Detailed Information on Publication Record
2014
Hi-fi phenomenological description of eclipsing binary light variations as the basis for their period analysis
MIKULÁŠEK, Zdeněk, Miloslav ZEJDA, Marek CHRASTINA, Shengbang QIAN, Liying ZHU et. al.Basic information
Original name
Hi-fi phenomenological description of eclipsing binary light variations as the basis for their period analysis
Name in Czech
Hi-fi fenomenologický popis změn jasnosti zákrytových dvojhvězd jako základ pro studium proměnnosti periody
Authors
MIKULÁŠEK, Zdeněk (203 Czech Republic, guarantor, belonging to the institution), Miloslav ZEJDA (203 Czech Republic, belonging to the institution), Marek CHRASTINA (703 Slovakia, belonging to the institution), Shengbang QIAN (156 China) and Liying ZHU (156 China)
Edition
Les Ulis (France), EAS Publications Series, Volume 64, 2013, p. 299-302, 4 pp. 2014
Publisher
EAS, EDP Sciences
Other information
Language
English
Type of outcome
Stať ve sborníku
Field of Study
10308 Astronomy
Country of publisher
France
Confidentiality degree
není předmětem státního či obchodního tajemství
Publication form
printed version "print"
References:
RIV identification code
RIV/00216224:14310/14:00081980
Organization unit
Faculty of Science
ISBN
978-2-7598-1161-8
ISSN
Keywords in English
photometry; modelling
Tags
International impact, Reviewed
Změněno: 11/3/2016 14:24, prof. RNDr. Zdeněk Mikulášek, CSc.
V originále
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.
In Czech
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.