\begin{table}%t3
  \caption{\label{table:log}Observation log of the TIMMI2 and VISIR data.}
 %\centerline
{\small 
    \begin{tabular}{lllllll} 
      \hline
      \hline
      Object & RA ($^{\rm h}$ $^{\rm m}$ $^{\rm s}$)   & Dec ($\degr$ $^{\prime}$ $^{\prime\prime}$) & Date           & Calibrator star      & Instrument & Photometry$^{(1)}$ \\
             & (J2000)               & (J2000)                                     &                &                      &            & [Jy]                      \\
      \hline
      IRAS 06084 VLA1  & 06 10 50.57 & --06 11 49.7                                 & 2003-11-16     & HD~39523              & TIMMI2     &  4.51                     \\
      IRAS 06084 VLA4  & 06 10 50.32 & --06 11 57.6                                 & 2003-11-17     & HD~47205              & TIMMI2     &  1.72                     \\
      CD-42 11721      & 16 59 06.78 & --42 42 08.4                                 & 2005-02-25     & HD~151249             & TIMMI2     &  6.63                     \\
      TY CrA           & 19 01 40.83 & --36 52 33.9                                 & 2006-06-20     & HD~178345             & VISIR      & --                         \\
      HD~176386         & 19 01 38.93 & -36 53 26.6                                 & 2007-08-29     & HD~178345             & VISIR      & --                         \\
      \hline
    \end{tabular}}        
\par
      \medskip
      $(1)$ TIMMI2 11.9~$\mu$m (N11.9-OCLI filter) flux -- determined as $2\pi\sigma^{2}A$, where $\sigma$ and $A$ are the best fit values for the width and peak when fitting a 2D Gaussian to the source on the images.
\end{table}