\begin{table}%t2
\par
\caption{\label{table:lineScanSpectralCoverage}The wavelength range seen in a nominal line scan.}
\small
%\centering
\par
\begin{tabular}{c c c c c c c} 
\hline\hline\noalign{\smallskip}
Band  & $\lambda$ & \multicolumn{2}{c}{Full range} & Every pixel &  \multicolumn{2}{c}{{\it FWHM}} \\
      & ($\mu$m)   & (km~s$^{-1}$)     & ($\mu$m)   & ($\mu$m)         & ($\mu$m)  &(km~s$^{-1}$) \\
      \hline
B3A   & 55         & 1880       & 0.345      & 0.095            & 0.021      & 115 \\
B3A   & 72         & 800        & 0.192      & 0.053            & 0.013       & 55 \\
B2B   & 72         & 2660       & 0.638      & 0.221            & 0.039      & 165 \\ 
B2B   & 105        & 1040       & 0.364      & 0.126            & 0.028     & 80 \\
R1    & 105        & 5210       & 1.825      & 0.875            & 0.111      & 315 \\
R1    & 158        & 2870       & 1.511      & 0.724            & 0.126      & 240 \\
R1    & 175        & 2340       & 1.363      & 0.654            & 0.124      & 210 \\
R1    & 210        & 1310       & 0.92       & 0.441            & 0.098       & 140 \\
\hline
\end{tabular} 
\tablefoot{This range varies over  the spectral bands. The column ``every pixel'' refers
to the range that is seen by every spectral pixel.}
\end{table}