\begin{table}%t2
\par
\caption{\label{tablevisir}Observation parameters.}
%\centerline
 {
\begin{tabular}{llllrllrrrlll}
\hline \hline
\noalign{\smallskip}
PKS &  Alias & Date & Dist. &  $F_{11.85~\mu{\rm m}}^{{\rm core}}$  &  Lit. & Ref. &  $\log{\nu L_{11.85~\mu{\rm m}}^{{\rm core}}}$  &  $\log{\nu L_{5{\rm GHz}}^{{\rm core}}}$ &  $\log{\nu L_{12~\mu{\rm m}}^{{\rm total}}}$ & $R50$ & \multicolumn{2}{c}{{\it FWHM}} \\
&&&&&&&&&&& Obj. & St. \\
 & & & Mpc & (mJy) & (mJy) & & (${\rm erg}~{\rm s}^{-1}$) & (${\rm erg}~{\rm s}^{-1}$) & (${\rm erg}~{\rm s}^{-1}$) & (pc) & ($\arcsec$) & ($\arcsec$) \\
(1)&(2)&(3)&(4)&(5)&(6)&(7)&(8)&(9)&(10)&(11)&(12)&(13)\\
\hline
0007+12        & \object{4C12.03}      & 2006-06-18   &   710 & $<$3            &    $\dots$  & $\dots$     & $<$43.58      & 40.28   &    $\dots$ &     $\dots$ &  $\dots$ &  $\dots$ \\
0034$-$01      & \object{3C~015}        & 2006-06-18   &   310 & $<$3            &  6 & 4  & 
$<$42.93      & 41.21   &    $\dots$ &     $\dots$ &  $\dots$ &  $\dots$ \\
0055$-$01      & \object{3C~029}        & 2006-12-27   &   190 & $<$4            &  2 & 4  & 
$<$42.56      & 40.28   &    $\dots$ &     $\dots$ &  $\dots$ &  $\dots$ \\
0123$-$01      & \object{3C~040}        & 2006-12-27   &    70 & $<$4            &    $\dots$  & $\dots$     & $<$41.76      & 39.51   &$<$43.27   &     $\dots$ &  $\dots$ &  $\dots$ \\
0305+03        & \object{3C~078}        & 2006-12-27   &   120 & $<$4            &    $\dots$  & $\dots$     & $<$42.18      & 40.78   &$<$43.57   &     $\dots$ &  $\dots$ &  $\dots$ \\
0320$-$37      & \object{Fornax~A}     & 2006-12-27   &    20 & $<$9            &    $\dots$  & $\dots$     & $<$41.03      & 37.81   &    42.44   &     $\dots$ &  $\dots$ &  $\dots$ \\
0340+04        & \object{3C~093 }       & 2006-12-27   &  1800 & $<$5            &    $\dots$  & $\dots$     & $<$44.56      & 40.75   &    $\dots$ &     $\dots$ &  $\dots$ &  $\dots$ \\
0356+10        & \object{3C~098}        & 2005-12-18   &   130 &       20~$\pm$~1.4    &     24      & 2           & 42.93~$\pm$~0.04 & 38.91   &$<$42.95   &   180       &  0.47    &  0.37 \\
0404+03        & \object{3C~105}        & 2005-12-18   &   390 & $<$2            &    $\dots$  & $\dots$     & $<$42.93      & 40.06   &    $\dots$ &     $\dots$ &  $\dots$ &  $\dots$ \\
0430+05        & \object{3C~120}        & 2006-12-27   &   140 &      240~$\pm$~15     &    109      & 1           & 44.10~$\pm$~0.03 & 41.58   &    44.20   &   170       &  0.36    &  0.33 \\
0511+00        & \object{3C~135}        & 2006-12-27   &   570 & $<$4            &    $\dots$  & $\dots$     & $<$43.51      & 39.89   &    $\dots$ &     $\dots$ &  $\dots$ &  $\dots$ \\
0518$-$45      & \object{Pictor~A}     & 2006-12-27   &   150 &       68~$\pm$~4.3    &    $\dots$  & $\dots$     & 43.59~$\pm$~0.04 & 41.09   &    43.82   &   200       &  0.34    &  0.33 \\
0819+06        & \object{3C~198 }       & 2006-12-27   &   350 & $<$4            &    $\dots$  & $\dots$     & $<$43.13      & 39.13   &    $\dots$ &     $\dots$ &  $\dots$ &  $\dots$ \\
0945+07        & \object{3C~227}        & 2006-12-27   &   370 &       29~$\pm$~3.1    &    $\dots$  & $\dots$     & 44.01~$\pm$~0.05 & 40.38   & $<$44.96   &   410       &  0.36    &  0.33 \\
1216+06        & \object{3C~270}        & 2006-06-18   &    30 & $<$2            &       27    & 4           & $<$40.72      & 39.17   & $<$42.44   &     $\dots$ &  $\dots$ &  $\dots$ \\
