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Titlebook: Very High Angular Resolution Imaging; Proceedings of the 1 J. G. Robertson,W. J. Tango Conference proceedings 1994 Springer Science+Busines

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D. L. Jauncey,J. E. Reynolds,A. K. Tzioumis,R. H. Ferris,R. P. Norris,M. W. Sinclair,V. Migenes,R. G
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The Very Long Baseline Arrayof 512 Mb/s and unattended operation for a day recording at 128 Mb/s. The antennas are controlled and monitored by a single operator located in the Array Operations Center (AOC) in Socorro, New Mexico. The AOC also houses the 20 station correlator which processes the data recorded at the antennas.
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Comparing Optical and Radio - Quantum Issuesw techniques emerge, we clearly need to do better. Coherent and incoherent detection, heterodyning and interferometry are all situations where a full analysis involves quantum behaviour of the radiation. This informal review covers the general approach needed and goes over some points of principle which arise.
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Direct Maximum-Entropy Image Reconstruction from the Bispectrumce fast as possible. Radio-astronomical imaging strategies, on the other hand, have always been designed to cope with sparse and missing data, and many sophisticated algorithms have been designed to make maximum use of a-priori constraints with iterative global fitting techniques.
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