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SuperWASP-N extrasolar planet candidates between 18 < RA < 21 h
Authors:R A Street  D J Christian  W I Clarkson  A Collier Cameron  B Enoch  S R Kane  T A Lister  R G West  D M Wilson  A Evans  A Fitzsimmons  C A Haswell  C Hellier  S T Hodgkin  K Horne  J Irwin  F P Keenan  A J Norton  J Osborne  D L Pollacco  R Ryans  I Skillen  P J Wheatley  J Barnes
Institution:Astrophysics Research Centre, Department of Physics and Astronomy, Queen's University Belfast, Belfast BT7 1NN;Las Cumbres Observatory, 6740B Cortona Drive, Goleta, CA 93117, USA;Department of Physics, Broida Hall, University of California, Santa Barbara, CA 93106-9530, USA;Department of Physics &Astronomy, The Open University, Milton Keynes MK7 6AA;Space Telescope Science Institute (STScI), 3700 San Martin Drive, Baltimore, MD 21218, USA;School of Physics &Astronomy, University of St. Andrews, North Haugh, St. Andrews, Fife KY16 9SS;Dept. of Astronomy, University of Florida, 211 Bryant Space Science Center, Gainesville, FL 32611-2055, USA;Astrophysics Group, School of Chemistry &Physics, Keele University, Staffordshire ST5 5BG;Department of Physics &Astronomy, University of Leicester, Leicester LE1 7RH;Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA;Isaac Newton Group of Telescopes, Apartado de correos 321, E-38700 Santa Cruz de la Palma, Tenerife, Spain;Department of Physics, University of Warwick, Coventry CV4 7AL;Centre for Astrophysics Research, Science &Technology Research Institute, University of Hertfordshire, Hatfield AL10 9AB
Abstract:
Keywords:techniques: photometric  methods: data analysis  surveys  binaries: eclipsing  planetary systems
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