Table 5.
Sample of LRNe shown in Fig. 13.
| Object | Distance | E(B − V) | Filter | Mpeak | tplateau | FWHM | Progenitor mass | References |
|---|---|---|---|---|---|---|---|---|
| (pc) | (mag) | (mag) | (days) | (km s−1) | (M⊙) | |||
| V1309Sco | (2.10±0.70)×103 | 0.550 | V | –5.82±0.92 | 27±5 | 150±15 | 1.5 |
[1] [2] [3] |
| V4332Sgr | (5.00±1.00)×103 | 0.320 | V | –3.70±0.44 | 13±10 | 200±20 | 1.0 |
[4] [3] |
| V838Mon | (5.90±0.40)×103 | 0.850 | R | –9.80±0.15 | 76±7 | 500±50 | 7.5 |
[5] [6] [7] [8] |
| M31-LRN2015 | (0.76±0.02)×106 | 0.120 | R | –9.60±0.20 | 41±4 | 300±20 | 4.0 |
[9] [10] [11] |
| AT2019zhd | (0.76±0.02)×106 | 0.055 | r | –9.61±0.08 | 26±3 | 280±30 | – | [12] |
| AT2020hat | (5.16±0.21)×106 | 0.090 | r | –11.01±0.10 | 100±20 | 250±30 | – | [13] |
| M101-OT2015-1 | (6.43±0.20)×106 | 0.008 | R | –12.40±0.50 | 230±10 | 500±50 | 18.0 |
[14] |
| AT2018bwo | (6.64±0.10)×106 | 0.029 | r | –10.91±0.03 | 41±5 | 500±65 | 13.0 |
[15] |
| SN1997bs* | (9.20±0.60)×106 | 0.210 | R | –13.65±0.14 | 140±40 | 850±150 | – | [16] [17] |
| NGC4490-2011OT1 | (9.60±1.40)×106 | 0.320 | R | –14.40±0.29 | 210±10 | 800±100 | 30.0 |
[18] [17] |
| NGC3437-2011OT1* | (20.90±4.60)×106 | 0.020 | R | –13.85±0.43 | 147±15 | 700±70 | – | [17] |
| AT2018hso | (21.30±0.56)×106 | 0.300 | r | –13.93±0.06 | 210±20 | 500±50 | – | [19] |
| AT2014ej* | (22.10±1.50)×106 | 0.310 | r | –15.09±0.48 | 83±20 | 900±80 | – | [20] |
| AT2020kog | (22.50±2.00)×106 | 0.370 | r | –13.20±0.50 | 120±30 | 470±50 | – | [13] |
| SNHunt248* | (22.50±4.00)×106 | 0.040 | R | –15.06±0.36 | 154±15 | 1200±100 | 60.0 |
[21] [22] |
| AT2017jfs | (35.70±2.70)×106 | 0.022 | r | –15.60±0.17 | 176±5 | 700±70 | – | [23] |
| UGC12307-2013OT1 | (39.70±2.80)×106 | 0.220 | R | –15.00±0.15 | 148±72 | 900±100 | – | [17] |
Notes. Magnitudes in V and R filters are reported in the Vega magnitude system. Magnitudes in the r filter are reported in the AB system. The sign * indicates LRN candidates.
References. [1]: Mason et al. (2010), [2]: Tylenda et al. (2011), [3]: Kamiński et al. (2018), [4]: Martini et al. (1999), [5]: Munari et al. (2002), [6]: Ortiz-León et al. (2020), [7]: Kimeswenger et al. (2002), [8]: Afşar & Bond (2007), [9]: Williams et al. (2015), [10]: Kurtenkov et al. (2015), [11]: MacLeod et al. (2017), [12]: Pastorello et al. (2021a), [13]: Pastorello et al. (2021b), [14]: Blagorodnova et al. (2017), [15]: This work, [16]: Van Dyk et al. (2000), [17]: Pastorello et al. (2019b), [18]: Smith et al. (2016), [19]: Cai et al. (2019), [20]: Stritzinger et al. (2020), [21]: Kankare et al. (2015), [22]: Mauerhan et al. (2015), [23]: Pastorello et al. (2019a).
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