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Astro-WISE for KiDS survey production and quality control

2011/12/05 by Gijs Verdoes Kleijn, Jelte T. A. de Jong, J. T. A. de Jong +7 · 1 citation
Engineering · Physics and Astronomy · #Adaptive optics and wavefront sensing #Astronomical Observations and Instrumentation #Astronomy and Astrophysical Research #Cosmology and Nongalactic Astrophysics (astro-ph.CO) #FOS: Physical sciences #Instrumentation and Methods for Astrophysics (astro-ph.IM) #astro-ph.CO #astro-ph.IM

paper · pdf · doi:10.48550/arxiv.1112.0886

Proceedings ADASS XXI, 2011, ASP Conference Series

arxiv created 2011/12/05 · openalex publication_date 2011/12/05 · arxiv updated 2019/08/15 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

The Kilo Degree Survey (KiDS) is a 1500 square degree optical imaging survey with the recently commissioned OmegaCAM wide-field imager on the VLT Survey Telescope (VST). A suite of data products will be delivered to ESO and the community by the KiDS survey team. Spread over Europe, the KiDS team uses Astro-WISE to collaborate efficiently and pool hardware resources. In Astro-WISE the team shares, calibrates and archives all survey data. The data-centric architectural design realizes a dynamic 'live archive' in which new KiDS survey products of improved quality can be shared with the team and eventually the full astronomical community in a flexible and controllable manner

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