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Fig. 3


Color evolution of SN 2010ev compared with high velocity gradient (HVG) SNe Ia: SN 2002bo, SN 2002dj, and SN 2002er. The SN colors have been dereddened for MW extinction only. We also show the colors of the B15 model without extinction (solid gray line) and with the host extinction (dashed gray line) obtained in Sect. 3.6.

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