\begin{table}%t1
  \caption{Averaged observed amplitude ratios and phase differences from 2000/1 to 2004/5. Only frequencies detected in both photometric and spectroscopic data are listed. In the last two columns the predicted spherical degree from our mode identification (see Sect.~\ref{sec:modeID}) and the azimuthal number~$m$ from Zima et~al. (2007) are given. For $f_9$ no reliable results could be derived due to the influence of the close and more dominant frequency $f_6$.
  \label{table:1}}
  %\centering
\par
  \begin{tabular}{lrrrrr}
	\hline\hline
	 & Frequency     & $A_v$/$A_y$  & $\phi_v$-$\phi_y$  & $\ell$ & $m$ \\
	 & [cd$^{-1}$]  & [mmag]       &  [$^\circ$]        &     &        \\
	\hline
	$f_1$ & 6.8980& 1.44 $\pm$ 0.01 & +2.96 $\pm$ 0.22 & 0& 0\\ 
	$f_2$ & 7.0060& 1.43 $\pm$ 0.01 & --1.83 $\pm$ 0.39 & 1& 1\\ 
	$f_3$ & 9.1175& 1.46 $\pm$ 0.02 & --1.85 $\pm$ 0.29 & 1& 1\\ 
	$f_4$ &11.5196& 1.42 $\pm$ 0.01 & --1.75 $\pm$ 0.50 & 1& 0\\
	$f_5$ & 8.9606& 1.45 $\pm$ 0.03 & +2.35 $\pm$ 0.36 & 0& 0\\
	$f_6$ & 9.5613& 1.46 $\pm$ 0.02 & --1.40 $\pm$ 0.32 & 1&  \\
	$f_7$ & 7.3034& 1.45 $\pm$ 0.06 & --6.75 $\pm$ 1.61 & 2& 0\\ 
	$f_8$ & 6.7953& 1.38 $\pm$ 0.08 & --7.26 $\pm$ 4.57 & 2& 0\\
	$f_9$ & 9.5801& --               & --                &  &  \\
	$f_{10}$& 6.3391& 1.40 $\pm$ 0.10 & --4.97 $\pm$ 5.69 & 2& \\
	$f_{11}$& 8.6393& 1.35 $\pm$ 0.09 & --7.44 $\pm$ 1.58 &  & 0\\
	$f_{12}$&11.2919& 1.32 $\pm$ 0.19 & --3.21 $\pm$ 5.35 &  &  \\ 
	\hline
  \end{tabular}
\end{table}