2025RAA....25d5004X

The Square Kilometre Array (SKA) has the potential to revolutionize astronomical research through its unparalleled precision. A critical aspect of SKA imaging is the computation of the UVW coordinates, which must be accurate and reliable for the development of the SKA scientific data processor. Katpoint is the current method used to calculate UVW in MeerKAT. Using a pseudo-source, we employ a simple cross-product method to determine UVWs. In this study, we explore the applicability of Katpoint for SKA1-low and SKA1-mid and evaluate its precision. The conventional method, CALC/OmniUV, and Katpoint were quantitatively assessed through simulations. The results indicate that Katpoint exhibits substantial accuracy with MeerKAT compared to traditional techniques. However, its precision is slightly inadequate for the long baselines of SKA1. We improved the precision of Katpoint by identifying optimal offset values for pseudo-sources on the SKA1 telescope through simulation, finding a 0$\mathop{.}\limits^{\unicode{x000B0}}$11 offset suitable for SKA1-Mid and a 0$\mathop{.}\limits^{\unicode{x000B0}}$045 offset for SKA1-Low. Final result validations demonstrate that these adjustments render the computational accuracy fully comparable to the standard CALC/OmniUV method, which would meet the requirements of SKA high-precision imaging and offer a solution for high-precision imaging in radio interferometers.