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Table 2.
Parameters in SED fitting.
| SFH, delayed | |
|---|---|
| τ | 50, 100, 500, 1000, 2000.0, 5000, 10 000 |
| Age | 10, 50, 100, 500, 1000, 2000 |
| Stellar population, Bruzual & Charlot (2003) | |
| IMF | Salpeter (1955) |
| Metallicity | 0.0004, 0.004, 0.02 (Z⊙ = 0.02) |
| Nebular, Inoue (2011) | |
| fesc | 0.2 |
| logU | −2.5 |
| Dust attenuation, modified C00 | |
| E(B − V)lines | 0.05, 0.1, 0.15, 0.2, 0.25, 0.3, 0.4, 0.5, 0.6, 0.7, 0.8, 0.9, 1.0, |
| 1.1, 1.2, 1.3, 1.4, 1.5 | |
| δ | −0.5, −0.4, −0.3, −0.2, −0.1, 0.0, 0.1, 0.2, 0.3, 0.4 |
| febv | 0.1, 0.2, 0.3, 0.4, 0.5, 0.6, 0.7, 0.8, 0.9, 1.0 |
| Line emission extinction | MW extinction law for lines, Rv = 3.1 |
| Dust emission, Dale et al. (2014) | |
| α | 2.0 |
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