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Fig. 3


Colour evolution of SN 2015H compared to other SNe Iax and the normal SN Ia, SN 2011fe (Richmond & Smith 2012). In panel a) we show the gr colour while panel b) shows the ri colour. SN 2005hk is shown assuming negligible host extinction (Foley et al. 2013). SN 2012Z and SN 2011fe have been corrected for host extinction, with data taken from Stritzinger et al. (2015) and Richmond & Smith (2012), respectively. Note that the colour of SN 2011fe is derived from BVRI magnitudes (Jester et al. 2005). Maximum refers to the date of r-band maximum.

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