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Imaging with a compact configuration - |
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| | The uv-coverage (central area only!) displayed in Fig. 1 leads to a low-resolution image, still with the characteristics of the interferometer beam in it, a so-called ``dirty'' image.It has low resolution, but high sensitivity to extended emission. |
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|  | Fig. 2: ATCA 375-m configuration dirty image of NGC 1511 and its surroundings; the field of view is ca. 30 arcmin across. |
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