The VISTA Data Flow System
ESO ASTROPHYSICS SYMPOSIA(2008)
摘要
The Visible and Infrared Survey Telescope for Astronomy (VISTA) is a new ESO telescope that will be commissioned in late 2007. The telescope has been specifically designed for survey work in both the visible and near infrared, but to start with will only have an infrared camera (VIRCAM). The focal plane of VIRCAM will consist of 16 2k by 2k non-buttable detectors with a pawprint of 0.6 square degrees. With an expected nightly data rate of 200–500 Gb, automated pipeline processing and data management requirements are paramount.
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关键词
Science Archive,Photometric Calibration,Reduction Pipeline,Monitor Data Quality,Data Management Requirement
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