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Table C.1.

SN II sample taken from Anderson (2019).

SN Host Host dL ( † ) Nickel mass (§) Host References( ⋆ )
SN1969L N1058 5.2 0.075 0.015 H03, E03
SN1970G N5457 6.6 0.044 0.185 H03, E03
SN1973R N3627 9.6 0.084 1.400 H03
SN1980K N6946 5.5 0.006 0.000 PP15
SN1986I N4254 15.2 0.117 0.200 H03
SN1986L N1559 14.9 0.040 0.157 H03, G17, N03
SN1987A LMC 0.05 0.072 0.135 Arnett et al. (1989), (a), (b), N03
SN1988A N4579 18.4 0.077 0.033 H03, N03, E03
SN1989L N7339 22.0 0.015 0.150 H03
SN1990E N1035 17.4 0.056 0.930 V16, H03, N03, E03
SN1990K N150 19.3 0.039 0.200 H03
SN1991al P140858 64.2 0.058 0.097 H03, G17, N03
SN1991G N4088 13.9 0.022 0.000 H03
SN1992af E-340-G038 64.4 0.158 0.010 H03, G17, N03
SN1992am M-01-04-039 165.0 0.308 0.305 H03, N03
SN1992ba N2082 18.3 0.024 0.115 M17, H03, G17, N03
SN1992H N5377 26.2 0.177 0.003 PP15, H03, E03
SN1994N U5695 45.3 0.006 0.000 (c), (d)
SN1995ad N2139 27.1 0.060 0.575 PP15, (e)
SN1996W N4027 12.2 0.128 0.895 PP15, (e)
SN1997D N1536 13.4 0.006 0.002 (c), (d), E03, (f), (g)
SN1998A IC2627 9.0 0.110 0.000 (b), Pastorello (2005)
SN1999br N4900 21.5 0.002 0.163 (c), (d), H03, G17
SN1999ca N3120 30.3 0.043 0.470 H03, G17
SN1999cr E-576-G034 78.1 0.088 0.025 H03, N03
SN1999em N1637 11.5 0.044 0.169 V16, PP15, H03, G17, (h), (i), N03, E03
SN1999eu N1097 17.2 0.001 0.000 (c)
SN1999ga N2442 21.0 0.013 0.430 Pastorello (2009)
SN1999gi N3184 12.3 0.025 0.618 V16, H03, N03, E03
SN2000cb IC1158 31.9 0.092 0.310 (a), (b)
SN2001dc N5777 44.3 0.005 1.537 PP15, (c), (d)
SN2001X N5921 17.4 0.055 0.220 V16
SN2002fa GALEX..(*) 268.5 0.066 0.000 G17
SN2002gw N0922 42.6 0.028 0.150 M17, G17
SN2002hh N6946 5.5 0.085 3.750 V16, PP15, (h)
SN2002hj P3092113 95.5 0.026 0.000 G17
SN2002hx P023727 124.3 0.053 0.000 G17
SN2003B N1097 17.2 0.020 0.090 M17, G17
SN2003bn P831618 58.2 0.035 0.085 M17, G17
SN2003cx NEAT..(+) 174.3 0.051 0.000 G17
SN2003E E-485-G004 57.1 0.083 0.640 M17
SN2003ef N4708 63.1 0.091 0.990 M17
SN2003fb U11522 72.4 0.033 0.655 M17, G17
SN2003gd N0628 7.5 0.012 0.413 G17, (h), Hendry (2005)
SN2003hd E-543-G017 144.8 0.032 0.147 M17, V16, G17
SN2003hk N1085 85.3 0.017 0.000 G17
SN2003hn N1448 16.4 0.031 0.523 M17, V16, G17, V15
SN2003ho E-235-G058 59.4 0.009 1.115 M17, G17
SN2003T U4864 104.8 0.030 0.325 M17, G17
SN2003Z N2742 22.5 0.005 0.000 V16, (c)
SN2004A N6207 17.0 0.040 0.230 PP15, Gurugubelli et al. (2008)
SN2004dj N2403 3.4 0.018 0.080 PP15, Vinkó et al. (2006)
SN2004eg U3053 31.9 0.007 0.000 (c)
SN2004ej N3095 32.7 0.019 0.140 G17
SN2004et N6946 5.5 0.048 0.255 V16, PP15, (c), (h)
SN2004fx M-02-14-03 34.0 0.014 0.000 G17
SN2005af N4945 4.2 0.026 0.000 G17
SN2005cs N5194 7.5 0.004 0.200 V16, PP15, (c), (h), Pastorello (2009)
SN2005dx M-03-11-09 124.8 0.007 0.000 G17
SN2005dz U12717 87.5 0.021 0.000 G17
SN2006ai E-5-G9 59.3 0.050 0.000 G17
SN2006au U11057 112.3 0.073 0.440 (b)
SN2006bc N2397 22.0 0.027 1.050 (h)
SN2006bp N3953 16.6 0.002 1.210 PP15
SN2006ms N6935 52.2 0.056 0.000 G17
SN2006ov N4303 14.6 0.002 0.000 (c)
SN2006V U6510 70.0 0.127 0.000 (b)
SN2006Y A071317-5141 146.3 0.034 0.000 G17
SN2007ab M-01-43-02 101.2 0.040 0.000 G17
SN2007av N3279 35.4 0.015 0.000 G17
SN2007hm A205755-0723 144.3 0.045 0.000 G17
SN2007it N5530 12.2 0.078 0.020 V16, G17, Andrews (2011)
SN2007od U12846 27.3 0.007 0.115 V16, PP15
SN2008aw N4939 36.4 0.050 0.320 G17
SN2008bk N7793 3.8 0.010 0.073 PP15, (c), G17, Lisakov et al. (2017)
SN2008bm P45053 135.3 0.014 0.000 G17, Rodríguez et al. (2020)
SN2008br IC2522 35.3 0.026 0.000 G17
SN2008bu E-586-G2 71.5 0.020 0.000 G17
SN2008in N4303 14.6 0.016 0.253 V16, PP15, (c), Roy et al. (2011b)
SN2008if P26411 54.8 0.063 0.210 G17
SN2008gz N3672 24.9 0.050 0.100 Roy et al. (2011a)
SN2008K E-504-G5 116.0 0.013 0.000 G17
SN2008M E-121-G26 40.0 0.020 0.000 G17
SN2009E N4141 40.8 0.040 0.030 (b), Pastorello (2012)
SN2009bw U2890 13.6 0.019 0.480 V16, PP15
SN2009dd N4088 13.9 0.031 1.127 V16, PP15, (e)
SN2009ib N1559 14.9 0.058 0.427 M17, V16, Takáts et al. (2015)
SN2009js N918 19.1 0.064 0.500 PP15
SN2009kr N1832 24.4 0.009 0.015 V16, V15
SN2009N N4487 17.2 0.022 0.405 V16, PP15, (c), Takáts et al. (2014)
SN2009md N3389 22.0 0.004 0.275 V16, (c)
SN2012A N3239 9.7 0.010 0.033 V16, PP15, V15
SN2012aw N3351 9.9 0.058 0.223 V16, PP15, V15, Bose et al. (2013)
SN2012ec N1084 19.1 0.035 0.370 M17, V16, (j), (k)
SN2013K E-9-G10 34.3 0.012 0.310 Tomasella et al. (2018)
SN2013ab N5669 19.4 0.061 0.120 M17, V16
SN2013am N3623 12.2 0.015 1.930 Tomasella et al. (2018)
SN2013bu N7331 13.4 0.002 0.000 V16
SN2013by E-138-G10 14.7 0.031 0.000 V16, V15
SN2013ej N628 7.5 0.018 0.070 M17, V16, (l), (m), (n), (o), V15
SN2013fs N7610 38.7 0.070 0.155 M17, V16
LSQ13dpa LCSB-S1492O 115.8 0.070 0.000 V16
SN2014cy N7742 25.8 0.004 0.000 V16
SN2014dw N3568 25.1 0.009 0.340 V16
SN2014G N3448 23.8 0.037 0.455 M17, V16, V15, Terreran et al. (2016)
ASASSN-14dq U11860 61.9 0.046 0.000 V16
ASASSN-14gm N337 19.4 0.076 0.000 M17, V16
ASASSN-14ha N1556 10.0 0.005 0.000 M17, V16
SN2015ba U3777 46.3 0.032 0.090 Dastidar et al. (2018)
SN2015bs Anon 110.8 0.049 0.000 Anderson et al. (2018)
SN2015W U3617 56.6 0.031 0.000 V16
SN2016X U8041 15.3 0.034 0.050 Huang et al. (2018)
SN2016bkv N3184 12.3 0.022 0.000 Hosseinzadeh et al. (2018)
SN2016ija N1532 17.9 0.208 6.050 Tartaglia et al. (2018)
SN2017eaw N6946 5.5 0.050 0.000 Tsvetkov et al. (2018)

