\begin{table}%T12
\caption{\label{SPB-SMC-param}Basic light curve and physical properties of SMC 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
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\begin{tabular}{ccccc}
\hline\hline
Object identifier&$f_1$ ($c/d$)&$f_2$ ($c/d$)&$\log T_{\rm eff}$&$\log (L/L_{\odot})$\\
\hline
OGLE004522.52-732811.1&$0.995 $&$6.800 $&$4.06 $&$3.49 $\\
OGLE004553.80-730754.7&$0.019 $&$0.286 $&$4.07 $&$3.72 $\\
OGLE004633.16-731048.0&$1.304 $&$2.792 $&$4.07 $&$3.41 $\\
OGLE004709.37-731317.8&$1.535 $&$0.488 $&$4.10 $&$3.65 $\\
OGLE004854.37-732844.1&$0.969 $&$1.001 $&$4.04 $&$3.88 $\\
OGLE004855.91-732519.0&$0.998 $&$1.005 $&$4.11 $&$3.89 $\\
OGLE004940.01-732128.8&$0.986 $&$0.493 $&$4.08 $&$3.36 $\\
OGLE004954.18-731815.8&$1.006 $&$0.002 $&$4.05 $&$3.67 $\\
OGLE005048.72-732316.4&$1.086 $&$1.163 $&$4.10 $&$3.39 $\\
OGLE005123.10-730614.7&$2.005 $&$3.127 $&$4.05 $&$3.09 $\\
OGLE005212.33-731838.2&$1.004 $&$6.006 $&$4.08 $&$4.19 $\\
OGLE005228.58-723926.2&$1.004 $&$0.273 $&$4.11 $&$3.38 $\\
OGLE005304.91-725218.9&$1.524 $&$2.254 $&$4.07 $&$4.35 $\\
OGLE005720.47-723014.9&$0.723 $&$1.620 $&$4.06 $&$3.27 $\\
OGLE010126.00-723601.6&$1.216 $&$0.998 $&$4.11 $&$3.20 $\\
OGLE010211.58-720854.0&$1.542 $&$0.001 $&$4.09 $&$3.12 $\\
OGLE010325.80-725726.8&$1.291 $&$1.368 $&$4.03 $&$3.12 $\\
OGLE010603.65-723901.6&$1.777 $&$0.003 $&$4.08 $&$3.15 $\\
OGLE010646.84-721948.7&$1.292 $&$0.999 $&$4.14 $&$3.67 $\\
OGLE010741.81-722701.7&$1.004 $&$3.009 $&$4.11 $&$3.67 $\\
\hline
\end{tabular}
\end{table}