Top: A comparison of the measured Faraday depths for the 51 sources present in both our catalog and the Taylor et al. (2009) catalog. The diagonal line marks 1:1 correspondence. The errors in our measured Faraday depth are almost always much smaller than the symbol size. Bottom: The distribution of Faraday depths for our catalog and the Taylor et al. (2009) catalog. The absence of sources near 0 rad m⁻² in our catalog is due to our procedure of ignoring the Faraday depths very close to the instrumental leakage.