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Table 4

Stellar properties derived from SED modelling using LePhare in combination with BC03 templates.

ID Log(M/M) Log(AgeSSP/ yr) E(BV) Log(SFRSED/(M yr-1)) Log(sSFR/yr) β MUV

NE-91 8.02 8.26 0.03 –0.38 –8.56 2.42 ± 0.09 –17.77
SW-49 6.91 6.70 0.045 –0.16 –7.00 2.79 ± 0.08 –17.09
SW-50 8.23 6.28 0.30 1.88 –6.34 1.95 ± 0.05 –18.05
SW-68 7.78 7.12 0.10 0.36 –7.39 2.09 ± 0.08 –18.18
NE-93 6.24 6.49 0.035 -0.47 –6.61 2.85 ± 0.46 –15.63
SW-51 6.81 7.59 0.05 –0.96 –7.87 2.31 ± 0.05 –15.83
NE-94 8.50 6.70 0.30 1.61 –6.74 1.77 ± 0.08 –18.30
NE-96 7.33 7.24 0.10 –0.36 –7.46 2.14 ± 0.22 –16.60
NE-97 6.35 6.40 0.03 –0.18 –6.47 2.90 ± 0.15 –15.98
SW-52 6.36 7.12 0.03 –0.90 –7.26 2.50 ± 0.28 −15.33
NE-98 6.46 6.16 0.01 0.28 –6.19 3.17 ± 0.02a –16.19
NE-99 –14.42
NE-100 >–14.70
SW-53 7.47 6.04 0.00 1.37 –6.10 −3.17 ± 0.02 a –18.97

Notes. The properties were derived after averaging the results of multiple images of the same source, if applicable. See Appendix C for results of all individual LAEs.

(a)

This is the maximal UV slope in our used templates, the photometric UV-slope is steeper and the small errors are therefore not representative but a result of our method of calculating β.

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