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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: shenghonggu@ynao.ac.cn
Andrew Collier Cameron
Affiliation:
School of Physics and Astronomy, University of St Andrews, Fife KY16 9SS, UK email: acc4@st-and.ac.uk
Xiao-bin Wang
Affiliation:
National Astronomical Observatories/Yunnan Observatory, CAS, Kunming 650011, China email: shenghonggu@ynao.ac.cn
Li-yun Zhang
Affiliation:
National Astronomical Observatories/Yunnan Observatory, CAS, Kunming 650011, China email: shenghonggu@ynao.ac.cn
Xiang-song Fang
Affiliation:
National Astronomical Observatories/Yunnan Observatory, CAS, Kunming 650011, China email: shenghonggu@ynao.ac.cn
Xue-jing Li
Affiliation:
National Astronomical Observatories/Yunnan Observatory, CAS, Kunming 650011, China email: shenghonggu@ynao.ac.cn
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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

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