Discussion of resuts obtained by the Kwee-van Woerden method

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F14%3A00076042" target="_blank" >RIV/00216224:14310/14:00076042 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Result language
angličtina
Original language name
Discussion of resuts obtained by the Kwee-van Woerden method
Original language description
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.
Czech name
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Czech description
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Project
<a href="/en/project/7AMB13PL019" target="_blank" >7AMB13PL019: Variables in Open Clusters and Their Vicinities</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2014
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection
Wykorzystanie malych teleskopow 2013
ISBN
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ISSN
1230-2295
e-ISSN
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Number of pages
5
Pages from-to
185-189
Publisher name
Uniwersytet Pedagogiczny w Krakowie and Polskie Towarzystwo Milosnikow Astronomii
Place of publication
Krakow
Event location
Koninki
Event date
May 10, 2014
Type of event by nationality
EUR - Evropská akce
UT code for WoS article
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