Table 3.
Properties of the three selected SED-fitting solutions (see text) and their predicted line luminosities.
| High Z | Low Z | Young | |
|---|---|---|---|
 |
4.04 | 3.90 | 3.95 |
| Z | 0.02 | 0.0004 | 0.0001 |
| Age (Gyr) | 0.29 | 0.29 | 0.002 |
| SFR (M⊙ yr−1) | 10 | 8.4 | 77 |
| M⋆ (109 M⊙) | 2.1 | 1.7 | 0.16 |
| AV (mag.) | 0.0 | 0.0 | 0.0 |
| [O II] λ3727 | 1.1 × 10−18 | 1.5 × 10−19 | 1.7 × 10−19 |
| Hβ | 9.4 × 10−19 | 1.3 × 10−18 | 6.3 × 10−18 |
| [O III] λ5007 | 2.9 × 10−18 | 1.4 × 10−18 | 1.9 × 10−18 |
| Hα | 2.8 × 10−18 | 3.6 × 10−18 | 1.8 × 10−17 |
| [O III]/[O II] | 2.6 | 9.3 | 11 |
| [O III]/Hβ | 3.1 | 1.1 | 0.30 |
Notes. The table shows the reduced chi-square (
), the absolute metallicity (Z), the Age, SFR, stellar mass (M⋆), dust extinction (AV) along with predicted line fluxes (in units of erg s−1 cm−2) and line ratios (
and O III λ5007/Hβ).
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