Image Details
Caption: Figure 6.
Dispersion-corrected δOPDmeas plotted against the projected baseline component B∥ for the MJD = 60918 A–B sequence. B∥ is computed from the (u, v) coordinates via B∥ = (uΔα + vΔδ)/∣θ∣, where Δα and Δδ are the east and north components of θ = rA − rB. Each color denotes a baseline (W2 reference), and the black line is the best-fitting linear relation. For a fixed separation vector, δOPD scales linearly with B∥ (the component of the projected baseline along the A–B separation; using ∣B∣ would not yield a linear relation), so the alignment of the multibaseline points provides a direct consistency check on the OPD sign conventions and time matching. The residual scatter about the fit reflects the ∼0.37 μm effective OPD noise used in the bootstrap uncertainty estimate.
© 2026. The Author(s). Published by the American Astronomical Society.