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Table 5.
Line fluxes of the most prominent lines visible in the optical spectrum of SALT as fitted in the narrower window with the best coverage of the Fe II templates (model B).
| Line | Wavelength | Shift | FWHM | Flux | Wλ |
|---|---|---|---|---|---|
| [Å] | [km s−1] | [km s−1] | [10−17 erg s−1 cm−2] | [Å] | |
| Fe II | 4434–4684 | 108.3 |
1750 ± 250 | 1966 ± 22 | 61.95 |
| Fe II | 4434–4684 | 470.4 |
10000 ± 250 | 1117 |
35.19 |
| Hβ | 4861.3 | −83 ± 11 | 431 |
59 ± 13 | 1.89 ± 0.41 |
| Hβ | 4861.3 | −496 |
849 ± 37 | 159 |
5.09 |
| Hβ | 4861.3 | 93 ± 13 | 2035 |
1076 ± 23 | 34.36 ± 0.71 |
| Hβ | 4861.3 | −694.7 |
4535 |
463 |
14.76 |
| Hγ | 4340.4 | 326.8 |
98 |
1.57 |
0.0489 |
| Hγ | 4340.4 | 2189 |
648 |
18.9 |
0.59 ± 0.17 |
| Hγ | 4340.4 | 2862 |
832 |
31.9 |
1.00 |
| Hγ | 4340.4 | 703 |
1710 |
490.3 |
15.30 |
| [O III] | 5006.843 | −81.6 |
227.1 |
54.8 |
1.76 |
| [O III] | 5006.843 | −388 |
402.3 |
93.5 |
3.00 ± 0.12 |
Notes. Flux of the narrowest [O III] component was used to normalize the SALT spectrum to the corresponding flux of the MUSE fit.
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