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: http://www.atnf.csiro.au/whats_on/workshops/synthesis2003/talks/reduc_demo/375_uv.html
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Imaging with a compact configuration - |
| | Baseline lengths are most naturally described in units of wavelengths, |
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|  | Fig. 1: ATCA 375-m configuration uv coverage for a complete 12-hour synthesis. |
. The ``uv-plane'' is the surface of our synthesised large telescope. The 375-m configurations provides very short baselines (central tracks). The long baselines with antenna 6 cannot be used for imaging, because it is not possible to synthesise such a huge telescope without having information in the empty areas.