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Table 1
Stellar initial mass functions used in BPASS v2.2 (above line) and the extended parameter grid explored in this work.
| M0 / M⊙ | αl | Ml | αm | Mm / M⊙ | αu | Mu / M⊙ |
|---|---|---|---|---|---|---|
| 0.1 | −1.30 | 0.5 | – | – | −2.00 | [100, 300] |
| 0.1 | −1.30 | 0.5 | – | – | −2.35 | [100, 300] |
| 0.1 | −1.30 | 0.5 | – | – | −2.70 | [100, 300] |
| 0.1 | −2.35 | 0.5 | – | – | −2.35 | 100 |
| 0.1 | C03 | 1.0 | – | – | −2.30 | [100, 300] |
| 0.1 | −1.30 | 0.5 | – | – | −2.35 | [150, 200, 250] |
| 0.1 | −1.30 | 0.5 | – | – | [−1.8,−1.9,...−2.6, −2.7] | [100, 150, 200, 300] |
| 0.1 | −1.30 | 0.5 | −2.35 | [1,5,10,15,20,30,50] | −2.00 | [100, 150, 200, 300] M⊙ |
| 0.1 | −1.30 | 0.5 | – | – | −2.35 | 300 M⊙ with prob. cut-off |
| for Mtot = [1,3,7] × [102,3,4,5,6,7,8] M⊙ | ||||||
Notes. “C03” indicates an exponential cut-off of the form proposed by Chabrier (2003). The total starburst mass dependent probability cut-off in the final model grid is explained in Sect. 5.
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