Table D.1
Results from the Lyα line modelling simulations of all images of LAEs.
| ID | z | f Ly α | Log(LLyα/(erg/s)) | Log(NH/cm-2) | v exp | SFR Lyα |
| 10-20 erg/s/cm-2 | km s-1 | M⊙ yr-1 | ||||
|
|
||||||
| NE-91 | 2.9760 | 4.7 ± 0.6 | 40.9 ± 0.0611 | – | – | 0.0741 |
| SW-49a | 3.1169 | 179.0 ± 21.3 | 42.0 ± 0.0551 | 17.1 |
72.9 |
0.83 |
| SW-49b | 3.1169 | 198.0 ± 33.1 | 42.0 ± 0.0795 | 17 |
60.7 |
0.965 |
| SW-50 | 3.1169 | 110.0 ± 2.0 | 41.9 ± 0.00803 | 17.5 |
124 |
0.757 |
| SW-68a | 3.1166 | 118.0 ± 1.0 | 42.2 ± 0.00364 | 20 |
463 |
1.49 |
| NE-93a | 3.1696 | 15.8 ± 1.6 | 41.4 ± 0.0469 | 19 |
42.9 |
0.255 |
| NE-93b | 3.1701 | 21.9 ± 1.3 | 41.6 ± 0.0265 | 17.7 |
46.4 |
0.345 |
| SW-51 | 3.2271 | 19.8 ± 0.9 | 40.5 ± 0.0206 | 18.5 |
98 |
0.0297 |
| NE-94a | 3.2848 | 37.2 ± 1.9 | 41.7 ± 0.0228 | 19.4 |
192 |
0.458 |
| NE-94b | 3.2854 | 44.4 ± 2.2 | 41.7 ± 0.0219 | 19 |
174 |
0.477 |
| NE-96 | 3.4514 | 10.9 ± 0.7 | 41.4 ± 0.0291 | 18.6 |
56.7 |
0.224 |
| NE-97 | 3.7131 | 4.6 ± 0.6 | 41.3 ± 0.0581 | 20.4 |
181 |
0.181 |
| SW-52a | 4.1130 | 24.9 ± 0.9 | 41.2 ± 0.0165 | 17.3 |
87.8 |
0.157 |
| SW-52b | 4.1128 | 29.8 ± 1.1 | 41.2 ± 0.0167 | 17 |
108 |
0.159 |
| NE-98a | 5.0514 | 16.5 ± 0.7 | 41.7 ± 0.0198 | 19.4 |
149 |
0.451 |
| NE-98b | 5.0549 | 4.7 ± 0.7 | 41.1 ± 0.0693 | 18.2 |
-4.93 |
0.127 |
| NE-99a | 5.2399 | 10.5 ± 1.2 | 41.5 ± 0.0506 | 18.5 |
236 |
0.28 |
| NE-99b | 5.2415 | 12.1 ± 1.1 | 41.5 ± 0.0423 | 17.4 |
-19.8 |
0.315 |
| NE-100 | 5.8940 | 4.7 ± 2.5 | 41.4 ± 0.329 | – | – | 0.207 |
| NE-101d | 6.1074 | 150.0 ± 1.9 | 43 ± 0.00546 | – | – | 8.67 |
| SW-53a | 6.1074 | 63.4 ± 2.7 | 42.7 ± 0.0189 | 19.8 |
151 |
4.31 |
| SW-53b | 6.1074 | 161.0 ± 4.0 | 43 ± 0.0109 | – | – | 10.2 |
| SW-70a | 3.6065 | – | 41.2 ± 2.0 | – | – | 0.129 |
| SW-70b | 3.6065 | – | 41.3 ± 2.0 | – | – | 0.188 |
Notes. We report in Col. 2 the intrinsic redshift obtained from modelling the Lyα profile. Column 3 gives the observed Lyα flux without correcting for lensing, while we corrected LLya and SFRLyα for the effect of gravitational magnification using the magnification factors given in Table C.1.
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