\begin{table}%t1
\caption{\label{table1}{\it UBV}~photometry for stars in the fields of IC~2395 and~BH~47.}
%\centerline
{
\begin{tabular}{lccccccccccc}
\hline\hline
\noalign{\smallskip}
Star & $X$ & $Y$ & $\alpha_{2000}$  &  $\delta_{2000}$  &  $V$ & $B-V$ & $U-B$ & $n$ & 
Name(s) & Spec. type  &  Membership \\
  &  &  &  ($^{\rm h m s}$)  & ($\degr$ $\arcmin$)  &  &  &  &  &  &  &  \\
\noalign{\smallskip}
\hline\noalign{\smallskip}
1  & 464 & 542 & 8 42 15.9  &  --48 06.1   & 5.485  &  --0.179  &   --0.957 & 2 &   HD~74455, L~1  & B2/3 IV-V  & M, 96\% \\
2 & 465 & 575 &  8 42 15.8  &  --48 04.4   &  11.696 & 0.291 & 0.144  & 3 & L~18 &    &  M \\
3  & 472 & 584 & 8 42 17.9  &  --48 03.9   &  10.739  & 0.026  &  --0.121  & 3 &   L~15, CD~--47$\degr$4253  &    & M \\
4  & 453 & 573 & 8 42 12.2  &  --48 04.5   &  11.698  &  1.687  &  1.814  & 3 &   L~42, CD~--47$\degr$4250  &  &  NM \\
5  & 450 & 532 & 8 42 11.7  &  --48 06.6   &  10.395  &  0.001  &  --0.186 & 4 &   L~43, CD~--47$\degr$4247 &  & M \\
6  & 459 & 525 & 8 42 14.6  &  --48 06.9   &  11.281  &  0.089  &   0.034 & 4 &   L~44  &    &   M \\
7  & 459 & 517 & 8 42 14.6  &  --48 07.3   &  12.531  &  0.680  &   0.126 & 3 &   L~45  &    &   NM \\
8  & 444 & 497 & 8 42 10.3  &  --48 08.4   &  12.724  &  0.379  &   0.267 & 3 &   L~48  &    &  NM \\
\hline
\end{tabular}}
\smallskip
{Note:} Stars Nos. 153, 156, 174 and 233 are double stars. Photometry refers to the combined light of both components. 
Stars Nos.~170, 217 and~222 were previously reported as variables (Lapasset \& Clari\'a \cite{Lapasset1985}). Star No.~82 was found to be 
variable, its individual~$\Delta V$ variations being $\sim$0.3~mag. All the MK~spectral types are from Houck (\cite{Houck1978}), 
except that of star No.~1, which is from Garrison et~al. (\cite{Garrison1977}).
\end{table}