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Imaging with a multi-configuration array - |
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| | Now the full source flux, both extended plus compact sources, is recovered by the observations. A residual error is visible in the form of concentric ellipses around the phase centre, which was placed 1 arcmin south of the galaxy centre. |
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|  | Fig. 9: ATCA multi-configuration cleaned image of NGC 1511 and its surroundings. |
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