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SuperWASP-North extrasolar planet candidates between 3h < RA < 6h
Authors:W I Clarkson  B Enoch  C A Haswell  A J Norton  D J Christian  A Collier Cameron  S R Kane  K D Horne  T A Lister  R A Street  R G West  D M Wilson  N Evans  A Fitzsimmons  C Hellier  S T Hodgkin  J Irwin  F P Keenan  J P Osborne  N R Parley  D L Pollacco  R Ryans  I Skillen  P J Wheatley
Institution:Department of Physics &Astronomy, The Open University, Milton Keynes MK7 6AA;Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA;APS Division, Department of Physics and Astronomy, Queen's University Belfast, Belfast BT7 1NN;SUPA, School of Physics &Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS;University of Florida, PO Box 112005, 211 Bryant Space Science Centre, Gainesville, FL 32611-2055, USA;Astrophysics Group, School of Chemistry &Physics, Keele University, Staffordshire ST5 5BG;Las Cumbres Observatory, 6740B Cortona Drive, CA 93117, USA;Department of Physics, Broida Hall, University of California, Santa Barbara, CA 93106-9530, USA;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-3700 Santa Cruz de la Palma, Tenerife, Spain;Department of Physics, University of Warwick, Coventry CV4 7AL
Abstract:
Keywords:methods: data analysis  planetary systems  stars: variables: other
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