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Table 5

Detected emission lines in the catalogue.

Transition(s) IDENTa Air wavelength(s)b Vacuum wavelength(s)b Detections Commentsc
[Å] [Å]
O vi λλ1032, 1038 O6_2 ... 1031.93, 1037.62 2 (1)
Lyαλ1216 Lya ... 1215.670 242 (2), (3)
N v λλ1238, 1242 N5 ... 1238.821, 1242.804 1 (4)
C iv λλ1549, 1550 C4 ... 1548.203, 1550.777 3 (3), (4)
Mg ii λ2796 Mg2 2795.528 2796.290 1
[O ii]λλ3726, 3729 O2 3726.032, 3728.815 3727.048, 3729.832 480 (3), (5)
[Ne iii]λ3869 Ne3 3869.06 3870.115 49
[Ne iii]λ3968 Ne32 3967.79 3968.872 3 (6)
Hζλ3889 Hzet 3889.049 3890.109 2
Hελ3970 Heps 3970.072 3971.154 1
Hδλ4102 Hd 4101.734 4102.852 18
Hγλ4340 Hg 4340.464 4341.647 74
[O iii]λ4363 O3_3 4363.210 4364.400 2
Hβλ4861 Hb 4861.325 4862.650 183 (3)
[O iii]λ4959 O3_1 4958.911 4960.263 135 (3)
[O iii]λ5007 O3_2 5006.843 5008.208 304 (3)
He i λ5876 He1 5875.615 5877.217 6
[O i]λ6300 O1 6300.304 6302.022 3
[N ii]λ6549 N2_1 6548.04 6549.825 4
Hαλ6563 Ha 6562.80 6564.589 73 (3)
[N ii]λ6583 N2_2 6583.46 6585.255 19
[S ii]λ6717 S2_1 6716.44 6718.271 30
[S ii]λ6730 S2_2 6730.81 6732.645 17

Notes.

(a)

Emission line identifier code used in the IDENT column of the emission line table described in Sect. 4.2.

(b)

Wavelengths are from the “Atomic Line List” compiled by P. van Hoof: http://www.pa.uky.edu/~peter/atomic/. Wavelengths longward of 2000 Å were queried in air wavelengths and converted to vacuum wavelengths with the formula used in the Vienna atomic line database (Ryabchikova et al. 2015): http://www.astro.uu.se/valdwiki/Air-to-vacuum%20conversion.

(c)

(1): Doublet in single object resolved into two individual line detections. (2): 237 LAEs, with five having the double peak profile resolved into two individual line detections. (3): Used for redshift determination. (4): Doublet unresolved, i.e. always detected as single line. (5): In all except eight detections (103035109, 105019069, 109021072, 109023081, 114015092, 115046179, 124009024, and 124040076) the [O ii]λλ3726, 3729 doublet is unresolved. (6): Blend with Hε.

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