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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
Affiliation: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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