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Table 2.
Fluxes of the mid-IR nebular lines for the galaxies analysed in this work (in 10−17 W m−2 ≡ 10−14 erg cm−2 s−1).
| Object | [S IV]10.5 μm | [Ne II]12.8 μm | [Ne III]15.6 μm | [S III]18.7 μm | [O IV]25.9 μm |
|---|---|---|---|---|---|
| NGC 1386 | 24.3 ± 0.8 | 11.8 ± 0.4 | 38.1 ± 0.6 | 16.2 ± 0.6 | 97 ± 5 (a) |
| NGC 1097 | < 0.45 | 12 ± 2 | 1.7 ± 0.5 | 8.4 ± 0.5 | 3 ± 1 |
| NGC 1052 | < 1.2 | 22.4 ± 0.6 | 12.3 ± 0.7 | 4.8 ± 0.8 | 2.4 ± 0.6 (a) |
| NGC 4579 | < 1.6 | 13.1 ± 0.5 | 5.0 ± 0.2 | 2.3 ± 0.3 | 2 ± 1 (a) |
| NGC 3169 | < 0.24 | 7.5 ± 0.1 | 2.8 ± 0.2 | 1.2 ± 0.1 | 2.0 ± 0.8 (a) |
| NGC 4261 | < 0.27 | 3.0 ± 0.2 | 2.0 ± 0.2 | 0.7 ± 0.1 | 0.7 ± 0.3 (a) |
| M87 | 0.7 ± 0.3 | 4.9 ± 0.3 | 4.3 ± 0.3 | 2.0 ± 0.2 | 0.7 ± 0.3 (a) |
| NGC 4594 | 1.9 ± 0.5 | 8.5 ± 0.2 | 7.1 ± 0.2 | 1.3 ± 0.3 | 2.4 ± 0.6 (a) |
| NGC 404 | < 0.21 | 2.5 ± 0.1 | 0.50 ± 0.05 | 0.6 ± 0.1 | < 1.0 |
| 3C 273 | 3.6 ± 0.3 | 1.1 ± 0.2 | 4.2 ± 0.3 | 2.6 ± 0.5 | 8.5 ± 0.6 |
Notes. All fluxes have been extracted from Spitzer/IRS spectra acquired with the high-spectral resolution mode (R = 600) obtained from the CASSIS database and the Spitzer Heritage Archive.
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