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This paper details the data reduction pipeline and initial results from the Antarctic TianMu Staring Observation Program, a time-domain optical sky survey. The project leverages the unique observing conditions of Antarctica for high-cadence sky surveys. The paper's significance lies in demonstrating the feasibility and performance of the prototype telescope, providing valuable data products (reduced images and a photometric catalog) and establishing a baseline for future research in time-domain astronomy. The successful deployment and operation of the telescope in a challenging environment like Antarctica is a key achievement.
Reference

The astrometric precision is better than approximately 2 arcseconds, and the detection limit in the G-band is achieved at 15.00~mag for a 30-second exposure.