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Astronomical Image Processing System ''++'' is a software package whose development was started in the early nineties, written almost entirely in C++, and which initial goal was to replace the by then already aging AIPS software. It has now been reborn as CASA and is the basis of the image processing systems for several next-generation radio telescopes including ALMA, eVLA, and ASKAP. ==Early history== In 1988-89, the Director of National Radio Astronomy Observatory (NRAO), Paul Vanden Bout, convened an independent review panel, the Software Advisory Group (SWAG) to produce recommendations for the future of processing software for NRAO. SWAG was chaired by Tim Cornwell, and its members included Geoff Croes, Gareth Hunt, Jan Noordam, and Ray Norris. SWAG recommendations were that: * All data processing in NRAO should be coordinated by a new Assistant Director for Computing * AIPS should be re-designed and re-implemented following certain general guidelines * An equal amount of attention should be devoted to single-dish software. In late 1990 the NRAO Director accepted the recommendations, and the task of defining the new package began. The project was originally an effort by several astronomical institutes together in a consortium, the Australia Telescope National Facility (ATNF), the Jodrell Bank Observatory (JBO) and the MERLIN/VLBI National Facility (MERLIN/VLBI), the Berkeley-Illinois-Maryland Association (BIMA), the National Radio Astronomy Observatory (NRAO) and the Netherlands Foundation for Research in Astronomy ASTRON. 抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)』 ■ウィキペディアで「AIPS++」の詳細全文を読む スポンサード リンク
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