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Table 2
SSP settings for BPASS and SB99 SED modelling.
| M* | IMF exponent (a) | IMF exponent (b) | M* range |
|---|---|---|---|
| (M⊙) | (0.1–0.5 M⊙) | (0.5–300 M⊙) | (M⊙) |
| 106 | −1.30 | −2.35 | 0.1–300 |
Notes. The two IMF exponents are valid in the reported range of masses. An IMF constructed with these exponents exhibits behaviour similar to a Chabrier one (Kennicutt & Evans 2012). The first column, M* , is the mass of stars formed in each starburst.
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