Table A.1.
Sample of SE SNe used in this work.
| SN | Type | Host | Host redshift( + ) | Host dL ( † ) | MW E(B − V) | Host E(B − V)( * ) | t0 | References |
|---|---|---|---|---|---|---|---|---|
| SN1993J | IIb | M81 | -0.00011 | 3.63 | 0.07 | 0.10 | 49073.50 | (a) |
| SN2004ex | IIb | NGC0182 | 0.01755 | 70.60 | 0.02 | 0.08 | 53287.90 | (CSP) |
| SN2004ff | IIb | ESO-552-G040 | 0.0226 | 92.70 | 0.03 | 0.10 | 53297.66 | (CSP) |
| SN2004gq | Ib | NGC1832 | 0.006468 | 25.10 | 0.06 | 0.08 | 53346.87 | (CSP),(Cfa) |
| SN2004gv | Ib | NGC0856 | 0.019973 | 79.60 | 0.03 | 0.03 | 53345.27 | (CSP) |
| SN2005aw | Ic | IC4837A | 0.009498 | 41.50 | 0.05 | 0.21 | 53445.67 | (CSP) |
| SN2005em | Ic | IC0307 | 0.025981 | 105.00 | 0.08 | 0.00 | 53635.00 | (CSP) |
| SN2005hg | Ib | UGC1394 | 0.02131 | 86.00 | 0.09 | None | 53665.75 | (CSP) |
| SN2005kl | Ic | NGC4369 | 0.003485 | 21.57 | 0.02 | None | 53686.14 | (Cfa) |
| SN2005mf | Ic | UGC4798 | 0.02676 | 113.00 | 0.01 | None | 53723.33 | (Cfa) |
| SN2006aj | Ic-GRB | A032139+1652 | 0.033 | 132.40 | 0.13 | 0.00 | 53784.15 | (Cfa),(b) |
| SN2006ba | IIb | NGC2980 | 0.01908 | 82.70 | 0.04 | 0.10 | 53801.11 | (Cfa),(CSP) |
| SN2006ep | Ib | NGC0214 | 0.015134 | 61.90 | 0.03 | None | 53975.49 | (Cfa),(CSP) |
| SN2006fo | Ib | UGC02019 | 0.020698 | 82.70 | 0.02 | 0.21 | 53983.36 | (Cfa),(CSP) |
| SN2006lc | Ib | NGC7364 | 0.016228 | 59.20 | 0.06 | 0.36 | 54014.74 | (Cfa),(CSP) |
| SN2006T | IIb | NGC3054 | 0.008091 | 31.60 | 0.06 | 0.14 | 53757.64 | (Cfa),(CSP) |
| SN2007C | Ib | NGC4981 | 0.005604 | 21.00 | 0.04 | 0.43 | 54095.44 | (Cfa),(CSP) |
| SN2007gr | Ic | NGC1058 | 0.0017 | 9.29 | 0.09 | 0.03 | 54325.00 | (Cfa),(c) |
| SN2007kj | Ib | NGC7803 | 0.017899 | 72.50 | 0.07 | 0.00 | 54363.61 | (Cfa),(CSP) |
| SN2007uy | Ib | NGC2770 | 0.0065 | 31.33 | 0.02 | 0.63 | 54462.33 | (Cfa),(d) |
| SN2007Y | Ib | NGC1187 | 0.004637 | 18.40 | 0.02 | 0.00 | 54145.00 | (CSP),(e) |
| SN2008aq | IIb | MCG-02-33-020 | 0.007972 | 26.90 | 0.04 | 0.00 | 54510.79 | (Cfa),(CSP) |
| SN2008ax | IIb | NGC4490 | 0.0019 | 9.20 | 0.02 | 0.28 | 54528.30 | (Cfa),(f) |
| SN2008D | Ib | NGC2770 | 0.0065 | 31.33 | 0.02 | 0.63 | 54474.50 | (Cfa),(g) |
| SN2008hh | Ic | IC0112 | 0.01941 | 77.70 | 0.04 | 0.00 | 54780.69 | (Cfa),(CSP) |
| SN2009bb | Ic-BL | NGC3278 | 0.00988 | 39.80 | 0.09 | 0.48 | 54909.10 | (CSP),(h) |
| SN2009iz | Ib | UGC02175 | 0.01419 | 58.60 | 0.07 | None | 55083.00 | (Cfa) |
| SN2009jf | Ib | NGC7479 | 0.0079 | 33.73 | 0.10 | 0.05 | 55099.00 | (Cfa),(i) |
| SN2009K | IIb | NGC1620 | 0.011715 | 44.10 | 0.05 | 0.06 | 54843.57 | (Cfa),(CSP) |
| SN2010as | IIb | NGC6000 | 0.0073 | 27.16 | 0.15 | 0.42 | 55270.75 | (j) |
| SN2010bh | Ic-GRB | A071031-5615 | 0.059 | 244.34 | 0.10 | 0.14 | 55271.53 | (k) |
| SN2011fu | IIb | UGC1626 | 0.019 | 74.47 | 0.07 | 0.01 | 55824.00 | (l) |
| SN2011dh | IIb | M51 | 0.002 | 7.87 | 0.03 | 0.05 | 55712.50 | (m) |
| SN2011hs | IIb | IC5267 | 0.0057 | 24.10 | 0.01 | 0.16 | 55871.50 | (n) |
| SN2013df | IIb | NGC4414 | 0.0024 | 21.37 | 0.02 | 0.08 | 56447.30 | (o) |
| SN2016coi | Ic-BL | UGC11868 | 0.00364 | 17.20 | 0.07 | 0.12 | 57532.50 | (p) |
| SN2017czd | IIb | UGC9567 | 0.00835 | 32.00 | 0.02 | 0.00 | 57845.00 | (q) |
Notes. Selection criteria for this sample is described in Sect. 2. ( + ): Heliocentric redshift. ( † ): Luminosity distance, in Mpc. ( * ): If no published value is found, we quote “None”. Zero values are consistent with no host reddening, as published in the proper references. (CSP): Taddia et al. (2018), (Cfa): Bianco et al. (2014), (a): Richmond et al. (1994), (b): Mirabal et al. (2006), (c): Hunter et al. (2009), (d): Roy et al. (2013), (e): Stritzinger et al. (2009), (f): Pastorello (2008), (g): Mazzali et al. (2008), Tanaka et al. (2009) (h): Pignata et al. (2011), (i): Valenti et al. (2011), (j): Foley et al. (2014), (k): Cano et al. (2011), Olivares et al. (2012), (l): Morales-Garoffolo et al. (2015), (m): Arcavi et al. (2011), Sahu et al. (2013), Ergon et al. (2015), (n): Bufano et al. (2014), (o): Van Dyk et al. (2014), (p): Yamanaka et al. (2017), Prentice et al. (2018), (q): Nakaoka et al. (2019).
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