Table 2
Spectroscopically identified line emitters.
| Emission line(s) | Air namesa | z 1 | z 2 | N |
|
|
||||
| [S iii]9533 | [S iii]9531 | 0.238 | 0.260 | 8 |
| [S iii]9071 | [S iii]9069 | 0.301 | 0.324 | 1 |
| [Ar iii]7138 | [Ar iii]7135 | 0.654 | 0.683 | 1 |
| [S ii]6718,6733 | [S ii]6716,6731 | 0.753 | 0.788 | 14 |
| Hα+[N ii] | Hα+[N ii] | 0.793 | 0.834 | 66 |
| [O iii]4960,5008 | [O iii]4959,5007 | 1.357 | 1.422 | 6 |
| Hβ | Hβ | 1.428 | 1.471 | 6 |
| [O ii]3727,3730 | [O ii]3726,3729 | 2.165 | 2.224 | 3 |
| Mg ii2796,2804 | Mg ii2796,2803 | 3.211 | 3.297 | 0 |
| Unidentified | Unidentified | ... | ... | 3 |
Notes. The table contains the candidate emission line objects with secure spectroscopic redshifts (see text). Each row corresponds to an emission line or a group of emission lines defined by the redshift interval z1,z2. The last row gives the number of objects that do not fall into any of these redshift intervals; one of these objects is likely an Mg ii emitting AGN, see text.
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