ZTF SN Ia DR2
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Table 6.

Parameters used for rate estimation simulations for each object.

Object Start epoch Duration Strength Nsample Late-time CSM Late-time CSM
(d) (d) (SN 2015cp) fraction rate (Gpc−3 yr−1)
SN 2018grt (worst) 1375 ( * ) 100 60 748 0 . 0084 0.0041 + 0.0183 $ 0.0084_{-0.0041}^{+0.0183} $ 203 97 + 438 $ 203_{-97}^{+438} $
SN 2018grt (best) 1275 ( * ) 200 100 988 0 . 0015 0.0007 + 0.0032 $ 0.0015_{-0.0007}^{+0.0032} $ 36 18 + 76 $ 36_{-18}^{+76} $
SN 2019ldf (worst) 1050 ( * ) 200 60 1931 0 . 0019 0.0009 + 0.0036 $ 0.0019_{-0.0009}^{+0.0036} $ 45 22 + 87 $ 45_{-22}^{+87} $
SN 2019ldf (best) 875 ( * ) 500 60 2505 0 . 0023 0.0011 + 0.0038 $ 0.0023_{-0.0011}^{+0.0038} $ 54 26 + 91 $ 54_{-26}^{+91} $
SN 2020tfc (worst) 550 250 100 3439 0 . 0004 0.0002 + 0.0009 $ 0.0004_{-0.0002}^{+0.0009} $ 10 5 + 22 $ 10_{-5}^{+22} $
SN 2020tfc (best) 450 500 150 3493 0 . 0003 0.0002 + 0.0008 $ 0.0003_{-0.0002}^{+0.0008} $ 8 4 + 20 $ 8_{-4}^{+20} $

Notes. For each of the three SNe we assumed a worst and best case scenario for detecting them in our sample, giving upper and lower limits for a simulated observing campaign. The efficiency curves generated from these simulations were then used to determine the intrinsic fraction of SNe Ia with late-time CSM interaction in an MCMC process, with the assumption that only one object was recovered in a sample size that is the same as the amount of DR2 objects with observations after the start epoch (Nsample). The last two columns show the found late-time CSM interaction fraction of the total SN Ia rate and the late-time CSM interaction rate.

( * )When the start epoch of the late-time excess is > 750 d, 750 d is used as the start epoch because of limitations of the available ZTF survey plan. See Sect. 4.3 for more details.

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