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dc.contributor.authorSipocz, B.
dc.contributor.authorKovacs, G.
dc.contributor.authorPinfield, D.J.
dc.contributor.authorHodgkin, S.T.
dc.date.accessioned2011-06-01T16:21:12Z
dc.date.available2011-06-01T16:21:12Z
dc.date.issued2011
dc.identifier.citationIn: Detection and Dynamics of Transiting Exoplanets 11 Art. No. 06003en_US
dc.identifier.other905462
dc.identifier.urihttp://dx.doi.org/10.1051/epjconf/20101106003
dc.identifier.urihttp://hdl.handle.net/2299/5874
dc.descriptionOriginal article can be found at : http://www.epj-conferences.org/ This is an Open Access article distributed under the terms of the Creative Commons Attribution-Noncommercial License 3.0, which permits unrestricted use, distribution, and reproduction in any noncommercial medium, provided the original work is properly cited.en_US
dc.description.abstractThe WFCAM Transit Survey (WTS) has been obtaining data on the United Kingdom Infrared Telescope since 2007. The WTS targets about 8,000 M dwarfs over several square degrees of sky, and aims to find low-mass eclipsing binaries and planets, down to the size of the Earth, transiting M dwarf stars with periods up to a few days.en_US
dc.language.isoenen_US
dc.publisherEDP Sciencesen_US
dc.titleThe WFCAM transit survey.en_US
dc.typeConference paperen_US
herts.preservation.rarelyaccessedtrue


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