support from the National Natural Science Foundation of China(NSFC,Grant No.11273051);partially supported by the Chinese Academy of Sciences(CAS) “Light of West China” program(2015-XBQN-A-02);supported by the Strategic Priority Research Program of CAS(Grant No.XDB23040100);support from the Joint Fund of Astronomy of NSFC and CAS(Grant U1231202 and 11673003);the National Basic Research Program of China(973 Program 2014CB845700 and 2013CB834900);the LAMOST FELLOWSHIP supported by Special Funding for Advanced Users,budgeted and administrated by the Center for Astronomical MegaScience,Chinese Academy of Sciences(CAMS);support from the NSFC(No.11403088)
We present a study on pulsations of the high-amplitudeδScuti star YZ Boo based on photometric observations in Johnson V and R bands with both the Nanshan 1-m telescope of Xinjiang Astronomical Observatory(XAO)and t...
Supported by the National Natural Science Foundation of China (Grant No. U1231202);partially supported by the National Basic Research Program of China (973 Program, 2013CB834900);the Fundamental Research Funds for Central Universities
Time-series photometric observations were made for the high amplitudeδScuti star CW Ser between 2011 and 2012 at the Xinglong Station of National Astronomical Observatories,Chinese Academy of Sciences.After performin...