"The aim of this project was to obtain precise photometric measurements of selected eclipsing binaries and stars with exoplanets. Solving it we published 2 articles and presented 6 contributions on seminars and conferences."@en . . "MEB050819" . "2010-06-30+02:00"^^ . . . . "Hlavn\u00EDm odborn\u00FDm c\u00EDlem projektu je prov\u00E1d\u011Bt fotometrick\u00E9 studium vybran\u00FDch z\u00E1krytov\u00FDch dvojhv\u011Bzd a hv\u011Bzd s exoplanetami. P\u0159esn\u00E1 fotometrick\u00E1 pozorov\u00E1n\u00ED budeme prov\u00E1d\u011Bt hlavn\u011B na observato\u0159i Krakovsk\u00E9 pedagogick\u00E9 univerzity na Suho\u0159e. Tato data spolu se spektroskopick\u00FDmi m\u011B\u0159en\u00EDmi z\u00EDskan\u00FDmi na David Dunlap Observatory (Kanada) budou zpracov\u00E1na s pou\u017Eit\u00EDm nov\u00FDch metod zpracov\u00E1n\u00ED (PCA, v\u00E1\u017Een\u00E1 robustn\u011B regrese apod.). Pak sestroj\u00EDme model studovan\u00E9ho syst\u00E9mu s pomoc\u00ED programu Phoebe. D\u016Fle\u017Eitou sou\u010D\u00E1st\u00ED projektu je prezentace na\u0161ich v\u00FDsledk\u016F v publikac\u00EDch a na konferenc\u00EDch. T\u00E9\u017E zorganizujeme kr\u00E1tkou konferenci pro n\u00E1\u0161 t\u00FDm a jeho spolupracovn\u00EDky z \u0159ad student\u016F v\u011Bnovan\u00FD metod\u00E1m spr\u00E1vn\u00E9ho zpracov\u00E1n\u00ED pozorovac\u00EDch dat." . "1"^^ . . "binary stars" . . . "2009-12-31+01:00"^^ . . "3"^^ . . "0"^^ . "C\u00EDlem projektu bylo po\u0159\u00EDdit p\u0159esn\u00E1 fotometrick\u00E1 m\u011B\u0159en\u00ED vybran\u00FDch z\u00E1krytov\u00FDch dvojhv\u011Bzd a hv\u011Bzd s exoplanetami. P\u0159i jeho \u0159e\u0161en\u00ED jsme publikovali 2 \u010Dl\u00E1nky a p\u0159ednesli 6 p\u0159\u00EDsp\u011Bvk\u016F na semin\u00E1\u0159\u00EDch a konferenc\u00EDch."@cs . "3"^^ . . "http://www.isvav.cz/projectDetail.do?rowId=MEB050819"^^ . . . "binary stars; stellar characteristics; observation; data processing"@en . " observation" . "The main scientific aim of the project is to do photometric study of selected eclipsing binaries and stars with exoplanets. Precise photometric measurements will be made mainly at Mt. Suhora observatory (Cracow Pedagogical University). These data together with spectroscopic observations obtained on David Dunlop Observatory will be processed using new methods of data processing (PCA, weighted robust regression...). Then we build the model of studied system by the help of Phoebe code. The essential part of the project is presentation of our result in papers, on conferences. We also organize a short workshop for our team and collaborators (students) devoted to the method of correct processing of observational data."@en . "0"^^ . . . "2008-01-01+01:00"^^ . . . "Binarity - a tool for study of stellar characteristics"@en . . "2009-03-09+01:00"^^ . " stellar characteristics" . "Dvojhv\u011Bzdnost - n\u00E1stroj pro studium hv\u011Bzdn\u00FDch charakteristik" .