Image Details
Caption: Figure 9.
The measured polarization angle of the fixed sparse wire grid calibrator as a function of telescope elevation with and without correction of ϕi. The solid black line shows the expected shift of polarization angle due to ϕi. Without correction, the measured polarization angle rotates depending on elevation. The measured polarization angle after correction is almost constant with elevation. This measurement was conducted with SAT3.
© 2026. The Author(s). Published by the American Astronomical Society.