Observations of Cepheids in Pi of the Sky experiment
2011
In this paper we present analysis of Cepheids using data obtained by the Pi of the Sky detector located
in Las Campanas Observatory in season 2006-2009. We have identified nearly 150 Cepheids classified as
classical, overtone or population II Cepheids. The calculation of Fourier parameters of Cepheid light curves
is described. In order to facilitate Fourier analysis we developed a new program capable to determine a
variability period and calculate Fourier coefficients. Additional program allow for automatic classification
of the variability type of Cepheid basing on neural network. Results of automatic classification of Cepheids
based on a neural network are shown.
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