Table 2.
Supernova LC models presented in our study.
| Model name | bare | W12 | W13 | W14 | W15 | W16 | W17 | W5 | W1 | W2 | W3 | W4 | W6 | W9 | W8 | W7 | W10 | W11 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| RCSM[1014 cm] | – | 1.5 | 6 | 10 | ||||||||||||||
| MCSM[M⊙] | – | 0.07 | 0.17 | 0.3 | 0.55 | 0.83 | 1.56 | 0.07 | 0.17 | 0.3 | 0.55 | 0.85 | 1.56 | 0.07 | 0.17 | 0.3 | 0.55 | 0.83 |
| ρin[10−12 g cm−3] | – | 52.6 | 95.5 | 184.3 | 381.0 | 609.8 | 1176.4 | 5.7 | 14.2 | 27.3 | 52.6 | 95.5 | 184.3 | 3.0 | 6.9 | 14.2 | 27.3 | 52.6 |
| Correlation coefficient | – | –0.45 | –0.44 | 0.09 | –0.09 | –0.32 | –0.22 | –0.27 | 0.40 | 0.68 | 0.69 | 0.58 | 0.40 | 0.56 | 0.79 | 0.82 | 0.92 | 0.91 |
Notes. With ‘bare’ we denote the modified progenitor model without any appended CSM, that is, a bare model (for details, see the text). ‘W’ models are those that combine the bare progenitor with an appended CSM (‘W’ stands for ‘wind’). RCSM is the outer radius of the wind-like CSM region, MCSM the CSM mass, and ρin the density at the inner radius of the CSM region. The Spearman correlation coefficients for the g-band LCs, which we discuss in Sect. 3, are listed in the bottom row. The numbering of the models corresponds to the sequence in which they were computed.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.