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Fig. 3.

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(r − J) and (i − H) colour evolution of SN 2019wxt compared to the colour evolution of the well-observed Type Ibc events SN 2007Y (Stritzinger et al. 2009), SN 2007gr (Bianco et al. 2014), SN 2006jc (Bianco et al. 2014) and SN 2002ap (Yoshii et al. 2003). All the magnitudes are in the AB system.

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