Table 3
Emission lines from the warm ISM.
| Species | Wavelength (Å) | N 0 | Group ID |
| (1) | (2) | (3) | (4) |
|
|
|||
| [O ii] | 3728.73 | Single | 1 |
| [Ne iii] | 3868.69 | Group | 2 |
| [He i] | 3888.65 | Group | 2 |
| [Ne iii] | 3967.40 | Group | 2 |
| Hϵ | 3970.07 | Group | 2 |
| Hδ | 4101.73 | Group | 2 |
| Hγ | 4340.46 | Group | 3 |
| [O iii] | 4363.15 | Group | 3 |
| Hβ | 4861.32 | Single | 4 |
| [O iii] | 4958.83 | Doublet | 5 |
| [O iii] | 5006.70 | Doublet | 5 |
| [O i] | 6300.20 | Doublet | 6 |
| [O i] | 6363.67 | Doublet | 6 |
| [N ii] | 6547.96 | Group | 7 |
| Hα | 6562.80 | Group | 7 |
| [N ii] | 6583.34 | Group | 7 |
| [S ii] | 6716.31 | Doublet | 8 |
| [S ii] | 6730.68 | Doublet | 8 |
Notes. Emission lines (Col. 2) are evaluated as single lines, doublets, or groups (Col. 1). The central wavelength of each line and its group ID are given in Cols. 3 and 4, respectively. We note that the [O ii] line is in reality a line doublet, separated by 3 Å. The doublet is unresolved at the spectral resolution of GAMA (5.5 Å) and the line profile is well described by a single Gaussian.
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