M. Siudek,1 A. Barnacka,2 M. Ćwiok,3 A. Majczyna,4 L. Mankiewicz,1 K. Malek,1 M. Sokołowski,4 A. F. Żarnecki3
1Ctr. for Theoretical Physics (Poland) 2Copernicus Astronomical Ctr. (Poland) 3Univ. of Warsaw (Poland) 4Andrzej Sołtan Institute for Nuclear Studies (Poland)
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One of the goals of "Pi of the Sky" project is to observe and analyze variable stars. In the second edition of variable
stars we have identified over 70 Cepheids, which we classified further analysis. We identified type of pulsation of these
stars using "Pi of the Sky" data collected since 2006. This paper describes analysis of Cepheids based on Fourier
decomposition, which is powerful method for classification purposes.
M. Siudek,A. Barnacka,M. Ćwiok,A. Majczyna,L. Mankiewicz,K. Malek,M. Sokołowski, andA. F. Żarnecki
"Analysis of Cepheids based on photometric data from the Pi of the Sky experiment", Proc. SPIE 7745, Photonics Applications in Astronomy, Communications, Industry, and High-Energy Physics Experiments 2010, 77450F (14 September 2010); https://doi.org/10.1117/12.872251
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M. Siudek, A. Barnacka, M. Ćwiok, A. Majczyna, L. Mankiewicz, K. Malek, M. Sokołowski, A. F. Żarnecki, "Analysis of Cepheids based on photometric data from the Pi of the Sky experiment," Proc. SPIE 7745, Photonics Applications in Astronomy, Communications, Industry, and High-Energy Physics Experiments 2010, 77450F (14 September 2010); https://doi.org/10.1117/12.872251