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Kwee-van Woerden. method: To use or not to use?
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
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
会议录出版地ASTRONOMICAL INST, TATRANSKA LOMINICA, SK-059 60, SLOVAKIA
学科主题Astronomy & Astrophysics
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
内容类型会议论文
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.
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