Table 4.
Type II SN comparison sample.
| SN | Host | Explosion | Redshift | Distance | E(B − V)host | References |
|---|---|---|---|---|---|---|
| galaxy | Epoch (MJD) | modulus (mag) | (mag) | |||
| 2013by | ESO138-G010 | 56401.6 ± 3.6 | 0.00382 | 30.46 ± 0.29 | – | 1 |
| 2013fs | NGC 7610 | 56570.8 ± 0.5 | 0.01185 | 33.32 ± 0.18 | – | 4, 5 |
| 2014G | NGC 3448 | 56669.3 ± 0.8 | 0.00450 | 31.96 ± 0.14 | 0.268 ± 0.046 | 2, 3 |
| 2015bf | NGC 7653 | 57367.3 |
0.013654 | 33.89 ± 0.05 | 0.148 | 6 |
| 2017ahn | NGC 3318 | 57791.8 ± 0.5 | 0.00925 | 32.84 ± 0.10 | 0.233 ± 0.148 | 7 |
| 2018zd | NGC 2146 | 58178.4 |
0.002979 | 31.32 ± 0.53 | 0.17 ± 0.05 | 8, 9, 10 |
| 2020pni | UGC 09684 | 59045.8 ± 0.1 | 0.01665 | 34.34 ± 0.15 | 0.080 ± 0.010 | 11 |
| 2023ixf | M101 | 60082.7 ± 0.01 | 0.000804 | 29.19 ± 0.04 | 0.038 ± 0.009 | 12, 13, 14, 15, 16, 17 |
| 2019nyk | HIPASS J0015-08 | 58713.9 ± 2.0 | 0.02100 | 34.88 ± 0.17 | – | This work |
References. [1] Valenti et al. (2015), [2] Bose et al. (2016), [3] Terreran et al. (2016), [4] Yaron et al. (2017), [5] Bullivant et al. (2018), [6] Lin et al. (2021), [7] Tartaglia et al. (2021), [8] Zhang et al. (2020), [9] Hiramatsu et al. (2021), [10] Callis et al. (2021), [11] Terreran et al. (2022), [12] Jencson et al. (2023), [13] Jacobson-Galán et al. (2023), [14] Hosseinzadeh et al. (2023), [15] Bostroem et al. (2023), [16] Teja et al. (2023), [17] Hiramatsu et al. (2023).
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