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Fig. A.2.

image

N10def model spectra at various epochs, with varying helium abundances given as percentages of ejecta mass. Shaded regions show the difference produced in the spectra by varying the helium abundance. Phases relative to bolometric maximum light are given in black, while times since explosion are given in red. Left panel: grey shaded regions represent He Iλ5876, λ6678, λ7065, λ10830, and λ20587 at rest and blue-shifted by the maximum velocity of the model (∼12 700 km s−1). Right panel: zoomed in regions surrounding He Iλ10830. Each shaded region corresponds to a blue-shift of 2500 km s−1.

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