\begin{table}%T4
      \caption{\label{table.mu30}SIMBAD stars with USNO-B1 proper motions between 30 and 40~mas~a$^{-1}$.}  
         \small%\centering
\par
         \begin{tabular}{l cc cc c l}
            \hline
            \hline
            \noalign{\smallskip}
Name  						& $\alpha^{J2000}$	& $\theta^{J2000}$	& $\mu_\alpha \cos{\delta}$	& $\mu_\delta$		& $J$ 			& Remarks\tablefootmark{a}		\\
  						& 			& 			& [mas~a$^{-1}$]		& [mas~a$^{-1}$]	& [mag]			&		\\
              \hline 
\object{[SWW2004] J053856.630-025702.20}	& 084.735971		& --02.950597		& +28				& --24			& 12.10~$\pm$~0.03    	& 		\multicolumn{1}{l}{...}		\\
\object{[HHM2007] 752}				& 084.706060		& --02.832448		& +16				& --36			& 13.44~$\pm$~0.03    	& 		\multicolumn{1}{l}{...}		\\
\object{[KJN2005] 4.03~29}			& 084.595128		& --02.758452		& --22				& --30			& 14.32~$\pm$~0.03    	& No V$_r$ in Bu05		\\
\object{[HHM2007] 527}				& 084.616111		& --02.699823		& +30				& +4			& 14.66~$\pm$~0.04    	& 			\multicolumn{1}{l}{...}	\\
\object{2MASS J05392675--0233378}		& 084.861494		& --02.560502 		& +34				& --14			& 11.44~$\pm$~0.03    	& No $\mu$ in Ca08c		\\
\object{2MASS J05365466--0232069}		& 084.227779 		& --02.535264		& --18				& +26			& 11.50~$\pm$~0.02    	& No Li~{\sc i} and no $\mu$ in Ca06\\ % SO221028
\object{2MASS J05381906--0232014}		& 084.579439		& --02.533739		& --28				& +16			& 11.99~$\pm$~0.03    	& No Li~{\sc i} in Ca06		\\ % SO121219
\object{[HHM2007] 120}				& 084.406798		& --02.428913		& --4				& --32			& 14.66~$\pm$~0.05    	& 		\multicolumn{1}{l}{...}		\\
\object{[HHM2007] 1242}				& 084.962323		& --02.397435		& --38				& --10			& 14.46~$\pm$~0.04    	& 		\multicolumn{1}{l}{...}		\\
\object{[HHM2007] 998}				& 084.833748		& --02.365726		& --34				& --8			& 15.08~$\pm$~0.03    	& 		\multicolumn{1}{l}{...}		\\   \hline
         \end{tabular}
  \tablefoot{\tablefoottext{a}{``No $V_{\rm r}$'', ``no Li~{\sc i}'', and ``no $\mu$'' stand for 
radial velocity, p$EW$(Li~{\sc i}), and proper motion inconsistent with cluster 
membership, respectively.
The references are Burningham et~al. (\cite{Burningham2005}), Bu05, Caballero (\cite{Caballero2006}), Ca06, and
Caballero (\cite{Caballero2008c}), Ca08c.} }
   \end{table}