\begin{table}%t1
%\centering
\par
\caption{\label{tab,evn}The parsec-scale structure of Arp 299-A as imaged with the EVN.} 
\begin{tabular}{llcclrrl}
\hline \hline\noalign{\smallskip}
Source & Source & $\Delta~\alpha$\tablefootmark{a} & $\Delta~\delta$\tablefootmark{a} &
Angular size\tablefootmark{b} & $S_{1.7}$ ($\mu$Jy) \tablefootmark{c} 
&$S_{5.0}$ ($\mu$Jy)\tablefootmark{c}&Spectral index  \\
name&type&(J2000.0)&(J2000.0)& (milliarcsec)&&&$\alpha_{1.7}^{5.0}$ \\[1mm]
 \hline 
A0  & SN & 33.6213 & 46.707 & $\leq$$ 4.1\times4.0$ & $\leq$75 & $307 \pm 27$ &  $\geq$1.28  \\
A1   &   AGN (core)    & 33.6199 & 46.699 & $\leq$$6.1\times 2.7$  & $822 \pm 48$ & $716 \pm 42$ & --$0.13 \pm 0.11$\\
A1b &  AGN (jet) & 33.6190 & 46.699 & $\leq$$10.1\times 5.1$  & $314 \pm 30$ & $\leq$66 &  $\leq$--1.42  \\
A1c &  AGN (jet)     & 33.6183 & 46.695 &  $\leq$$14.3 \times 6.2$
& $267 \pm 28$ &  $\leq$66 & $\leq$--1.27 \\
A5  &   AGN (jet) & 33.6176 & 46.694 & $\leq$$6.9 \times 5.0$     &$246 \pm 28$  & $183 \pm 24$  &  --$0.27 \pm 0.22$ \\
\hline
\end{tabular}
\tablefoot{\tablefoottext{a}{Coordinates are given with respect
  to $\alpha$~=~11:28:00.0000 and $\delta$ =
  58:33:00.000, and the typical uncertainty is less than 1~mas;}
  \tablefoottext{b}{upper limits to the deconvolved angular size (Major axis $\times$ Minor axis, in mas) as obtained using  task IMFIT within AIPS, using our 5.0~GHz for all components but A1b and A1c, which were only detected at 1.7~GHz;}
  \tablefoottext{c}{the uncertainty in the reported flux density (and derived spectral index) for the detected compact components corresponds to 1$\sigma$, where $\sigma$ was determined by adding in quadrature the off-source rms  in each image and a 5\% of the local maxima, to conservatively account for possible inaccuracies in the EVN calibration. Upper limits for undetected sources are three times the off-source rms.}}
\end{table}