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Fig. 5

image

Left: comparison of the R-band light curve of SN 2015da with those of SNe 1988Z (Turatto et al. 1993), 2005ip, 2006jl (Stritzinger et al. 2012) and 2010jl (Fransson et al. 2014). Absolute magnitudes were obtained using Milky Way and host galaxy extinctions and adopting distances reported in the literature. The representative error barcorresponds to the uncertainty on the distance of NGC 5337. Right: comparison of the R-band light curve of SN 2015da with that of the overluminous SN 2006gy up to ≃ 250 d.

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