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The Faint Sky Variability Survey – I. Goals and data reduction process
Authors:P J Groot  P M Vreeswijk  M E Huber  M E Everett  S B Howell  G Nelemans  J van Paradijs  E P J van den Heuvel  T Augusteijn  E Kuulkers  R G M Rutten  J Storm
Institution:Department of Astrophysics, University of Nijmegen, PO Box 9010, 6500 GL Nijmegen, the Netherlands;Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, 02138 MA, USA;Astronomical Institute 'Anton Pannekoek'/CHEAF, Kruislaan 403, 1098 SJ, Amsterdam, the Netherlands;Astrophysics Group, Planetary Science Institute, 620 N. 6th Ave., Tucson, AZ, USA;Department of Physics and Astronomy, University of Wyoming, PO Box 3905, Laramie, WY 82071, USA;Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA;Physics Department, University of Alabama in Huntsville, Huntsville, USA;Isaac Newton Group of Telescopes, Apartado de Correos 321, 38700 Sta Cruz de La Palma, Canary Islands, Spain;Nordic Optical Telescope, Apartado de Correos 474, 38700 Sta de La Palma, Canary Islands, Spain;ESA-ESTEC, Science Operations and Data Systems Division, SCI-SDG, Keplerlaan 1, 2201 AZ Noordwijk, the Netherlands;Astrophysikalisches Institut Potsdam, An der Sternwarte 16, D-14482 Potsdam, Germany
Abstract:
Keywords:methods: data analysis  techniques: photometric  surveys  stars: variables: other  Galaxy: stellar content
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