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- W2062180619 abstract "The dual feed astrometric instrument software of PRIMA (PACMAN) that is currently being integrated at the VLTI will use two spatially modulated fringe sensor units and a laser metrology system to carry out differential astrometry. Its software and hardware compromises a distributed system involving many real time computers and workstations operating in a synchronized manner. Its architecture has been designed to allow the construction of efficient and flexible calibration and observation procedures. In parallel, a novel scheme of integrating M-code (MATLAB/OCTAVE) with standard VLT (Very Large Telescope) control software applications had to be devised in order to support numerically intensive operations and to have the capacity of adapting to fast varying strategies and algorithms. This paper presents the instrument software, including the current operational sequences for the laboratory calibration and sky calibration. Finally, a detailed description of the algorithms with their implementation, both under M and C code, are shown together with a comparative analysis of their performance and maintainability." @default.
- W2062180619 created "2016-06-24" @default.
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- W2062180619 date "2010-07-22" @default.
- W2062180619 modified "2023-09-23" @default.
- W2062180619 title "PACMAN: PRIMA astrometric instrument software" @default.
- W2062180619 doi "https://doi.org/10.1117/12.857388" @default.
- W2062180619 hasPublicationYear "2010" @default.
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