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Imaging with a large configuration - |
| | The uv-coverage displayed in Fig. 4 leads to a high-resolution dirty image as shown in Fig. 5. Substructure becomes visible not only in the primary target, NGC 1511, but also in several background sources (e.g. the one to the right). |
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| | Fig. 5: ATCA 6A configuration dirty image of NGC 1511 and its surroundings. Note: The field of view displayed here is smaller than for the 375-m configuration (otherwise one would not see the details). |
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