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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