Analysis of broad-lined Type Ic supernovae from the (intermediate) Palomar Transient Factory

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Fig. 13.

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Individual g − r color evolution for our SNe, fit with the g − r template shown in Fig. 12. In the case of PTF10ysd, iPTF13u, iPTF13dnt, and iPTF13ebw, where we have no significant g-band observations, we assume the template of Fig. 12 to be their g − r color.

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