Abstract: The Wide Field Survey Telescope (WFST) is located at 4200 m on Saishiteng Mountain in Lenghu, Qinghai Province, China. It features a primary mirror with a diameter of 2.5 m and a camera equipped with nine CCDs, providing a wide field of view of approximately 3\times 3 square degrees. Calibration parameters are essential to ensure the precision of astrometric observations with the WFST. These parameters are derived from geometric distortion (GD) and gaps through astrometric modeling and are subsequently validated via the Yao’An High Precision Telescope (YAHPT). The GD solutions show maximum distortions between 1.18 and 10.29 pixels for the WFST chips, with central chips exhibiting lower distortion. After applying the GD correction, the precision of the WFST reaches 4 mas. The interchip gaps of the WFST range from 1.922 mm to 7.765 mm, corresponding to 10 μm/pixel, aligning with the design and measurements. The calibrated parameters guarantee that the WFST can perform highly accurate astrometric measurements. Furthermore, as the WFST undergoes updates, the parameter model remains consistently applicable.