Table A.1.
SED fitting: Full results.
| [Z/H] |  |
log(age) |  |
 |
log(LHα, int) |
|---|---|---|---|---|---|
| Burst | |||||
| -3.15 | +0.77 | 6.4 | 13.5 | 4.01 | 43.93 |
| -2.15 | 0.0 | 6.5 | 4.33 | 4.26 | 43.58 |
| -1.15 | +0.86 | 6.6 | 6.54 | 3.87 | 43.15 |
| -0.85 | +1.27 | 6.6 | 6.75 | 10.42 | 43.13 |
| -0.54 | +2.12 | 6.5 | 7.28 | 18.96 | 43.21 |
| -0.37 | +2.61 | 6.5 | 6.19 | 26.44 | 43.15 |
| -0.24 | +3.18 | 6.5 | 6.61 | 29.93 | 43.20 |
| -0.15 | +5.61 | 6.6 | 19.94 | 25.73 | 43.18 |
| 0.00 | +5.94 | 6.5 | 21.60 | 24.30 | 43.03 |
| Cont. | |||||
| -3.15 | +0.45 | 7.4 | 11.57 | 5.81 | 43.64 |
| -2.15 | +0.03 | 6.9 | 5.31 | 4.09 | 43.64 |
| -1.15 | 0.0 | 7.3 | 3.52 | 4.67 | 43.30 |
| -0.85 | +0.34 | 7.3 | 3.55 | 7.14 | 43.26 |
| -0.54 | +1.28 | 7.3 | 5.10 | 11.60 | 43.20 |
| -0.37 | +2.04 | 7.3 | 7.03 | 14.48 | 43.14 |
| -0.24 | +2.73 | 7.3 | 8.78 | 17.03 | 43.10 |
| -0.15 | +3.32 | 7.6 | 11.58 | 13.33 | 42.86 |
| 0.00 | +4.03 | 7.3 | 14.87 | 16.49 | 43.08 |
We list the best-fit model for each stellar metallicity and for a single-burst or continuous star formation that satisfies the additional bounds from the IR photometry (F105W> 25.2 and [4.5]> 25.3). The age is in yr. We list the goodness of fit using the full spectral data relative to the best model for a certain SFH (
). The best-fit χ2red, full are 3.00 and 3.17 for the single-burst and continuous star formation models, respectively. We also list 
when only using wavelength layers around the N V and C IV P Cygni profiles. For each model we also list the intrinsic Hα luminosity in erg s−1.
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