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Table 2
Same as Table 1 for the IUE sample.
| Object | RA | Dec | z | Lyα | [Oii] | Hβ | [Oiii]λ5007 | Hα | [Nii]λ6583 |
| (J2000) | (J2000) | ||||||||
|
|
|||||||||
| Haro15 | 00:48:35.4 | –12:43:00 | 0.0210 | 8.2 ± 0.4 | 25.91 ± 0.16 | 7.88 ± 0.17 | 18.72 ± 0.17 | 36.71 ± 0.20 | 5.13 ± 0.21 |
| IC1586 | 00:47:56.3 | +22:22:22 | 0.0193 | 2.5 ± 0.2 | 14.57 ± 0.12 | 4.80 ± 0.11 | 5.32 ± 0.11 | 21.39 ± 0.09 | 3.99 ± 0.09 |
| IC214 | 02:14:05.6 | +05:10:24 | 0.0301 | –9.1 ± 0.8 | 3.87 ± 0.08 | 2.82 ± 0.07 | 3.87 ± 0.08 | 15.43 ± 0.06 | 4.78 ± 0.06 |
| Mrk357 | 01:22:40.6 | +23:10:15 | 0.0528 | 15.0 ± 1.0 | 14.00 ± 0.06 | 7.85 ± 0.06 | 21.63 ± 0.07 | 31.09 ± 0.06 | 4.72 ± 0.06 |
| Mrk477 | 14:40:38.1 | +53:30:16 | 0.0381 | 77.0 ± 0.9 | 23.75 ± 0.20 | 12.32 ± 0.22 | 121.00 ± 0.21 | 49.29 ± 0.17 | 20.77 ± 0.16 |
| Mrk499 | 14:40:38.1 | +53:30:16 | 0.0256 | –20.6 ± 0.8 | 6.68 ± 0.07 | 2.42 ± 0.07 | 6.24 ± 0.07 | 13.58 ± 0.06 | 3.49 ± 0.06 |
| Mrk66 | 13:25:53.8 | +57:15:16 | 0.0216 | 7.1 ± 0.4 | 15.55 ± 0.12 | 5.08 ± 0.11 | 15.23 ± 0.12 | 13.53 ± 0.09 | 2.17 ± 0.09 |
| NGC5860 | 15:06:33.8 | +42:38:29 | 0.0181 | 4.7 ± 0.4 | 3.73 ± 0.16 | 4.06 ± 0.11 | 2.75 ± 0.17 | 31.47 ± 0.09 | 13.99 ± 0.09 |
| NGC6090 | 16:11:40.7 | +52:27:24 | 0.0293 | 11.0 ± 0.5 | 16.03 ± 0.19 | 13.43 ± 0.20 | 8.11 ± 0.20 | 65.86 ± 0.15 | 28.21 ± 0.15 |
| 1941-543 | 19:45:00.5 | –54:15:03 | 0.0193 | 7.3 ± 0.9 | 20.73 ± 0.21 | 7.74 ± 0.22 | 25.31 ± 0.21 | 28.02 ± 0.24 | 2.53 ± 0.25 |
| Tol1924-416 | 19:27:58.2 | –41:34:32 | 0.0098 | 58.0 ± 0.4 | 71.97 ± 0.17 | 36.73 ± 0.15 | 173.50 ± 0.16 | 112.22 ± 0.15 | 2.50 ± 0.14 |
Notes. The line fluxes are in units of 10-14 erg s-1 cm-2. The Lyα flux is measured in the IUE spectra.
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