Taddia, F.F.Taddia0000-0002-7259-4624Sollerman, J.J.SollermanFremling, C.C.FremlingPASTORELLO, AndreaAndreaPASTORELLOLeloudas, G.G.LeloudasFransson, C.C.FranssonNyholm, A.A.NyholmStritzinger, M. D.M. D.StritzingerErgon, M.M.ErgonRoy, R.R.RoyMigotto, K.K.Migotto2020-04-212020-04-212015http://hdl.handle.net/20.500.12386/24151In Table 1 we report the list of 60 transients included in our sample. Thirty-five of them are SNe IIn, six are SNe Ibn, one is a SN Ia-CSM, 18 are SN IMs (if we also count SN 2009ip in the SN IMs, then we have 19 of these transients). With the NOT, long-slit spectra were obtained for the host galaxies of 13 SNe IIn, five SNe Ibn, one SN Ia-CSM, and 16 SN IMs (the derived metallicity for SN 2007sv was published in Tartaglia et al. 2015MNRAS.447..117T). The host galaxies observed at the NOT are marked with the letter "o" in the third column of Table 1. With the NOT, we also obtained broad-band R and narrow-band Hα images for the SNe IIn (except for SN 1995G) and Ibn. We complemented our observed sample with host galaxies whose metallicities (at the center of the galaxy or at the SN position) were already available in the literature (marked with the letter "l" in the third column of Table 1) or whose spectra were available in public archives (marked with the letter "a" in the third column of Table 1).(7 data files).enDatabasehttp://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/580/A1312015yCat..35800131TFIS/05 - ASTRONOMIA E ASTROFISICA