J 2016

Fine detrending of raw Kepler and MOST photometric data of KIC 6950556 and HD 37633

MIKULÁŠEK, Zdeněk, Ernst PAUNZEN, Miloslav ZEJDA, Evgenij SEMENKO, Klaus BERNHARD et. al.

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

Language

English

Type of outcome

Článek v odborném periodiku

Field of Study

10308 Astronomy

Country of publisher

Bulgaria

Confidentiality degree

není předmětem státního či obchodního tajemství

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

Tags

International impact, Reviewed
Změněno: 3/4/2019 14:11, RNDr. Jan Janík, Ph.D.

Abstract

V originále

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 project
Name: Ztráta hmoty horkých hmotných hvězd
Investor: Czech Science Foundation
LH14300, research and development project
Name: Výzkum zvláštních proměnných hvězd
Investor: Ministry of Education, Youth and Sports of the CR
3SGA5916, interní kód MU
Name: Hvězdy a hvězdokupy v Magellanových mračnech (Acronym: Webda MaC)
Investor: South-Moravian Region, Incoming grants