\begin{table}%t1
\caption{Sample of galactic early B supergiants from Crowther et~al. 
(\cite{Crowther}).}
\label{targets}
%\centerline
{
  \begin{tabular}{rrrlccrlccrrcc}
    \hline
    \hline\noalign{\smallskip}
\# &  HD  & Name & Sp. Type & $V$  & $B-V$  & D.M.& Ref.
%\footnote{References to the distances modulus, D.M., are (a) Brown et~al. (\cite{Brown}); (b) Blaha \& Humphreys (\cite{Blaha}); (c) Baume et~al. (\cite{Baume1}); (d) Baume et~al.  (\cite{Baume2}); (e) Garmany \& Stencel (\cite{Garmany}); (f) Humphreys (\cite{Humphreys}); (g) Crowther et~al. (\cite{Crowther}).} 
& $T_{\rm eff}$ & $\log g$ & $R_{*}$ & $\varv_{\infty}$ & $\dot{M}$ & $\beta$ \\
 &      &      &       & [mag]  & [mag]  &  & & [K] &  &  [$R_{\odot}$] & [km~s$^{-1}$] & [$10^{-6}~M_{\odot}$~yr$^{-1}$] &  \\
   \hline
 1 &  30614 & $\alpha$ Cam    & O9.5 Ia      & 4.29 & +0.02 &  10.0 & g & 29~000 &  3.00 & 26.0 &  1560 &  5.00 & 1.5  \\ 
 2 &  37128 & $\epsilon$ Ori  & B0 Ia        & 1.70 & $-0.19$ &   7.8 & a & 27~000 &  2.90 & 24.0 &  1910 &  2.50 & 1.5  \\
 3 &  91969 &                 & B0 Ia        & 6.52 & +0.00 &  12.2 & d & 27~500 &  2.95 & 25.3 &  1470 &  1.00 & 1.5  \\
 4 &  94909 &                 & B0 Ia        & 7.34 & +0.48 &  11.5 & g & 27~000 &  2.90 & 25.5 &  1050 &  2.00 & 1.5  \\
 5 & 122879 &                 & B0 Ia        & 6.42 & +0.12 &  11.7 & g & 28~000 &  2.95 & 24.4 &  1620 &  3.00 & 1.5  \\
 6 &  38771 & $\kappa$ Ori    & B0.5 Ia      & 2.05 & $-0.18$ &   8.0 & a & 26~500 &  2.90 & 22.2 &  1525 &  0.90 & 1.5  \\
 7 & 115842 &                 & B0.5 Ia      & 6.02 & +0.29 &  11.3 & g & 25~500 &  2.85 & 34.2 &  1180 &  2.00 & 1.5  \\
 8 & 152234 &                 & B0.5 Ia      & 5.44 & +0.20 &  11.5 & c & 26~000 &  2.85 & 42.4 &  1450 &  2.70 & 1.5  \\
 9 &   2905 & $\kappa$ Cas    & BC0.7 Ia     & 4.16 & +0.14 &  10.2 & b & 21~500 &  2.60 & 41.4 &  1105 &  2.00 & 2.0  \\
10 &  91943 &                 & B0.7 Ia      & 6.73 & +0.07 &  12.2 & d & 24~500 &  2.80 & 26.3 &  1470 &  0.75 & 1.2  \\
11 & 152235 &                 & B0.7 Ia      & 6.34 & +0.51 &  11.5 & c & 23~000 &  2.65 & 47.1 &   850 &  1.25 & 1.5  \\
12 & 154090 &                 & B0.7 Ia      & 4.87 & +0.26 &  10.2 & g & 22~500 &  2.65 & 36.0 &   915 &  0.95 & 1.5  \\
13 &  13854 &                 & B1 Iab       & 6.48 & +0.28 &  11.8 & e & 21~500 &  2.55 & 37.4 &   920 &  0.85 & 2.0  \\
14 &  91316 & $\rho$ Leo      & B1 Iab       & 3.85 & $-0.14$ &  10.5 & g & 22~000 &  2.55 & 37.4 &  1110 &  0.35 & 1.0  \\
15 & 148688 &                 & B1 Ia        & 5.33 & +0.33 &  10.5 & g & 22~000 &  2.60 & 36.7 &   725 &  1.75 & 2.0  \\
16 &  14956 &                 & B1.5 Ia      & 7.19 & +0.72 &  11.8 & e & 21~000 &  2.50 & 50.6 &   500 &  1.00 & 2.0  \\
17 & 152236 & $\zeta^{1}$ Sco & B1.5 Ia$^{+}$& 4.73 & +0.48 &  11.5 & c & 18~000 &  2.20 &112.4 &   390 &  6.00 & 2.0  \\
18 & 190603 &                 & B1.5 Ia$^{+}$& 5.65 & +0.54 &  10.9 & g & 18~500 &  2.25 & 59.6 &   485 &  2.50 & 3.0  \\
19 &  14143 &                 & B2 Ia        & 6.66 & +0.50 &  11.8 & e & 18~000 &  2.25 & 52.9 &   645 &  1.05 & 2.0  \\
20 &  14818 & 10 Per          & B2 Ia        & 6.25 & +0.30 &  11.8 & e & 18~500 &  2.40 & 46.1 &   565 &  0.55 & 2.0  \\
21 &  41117 & $\chi^{2}$ Ori  & B2 Ia        & 4.63 & +0.28 &  10.9 & b & 19~000 &  2.35 & 61.9 &   510 &  0.90 & 2.0  \\
22 & 194279 &                 & B2 Ia        & 7.05 & +1.02 &  10.4 & f & 19~000 &  2.30 & 44.7 &   550 &  1.05 & 2.5  \\
23 & 198478 & 55 Cyg          & B2.5 Ia      & 4.86 & +0.42 &   9.5 & f$^{1}$%\footnote{Humphreys (\cite{Humphreys}) gives for this object a distance of 10.22~mag. To stay conform with CLW, we will use their value of 9.5.} 
& 16~500 &  2.15 & 40.0 &   470 &  0.23 & 2.0  \\
24 &  14134 &                 & B3 Ia        & 6.55 & +0.45 &  11.8 & e & 16~000 &  2.05 & 56.7 &   465 &  0.52 & 2.0  \\
25 &  53138 & $o^{2}$ CMa     & B3 Ia        & 3.01 & $-0.08$ &  10.2 & g & 15~500 &  2.05 & 65.0 &   865 &  0.36 & 2.0  \\
    \hline
  \end{tabular}}
  \medskip
\par
References to the distance modulus, D.M., are (a) Brown et~al. (\cite{Brown}); (b) Blaha \& Humphreys (\cite{Blaha}); (c) Baume et~al. (\cite{Baume1}); (d) Baume et~al.  (\cite{Baume2}); (e) Garmany \& Stencel (\cite{Garmany}); (f) Humphreys (\cite{Humphreys}); (g) Crowther et~al. (\cite{Crowther}).\protect\\
$^{1}$The distance modulus for the star HD~198478 is 10.22~mag according to Humphreys (\cite{Humphreys}). To stay conform with CLW, we will use their value of 9.5.  
\end{table}