\begin{table}%t1
  \caption{\label{T1}The stellar sample. I. Photometric observations.}
\par
  %\centerline
{\small
  \begin{tabular}{lrlrrc}
  \hline\hline
  Star & Rot. Per.$^a$   &  Sp. type & \multicolumn{1}{c}{$v\sin i$} & \multicolumn{1}{c}{$i$} & \multicolumn{1}{c}{Time-base}\\
       & (days)      &          &\multicolumn{1}{c}{(\kms )} & \multicolumn{1}{c}{(\fok)}  & \multicolumn{1}{c}{(years)} \\
  \hline
AB Dor    &  0.515 & K0V       & 91    & 60 & 18 \\
LQ Hya    &  1.601 & K2V       & 27    & 65 & 25 \\
V833 Tau  &  1.788 & K5V       &  6.3  & 20 & 20 \\
 \multicolumn{1}{c}{"}      &  \multicolumn{4}{l}{photographic + photometric 
data}   & 109\\
V410 Tau  &  1.872 & K4        & 74    & 70 & 34 \\
EI Eri    &  1.947 & G5IV      & 51    & 46 & 28 \\
FK Com    &  2.400 & G4III     &155    & 60 & 28 \\
V711 Tau  &  2.838 & G5IV/K1IV & 41    & 40 & 30 \\
UZ Lib    &  4.768 & K0III     & 67    & 50 & 17 \\
UX Ari    &  6.437 & G5V/K0IV  & 39    & 60 & 23 \\
HU Vir    & 10.388 & K1IV-III  & 25    & 65 & 17 \\
IL Hya    & 12.905 & K0III-IV  & 26.5  & 55 & 20 \\
XX Tri    & 23.969 & K0III     & 21    & 60 & 21 \\
HK Lac    & 24.428 & K0III     & 20    & 65 & 50 \\
IM Peg    & 24.649 & K2III-II     & 26.5  & 70 & 29 \\
  \hline
  \end{tabular}}
\par
The stellar parameters are from Strassmeier (\cite{klaus_sum}), and the references 
therein.
$^a$ The orbital period is given in case of synchronised binary.
\end{table}