PITL. Violin plots depict the distribution of the centroid’s 1-sigma spread in pixels for isolated, semi-isolated, and contaminated stars in both IFSW and DRP datasets. For isolated stars, a bimodal distribution is evident, characterised by a peak around 0.3 arcseconds shared by both IFSW and DRP, and a secondary peak with larger/smaller values for IFSW and DRP, respectively. The shared peak can be attributed to visits with exposure times exceeding 24 seconds, while the discrepancies in the two datasets are due to very high-cadence observations with stacking in the case of DRP, effectively enhancing precision.