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Table 2.
Additional emission lines detected in the Mg II parent sample.
| Mg II class |
|||||
|---|---|---|---|---|---|
| Emitters (66) | P-Cygni (19) | Absorbers (42) | No detection (265) | Galaxies with MUSE coverage | |
| [O III]λ5007 | 8 | – | 6 | 48 | 67 |
| [O III]λ4959 | 7 | – | 6 | 35 | 67 |
| [Ne III]λ3869 | 37 | 13 | 21 | 88 | 301 |
| [O II]λ3726 | 50 | 14 | 29 | 188 | 323 |
| [O II]λ3729 | 50 | 14 | 29 | 213 | |
| [C III]λ1907 | 10 | 2 | 2 | 13 | 57 |
| [C III]λ1909 | 9 | 1 | 1 | 15 | |
| Hβ | 10 | 1 | 7 | 43 | 77 |
| Hγ | 30 | 8 | 24 | 95 | 215 |
| Hδ | 30 | 10 | 26 | 71 | 239 |
Notes. Number of galaxies with an emission line S/N > 3 from PLATEFIT. The last column reports the total number of galaxies of the Mg II parent sample with a MUSE spectrum that covers the rest-frame wavelength of the line.
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