K. Vida
Eötvös Loránd University
8 Papers
15 Citations
K. Vida is an academic researcher from Eötvös Loránd University. The author has contributed to research in topics: Starspot & Light curve. The author has an hindex of 3, co-authored 8 publications. Previous affiliations of K. Vida include Hungarian Academy of Sciences & Konkoly Thege Miklós Astronomical Institute.
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Papers
Optical flares from the faint mid-dM star 2MASS J00453912+4140395
Zs. Kővári,Francesc Vilardell,Ignasi Ribas,K. Vida,K. Vida,L. van Driel-Gesztelyi,L. van Driel-Gesztelyi,L. van Driel-Gesztelyi,Carme Jordi,Carme Jordi,Katalin Oláh +10 more
TL;DR: In this article, the authors presented B and V light curves of a large stellar flare obtained with the Wide Field Camera at the Isaac Newton 2.5m telescope (La Palma).
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Superflares on the late-type giant KIC 2852961: Scaling effect behind flaring at different energy levels
Zs. Kővári,Katalin Oláh,Maximilian N. Günther,K. Vida,K. Vida,Levente Kriskovics,Levente Kriskovics,Bálint Seli,G. Á. Bakos,Joel D. Hartman,Z. Csubry,Waqas Bhatti +11 more
TL;DR: In this article, the authors analyzed the flaring activity of KIC 2852961, a late-type giant star, in order to understand how the flare statistics are related to that of other stars with flares and superflares and what the role of the observed stellar properties in generating flares is.
Superflares on the late-type giant KIC 2852961 -- Scaling effect behind flaring at different energy levels
Zs. Kővári,Katalin Oláh,Maximilian N. Günther,K. Vida,K. Vida,Levente Kriskovics,Levente Kriskovics,Bálint Seli,G. Á. Bakos,Joel D. Hartman,Z. Csubry,Waqas Bhatti +11 more
TL;DR: In this paper, the authors analyzed the flaring activity of KIC 2852961, a late-type giant star, in order to understand how the flare statistics are related to that of other stars with flares and superflares and what the role of the observed stellar properties in generating flares is.
Results of the photometry of the spotted dM1‐2e star EY Draconis
TL;DR: In this paper, the authors observed EY Draconis with the 60-cm telescope of Konkoly Observatory in Budapest for 64 nights and observed the evolution of the spotted stellar surface.
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