\begin{table}%T1
\caption{Program stars and log of observations.}
\label{logobs} 
%\centerline
 {\small
\begin{tabular}{rlrcccl}
\hline\hline
%\noalign{\smallskip}
Object&Sp.T&$V\sin i$&$\log T_{\rm eff}$&$\log g$& $i$   & Date \\          
    &    &km~s$^{-1}$       &                  &        & [deg] &      \\
\hline 
%\noalign{\smallskip}
\scriptsize{\object{HD 41335}} &\scriptsize{B1.5IIIne}& 358 & 4.320 & 3.89 & 69 & \scriptsize{1,2} \\
%\noalign{\smallskip}
\scriptsize{\object{HD 45725}} &\scriptsize{B2.5IV-Ve}& 330 & 4.251 & 3.90 & 67 &\scriptsize{3} \\
%\noalign{\smallskip}
\scriptsize{\object{HD 48917}} &\scriptsize{B2III-IVe}& 205 & 4.308 & 3.40 & 45 &\scriptsize{3} \\
%\noalign{\smallskip}
\scriptsize{\object{HD 50013}} &\scriptsize{B1.5IVne} & 243 & 4.391 & 4.02 & 37 &\scriptsize{1,2} \\
%\noalign{\smallskip}
\scriptsize{\object{HD 56139}} &\scriptsize{B2IVe}    &  84 & 4.291 & 3.62 & 17 &\scriptsize{3} \\
%\noalign{\smallskip}
\scriptsize{\object{HD 58978}} &\scriptsize{B0Vpe}    & 375 & 4.388 & 4.15 & 55 &\scriptsize{3} \\
%\noalign{\smallskip}
\scriptsize{\object{HD 63462}} &\scriptsize{B0Ve}     & 435 & 4.424 & 3.60 & 90 &\scriptsize{1,2} \\
%\noalign{\smallskip}
\scriptsize{\object{HD 88661}} &\scriptsize{B2IVpne}  & 237 & 4.333 & 3.99 & 39 &\scriptsize{1,2} \\
%\noalign{\smallskip}
\scriptsize{\object{HD 91465}} &\scriptsize{B3IIIne}  & 266 & 4.240 & 3.52 & 67 &\scriptsize{1,2} \\
%\noalign{\smallskip}
\scriptsize{\object{HD 105435}}&\scriptsize{B2IVne}   & 258 & 4.349 & 3.92 & 42 &\scriptsize{1,2} \\
%\noalign{\smallskip}
\scriptsize{\object{HD 110335}}&\scriptsize{B6IVe}    & 208$^a$ & 4.120$^b$ & 3.28$^b$ & 63 &
\scriptsize{3} \\
%\noalign{\smallskip}
\scriptsize{\object{HD 112091}}&\scriptsize{B5Vne}    & 210 & 4.309 & 3.93 & 36 &\scriptsize{3} \\
%\noalign{\smallskip}
\scriptsize{\object{HD 120991}}&\scriptsize{B2IIIe}   &  70 & 4.347 & 3.69 & 13 &\scriptsize{1,2} \\
%\noalign{\smallskip}
\scriptsize{\object{HD 124367}}&\scriptsize{B4IVne}   & 295 & 4.243 & 3.76 & 63 &\scriptsize{1,2} \\
%\noalign{\smallskip}
\scriptsize{\object{HD 148184}}&\scriptsize{B0.5Vpe}  & 144 & 4.459 & 3.91 & 20 &\scriptsize{1,2,4} \\
%\noalign{\smallskip}
\scriptsize{\object{HD 157042}}&\scriptsize{B2IVe}    & 340 & 4.338 & 4.06 & 53 &\scriptsize{4} \\ 
%\noalign{\smallskip}
\scriptsize{\object{HD 158427}}&\scriptsize{B3Vne}    & 290 & 4.256 & 3.99 & 51 &\scriptsize{4} \\
%\noalign{\smallskip}
\scriptsize{\object{HD 164284}}&\scriptsize{B2Ve}     & 262 & 4.426 & 3.95 & 53 &\scriptsize{4} \\
%\noalign{\smallskip}
\hline
%\noalign{\smallskip}
\end{tabular}}
\medskip
Dates: 1 $\equiv$ 5 Mar. 1996, 2 $\equiv $ 6 Mar.
1996, 3 $\equiv$ 7 Mar. 1996, 4 $\equiv$ 21 
Sep. 1996. Julian days are given in the online Table~\ref{jd}. $^a$ Yudin 
(\cite{yudin}); $^b$ de Geus et~al. (\cite{degeus}). The 
inclination angle $i$ was derived 
using stellar atmospheres calculated for rotationally 
deformed and 
gravitationally darkened stars (Fr\'emat et~al. 2005).
\end{table}