Kwee-van Woerden. method: To use or not to use?
文献类型：会议论文
| 作者 | Mikulasek, Z.1,2; Chrastina, M.1; Liska, J.1; Zejda, M.;1; Janik, J.1; Zhu LY(朱俐颖)3,4 ; Qian SB(钱声帮)3,4
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| 出版日期 | 2014-03 |
| 会议名称 | Workshop on Observing Techniques, Instrumentation and Science for Metre-Class Telescopes |
| 会议日期 | 2013-09-23 |
| 会议地点 | Stara Lesna, SLOVAKIA |
| 关键词 | Kwee-van Woerden method |
| 卷号 | 43 |
| 期号 | 3 |
| 页码 | 382-387 |
| 通讯作者 | Mikulasek, Z (reprint author), Masaryk Univ, Dept Theoret Phys & Astrophys, Kotlarska 2, CZ-61137 Brno, Czech Republic |
| 英文摘要 | The credibility of orbital period analyses of eclipsing binaries strictly depends on the correctness of the observed mid-eclipse time determination, as well as the reliability of its uncertainty estimation. The majority of them have been determined by means of the Kwee-van Woerden method (KWM). There are also other possibilities - e.g. to use physical models of eclipsing binaries or light curve templates and to determine mid-eclipse times using the least square method (LSM). We compared results yielded by both methods by means of a computer simulation on the synthetic model of the AR Aur primary minimum. Minima times determined by the KWM and the exact LSM approach are nearly the same, while the scatter of LSM times is always smaller than the scatter of KWM times. KWM uncertainties are systematically underestimated. We think that the time is ripe for the Kwee-van Woerden method to retire. |
| 收录类别 | SCI ; CPCI |
| 产权排序 | 第三完成单位 |
| 会议网址 | http://adsabs.harvard.edu/abs/2014CoSka..43..382M |
| 会议录 | CONTRIBUTIONS OF THE ASTRONOMICAL OBSERVATORY SKALNATE PLESO
 |
| 会议录出版者 | SLOVAK ACADEMY SCIENCES ASTRONOMICAL INST, SLOVAK ACADEMY SCIENCES |
| 学科主题 | Astronomy & Astrophysics |
| 会议录出版地 | ASTRONOMICAL INST, TATRANSKA LOMINICA, SK-059 60, SLOVAKIA |
| 语种 | 英语 |
| ISSN号 | 1335-1842 |
| WOS记录号 | WOS:000338483100037 |
| 研究领域[WOS] | Astronomy & Astrophysics |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/9243]  |
| 专题 | 云南天文台_双星与变星研究组 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.Department of Theoretical Physics and Astrophysics, Masaryk University, Brno, Kotl´aˇrsk´a 2, CZ-611 37 Brno, Czech Republic 2.Observatory and Planetarium of Johann Palisa, VˇSB–Technical University, Ostrava, Czech Republic 3.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming, China 4.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming, China |
| 推荐引用方式 GB/T 7714 | Mikulasek, Z.,Chrastina, M.,Liska, J.,et al. Kwee-van Woerden. method: To use or not to use?[C]. 见:Workshop on Observing Techniques, Instrumentation and Science for Metre-Class Telescopes. Stara Lesna, SLOVAKIA. 2013-09-23.http://adsabs.harvard.edu/abs/2014CoSka..43..382M. |
入库方式： OAI收割
来源：云南天文台
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