\begin{table}%t3
\caption{Fit parameters describing the shape of the spectra (low-frequency spectral index, break frequency, cutoff frequency)  shown in Fig.~\ref{f:ana.fits.obs1}.}\label{t:ana.fits.fitpars} 
%%\centerline
\par
{
\begin{tabular}{lrr|rll|rll}
\hline\hline
 & & & \multicolumn{3}{c}{Model A} & \multicolumn{3}{c}{Model B/HS} \\
Location & $r^a$ &  $\delta_{y}$$^b$ & $\alpha_{{\rm low}} $  & \nub  &
\nuc$^c$  & $\alpha_{{\rm low}} $  & \nub  & \nuc \\
 & \arcsec & \arcsec & & Hz & Hz & & Hz & Hz \\
\hline
A & 13.0 & 0.0 & $-$0.35 & $1.83\times 10^{10}$ & $1.83\times
 10^{16}$ $\dagger$ & \ldots & \ldots & \ldots \\
A-B1 & 13.7 & 0.0 & $-$0.38 & $2.25\times 10^{9}$ & $2.25\times 10^{15}$ & $-$0.38 & $2.15\times 10^{9}$ & $2.15\times 10^{15}$ \\
B1 & 14.2 & 0.1 & $-$0.35 & $7.13\times 10^{9}$ & $7.14\times 10^{15}$
 $\dagger$ &  \ldots & \ldots & \ldots \\
B2 & 15.2 & $-$0.1 & $-$0.44 & $2.78\times 10^{11}$ & $3.81\times
 10^{16}$ $\dagger$ &  \ldots & \ldots & \ldots \\
B3 & 15.6 & $-$0.1 & $-$0.48 & $2.71\times 10^{11}$ & $3.34\times 10^{16}$ & $-$0.46 & $1.98\times 10^{11}$ & $2.38\times 10^{16}$ \\
B3-C1 & 16.3 & 0.0 & $-$0.38 & $3.12\times 10^{9}$ & $3.13\times 10^{15}$ & $-$0.35 & $1.36\times 10^{9}$ & $1.36\times 10^{15}$ \\
C1 & 16.8 & 0.1 & $-$0.39 & $1.65\times 10^{10}$ & $5.24\times 10^{15}$ & $-$0.38 & $1.59\times 10^{10}$ & $3.74\times 10^{15}$ \\
C1-C2 & 17.3 & 0.0 & $-$0.37 & $1.45\times 10^{11}$ & $4.42\times 10^{14}$ & $-$0.35 & $1.35\times 10^{11}$ & $3.67\times 10^{14}$ \\
C2 & 17.7 & 0.0 & $-$0.36 & $2.86\times 10^{10}$ & $9.38\times 10^{14}$ & $-$0.35 & $3.07\times 10^{10}$ & $8.19\times 10^{14}$ \\
C2-D1 & 18.3 & 0.2 & $-$0.49 & $2.39\times 10^{10}$ & $7.88\times 10^{15}$ & $-$0.35 & $8.65\times 10^{9}$ & $5.46\times 10^{14}$ \\
D1 & 18.9 & 0.1 & $-$0.48 & $1.06\times 10^{10}$ & $4.34\times 10^{15}$ & $-$0.35 & $9.58\times 10^{8}$ & $4.65\times 10^{14}$ \\
D1-D2 & 19.5 & $-$0.2 & $-$0.35 & $4.62\times 10^{9}$ & $3.16\times 10^{14}$ & $-$0.35 & $5.78\times 10^{9}$ & $3.23\times 10^{14}$\\
D2 & 19.8 & $-$0.2 & $-$0.35 & $7.92\times 10^{9}$ & $5.26\times 10^{14}$ & $-$0.35 & $9.27\times 10^{9}$ & $5.15\times 10^{14}$ \\
H3 & 20.2 & $-$0.3 & $-$0.39 & $2.20\times 10^{9}$ & $8.75\times 10^{14}$ & $-$0.35 & $1.08\times 10^{9}$ & $5.10\times 10^{14}$ \\
H2 & 21.3 & 0.0 & \ldots & \ldots & \ldots & $-$0.60 & $1.14\times 10^{10}$ & $7.50\times 10^{14}$ \\
H1 & 22.1 & $-$0.2 & \ldots & \ldots & \ldots & $-$0.44 & $2.28\times 10^{9}$ & $5.79\times 10^{13}$ \\
\hline
\end{tabular}}
\medskip
$^a$ Distance along radius vector.  \\
$^b$ Distance from the radius vector; negative offsets are to the south.  \\
$^c$ The $\dagger$ mark indicates locations where there is no cutoff to
 the optical spectrum in the observed range and the value given is a lower limit to the true
 cutoff frequency. Both fits are identical in this case.  
\end{table}