\begin{table}%t1
\caption{\label{tab:results}Source properties and results.}
\small%\centerline
{
\begin{tabular}{lllllllll}
\hline
\hline
Source Name &RA& Dec & Beam size & $\sigma_{{\rm rms}}$ & $S_{610}^{j, k}$   &$\alpha_{74~{\rm MHz}}^{1400~{\rm MHz}}$ & LAS$^{h}$ & Redshift \\
                         & (J2000)& (J2000)& arcsec        &  $\mu$Jy  &  mJy              &  & arcsec & $z$ \\
\hline\noalign{\smallskip}
VLSS J0004.9$-$3457 &00 04 53.63 &$-$34 56 34.1  & 11.4 $\times$ 6.6 & 73&$158 \pm 16$&$-1.40 \pm 0.04$ &116 & $0.29 \pm 0.08^{a}$\\  
VLSS J0227.4$-$1642  &  02 27 26.74  &  $-$16 42 47.2     & 5.3 $\times$ 4.0 &  94    &  $37.0 \pm 6.2$ &$-1.50 \pm 0.06$ &89 &$\ga$$0.7$ \\ %s1
VLSS J0250.5$-$1247 & 02 50 30.83   &  $-$12 47 30.3 &   9.4 $\times$ 3.7 &  118   & $33.2 \pm 3.3 $    &$-1.94 \pm 0.07$&21 &$\ga$$0.7$ \\%s2
VLSS J0511.6+0254     &05 11 37.79 &+02 54 19.4 & 8.7 $\times$ 6.1& 139& $98.0 \pm 10.3$ & $-1.42 \pm 0.05$& 45 & $ 0.20 \pm 0.05^{a}$\\  
VLSS J0516.2+0103     &05 16 17.89 &+01 03 40.1 & 8.1 $\times$ 6.5 &79&$17.4 \pm 4.4 $& $-1.73 \pm 0.06$& 35 & $\ga$$0.7$\\  
VLSS J0646.8$-$0722 &06 46 52.10   &  $-$07 22 37.9    & 5.7  $\times$ 4.8&  63  &   $120\pm 13$     &$-1.70 \pm 0.05$ & 59& $0.23 \pm 0.06^{a}$\\ %s3 
VLSS J0717.5+3745$^{i}$    &07 17 30.92 &+37 45 29.7 & 8.2 $\times$ 6.0 &78& $501 \pm 50 $&$-1.15 \pm 0.04$ & 171 & 0.5548$^{f}$ \\  
VLSS J0915.7+2511$^{i}$    & 09 15 41.51& +25 11 48.2  & 8.6 $\times$5.9 &134&  $194  \pm 21$  &$-1.52 \pm 0.04$ & 63 &$0.324^{c}$ \\%\pm 0.00020^{c}$ \\ %S22
VLSS J1117.1+7003  & 11 17 06.46   &     +70 03 57.1   & 7.8 $\times$ 4.3 &  52  &  $9.1 \pm 0.9$  &$-1.87 \pm 0.07$ &18 &$\ga$$0.7$ \\  %s4
VLSS J1133.7+2324  & 11 33 44.73 &+23 24 50.6&6.6 $\times$ 3.9& 51 &    $80.6 \pm 10.1$&$-1.69 \pm 0.06$ &84 & $0.61 \pm 0.16^{d}$\\  
VLSS J1431.8+1331  &  14 31 49.90 &+13 31 54.1&5.3  $\times$ 4.8 & 51  & $120 \pm 13$    &$-2.03 \pm 0.05$ &101 & $0.159936^{c}$ \\ % \pm 0.000182^{c}$  \\ %s6 
VLSS J1515.1+0424$^{i}$    &  15 15 09.18 &+04 24 41.1 &7.6 $\times$ 5.4&79 & $192 \pm 33$& $-1.50 \pm 0.05$& 169 & 0.0972$^{g}$ \\  
VLSS J1636.5+3326  &16 36 34.93 &+33 26 33.9& 5.2 $\times$ 4.7 & 40 &   $16.1 \pm 1.9$  &$-1.84 \pm 0.14$& 28&$0.65 \pm 0.19^{d}$\\  %s7
VLSS J1710.5+6844  &17 10 35.03 &+68 44 58.4  & 8.9 $\times$ 4.7 & 63  & $ 23.3 \pm 2.8 $ &$-1.75 \pm 0.06$ &45&$0.28 \pm 0.08^{a}$ \\  %s8
