Table 3
Parameter space used for constructing stellar templates used in our SED fitting.
| Range | Nr. steps | |
|
|
||
| Age | 0.01 Myr–2.3 Gyr | 50 |
| E(B−V) | 0–1.5 | 20 |
| Z | 0.0004–0.02 (Z⊙) | 4 |
| τ | 0.001 Gyr–5 Gyr | 5 |
Notes. The stepsizes are logarithmic distributed for the ages, while we use an irregular spacing for the stepsizes of E(B−V) where we finely sample the low values, and use larger steps for the higher values. The metallicities correspond to the m32, m42, m52 and m62 models of BC03.
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