activity
20062008
most citedEfficient identification of exoplanetary transit candidates from SuperWASP light curves

365 citations · 681 across the 8 of their papers we have counts for

collaborators

6 papers

astro-ph200893 cited

WASP-10b: a 3M_J, gas-giant planet transiting a late-type K star

D. J. Christian, N. P. Gibson, E. K. Simpson +37

We report the discovery of WASP-10b, a new transiting extrasolar planet (ESP) discovered by the WASP Consortium and confirmed using NOT FIES and SOPHIE radial velocity data. A 3.09…

astro-ph200715 cited

SuperWASP-N Extra-solar Planet Candidates from Fields 06hr < RA < 16hr

S. R. Kane, W. I. Clarkson, R. G. West +21

The Wide Angle Search for Planets (WASP) survey currently operates two installations, designated SuperWASP-N and SuperWASP-S, located in the northern and southern hemispheres respe…

astro-ph2007365 cited

Efficient identification of exoplanetary transit candidates from SuperWASP light curves

A. Collier Cameron, D. M. Wilson, R. G. West +29

Transiting extrasolar planets constitute only a small fraction of the range of stellar systems found to display periodic, shallow dimmings in wide-field surveys employing small-ape…

astro-ph200726 cited

SuperWASP-N Extra-solar Planet Candidates Between 18hr < RA < 21hr

R. A. Street, D. J. Christian, W. I. Clarkson +21

The SuperWASP-I instrument observed 6.7 million stars between 8-15 mag from La Palma during the 2004 May-September season. Our transit-hunting algorithm selected 11,626 objects fro…

astro-ph2007141 cited

New periodic variable stars coincident with ROSAT sources discovered using SuperWASP

A. J. Norton, P. J. Wheatley, R. G. West +17

We present optical lightcurves of 428 periodic variable stars coincident with ROSAT X-ray sources, detected using the first run of the SuperWASP photometric survey. Only 68 of thes…

astro-ph2006

The SuperWASP wide-field exoplanetary transit survey: Candidates from Fields 23hr < RA < 03hr

D. J. Christian, D. L. Pollacco, I. Skillen +20

Photometric transit surveys promise to complement the currently known sample of extra-solar planets by providing additional information on the planets and especially their radii. H…