The Open UniversitySkip to content
 

The SuperWASP wide-field exoplanetary transit survey: candidates from fields 23 h < RA < 03 h

Christian, D. J.; Pollacco, D. L.; Skillen, I.; Street, R. A.; Keenan, F. P.; Clarkson, W. I.; Collier Cameron, A.; Kane, S. R.; Lister, T .A.; West, R. G.; Enoch, B.; Evans, A.; Fitzsimmons, A.; Haswell, C. A.; Hellier, C.; Hodgkin, S. T.; Horne, K.; Irwin, J.; Norton, A. J.; Osborne, J.; Ryans, R.; Wheatley, P. J. and Wilson, D. M. (2006). The SuperWASP wide-field exoplanetary transit survey: candidates from fields 23 h < RA < 03 h. Monthly Notices of the Royal Astronomical Society, 372(3) pp. 1117–1128.

DOI (Digital Object Identifier) Link: https://doi.org/10.1111/j.1365-2966.2006.10913.x
Google Scholar: Look up in Google Scholar

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.

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/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Item ID: 8283
Depositing User: Andrew Norton
Date Deposited: 02 Jul 2007
Last Modified: 07 Dec 2018 09:04
URI: http://oro.open.ac.uk/id/eprint/8283
Share this page:

Metrics

Altmetrics from Altmetric

Citations from Dimensions

Actions (login may be required)

Policies | Disclaimer

© The Open University   contact the OU