\begin{table}%t1
\caption{\label{tab:spec}The 10 spectra used for the spectroscopic analysis.}
%%\centerline

{\small
\begin{tabular}{lccrrr}
\hline
\hline
Spec.   &  Date      & Time      & \multicolumn{1}{c}{$t_{\rm exp}$}  &   &   \\
ID      &  UT        &  UT       &  \multicolumn{1}{c}{ [s] } & \multicolumn{1}{c}{$S/N$} & \\ \hline
H1      &2008-12-26                        & 04:56     & 2700 &  95 &  \\ 
H2      &2009-01-15                        & 05:39     & 2700 &  90 &  \\ 
H3      &2009-01-17                        & 01:45     & 2700 &  95 &  \\ 
H1--7   &\multicolumn{1}{l}{Combined spec.}&           &      & 235 &  \\
H1--107 &\multicolumn{1}{l}{Combined spec.}&           &      & 700 &  \\
U1      & 2008-09-13                       & 08:39     & 3600 & 470 &  \\ 
\hline                                                                    
Ceres   & 2006-07-16                       & 07:50     & 1800 & 220 &  \\ %% info from header
Ganymede& 2007-04-13                       & 09:40     &  300 & 340 &  \\ %% info from header
Moon    & 2008-08-09                       & 02:39     &  300 & 400 &  \\ 
\hline 
  \acenb  &\multicolumn{1}{l}{Combined spec.}&           &      &1030 \\ %% From bruntt_spec.tex
\hline
\end{tabular}}
\tablefoot{H1 to H3 are individual HARPS spectra, H1--7 is 7 co-added spectra, and H1--107 is the weighed sum of 107 spectra. U1 is the \uves\ spectrum. Ceres, Ganymede, and Moon 
are solar spectra from \harps, while \acenb\ refers to 25 co-added \harps\ spectra from 2004-05-15.}
\end{table}