Table 4: Polarization properties of the supernova remnants. The polarized intensity was corrected for noise bias (see text Sect. 3.2). The peak polarization in Col. 4 is an approximate value. SNRs with no detectable polarization were removed from the table.
\begin{displaymath}\begin{tabular}{lr@{$~\pm~$}lr@{$~\pm~$}lc}
\hline\hline
So...
...9 \\
G166.0$+$4.3&440&50&8.6&1.2&57 \\
\hline
\end{tabular}\end{displaymath}


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