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@inproceedings{1193741,
author = {Mikulášek, Zdeněk and Janík, Jan and Chrastina, Marek and Liška, Jiří and Zejda, Miloslav},
address = {Krakow},
booktitle = {Wykorzystanie malych teleskopow 2013},
editor = {Katarzyna Bajan and Krzysztof Ziolkowski},
keywords = {Kwee-van Woerden method},
howpublished = {tištěná verze "print"},
language = {eng},
location = {Krakow},
pages = {185-189},
publisher = {Uniwersytet Pedagogiczny w Krakowie and Polskie Towarzystwo Milosnikow Astronomii},
title = {Discussion of results obtained by the Kwee-van Woerden method},
year = {2014}
}
TY - JOUR
ID - 1193741
AU - Mikulášek, Zdeněk - Janík, Jan - Chrastina, Marek - Liška, Jiří - Zejda, Miloslav
PY - 2014
TI - Discussion of results obtained by the Kwee-van Woerden method
PB - Uniwersytet Pedagogiczny w Krakowie and Polskie Towarzystwo Milosnikow Astronomii
CY - Krakow
KW - Kwee-van Woerden method
N2 - The majority of mid-eclipse time determination has 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 ARAur 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.
ER -
MIKULÁŠEK, Zdeněk, Jan JANÍK, Marek CHRASTINA, Jiří LIŠKA a Miloslav ZEJDA. Discussion of results obtained by the Kwee-van Woerden method. In Katarzyna Bajan and Krzysztof Ziolkowski. \textit{Wykorzystanie malych teleskopow 2013}. Krakow: Uniwersytet Pedagogiczny w Krakowie and Polskie Towarzystwo Milosnikow Astronomii. s.~185-189. ISSN~1230-2295. 2014.
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