Table 3
Various IMFs taken from the literature as defined in Table 2 of Baldry & Glazebrook (2003).
| Name | 0.1−0.5 | 0.5−1.0 | 1.0−10. | 10.–120 | C |
|
|
|||||
| Kr01 | –0.8 | –1.7 | 0.331 | ||
| S55 | –1.35 | 0.171 | |||
| Sc98 | –0.2 | –1.7 | –1.3 | 0.395 | |
| B03 | –0.5 | –1.2 | 0.323 | ||
|
|
|||||
| SSP mass fraction | |||||
|
|
|||||
| Name | SNII | AGB | 8−3. | 2.6−1.8 | 1.5−0.9 |
|
|
|||||
| Kr01 | 0.363 | 0.630 | 0.233 | 0.111 | 0.187 |
| S55 | 0.337 | 0.655 | 0.235 | 0.117 | 0.202 |
| Sc98 | 0.240 | 0.750 | 0.207 | 0.135 | 0.286 |
| B03 | 0.792 | 0.207 | 0.121 | 0.030 | 0.030 |
Notes. IMFs are normalised between 0.1−100 M⊙. Kr01 is from Kroupa (2001), S55 is Salpeter (1955), Sc98 is from Scalo (1998), B03 is from Baldry & Glazebrook (2003). C is the constant of normalisation between 0.1 and 100 M⊙. The lower section of the table shows the integrated mass fraction of stars involved in SNII, AGB, and the different components of the SNIa.
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