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The New Photometric Observations for Transiting Exoplanet HAT-P-24b
Wang XB(王晓彬)1,2; Andrew Collier Cameron33; Gu SH(顾盛宏)1,2
会议录名称Proceedings of the International Astronomical Union (IAU) Symposium - Formation, Detection, and Characterization of Extrasolar Habitable Planets
2014-04
卷号293
页码122-124
DOI10.1017/S1743921313012672
产权排序第1完成单位
收录类别其他
会议名称293th IAU Symposium - Formation, Detection, and Characterization of Extrasolar Habitable Planets
会议日期2012-08-27
会议地点Beijing, China
关键词Exoplanetary System Transit Individual:Hat-p-24
摘要The transiting exoplanetary system HAT-P-24 was observed by using CCD cameras at Yunnan Observatory and Hokoon Astronomical Centre, China in 2010 and 2012. Three new transit light curves are analyzed by means of MCMC technique, and the new physical parameters of the system are derived, which are compatible with the old ones in the discovery paper. The orbital period of HAT-P-24b is refined and no obvious TTV signal can be found from five transit events during 2010-2012.
语种英语
ISBN号978-1107033825
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归档日期2015-11-19
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文献类型会议论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/9671
专题系外行星研究组
中国科学院天体结构与演化重点实验室
作者单位1.National Astronomical Observatories/Yunnan Observatory Chinese Academy of Sciences, Kunming 650011, China
2.Key Laboratory for the Structure and Evolution of Celestial Objects Chinese Academy of Sciences, Kunming 650011, China
3.School of Physics and Astronomy, University of St Andrews North Haugh, St Andrews, Fife KY16 9SS, UK
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Wang XB,Andrew Collier Cameron3,Gu SH. The New Photometric Observations for Transiting Exoplanet HAT-P-24b[C],2014:122-124.
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