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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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Radio Arrays — mm to Metersterferometer arrays, and their acceptance as essential tools in astronomy are a result of the remarkable flexibility and imaging capabilities of modern arrays. Much of the success of these arrays’ is due to advances in data processing and imaging brought about by innovative and powerful algorithms.
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The Very Long Baseline Arraydiameter reflector antennas located so as to give optimum coverage of baselines up to 8600 kin. Instrumentation provided at each antenna includes receivers for nine frequency bands between 327 MHz and 43 GHz, a hydrogen maser frequency standard and a tape recorder system capable of a peak data rate
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The Sydney University Stellar Interferometer (SUSI)wavefront-tilt compensation and dynamic optical path length compensation. Initially it will operate in the blue part of the visual spectrum but provision has been made for the addition of an additional beam-combining system for a second spectral band. The rationale behind the choice of instrumental
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1743-9213 truments and pow­ erful imaging algorithms have generated images of unprecedented resolution and quality. In the optical and infrared, the great technical difficulties associated with constructing separated-aperture interferometers have been largely overcome, and many new instruments are now operati
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T. J. Cornwellbiete, sowie der Satz von Goursat. Daraus lässt sich der Cauchy’sche Integralsatz für Sterngebiete ableiten. Für einfach zusammenhängende Gebiete erhält man ihn ebenfalls, wenn man jene Gebiete „einfach zusammenhängend“ nennt, auf denen jede holomorphe Funktion eine Stammfunktion besitzt. Dass diese
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Modeling Pipeline Applications in POETRIES phases of the development cycle of these kinds of application. This study specifically presents the development of an analytical performance model for pipelined applications. This model is intended to be used in the POETRIES distributed-program development environment, which is aimed at dynamic per
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