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Table 4
Estimated minimum mass of CC SN progenitors in different galaxy samples derived considering a control time of 13 years and different assumptions about the number of CC SNe discovered in the last 13 years, the maximum mass for progenitors of CC SNe with optical signature, the IMF and the distance scale.
| Sample |
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| dubious SNe |
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Kroupa IMF | distance | |
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| A | 5.3 ± 0.9 | 5.4 ± 0.9 | 5.8 ± 1.2 | 6.3 ± 1.3 |
| B | 7.4 ± 1.5 | 7.3 ± 1.3 | 8.4 ± 1.8 | 9.0 ± 1.9 |
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