\begin{table}%t1
\caption{Frequencies detected in multisite data of 44~Tau, according to Antoci et~al.~(\cite{Antoci2006}). $A_v$ and $A_y$ are the published amplitudes (mmag) in Str\o mgren $v$ and $y$ for the 2001/02 multisite data (3890~points in $v$, 3582~points in $y$). The corresponding columns indicated by "S/N'' contain a cross-identification for the data obtained by the Vienna University Automatic Photoelectric Telescope (Strassmeier et~al.~\cite{Strassmeier1997}; Granzer et~al.~\cite{Granzer2001}) in the course of this campaign (3280~points in $v$, 2981~points in $y$). An amplitude signal-to-noise ratio $>$$4$ was used. The columns indicated by "sig'' represent the cross-identification of the Vienna APT data with the complete campaign dataset using the result of the S{\sc ig}S{\sc pec} analysis, based on a spectral significance limit of $5.46$. Amplitudes in {\it italic} print refer to 1~d$^{-1}$ alias peaks. Since the peaks for the APT subset were assigned to corresponding peaks in the total dataset, individual frequencies are not displayed.}\label{TAB44Tau}
\small%\centering
\par
\begin{tabular}{lrrrrrrr}
\hline\hline\noalign{\smallskip}
             & $f$ $\left[{\rm d}^{-1}\right]$                            & \multicolumn{2}{c}{Total} & \multicolumn{2}{c}{APT, S/N} & \multicolumn{2}{c}{APT, sig} \\
\cline{3-4} \cline{5-6} \cline{7-8}\noalign{\smallskip} 
id&&\multicolumn{1}{c}{$A_v$}&\multicolumn{1}{c}{$A_y$}&\multicolumn{1}{c}{$A_v$}&\multicolumn{1}{c}{$A_y$}&\multicolumn{1}{c}{$A_v$}&\multicolumn{1}{c}{$A_y$}\\
$f_1$     & 6.8980&39.51&27.27&39.41&27.20&39.95&27.14\\
$f_2$     & 7.0060&17.20&12.15&18.90&13.21&19.95&13.61\\
$f_3$     & 9.1175&21.02&14.57&16.96&11.62&16.34&11.24\\
$f_4$     &11.5196&16.56&11.79&18.28&12.88&17.56&12.90\\
$f_5$     & 8.9606&13.73& 9.32&13.86& 9.80&14.63& 9.75\\
$f_6$     & 9.5613&18.62&12.92&10.84& 7.38& 9.94& 6.68\\
$f_7$     & 7.3034& 5.46& 3.76& 7.23& 4.83& 7.37& 5.06\\
$f_8$     & 6.7953& 4.83& 3.27& 3.77& 2.79& 4.32& 3.03\\
$f_9$     & 9.5801& 3.64& 2.25& 1.97& 1.28& 2.23& 1.53\\
$f_{10}$  & 6.3390& 2.08& 1.62& 2.34& 1.78& 2.25& 1.86\\
$f_{11}$  & 8.6394& 1.71& 1.45& 2.00& 1.56& 1.72& 1.21\\
$f_{12}$  &11.2946& 1.35& 0.92& 1.02&  --&{\it 0.72}&  -- \\
$f_{13}$  &12.6967& 0.24& 0.52&  --&  --&{\it 0.59}&  -- \\
\hline
$2f_1$    &13.7962& 1.58& 1.18& 1.52& 1.38& 1.65& 1.32\\
$f_1+f_2$ &13.9040& 1.45& 1.02& 1.35&{\it 1.02}& 1.24 &{\it 0.98}\\
$2f_2$    &14.0120& 0.40& 0.50&  --&  --&{\it 0.80} &  -- \\
$f_1+f_5$ &15.8586& 1.16& 1.02& 1.22&  --& 1.22&{\it 0.80}\\
$f_1+f_3$ &16.0155& 1.63& 1.29&{\it 0.93}&  --   &{\it 0.69}&{\it 0.64}\\
$f_2+f_3$ &16.1235& 0.79& 0.85&  --&  --&{\it 0.43}& 0.41\\
$f_1+f_6$ &16.4593& 1.25& 0.66&  --&  --&{\it 0.36}&  -- \\
$f_2+f_6$ &16.5673& 0.65& 0.32&  --&  --&  --& 0.46\\
$f_4+f_8$ &18.3149& 1.11& 0.48&  --&  --& 0.56& 0.55\\
$f_1+f_4$ &18.4177& 1.69& 1.10&{\it 1.67}&{\it 1.27}&{\it 1.95}&{\it 1.45}\\
$f_2+f_4$ &18.5256& 1.14& 0.96& 0.96&  --& 0.98& 0.59\\
$f_4+f_5$ &20.4802& 1.22& 0.94& 1.24& 1.07& 1.24& 1.09\\
$f_3+f_4$ &20.6371& 0.91& 0.81&  --&  --& 0.40&  -- \\
$f_4+f_6$ &21.0809& 0.77& 0.46&  --&  --&{\it 0.58}& 0.46\\
$2f_4$    &23.0392& 1.12& 0.78& 1.17&  --& 1.11& 0.78\\
$2f_4+f_1$&29.9373& 0.57& 0.35&  --&  --& 0.70& 0.50\\
\hline
\end{tabular}
\end{table}