Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/18786
Title: The SuperWASP wide-field exoplanetary transit survey: Candidates from fields 23 h < RA < 03 h
Authors: Christian, D. J.
Pollacco, D. L.
Street, R. A.
Keenan, F. P.
Fitzsimmons, A.
Ryans, R.
Skillen, I.
Clarkson, W. I.
Enoch, B.
Haswell, C. A.
Norton, A. J.
Collier Cameron A.
Kane, S. R.
Lister, T. A.
Horne, K.
West, R. G.
Osborne, J.
Lister, T. A.
Evans, A.
Hellier, C.
Wilson, D. M.
Hodgkin, S. T.
Irwin, J.
Wheatley, P. J.
First Published: 1-Nov-2006
Publisher: Royal Astronomical Society (RAS)
Citation: Monthly Notices of the Royal Astronomical Society, 2006, 372 (3), pp. 1117-1128
Abstract: Photometric transit surveys promise to complement the currently known sample of extra-solar planets (ESPs) by providing additional information on the planets and especially their radii. Here, we present ESP candidates from one such survey called, the Wide Angle Search for Planets (WASP) obtained with the SuperWASP wide-field imaging system. Observations were taken with SuperWASP North located in La Palma during the 2004 April to October observing season. The data cover fields between 23 and 03 h in RA at declinations above +12. This amounts to over ≈400 000 stars with V magnitudes 8–13.5. For the stars brighter than 12.5, we achieve better than 1 per cent photometric precision. Here, we present 41 sources with low-amplitude variability between ≈1 and 10 mmag, from which we select 12 with periods between 1.2 and 4.4 d as the most promising ESP candidates. We discuss the properties of these ESP candidates, the expected fraction of transits recovered for our sample and implications for the frequency and detection of hot-Jupiters.
DOI Link: 10.1111/j.1365-2966.2006.10913.x
ISSN: 0035-8711
eISSN: 1365-2966
Links: http://hdl.handle.net/2381/18786
http://mnras.oxfordjournals.org/content/372/3/1117
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2006 the authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. Deposited with reference to the publisher’s archiving policy available on the SHERPA/RoMEO website.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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