Fig. 6
IRAC (3.6 μm – open squares, 4.5 μm – filled squares, 5.8 μm – open circles, 8.0 μm – filled circles), IRS PUI (open triangles) and MIPS 24.0 μm (filled triangles) light curves of SN 2004dj. The excess emission appearing on 3.6, 5.8 and 8.0 μm peaks later at longer wavelengths, which is consistent with a warm, cooling dust formed one year after the core collapse.
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