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Table 3

Lyα luminosity and EW.

Candidate LLy α(1042 erg s-1) E WLy α

NB392_6-1 4.2 ± 3.3 116 ± 90
NB392_6-2 6.8 ± 4.0 190 ± 112

NB401_6-1 4.2 ± 4.2 66 ± 65
NB401_6-2 11.3 ± 8.5 160 ± 120
NB401_6-3 2.3 ± 2.4 112 ± 117
NB401_6-4 5.5 ± 3.1 47 ± 26
NB401_6-5 2.8 ± 2.1 93 ± 71
NB401_6-6 3.1 ± 2.1 297 ± 203
NB401_6-7 2.8 ± 3.7 24 ± 32
NB401_6-8 4.1 ± 3.0 150 ± 107
NB401_6-9 3.5 ± 2.4 75 ± 52
NB401_6-10 1.9 ± 2.1 35 ± 39
NB401_6-11 5.1 ± 4.3 30 ± 26
NB401_6-12 5.2 ± 5.3 87 ± 89
NB401_6-13 1.5 ± 1.5 58 ± 55
NB401_6-14 2.5 ± 2.1 58 ± 49
NB401_6-15 2.4 ± 2.7 66 ± 74
NB401_6-16 5.6 ± 5.0 115 ± 102
NB401_6-17 2.3 ± 2.3 98 ± 99
NB401_6-18 1.9 ± 2.3 54 ± 65
NB401_6-19 3.3 ± 2.2 60 ± 41
NB401_6-20 2.1 ± 1.5 125 ± 87
NB401_6-21 7.6 ± 6.5 120 ± 103

NB406_6-1 6.7 ± 5.4 142 ± 114

NB412_18-1 7.6 ± 10.2 103 ± 139

Notes. Lyα luminosities and equivalent widths for our LAE candidates. These quantities were calculated using the SED fit from model A for the continuum estimation. Candidates with detections in the far-IR (Sect. 5) are marked in bold.

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