Precision Asteroseismology Proceedings IAU Symposium No. 301, 2013

• Main Authors: J. A. Guzik, W. J. Chaplin, A. Pigulski, J. N. Fu, W. K. Zong, Y. Yang, A. Moore, M. C. B. Ashley, X. Q. Cui, L. L. Feng, X. F. Gong, J. S. Lawrence, D. Luong-van, Q. Liu, C. R. Pennypacker, Z. H. Shang, J. W. V. Storey, L. Z. Wang, L. F. Wang, H. G. Yang, X. Y. Yuan, D. G. York, X. Zhou, Z. H. Zhu
• Other Authors: The Pennsylvania State University CiteSeerX Archives
• Format: Text
• Language: English
• Subjects: Antarc*; Antarctica
• Online Access: http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.637.4050; http://www.phys.unsw.edu.au/jacara/Papers/pdf/S1743921313014798a.pdf

Abstract. Gattini and CSTAR have been installed at Dome A, Antarctica, which provide time-series photometric data for a large number of pulsating variable stars. We present the study for several variable stars with the data collected with the two facilities in 2009 to demonstrate the scientific potential of observations from Dome A for asteroseismology. 1.