SuperWASP-N extrasolar planet candidates between 18h < RA < 21h

Street, R. A.; Christian, D. J.; Clarkson, W. I.; Collier Cameron, A.; Enoch, B.; Kane, S. R.; Lister, T .A.; West, R. G.; Wilson, D. M.; Evans, A.; Fitzsimmons, A.; Haswell, C. A.; Hellier, C.; Horne, K.; Hodgkin, S. T.; Irwin, J.; Keenan, F. P.; Norton, A. J.; Osborne, J.; Pollacco, D. L.; Ryans, R.; Skillen, I.; Wheatley, P. J. and Barnes, J.R. (2007). SuperWASP-N extrasolar planet candidates between 18h < RA < 21h. Monthly Notices of the Royal Astronomical Society, 379(2) pp. 816–832.

DOI: https://doi.org/10.1111/j.1365-2966.2007.11987.x

Abstract

The SuperWASP-I (Wide Angle Search for Planets-I) instrument observed 6.7 million stars between 8 and 15mag from La Palma during the 2004 May-September season. Our transit-hunting algorithm selected 11626 objects from the 184442 stars within the RA (right ascension) range 18-21h. We describe our thorough selection procedure whereby catalogue information is exploited along with careful study of the SuperWASP data to filter out, as far as possible, transit mimics. We have identified 35 candidates which we recommend for follow-up observations.

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About

• Item ORO ID
• 9838
• Item Type
• Journal Item
• ISSN
• 1365-2966
• Extra Information
• Click here to view other publications available on this repository relating to the SuperWASP Project.
• Keywords
• methods; data analysis; planetary systems formation;
• Academic Unit or School
• Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
  Faculty of Science, Technology, Engineering and Mathematics (STEM)
• Depositing User
• Andrew Norton