1322$-$42      & \object{Centaurus~A}  & 2006-12-27   &   3.8 &     1200~$\pm$~47     &    1800     & 3           & 41.69~$\pm$~0.03 & 38.79   &    42.69   &     5       &  0.37    &  0.33 \\
1417$-$19      & \object{PKS1417$-$19} & 2006-12-27   &   530 &       26~$\pm$~4.3    &    $\dots$  & $\dots$     & 44.27~$\pm$~0.08 & 39.90   &    $\dots$ &   770       &  0.44    &  0.33 \\
1514+07        & \object{3C~317}        & 2006-06-18   &   142 & $<$3            &  3 & 4  & 
$<$42.24      & 40.66   & $<$43.67   &     $\dots$ &  $\dots$ &  $\dots$ \\
1559+02        & \object{3C~327}        & 2005-07-02   &   460 &       78~$\pm$~7.5    &    $\dots$  & $\dots$     & 44.62~$\pm$~0.05 & 40.50   & $<$44.68   &  1300       &  1.25    &  0.42 \\
1717$-$00      & \object{3C~353}        & 2005-07-02   &   125 & $<$4            &    $\dots$  & $\dots$     & $<$42.28      & 40.02   &   $\dots$  &     $\dots$ &  $\dots$ &  $\dots$ \\
1839$-$48      & \object{PKS1839$-$48} & 2006-06-18   &   490 & $<$4            &    $\dots$  & $\dots$     & $<$43.40      & 41.33   &   $\dots$  &     $\dots$ &  $\dots$ &  $\dots$ \\
1949+02        & \object{3C~403}        & 2006-06-18   &   250 &       89~$\pm$~6.8    &    $\dots$  & $\dots$     & 44.17~$\pm$~0.04 & 39.55   &     44.50  &   330       &  0.34    &  0.37 \\
1949$-$01      & \object{3C~403.1 }     & 2006-06-18   &   230 & $<$4            &    $\dots$  & $\dots$     & $<$ 42.78      & $\dots$ &    $\dots$ &     $\dots$ &  $\dots$ &  $\dots$ \\
2045+06        & \object{3C~424  }      & 2006-06-18   &   560 & $<$4            &  2 & 4  & 
$<$43.46      & 40.48   &    $\dots$ &     $\dots$ &  $\dots$ &  $\dots$ \\
2158$-$380     & \object{PKS2158$-$380}& 2006-06-18   &   140 &       17~$\pm$~2.8    &    $\dots$  & $\dots$     & 42.94~$\pm$~0.07 &$<$38.88 & $<$43.68  &   200       &  0.37    &  0.33 \\
2221$-$02      & \object{3C~445   }     & 2005-07-02   &   240 &      190~$\pm$~16     &    210      &  2          & 44.46~$\pm$~0.04 & 40.44   &     44.44  &   390       &  0.42    &  0.42 \\
2354$-$35      & \object{PKS2354$-$35} & 2006-06-18   &   210 & $<$3            &    $\dots$  & $\dots$     & $<$42.55      & 39.08   &    $\dots$ &     $\dots$ &  $\dots$ &  $\dots$ \\
\hline
\end{tabular}}
\tablefoot {\textit{Column~(1)} Parkes Radio catalogue reference. \textit{Column~(3)} Date of observation. 
\textit{Column~(4)} Distances under the chosen cosmology, determined from the redshifts. 
\textit{Columns~(5--7)} VISIR mid-infrared core flux and 3-$\sigma$ upper limits, at the SiC-band (11.9~$\mu$m), compared to literature values: 1~=~\cite{2004ApJ...605..156G} (TIMMI, 1.5~$\arcsec$, 10.8~$\mu$m), 2~=~\cite{2004AetA...421..129S} (ISOCAM, 5~$\arcsec$, 14.3~$\mu$m), 3~=~\cite{2004ApJ...602..116W} (Keck, 0.3$\arcsec$, 11.7~$\mu$m) and 4~=~\cite{2009ApJ...701..891L} (Spitzer IRS, 15~$\mu$m). \textit{Column~(8)} VISIR mid-infrared core luminosity at rest wavelength. \textit{Column~(9)} Radio (5~GHz) core luminosity at rest wavelength from fluxes tabulated in Table~\ref{coresed}. \textit{Column~(10)} IRAS mid-infrared galaxy luminosity at rest wavelength derived for most sources from flux from \cite{1988AJ.....95...26G}, for 3C~227 from \cite{1995AetA...303....8H}, and for PKS2158$-$380 from \cite{1990IRASF.C......0M}. \textit{Columns~(11--13)} The radius at $50\%$ of the flux, the full width half maximum 
({\it FWHM}) of the flux of the source and of the standard star.}
\vspace*{3mm}
\end{table}