SuperWASP-North Extra-solar Planet Candidates between 3hr < RA < 6hr
W. I. Clarkson, B. Enoch, C. A. Haswell, A. J. Norton, D. J., Christian, A. Collier Cameron, S. R. Kane, K. D. Horne, T. A. Lister, R. A., Street, R. G. West, D. M. Wilson, N. Evans, A. Fitzsimmons, C. Hellier, S., T.Hodgkin, J. Irwin, F. P. Keenan, J. P. Osborne, N. R. Parley

TL;DR
This paper reports on the detection of four promising extrasolar planet candidates from the SuperWASP-North survey, based on analysis of 1.3 billion data points from 6.7 million stars, focusing on the 3h-6h RA range.
Contribution
The study presents a large-scale photometric survey and a detailed candidate selection process, identifying new potential hot-Jupiter exoplanets with rigorous filtering techniques.
Findings
Identified 4 strong exoplanet candidates for follow-up.
Processed 1.3 billion data points from 6.7 million stars.
Developed a systematic candidate filtering methodology.
Abstract
The Wide Angle Search for Planets (WASP) photometrically surveys a large number of nearby stars to uncover candidate extrasolar planet systems by virtue of small-amplitude lightcurve dips on a < 5-day timescale typical of the ``Hot-Jupiters.'' Observations with the SuperWASP-North instrument between April and September 2004 produced a rich photometric dataset of some 1.3 billion datapoints from 6.7 million stars. Our custom-built data acquisition and processing system produces ~0.02 mag photometric precision at V=13. We present the transit-candidates in the 03h-06h RA range. Of 141,895 lightcurves with sufficient sampling to provide adequate coverage, 2688 show statistically significant transit-like periodicities. Of these, 44 pass visual inspection of the lightcurve, of which 24 are removed through a set of cuts on the statistical significance of artefacts. All but 4 of the remaining…
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