MIKULÁŠEK, Zdeněk, Ernst PAUNZEN, Miloslav ZEJDA, Evgenij SEMENKO, Klaus BERNHARD, Stefan HUMMERICH, Jia ZHANG, Swetlana HUBRIG, Rainer KUSCHNIG, Jan JANÍK and Miroslav JAGELKA. Fine detrending of raw Kepler and MOST photometric data of KIC 6950556 and HD 37633. Bulgarian Astronomical Journal. Sofia: Institute of Astronomy, Bulgarian Academy of Sciences, 2016, vol. 25, summer, p. 19-26. ISSN 1313-2709.
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Basic information
Original name Fine detrending of raw Kepler and MOST photometric data of KIC 6950556 and HD 37633
Name in Czech Jemné detrendování surových fotometrických dat KIC 6950556 a HD 37633 z družic Kepler a MOST
Authors MIKULÁŠEK, Zdeněk (203 Czech Republic, guarantor, belonging to the institution), Ernst PAUNZEN (40 Austria, belonging to the institution), Miloslav ZEJDA (203 Czech Republic, belonging to the institution), Evgenij SEMENKO (643 Russian Federation), Klaus BERNHARD (276 Germany), Stefan HUMMERICH (276 Germany), Jia ZHANG (156 China, belonging to the institution), Swetlana HUBRIG (276 Germany), Rainer KUSCHNIG (40 Austria), Jan JANÍK (203 Czech Republic, belonging to the institution) and Miroslav JAGELKA (703 Slovakia, belonging to the institution).
Edition Bulgarian Astronomical Journal, Sofia, Institute of Astronomy, Bulgarian Academy of Sciences, 2016, 1313-2709.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher Bulgaria
Confidentiality degree is not subject to a state or trade secret
RIV identification code RIV/00216224:14310/16:00088324
Organization unit Faculty of Science
UT WoS 000413255500002
Keywords (in Czech) zpracování dat; fotometrie z Keplera a MOSTu;chemicky pekuliární hvězdy; jednotlivé hvězdy: KIC 6950556; HD 37633
Keywords in English data processing; Kepler and MOST photometry; chemically peculiar stars; stars individual: KIC 6950556; HD 37633
Tags AKR
Tags International impact, Reviewed
Changed by Changed by: RNDr. Jan Janík, Ph.D., učo 17241. Changed: 3/4/2019 14:11.
Abstract
We present a simple phenomenological method for detrending of raw Kepler and MOST photometry, which is illustrated by means of photometric data processing of two periodically variable chemically peculiar stars, KIC 6950556 and HD 37633. In principle, this method may be applied to any type of periodically variable objects and satellite or ground based photometries. As a by product, we have identified KIC 6950556 as a magnetic chemically peculiar star with an ACV type variability.
Links
GA13-10589S, research and development projectName: Ztráta hmoty horkých hmotných hvězd
Investor: Czech Science Foundation
LH14300, research and development projectName: Výzkum zvláštních proměnných hvězd
Investor: Ministry of Education, Youth and Sports of the CR
3SGA5916, interní kód MUName: Hvězdy a hvězdokupy v Magellanových mračnech (Acronym: Webda MaC)
Investor: South-Moravian Region, Incoming grants
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