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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.


Names using the air wavelengths of the emission lines.

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