\begin{table}%t3
%\centering
\par
\caption{\label{tab:lcall}Results of analysis for ten asteroids from Table~\ref{tab:lc}.}
\begin{tabular}{lrrclllcccc}
\hline\hline \noalign{\smallskip}
Asteroid&$H_{\rm MPC}$ & $H$ &$G$ & $P$ & $\sigma_P$ & $\Delta P$ & $A$  & $n$ & RMS & RMS$_{\rm SDSS}$\\
&&      &     & h  & h     & h     &  mag &     &  mag & mag \\
\hline
%\multicolumn{2}{l}{$H_{MPC} = 12.8$}&&\multicolumn{3}{l}{$\bf (728) ~Leonisis$}&\\
% 0.15 & 13.03 &~5.5784 & 0.0006 & ~~~0.0002 & 0.33 & 2 & &0.027 \\
% 0.17 & 13.05 &~5.5783 & 0.0006 &           & 0.33 & 2 & &0.026 \\
~~~~(728) ~Leonisis& 12.8 & 13.04 & 0.15 &~5.5789 & 0.0004 & ~~~0.0002 & 0.33 & 3 & &0.015 \\
%\multicolumn{2}{l}{$H_{MPC} = 11.7$}&&\multicolumn{3}{l}{$\bf (1534) ~N\ddot{a}si$}\\ %\"{a}$\ddot{a}$si
%0.15 & 11.90 & 7.929  & 0.002  & ~~~0.0005 & 0.49 & 2 & 0.087 \\
%0.02 & 11.79 & 7.928  & 0.002  &           & 0.46 & 2 & 0.082 \\
%0.15 & 11.95 & 7.9304 & 0.0004 &           & 0.68 & 3 & 0.041 \\
%0.33 & 12.10 & 7.9308 & 0.0003 &           & 0.84 & 3 & 0.032 \\
%&&&&&\\
% 0.15 & 11.91 &~7.933  & 0.001  & ~~~0.0005 & 0.41 & 2 & &0.034 \\
% 0.05 & 11.83 &~7.9329 & 0.0009 &           & 0.43 & 2 & &0.025 \\
% 0.15 & 11.92 &~7.9337 & 0.0004 &           & 0.50 & 3 & &0.012 \\
~~(1534) ~N\"asi&11.7& 11.96 & 0.19 &~7.9338 & 0.0003 & ~~~0.0005  & 0.51 & 3 & &0.011 \\
%\multicolumn{2}{l}{$H_{MPC} = 12.5$}&&\multicolumn{3}{l}{$\bf (1829) ~Dawson$}\\
% 0.15 & 12.73 &~4.2502 & 0.0004 & ~~~0.0004 & 0.36 & 2&     & 0.022 \\
% 1.13 & 13.62 &~4.2519561 & 0.000002 &           & 0.37 & 2&     & 0.000 \\
% 0.15 & 12.71 &~4.2501 & 0.0001 & ~~~0.00026& 0.26 & 4&0.020& 0.035 \\
% 0.11 & 12.66 &~4.2501 & 0.0001 &           & 0.26 & 4&0.020& 0.035 \\
~~(1829) ~Dawson&12.5& 12.71 &(0.15) &~4.25009& 0.00008& ~~~0.00026& 0.28 & 6&0.017& 0.029 \\
% 0.11 & 12.65 &~4.25008& 0.00008&           & 0.28 & 6&0.017& 0.029 \\
%\multicolumn{2}{l}{$H_{MPC} = 11.2$}&&\multicolumn{3}{l}{$\bf (2453) ~Wabash$}\\
~~(2453) ~Wabash&11.2& 11.39 &(0.15) &~6.8792 & 0.0001 & ~~~0.0003 & 0.63 & 5&0.029& 0.023 \\
% 0.10 & 11.34 &~6.8792 & 0.0001 &           & 0.63 & 5&0.029& 0.022 \\
%\multicolumn{2}{l}{$H_{MPC} = 11.2$}&&\multicolumn{3}{l}{$\bf (2659) ~Millis$}\\
% 0.15 & 11.82 &~6.125  & 0.001 & $<0.0001$ & 0.88 & 2&     & 0.044 \\
~~(2659) ~Millis& 11.2& 11.59 &-0.08~ &~6.1242 & 0.0008& $<$0.0001 & 0.84 & 2&     & 0.035 \\
%\multicolumn{2}{l}{$H_{MPC} = 13.2$}&&\multicolumn{3}{l}{$\bf (7760) ~1990 ~RW_{3}$}\\
~~(7760) ~1990 ~RW$_{3}$&13.2& 13.61 &(0.15)& 25.911 & 0.003 & ~~~0.010   & 0.35 & 6&0.020& 0.037 \\
% 0.25 & 13.71 & 25.909 & 0.003 &            & 0.34 & 6&0.020& 0.036 \\
%\multicolumn{2}{l}{$H_{MPC} = ~9.0$}&&\multicolumn{3}{l}{$\bf (8405) ~Asbolus$}\\
% 0.15 &  9.24 &~4.4690  & 0.0004 & $<0.0001$  & 0.35 & 1&     & 0.028 \\
~~(8405) ~Asbolus&~~9.0&  9.26 & 0.35 &~4.4682  & 0.0003 & $<$0.0001  & 0.34 & 1&     & 0.023 \\
% 0.15 &  9.26 &~8.939  & 0.001 & $<0.001$  & 0.34 & 2&     & 0.031 \\
% 0.37 &  9.28 &~8.936  & 0.001 &           & 0.34 & 2&     & 0.026 \\
%\multicolumn{2}{l}{$H_{MPC} = 13.7$}&&\multicolumn{3}{l}{$\bf (9368) ~Esashi$}\\
~~(9368) ~Esashi&13.3& 13.71 & 0.15 &~2.9196 & 0.0002& ~~~0.0001  & 0.14 & 2&     & 0.015 \\ %Hmpc was 13.7
%\multicolumn{2}{l}{$H_{MPC} = 14.8$}&&\multicolumn{3}{l}{$\bf (30825) ~1990 ~TG_{1}$}\\
% 0.15 & 14.82 &~2.6199 & 0.0002 &~~~0.00008  & 0.13 & 2&     & 0.006 \\
% 0.07 & 14.72 &~2.62030& 0.00009&            & 0.13 & 2&     & 0.002 \\
(30825) ~1990 ~TG$_{1}$&14.8& 14.81 & (0.15) & (2.6243) &     &~~~0.0001   & 0.11 & 2&     & 0.022 \\
%\multicolumn{2}{l}{$H_{MPC} = 14.0$}&&\multicolumn{3}{l}{$\bf (35690) ~1999 ~CT_{21}$}\\
(35690) ~1999 ~CT$_{21}$&14.0& 14.47 & (0.15) &~9.028  & 0.003 & $<$0.001   & 0.50 & 2&     & 0.061 \\
% 0.23 & 14.51 &~9.029  & 0.003 &            & 0.51 & 2&     & 0.059 \\
% 0.15 & 14.46 &~9.026  & 0.003 & $<0.001$   & 0.53 & 3&     & 0.055 \\
% 0.19 & 14.48 &~9.027  & 0.003 &            & 0.54 & 3&     & 0.054 \\
\hline
\end{tabular}
\tablefoot{$H_{\rm MPC}$ is the absolute magnitude used in Minor Planet Center.
Values in parenthesis are assumed.  RMS is related to all available observations (including SDSS).}
\end{table}