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Table 1.

Our sample of 27 Type IIn SNe.

IAU name RA Dec z Host galaxy AV, MW Surveys tprec (days)
SN 1994ak 09:14:01.47 40:06:21.5 0.0085 NGC 2782 0.044
SN 1999el 20:37:17.72 66:06:11.5 0.0044 NGC 6951 1.020
SN 2002A 07:22:36.14 71:35:41.5 0.0096 UGC 3804 0.071
SN 2002fj 08:40:45.10 –04:07:38.5 0.0147 NGC 2642 0.060
SN 2008fq 20:25:06.20 –24:48:28.0 0.0106 NGC 6907/8 0.174 CHASE
SN 2009au 12:59:46.00 –29:36:07.5 0.00944 ESO 443-21 0.250 CHASE
SN 2010jl 09:42:53.33 09:29:41.8 0.0107 UGC 5189A 0.075 PTF, CHASE
SN 2010jp 06:16:30.63 –21:24:36.3 0.0091 NGC 2207 0.239 CHASE
SN 2011A (1) 13:01:01.19 –14:31:34.8 0.00892 NGC 4902 0.137 CHASE
SN 2011fh 12:56:14.01 –29:29:54.0 0.00803 NGC 4806 0.237 CHASE ≤ − 1235 to 0
SN 2011js 02:48:04.96 –13:57:51.1 0.0139 NGC 1103 0.065 CHASE
PTF11qnf (2) 05:44:54.14 69:09:06.9 0.01428 UGC 3344 0.330 PTF
SN 2013gc 08:07:11.88 –28:03:26.32 0.003406 ESO 430-G20 1.252 PTF, CHASE −1263 to −230
SN 2013ha 06:15:49.85 66:50:19.4 0.0131 LEDA 18729 0.295 PTF
SN 2015bf 23:24:49.03 15:16:52.0 0.01424 NGC 7653 0.183
SN 2015da 13:52:24.11 39:41:28.6 0.00667 NGC 5337 0.040 PTF
ASASSN-15lf 12:06:45.56 67:09:24.0 0.0083 NGC 4108 0.049 PTF
SN 2016aiy 13:08:25.39 –41:58:50.2 0.01 ESO 323-G84 0.354 DES −1070 to −249
SN 2016cvk 22:19:49.39 –40:40:03.2 0.0107 ESO 344-G21 0.035 CHASE, DES −1117 to −319
SN 2016ehw (3) 08:36:37.50 73:35:04.8 0.012 PGC 24209 0.054 PTF
SN 2017gas 20:17:11.35 58:12:09.0 0.01 Anonymous 1.066 PTF, ZTF
SN 2018lkg (4) 07:06:34.89 63:50:55.3 0.0107 UGC 3660 0.131 PTF, ZTF
SN 2019bxq 16:57:58.58 78:36:13.5 0.014 LEDA 84787 0.137 PTF, ZTF −3552 to −18
SN 2019esa 07:55:00.89 –76:24:43.1 0.00589 ESO 035-G18 0.497 DES
SN 2019fmb 12:26:43.68 56:04:32.8 0.016 LEDA 40731 0.044 ZTF −136 to −19
SN 2019njv 20:19:57.2 15:22:38.7 0.01458 Anonymous 0.451 ZTF
SN 2021foa(5) 13:17:12.35 –17:15:25.77 0.008386 IC 863 0.223 PTF, CHASE −20 to −1

Notes. For each object, we report the IAU name, celestial coordinates, redshift, host galaxy, Galactic reddening (from Schlafly & Finkbeiner 2011), surveys from which we collected data and approximate time interval tprec before the explosion between the first and last observation of the precursors or activities. The redshifts are from the classification spectrum of each object. Objects for which we detected one or more eruptive episodes before the explosion are highlighted in bold.

(1)

SN Impostor according to de Jaeger et al. (2015).

(2)

Possibly an Impostor for Nyholm et al. (2017).

(3)

Classification as SN IIn from Pan et al. (2016), Tsvetkov et al. (2020).

(4)

Likely AGN activity or a Tidal Disruption Event, see Appendix A.

(5)

Precursor activity observed by ATLAS.

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