Extended Aperture Photometry of K2 RR Lyrae stars

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Publikace nespadá pod Filozofickou fakultu, ale pod Přírodovědeckou fakultu. Oficiální stránka publikace je na webu muni.cz.
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PLACHY Emese MOLNAR Laszlo BODI Attila SKARKA Marek SZABO Pal SZABO Robert) KLAGYIVIK Peter SODOR Adam POPE Benjamin J. S.

Rok publikování 2019
Druh Článek v odborném periodiku
Časopis / Zdroj ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
Fakulta / Pracoviště MU

Přírodovědecká fakulta

Citace
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Doi http://dx.doi.org/10.3847/1538-4365/ab4132
Klíčová slova ANOMALOUS CEPHEIDS; OGLE COLLECTION; MODE; CATALOG
Popis The Kepler Space Telescope observed thousands of RR Lyrae stars in the K2 mission. In this paper, we present our photometric solutions using extended apertures in order to conserve the flux of the stars to the highest possible extent. With this method, we are able to avoid most of the problems that RR Lyrae light curves produced by other pipelines suffer from. For post-processing, we apply the K2SC pipeline to our light curves. We provide the EAP (Extended Aperture Photometry) of 432 RR Lyrae stars observed in campaigns 3, 4, 5, and 6. We also provide subclass classifications based on Fourier parameters. We investigated in particular the presence of the Blazhko effect in the stars and found it to be 44.7% among the RRab stars, in agreement with results from independent samples. We found that the amplitude and phase modulation in the Blazhko stars may behave rather differently, at least over the length of a K2 Campaign. We also identified four anomalous Cepheid candidates in the sample, one of which is potentially the first Blazhko-modulated member of its class.
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