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Table 1.
Optical and near-IR rest-frame lines that we are able to detect in our spectra of star-forming galaxies and AGN in the redshift range 0 ≤ z ≤ 3, and that we consider in this paper.
| Ion | λrest [μm] |
|---|---|
| Hβ | 0.4861 |
| [O III] | 0.4959, 0.5007 |
| [O I] | 0.6300 |
| [N II] | 0.6548, 0.6583 |
| Hα | 0.6563 |
| [S II] | 0.6716, 0.6731 |
| [O II] | 0.7331, 0.7320 |
| [S III] | 0.9069, 0.9531 |
| [C I] | 0.985026 |
| Paδ | 1.0049 |
| He I | 1.083 |
| Paγ | 1.0938 |
| [P II] | 1.18828 |
| Paβ | 1.2818 |
| [Fe II] | 1.257, 1.32 |
| [Fe II] | 1.64 |
| Paα | 1.875 |
| [Si VI] | 1.962 |
| H2 | 2.121 |
| Brγ | 2.1655 |
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