Table 5
Summary of the optical and Spitzer-IRS analyses.
| Ident. | Activity | Spectrum |
| class Opt. | Morph. MIR | |
|
|
||
| NGC 1052 | LIN(H) | 4 |
| NGC 1209 | LIN(H) | 1 |
| NGC 1297 | LIN(H) | 2 |
| NGC 1366 | IN | 1 |
| NGC 1389 | IN | 0 |
| NGC 1407 | IN | 0 |
| NGC 1426 | IN | 0 |
| NGC 1453 | LIN(H) | 2 |
| NGC 1533 | LIN(H) | 2 |
| NGC 1553 | LIN(W) | 2 |
| NGC 2974 | LIN(H) | 2 |
| NGC 3258 | Comp(H) | 3 |
| NGC 3268 | LIN(H) | 3 |
| NGC 3557 | LIN(W) | 2 |
| NGC 3818 | IN(Traces) | 0 |
| NGC 3962 | LIN(H) | 2 |
| NGC 4374 | LIN(H) | 2 |
| NGC 4552 | Comp(W) | 2 |
| NGC 4636 | LIN(H) | 2 |
| NGC 4696 | LIN(H) | 2 |
| NGC 4697 | LIN(W) | 3 |
| NGC 5011 | LIN(W) | 1 |
| NGC 5044 | LIN(H) | 2 |
| NGC 5077 | LIN(H) | 2 |
| NGC 5090 | LIN(H) | 2 |
| NGC 5638 | IN | 0 |
| NGC 5812 | IN | 0 |
| NGC 5813 | LIN(W) | 1 |
| NGC 5831 | IN | 0 |
| NGC 5846 | LIN(H) | 1 |
| NGC 5898 | LIN(W) | 2 |
| NGC 6868 | LIN(H) | 2 |
| NGC 7079 | LIN(W) | 2 |
| NGC 7192 | LIN(W) | 1 |
| NGC 7332 | IN(Traces) | 1 |
| IC 1459 | LIN(H) | 2 |
| IC 2006 | Comp(W) | 0 |
| IC 3370 | LIN(H) | 2 |
| IC 4296 | LIN(H) | 2 |
| IC 5063 | AGN | 4 |
Notes. Summary of the present observations and comparison with Paper IV. The optical activity class (Col. 2: Paper IV) uses the following notation: LIN = LINER; AGN = AGN like emission; IN = either faint (Traces) or no emission lines; Comp = transition between HII regions and LINERs. W and H indicate weak emission (EW(Hα + [N ii]λ6584) < 3 Å) and strong emission line galaxies, respectively. In Col. 3 we report the MIR spectrum morphology discussed in Sect. 4.
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