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\begin{table}[h!]
\begin{center}
\begin{tabular}{|l|r|r|r|r|} 
\hline
\multirow{2}{*}{Energy cut}  & \multicolumn{2}{|c|}{Upper limit $N_{osc}$ ($P_{\mu e}$, $P_{ee}=1$)}             & \multicolumn{2}{|c|}{Sensitivity $N_{osc}$ ($P_{\mu e}$, $P_{ee}=1$)}               \\ \hhline{~----}
							 & Bayes			& F\&C           &  Bayes         & F\&C                \\ \hline
10 GeV                       & 3.37 (0.0272) 	& 3.57 (0.0288)  & 3.37 (0.0272)  & 3.57 (0.0288)  \\
20 GeV                       & 6.75 (0.0061) 	& 7.26 (0.0066)  & 5.81 (0.0053)  & 5.98 (0.0054)  \\
\rowcolor{Green}
30 GeV                       & 8.58 (0.0034) 	& 9.22 (0.0037)  & 6.91 (0.0028)  & 6.72 (0.0027)  \\
40 GeV                       &10.01 (0.0037)	&11.10 (0.0037)  & 8.62 (0.0032)  & 8.60 (0.0028)  \\
50 GeV                       & 9.32 (0.0033) 	& 9.22 (0.0033)  & 9.32 (0.0033)  & 9.23 (0.0032)  \\
No cut                       &12.79 (0.0041)    &14.84 (0.0047)  & 10.48 (0.0033) & 11.38 (0.0036)  \\ \hline
\end{tabular}
\end{center}
\label{table:up_sens}
\caption{The upper limits and sensitivities on $N_{osc}$ and $P_{\mu e}$ (under assumption $P_{ee}=1$) at 90\% C.L.} The 30 GeV cut is the best one in sense of sensitivity to $P_{\mu e}$.
\end{table}
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