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Table 1.

Details of the SNe.

Type Host galaxy texp (MJD) Redshift μ (mag) AV (mag)
SN 2017gmr IIP NGC 988 57 999.09 0.005037 31.46 ± 0.15 1.14
SN 2017ahn IIL NGC 3318 57 791.76 0.009255 32.59 ± 0.43 0.82
SN 2013ej IIL M 74 56 496.90 0.002192 29.91 ± 0.16 0.19
SN 2012ec IIP NGC 1084 56 143.00 0.004693 31.10 ± 0.06 0.45
SN 2012dh IIL ESO 443-G80 56 104.98 0.007055 31.85 ± 0.45 0.20
SN 2012aw IIP M 95 56 002.10 0.002595 30.01 ± 0.09 0.23
SN 2010hv II 2MASX J23242536-1902139 55 418.20 ± 8.00 0.024280
SN 2010co II NGC6862 55 310.60 ± 11.50 0.014026
SN 2008bk IIP NGC 7793 54 549.50 0.000767 27.66 ± 0.04 0.07
SN 2007aa IIP NGC 4030 54 126.70 0.004887 32.38 ± 0.20 0.06
SN 2006ov IIP NGC 4303 53 974.00 0.005224 30.5 ± 0.4 0.06
SN 2004dj IIP NGC 2403 53 186.50 0.000445 27.70 ± 0.19 0.22
SN 2001du II NGC 1365 52 145.20 ± 0.50 0.005457
SN 2001dh II ESO 340-G9 52 099.50 ± 13.40 0.008700
SN 1999em IIP NGC 1637 51 475.10 0.002392 30.34 ± 0.24 0.31

Notes. The SN type is based on the light-curve shape (see Paper II). The estimated explosion date is texp (see Sect. 2). The redshifts for the SNe are assumed to be those of their host galaxies, provided by the NED. The references for the distance module are provided in Sect. 2. The Galactic extinction in the V band is AV.

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