L. Çelik, F. Ekmekçi, J. Nemec, K. Kolenberg, J. M. Benkő, R. Szabó, D. W. Kurtz, K. Kinemuchi, H. V. Şenavcı
One of the most challenging difficulties that precedes the frequency analysis
of {\it Kepler} data for a Blazhko star is stitching together the data from
different seasons (quarters). We discuss the preliminary steps in the
stitching, detrending and rescaling process using the data for long-term
Blazhko stars. We present the process on {\it Kepler} data of a Blazhko star
with a variable Blazhko cycle and some first results of our analysis.
View original:
http://arxiv.org/abs/1202.3607
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