Fig. 17
Top: brightness temperature of Jupiter (Tbr) compared with the data from Weiland et al. (2011), linearly rescaled in frequency to match LFI’s central frequencies νcen and corrected for difference between the LFI and WMAP dipoles. Bottom: deviation from unity of the ratio between LFI’s estimate for Tbr and WMAP’s. The agreement is excellent among the three frequencies.
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