Fig. 3
SEDs of the millimeter-centimeter excess in the LMC (in green) and in the SMC (in black). The spectral shape of the CMB fluctuations (dBν(2.725 K) / dT × DeltaTFixsen 2009) is scaled to the SMC excess brightnesses for comparison. Modified black body fits to the LMC and the SMC excess representing a possible cold dust component are shown as dotted lines.
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