The Observations and Analysis of Transit Events In the XO-1 Planetary System
碩士 === 國立清華大學 === 天文研究所 === 102 === We observed two newly transits of the XO-1 planetary system. The observations of one of these transit events are done by using the 46-cm telescope hosted by Wise Observatory in Israel. The observations of the other one are done by using both 104-cm and 130-cm tele...
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ndltd-TW-102NTHU51990022016-03-09T04:31:09Z http://ndltd.ncl.edu.tw/handle/57166637360335136176 The Observations and Analysis of Transit Events In the XO-1 Planetary System XO-1行星系統之凌星事件的觀測與研究 Lin, Yi-Ling 林怡伶 碩士 國立清華大學 天文研究所 102 We observed two newly transits of the XO-1 planetary system. The observations of one of these transit events are done by using the 46-cm telescope hosted by Wise Observatory in Israel. The observations of the other one are done by using both 104-cm and 130-cm telescopes located at ARIES in India. We investigate the possibility for the transit timing variations (TTVs) in the orbital period of XO-1b that may aroused by the existents of an additional planet in this system, so we collected 28 transits from public data and analyzed with our own data. After the O-C diagram of the XO-1 system is obtained and analyzed, we found that a null TTV produces a fit with χred2=2.1764. We also find that the ephemeris with a sinusoidal function of a frequency 0.483985 has a fit with χred2=1.7962 and the one of a frequency 0.10706 has a fit with χred2=2.0867. Jiang, Ing-Guey 江瑛貴 2014 學位論文 ; thesis 56 en_US |
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Others
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碩士 === 國立清華大學 === 天文研究所 === 102 === We observed two newly transits of the XO-1 planetary system. The observations of one of these transit events are done by using the 46-cm telescope hosted by Wise Observatory in Israel. The observations of the other one are done by using both 104-cm and 130-cm telescopes located at ARIES in India. We investigate the possibility for the transit timing variations (TTVs) in the orbital period of XO-1b that may aroused by the existents of an additional planet in this system, so we collected 28 transits from public data and analyzed with our own data. After the O-C diagram of the XO-1 system is obtained and analyzed, we found that a null TTV produces a fit with χred2=2.1764. We also find that the ephemeris with a sinusoidal function of a frequency 0.483985 has a fit with χred2=1.7962 and the one of a frequency 0.10706 has a fit with χred2=2.0867.
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author2 |
Jiang, Ing-Guey |
author_facet |
Jiang, Ing-Guey Lin, Yi-Ling 林怡伶 |
author |
Lin, Yi-Ling 林怡伶 |
spellingShingle |
Lin, Yi-Ling 林怡伶 The Observations and Analysis of Transit Events In the XO-1 Planetary System |
author_sort |
Lin, Yi-Ling |
title |
The Observations and Analysis of Transit Events In the XO-1 Planetary System |
title_short |
The Observations and Analysis of Transit Events In the XO-1 Planetary System |
title_full |
The Observations and Analysis of Transit Events In the XO-1 Planetary System |
title_fullStr |
The Observations and Analysis of Transit Events In the XO-1 Planetary System |
title_full_unstemmed |
The Observations and Analysis of Transit Events In the XO-1 Planetary System |
title_sort |
observations and analysis of transit events in the xo-1 planetary system |
publishDate |
2014 |
url |
http://ndltd.ncl.edu.tw/handle/57166637360335136176 |
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