Notes. The table lists SN names, SN host galaxies, host galaxy luminosity distances and host galaxy extinction values. References for nickel masses and host galaxy extinction values are listed in the last column. ( * ): GALEXASCJ205221.54+020843.8; ( + ): NEATJ135706.53-170220.0. Host galaxies names have been shortened according to NGC:N, UGC:U, PGC:P, ESO:E, MCG:M. ( † ): All host luminosity distances, in Mpc, are taken from NED. (§): All nickel masses are the mean of the individual measurements given in the references. (¶): The host reddening is also the mean of the values given in these references. Using the nickel mass and extinction from this table the results of Sect. 4.2.3 can be accurately reproduced. ( ⋆ ): H03 : Hamuy (2003), E03: Elmhamdi et al. (2003), N03: Nadyozhin (2003), PP15: Pejcha & Prieto (2015), V15: Valenti et al. (2015), V16: Valenti et al. (2016), G17: Gutiérrez et al. (2017), M17: Müller et al. (2017), (a): Kleiser et al. (2011), (b): Taddia et al. (2012), (c): Spiro et al. (2014), (d): Pastorello (2004), (e): Inserra (2013), (f): Zampieri et al. (2003), (g): Turatto et al. (1998), (h): Otsuka et al. (2012), (i): Bersten et al. (2011), (j): Jerkstrand et al. (2015), (k): Barbarino (2015), (l): Yuan et al. (2016), (m): Dhungana et al. (2016), (n): Huang et al. (2015), (o): Bose et al. (2015).

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