Observations and Study of Transit Events in the Exoplanet System WASP-10

碩士 === 國立清華大學 === 天文研究所 === 101 === We observed one new transit of WAP-10b using a 46 cm telescope located at WISE Observatory in Israel, in order to search for transit timing variations (TTVs) which can be induced by the existing of the additional planets in the system. Employing 34 available light...

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Main Authors: Chien, Ping, 簡屏
Other Authors: Jiang, Ing-Guey
Format: Others
Language:en_US
Published: 2012
Online Access:http://ndltd.ncl.edu.tw/handle/93732438859215351690
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spelling ndltd-TW-101NTHU51990012015-10-13T21:55:44Z http://ndltd.ncl.edu.tw/handle/93732438859215351690 Observations and Study of Transit Events in the Exoplanet System WASP-10 WASP-10 系外行星系統之凌星事件的觀測研究 Chien, Ping 簡屏 碩士 國立清華大學 天文研究所 101 We observed one new transit of WAP-10b using a 46 cm telescope located at WISE Observatory in Israel, in order to search for transit timing variations (TTVs) which can be induced by the existing of the additional planets in the system. Employing 34 available light curves within about 3 yr, the transit timings and O-C diagram are obtained. We found a TTVs signal which has a period about 11d and an amplitude near 1 min with $\chi_{red}^{2}$ = 1.69 fitted to the O-C diagram. Comparing with no TTVs case, the WASP-10b rotates periodically with a linear ephemeris which corresponds to a $\chi_{red}^{2}$ value of 2.05. We also consider the TTV signal reported by Maciejewski et al.(2011a) which is inconsistent with our new-fitted data, $\chi_{red}^{2}$ = 10.07. Jiang, Ing-Guey 江瑛貴 2012 學位論文 ; thesis 45 en_US
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language en_US
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description 碩士 === 國立清華大學 === 天文研究所 === 101 === We observed one new transit of WAP-10b using a 46 cm telescope located at WISE Observatory in Israel, in order to search for transit timing variations (TTVs) which can be induced by the existing of the additional planets in the system. Employing 34 available light curves within about 3 yr, the transit timings and O-C diagram are obtained. We found a TTVs signal which has a period about 11d and an amplitude near 1 min with $\chi_{red}^{2}$ = 1.69 fitted to the O-C diagram. Comparing with no TTVs case, the WASP-10b rotates periodically with a linear ephemeris which corresponds to a $\chi_{red}^{2}$ value of 2.05. We also consider the TTV signal reported by Maciejewski et al.(2011a) which is inconsistent with our new-fitted data, $\chi_{red}^{2}$ = 10.07.
author2 Jiang, Ing-Guey
author_facet Jiang, Ing-Guey
Chien, Ping
簡屏
author Chien, Ping
簡屏
spellingShingle Chien, Ping
簡屏
Observations and Study of Transit Events in the Exoplanet System WASP-10
author_sort Chien, Ping
title Observations and Study of Transit Events in the Exoplanet System WASP-10
title_short Observations and Study of Transit Events in the Exoplanet System WASP-10
title_full Observations and Study of Transit Events in the Exoplanet System WASP-10
title_fullStr Observations and Study of Transit Events in the Exoplanet System WASP-10
title_full_unstemmed Observations and Study of Transit Events in the Exoplanet System WASP-10
title_sort observations and study of transit events in the exoplanet system wasp-10
publishDate 2012
url http://ndltd.ncl.edu.tw/handle/93732438859215351690
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