This article has an erratum: [https://doi.org/10.1051/0004-6361/201322612e]
Example SEDs (see text for description of individual SEDs) of sources with little or no AME (see Fig. 8 for SEDs with significant AME). Data points are shown as circles with errors and are colour-coded for radio data (cyan), WMAP (red), Planck (blue), and DIRBE/ IRAS (black). The best-fitting model of free-free (dotted line), synchrotron (long-dashed line), thermal dust (short-dashed line), CMB (triple-dot-dashed line), and spinning dust (dot-dashed line) are shown. Data included in the fit are shown as filled circles, while the other data are unfilled. The residual spectrum, after subtraction of free-free, synchrotron, CMB and thermal dust components, is shown as an insert.
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