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Fig. E.1


The amount of SN Ia ejecta mass probed by the emission contained within the uvm2, U, B, and V bands as a function of days past explosion. These calculations are based on the DD model 5p0z22.18b. The masses are calculated by first averaging the opacity across the filter range, and then the total mass at this opacity is integrated from infinity down to an optical depth of unity.

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