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Table 5.

Number of recovered signals for each SN type in our sample.

Type No. Tails Siblings Nuclear CSM




No. % No. % No. %
Ia 4991 18 0.4 6 (a) 0.1 7 0.1 3 0.1
II 1311 19 1.4 4 (b) 0.3 0 0 0 0
Ib/c 339 3 0.9 0 0 0 0 0 0
IIn 279 8 2.9 0 0 0 0 0 0
I 58 2 3.4 0 0 0 0 0 0
Ibn 17 0 0 0 0 0 0 0 0

Notes. As it is unclear whether SN 2016cob and SN2017fby should be counted as nuclear transients or due to CSM interaction, they have been counted in both.

(a)

This includes the unconfirmed but likely sibling at the position of SN 2017ige determined from our binned light curve analysis.

(b)

This includes one sibling pair (SN 2009hz/AT 2018iml) where the ZTF transient was a likely CV based on its light curve.

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