\begin{table}%t1
    \caption{\label{Sources}Source parameters.} 
    %\centerline
{
   \begin{tabular}{lllclllll}
    \hline \hline\noalign{\smallskip}
   Source name &Date &Inst/AOT $^{{a}}$ &FOV/slit $^{{b}}$ &$R$  &$\alpha (2000)$
 &$\delta (2000)$ &$z$ &$L$ Mag $^{{c}}$\\
\hline
Galactic center & & & & & & & &\\
\hline
GC SgrA$*$	&19 {\rm Feb.} 1996	&{\rm ISO}/{\rm SWS01} &$14''\times 20''$  &$R$	&17h45m39.97s 	&$-$29d00$'$28.7$''$  &$-$ &3.1\\
GC SgrA$*$        &21 {\rm Feb.} 1997 &{\rm ISO}/{\rm SWS06}  &$14''\times 20''$ &$R$   &17h45m39.97s &$-$29d00$'$28.8$''$  &$-$ &\\
GCS 3 I          &29 {\rm Aug.} 1996             &{\rm ISO}/{\rm SWS01}  &$14''\times20''$ &$R$ &17h46m14.84s &$-$28d49$'$33.8$''$  &$-$ &3.2\\
GCS 3 I            &08 {\rm Oct.} 1996        &{\rm ISO}/{\rm SWS06} &$14''\times20''$ &$R$ &17h46m14.84s &$-$28d49$'$33.7$''$  &$-$ &\\
IRAS 17424--2859      &01 {\rm Apr.} 1996          &{\rm ISO}/{\rm SWS01} &$14''\times20''$ &$R$  &17h45m39.93s &$-$29d00$'$22.8$''$ &$-$ &5\\
GC IRS7        &29 {\rm May} 2002 &VLT ISAAC/LWS3 LR &0.6$''$ &600 &17h45m41.1s     &$-$29d00$'$44.8$''$     &$-$ &5\\
\hline
Seyfert sources & & & & & & & &\\
\hline
NGC 1068        &18 {\rm Aug.} 2001 &VLT ISAAC/LWS3 LR &1.0$''$ &360 &02h42m40.7s     &$-$00d00m48s      &0.003793 &5.4\\
NGC 7172        &05 {\rm Aug.} 2001 &VLT ISAAC/LWS3 LR &1.0$''$ &360 &22h02m01.7s     &$-$31d52m18s      &0.008683 &8.5\\
IRAS 19254--7245 &04 {\rm Jun.} 2002 &VLT ISAAC/LWS3 LR &1.0$''$ &360 &19h31m21.4s     &$-$72d39m18s      &0.061709 &11.4\\
NGC 5506        &18 {\rm Jun.} 2003 &VLT ISAAC/LWS3 LR &1.0$''$ &360 &14h13m14.87s    &$-$03d12m27s      &0.006068 &7.4\\
            \hline
         \end{tabular}}
         \smallskip
\begin{list}{}{}
\item  $^a$  AOT: Astronomical Observation Template.
\item  $^b$  FOV: Field Of View, for ISO-SWS data; slit width for VLT-ISAAC ones.
\item  $^c$  given $L$~band magnitude are approximate as they are aperture dependent for most of the sources. ISO-SWS spectra are recorded in a source crowded area with a beam size of about $14''\times20''$.
\end{list}
   \end{table}