Fig. 7
Left: images of sources 08 (top) and 10 (bottom) at U band showing the core+jet emission fitted to Gaussian emission distributions (see text). The contours are spaced logarithmically in ten levels, running from two times the rms of the residuals to the image peak. Right: post-fit residuals of UVMULTIFIT after fitting Gaussian brightness distributions to the core+jet emission of each source.
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