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Photometric follow-up observation of some SuperWASP transiting planet candidates

Published online by Cambridge University Press:  01 October 2007

Sheng-hong Gu ,
Andrew Collier Cameron ,
Xiao-bin Wang ,
Li-yun Zhang ,
Xiang-song Fang  and
Xue-jing Li
Sheng-hong Gu
Affiliation:
National Astronomical Observatories/Yunnan Observatory, CAS, Kunming 650011, China email: [email protected]
Andrew Collier Cameron
Affiliation:
School of Physics and Astronomy, University of St Andrews, Fife KY16 9SS, UK email: [email protected]
Xiao-bin Wang
Affiliation:
National Astronomical Observatories/Yunnan Observatory, CAS, Kunming 650011, China email: [email protected]
Li-yun Zhang
Affiliation:
National Astronomical Observatories/Yunnan Observatory, CAS, Kunming 650011, China email: [email protected]
Xiang-song Fang
Affiliation:
National Astronomical Observatories/Yunnan Observatory, CAS, Kunming 650011, China email: [email protected]
Xue-jing Li
Affiliation:
National Astronomical Observatories/Yunnan Observatory, CAS, Kunming 650011, China email: [email protected]
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Abstract

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Three SuperWASP transiting planet candidates were observed through R or I filters using the 1-meter telescope and CCD camera of Yunnan Observatory from 2006 to 2007. The relative photometric data were corrected for the systematic errors by means of Tamuz et al. (2005) and Collier Cameron et al. (2006)'s algorithms. The resulting light curves demonstrate that one of three targets is a potential exoplanet candidate, which is worthy to perform further follow-up observation to clarify.

Keywords

exoplanettransitphotometry
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S249: Exoplanets: Detection, Formation and Dynamics , October 2007 , pp. 83 - 84
Copyright
Copyright © International Astronomical Union 2008

References

Christian, D. J. et al. 2006, MNRAS, 372, 1117CrossRefGoogle Scholar
Clarkson, W. I. et al. 2007, MNRAS, 381, 851CrossRefGoogle Scholar
Collier Cameron, A. et al. 2006, MNRAS, 373, 799CrossRefGoogle Scholar
Collier Cameron, A. et al. 2007, MNRAS, 380, 1230CrossRefGoogle Scholar
Lister, T. A. et al. 2007, MNRAS, 379, 647CrossRefGoogle Scholar
Pollacco, D. L. et al. 2006, PASP, 118, 1407CrossRefGoogle Scholar
Street, R. A. et al. 2007, MNRAS, 379, 816CrossRefGoogle Scholar
Tamuz, O., Mazeh, T. & Zucker, S. 2005, MNRAS, 356, 1466CrossRefGoogle Scholar