帳號:guest(3.145.50.222)          離開系統
字體大小: 字級放大   字級縮小   預設字形  

詳目顯示

以作者查詢圖書館館藏以作者查詢臺灣博碩士論文系統以作者查詢全國書目
作者(中文):李巧瑜
作者(外文):Lee, Chiao Yu
論文名稱(中文):Qatar-1b系外行星系統之凌星時間變化的觀測研究
論文名稱(外文):Investigating Transit Timing Variations of the Exoplanet System Qatar-1b
指導教授(中文):江瑛貴
指導教授(外文):Jiang, Ing Guey
口試委員(中文):陳林文
葉麗琴
口試委員(外文):Chen, Lin wen
Yeh, Li Chin
學位類別:碩士
校院名稱:國立清華大學
系所名稱:天文研究所
學號:103025504
出版年(民國):105
畢業學年度:104
語文別:英文
論文頁數:48
中文關鍵詞:Qatar-1b掩星現象系外行星transit timing variation
外文關鍵詞:Qatar-1btransitingexoplanettransit timing variation
相關次數:
  • 推薦推薦:0
  • 點閱點閱:223
  • 評分評分:*****
  • 下載下載:50
  • 收藏收藏:0
Qatar-1b 是一個被觀測到有掩星現象的系外行星,被曾經被宣稱這個系統可能有 transit timing variation (TTV)的訊號,或許是由於有其他的星體存在,在這個系外行星系統並對 Qatar-1b 的運行軌道造成影響而產生。所以我們收集了來自 Palomar 天文台及克里米亞天文台的 10 條掩星光變曲線,再加上從以前文獻上得到了,總共 40 條光變曲線作分析。我們使用 Transit Analysis Package (TAP) 來得到這個系統的軌道及恆星參數以及各自的誤差。接著把每次的掩星事件中心時間去擬合線性的函式,得到了 reduced χ 2 為 0.3938,並利用其結果和觀測值做比較,把這個差值拿去做週期性震盪的擬合,我們使用了三個可能的頻率,0.03881、0.02998 以及 0.00554,並分別得到了 reduced χ 2 為 4.02、3.643 以及 4.047。而我們考慮了這個擬合的錯誤機率(FAP),顯示沒有任何震幅大於 25 秒的週期性的 TTV 訊號存在其中。
Qatar-1b is a transiting exoplanet which was claimed with possible transit timing variation (TTV) in this system. We have obtained ten light curves from our observations using the Palomar Observatory and the Crimean Astrophysical Observatory, combined with the public data in literatures, there are 40 light curves in total. Transit Analysis Package (TAP) is a package we use to get refined system parameters and uncertainties. The null TTV produces a fit with χ2red = 3.938. The residuals of linear fitting to mid- transit time of each transit infer there might be possible TTV. We have used three possible frequencies, 0.03881, 0.02998 and 0.00554, to fit sinusoidal function and the result of χ2red are 4.02, 3.643 and 4.047. Then we also check the false alarm probability of the frequencies, and it shows that there is no evidencd for periodic TTVs with a amplitude more than abou 25 seconds.
1 Introduction 6
2 Observation and Data Reduction 8
2.1 TheObservatoryandTelescopes ................................ 8
2.1.1 PalomarObservatory .................................. 8
2.1.2 CrimeanAstrophysicalObservatory .......................... 9
2.2 ObservationandDataReduction ................................ 10
2.2.1 DataCalibration..................................... 10
2.2.2 SelectionofComparisonStar .............................. 11
2.2.3 TheNormalizationofLightCurves........................... 12
2.3 LightCurvesfromtheLiterature ................................ 13
3 The Analysis of Light Curves 16
3.1 InitialValuesofthePlanetarySystemParameters ...................... 16
3.2 TheResultsofLightCurveModeling.............................. 18
4 Timing Analysis 30
4.1 NewEphemeris.......................................... 30
4.2 FrequencyAnalysis........................................ 33
5 The Summary
A The Figures of Normalized Results
Alsubai, K. A., Parley, N. R., Bramich, D. M., et al. 2011, MNRAS, 417, 709 Carter, J. A., & Winn, J. N. 2009, ApJ, 704, 51
Claret, A., & Bloemen, S. 2011, A&A, 529, A75
Covino, E., Esposito, M., Barbieri, M., et al. 2013, A&A, 554, A28
Eastman, J., Gaudi, B. S., & Agol, E. 2013, PASP, 125, 83
Gazak, J. Z., Johnson, J. A., Tonry, J., et al. 2012, Advances in Astronomy, 2012, 697967
Jiang, I.-G., Lai, C.-Y., Savushkin, A., et al. 2016, AJ, 151, 17
Maciejewski, G., Dimitrov, D., Neuh ̈auser, R., et al. 2011, MNRAS, 411, 1204
Maciejewski, G., Fern ́andez, M., Aceituno, F. J., et al. 2015, A&A, 577, A109
Mandel, K., & Agol, E. 2002, ApJ, 580, L171
Mu ̈ller, H. M., Huber, K. F., Czesla, S., Wolter, U., & Schmitt, J. H. M. M. 2013, A&A, 560, A112 Murgas, F., Pall ́e, E., Zapatero Osorio, M. R., et al. 2014, A&A, 563, A41
Press, W. H., & Rybicki, G. B. 1989, ApJ, 338, 277
von Essen, C., Schr ̈oter, S., Agol, E., & Schmitt, J. H. M. M. 2013, A&A, 555, A92
 
 
 
 
第一頁 上一頁 下一頁 最後一頁 top
* *