Fig. 4
Generated Stokes Q and U instrument models in the two scanning directions, the azimuth in the top panels and the elevation in the bottom panels for (a) the 4.85 GHz (upper two rows) and (b) 8.35 GHz (lower two rows) receivers. The models were generated for 65 observing sessions. The variability of the plotted models is comparable to the respective errors of the fit.
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