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Table 4

Supernovae in the SVISS.

SVISS ID Type (Subtype) Pt(Ps)a log ℒ z M B,peak te (days)b Ext./E(B − V)c

SVISS-SN43 TN(Ia-normal) 0.886(0.733) 4.7 0.43 –19.88 140 –/0.0
SVISS-SN161 TN(Ia-faint) 1.00(0.910) –19.1 0.50 –18.28 –47 –/0.0
SVISS-SN115 TN(Ia-91t) 1.00(1.00) –17.8 0.40 –19.04 1 –/0.0
SVISS-SN116 TN(Ia-faint) 1.00(1.00) 1.1 0.55 –18.98 –6 –/0.0
SVISS-SN309 TN(Ia-faint) 1.00(1.00) –14.8 0.47 –17.96 –77 –/0.0
SVISS-SN402 TN(Ia-faint) 1.00(0.929) 6.1 0.22 –18.66 –127 CZ/0.4
SVISS-SN135 TN(Ia-normal) 0.950(0.580) 9.6 0.98 –18.9 –25 C3/0.2

SVISS-SN14 CC (IIn) 0.623(0.551) 11.2 0.36d –18.64 133 –/0.0
SVISS-SN51 CC (IIP) 1.00 (0.980) 9.0 0.51 –17.56 25 C2/0.6
SVISS-SN54 CC (IIn) 0.812 (0.733) 9.8 0.77 –19.04 72 C2/0.2
SVISS-SN261 CC (Ibc-normal) 0.734 (0.364) 10.1 0.37d –17.48 –110 C2/0.4
SVISS-SN55 CC (IIP) 0.995 (0.854) 3.8 0.83 –17.91 –17 –/0.0
SVISS-SN31 CC (IIL) 0.999 (0.795) 4.4 0.12d –16.52 64 –/0.0
SVISS-SN56 CC (Ibc-bright) 0.930 (0.912) 0.037 0.57 –19.27 –74 C1/0.6
SVISS-SN357 CC (IIn) 1.00 (1.00) 6.0 1.4 –19.08 –91 –/0.0
SVISS-SN24 CC (Ibc-bright) 0.643 (0.643) 7.2 0.81 –19.56 25 C2/0.5

Notes. 

(a)

Pt refers to the co-added probability for the best-fitting main type (TN/CC), Ps refers to the subtype probability from the typing code.

(b)

This is the time since explosion in the observers frame.

(c)

Extinction models are as follows: C3, Cardelli with RV = 3.1; C2, Cardelli with RV = 2.1; CZ, Calzetti. For the SNe with a most likely extinction of zero, no best-fit model is given.

(d)

“Hostless” SNe, for these a flat redshift prior was used, see text for details.

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