The New Photometric Observations for Transiting Exoplanet HAT-P-24b

doi:10.1017/S1743921313012672

	The New Photometric Observations for Transiting Exoplanet HAT-P-24b
	Wang XB(王晓彬)1,2 ; Andrew Collier Cameron 3; Gu SH(顾盛宏)1,2
	2014-04
会议日期	2012-08-27
会议地点	Beijing, China
关键词	Exoplanetary System Transit Individual:Hat-p-24
卷号	293
DOI	10.1017/S1743921313012672
页码	122-124
英文摘要	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.
产权排序	第1完成单位
会议录	Proceedings of the International Astronomical Union (IAU) Symposium - Formation, Detection, and Characterization of Extrasolar Habitable Planets
资助机构	National Natural Science Foundation of China ; Chinese Academy of Sciences ; Sik Sik Yuen of Hong Kong, China
学科主题	天文学 ; 天体物理学
语种	英语
URL标识	查看原文
资助项目	National Natural Science Foundation of China[10873031] ; Chinese Academy of Sciences[KJCX2-YW-T24] ; the special grant from Sik Sik Yuen of Hong Kong, China
ISBN号	978-1107033825
内容类型	会议论文
源URL	[http://ir.ynao.ac.cn/handle/114a53/9671]
专题	云南天文台_系外行星研究组云南天文台_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
推荐引用方式 GB/T 7714	Wang XB,Andrew Collier Cameron,Gu SH. The New Photometric Observations for Transiting Exoplanet HAT-P-24b[C]. 见:. Beijing, China. 2012-08-27.