July 31, 2017 to August 3, 2017
Royal Observatory of Belgium
UTC timezone
<br>2nd LAMOST-Kepler workshop<br><br>LAMOST in the era of large spectroscopic surveys<P><img src="https://events.oma.be/indico/event/26/picture/0.jpg" width="466" height="50">

Asteroseismic analysis of selected High Amplitude Delta Scuti Candidates in the Kepler field

Aug 1, 2017, 12:40 PM
20m
Meridian Room (Royal Observatory of Belgium)

Meridian Room

Royal Observatory of Belgium

Av. Circulaire - 3 - Ringlaan 1180 Brussels
Contributed talk 2.3 The LAMOST as a large spectroscopic survey 2.3 The LAMOST as a large spectroscopic survey

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)

Presentation materials