Table C.1
SED fitting results of every individual LAE image.
ID | μ | Log(M⋆/M⊙) | Log(AgeSSP/ yr) | E(B−V) | Log(SFR/(M⊙ yr-1)) | Log(sSFR/yr) | β | f esc,Lyα | M F 814 W |
|
|||||||||
NE-91 | 4.41 ± 0.11 | 8.04![]() |
8.26![]() |
0.03![]() |
–0.38![]() |
–8.56![]() |
−2.42 ± 0.09 | 0.18 | 26.176 |
SW-49a | 16.50 ± 1.00 | 6.79![]() |
6.82![]() |
0.03![]() |
–0.52![]() |
–7.42![]() |
−2.79 ± 0.10 | 2.10 | 25.648 |
SW-49b | 15.80 ± 0.92 | 7.01![]() |
6.64![]() |
0.06![]() |
0.15![]() |
–6.70![]() |
−2.79 ± 0.05 | 0.68 | 25.568 |
SW-50 | 11.20 ± 0.76 | 8.23![]() |
6.28![]() |
0.30![]() |
1.88![]() |
-6.34![]() |
−1.95 ± 0.05 | 0.01 | 24.825 |
SW-68a | 6.09 ± 0.12 | 7.78![]() |
7.18![]() |
0.10![]() |
0.30![]() |
–7.50![]() |
−2.09 ± 0.08 | 0.56 | 25.392 |
NE-93a | 4.95 ± 0.12 | 6.28![]() |
6.46![]() |
0.03![]() |
–0.39![]() |
–6.58![]() |
–2.85± 0.50 | 0.63 | 28.264 |
NE-93b | 5.08 ± 0.11 | 6.20![]() |
6.52![]() |
0.04![]() |
–0.55![]() |
–6.64![]() |
−2.85 ± 0.41 | 1.23 | 28.466 |
SW-51 | 55.60 ± 8.95 | 6.81![]() |
7.59![]() |
0.05![]() |
–0.96![]() |
–7.87![]() |
–2.31± 0.05 | 0.27 | 25.440 |
NE-94a | 7.09 ± 0.15 | 8.50![]() |
6.70![]() |
0.30![]() |
1.61![]() |
–6.74![]() |
–1.76 ± 0.08 | 0.03 | 24.734 |
NE-94b | 8.12 ± 0.21 | 8.15![]() |
7.30![]() |
0.20![]() |
0.55![]() |
–7.42![]() |
−1.85 ± 0.18 | 0.07 | 25.445 |
NE-96 | 4.78 ± 0.13 | 7.33![]() |
7.24![]() |
0.10![]() |
–0.36![]() |
–7.48![]() |
−2.14 ± 0.22 | 0.52 | 27.487 |
NE-97 | 2.98 ± 0.06 | 6.35![]() |
6.46![]() |
0.03![]() |
–0.23![]() |
–6.52![]() |
−2.90 ± 0.15 | 0.27 | 28.704 |
SW-52a | 23.6 ± 1.47 | 5.93![]() |
6.22![]() |
0.03![]() |
–0.32![]() |
–6.28![]() |
−3.05 ± 0.10 | 0.32 | 27.557 |
SW-52b | 27.9 ± 1.56 | 6.40![]() |
7.12![]() |
0.03![]() |
–0.91![]() |
–7.30![]() |
–2.50 ± 0.28 | 2.46 | 26.719 |
NE-98a | 8.84 ± 0.35 | 6.46![]() |
6.16![]() |
0.01![]() |
0.28![]() |
–6.19![]() |
−3.17 ± 0.02 | 0.24 | 27.491 |
NE-98b | 8.95 ± 0.24 | – | – | – | – | – | – | – | 27.855 |
NE-99a | 9.91 ± 0.33 | – | – | – | – | – | – | – | 28.854 |
NE-99b | 10.10 ± 0.29 | – | – | – | – | – | – | – | 29.584 |
NE-100 | 7.87 ± 0.21 | – | – | – | – | – | – | – | – |
NE-101d | 6.53 ± 0.51 | 8.13![]() |
6.34![]() |
0.02![]() |
1.72![]() |
–6.40![]() |
−3.18 ± 0.00 | 0.17 | – |
SW-53a | 5.56 ± 0.33 | 7.59![]() |
5.95![]() |
0.00![]() |
1.68![]() |
–5.95![]() |
−3.02 ± 0.05 | 0.09 | 26.198 |
SW-53b | 5.97 ± 0.12 | 7.47![]() |
6.04![]() |
0.00![]() |
1.37![]() |
–6.10![]() |
−3.17 ± 0.02 | 0.43 | 26.627 |
SW-70aa | 8.43 ± 0.248 | 8.58![]() |
6.10![]() |
0.25![]() |
2.45![]() |
–6.16![]() |
−2.00 ± 0.02 | 0.00 | 23.233 |
SW-70ba | 5.79 ± 0.146 | 8.84![]() |
7.00![]() |
0.20![]() |
1.81![]() |
–7.03![]() |
−1.83 ± 0.12 | 0.01 | 24.018 |
Notes. Results of SED modelling of all individual images of LAEs. The stellar masses and SFRs have been corrected for lensing, using the magnification factor given in the second column. The last column shows the observed magnitude in the F814W HST band without correcting for magnification. LAEs NE-98b, NE-99a, NE-99b, and NE-100 did not have enough photometric detections to perform a sensible modelling.
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