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Table 3
Optimized range of SFR parameters for each galaxy spectral type.
| Early-type galaxies | |
|
|
|
| p1 | 10–2000 (Myr) |
| p2 | 0.5–1.5 (M⊙) |
|
|
|
| Spiral galaxies | |
| p1 | 0.3–2.4 |
| p2 | 5–5000 (Myr/M⊙) |
| tinfall | 5–16 000 (Myr) |
|
|
|
| Irregular galaxies | |
| p1 | 0.6–3.9 |
| p2 | 4000–40 000 (Myr/M⊙) |
| tinfall | 5000–20 000 (Myr) |
|
|
|
| QSFG | |
| p1 | 0.6–3.9 |
| p2 | 4000–40 000 (Myr/M⊙) |
| p3 | 1–10 (Myr) |
| tinfall | 5000–20 000 (Myr) |
Notes. The p1, p2 parameters correspond to the adopted SFL respectively.
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