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Table 1
Supernovae in the SVISS.
| SVISS ID | Type | P(type) | z | |
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| SVISS-SN43 | Ia | 0.886 | 0.43 | |
| SVISS-SN161 | Ia | 1.000 | 0.50 | |
| SVISS-SN115 | Ia | 1.000 | 0.40 | |
| SVISS-SN116 | Ia | 1.000 | 0.55 | |
| SVISS-SN309 | Ia | 1.000 | 0.47 | |
| SVISS-SN402 | Ia | 1.000 | 0.22 | |
| SVISS-SN135 | Ia | 0.950 | 0.98 | |
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| SVISS-SN14 | CC | 0.623 | 0.36 | |
| SVISS-SN51 | CC | 1.000 | 0.51 | |
| SVISS-SN54 | CC | 0.812 | 0.77 | |
| SVISS-SN261 | CC | 0.734 | 0.37 | |
| SVISS-SN55 | CC | 0.995 | 0.83 | |
| SVISS-SN31 | CC | 0.999 | 0.12 | |
| SVISS-SN56 | CC | 0.930 | 0.57 | |
| SVISS-SN357 | CC | 1.000 | 1.40 | |
| SVISS-SN24 | CC | 0.643 | 0.81 | |
Notes. P(type) is the probability (Bayesian evidence) for the best fitting main type (TN/CC).
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