Bolometric, Swift U, and JohnsonBV RI light curves for our v7500_d0_n8 density profile, with various scaling parameters (s = 3, 9.7, and 100), and the UBV RI light curves of SN 2009ig. Light curves of SN 2009ig are shown assuming μ = 32.6 ± 0.4, negligible host extinction, and an explosion epoch of JD = 2455063.41 ± 0.08 (Foley et al. 2012). Filled points represent KAIT light curves, while unfilled points show Swift light curves. We note that for our s = 3 model t_start = 0.5 days, hence we have omitted the light curve for t < 1 days. For s = 9.7 and 100, t_start = 1.5 days, and wehave omitted the light curve for t < 2 days in these cases.