Image Details
Caption: Figure 8.
The expected closure-phase signal from the known planet HIP 65426b is shown with cyan circles and the maroon lines are the measured closure phases from the observation. The smaller error bars are the statistical errors (calculated by measuring the scatter around the mean) and the larger error bars are the adopted errors (as discussed in Section 4.2).
© 2025. The Author(s). Published by the American Astronomical Society.