\begin{table}%T1
\caption{\label{newUBVRI}New Johnson-Cousins photoelectric photometry obtained for some of the metal-poor stars in the sample.}
\small%\centering
\par
\begin{tabular}{lccccc}
\hline\hline\noalign{\smallskip}
Name	     &        $U$    &    $B$  &  $V$   & $R_{\rm C}$  &   $I_{\rm C}$ \\     
\hline
HD~3567       &        9.556  &   9.695 &  9.240 &  8.941 &  8.631  \\ 
HD~16031      &       10.004  &  10.197 &  9.770 &  9.484 &  9.184  \\ 
HD~19445	     &        8.207  &   8.503 &  8.026 &  7.737 &  7.394  \\ 
HD~34328	     &        9.683  &   9.903 &  9.416 &  9.106 &  8.773  \\ 
HD~45282      &        8.659  &   8.672 &  8.010 &  7.610 &  7.196  \\
HD~59392	     &       10.048  &  10.217 &  9.761 &  9.457 &  9.142  \\ 
HD~64090	     &        8.762  &   8.951 &  8.295 &  7.935 &  7.536  \\ 
HD~64606      &        8.277  &   8.140 &  7.412 &  6.994 &  6.561  \\
HD~74000      &        9.880  &  10.071 &  9.656 &  9.381 &  9.080  \\ 
HD~84937      &        8.485  &   8.702 &  8.306 &  8.047 &  7.759  \\ 
HD~94028	     &        8.421  &   8.640 &  8.202 &  7.917 &  7.585  \\ 
HD~102200     &        9.009  &   9.189 &  8.739 &  8.449 &  8.141  \\ 
HD~106038     &       10.431  &  10.627 & 10.153 &  9.857 &  9.529  \\ 
HD~108177     &        9.874  &  10.082 &  9.647 &  9.362 &  9.052  \\ 
HD~110621     &       10.230  &  10.385 &  9.932 &  9.628 &  9.313  \\ 
HD~114762     &        7.738  &   7.833 &  7.283 &  6.967 &  6.629  \\
HD~116064     &        9.099  &   9.282 &  8.833 &  8.520 &  8.189  \\ 
HD~122196     &        9.055  &   9.212 &  8.753 &  8.444 &  8.112  \\
HD~132475     &        8.983  &   9.100 &  8.563 &  8.216 &  7.855  \\
HD~134169     &        8.115  &   8.193 &  7.663 &  7.342 &  7.011  \\
HD~134439     &       10.033  &   9.881 &  9.118 &  8.661 &  8.220  \\ 
HD~140283     &        7.502  &   7.692 &  7.205 &  6.876 &  6.522  \\ 
HD~160617     &        9.014  &   9.188 &  8.740 &  8.431 &  8.108  \\ 
HD~163810     &       10.185  &  10.272 &  9.660 &  9.280 &  8.897  \\
HD~179626     &        9.601  &   9.710 &  9.188 &  8.849 &  8.502  \\ 
HD~181743     &        9.911  &  10.140 &  9.683 &  9.375 &  9.062  \\ 
HD~188510     &        9.303  &   9.452 &  8.851 &  8.486 &  8.100  \\ 
HD~189558     &        8.214  &   8.299 &  7.740 &  7.392 &  7.034  \\ 
HD~193901     &        9.049  &   9.183 &  8.644 &  8.307 &  7.964  \\ 
HD~194598     &        8.666  &   8.844 &  8.356 &  8.055 &  7.739  \\ 
HD~199289     &        8.660  &   8.803 &  8.287 &  7.972 &  7.643  \\
HD~201891     &        7.740  &   7.908 &  7.390 &  7.081 &  6.737  \\ 
HD~213657     &        9.869  &  10.063 &  9.646 &  9.368 &  9.068  \\ 
HD~215801     &       10.272  &  10.471 & 10.038 &  9.732 &  9.418  \\ 
HD~219617     &        8.425  &   8.621 &  8.153 &  7.845 &  7.525  \\ 
HD~284248     &        9.407  &   9.650 &  9.208 &  8.927 &  8.608  \\ 
HD~298986     &       10.316  &  10.506 & 10.062 &  9.774 &  9.470  \\ 
BD+17 4708   &        9.718  &   9.922 &  9.476 &  9.183 &  8.854  \\ 
BD+02 3375   &       10.174  &  10.414 &  9.944 &  9.635 &  9.297  \\ 
BD-04 3208   &       10.203  &  10.375 &  9.977 &  9.709 &  9.417  \\ 
BD-13 3442   &       10.529  &  10.655 & 10.266 &  9.994 &  9.704  \\ 
CD-30 18140  &       10.155  &  10.365 &  9.946 &  9.663 &  9.353  \\ 
CD-33 3337   &        9.436  &   9.581 &  9.109 &  8.814 &  8.490  \\ 
\hline
\end{tabular}
\tablefoot{
Each measurement comprises an average of 4 observations per star. The rms of individual observations are $0.02$ for the $V$ magnitude, $0.015$ for the $U-B$ colour and $0.008$~mag for~$B-V$, $V-R$, $R-I$, $V-I$~colours.}
\end{table}