Speaker
Dr
Ceren Ulusoy
(1.Girne American University, University Drive, PO Box 5, 99428 Karmi Campus, Karaoğlanoğlu, Kyrenia, Turkey 2.College of Graduate Studies, University of South Africa, PO Box 392, Unisa, 0003, Pretoria, South Africa)
Description
We present preliminary results on the analysis of the *Kepler* light curve of selected HADS candidates. Initially, *Kepler* data are used to derive frequency content of the variability of the stars. Then, the frequency analysis has been performed for each star using the software package SigSpeC (Reegen, 2007). The period ratios for the modes of highest amplitude are therefore discussed in the Petersen Diagram (Petersen, 1973).
Primary author
Dr
Ceren Ulusoy
(1.Girne American University, University Drive, PO Box 5, 99428 Karmi Campus, Karaoğlanoğlu, Kyrenia, Turkey 2.College of Graduate Studies, University of South Africa, PO Box 392, Unisa, 0003, Pretoria, South Africa)
Co-author
Dr
Burak Ulaş
(Izmir Turk College Planetarium, 8019/21 sok., No: 22, İzmir, Turkey)
