Table 2
Emission line strengths for the central aperture.
| Galaxy | [O ii] | [Ne iii] | [O iii] | [O iii] | [N ii] | [S ii] | [S ii] |
| 3727 | 3868 | 4959 | 5007 | 6583 | 6717 | 6731 | |
|
|
|||||||
| NGC 1169 | 525 ± 25 | – | – | 207 ± 10 | – | – | – |
| NGC 1358 | 278 ± 13 | 65 ± 3 | 370 ± 18 | 1153 ± 55 | – | – | – |
| NGC 1433 | – | – | 51 ± 2 | 155 ± 7 | 103 ± 6 | 34 ± 2 | 28 ± 2 |
| NGC 1530 | 135 ± 40 | – | – | 23.5 ± 1.5 | – | – | – |
| NGC 1832 | 28.6 ± 1.4 | – | 26.9 ± 1.3 | 33.5 ± 1.6 | – | – | – |
| NGC 2217 | – | – | 100 ± 5 | 306 ± 14 | 226 ± 13 | 131 ± 11 | 115 ± 10 |
| NGC 2273 | 168 ± 8 | 68 ± 3 | 237 ± 11 | 184 ± 9 | – | – | – |
| NGC 2523 | 211 ± 10 | – | 194 ± 9 | 306 ± 15 | – | – | – |
| NGC 2665 | – | – | 23 ± 1 | 72 ± 3 | 67 ± 3 | 19 ± 1 | 20 ± 1 |
| NGC 2681 | 71 ± 3 | – | 105 ± 5 | 164 ± 8 | – | – | – |
| NGC 2859 | 421 ± 20 | – | 99 ± 5 | 178 ± 8 | – | – | – |
| NGC 2935 | – | – | 45 ± 2 | 128 ± 6 | 71 ± 3 | 24 ± 1 | 19 ± 1 |
| NGC 2950 | – | – | – | – | – | – | – |
| NGC 2962 | 399 ± 19 | – | 67 ± 3 | 174 ± 8 | – | – | – |
| NGC 3081 | – | 84 ± 4 | 414 ± 20 | 1242 ± 60 | 88 ± 6 | 23 ± 1 | 21 ± 2 |
| NGC 4245 | – | – | – | – | – | – | – |
| NGC 4314 | 230 ± 11 | – | 93 ± 4 | 203 ± 10 | – | – | – |
| NGC 4394 | 289 ± 14 | – | 108 ± 5 | 205 ± 10 | – | – | – |
| NGC 4643 | – | – | 115 ± 5 | 73 ± 3 | 98 ± 12 | 31 ± 5 | – |
| NGC 5101 | – | – | 86 ± 4 | 114 ± 5 | 189 ± 12 | 75 ± 7 | 59 ± 6 |
Notes. Emission line strengths for the central aperture of the galaxies, except for NGC 4314, which is at 0.8 arcsec from the galaxy center. The line fluxes of [O ii], [Ne iii], and [O iii] lines are measured relative to a Hβ flux of 100 and those of [N ii] and [S ii] lines are measured relative to a Hα flux of 100.
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