The Chinese Small Telescope Array (CSTAR) is the first telescope facility built at Dome A, Antarctica. During the 2008 observing season, the installation provided long-baseline and high-cadence photometric observations in the i-band for 18145 targets within 20deg^2^ CSTAR field around the South Celestial Pole for the purpose of monitoring the astronomical observing quality of Dome A and detecting various types of photometric variability. Using sensitive and robust detection methods, we discover 274 potential variables from this data set, 83 of which are new discoveries. We characterize most of them, providing the periods, amplitudes, and classes of variability.

Cone search capability for table J/ApJS/218/20/variables (Catalog of variables in the CSTAR field: recovered (table1) and newly discovered (table2))

Cone search capability for table J/ApJS/218/20/table3 (Missed variables during our variability search)