Image Details
Caption: Figure 3.
Error distributions (normalized by reported uncertainty) in the Faraday depth (left panels), polarized intensity (center panels), and derotated polarization angle (right panels), for RM-synthesis (top row) and QU-fitting (bottom row). All distributions appear to be well described by a Gaussian of unit width (dashed lines)
© 2026. The Author(s). Published by the American Astronomical Society.