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Fig. 13

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Calibration with an improved sky model. This shows single-band residual images after Gp and Mpq solutions. The left image is from the original reduction, the right image uses a sky model improved via my ΔE analysis. Crosses indicate the positions of sources for which the model was improved, plus 3C 147 itself (source A).

This figure is made of several images, please see below:

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