Cool Stars 14 - Submitted Abstract # 94
This version created on 05 October 2006

Brown Dwarf and Low-Mass Binaries from SuperWASP-N.


R.A. Street, Queen's University, Belfast
D.J. Christian, Queen's University, Belfast
W.I. Clarkson, STScI
A.C. Cameron, University of St. Andrews
B. Enoch, The Open University
S.R. Kane, University of Florida, 
T.A. Lister, Keele University
R.G. West, University of Leicester
D.M. Wilson, Keele University
A. Evans, Keele University
A. Fitzsimmons, Queen's University Belfast
C.A. Haswell, The Open University
C. Hellier, Keele University
S.T. Hodgkin, University of Cambridge
Keith Horne, University of St. Andrews
J. Irwin, University of Cambridge
F.P. Keenan, Queen's University Belfast
A.J. Norton, The Open University
D.L. Pollacco, Queen's University Belfast
R. Ryans,  Queen's University Belfast
I. Skillen,  Isaac Newton Group, 
P.J. Wheatley, University of Leicester

The SuperWASP-N station was inaugurated in April 2004 and observed 6.7
million stars with V=8-15mag continuously until September of that
year.  Observations recommenced following an upgrade in 2006.  We have
mined SW's extensive photometric database, in conjunction with the
2MASS catalogue, for eclipsing low-mass stellar and brown dwarf
binaries.  Here we present the catalogue of objects identified
together with spectroscopic follow-up obtained from the Isaac Newton
Telescope.

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