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Fig. 8


Temporal evolution of the observed BV pseudo-colour. The filled red circles, black squares, light-green triangles, pink diamonds, and golden downward triangles represent the data of (respectively) SN 2011iv, SN 2007on, iPTF13ebh, SN 2006mr, and SN 2006dd. The data of the normal SN 2006dd and the subluminous SN 2006mr are from Stritzinger et al. (2010) and Contreras et al. (2010), respectively. All colours have been corrected for Galactic reddening. The Lira relation from Folatelli et al. (2010) is indicated as a red dashed line, and Lira-relation fits to the data are shown as red (SN 2011iv) and blue (SN 2007on) solid lines. The top-right inset contains the BV colour evolution of SN 2007on and SN 2011iv compared to their corresponding modelled BV colour evolution predicted by the best-fit DD models presented in Appendix D.

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