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

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F16%3A00088324" target="_blank" >RIV/00216224:14310/16:00088324 - isvavai.cz</a>

  • Result on the web

  • DOI - Digital Object Identifier

Alternative languages

  • Result language

    angličtina

  • Original language name

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

  • Original language description

    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.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Others

  • Publication year

    2016

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Bulgarian Astronomical Journal

  • ISSN

    1313-2709

  • e-ISSN

  • Volume of the periodical

    25

  • Issue of the periodical within the volume

    summer

  • Country of publishing house

    BG - BULGARIA

  • Number of pages

    8

  • Pages from-to

    19-26

  • UT code for WoS article

  • EID of the result in the Scopus database

    2-s2.0-84961279294