Open Access
Table 1.
Pre-SN luminosities of SN II progenitors in the sample analysed in this work.
| SN | log L/L⊙ | Reference |
|---|---|---|
| 2004A | 4.90 ± 0.10 | Davies & Beasor (2018) |
| 2004et | 4.77 ± 0.07 | Davies & Beasor (2018) |
| 2006my | 4.97 ± 0.18 | Davies & Beasor (2018) |
| 2008bk | 4.53 ± 0.07 | Davies & Beasor (2018) |
| 2008cn | 5.10 ± 0.07 | Davies & Beasor (2018) |
| 2009hd | 5.24 ± 0.08 | Davies & Beasor (2018) |
| 2009ib | 5.12 ± 0.14 | Takáts et al. (2015) |
| 2009kr | 5.13 ± 0.23 | Davies & Beasor (2018) |
| 2009md | 4.50 ± 0.20 | Davies & Beasor (2018) |
| 2012A | 4.57 ± 0.09 | Davies & Beasor (2018) |
| 2012aw | 4.92 ± 0.12 | Davies & Beasor (2018) |
| 2012ec | 5.16 ± 0.07 | Davies & Beasor (2018) |
| 2013ej | 4.69 ± 0.07 | Davies & Beasor (2018) |
| 2017eaw | 5.08 ± 0.07 | Van Dyk et al. (2019) |
| 2018zd | 4.50−5.10 | Hiramatsu et al. (2021) |
| 2018aoq | 4.72 ± 0.12 | O’Neill et al. (2019) |
| 2022acko | 4.30−4.50 | Van Dyk et al. (2023) |
| 2023ixf | 4.95 ± 0.07 | Van Dyk et al. (2024) |
| 2024ggi | 4.92 ± 0.05 | Xiang et al. (2024) |
| 2024abfl | 4.32−4.80 | Luo et al. (2025) |
| 2025pht | 5.00 ± 0.09 | Kilpatrick et al. (2025) |
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