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Current status of the SuperWASP project

Christian, D. J.; Pollacco, D. L.; Clarkson, W. I.; Collier Cameron, A.; Evans, A.; Fitzsimmons, A.; Haswell, C. A.; Hellier, C.; Hodgkin, S. T.; Horne, K.; Kane, S. R.; Keenan, F. P.; Lister, T. A.; Norton, A. J.; Ryans, R.; Skillen, I.; Street, R. A.; West, R. G. and Wheatley, P. J. (2005). Current status of the SuperWASP project. In: 13th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun, 5-9 Jul 2004, Hamburg, Germany.

URL: http://www.hs.uni-hamburg.de/cs13/abstracts_all.ht...
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Abstract

We present the current status of the SuperWASP project, a Wide Angle Search for Planets. SuperWASP consists of up to 8 individual cameras using ultra-wide field lenses backed by high-quality passively cooled CCDs. Each camera covers 7.8 x 7.8 sq degrees of sky, for nearly 500 sq degrees of sky coverage. SuperWASP I, located in LaPalma, is currently operational with 5 cameras and is conducting a photometric survey of a large numbers of stars in the magnitude range ~7 to 15. The collaboration has developed a custom-built reduction pipeline and aims to achieve better than 1 percent photometric precision. The pipeline will also produce well sampled light curves for all the stars in each field which will be used to detect: planetary transits, optical transients, and track Near-Earth Objects. Status of current observations, and expected rates of extrasolar planetary detections will be presented. The consortium members, institutions, and further details can be found on the web site at: http://www.superwasp.org.

Item Type: Conference or Workshop Item
Copyright Holders: 2005 European Space Agency
Extra Information: Edited by F. Favata, G.A.J. Hussain, and B. Battrick.
ESA SP-560, European Space Agency, 2005, pp475-477
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
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Item ID: 24787
Depositing User: Andrew Norton
Date Deposited: 06 May 2011 09:37
Last Modified: 07 Dec 2018 09:43
URI: http://oro.open.ac.uk/id/eprint/24787
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