Observed occultation chords (black line segments) from the March 3, 2024 event, projected onto the sky plane, together with the best-fit non-convex ADAM shape model of asteroid Oersted (gray silhouette) at the corresponding rotational phase. Each chord represents the stellar disappearance and reappearance as seen from a specific observer location listed in Table 1. The model silhouette is scaled and oriented to minimize residuals between the chord endpoints and the projected shape boundary. The close match demonstrates the validity of the shape and spin solution.