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@inproceedings{1168437, author = {Mikulášek, Zdeněk and Zejda, Miloslav and Chrastina, Marek and Qian, Shengbang and Zhu, Liying}, address = {Les Ulis (France)}, booktitle = {EAS Publications Series, Volume 64, 2013}, doi = {http://dx.doi.org/10.1051/eas/1364041}, editor = {K. Pavlovski , A. Tkachenko and G. Torres}, keywords = {photometry; modelling}, howpublished = {tištěná verze "print"}, language = {eng}, location = {Les Ulis (France)}, isbn = {978-2-7598-1161-8}, pages = {299-302}, publisher = {EAS, EDP Sciences}, title = {Hi-fi phenomenological description of eclipsing binary light variations as the basis for their period analysis}, url = {http://www.eas-journal.org/article_S1633476064000412}, year = {2014} }
TY - JOUR ID - 1168437 AU - Mikulášek, Zdeněk - Zejda, Miloslav - Chrastina, Marek - Qian, Shengbang - Zhu, Liying PY - 2014 TI - Hi-fi phenomenological description of eclipsing binary light variations as the basis for their period analysis PB - EAS, EDP Sciences CY - Les Ulis (France) SN - 9782759811618 KW - photometry KW - modelling UR - http://www.eas-journal.org/article_S1633476064000412 L2 - http://www.eas-journal.org/article_S1633476064000412 N2 - In-depth analysis of eclipsing binary (EB) observational data collected for several decades can inform us about a lot of astrophysically interesting processes taking place in the systems. We have developed a wide-ranging method for the phenomenological modelling of eclipsing binary phase curves that enables us to combine even very disparate sources of phase information. This approach is appropriate for the processing of both standard photometric series of eclipses and data from photometric surveys of all kind. We conclude that mid-eclipse times, determined using the latest version of our "hi-fi" phenomenological light curve models, as well as their accuracy, are nearly the same as the values obtained using much more complex standard physical EB models. ER -
MIKULÁŠEK, Zdeněk, Miloslav ZEJDA, Marek CHRASTINA, Shengbang QIAN a Liying ZHU. Hi-fi phenomenological description of eclipsing binary light variations as the basis for their period analysis. In K. Pavlovski , A. Tkachenko and G. Torres. \textit{EAS Publications Series, Volume 64, 2013}. Les Ulis (France): EAS, EDP Sciences, 2014, s.~299-302. ISBN~978-2-7598-1161-8. Dostupné z: https://dx.doi.org/10.1051/eas/1364041.
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