |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) |
|
|
||||||
| Mrk 938 | 0.020 | Sy2 | 1.2 | 10.09 | 0 | 0.440 |
| NGC 1125 | 0.011 | Sy2 | 1.0 | 9.12 | 0.81 | 0.258 |
| I 08572+3915 | 0.058 | Sy2 | 3.5 | 11.51 | 0.98 | <0.021 |
| UGC 5101 | 0.039 | Sy1 | 1.4 | 10.52 | 0 | 0.229 |
| NGC 3079 | 0.004 | Sy2 | 1.3 | 9.10 | 0 | 0.458 |
| Mrk 266 | 0.028 | Sy2 | 1.0 | 10.03 | 0 | 0.608 |
| Mrk 273 | 0.038 | Sy2 | 1.7 | 10.51 | 0 | 0.192 |
| Arp 220 | 0.018 | Sy2 | 2.4 | 9.86 | 0 | 0.344 |
| I 19254-7245 | 0.062 | Sy2 | 1.2 | 11.03 | 0.88 | 0.064 |
| NGC 7172 | 0.009 | Sy2 | 1.9 | 9.75 | 0.2 | 0.045 |
| NGC 7582 | 0.005 | Sy2 | 1.0 | 9.56 | 0 | 0.274 |
Notes. The columns are: (1) Name; (2) Redshift; (3) Optical AGN type; (4) Optical depth at 9.7 μm; (5) Logarithm of νLν IR monochromatic luminosity; at 6 μm in units of solar luminosity; (6) Fraction of AGN contribution at 6 μm according to the spectral decomposition based on broad-band mid-IR photometry available from NED (see Sect. 3.2.3 for details of the models used); (7) Equivalent-width of PAH 6.2 μm feature in units of μm taken from Wu et al. (2009).
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