Notes. Nominal geocentric mid-time (Date, UT). Geocentric distances (Δ) and apparent sky-plane velocities (v) are evaluated at mid-event. Stellar angular diameters (θ_⋆) are those adopted in the light-curve modelling. S^a denotes the typical along-chord distance represented by a single photometric data point, combining exposure time with the apparent shadow velocity. ‘Chords’ refers to the total number of observing stations; ‘Positive’ indicates successful detections; ‘Negative’ indicates stations where no flux drop was recorded within the predicted window; and ‘Other’ includes stations affected by poor weather, technical problems, or incomplete/unreported observations. Detailed ingress and egress timings for all positive detections are listed in Table A.1. Star identifiers and NIMA solutions used for event predictions appear in Table 2.