activity
19972013
most citedEfficient identification of exoplanetary transit candidates from SuperWASP light curves

365 citations · 2.3k across the 26 of their papers we have counts for

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Showing 2006Show all

11 papers · 1 filter

astro-ph2006

The colour of noise in SuperWASP data and the implications for finding extra-solar planets

A. M. S. Smith, A. Collier Cameron, D. J. Christian +19

A recent study demonstrated that there is significant covariance structure in the noise on data from ground-based photometric surveys designed to detect transiting extrasolar plane…

astro-ph200639 cited

Mass transfer during low mass X-ray transient decays

Craig R. Powell, Carole A. Haswell, Maurizio Falanga

The outbursts of low mass X-ray binaries are prolonged relative to those of dwarf nova cataclysmic variables as a consequence of X-ray irradiation of the disc. We show that the tim…

astro-ph20062 cited

Artificial variability in XMM-Newton observations of X-ray sources: M31 as a case study

R. Barnard, S. Trudolyubov, C. A. Haswell +3

Power density spectra (PDS) that are characteristic of low mass X-ray binaries (LMXBs) have been previously reported for M31 X-ray sources observed by XMM-Newton. However, we have…

astro-ph2006226 cited

A fast hybrid algorithm for exoplanetary transit searches

A. Collier Cameron, D. Pollacco, R. A. Street +22

We present a fast and efficient hybrid algorithm for selecting exoplanetary candidates from wide-field transit surveys. Our method is based on the widely-used SysRem and Box Least-…

astro-ph2006302 cited

WASP-1b and WASP-2b: Two new transiting exoplanets detected with SuperWASP and SOPHIE

A. Collier Cameron, F. Bouchy, G. Hebrard +36

We have detected low-amplitude radial-velocity variations in two stars, USNO-B1.0 1219-0005465 (GSC 02265-00107 = WASP-1) and USNO-B1.0 0964-0543604 (GSC 00522-01199 = WASP-2). Bot…

astro-ph200647 cited

The impact of correlated noise on SuperWASP detection rates for transiting extra-solar planets

A. M. S. Smith, A. Collier Cameron, D. J. Christian +19

We present a model of the stellar populations in the fields observed by one of the SuperWASP-N cameras in the 2004 observing season. We use the Besancon Galactic model to define th…