Fig. A.2.
Illustration of the influence of the albedo on type II-P SN radiation. Left: bolometric light curves for 12 M⊙ 2P smooth 1D ejecta but adopting a fixed albedo of 0.1 (absorption dominates the opacity), 0.9, 0.99, and 0.999 (scattering vastly dominates the opacity). Right: same as left, but now for a 2P-2D clumped ejecta with ξ0 = 0.1, Vcl = 0 km s−1 and ΔVcl = 6000 km s−1.
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