\begin{table}%T14
\caption{\label{SPB-LMC-param}Basic light curve and physical properties of LMC stars classified as SPB with both the MSBN and the GM method. The dominant frequency $f_1$, the second frequency $f_2$, the effective temperature $\log T_{\rm eff}$ and the luminosity $\log (L/L_{\odot})$ are listed. Several of these stars might be evolved pulsators, termed PVSG here, rather than SPB.}
\renewcommand{\tabcolsep}{1.1mm}
\small%\centering
\par
\begin{tabular}{ccccc}
\hline\hline
Object identifier&$f_1$ ($c/d$)&$f_2$ ($c/d$)&$\log T_{\rm eff}$&$\log (L/L_{\odot})$\\
\hline
OGLE052848.51-694726.2&$0.998 $&$2.006 $&$4.09 $&$3.24 $\\
OGLE052526.06-695226.9&$1.001 $&$8.362 $&$4.19 $&$2.86 $\\
OGLE052629.22-700000.6&$0.998 $&$1.003 $&$3.96 $&$3.40 $\\
OGLE051259.38-691853.9&$0.999 $&$1.014 $&$4.08 $&$2.77 $\\
OGLE051448.80-685739.1&$1.004 $&$0.992 $&$4.18 $&$3.11 $\\
OGLE050812.19-685432.5&$1.004 $&$1.005 $&$4.17 $&$3.18 $\\
OGLE050851.08-684737.8&$1.477 $&$8.872 $&$4.10 $&$2.74 $\\
OGLE050713.75-690725.9&$1.976 $&$6.631 $&$4.06 $&$3.69 $\\
OGLE050259.73-692328.6&$1.004 $&$0.999 $&$4.05 $&$3.06 $\\
OGLE050422.37-685533.5&$1.004 $&$1.006 $&$3.99 $&$2.81 $\\
OGLE050452.11-691652.8&$0.007 $&$0.990 $&$4.10 $&$2.87 $\\
OGLE050458.68-690227.0&$0.024 $&$0.049 $&$4.01 $&$2.89 $\\
OGLE050502.21-685846.5&$0.999 $&$0.031 $&$4.11 $&$3.06 $\\
OGLE050014.17-692514.1&$0.937 $&$2.082 $&$4.05 $&$3.14 $\\
OGLE050030.25-692403.8&$1.438 $&$3.278 $&$4.15 $&$3.14 $\\
\hline
\end{tabular}
\end{table}