\begin{table}%t4
\caption{\label{amplikepler}\Kepler\ performance.}
%\centerline
{
\begin{tabular}{llrrrrrrrrrrrrr}
\hline\hline
        &     &       & &\multicolumn{5}{c}{90-day run} & & \multicolumn{5}{c}{4-year run}\\
Stellar  &Type & $B-V$ & &\multicolumn{5}{c}{$m\ind{V}$ magnitude}& &\multicolumn{5}{c}{$m\ind{V}$ magnitude}\\
type as  &     &       & &  9  &    10 &    11 & 12    &   13 & &    9  &    10 &    11 &    12 & 1   3\\
\hline
HD~181907 &G8III&  1.09 & &  23 &    23 &    23 &    23 &    22& &   379 &   378 &   377 &   373 &   364\\
\hline
HD 49385 & G0IV&  0.51 & & 167 &    53 &    14 &   3.6 &   0.9& &  2709 &   864 &   233 &    58 &    14\\
\hline
HD 49933 & F5V &  0.35 & &  44 &    11 &   2.9 &   0.7 &   0.2& &   715 &   188 &    46 &    11 &   2.7\\
HD~181420 & F2V &  0.40 & &  36 &    10 &   2.5 &   0.6 &   0.1& &   598 &   161 &    40 &   9.8 &   2.3\\
HD~181906 & F8V &  0.43 & &  27 &   6.9 &   1.7 &   0.4 &   0.1& &   446 &   111 &    27 &   6.5 &   1.5\\
HD~175726 & G0V &  0.53 & & 3.3 &   0.8 &   0.2 &   0.0 &   0.0& &    54 &    13 &   3.3 &   0.8 &   0.2\\
\hline
\end{tabular}}
\par
\medskip
Maximum amplitude $\ampmax$ for \Kepler\ performance on CoRoT-like targets with varying magnitudes.
\end{table}