VLSS J1930.4+1048  &19 30 27.19 &+10 48 02.5  & 5.3 $\times$ 4.8 & 56 &  $67.4 \pm 7.0 $  & $-1.90 \pm 0.06$    &101  &   \ldots     \\  %s9
VLSS J2043.9$-$1118  &20 43 58.46 &$-$11 18 45.6 & 5.8 $\times$ 4.2  &  77 &  $53.9 \pm 6.3$  &$-1.74 \pm0.05$ &41 & $0.43 \pm 0.15^{b}$ \\  %s10
VLSS J2044.7+0447  & 20 44 43.64 &+04 47 24.5  &10.5 $\times$ 7.5 & 202 &  $57.7 \pm 5.8  $ & $-1.55 \pm 0.06$&71 & $0.46 \pm 0.15^{b}$  \\  % 180 rms S11
VLSS J2122.9+0012  & 21 22 54.14 &+00 12 03.4  & 5.8 $\times$ 3.8  & 81  & $24.0 \pm 2.4$  & $-2.00 \pm 0.08$&12 &$\ga$$1.4$ \\ %s12, R_vega = r -0.16 
VLSS J2209.5+1546   &22 09 32.91& +15 46 29.9 &6.9 $\times$ 6.2 & 64& $36.4 \pm 3.8$ & $-1.56 \pm 0.07$ & 61 & $\ga$$0.7$\\  
VLSS J2213.2+3411  & 22 13 12.45 &+34 11 51.6   & 5.5 $\times$  4.6 & 94 &  $127 \pm 13$   &$-1.55 \pm 0.04$ &62&$1.6 \pm 0.5^{a, e}$\\   
VLSS J2217.5+5943  & 22 17 30.39 &+59 43 05.3  & 6.3 $\times$ 4.3 & 47  &  $79.9 \pm 8.0$  & $-2.20 \pm 0.06$   &   99&   \ldots     \\  %s14
VLSS J2229.1$-$0136  &22 29 11.95 &$-$01 36 58.8 & 8.6 $\times$  4.2 & 101 &   \ldots   & \ldots  &   \ldots   & \ldots   \\  
VLSS J2241.3$-$1626  & 22 41 22.57& $-$16 25 35.7  &6.1 $\times$ 5.8&129 &$69.7 \pm 7.3$ &$-1.44 \pm 0.06$ & 47 &  $\ga$$0.7$\\  
VLSS J2341.1+1231  &23 41 06.91 &+12 31 36.9  & 5.5 $\times$ 4.4  & 50  & $117  \pm 14$  & $-1.70 \pm 0.04$&115&$0.62 \pm 0.15^{b}$  \\  %s16
VLSS J2345.2+2157  & 23 45 15.47& +21 57 55.1  & 4.8 $\times$ 4.2 & 63 &   $79.3 \pm 8.4$   &$-2.14 \pm 0.05$ &70&$0.23 \pm 0.06^{a}$\\  
VLSS J2357.0+0441     &23 57 05.54 &+04 41 14.7&7.8 $\times$ 4.9&82& \ldots  & \ldots  & \ldots & \ldots\\   
\hline
\end{tabular}}
\smallskip
$^{a}$ Redshift estimated using the fitted Hubble-K relation from \cite{2003MNRAS.339..173W}.\\
$^{b}$ Redshift estimated using the fitted Hubble-R relation from \cite{2007AetA...464..879D}. \\
$^{c}$ Spectroscopic redshift from SDSS DR7.\\
$^{d}$ Median photometric redshift from SDSS DR7.\\
$^{e}$ Using the $K_{\rm s}$ band magnitude from \cite{2002AJ....123..637D}.\\
$^{f}$  \cite{2003MNRAS.339..913E}.\\
$^{g}$  \cite{1999ApJS..125...35S}.\\
$^{h}$ LAS = largest angular size.\\
$^{i}$ Resolved out in the 1.4~GHz FIRST survey.\\
$^{j}$ Fluxes are extracted from the regions indicated in the figures by dotted lines. \\
$^{k}$ For the compact sources (LAS $< 45\arcsec$) the fluxes were measured by fitting single Gaussians to the sources after convolving the maps to the 45\arcsec\  NVSS resolution.\\
\end{table}