Fig. 9
Top panels: WMAP/Planck light curves for the sources that are well fit by both the VLTL-flare model and the rotating jet model. The WMAP data are shown by filled symbols and the later Planck data are shown by open symbols. Middle panels: residuals between the normalised WMAP flux densities (Eq. (11)) and the VLTL-flare model. Bottom panels: residuals between the normalised WMAP flux densities and the rotating jet model. Grey dash dot lines indicate the zero level in the residual plots.
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