\begin{table}%t3
%\centering
\par
\caption{Spectral types of the program stars from Wang \& Hu (\cite{wang}),
from photometry in the Vilnius system by Kazlauskas \& Jasevicius (\cite{Kaz86})
transformed by us into spectral types following Stray\v{z}is (\cite{Str77}), and
from classification of our Echelle spectra against the Yamashita et~al.
(\cite{yamashita}) reference spectral atlas. The last columns give the $E_{B-V}$ (from
Fitzgerald \cite{fitzgerald} intrinsic colors) and the spectro-photometric distances for
our spectral classification and the photometry in Table~\ref{t1}.}\label{t3}
\begin{tabular}{rlcclc}
\hline\hline
    &\multicolumn{3}{c}{spectral type}&\\ 
    \cline{2-4}
\#  & WH00&Vilnius&our&$E_{B-V}$ & $d$ (kpc) \\ 
      1  & F0 III  & F1 V  &  F0 III     & 0.11 & 0.2 \\ 
      2  & B0 I    & B1 Ia &  B0 I       & 0.97 & 2.0 \\
      3  & B0 I    & B1 Ia &  B0 I/II    & 1.06 & 1.4 \\
      4  & O7 II   & B1 Ia &  O9 Ib      & 0.92 & 2.3 \\
      5  & B0 IIIe &       &  B0 IIIe    & 1.07 & 1.2 \\
      6  & B0 II   & B2 Ia &  B0 V       & 0.93 & 1.1 \\
      7  & B4 II   & B3 V  &  B5 IV      & 0.26 & 1.6 \\
      8  & B0 III  & B0 III&  B0 Ib/II   & 0.99 & 3.0 \\
      9  & A4 V    & F0 V  &  A4 V       & 0.23 & 0.3 \\
     10  & B6 II   & B2 V  &  B5 V/IV    & 0.41 & 1.2 \\
     11  &         & A5 V  &  A5 III/II  & 0.39 & 1.9 \\
     12  &         & B2 V  &  B2 V       & 0.26 & 5.3 \\
     13  & G6 III  &       &  G5 III     & 0.00 & 1.1 \\
     14  & A8 II   & A4 V  &  F7 IV      & 0.00 & 0.7 \\
     15  & B1 II   & B3 Ib &  B1 III     & 1.38 & 1.6 \\
     16  &         & B1 II &  B0 V       & 0.83 & 2.8 \\
\hline
\end{tabular}
\end{table}