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Fig. 9

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Kp−Δυsys map of the pre-eclipse Fe signal, with the detection significance computed using a region where KP>210 km s−1 and Δυsys< − 40 km s−1, avoiding the planetary signal near the expected Kp and Δυsys. While choosing a different region reduced the detection significance to ≈5σ, Fe remains significantly detected, with the alpha detection significance constrained to be non-zero at more than 4.2σ, supporting the robustness of the Fe signal.

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