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Table C.1

SED fitting results of every individual LAE image.

ID μ Log(M/M) Log(AgeSSP/ yr) E(BV) 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.

(a)

Lyman break galaxy, no significant Lyα emission.

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