\begin{table}%t1
%\centering
\par
  \caption{\label{tab:results} Properties of the sample stars. Rotation period and results from Stokes~$V$ measurements are from \citet{Donati08} and \citet{Morin08}. Rossby numbers are from \citet{Kiraga07}. Sources of Stokes~$I$ measurements are given in the table. The total magnetic energy is estimated from total magnetic flux using a scaling that involves a factor $f$. We use $f = 1.25$ (see text).} 
  \begin{tabular}{llccccccccc}
    \hline\hline
    \noalign{\smallskip}
    Name & Other & Mass & $P_{\rm rot}$ & $Ro$ & $\langle B_{V}\rangle $ & $\langle B_{I}\rangle $ & $\frac{\langle B_V\rangle }{\langle B_I\rangle }$ & $\langle B_V^2 \rangle $ & $ f \cdot \langle B_I \rangle ^2 $ &  $\frac{\langle B_V^2\rangle}{f \cdot \langle B_I\rangle ^2}$\\
    %\noalign{\smallskip}
    &&[$M_{\sun}$] & [d] & & [kG] & [kG] & [$\%$] & [kG$^2$] & [kG$^2$] & [$\%$]\\
    %\noalign{\smallskip}
    \hline
    \noalign{\smallskip}
%    \multicolumn{11}{c}{Partially convective stars}\\
%    \noalign{\smallskip}
%    \hline
%    \noalign{\smallskip}
    Gl 182  &        & 0.75 & 4.35 & 0.17 & 0.17 & 2.5$^{a}\pm0.8$ & $6.3\pm1.9$ & 0.04 & \phantom{1}$ 9.1\pm3.9$ & $0.4\pm0.2$\\
    Gl 494A & DT Vir & 0.59 & 2.85 & 0.09 & 0.15 & 3.0$^{b}\pm0.8$ & $5.0\pm1.3$ & 0.03 & $11.3\pm4.3$            & $0.3\pm0.1$\\
    Gl 569A & CE Boo & 0.48 & 14.7 & 0.35 & 0.10 & 1.8$^{a}\pm0.8$ & $5.6\pm2.5$ & 0.01 & \phantom{1}$ 4.1\pm2.6$ & $0.4\pm0.2$\\ 
    Gl 388  & AD Leo & 0.42 & 2.24 & 0.05 & 0.19 & 2.9$^{c}\pm0.8$ & $6.6\pm1.8$ & 0.06 & $10.5\pm4.1$            & $0.6\pm0.2$\\
    %\noalign{\smallskip}
    \hline
%    \noalign{\smallskip}
%    \multicolumn{11}{c}{Fully convective stars}\\
%    \noalign{\smallskip}
%    \hline
    \noalign{\smallskip}
    Gl 873  & EV Lac & 0.32 & 4.38 & 0.07 & 0.53 & \phantom{$>$}3.9$^{d}\pm0.8$ & \phantom{$<$}$13.6\pm2.8$ & 0.39 & \phantom{$>$}$19.0\pm5.6$ & \phantom{$<$}$2.0\pm0.6$\\
    Gl 285  & YZ Cmi & 0.31 & 2.77 & 0.04 & 0.56 & $\ga$3.9$^{c}\pm0.8$& $\la$$14.4\pm3.0$ & 0.52 & $\ga$$19.0\pm5.6$ & $\la$$2.7\pm0.8$\\ 
%    \noalign{\smallskip}
    \hline
  \end{tabular}
 % \flushleft
  %\small
  $^{a}$ {This work}; $^{b}$ {\cite{Saar96}, see text}; $^{c}$ {\cite{Reiners07}}; $^{d}$ {\cite{JKV00}}.
  \normalsize
\end{table}