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Table 4.

Progenitor initial masses from non-rotating and DBR models for each SN II in the sample.

SN Progenitor initial mass (M)

Non-rotating models DBR models
16th 50th 84th 16th 50th 84th
2004A 12.1 13.4 15.0 11.5 12.8 14.5
2004et 10.8 11.7 12.6 10.5 11.3 12.2
2006my 12.0 14.6 18.0 11.5 13.7 16.8
2008bk 9.0 9.1 9.7 9.0 9.0 9.7
2008cn 15.4 16.7 18.5 14.5 16.0 17.5
2009hd 18.2 19.7 21.3 16.5 18.6 21.2
2009ib 14.6 17.1 20.1 13.8 16.3 19.4
2009kr 13.5 17.4 22.3 12.6 16.5 21.5
2009md 9.0 9.0 10.8 9.0 9.0 10.5
2012A 9.0 9.5 10.4 9.0 9.0 10.5
2012aw 12.1 13.7 15.6 11.5 13.2 15.1
2012ec 16.5 18.2 19.6 15.4 17.2 18.7
2013ej 9.9 10.7 11.5 9.7 10.5 11.4
2017eaw 15.2 16.3 18.1 14.2 15.5 17.3
2018zd 10.8 12.1 13.4 10.5 11.5 12.9
2018aoq 9.8 11.0 12.6 9.4 10.6 12.2
2022acko 9.0 9.0 9.0 9.0 9.0 9.0
2023ixf 13.2 14.2 15.3 12.5 13.5 14.6
2024ggi 13.0 13.7 14.5 12.3 13.2 14.0
2024abfl 9.0 9.4 10.1 9.0 9.0 10.2
2025pht 13.6 15.0 16.5 12.8 14.3 15.8

Notes. The results are given as the 16th, 50th, and 84th percentiles of the posterior distribution.

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