MIKULÁŠEK, Zdeněk, Ernst PAUNZEN, Martin NETOPIL and Miloslav ZEJDA. New Tools for Finding and Testing Weak Periodic Variability. In Kudryavtsev, D. O.; Balega, Yu. Yu.; Romanyuk, I. I. Physics and Evolution of Magnetic and Related Stars. 494th ed. San Francisco: Astronomical Society of the Pacific, 2015, p. 320-330. ISBN 978-1-58381-873-2.
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Basic information
Original name New Tools for Finding and Testing Weak Periodic Variability
Name in Czech Nové nástroje pro hledání a testování slabé periodické proměnnosti
Authors MIKULÁŠEK, Zdeněk (203 Czech Republic, guarantor, belonging to the institution), Ernst PAUNZEN (40 Austria, belonging to the institution), Martin NETOPIL (40 Austria, belonging to the institution) and Miloslav ZEJDA (203 Czech Republic, belonging to the institution).
Edition 494. vyd. San Francisco, Physics and Evolution of Magnetic and Related Stars, p. 320-330, 11 pp. 2015.
Publisher Astronomical Society of the Pacific
Other information
Original language English
Type of outcome Proceedings paper
Field of Study 10308 Astronomy
Country of publisher United States of America
Confidentiality degree is not subject to a state or trade secret
Publication form printed version "print"
RIV identification code RIV/00216224:14310/15:00080813
Organization unit Faculty of Science
ISBN 978-1-58381-873-2
UT WoS 000366452300040
Keywords in English periodograms
Tags AKR, rivok
Changed by Changed by: Ing. Andrea Mikešková, učo 137293. Changed: 28/4/2016 14:29.
Abstract
Our paper presents new methods for finding and testing weak periodic variability of stellar objects, developed for the purpose of detecting the expected regular light variations of magnetic chemically peculiar (mCP) candidates in the Large Magellanic Cloud. We introduce two new periodograms of the mCP star BS Cir (HD 125630), appropriate for rotating the spotted variables, and compare the results with those obtained by the well-known Lomb–Scargle periodogram. The use of periodograms and testing the significance of the found period candidates are demonstrated with two examples: the observed and simulated observations of the magnetic field of the mCP star CQ UMa (HD 119213) and the mCP candidate OGLE LMC136.7 16501. Three newly developed tests of periodic variability, namely the shuffling, bootstrap, and subsidiary ones, are presented. We demonstrate that the found periodic variations known with the signal-to-noise ratio larger than 6 can be approved to be real.
Links
GAP209/12/0217, research and development projectName: Multispektrální proměnnost horkých hvězd a její příčiny
Investor: Czech Science Foundation
3SGA5916, interní kód MUName: Hvězdy a hvězdokupy v Magellanových mračnech (Acronym: Webda MaC)
Investor: South-Moravian Region, Incoming grants
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