\begin{table}%t1
\caption{Amplitudes and phases of the modulations derived from the
   optical and ultra-violet light curves.}\label{gtab}
%\centerline
{
 \begin{tabular}{cccccccc}
\hline  \hline
 Mode & Period  &  Frequency & $A_{\rm L}$         & $\Phi_{\rm L}$           \\
      & (s)     &  ($\mu$Hz) & (\%)          &  (\arcdeg)         \\ 
\hline 
\sidehead{Optical (5500~{\AA})}
   F1 &  215.20 &  4646.9 & 2.01 $\pm$ 0.13  &  $-$153    $\pm$ \phn4 \\
   F2 &  271.95 &  3677.1 & 0.63 $\pm$ 0.13  &  \phs107   $\pm$ 12    \\
  (F2 &  270.46 &  3697.5 & 0.58 $\pm$ 0.13 & $\;$\phs109   $\pm$ 13)  \\
   F3 &  304.05 &  3288.9 & 0.96 $\pm$ 0.13  &  \phn$-$55 $\pm$ \phn8 \\
\sidehead{Optical (4585~{\AA})}
   F1 &   215.20 &  4646.9 & 2.37 $\pm$ 0.23 & $-$152     $\pm$ \phn6  \\
   F2 &   271.95 &  3677.1 & 0.99 $\pm$ 0.23 & \phs\phn94    $\pm$ 13  \\
  (F2 &   270.46 &  3697.5 & 0.77 $\pm$ 0.23 &$\;$\phs\phn96   $\pm$ 17)  \\
   F3 &   304.05 &  3288.9 & 1.07 $\pm$ 0.23 &  \phn$-$50 $\pm$ 12  \\
\sidehead{Optical (4210~{\AA})}
   F1 &   215.20 &  4646.9 &  2.50 $\pm$ 0.37 &  $-$153      $\pm$ \phn8  \\
   F2 &   271.95 &  3677.1 &  1.22 $\pm$ 0.37 &  \phs\phn97  $\pm$ 17  \\
  (F2 &   270.46 &  3697.5 &  0.83 $\pm$ 0.37 &  $\;$\phs\phn96  $\pm$ 26)  \\
   F3 &   304.05 &  3288.9 &  1.08 $\pm$ 0.37 &  \phn$-$39   $\pm$ 20  \\ 
\sidehead{UV; $v3$ (1920~{\AA})}
   F1 & 215.20 & 4646.9 & 4.56 $\pm$ 0.33 & $-$55 $\pm$ \phn4  \\
   F2 & 271.95 & 3677.1 & 1.61 $\pm$ 0.33 & $-$20 $\pm$ 12    \\
  (F2 & 270.46 & 3697.5 & 1.72 $\pm$ 0.33 & $\;$\phn$-$16 $\pm$ 11)   \\
   F3 & 304.05 & 3288.9 & 2.01 $\pm$ 0.33 & $-$20 $\pm$ \phn9    \\
\sidehead{UV; $v4$ (1920~{\AA})}
   F1 & 215.20 & 4646.9 & 5.04 $\pm$ 0.32 & \phs152 $\pm$  \phn4  \\
   F2 & 271.95 & 3677.1 & 2.00 $\pm$ 0.32 & $-$128  $\pm$  \phn9  \\
  (F2 & 270.46 & 3697.5 & 2.27 $\pm$ 0.32 & $\;$$-$124  $\pm$  \phn8)  \\
   F3 & 304.05 & 3288.9 & 1.19 $\pm$ 0.33 & $-$157  $\pm$   16  \\
\sidehead{UV; $v1$ (1570~{\AA})}
   F1 & 215.20 & 4646.9 & 9.51 $\pm$ 1.34 & $-$128    $\pm$ \phn8  \\
   F2 & 271.95 & 3677.1 & 1.43 $\pm$ 1.34 & \phn$-$66 $\pm$ 54     \\
  (F2 & 270.46 & 3697.5 & 1.25 $\pm$ 1.34 & $\;$\phn$-$95 $\pm$ 62)   \\
   F3 & 304.05 & 3288.9 & 3.12 $\pm$ 1.34 & $-$153    $\pm$ 24     \\ 
\hline
\end{tabular}}
\medskip
Notes. $A_{\rm L}$ and $\Phi_{\rm L}$ are the amplitudes and phases
 obtained by iterative least squares fitting of the light curves.
 The periods have been fixed to those determined from WET data
 \citep{kepler:95} and with a precision higher than that listed
 above: F1 = 215.1968~s, F2 = 271.95~s, F3 = 304.052~s.
 As such, in the ultra-violet, the measurements above represent limits 
 to the amplitudes at a given frequency when the signal is not clearly
 detected (see Fig.~\ref{fig:glcft}).
 Also shown in parenthesis, are the values obtained for the 270.46~s
 periodicity which was assigned a lower probability of being
 a false peak by \citet{kepler:95}.
 Limits for 119.84~s (8344.7~$\mu$Hz), a potential real mode
 reported by \citet{kepler:95} are: v1 $4.08\pm1.34$\%
 v3 $0.72\pm0.33$\%, v4 $0.94\pm0.32$\%; optical (5500~{\AA}): 
 $0.09\pm0.11$\%. The "v'' numbers merely denote abbreviated run
 numbers.
   \end{table}